J/ApJS/262/36ivo://CDS.VizieR/J/ApJS/262/36doi:10.26093/cds/vizier.22620036CDSSanchez S.F.Barrera-Ballesteros J.K.Lacerda E.Mejia-Narvaez A.,Camps-farina A.Bruzual G.Espinosa-Ponce C.Rodriguez-Puebla A.,Calette A.R.Ibarra-Medel H.Avila-Reese V.Hernandez-Toledo H.,Bershady M.A.Cano-Diaz M.Munguia-Cordova A.M.2023-02-15T07:33:07Z2022-12-16T11:34:26ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiesspectroscopyline-intensitieschemical-abundancesgalaxy-kinematicssurveysvisible-astronomysloan-photometrytwo-color-diagramsabsolute-magnitudegalaxy-classification-systemsWe present here the analysis performed using the pyPipe3D pipeline for the final MaNGA data set included in the Sloan Digital Sky Survey data release 17. This data set comprises more than 10,000 individual data cubes, being the integral field spectroscopic (IFS) galaxy survey with the largest number of galaxies. pyPipe3D processes the IFS data cubes to extract spatially resolved spectroscopic properties of both the stellar population and the ionized gas emission lines. A brief summary of the properties of the sample and the characteristics of the analyzed data are included. The article provides details of: (i) the analysis performed; (ii) a description of the pipeline; (iii) the adopted stellar population library; (iv) the morphological and photometric analysis; (v) the adopted data model for the spatially resolved properties derived; and (vi) the individual integrated and characteristic galaxy properties included in the final catalog. Comparisons with the results from a previous version of the pipeline for earlier data releases and from other tools using this data set are included. A practical example of how to use the full data set and the final catalog illustrates how to handle the delivered product. Our full analysis can be accessed and downloaded from our web page.2022ApJS..262...36Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/262/36CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIII/232 : STELIB: A library of stellar spectra at R~2000 (Le Borgne+, 2003)V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)J/A+AS/139/29 : Empirical calibration of the 4000 A break (Gorgas+, 1999)J/ApJS/152/251 : Indo-US library of coude feed stellar spectra (Valdes+, 2004)J/ApJ/617/240 : Oxygen abundances in GOODS-North field (Kobulnicky+, 2004)J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006)J/ApJS/186/427 : Detailed morphology of SDSS galaxies (Nair+, 2010)J/MNRAS/403/1213 : Stellar mass-loss. I. (Gonzalez-Lopezlira+, 2010)J/MNRAS/404/1639 : MILES base models & new line index syst. (Vazdekis+, 2010)J/ApJS/190/233 : Sp. & abundances of SINGS galaxies (Moustakas+, 2010)J/MNRAS/414/888 : ATLAS3D project. III. (Emsellem+, 2011)J/A+A/531/A165 : MILES atmospheric parameters (Prugniel+, 2011)J/A+A/559/A114 : Updated O3N2 and N2 abundance indicators (Marino+, 2013)J/MNRAS/435/2835 : Morphological types from Galaxy Zoo 2 (Willett+, 2013)J/A+A/576/A135 : CALIFA DR2 (Garcia-Benito+, 2015)J/A+A/581/A103 : CALIFA survey across the Hubble sequence (Gonzalez+, 2015)J/A+A/584/A87 : CALIFA sample SFR calibration (Catalan-Torrecilla+, 2015)J/A+A/587/A70 : CALIFA face-on spiral galaxies (Sanchez-Menguiano+, 2016)J/MNRAS/466/2570 : Low ionization emission-line galaxies (Belfiore+, 2017)J/AJ/154/86 : MaNGA catalog, DR15 (Wake+, 2017)J/AJ/156/18 : APOGEE DR14:Binary companions (Price-Whelan+, 2018)J/MNRAS/476/1765 : MaNGA E and S galaxies properties (Li+, 2018)J/MNRAS/477/4711 : Stellar angular momentum in ManGa gal. (Graham+, 2018)J/MNRAS/483/2057 : SDSS-IV MaNGA Morphological Catalogues (Fischer+, 2019)J/MNRAS/484/3042 : The gas-phase mass-metallicity relation (Sanchez+, 2019)J/ApJ/882/9 : SFR & metallicities in MaNGA (Sanchez-Menguiano+, 2019)J/ApJ/883/175 : 1st release of MaNGA Stellar Library (MaStar) (Yan+, 2019)J/A+A/623/A122 : Sample of MaNGA galaxies properties (Pilyugin+, 2019)J/A+A/623/A171 : Mkn 848 MaNGA 3-D data cube (Perna+, 2019)J/MNRAS/492/3073 : CALIFA galaxies hosting an AGN (Lacerda+, 2020)J/AJ/159/167 : AMUSING++ nearby galaxy compil. I. (Lopez-Coba+, 2020)J/ApJ/894/57 : Star formation activities in MaNGA (Sun+, 2020)J/ApJ/901/109 : Ages & [Fe/H] of MW bulge with APOGEE (Hasselquist+, 2020)J/ApJ/903/52 : MaNGA; param. of 668 galaxies (Sanchez-Menguiano+, 2020)J/ApJ/903/145 : ALMaQUEST. IV. ALMA-MaNGA (Lin+, 2020)J/ApJ/909/120 : Close galaxy pairs and multiples in MaNGA (Steffen+, 2021)J/MNRAS/507/300 : Massive Compact Galaxies in MaNGA (Schnorr-Mueller+, 2021)J/MNRAS/508/1084 : MaNGA star-forming galaxies (Kumari+, 2021)J/other/RAA/21.306 : Supernova host galaxies in SDSS-IV MaNGA (Zhang+, 2021)J/A+A/659/A131 : Ionized Gas Kinematics in MaNGA (Deconto-Machado+, 2022)http://ifs.astroscu.unam.mx/MaNGA/Pipe3D_v3_1_1/ : MaNGA Pipe3D home pagehttp://www.sdss.org/dr17/manga/ : MaNGA DR17 data on SDSShttp://nsatlas.org/ : the NASA-Sloan Atlas home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/262/36https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/262/36http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/262/36https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/262/36https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/262/36http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/262/36GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/262/36/catalog (Integrated and characteristic parameters delivered for each analyzed data cube)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/262/36/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/262/36/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/262/36/catalog?GETtext/xml+votable180.050000true133.371090657.59842510.0055555555555555564/297 302-303 313 347 372-373 402 414-415 591 594 620-621 648 651 693 706 5/138 1024-1025 1027 1032 1163 1179 1183 1185 1187 1196-1197 1200 1202-1204 1206-1207 1227 1230-1231 1234 1240 1242 1246-1248 1250 1257 1279 1342-1343 1382-1383 1394-1395 1400-1402 1404-1406 1409 1411 1416-1417 1419 1437 1439 1450 1456-1457 1476 1479-1480 1484 1553-1555 1557-1560 1564-1565 1567 1599 1602 1614-1615 1626-1627 1630 1632-1633 1635-1636 1638-1641 1643-1646 1650-1652 1655 1685 1728 1793 1808 1830 1832 1834-1835 2058 2067-2068 2070 2072 2074 2141 2143 2165 2167 2172-2173 2259 2262 2264 2267-2268 2302 2308-2309 2312-2314 2316-2317 2327 2331 2333-2337 2339 2341-2342 2344 2348-2349 2356-2357 2359 2361 2368 2370-2371 2401 2403 2408 2410 2446 2449 2451-2453 2457-2458 2462-2463 2470-2471 2473 2475-2477 2488 2490 2493-2496 2504 2506 2528 2530 2545 2547-2548 2561 2564-2565 2567 2572-2573 2575 2586-2587 2597-2600 2608 2610 2613 2615 2621 2636 2638-2639 2648 2650 2655 2664 2667-2668 2672 2675 2677-2678 2680 2684-2685 2699 2703 2715 2723-2724 2727 2731 2736-2738 2749-2750 2753 2758 2760 2762 2766-2767 2776 2784 2788-2789 2821 2828 2830-2831 2845 2849 2851-2852 2858 2864 2897-2898 3095 3099 4437-4438 4441-4442 4453-4454 4502 4504 4517-4518 4575 4597-4598 4601-4602 4694 4709 4736-4738 4758 4762 4774 4778 4845-4846 4917-4918 4921 4924 4933-4934 4937-4938 4998-5002 5463 5469 5679 5797-5798 5801-5802 6551 6762 6767 6809 6814-6815 6823 6828 6831-6832 6835-6836 6848 6852 6854 6857 6859 7031 7037 7070 7089-7090 7133 7509-7510 7914 7929 8102 8107 8109 8111 8120 8170 9182 12280 6/0-1 521-523 526-527 544-546 548-550 556 640 4104-4106 4114 4117 4120 4123 4132-4134 4136-4138 4140 4160-4162 4318-4319 4341 4343 4383 4407 4426-4427 4448-4449 4451 4456 4490-4491 4512-4514 4523 4526 4647 4650-4651 4661 4663 4666-4667 4682 4704-4706 4712-4713 4715 4726-4728 4730-4731 4736 4738-4739 4745 4747 4769 4772-4773 4775 4781 4793-4796 4798-4799 4804 4806-4807 4821-4823 4864-4865 4867 4869-4871 4898-4899 4902-4904 4906-4907 4914 4917-4919 4964 4966-4967 4972-4974 4976 4978 4982 4998-4999 5005-5007 5024-5025 5033 5040 5056 5058-5062 5064 5066 5073 5076-5077 5294-5295 5306-5307 5327 5338 5349-5351 5356 5358-5360 5362-5363 5463 5469-5471 5492-5494 5523 5526-5527 5547 5551 5574-5575 5584 5586-5588 5590 5592 5594-5596 5598 5612-5613 5615 5628-5630 5633 5649-5650 5652 5656-5658 5672-5674 5680 5683 5688 5690 5713 5715-5717 5719 5726-5727 5738-5739 5741-5743 5745 5752 5754-5755 5781 5783 5789 5791 5797-5799 5804-5806 5808 5810 5816 5819 5833-5834 5836 5838 5840-5841 5844-5846 5857 5859-5860 5862 5865 5867-5868 5870 5888-5890 5908 5910 5912-5913 5915 5926 5928-5929 5933 5935 5940-5942 5944 5947 5984 5987-5990 6161 6197 6205 6208-6209 6211 6225-6227 6244-6245 6247-6250 6253-6255 6264-6266 6340 6343 6352-6354 6356 6359 6367 6385 6387 6389-6391 6393 6395 6402 6414-6415 6448 6450-6453 6455 6499 6503 6513-6515 6518 6537-6539 6548-6549 6551 6569-6571 6588-6589 6591 6593-6597 6599 6612 6614-6618 6916-6917 6928-6930 6932-6933 6976 6980-6981 6992-6993 6996 7169 7184-7186 7213 7215 7224-7226 7230-7231 7236-7237 7274 7298-7299 7301 7304 7306-7309 7311 7313-7315 7317-7319 7324 7326 7333-7335 7344-7345 7352 7354-7355 7360-7361 7363-7364 7366-7370 7680-7681 7685 7696-7697 8194 8218 8226 8228 8230-8231 8240-8242 8245-8247 8253-8255 8263 8265-8267 8277-8278 8292 8302 8304-8305 8307 8320 8322-8323 8385-8387 8448-8450 8518 8524 8526-8527 8531 8537 8539 8569-8571 8655-8657 8659 8665-8667 8677-8679 8684-8685 8687 8696 8698-8702 8888 8890-8891 8894-8895 8938 9029 9031 9035 9040 9042-9043 9045-9047 9052 9060 9062-9063 9065 9067 9080-9081 9083-9084 9110-9111 9116-9117 9119 9141 9153-9156 9161-9163 9166 9169 9172 9184 9186 9188 9191 9197 9199 9203 9206 9215 9221 9224 9227 9229 9231 9240 9242-9244 9246-9247 9260-9262 9272-9274 9277-9279 9281-9284 9286-9290 9292 9294 9301-9303 9306 9312 9314-9317 9319-9321 9323 9329 9331 9352-9354 9361-9363 9373-9374 9381 9383-9386 9389 9400 9413 9416 9418 9423 9433-9435 9440 9451 9454 9478 9520 9601 9609-9611 9624 9638 9644 9646-9647 9728 9777 9779-9780 9788 9790 9792-9793 9795 9803 9816-9818 9820-9822 9836-9837 9839-9841 9844 9847 9875 9877-9878 9891 9897-9899 9912 9914 9956 9958 9964 9968-9969 9971 9988 9990 9992-9993 9995-9996 9998 10022 10030 10061-10063 10072 10074 10085-10086 10092-10093 10095-10096 10098-10099 10104-10106 10144-10146 10152 10154 10179 10185 10187 10200-10202 10211-10213 10215 10217 10219-10222 10226 10253 10264-10265 10267 10277 10280 10282-10283 10285-10286 10296-10297 10304 10306 10312-10313 10336 10338-10339 10342 10385-10387 10404 10406 10408 10413 10436-10438 10449 10451 10456-10457 10459 10464 10466 10472 10493 10526 10542-10543 10548 10551 10574 10576 10580-10581 10583 10596 10604 10627-10629 10631 10633 10635-10638 10641 10644 10649-10652 10654 10662-10665 10667 10676-10677 10681 10683 10692 10694-10696 10698-10699 10704 10706-10707 10716-10718 10725-10726 10733 10745-10750 10769 10772-10773 10775 10784 10789 10791-10793 10795 10808-10810 10816 10855 10857-10859 10866-10867 10869-10874 10880-10881 10883 10885 10889 10900 10902-10904 10906 10918 10921 10928-10930 10932-10934 10936-10937 10939-10941 10956-10957 10959-10960 10962-10963 10973-10978 10992-10993 10995 11004-11006 11017-11019 11021 11023-11024 11036-11038 11044-11045 11047 11053 11055 11058-11062 11079-11082 11084-11086 11108 11110-11114 11116 11120 11140-11142 11144 11146-11147 11149-11151 11160 11164-11165 11168-11170 11172-11173 11176 11178-11179 11182 11200 11202 11206 11208 11264-11266 11268-11269 11271 11273-11276 11279 11282-11283 11288 11290-11291 11293-11294 11318-11319 11328 11330-11331 11336-11337 11344-11345 11347-11350 11355-11358 11360 11362 11368 11370-11372 11374 11377 11379 11384 11388 11392-11394 11401-11403 11412 11414 11416 11424 11426-11428 11430 11436 11438 11460 11462 11520 11528 11586-11587 11596-11598 11600 11602 11776-11778 11784 12288 12290 12375 12387 12389-12392 12395 12404-12405 12408 12481 12552 12554 12576 17726-17727 17741-17743 17745-17747 17756 17758 17761 17772 17776 17778 17805 17807 17809-17811 17820-17822 17829 17841 17856 17997-17998 18001-18005 18007 18020-18022 18028-18029 18032 18061-18063 18065-18066 18076-18077 18084-18085 18097 18114 18295 18299 18365 18367 18381 18383 18385-18387 18396 18402 18412-18414 18416-18418 18604 18606-18607 18616 18618 18685-18687 18765 18767 18769 18771-18772 18774-18775 18780 18782 18788 18801 18831 18833 18842 18844-18845 18850-18851 18853-18858 18860-18861 18864 18956 18960 19005-19007 19023 19025 19028-19029 19031 19036 19043-19045 19047 19052 19056-19058 19086-19087 19090-19092 19094-19095 19100-19102 19105 19107 19109-19111 19116-19118 19120-19122 19136 19144 19200 19202 19319 19325 19389-19390 19398-19399 19405 19407 19413 19416-19418 19424 19426 19432-19433 19663 19666-19667 19676-19678 19681 19683 19689 19694-19695 19700 19704 19725 19731 19740 19742 19756-19758 19760-19761 19764 19777-19778 19840-19842 19844 19848 19982-19983 19985-19988 19990-19991 20012 20016-20018 20096 21845-21847 21849 21851 21873 21885-21887 21973 22396-22397 22399 22485 22710 22760 23043 23045 23047 23049-23052 23057-23062 23072-23074 23076 23101-23103 23144 23146-23147 23181-23183 23185-23187 23196-23198 23201-23203 23212 23214 23216 23218 23232-23233 25846 25851-25852 25854-25855 25940 25942-25943 25949 25972 25974-25975 25977 25980-25982 26016 26018 26024-26025 26027 26043-26044 26046-26047 26068-26069 26196 26198 26203 26228-26229 26385 26388-26389 26432 26877 26879 27037-27039 27052-27054 27060 27065-27067 27082-27083 27085-27087 27096 27104-27106 27109 27112 27120 27198-27199 27214-27215 27217-27220 27222-27226 27229 27233 27235 27240-27242 27244-27245 27247-27248 27250-27251 27279 27285-27287 27290-27291 27303 27305 27307-27308 27310-27311 27316-27318 27321 27333-27335 27337-27339 27348-27350 27352 27354-27356 27358 27360-27362 27364-27365 27367-27368 27370-27371 27378 27380 27397 27399 27401 27404 27407 27413-27414 27420 27422 27433-27435 27440-27441 27521-27522 27528 27659-27660 27662-27663 27681 27684-27686 28030-28031 28116 28118-28119 28269 28271 28286 28319 28340-28341 28364-28366 28368-28370 28384-28385 28418 28425-28427 28429 28431 28449 28452 28531 28537 28540-28542 28627 28629-28631 28633 28636 28638-28639 30033-30035 30044-30046 30065 31485 31487 31650 31654 31660 31662 31693-31694 31728 31730 32403 32413-32415 32421-32423 32432-32434 32442-32443 32456 32458-32459 32486 32489-32492 32494 32497 32499 32501-32503 32508-32509 32511 32672 32674 32684 36702-36703 36717 36719 36723 36725 36727 36732-36733 36759 36765 36767 36800 36802-36803 36808-36810 36812 36816-36817 36861-36863 48988-48989 49007 49018 49079 49084-49086 49091-49092 49094-49095 49097 49099-49102 49104 49106 49128-49130 49147 491512.4622242610829604e-19 3.264051565855503e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/262/36?format=asciiOpticaldefaultJ/ApJS/262/36/catalogIntegrated and characteristic parameters delivered for each analyzed data cubee_RJmag[0.05/1.3] Uncertainty on the RJmag (RJ_band_mag_error)magstat.error;phot.magfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameManga-plate-ifudsgn unique namemeta.idcharPlate[7443/12772]? Plate ID of the MaNGA cubemeta.id;instr.plateintnullableIFUdsgnIFU bundle ID of the MaNGA cubemeta.id;obscharalphaZReMW[-1.8/1.6]? Slope of the gradient of the MW log-metallicity of the stellar population in dex/Re (alpha_ZH_MW_Re_fit)arith.gradfloatnullablee_alphaZReMW[0.003/0.7]? alphaZReMW uncertainty (e_alpha_ZH_MW_Re_fit)stat.errorfloatnullableOH-M08c[8/74]? Oxygen abundance using the calibrator M08 at the central aperture (OH_M08_cen) (1)phys.abunddoublenullablee_OH-M08c[0/100]? OH-M08c uncertainty (e_OH_M08_cen)stat.errordoublenullableOH-T04c[-44/9.8]? Oxygen abundance using the calibrator T04 at the central aperture (OH_T04_cen) (1)phys.abunddoublenullablee_OH-T04c[0/83]? OH-T04c uncertainty (e_OH_T04_cen)stat.errordoublenullablee_logSII/Ha[0.0008/3.5]? logSII/Ha uncertainty (e_log_SII_Ha_ALL)stat.errordoublenullablelogOII/Hb[-0.99/5.2]? Log of the [OII]3727/H{beta} ratio within the entire FOV (log_OII_Hb_ALL)spect.line.intensity;arith.ratiodoublenullablee_logOII/Hb[0.0004/4.4]? logOII/Hb uncertainty (e_log_OII_Hb_ALL)stat.errordoublenullableZ-T70[-2.31/0.3] Stellar metallicity at T70 time (ZH_T70)log(Sun)phys.abund.ZfloatZ-T70Re[-3.4/0.7]? Stellar metallicity at Re at T70 time (ZH_Re_T70)log(Sun)phys.abund.ZfloatnullableaZH-T70[-2.2/2.1]? Slope of the ZH gradient at T70 time in dex/Re (a_ZH_T70)stat.fit.paramfloatnullableT80[0.88/12.1] Lookback time at which the galaxy has formed 80% of its stellar massGyrtime.intervalfloatZ-T80[-2.31/0.3] Stellar metallicity at T80 time (ZH_T80)log(Sun)phys.abund.ZfloatZ-T80Re[-3.4/0.5]? Stellar metallicity at Re at T80 time (ZH_Re_T80)log(Sun)phys.abund.ZfloatnullablelogSFRs10[-3.5/2.7]? Integrated SFR derived from the SSP analysis for t<10Myr (log_SFR_ssp_10Myr)log(solMass.yr**-1)phys.SFRfloatnullableVdispHac[12/823]? H{alpha} velocity dispersion at the central aperture (vel_disp_Ha_cen)km/sphys.veloc.dispersionfloatnullableVdispsc[0.28/466]? Stellar velocity dispersion at the central aperture (vel_disp_ssp_cen)km/sphys.veloc.dispersionfloatnullablee_FHac[0/7021] FHac uncertainty (e_F_Ha_cen)1e-19W.m**-2stat.errordoubleF[OII]26a[-11/1.3]? Flux intensity of [OII]3726.03 at 1Re in 10^-16^erg/s/cm^2^ (flux_OII3726_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[OII]26a[0.0003/3.2]? F[OII]26a uncertainty (e_flux[OII]3726.03_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[OII]28Re[-1.3/16]? Flux intensity of [OII]3728.82 at 1Re in 10^-16^erg/s/cm^2^ (flux_OII3728_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[OII]28Re[0.0005/3]? F[OII]28Re uncertainty (e_flux_OII3728_Re_fit)1e-19W.m**-2stat.errordoublenullablee_FHeI39a[0.00029/1.1]? FHeI39a uncertainty (e_flux_HeI3964_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[NeIII]Re[-0.75/10.3]? Flux intensity of [NeIII]3967.46 1Re in 10^-16^erg/s/cm^2^ (flux_[NeIII]3967_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[NeIII]Re[0.00028/2.8]? F[NeIII]Re uncertainty (e_flux_[NeIII]3967_Re_fit)1e-19W.m**-2stat.errordoublenullableF[NeIII]a[-7.3/1.2]? Flux intensity of [NeIII]3967.46 1Re in 10^-16^erg/s/cm^2^ (flux[NeIII]3967.46_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHba[0.0002/5.6]? FHba uncertainty (e_flux_Hb4861_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[OIII]49Re[-0.9/16]? Flux intensity of [OIII]4958.91 at 1Re in 10^-16^erg/s/cm^2^ (flux_[OIII]4958_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[OIII]49Re[0.0002/17]? F[OIII]49Re uncertainty (e_flux_OIII4958_Re_fit)1e-19W.m**-2stat.errordoublenullableFNaI89Re[-1/4.6]? Flux intensity of NaI5889.95 at 1Re in 10^-16^erg/s/cm^2^ (flux_NaI5889_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FNaI89Re[0.0002/4.6]? FNaI89Re uncertainty (e_flux_NaI5889_Re_fit)1e-19W.m**-2stat.errordoublenullableFNaI89a[-5.81/1.4]? Flux intensity of NaI5889.95 at 1Re in 10^-16^erg/s/cm^2^ (flux_NaI5889_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[SII]16Re[0.00014/2]? F[SII]16Re uncertainty (e_flux_SII6716_Re_fit)1e-19W.m**-2stat.errordoublenullableF[SII]16a[-4.6/1]? Flux intensity of [SII]6716.44 at 1Re in 10^-16^erg/s/cm^2^ (flux_SII6716_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[SII]16a[0.00012/1.5]? F[SII]16a uncertainty (e_flux_SII6716_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[SII]30Re[-0.6/5.3]? Flux intensity of [SII]6730.82 at 1Re in 10^-16^erg/s/cm^2^ (flux_[SII]6730.82_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[SIII]95Re[0.0003/1.6]? F[SIII]95Re uncertainty (e_flux_SIII9531_Re_fit)1e-19W.m**-2stat.errordoublenullableF[SIII]95a[-5.3/2]? Flux intensity of [SIII]9531.1 at 1Re in 10^-16^erg/s/cm^2^ (flux_SIII9531_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[SIII]95a[0.00027/1.4]? F[SIII]95a uncertainty (e_flux_SIII9531_alpha_fit)1e-19W.m**-2stat.errordoublenullableOH-Mar13-N2Re[8/8.8]? Oxygen abundance using the calibrator Mar13_N2 at 1Re (OH_Mar13_N2_Re_fit) (1)phys.abundfloatnullablee_OH-Mar13-N2Re[0.001/0.4]? OH-Mar13-N2Re uncertainty (e_OH_Mar13_N2_Re_fit)stat.errorfloatnullableOH-Mar13-N2a[-0.5/0.5]? Slope of the O/H gradient using the calibrator Mar13_N2 in dex/Re (OH_Mar13_N2_alpha_fit)arith.grad;phys.abunddoublenullablee_OH-Mar13-N2a[0.0008/0.21]? OH-Mar13-N2a uncertainty (e_OH_Mar13_N2_alpha_fit)stat.errordoublenullableOH-Mar13-O3N2Re[8.14/8.7]? Oxygen abundance using the calibrator Mar13_O3N2 at 1Re (OH_Mar13_O3N2_Re_fit) (1)phys.abunddoublenullableOH-Pet04-O3N2Re[8/9]? Oxygen abundance using the calibrator Pet04_O3N2 at 1Re (OH_Pet04_O3N2_Re_fit) (1)phys.abundfloatnullablee_OH-Pet04-O3N2Re[0.001/0.6]? OH-Pet04-O3N2Re uncertainty (e_OH_Pet04_O3N2_Re_fit)stat.errorfloatnullableOH-Pet04-O3N2a[-0.7/0.5]? Slope of the O/H gradient using the calibrator Pet04_O3N2 in dex/Re (OH_Pet04_O3N2_alpha_fit)arith.grad;phys.abunddoublenullablee_OH-Pet04-O3N2a[0.0008/0.4]? OH-Pet04-O3N2a uncertainty (e_OH_Pet04_O3N2_alpha_fit)stat.errordoublenullableOH-Kew02-N2O2Re[8/9.5]? Oxygen abundance using the calibrator Kew02_N2O2 at 1Re (OH_Kew02_N2O2_Re_fit) (1)phys.abundfloatnullablee_OH-Kew02-N2O2Re[0.0018/1.3]? OH-Kew02-N2O2Re uncertainty (e_OH_Kew02_N2O2_Re_fit)stat.errorfloatnullableOH-Kew02-N2O2a[-1.1/1.1]? Slope of the O/H gradient using the calibrator Kew02_N2O2 in dex/Re (OH_Kew02_N2O2_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-Kew02-N2O2a[0.0015/1]? OH-Kew02-N2O2a uncertainty (e_OH_Kew02_N2O2_alpha_fit)stat.errorfloatnullableOH-Pil10-ONSRe[7.5/9]? Oxygen abundance using the calibrator Pil10_ONS at 1Re (OH_Pil10_ONS_Re_fit) (1)phys.abunddoublenullablee_OH-Pil10-ONSRe[0.0009/2]? OH-Pil10-ONSRe uncertainty (e_OH_Pil10_ONS_Re_fit)stat.errordoublenullableOH-Pil10-ONSa[-1.6/1.3]? Slope of the O/H gradient using the calibrator Pil10_ONS (OH_Pil10_ONS_alpha_fit)arith.grad;phys.abunddoublenullablee_OH-Pil10-ONSa[0.0008/2.3]? OH-Pil10-ONSa uncertainty (e_OH_Pil10_ONS_alpha_fit)stat.errordoublenullableOH-Pil10-ONRe[7.5/9]? Oxygen abundance using the calibrator Pil10_ON at 1Re (OH_Pil10_ON_Re_fit) (1)phys.abundfloatnullablee_OH-Pil10-ONRe[0.0014/2]? OH-Pil10-ONRe uncertainty (e_OH_Pil10_ON_Re_fit)stat.errorfloatnullableOH-Pil10-ONa[-1.7/1.3]? Slope of the O/H gradient using the calibrator Pil10_ON in dex/Re (OH_Pil10_ON_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-Pil10-ONa[0.0012/2.2]? OH-Pil10-ONa uncertainty (e_OH_Pil10_ON_alpha_fit)stat.errorfloatnullableOH-Pil11-NSRe[7/9.3]? Oxygen abundance using the calibrator Pil11_NS at 1Re (OH_Pil11_NS_Re_fit) (1)phys.abundfloatnullableOH-Hoa[-0.9/1.2]? Slope of the O/H gradient using the calibrator Ho in dex/Re (OH_Ho_alpha_fit)arith.grad;phys.abundfloatnullablee_NO-Pil16Ra[0.0029/2]? NO-Pil16Ra uncertainty (e_NO_Pil16_R_alpha_fit)stat.errorfloatnullablee_Fe5270a[0.015/9]? Fe5270a uncertainty (e_Fe5270_alpha_fit)stat.errorfloatnullablee_C[5.9e-5/3.2] C uncertaintystat.errordoubleP(S0)[0.0001/0.94] Probability of being an S0 galaxystat.fit.goodnessdoubleP(Sa)[0.0002/0.92] Probability of being an Sa galaxystat.fit.goodnessdoubleP(Sab)[0.0001/0.8] Probability of being an Sab galaxystat.fit.goodnessdoubleP(Sb)[0.0005/0.9] Probability of being an Sb galaxystat.fit.goodnessdoubleP(Sbc)[0.0003/0.85] Probability of being an Sbc galaxystat.fit.goodnessdoubleNSAid[58/698275]? NSA identifier (nsa_nsaid)meta.idintnullableQ[0/7]? QC flag: 0=good, 2=bad, >2 warning (QCFLAG)meta.code.qualintnullableSimbadSimbad column added by the CDSmeta.ref.urlcharNEDNED column added by the CDSmeta.ref.urlcharDR15Display data from MaNGA DR15 (Wake+, 2017, J/AJ/154/86) if anymeta.ref.urlintnullablePlateIFUCode formed by the plate and ifu namesmeta.id;meta.maincharMaNGAIdMaNGA IDmeta.idcharRAJ2000Right ascension of the object (J2000) (objra)degpos.eq.ra;meta.mainindexedDEJ2000[-9.4/65.3] Declination of the object (J2000) (objdec)degpos.eq.dec;meta.mainindexedlogSFRHa[-5.4/3.9]? Integrated SFR derived from the integrated H{alpha} luminosity (log_SFR_Ha)log(solMass.yr**-1)phys.SFRfloatnullableFoV[-0.003/32] Ratio between the diagonal radius of the cube and effective radiusphot.fluxdoubleReff[-25635/137] Effective radius in kiloparsecs (Re_kpc)kpcphys.size.radiusdoublee_logMass[0.05/0.15] logMass uncertainty (e_log_Mass)log(solMass)stat.error;phys.massfloate_logSFRHa[0.05/4.5] logSFRHa uncertainty (e_log_SFR_Ha)log(solMass.yr**-1)stat.errorfloatlogMass[5.9/17.8] Integrated stellar mass in units of the solar mass in log (log_Mass)log(solMass)phys.massfloatlogSFRs[-3.9/2.4]? Integrated SFR derived from the SSP analysis t<32Myr (log_SFR_ssp)log(solMass.yr**-1)phys.SFRfloatnullablelogNII/Hac[-1.4/5]? Log of the [NII]6583/H{alpha} line ratio in the central aperture (log_NII_Ha_cen)spect.line.intensity;arith.ratiodoublenullablee_logNII/Hac[3.5e-5/1.3]? logNII/Hac uncertainty (e_log_NII_Ha_cen)stat.errordoublenullablelogOIII/Hbc[-1.3/4.6]? Log of the [OIII]5007/H{beta} line ratio in the central aperture (log_OIII_Hb_cen)spect.line.intensity;arith.ratiodoublenullablee_logOIII/Hbc[0.0015/5]? logOIII/Hbc uncertainty (e_log_OIII_Hb_cen)stat.errordoublenullablelogSII/Hac[-1/6.3]? Log of the [SII]6717+6731/H{alpha} line ratio in the central aperture (log_SII_Ha_cen)spect.line.intensity;arith.ratiodoublenullablee_logSII/Hac[0.0013/3.5]? logSII/Hac uncertainty (e_log_SII_Ha_cen)stat.errordoublenullablelogOII/Hbc[-0.94/4]? Log of the [OII]3727/H{beta} line ratio in the central aperture (log_OII_Hb_cen)spect.line.intensity;arith.ratiodoublenullablee_logOII/Hbc[0.0027/5.3]? logOII/Hbc uncertainty (e_log_OII_Hb_cen)stat.errordoublenullableEWHac[-465.1/-0.001]? Equivalent width of H{alpha} in the central aperture in {AA} (EW_Ha_cen)0.1nmspect.line.eqWidthdoublenullablee_EWHac[0.006/158]? EWHac uncertainty (e_EW_Ha_cen)0.1nmstat.errorfloatnullablelogZReLW[-1.6/0.2] Log of luminosity-weighted (LW) metallicity of the stellar population at the effective radius (ZH_LW_Re_fit)log(Sun)phys.abund.Zfloate_logZReLW[0/0.3]? logZReLW uncertainty (e_ZH_LW_Re_fit)log(Sun)stat.errorfloatnullablealphaZReLW[-0.9/0.6]? Slope of the gradient of the LW metallicity of the stellar population in dex/Re (alpha_ZH_LW_Re_fit)arith.gradfloatnullablee_alphaZReLW[0/0.3]? alphaZReLW uncertainty (e_alpha_ZH_LW_Re_fit)stat.errorfloatnullablelogZReMW[-1.7/0.4]? Log of mass-weighted (MW) metallicity of the stellar population at the effective radius (ZH_MW_Re_fit)log(Sun)phys.abund.Zfloatnullablee_logZReMW[0.0029/0.7]? logZReMW uncertainty (e_ZH_MW_Re_fit)stat.errorfloatnullablelogAgeReLW[7.4/10]? Log of LW age of the stellar population (Age_LW_Re_fit)log(yr)time.agedoublenullablee_logAgeReLW[0.004/0.8]? logAgeReLW uncertainty (e_Age_LW_Re_fit)log(yr)stat.errordoublenullablealphaAgeReLW[-1.9/1.6]? Slope of the gradient of the LW log-age of the stellar population in log(yr)/Re (alpha_Age_LW_Re_fit)arith.graddoublenullablee_alphaAgeReLW[0.004/1.3]? alphaAgeReLW uncertainty (e_alpha_Age_LW_Re_fit)stat.errordoublenullablelogAgeReMW[8.9/10.1]? Log of MW age of the stellar population (Age_MW_Re_fit)log(yr)time.agedoublenullablee_logAgeReMW[0.002/0.5]? logAgeReMW uncertainty (e_Age_MW_Re_fit)log(yr)stat.errordoublenullablealphaAgeReMW[-1/0.8]? Slope of the gradient of the MW log-age of the stellar population in log(yr)/Re (alpha_Age_MW_Re_fit)arith.graddoublenullablee_alphaAgeReMW[0.0039/0.8]? alphaAgeReMW uncertainty (e_alpha_Age_MW_Re_fit)stat.errordoublenullableReffA[0.46/162]? Adopted effective radius in arcseconds (Re_arc)arcsecphys.angSizedoublenullableDL[3e+24/2.2e+27] Adopted luminosity distanceMpcpos.distancedoubleDA[0.0047/2.6] Adopted angular diameter distanceMpcphys.size.diameterdoublePA[90/270] Adopted position angledegpos.posAngfloatell[0/0.95] Adopted ellipticity (ellip)src.ellipticitydoublelogMassgas[5/195]? Log of integrated gas mass (log_Mass_gas)log(solMass)phys.massdoublenullablevel/sig[0.017/1.1]? Velocity/dispersion ratio for the stellar populations within 1.5Re (vel_sigma_Re)phys.veloc;arith.ratiofloatnullablee_vel/sig[0/0.2]? vel/sig uncertainty (e_vel_sigma_Re)stat.errorfloatnullablelogSFRsf[-5.5/4]? Integrated SFR using only the spaxels compatible with SF (log_SFR_SF)log(solMass.yr**-1)phys.SFRfloatnullablelogSFRdc[-7.1/4]? Integrated SFR diffuse corrected (log_SFR_D_C)log(solMass.yr**-1)phys.SFRfloatnullableOH-O3N2c[8/9.5]? Oxygen abundance using the calibrator O3N2 at the central aperture (OH_O3N2_cen) (1)phys.abunddoublenullablee_OH-O3N2c[1.7e-6/0.3]? OH-O3N2c uncertainty (e_OH_O3N2_cen)stat.errordoublenullableOH-N2c[7.9/10.2]? Oxygen abundance using the calibrator N2 at the central aperture (OH_N2_cen) (1)phys.abunddoublenullablee_OH-N2c[0.0002/0.4]? OH-N2c uncertainty (e_OH_N2_cen)stat.errordoublenullableOH-ONSc[6.4/9.1]? Oxygen abundance using the calibrator ONS at the central aperture (OH_ONS_cen) (1)phys.abunddoublenullablee_OH-ONSc[1.8e-5/1.4]? OH-ONSc uncertainty (e_OH_ONS_cen)stat.errordoublenullableOH-R23c[-26.4/13.1]? Oxygen abundance using the calibrator R23 at the central aperture (OH_R23_cen) (1)phys.abunddoublenullablee_OH-R23c[0.00017/57]? OH-R23c uncertainty (e_OH_R23_cen)stat.errordoublenullableOH-pyqzc[7.7/9.3]? Oxygen abundance using the calibrator pyqz at the central aperture (OH_pyqz_cen) (1)phys.abunddoublenullablee_OH-pyqzc[0.0015/0.8]? OH-pyqzc uncertainty (e_OH_pyqz_cen)stat.errordoublenullableOH-t2c[8.2/10]? Oxygen abundance using the calibrator t2 at the central aperture (OH_t2_cen) (1)phys.abunddoublenullablee_OH-t2c[0.00047/0.8]? OH-t2c uncertainty (e_OH_t2_cen)stat.errordoublenullableOH-dopc[-870/18795]? Oxygen abundance using the calibrator dop at the central aperture (OH_dop_cen) (1)phys.abunddoublenullablee_OH-dopc[0.00037/33338]? OH-dopc uncertainty (e_OH_dop_cen)stat.errordoublenullableOH-O3N2-EPc[7/11]? Oxygen abundance using the calibrator O3N2_EPM09 at the central aperture (OH_O3N2_EPM09_cen) (1)phys.abunddoublenullablee_OH-O3N2-EPc[0.0003/2.4]? OH-O3N2-EPc uncertainty (e_OH_O3N2_EPM09_cen)stat.errordoublenullablelogOI/Hac[-2.8/4.8]? Log of the [OI]6301/H{alpha} within a central aperture (log_OI_Ha_cen)spect.line.intensity;arith.ratiodoublenullablee_logOI/Hac[0.00049/3.4]? logOI/Hac uncertainty (e_log_OI_Ha_cen)stat.errordoublenullableHa/Hbc[-29421/334448]? Ratio between the flux of H{alpha} and H{beta} within a central aperture (Ha_Hb_cen)spect.line.intensity;arith.ratiodoublenullablee_Ha/Hbc[-4531/9527]? Ha/Hbc uncertainty (e_Ha_Hb_cen)stat.errordoublenullablelogNII/HaRe[-1.4/4.3]? Log of the [NII]6583/H{alpha} line ratio at 1Re (log_NII_Ha_Re)spect.line.intensity;arith.ratiodoublenullablee_logNII/HaRe[0.002/2]? logNII/HaRe uncertainty (e_log_NII_Ha_Re)stat.errordoublenullablelogOIII/HbRe[-1.3/6.6]? Log of the [OIII]5007/H{beta} line ratio at 1Re (log_OIII_Hb_Re)spect.line.intensity;arith.ratiodoublenullablee_logOIII/HbRe[0.00013/3.5]? logOIII/HbRe uncertainty (e_log_OIII_Hb_Re)stat.errordoublenullablelogSII/HaRe[-0.99/4.8]? Log of the [SII]6717+6731/H{alpha} ratio at 1Re (log_SII_Ha_Re)spect.line.intensity;arith.ratiodoublenullablee_logSII/HaRe[0.0002/3.9]? logSII/HaRe uncertainty (e_log_SII_Ha_Re)stat.errordoublenullablelogOII/HbRe[-0.94/4.5]? Log of the [OII]3727/H{beta} ratio at 1Re (log_OII_Hb_Re)spect.line.intensity;arith.ratiodoublenullablee_logOII/HbRe[0.0004/3.8]? logOII/HbRe uncertainty (e_log_OII_Hb_Re)stat.errordoublenullablelogOI/HaRe[-2.6/6]? Log of the [OI]6301/H{alpha} ratio at 1Re (log_OI_Ha_Re)spect.line.intensity;arith.ratiodoublenullablee_logOI/HaRe[0.00013/5]? logOI/HaRe uncertainty (e_log_OI_Ha_Re)stat.errordoublenullableEWHaRe[-488/-0]? EW of H{alpha} at 1Re in {AA} (EW_Ha_Re)0.1nmspect.line.eqWidthdoublenullablee_EWHaRe[0.012/122]? EWHaRe uncertainty (e_EW_Ha_Re)0.1nmstat.errorfloatnullableHa/HbRe[2.8/123]? Ratio between the flux of H{alpha} and H{beta} within at 1Re (Ha_Hb_Re)spect.line.intensity;arith.ratiofloatnullablee_Ha/HbRe[0/309]? Ha/HbRe uncertainty (e_Ha_Hb_Re)stat.errorfloatnullablelogNII/Ha[-1.3/7.3]? Log of the [NII]6583/H{alpha} line ratio within the entire FOV (log_NII_Ha_ALL)spect.line.intensity;arith.ratiodoublenullablee_logNII/Ha[0.00037/2.8]? logNII/Ha uncertainty (e_log_NII_Ha_ALL)stat.errordoublenullablelogOIII/Hb[-1.2/6.4]? Log of the [OIII]5007/H{beta} line ratio within the FOV (log_OIII_Hb_ALL)spect.line.intensity;arith.ratiodoublenullablee_logOIII/Hb[0.00047/6]? logOIII/Hb uncertainty (e_log_OIII_Hb_ALL)stat.errordoublenullablelogSII/Ha[-0.99/7.8]? Log of the [SII]6717+6731/H{alpha} ratio within the entire FOV (log_SII_Ha_ALL)spect.line.intensity;arith.ratiodoublenullablelogOI/Ha[-2.6/5]? Log of the [OI]6301/H{alpha} ratio within the entire FOV (log_OI_Ha_ALL)spect.line.intensity;arith.ratiodoublenullablee_logOI/Ha[0.0018/5]? logOI/Ha uncertainty (e_log_OI_Ha_ALL)stat.error;phys.abunddoublenullableEWHa[-285/0]? EW of H{alpha} within the entire FOV in {AA} (EW_Ha_ALL)0.1nmspect.line.eqWidthdoublenullablee_EWHa[0/159]? EWHa uncertainty (e_EW_Ha_ALL)0.1nmstat.errorfloatnullableHa/Hb[2.8/58]? Ratio between the flux of H{alpha} and H{beta} within the entire FOV (Ha_Hb_ALL)spect.line.intensity;arith.ratiofloatnullablelogsigMc[0.6/4.5]? Stellar-mass surface density in the central aperture (Sigma_Mass_cen)log(solMass.pc**-2)phys.densitydoublenullablee_logsigMc[0/0.9]? logsigMc uncertainty (e_Sigma_Mass_cen)log(solMass.pc**-2)stat.errordoublenullablelogsigMRe[0.37/4.1]? Stellar-mass surface density at 1Re (Sigma_Mass_Re)log(solMass.pc**-2)phys.densitydoublenullablee_logsigMRe[0.0009/0.9]? logsigMRe uncertainty (e_Sigma_Mass_Re)log(solMass.pc**-2)stat.errordoublenullablelogsigM[0.5/3.8]? Average stellar-mass surface density within the entire FOV (Sigma_Mass_ALL)log(solMass.pc**-2)phys.densitydoublenullablee_logsigM[0.07/1.3]? logsigM uncertainty (e_Sigma_Mass_ALL)log(solMass.pc**-2)stat.errordoublenullableT30[2.3/13] Lookback time at which the galaxy has formed 30% of its stellar massGyrtime.intervalfloatZ-T30[-2.31/0.3] Stellar metallicity at T30 time (ZH_T30)log(Sun)phys.abund.ZfloatZ-T30Re[-9.4/1.1]? Stellar metallicity at Re at T30 time (ZH_Re_T30)log(Sun)phys.abund.ZfloatnullableaZ-T30[-1.94/2.1]? Slope of the ZH gradient at T30 time in dex/Re (a_ZH_T30)stat.fit.paramfloatnullableT40[1.9/12.8] Lookback time at which the galaxy has formed 40% of its stellar massGyrtime.intervalfloatZ-T40[-2.31/0.3] Stellar metallicity at T40 time (ZH_T40)log(Sun)phys.abund.ZfloatZ-T40Re[-9/2.3]? Stellar metallicity at Re at T40 time (ZH_Re_T40)log(Sun)phys.abund.ZfloatnullableaZ-T40[-2.5/2.1]? Slope of the ZH gradient at T40 time in dex/Re (a_ZH_T40)stat.fit.paramfloatnullableT50[1.49/12.7] Lookback time at which the galaxy has formed 50% of its stellar massGyrtime.intervalfloatZ-T50[-2.31/0.3] Stellar metallicity at T50 time (ZH_T50)log(Sun)phys.abund.ZfloatZ-T50Re[-5.8/0.8]? Stellar metallicity at Re at T50 time (ZH_Re_T50)log(Sun)phys.abund.ZfloatnullableaZ-T50[-2.5/2.1]? Slope of the ZH gradient at T50 time in dex/Re (a_ZH_T50)stat.fit.paramfloatnullableT60[1.26/12.5] Lookback time at which the galaxy has formed 60% of its stellar massGyrtime.intervalfloatZ-T60[-2.31/0.3] Stellar metallicity at T60 time (ZH_T60)log(Sun)phys.abund.ZfloatZ-T60Re[-4.3/2]? Stellar metallicity at Re at T60 time (ZH_Re_T60)log(Sun)phys.abund.ZfloatnullableaZ-T60[-2.4/2.1]? Slope of the ZH gradient at T60 time in dex/Re (a_ZH_T60)stat.fit.paramfloatnullableT70[1/12.3] Lookback time at which the galaxy has formed 70% of its stellar massGyrtime.intervalfloataZ-T80[-1.95/1.5]? Slope of the ZH gradient at T80 time in dex/Re (a_ZH_T80)stat.fit.paramfloatnullableT90[0.66/10.6] Lookback time at which the galaxy has formed 90% of its stellar massGyrtime.intervalfloatZ-T90[-2.1/0.3] Stellar metallicity at T90 time (ZH_T90)log(Sun)phys.abund.ZfloatZ-T90Re[-2.7/1.71]? Stellar metallicity at Re at T90 time (ZH_Re_T90)log(Sun)phys.abund.ZfloatnullableaZ-T90[-1.5/1.2]? Slope of the ZH gradient at T90 time in dex/Re (a_ZH_T90)stat.fit.paramfloatnullableT95[0.25/7.7] Lookback time at which the galaxy has formed 95% of its stellar massGyrtime.intervalfloatZ-T95[-2.2/0.3] Stellar metallicity at T95 time (ZH_T95)log(Sun)phys.abund.ZfloatZ-T95Re[-1.81/2.8]? Stellar metallicity at Re at T95 time (ZH_Re_T95)log(Sun)phys.abund.ZfloatnullableaZ-T95[-1.5/1.3]? Slope of the ZH gradient at T95 time in dex/Re (a_ZH_T95)stat.fit.paramfloatnullableT99[0.0074/4.2] Lookback time at which the galaxy has formed 99% of its stellar massGyrtime.intervalfloatZ-T99[-1.8/0.3] Stellar metallicity at T99 time (ZH_T99)log(Sun)phys.abund.ZfloatZ-T99Re[-2.2/0.4]? Stellar metallicity at Re at T99 time (ZH_Re_T99)log(Sun)phys.abund.ZfloatnullableaZ-T99[-1.4/1.3]? Slope of the ZH gradient at T99 time in dex/Re (a_ZH_T99)stat.fit.paramfloatnullablelogMgasAvg[5.7/10.7]? Log of integrated gas mass using the calibrator log_Mass_gas_Av_gas_OH (log_Mass_gas_Av_gas_OH)log(solMass)phys.massfloatnullablelogMgasAvs[6.4/10.8]? Log of integrated gas mass using the calibrator log_Mass_gas_Av_ssp_OH (log_Mass_gas_Av_ssp_OH)log(solMass)phys.massfloatnullableVels2Re[0.09/1042]? Stellar velocity at 2Re (vel_ssp_2)km/sphys.velocdoublenullablee_Vels2Re[0.029/696]? Vels2Re uncertainty (e_vel_ssp_2)km/sstat.errorfloatnullableVelHa2Re[0/1542]? H{alpha} velocity at 2Re (vel_Ha_2)km/sphys.velocdoublenullablee_VelHa2Re[0/919]? VelHa2Re uncertainty (e_vel_Ha_2)km/sstat.errorfloatnullableVels1Re[0.028/1580]? Stellar velocity at 1Re (vel_ssp_1)km/sphys.velocdoublenullablee_Vels1Re[0/875]? Vels1Re uncertainty (e_vel_ssp_1)km/sstat.errorfloatnullableVelHa1Re[0.01/2244]? H{alpha} velocity at 1Re (vel_Ha_1)km/sphys.velocdoublenullablee_VelHa1Re[0/865]? VelHa1Re uncertainty (e_vel_Ha_1)km/sstat.errorfloatnullablelogSFRs100[-4/1.9]? Integrated SFR derived from the SSP analysis for t<100Myr (log_SFR_ssp_100Myr)log(solMass.yr**-1)phys.SFRfloatnullableVdispHa1re[0.09/703]? H{alpha} velocity dispersion at 1Re (vel_disp_Ha_1Re)km/sphys.veloc.dispersionfloatnullableVdisps1Re[6/490]? Stellar velocity dispersion at 1Re (vel_disp_ssp_1Re)km/sphys.veloc.dispersionfloatnullablelogM1Re[5.9/16]? Integrated stellar mass within 1 optical Re (log_Mass_in_Re)log(solMass)phys.massfloatnullableMLint[0.2/4.4e+7] V-band mass-to-light ratio from integrated quantities (ML_int)solMass/solLumphys.composition.massLightRatiodoubleMLavg[0.00029/547] V-band mass-to-light ratio averaged across the FOV (ML_avg)solMass/solLumphys.composition.massLightRatiodoubleFHac[0/4454] Flux intensity of H{alpha} in the central aperture in 10^-16^erg/s/cm^2^ (F_Ha_cen)1e-19W.m**-2phot.fluxdoubleR50V[0.1/45]? Radius at which half of the light in the V-band within the FOV is integrated (R50_kpc_V)kpcphys.size.radiusfloatnullablee_R50V[0.02/14]? R50V uncertainty (e_R50_kpc_V)kpcstat.errorfloatnullableR50M[0.1/44.1]? Radius at which half of the stellar mass within the FOV is integrated (R50_kpc_Mass)kpcphys.size.radiusfloatnullablee_R50M[0.02/14]? R50M uncertainty (e_R50_kpc_Mass)kpcstat.errorfloatnullablelogMR50V[5.8/15.8]? Integrated stellar mass within R50V (log_Mass_corr_in_R50_V)log(solMass)phys.massfloatnullablee_logMR50V[0/1] logMR50V uncertainty (e_log_Mass_corr_in_R50_V)log(solMass)stat.errorfloatlogMgasAvgl[2.59/11.7]? Molecular gas mass derived from the dust extinction using the log-log calibration (log_Mass_gas_Av_gas_log_log)log(solMass)phys.massfloatnullableAvgas1Re[4.4e-5/3.4]? Dust extinction in the V band derived from the H{alpha}/H{beta} line ratio at 1Re (Av_gas_Re)magphys.absorptiondoublenullablee_Avgas1Re[0/1.3]? Avgas1Re uncertainty (e_Av_gas_Re)magstat.errordoublenullableAvs[5.9e-5/1.8]? Dust extinction in the V band derived from the analysis of the stellar population (Av_ssp_Re)magphys.absorptiondoublenullablee_Avs[0/0.6]? Avs uncertainty (e_Av_ssp_Re)magstat.errordoublenullableLambda1Re[0.014/1]? Specific angular momentum ({lambda}-parameter) for the stellar populations within 1Re (Lambda_Re)phys.angMomentumdoublenullablee_Lambda1Re[7e-6/0.5]? Lambda1Re uncertainty (e_Lambda_Re)stat.errordoublenullablezNSA[0.0002/0.15]? NSA redshift (nsa_redshift)src.redshift;pos.heliocentricdoublenullableMNSA[6.2/13.2]? Stellar mass derived by the NSA collaboration (nsa_mstar)log(solMass)phys.massfloatnullableIncNSA[4/86]? Inclination derived by the NSA collaboration (nsa_inclination)degsrc.orbital.inclinationfloatnullableF[OII]26Re[-2.4/16]? Flux intensity of [OII]3726.03 at 1Re in 10^-16^erg/s/cm^2^ (flux_OII3726_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[OII]26Re[0.00037/4]? F[OII]26Re uncertainty (e_flux_OII3726_Re_fit)1e-19W.m**-2stat.errordoublenullableF[OII]28a[-11/2.3]? Flux intensity of [OII]3728.82 at 1Re in 10^-16^erg/s/cm^2^ (flux_OII3728_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[OII]28a[0.0004/3]? F[OII]28a uncertainty (e_flux[OII]3728.82_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHI34Re[-2.5/16]? Flux intensity of HI3734.37 at 1Re in 10^-16^erg/s/cm^2^ (flux_HI3734_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHI34Re[0.0003/2.3]? FHI34Re uncertainty (e_flux_HI3734_Re_fit)1e-19W.m**-2stat.errordoublenullableFHI34a[-11/1.4]? Flux intensity of HI3734.37 at 1Re in 10^-16^erg/s/cm^2^ (flux_HI3734_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHI34a[0.00027/2]? FHI34a uncertainty (e_flux_HI3734_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHI97Re[-2.1/4.8]? Flux intensity of HI3797.9 at 1Re in 10^-16^erg/s/cm^2^ (flux_HI3797.9_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHI97Re[0.00024/5]? FHI97Re uncertainty (e_flux_HI3797_Re_fit)1e-19W.m**-2stat.errordoublenullableFHI97a[-5.82/1.1]? Flux intensity of HI3797.9 at 1Re in 10^-16^erg/s/cm^2^ (flux_HI3797_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHI97a[0.0002/4.5]? FHI97a uncertainty (e_flux_HI3797_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHeI38Re[-0.3/8]? Flux intensity of HeI3888.65 at 1Re in 10^-16^erg/s/cm^2^ (flux_HeI3888_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHeI38Re[0.00035/2.2]? FHeI38Re uncertainty (e_flux_HeI3888_Re_fit)1e-19W.m**-2stat.errordoublenullableFHeI38a[-4.8/0.7]? Flux intensity of HeI3888.65 at 1Re in 10^-16^erg/s/cm^2^ (flux_HeI3888_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHeI38a[0.0003/1.7]? FHeI38a uncertainty (e_flux_HeI3888_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHI89Re[-0.31/8]? Flux intensity of HI3889.05 at 1Re in 10^-16^erg/s/cm^2^ (flux_HI3889_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHI89Re[0.00027/5]? FHI89Re uncertainty (e_flux_HI3889_Re_fit)1e-19W.m**-2stat.errordoublenullableFHI89a[-4.8/2]? Flux intensity of HI3889.05 at 1Re in 10^-16^erg/s/cm^2^ (flux_HI3889_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHI89a[0.0002/4]? FHI89a uncertainty (e_flux_HI3889_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHeI39Re[-0.83/11]? Flux intensity of HeI3964.73 at 1Re in 10^-16^erg/s/cm^2^ (flux_HeI3964_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHeI39Re[0.00028/1.2]? FHeI39Re uncertainty (e_flux_HeI3964_Re_fit)1e-19W.m**-2stat.errordoublenullableFHeI39a[-7/1.4]? Flux intensity of HeI3964.73 at 1Re in 10^-16^erg/s/cm^2^ (flux_HeI3964_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[NeIII]a[0.00024/2.4]? F[NeIII]a uncertainty (e_fluxNeIII3967_alpha_fit)1e-19W.m**-2stat.errordoublenullableFCaIIRe[-0.72/10.4]? Flux intensity of CaII3968.47 at 1Re in 10^-16^erg/s/cm^2^ (flux_CaII3968_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FCaIIRe[0.00026/2.6]? FCaIIRe uncertainty (e_flux_CaII3968_Re_fit)1e-19W.m**-2stat.errordoublenullableFCaIIa[-7.4/1.2]? Flux intensity of CaII3968.47 at 1Re in 10^-16^erg/s/cm^2^ (flux_CaII3968_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FCaIIa[0.0002/2.2]? FCaIIa uncertainty (e_flux_CaII3968_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHepsRe[-0.7/10.4]? Flux intensity of H{epsilon}3970.07 at 1Re in 10^-16^erg/s/cm^2^ (flux_Hepsilon3970_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHepsRe[0.00025/2.4]? FHepsRe uncertainty (e_fluxHepsilon3970_Re_fit)1e-19W.m**-2stat.errordoublenullableFHepsa[-8.81/1.6]? Flux intensity of H{epsilon}3970.07 at 1Re in 10^-16^erg/s/cm^2^ (flux_Heps3970_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHepsa[0.0002/2.1]? FHepsa uncertainty (e_flux_Heps3970.07_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHdRe[-0.099/9.7]? Flux intensity of H{delta}4101.77 at 1Re in 10^-16^erg/s/cm^2^ (flux_Hdelta4101_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHdRe[0.0003/4.3]? FHdRe uncertainty (e_flux_Hdelta4101_Re_fit)1e-19W.m**-2stat.errordoublenullableFHda[-5.4/2]? Flux intensity of H{delta}4101.77 at 1Re in 10^-16^erg/s/cm^2^ (flux_Hdelta4101_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHda[0.00028/3.6]? FHda uncertainty (e_flux_Hdel4101_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHgRe[-1.25/11.9]? Flux intensity of H{gamma}4340.49 at 1Re in 10^-16^erg/s/cm^2^ (flux_Hgamma4340_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHgRe[0.0002/5.3]? FHgRe uncertainty (e_flux_Hgamma4340_Re_fit)1e-19W.m**-2stat.errordoublenullableFHga[-7/6.6]? Flux intensity of H{gamma}4340.49 at 1Re in 10^-16^erg/s/cm^2^ (flux_Hgamma4340_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHga[0.00018/4]? FHga uncertainty (e_flux_Hgam4340_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHbRe[-0.24/14.7]? Flux intensity of H{beta}4861.36 at 1Re in 10^-16^erg/s/cm^2^ (flux_Hbeta4861_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHbRe[0.00024/8.1]? FHbRe uncertainty (e_flux_Hbeta4861_Re_fit)1e-19W.m**-2stat.errordoublenullableFHba[-8.1/0.7]? Flux intensity of H{beta}4861.36 at 1Re in 10^-16^erg/s/cm^2^ (flux_Hbeta4861_alpha_fit)1e-19W.m**-2phot.fluxdoublenullableF[OIII]49a[-9.3/1.3]? Flux intensity of [OIII]4958.91 at 1Re in 10^-16^erg/s/cm^2^ (flux_OIII4958_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[OIII]49a[0.00017/11]? F[OIII]49a uncertainty (e_fluxOIII4958_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[OIII]50Re[-1.8/12]? Flux intensity of [OIII]5006.84 at 1Re in 10^-16^erg/s/cm^2^ (flux_OIII5006_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[OIII]50Re[0.0002/3.5]? F[OIII]50Re uncertainty (e_flux_OIII5006_Re_fit)1e-19W.m**-2stat.errordoublenullableF[OIII]50a[-12.6/1.1]? Flux intensity of [OIII]5006.84 at 1Re in 10^-16^erg/s/cm^2^ (flux_OIII5006_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[OIII]50a[0.00018/3]? F[OIII]50a uncertainty (e_fluxOIII5006_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHeI50Re[-2.2/8]? Flux intensity of HeI5015.68 at 1Re in 10^-16^erg/s/cm^2^ (flux_HeI5015_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHeI50Re[0.0002/3.5]? FHeI50Re uncertainty (e_flux_HeI5015_Re_fit)1e-19W.m**-2stat.errordoublenullableFHeI50a[-11/2]? Flux intensity of HeI5015.68 at 1Re in 10^-16^erg/s/cm^2^ (flux_HeI5015_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHeI50a[0.00018/2.5]? FHeI50a uncertainty (e_flux_HeI5015_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[NI]51Re[-0.22/4]? Flux intensity of [NI]5197.9 at 1Re in 10^-16^erg/s/cm^2^ (flux_NI5197_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[NI]51Re[0.00016/4.2]? F[NI]51Re uncertainty (e_flux_NI5197_Re_fit)1e-19W.m**-2stat.errordoublenullableF[NI]51a[-4.1/0.7]? Flux intensity of [NI]5197.9 at 1Re in 10^-16^erg/s/cm^2^ (flux_NI5197_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[NI]51a[0.00014/3.4]? F[NI]51a uncertainty (e_flux_NI5197_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[NI]52Re[-0.34/1.7]? Flux intensity of [NI]5200.26 at 1Re in 10^-16^erg/s/cm^2^ (flux_NI5200_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[NI]52Re[0.00018/3.1]? F[NI]52Re uncertainty (e_flux_NI5200_Re_fit)1e-19W.m**-2stat.errordoublenullableF[NI]52a[-2.6/1.1]? Flux intensity of [NI]5200.26 at 1Re in 10^-16^erg/s/cm^2^ (flux_NI5200_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[NI]52a[0.00015/3]? F[NI]52a uncertainty (e_flux_NI5200_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHeI58Re[-0.6/2.2]? Flux intensity of HeI5876.0 at 1Re in 10^-16^erg/s/cm^2^ (flux_HeI5876_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHeI58Re[0.00017/1.7]? FHeI58Re uncertainty (e_flux_HeI5876_Re_fit)1e-19W.m**-2stat.errordoublenullableFHeI58a[-2.8/0.95]? Flux intensity of HeI5876.0 at 1Re in 10^-16^erg/s/cm^2^ (flux_HeI5876_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHeI58a[0.00014/1.5]? FHeI58a uncertainty (e_flux_HeI5876_alpha_fit)1e-19W.m**-2stat.errordoublenullablee_FNaI89a[0.0002/3.4]? FNaI89a uncertainty (e_flux_NaI5889_alpha_fit)1e-19W.m**-2stat.errordoublenullableFNaI95Re[-1.01/4.4]? Flux intensity of NaI5895.92 at 1Re in 10^-16^erg/s/cm^2^ (flux_NaI5895_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FNaI95Re[0.00019/4]? FNaI95Re uncertainty (e_flux_NaI5895_Re_fit)1e-19W.m**-2stat.errordoublenullableFNaI95a[-6.22/2.7]? Flux intensity of NaI5895.92 at 1Re in 10^-16^erg/s/cm^2^ (flux_NaI5895_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FNaI95a[0.00016/3.2]? FNaI95a uncertainty (e_flux_NaI5895_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[OI]Re[-1.13/2.6]? Flux intensity of [OI]6300.3 at 1Re in 10^-16^erg/s/cm^2^ (flux_OI6300_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[OI]Re[0.00014/3.3]? F[OI]Re uncertainty (e_flux_OI6300_Re_fit)1e-19W.m**-2stat.errordoublenullableF[OI]a[-5.4/0.7]? Flux intensity of [OI]6300.3 at 1Re in 10^-16^erg/s/cm^2^ (flux_OI6300_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[OI]a[0.00012/2.7]? F[OI]a uncertainty (e_flux_OI6300_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[NII]48Re[-0.3/12.4]? Flux intensity of [NII]6548.05 at 1Re in 10^-16^erg/s/cm^2^ (flux_NII6548_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[NII]48Re[0.00016/3.4]? F[NII]48Re uncertainty (e_flux_NII6548_Re_fit)1e-19W.m**-2stat.errordoublenullableF[NII]48a[-10.1/0.6]? Flux intensity of [NII]6548.05 at 1Re in 10^-16^erg/s/cm^2^ (flux_NII6548_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[NII]48a[0.00014/2.5]? F[NII]48a uncertainty (e_flux_NII6548_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHaRe[-0.22/20.2]? Flux intensity of H{alpha}6562.85 at 1Re in 10^-16^erg/s/cm^2^ (flux_Halpha6562_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHaRe[0.00017/17.6]? FHaRe uncertainty (e_flux_Halpha6562_Re_fit)1e-19W.m**-2stat.errordoublenullableFHaa[-13/5.1]? Flux intensity of H{alpha}6562.85 at 1Re in 10^-16^erg/s/cm^2^ (flux_Halpha6562_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHaa[0.00015/10.6]? FHaa uncertainty (e_flux_Ha6562_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[NII]83Re[-0.3/16]? Flux intensity of [NII]6583.45 at 1Re in 10^-16^erg/s/cm^2^ (flux_NII6583_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[NII]83Re[0.0002/4.5]? F[NII]83Re uncertainty (e_flux_NII6583_Re_fit)1e-19W.m**-2stat.errordoublenullableF[NII]83a[-13/1]? Flux intensity of [NII]6583.45 at 1Re in 10^-16^erg/s/cm^2^ (flux_NII6583_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[NII]83a[0.00017/3.2]? F[NII]83a uncertainty (e_flux_NII6583_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[SII]16Re[-0.6/5.5]? Flux intensity of [SII]6716.44 at 1Re in 10^-16^erg/s/cm^2^ (flux_SII6716_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[SII]30Re[0.00017/2.1]? F[SII]30Re uncertainty (e_flux_SII6730_Re_fit)1e-19W.m**-2stat.errordoublenullableF[SII]30a[-5/1]? Flux intensity of [SII]6730.82 at 1Re in 10^-16^erg/s/cm^2^ (flux_SII6730_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[SII]30a[0.00014/1.8]? F[SII]30a uncertainty (e_flux_SII6730_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[ArIII]Re[-0.95/1.7]? Flux intensity of [ArIII]7135.8 at 1Re in 10^-16^erg/s/cm^2^ (flux_ArIII7135_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[ArIII]Re[0.00016/2.5]? F[ArIII]Re uncertainty (e_flux_ArIII7135_Re_fit)1e-19W.m**-2stat.errordoublenullableF[ArIII]a[-3/0.7]? Flux intensity of [ArIII]7135.8 at 1Re in 10^-16^erg/s/cm^2^ (flux_ArIII7135_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[ArIII]a[0.00015/2]? F[ArIII]a uncertainty (e_flux_ArIII7135_alpha_fit)1e-19W.m**-2stat.errordoublenullableFHI14Re[-1.6/2.2]? Flux intensity of HI9014.91 at 1Re in 10^-16^erg/s/cm^2^ (flux_HI9014_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHI14Re[0.00012/3]? FHI14Re uncertainty (e_flux_HI9014_Re_fit)1e-19W.m**-2stat.errordoublenullableFHI14a[-3.1/1.3]? Flux intensity of HI9014.91 at 1Re in 10^-16^erg/s/cm^2^ (flux_HI9014_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_FHI14a[0.0001/2.5]? FHI14a uncertainty (e_flux_HI9014_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[SIII]90Re[-0.5/3.4]? Flux intensity of [SIII]9069.0 at 1Re in 10^-16^erg/s/cm^2^ (flux_SIII9069_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[SIII]90Re[0.0001/3]? F[SIII]90Re uncertainty (e_flux_SIII9069_Re_fit)1e-19W.m**-2stat.errordoublenullableF[SIII]90a[-2.8/3]? Flux intensity of [SIII]9069.0 at 1Re in 10^-16^erg/s/cm^2^ (flux_SIII9069_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[SIII]90a[9.6e-5/2.6]? F[SIII]90a uncertainty (e_flux_SIII9069_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[FeII]Re[-0.91/0.71]? Flux intensity of [FeII]9470.93 at 1Re in 10^-16^erg/s/cm^2^ (flux_FeII9470_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[FeII]Re[0.00018/1.4]? F[FeII]Re uncertainty (e_flux_FeII9470_Re_fit)1e-19W.m**-2stat.errordoublenullableF[FeII]a[-1.2/0.5]? Flux intensity of [FeII]9470.93 at 1Re in 10^-16^erg/s/cm^2^ (flux_FeII9470_alpha_fit)1e-19W.m**-2phot.fluxdoublenullablee_F[FeII]a[0.00016/1.1]? F[FeII]a uncertainty (e_flux_FeII9470_alpha_fit)1e-19W.m**-2stat.errordoublenullableF[SIII]95Re[-0.92/8]? Flux intensity of [SIII]9531.1 at 1Re in 10^-16^erg/s/cm^2^ (flux_SIII9531_Re_fit)1e-19W.m**-2phot.fluxdoublenullablee_OH-Mar13-O3N2Re[0.00068/0.4]? OH-Mar13-O3N2Re uncertainty (e_OH_Mar13_O3N2_Re_fit)stat.errordoublenullableOH-Mar13-O3N2a[-0.42/0.3]? Slope of the O/H gradient using the calibrator Mar13_O3N2 in dex/Re (OH_Mar13_O3N2_alpha_fit)arith.grad;phys.abunddoublenullablee_OH-Mar13-O3N2a[0.00058/0.22]? OH-Mar13-O3N2a uncertainty (e_OH_Mar13_O3N2_alpha_fit)stat.errordoublenullableOH-T04Re[7/11]? Oxygen abundance using the calibrator T04 at 1Re (OH_T04_Re_fit) (1)phys.abundfloatnullablee_OH-T04Re[0.003/5.1]? OH-T04Re uncertainty (e_OH_T04_Re_fit)stat.errorfloatnullableOH-T04a[-3.9/2.8]? Slope of the O/H gradient using the calibrator T04 in dex/Re (OH_T04_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-T04a[0.0029/3.1]? OH-T04a uncertainty (e_OH_T04_alpha_fit)stat.errorfloatnullableOH-Pet04-N2linRe[7.9/9]? Oxygen abundance using the calibrator Pet04_N2_lin at 1Re (OH_Pet04_N2_lin_Re_fit) (1)phys.abundfloatnullablee_OH-Pet04-N2linRe[0.001/0.5]? OH-Pet04-N2linRe uncertainty (e_OH_Pet04_N2_lin_Re_fit)stat.errorfloatnullableOH-Pet04-N2lina[-0.9/0.6]? Slope of the O/H gradient using the calibrator Pet04_N2_lin in dex/Re (OH_Pet04_N2_lin_alpha_fit)arith.grad;phys.abunddoublenullablee_OH-Pet04-N2lina[0.0008/0.3]? OH-Pet04-N2lina uncertainty (e_OH_Pet04_N2_lin_alpha_fit)stat.errordoublenullableOH-Pet04-N2polRe[7.9/9.1]? Oxygen abundance using the calibrator Pet04_N2_poly at 1Re (OH_Pet04_N2_poly_Re_fit) (1)phys.abundfloatnullablee_OH-Pet04-N2polRe[0.002/0.6]? OH-Pet04-N2polRe uncertainty (e_OH_Pet04_N2_poly_Re_fit)stat.errorfloatnullableOH-Pet04-N2pola[-0.9/0.6]? Slope of the O/H gradient using the calibrator Pet04_N2_poly in dex/Re (OH_Pet04_N2_poly_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-Pet04-N2pola[0.0017/0.4]? OH-Pet04-N2pola uncertainty (e_OH_Pet04_N2_poly_alpha_fit)stat.errorfloatnullablee_OH-Pil11-NSRe[0.001/2.6]? OH-Pil11-NSRe uncertainty (e_OH_Pil11_NS_Re_fit)stat.errorfloatnullableOH-Pil11-NSa[-1.7/3.4]? Slope of the O/H gradient using the calibrator Pil11_NS in dex/Re (OH_Pil11_NS_alpha_fit)arith.grad;phys.abunddoublenullablee_OH-Pil11-NSa[0.0009/2.2]? OH-Pil11-NSa uncertainty (e_OH_Pil11_NS_alpha_fit)stat.errordoublenullableOH-Cur20-RS32Re[7.9/9]? Oxygen abundance using the calibrator Cur20_RS32 at 1Re (OH_Cur20_RS32_Re_fit) (1)phys.abundfloatnullablee_OH-Cur20-RS32Re[0.001/0.6]? OH-Cur20-RS32Re uncertainty (e_OH_Cur20_RS32_Re_fit)stat.errorfloatnullableOH-Cur20-RS32a[-0.6/0.8]? Slope of the O/H gradient using the calibrator Cur20_RS32 in dex/Re (OH_Cur20_RS32_alpha_fit)arith.grad;phys.abunddoublenullablee_OH-Cur20-RS32a[0.0008/0.5]? OH-Cur20-RS32a uncertainty (e_OH_Cur20_RS32_alpha_fit)stat.errordoublenullableOH-Cur20-R3Re[7.9/9]? Oxygen abundance using the calibrator Cur20_R3 at 1Re (OH_Cur20_R3_Re_fit) (1)phys.abundfloatnullablee_OH-Cur20-R3Re[0.001/0.6]? OH-Cur20-R3Re uncertainty (e_OH_Cur20_R3_Re_fit)stat.errorfloatnullableOH-Cur20-R3a[-0.6/0.8]? Slope of the O/H gradient using the calibrator Cur20_R3 in dex/Re (OH_Cur20_R3_alpha_fit)arith.grad;phys.abunddoublenullablee_OH-Cur20-R3a[0.0009/0.4]? OH-Cur20-R3a uncertainty (e_OH_Cur20_R3_alpha_fit)stat.errordoublenullableOH-Cur20-O3O2Re[7.9/9]? Oxygen abundance using the calibrator Cur20_O3O2 at 1Re (OH_Cur20_O3O2_Re_fit) (1)phys.abundfloatnullablee_OH-Cur20-O3O2Re[0.0013/0.7]? OH-Cur20-O3O2Re uncertainty (e_OH_Cur20_O3O2_Re_fit)stat.errorfloatnullableOH-Cur20-O3O2a[-0.6/0.5]? Slope of the O/H gradient using the calibrator Cur20_O3O2 in dex/Re (OH_Cur20_O3O2_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-Cur20-O3O2a[0.001/0.6]? OH-Cur20-O3O2a uncertainty (e_OH_Cur20_O3O2_alpha_fit)stat.errorfloatnullableOH-Cur20-S2Re[7.8/9]? Oxygen abundance using the calibrator Cur20_S2 at 1Re (OH_Cur20_S2_Re_fit) (1)phys.abundfloatnullablee_OH-Cur20-S2Re[0.0017/1.2]? OH-Cur20-S2Re uncertainty (e_OH_Cur20_S2_Re_fit)stat.errorfloatnullableOH-Cur20-S2a[-0.8/0.9]? Slope of the O/H gradient using the calibrator Cur20_S2 in dex/Re (OH_Cur20_S2_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-Cur20-S2a[0.0016/0.8]? OH-Cur20-S2a uncertainty (e_OH_Cur20_S2_alpha_fit)stat.errorfloatnullableOH-Cur20-R2Re[7.9/9]? Oxygen abundance using the calibrator Cur20_R2 at 1Re (OH_Cur20_R2_Re_fit) (1)phys.abundfloatnullablee_OH-Cur20-R2Re[0.0019/0.5]? OH-Cur20-R2Re uncertainty (e_OH_Cur20_R2_Re_fit)stat.errorfloatnullableOH-Cur20-R2a[-0.5/1.1]? Slope of the O/H gradient using the calibrator Cur20_R2 in dex/Re (OH_Cur20_R2_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-Cur20-R2a[0.0018/0.4]? OH-Cur20-R2a uncertainty (e_OH_Cur20_R2_alpha_fit)stat.errorfloatnullableOH-Cur20-N2Re[7.9/9]? Oxygen abundance using the calibrator Cur20_N2 at 1Re (OH_Cur20_N2_Re_fit) (1)phys.abundfloatnullablee_OH-Cur20-N2Re[0.0014/0.6]? OH-Cur20-N2Re uncertainty (e_OH_Cur20_N2_Re_fit)stat.errorfloatnullableOH-Cur20-N2a[-0.8/0.6]? Slope of the O/H gradient using the calibrator Cur20_N2 in dex/Re (OH_Cur20_N2_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-Cur20-N2a[0.0012/0.4]? OH-Cur20-N2a uncertainty (e_OH_Cur20_N2_alpha_fit)stat.errorfloatnullableOH-Cur20-R23Re[7.8/9]? Oxygen abundance using the calibrator Cur20_R23 at 1Re (OH_Cur20_R23_Re_fit) (1)phys.abundfloatnullablee_OH-Cur20-R23Re[0.0025/0.8]? OH-Cur20-R23Re uncertainty (e_OH_Cur20_R23_Re_fit)stat.errorfloatnullableOH-Cur20-R23a[-1.2/0.7]? Slope of the O/H gradient using the calibrator Cur20_R23 in dex/Re (OH_Cur20_R23_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-Cur20-R23a[0.002/0.7]? OH-Cur20-R23a uncertainty (e_OH_Cur20_R23_alpha_fit)stat.errorfloatnullableOH-Cur20-O3N2Re[8/9]? Oxygen abundance using the calibrator Cur20_O3N2 at 1Re (OH_Cur20_O3N2_Re_fit) (1)phys.abunddoublenullablee_OH-Cur20-O3N2Re[0.0007/0.5]? OH-Cur20-O3N2Re uncertainty (e_OH_Cur20_O3N2_Re_fit)stat.errordoublenullableOH-Cur20-O3N2a[-0.6/0.4]? Slope of the O/H gradient using the calibrator Cur20_O3N2 in dex/Re (OH_Cur20_O3N2_alpha_fit)arith.grad;phys.abunddoublenullablee_OH-Cur20-O3N2a[0.0006/0.3]? OH-Cur20-O3N2a uncertainty (e_OH_Cur20_O3N2_alpha_fit)stat.errordoublenullableOH-Cur20-O3S2Re[8/9]? Oxygen abundance using the calibrator Cur20_O3S2 at 1Re (OH_Cur20_O3S2_Re_fit) (1)phys.abundfloatnullablee_OH-Cur20-O3S2Re[0.002/0.9]? OH-Cur20-O3S2Re uncertainty (e_OH_Cur20_O3S2_Re_fit)stat.errorfloatnullableOH-Cur20-O3S2a[-0.8/0.6]? Slope of the O/H gradient using the calibrator Cur20_O3S2 in dex/Re (OH_Cur20_O3S2_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-Cur20-O3S2a[0.0019/0.7]? OH-Cur20-O3S2a uncertainty (e_OH_Cur20_O3S2_alpha_fit)stat.errorfloatnullableOH-KK04Re[7.8/9.8]? Oxygen abundance using the calibrator KK04 at 1Re (OH_KK04_Re_fit) (1)phys.abunddoublenullablee_OH-KK04Re[0.0008/2.1]? OH-KK04Re uncertainty (e_OH_KK04_Re_fit)stat.errordoublenullableOH-KK04a[-1.8/3.4]? Slope of the O/H gradient using the calibrator KK04 in dex/Re (OH_KK04_alpha_fit)arith.grad;phys.abunddoublenullablee_OH-KK04a[0.0007/2.1]? OH-KK04a uncertainty (e_OH_KK04_alpha_fit)stat.errordoublenullableOH-Pil16-RRe[7/9.1]? Oxygen abundance using the calibrator Pil16_R at 1Re (OH_Pil16_R_Re_fit) (1)phys.abundfloatnullablee_OH-Pil16-RRe[0.0019/2.4]? OH-Pil16-RRe uncertainty (e_OH_Pil16_R_Re_fit)stat.errorfloatnullableOH-Pil16-Ra[-1.6/1.5]? Slope of the O/H gradient using the calibrator Pil16_R in dex/Re (OH_Pil16_R_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-Pil16-Ra[0.0016/1.7]? OH-Pil16-Ra uncertainty (e_OH_Pil16_R_alpha_fit)stat.errorfloatnullableOH-Pil16-SRe[7.2/9]? Oxygen abundance using the calibrator Pil16_S at 1Re (OH_Pil16_S_Re_fit) (1)phys.abundfloatnullablee_OH-Pil16-SRe[0.0014/1.4]? OH-Pil16-SRe uncertainty (e_OH_Pil16_S_Re_fit)stat.errorfloatnullableOH-Pil16-Sa[-1.8/1.5]? Slope of the O/H gradient using the calibrator Pil16_S in dex/Re (OH_Pil16_S_alpha_fit)arith.grad;phys.abundfloatnullablee_OH-Pil16-Sa[0.0012/1.4]? OH-Pil16-Sa uncertainty (e_OH_Pil16_S_alpha_fit)stat.errorfloatnullableOH-HoRe[7.7/9.6]? Oxygen abundance using the calibrator Ho at 1Re (OH_Ho_Re_fit) (1)phys.abundfloatnullablee_OH-HoRe[0.0015/1.1]? OH-HoRe uncertainty (e_OH_Ho_Re_fit)stat.errorfloatnullablee_OH-Hoa[0.0013/1.2]? OH-Hoa uncertainty (e_OH_Ho_alpha_fit)stat.errorfloatnullableU-Dors-O32Re[-4.5/-1]? Log(U) ionization parameter using the calibrator Dors_O32 at 1Re (U_Dors_O32_Re_fit) (1)phys.ionizParam.radfloatnullablee_U-Dors-O32Re[0.0048/3]? U-Dors-O32Re uncertainty (e_U_Dors_O32_Re_fit)stat.errorfloatnullableU-Dors-O32a[-1.93/2.4]? Slope of the log(U) gradient using the calibrator Dors_O32 in dex/Re (U_Dors_O32_alpha_fit)phys.ionizParam.radfloatnullablee_U-Dors-O32a[0.004/2]? U-Dors-O32a uncertainty (e_U_Dors_O32_alpha_fit)stat.errorfloatnullableU-Dors-SRe[-5.21/1.8]? Log(U) ionization parameter using the calibrator Dors_S at 1Re (U_Dors_S_Re_fit) (1)phys.ionizParam.radfloatnullablee_U-Dors-SRe[0.004/4]? U-Dors-SRe uncertainty (e_U_Dors_S_Re_fit)stat.errorfloatnullableU-Dors-Sa[-3.1/2.4]? Slope of the log(U) gradient using the calibrator Dors_S in dex/Re (U_Dors_S_alpha_fit)phys.ionizParam.radfloatnullablee_U-Dors-Sa[0.003/2.5]? U-Dors-Sa uncertainty (e_U_Dors_S_alpha_fit)stat.errorfloatnullableU-Mor16-O23fsRe[-7/-0.3]? Log(U) ionization parameter using the calibrator Mor16_O23_fs at 1Re (U_Mor16_O23_fs_Re_fit) (1)phys.ionizParam.radfloatnullablee_U-Mor16-O23fsRe[0.009/6]? U-Mor16-O23fsRe uncertainty (e_U_Mor16_O23_fs_Re_fit)stat.errorfloatnullableU-Mor16-O23fsa[-3.8/4.5]? Slope of the log(U) gradient using the calibrator Mor16_O23_fs in dex/Re (U_Mor16_O23_fs_alpha_fit)phys.ionizParam.radfloatnullablee_U-Mor16-O23fsa[0.007/4]? U-Mor16-O23fsa uncertainty (e_U_Mor16_O23_fs_alpha_fit)stat.errorfloatnullableU-Mor16-O23tsRe[-4.7/-1.8]? Log(U) ionization parameter using the calibrator Mor16_O23_ts at 1Re (U_Mor16_O23_ts_Re_fit) (1)phys.ionizParam.radfloatnullablee_U-Mor16-O23tsRe[0.0039/2.4]? U-Mor16-O23tsRe uncertainty (e_U_Mor16_O23_ts_Re_fit)stat.errorfloatnullableU-Mor16-O23tsa[-1.6/2]? Slope of the log(U) gradient using the calibrator Mor16_O23_ts in dex/Re (U_Mor16_O23_ts_alpha_fit)phys.ionizParam.radfloatnullablee_U-Mor16-O23tsa[0.003/1.6]? U-Mor16-O23tsa uncertainty (e_U_Mor16_O23_ts_alpha_fit)stat.errorfloatnullableNH-Pil16RRe[5.3/9.1]? Nitrogen abundance using the calibrator Pil16_R at 1Re (NH_Pil16_R_Re_fit) (1)phys.abundfloatnullablee_NH-Pil16RRe[0.003/2]? NH-Pil16RRe uncertainty (e_NH_Pil16_R_Re_fit)stat.errorfloatnullableNH-Pil16Ra[-2.7/2.6]? Slope of the N/H gradient using the calibrator Pil16_R in dex/Re (NH_Pil16_R_alpha_fit)arith.grad;phys.abundfloatnullablee_NH-Pil16Ra[0.003/2]? NH-Pil16Ra uncertainty (e_NH_Pil16_R_alpha_fit)stat.errorfloatnullableNO-Pil16RRe[-2.7/0.5]? N/O abundance using the calibrator Pil16_R at 1Re (NO_Pil16_R_Re_fit) (1)phys.abundfloatnullablee_NO-Pil16RRe[0.003/3.1]? NO-Pil16RRe uncertainty (e_NO_Pil16_R_Re_fit)stat.errorfloatnullableNO-Pil16Ra[-2.4/1.9]? Slope of the N/O gradient using the calibrator Pil16_R in dex/Re (NO_Pil16_R_alpha_fit)arith.grad;phys.abundfloatnullableNO-Pil16-HoRRe[-3.5/0.5]? N/O abundance using the calibrator Pil16_Ho_R at 1Re (NO_Pil16_Ho_R_Re_fit) (1)phys.abundfloatnullablee_NO-Pil16-HoRRe[0.0028/2.3]? NO-Pil16-HoRRe uncertainty (e_NO_Pil16_Ho_R_Re_fit)stat.errorfloatnullableNO-Pil16-HoRa[-2.9/2.7]? Slope of the N/O gradient using the calibrator Pil16_Ho_R in dex/Re (NO_Pil16_Ho_R_alpha_fit)arith.grad;phys.abundfloatnullablee_NO-Pil16-HoRa[0.002/2.2]? NO-Pil16-HoRa uncertainty (e_NO_Pil16_Ho_R_alpha_fit)stat.errorfloatnullableNO-Pil16-N2R2Re[-1.61/-0.27]? N/O abundance using the calibrator Pil16_N2_R2 at 1Re (NO_Pil16_N2_R2_Re_fit) (1)phys.abundfloatnullablee_NO-Pil16-N2R2Re[0.0029/1.2]? NO-Pil16-N2R2Re uncertainty (e_NO_Pil16_N2_R2_Re_fit)stat.errorfloatnullableNO-Pil16-N2R2a[-1.2/1.1]? Slope of the N/O gradient using the calibrator Pil16_N2_R2 in dex/Re (NO_Pil16_N2_R2_alpha_fit) (1)arith.grad;phys.abundfloatnullablee_NO-Pil16-N2R2a[0.002/0.8]? NO-Pil16-N2R2a uncertainty (e_NO_Pil16_N2_R2_alpha_fit)stat.errorfloatnullableNe-Oster-SRe[1.39/3.6]? Electron density using the Oster_S estimator at 1Re (Ne_Oster_S_Re_fit)phys.density;phys.electronfloatnullablee_Ne-Oster-SRe[0.015/1]? Ne-Oster-SRe uncertainty (e_Ne_Oster_S_Re_fit)stat.errorfloatnullableNe-Oster-Sa[-0.98/1.6]? Slope of the n_e gradient using the Oster_S estimator in dex/Re (Ne_Oster_S_alpha_fit)arith.gradfloatnullablee_Ne-Oster-Sa[0.013/0.7]? Ne-Oster-Sa uncertainty (e_Ne_Oster_S_alpha_fit)stat.errorfloatnullableHdRe[-3.61/11]? Value of the Hd stellar index at 1Re in {AA} (Hd_Re_fit)0.1nmspect.indexfloatnullablee_HdRe[0.02/4.4]? HdRe uncertainty (e_Hd_Re_fit)0.1nmstat.errorfloatnullableHda[-32.3/17]? Slope of the gradient of the Hd index in {AA}/Re (Hd_alpha_fit)arith.gradfloatnullablee_Hda[0.03/6]? Hda uncertainty (e_Hd_alpha_fit)stat.errorfloatnullableHbRe[-2.02/16.2]? Value of the H{beta} stellar index at 1Re in {AA} (Hb_Re_fit)0.1nmspect.indexfloatnullablee_HbRe[0.018/6]? HbRe uncertainty (e_Hb_Re_fit)0.1nmstat.errorfloatnullableHba[-7.3/14]? Slope of the gradient of the H{beta} index in {AA}/Re (Hb_alpha_fit)stat.fit.paramfloatnullablee_Hba[0.015/7.5]? Hba uncertainty (e_Hb_alpha_fit)stat.errorfloatnullableMgbRe[-2.8/16.2]? Value of the Mgb stellar index at 1Re in {AA} (Mgb_Re_fit)0.1nmspect.indexfloatnullablee_MgbRe[0.019/6]? MgbRe uncertainty (e_Mgb_Re_fit)0.1nmstat.errorfloatnullableMgba[-8.8/17]? Slope of the gradient of the Mgb index in {AA}/Re (Mgb_alpha_fit)arith.gradfloatnullablee_Mgba[0.016/10]? Mgba uncertainty (e_Mgb_alpha_fit)stat.errorfloatnullableFe5270Re[-3.7/22.2]? Value of the Fe5270 stellar index at 1Re in {AA} (Fe5270_Re_fit)0.1nmphot.fluxfloatnullablee_Fe5270Re[0.017/5]? Fe5270Re uncertainty (e_Fe5270_Re_fit)0.1nmstat.errorfloatnullableFe5270a[-9.3/32]? Slope of the gradient of the Fe5270 index in {AA}/Re (Fe5270_alpha_fit)phot.fluxfloatnullableFe5335Re[-3.8/21]? Value of the Fe5335 stellar index at 1Re in {AA} (Fe5335_Re_fit)0.1nmphot.fluxfloatnullablee_Fe5335Re[0.016/18]? Fe5335Re uncertainty (e_Fe5335_Re_fit)0.1nmstat.errorfloatnullableFe5335a[-12/24]? Slope of the gradient of the Fe5335 index in {AA}/Re (Fe5335_alpha_fit)phot.fluxfloatnullablee_Fe5335a[0.013/12]? Fe5335a uncertainty (e_Fe5335_alpha_fit)stat.errorfloatnullableD4000Re[0.57/4.6]? Value of the D4000 stellar index at 1Re (D4000_Re_fit1)spect.indexfloatnullablee_D4000Re[0.002/1.3]? D4000Re uncertainty (e_D4000_Re_fit)stat.errorfloatnullableD4000a[-0.8/6]? Slope of the gradient of the D4000 index (D4000_alpha_fit)arith.gradfloatnullablee_D4000a[0.002/1.5]? D4000a uncertainty (e_D4000_alpha_fit)stat.errorfloatnullableHdmodRe[-3.2/14]? Value of the Hdmod stellar index at 1Re in {AA} (Hdmod_Re_fit)0.1nmspect.indexfloatnullablee_HdmodRe[0.05/6]? HdmodRe uncertainty (e_Hdmod_Re_fit)0.1nmstat.errorfloatnullableHdmoda[-27/24]? Slope of the gradient of the Hdmod index in {AA}/Re (Hdmod_alpha_fit)arith.gradfloatnullablee_Hdmoda[0.04/10]? Hdmoda uncertainty (e_Hdmod_alpha_fit)stat.errorfloatnullableHgRe[-5/11]? Value of the Hg stellar index at 1Re in {AA} (Hg_Re_fit)0.1nmspect.indexfloatnullablee_HgRe[0.03/6]? HgRe uncertainty (e_Hg_Re_fit)0.1nmstat.errorfloatnullableHga[-5.4/10]? Slope of the gradient of the Hg index in {AA}/Re (Hg_alpha_fit)arith.gradfloatnullablee_Hga[0.027/6]? Hga uncertainty (e_Hg_alpha_fit)stat.errorfloatnullableumag[14.48/23.15] u-band magnitude derived from the original cube (u_band_mag)magphot.mag;em.opt.Ufloate_umag[0.05/6] Uncertainty on the umag (u_band_mag_error)magstat.error;phot.magfloatuMag[-24.64/-7.9] u-band absolute magnitude derived from the original cube (u_band_abs_mag)magphot.magfloate_uMag[0.05/6] uMag uncertainty (u_band_abs_mag_error)magstat.error;phot.magfloatgmag[13.41/20.83] g-band magnitude derived from the original cube (g_band_mag)magphot.mag;em.opt.Bfloate_gmag[0.05/1.1] Uncertainty on the gmag (g_band_mag_error)magstat.error;phot.magfloatgMag[-25.15/-8.61] g-band absolute magnitude derived from the original cube (g_band_abs_mag)magphys.magAbsfloate_gMag[0.05/1.1] gMag uncertainty (g_band_abs_mag_error)magstat.error;phot.magfloatrmag[12.75/20.4] r-band magnitude derived from the original cube (r_band_mag)magphot.mag;em.opt.Rfloate_rmag[0.05/1.2] Uncertainty on the rmag (r_band_mag_error)magstat.error;phot.magfloatrMag[-25.3/-8.7] r-band absolute magnitude derived from the original cube (r_band_abs_mag)magphys.magAbs;em.opt.Rfloate_rMag[0.05/1.2] rMag uncertainty (r_band_abs_mag_error)magstat.error;phot.magfloatimag[12.32/21.76] i-band magnitude derived from the original cube (i_band_mag)magphot.mag;em.opt.Ifloate_imag[0.05/17.1] Uncertainty on the imag (i_band_mag_error)magstat.error;phot.magfloatiMag[-25.4/-8.7] i-band absolute magnitude derived from the original cube (iMag)magphys.magAbs;em.opt.Ifloate_iMag[0.05/17.1] iMag uncertainty (iMag_error)magstat.error;phot.magfloatBmag[13.6/20.6] B-band magnitude derived from the original cube (B_band_mag)magphot.mag;em.opt.Bfloate_Bmag[0.05/0.8] Uncertainty on the Bmag (B_band_mag_error)magstat.error;phot.magfloatBMag[-25.04/-8.5] B-band absolute magnitude derived from the original cube (B_band_abs_mag)magphot.magfloate_BMag[0.05/0.8] BMag uncertainty (B_band_abs_mag_error)magstat.error;phot.magfloatVmag[13.12/21.3] V-band magnitude derived from the original cube (V_band_mag)magphot.mag;em.opt.Vfloate_Vmag[0.05/2] Uncertainty on the Vmag (V_band_mag_error)magstat.error;phot.magfloatVMag[-25.25/-8.6] V-band absolute magnitude derived from the original cube (V_band_abs_mag)magphot.magfloate_VMag[0.05/2] VMag uncertainty (V_band_abs_mag_error)magstat.error;phot.magfloatRJmag[12.66/20.35] R-band magnitude derived from the original cube (RJ_band_mag)magphot.mag;em.opt.RfloatRJMag[-25.3/-8.7] R-band absolute magnitude derived from the original cube (RJ_band_abs_mag)magphys.magAbs;em.opt.Rfloate_RJMag[0.05/1.3] RJMag uncertainty (RJ_band_abs_mag_error)magstat.error;phot.magfloatR50[1.9/23] Radius at which half of the light within the FOV in the g-band is integratedarcsecphys.angSize;srcdoublee_R50[2.7e-5/9.6] R50 uncertainty (error_R50)arcsecstat.errordoubleR90[3.8/30.2] Radius at which 90% of the light within the FOV in the g-band is integratedarcsecphys.angSize;srcdoublee_R90[6e-7/2] R90 uncertainty (error_R90)arcsecstat.errordoubleC[1/6] R90/R50 concentration indexmeta.code;spect.indexdoubleB-V[-1/1.5] B-V color indexmagphot.color;em.opt.B;em.opt.Vfloate_B-V[0.07/2.1] B-V uncertainty (error_B-V)magstat.error;phot.color;em.opt.BfloatB-R[-0.28/2.2] B-R color indexmagphot.color;em.opt.B;em.opt.Rfloate_B-R[0.07/1.6] B-R uncertainty (error_B-R)magstat.error;phot.color;em.opt.BfloatlogMph[4.7/12] Stellar masses derived from the photometric data within the FOV (log_Mass_phot)log(solMass)phys.massfloate_logMph[0.13/4] logMph uncertainty (e_log_Mass_phot)log(solMass)stat.errorfloatSBV1Re[17.8/38.9] V-band surface brightness at 1Re (V-band_SB_at_Re)mag.arcsec**-2phot.mag.sb;em.opt.Vfloate_SBV1Re[0/9] SBV1Re uncertainty (error_V-band_SB_at_Re)mag.arcsec**-2stat.errorfloatSBVR50[18/39] V-band surface brightness at R50 (V-band_SB_at_R_50)mag.arcsec**-2phot.mag.sb;em.opt.Vfloate_SBVR50[0/10] SBVR50 uncertainty (error_V-band_SB_at_R_50)mag.arcsec**-2stat.errorfloatnNSA[0.5/6] NSA Sersic index (nsa_sersic_n_morph)stat.fit.paramdoubleu-g[-3.2/9.2] u-g NSA color indexmagphot.color;em.opt.U;em.opt.Bdoubleg-r[-0.94/2.5] g-r NSA color indexmagphot.color;em.opt.B;em.opt.Rdoubler-i[-2.2/2] r-i NSA color indexmagphot.color;em.opt.R;em.opt.Idoublei-z[-7/2.8] i-z NSA color indexmagphot.color;em.opt.I;em.opt.IdoubleP(CD)[0/1] Probability of being a cD galaxystat.fit.goodnessdoubleP(E)[0/0.97] Probability of being an E galaxystat.fit.goodnessdoubleP(Sc)[0.0004/0.92] Probability of being an Sc galaxystat.fit.goodnessdoubleP(Scd)[0/0.93] Probability of being an Scd galaxystat.fit.goodnessdoubleP(Sd)[0/0.94] Probability of being an Sd galaxystat.fit.goodnessdoubleP(Sdm)[0/0.99] Probability of being an Sdm galaxystat.fit.goodnessdoubleP(Sm)[0/0.94] Probability of being an Sm galaxystat.fit.goodnessdoubleP(Irr)[0/0.96] Probability of being an Irr galaxystat.fit.goodnessdoubleType[-2/10]? Best morphological type index based on the NN analysis (best_type_n)meta.code;src.morph.type;meta.modelledintnullablew_Vmax[0/0.0012]? Weight for the volume correction in volume in Mpc^-3^/dex (Vmax_w)stat.weightdoublenullablew_Num[0/13314]? Weight for the volume correction in number (Num_w)stat.weightdoublenullableSloanDisplay the online SDSS-DR16 data for the nearest objectmeta.ref.urlchar