J/MNRAS/483/1754ivo://CDS.VizieR/J/MNRAS/483/1754doi:10.26093/cds/vizier.74831754CDSDu W.Cheng C.Wu H.Zhu M.Wang Y.2024-08-19T20:15:38Z2022-08-10T15:23:25ZCDS support team

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

cds-question@unistra.frgalaxiescatalogsphotometryvisible-astronomyapparent-magnitudegalaxy-classification-systemsWe present a catalogue of an HI-selected sample of 1129 low surface brightness galaxies (LSBGs) searched from the {alpha}.40-SDSS DR7 survey. This sample, consisting of various types of galaxies in terms of luminosity and morphology, has extended the parameter space covered by the existing LSBG samples. Based on a subsample of 173 LSBGs that are selected from our entire LSBG sample to have the 2-horn shapes of the HI line profiles, minor-to-major axial ratios (b/a) less than 0.6 and signal-to-noise ratio of HI detection greater than 6.5, we investigated the Tully-Fisher relation (TFr) of LSBGs in the optical B, g, and r bands and near-infrared (NIR) J, H, and K bands as well. In optical bands, the LSBG subsample follows the fundamental TFr that was previously defined for normal spiral galaxies. In NIR bands, the TFrs for our LSBG subsample are slightly different from the TFrs for the normal bright galaxies. This might be due to the internal extinction issue. Furthermore, the mass-to-light ratio (M/L), disc scale length (h), and mass surface density ({sigma}) for our LSBG subsample were deduced from the optical TFr results. Compared with high surface brightness galaxies (HSBGs), our LSBGs have higher M/L, larger h, and lower {sigma} than HSBGs.2019MNRAS.483.1754Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/483/1754CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/483/1754https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/483/1754http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/483/1754https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/483/1754https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/483/1754http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/483/1754GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/483/1754/table1 (Catalogue of our LSBG from the {alpha}.40-SDSS DR7)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/483/1754/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/483/1754/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/483/1754/table1?GETtext/xml+votable180.050000true0.929658915.21797610.0055555555555555565/1045 1146 2179 2573-2574 6601 6611 6616 6964 7109 6/549 554-555 723 725-727 904 907-908 911 915 920 922 945 2063 2070 2083 2181 2183 2195 2201 2248 4123 4126 4137 4148 4166-4169 4177 4187-4188 4196 4198-4199 4203 4208 4211 4223-4224 4229 4243 4245-4246 4250 4256 4258-4260 4277 4293 4297 4302 4304 4308-4309 4311 4313-4314 4324 4335 4352-4353 4355-4357 4363-4364 4371 4376 4378-4382 4385-4387 4395 4401-4402 4418 4424 4479 4481 4559 4565 4573 4591 4593 4600 4602 4630 4647-4648 4652 4673 4819 4821 4823 4826 4829-4830 4835 4837 4839 4842-4843 4845-4850 4852-4853 4856 4858 4885 4891 4901-4902 4907 4911 4919-4920 4928-4930 4936 4938 4960-4961 4992 4994 4998-4999 5001 5003 5144-5145 5147 5155 5160-5161 5168-5169 5173 5175 5178-5180 5186-5187 5189 5195-5196 5200 5254 5258 5280 6163 6165 6198 6211-6212 6214 6216 8217 8221-8223 8230-8232 8235-8236 8240 8247 8250 8254 8262-8264 8267 8269-8270 8274 8283 8290 8292 8298-8299 8303 8307 8309 8311 8315 8319-8321 8325 8327 8331 8337 8341 8343-8345 8347 8351 8357 8365-8367 8370-8371 8373 8375-8376 8378 8381-8383 8390 8412-8413 8418 8421 8425 8427-8429 8449 8452 8454 8457-8461 8468-8470 8473 8478 8480-8481 8490 8494-8495 8497 8499-8500 8639 8655 8663 8665 8668 8676-8677 8681 8689 8696 8704 8712-8713 8715 8720 8722 8727-8729 8732-8733 8736-8737 8740-8742 8745-8749 8768 8770 8831 8834 8895 8919 8921-8924 8931 8938 8940 8942 8945-8946 8949 8953 8982 8985-8986 8989-8991 8998-8999 9002-9004 9006 9009 9018-9019 9026 9028 9089 9096 9098-9100 9120 9231 9241 9256-9258 9260-9262 9265 9267 9276 9346 9348-9349 9351-9353 9355-9356 10268 10270-10271 10279-10281 10286 10288-10290 10307 10311-10312 10314 10320 10376-10377 12592 13332 13383 13391 13412-13413 13423 13432 18385 18393-18394 18404-18405 18412 18416 19411 19670 19673-19675 19677-19678 19686 19698-19699 19736 19748-19749 19751 19754 19778 19840-19841 19931 19940 19942-19943 19952 19986-19987 19991 19993 19996 19998 20003-20004 20006 20010 20017 20034 20096 20159 20196 20200-20201 20205 20247-20248 20253 20275 20277 20281 20285 20288 20292 20328 20416 20418-20419 20424 21970 21993 21996 21999 22003 22008-22009 22012 22015 22351 22367 22372 22384 22389 22485 22493 26047 26062 26069 26072 26077 26087 26093 26098 26102 26104 26110 26319 26323-26324 26326-26329 26332 26338-26339 26345 26347 26349 26351 26354 26359-26362 26364-26365 26385 26390-26391 26394 26403 26409 26411 26417-26418 26426 26429 26432 26435 26437 26439-26440 26443 26449-26454 26456-26458 26460 26462-26463 26468 26475 26487 26494-26496 26499-26500 26517 26520 26528 26532 26536-26538 26542 26544 26546-26548 26550-26551 26554 26556 26561-26562 26566 26569-26570 26580 26588-26590 26593 26595-26596 26600 26602 26608 26610-26611 27087 27091 27093 27098-27100 27107 27109-27110 27115-27116 27120 27124-27126 27341 27349 27352 27364-27365 27378 27382-27384 27386 27391 27410 27419 27423 27429-27430 27433 27435 27438-27439 27441 27446 27463 27468 27472-27474 27479-27480 27482 27485 27487 27489 27491 27500 27513-27516 27518 27522 27524-27525 27529-27530 27534 27538-27540 27544 27548 27550 27554 27559 27561 27563 27567 27574 27576-27577 27579-27580 27589 27591 27597-27598 27602-27604 27608 27610 27617 27622-27623 27633 27668 27670-27671 27676 27683 27687 27693 27695 27697 27703 27705-27706 27711 27714-27716 27718-27720 27722-27725 27727 27729 27731 27736 27738-27740 27743 27745 27748-27749 27751 27753-27755 27757-27758 27760 27762-27764 27767-27768 27770-27771 27773-27776 27781-27783 27785-27786 27790 27792 27794 27797 27800 27803 27811 27826 27831 27833-27834 27836 27845-27846 27853 27860 27862 27865-27866 27868 27872 27874-27877 27880 27883-27885 27888 27906 27909 27911 27913 27920-27922 27926-27927 27929 27938 27941 27943 27945 27947-27948 27969 28031-28032 28035 28117 28122 28126-28127 28131-28132 28134 28138-28139 28144 28146 28149 28152-28154 28156 28160 28163-28166 28170-28173 28178 28180 28193 28200 28202 28207 28210 28226 28287 28367 28371 28373-28374 28377 28380-28381 28386 28388 28390 28395 28398 28400-28402 28405-28406 28408 28410-28412 28441-28442 28444 28446 28451 28453-28455 28458-28459 28461-28464 28466-28467 28469 28473-28475 28481-28482 28484 28486-28488 28490 28492 28496 28546 28549 28554 28576 31423 31439 31447-31448 31453 31455 31458 31461 31465 31469 31478-31479 31482-31486 31528 31535 31539 31617 31620 31624 31631 31639 31643 31645 31647 31651 31658 31664 31671 31677 31679 31683 31688 31690 31694 31717-31718 317264.0234554602041486e-19 4.920466254354166e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/483/1754?format=asciiOpticaldefaultJ/MNRAS/483/1754/table1Catalogue of our LSBG from the {alpha}.40-SDSS DR7SimbadNameSimbad column added by the CDSmeta.idcharnullablehgDisc scale length derived from fitting the sky-subtracted image of the galaxy with a single exponential profile using GALFITkpcphys.angSize;srcfloatReffgg-band effective radius given by SExtractorkpcphys.size.radiusfloatSB0gAUTOg-band central surface brightness calculated from the combination of gmag, b/a and hgmag.arcsec**-2phot.mag.sbfloatSB0BAUTOB-band central surface brightness based on the AUTO magnitudesmag.arcsec**-2phot.mag.sb;em.opt.BfloatSB0BISOB-band central surface brightness based on the ISO magnitudesphot.mag.sb;em.opt.BfloatSB0BISOCORB-band central surface brightness based on the ISOCOR magnitudesphot.mag.sb;em.opt.BfloatSB0BPETROB-band central surface brightness based on the PETRO magnitudesphot.mag.sb;em.opt.BfloatSB0BAVEB-band central surface brightness based on the average of the four magnitudes (AVE)phot.mag.sb;em.opt.BfloatMTypeMorphological type by decision trees with random forest of machine learning (3)src.morph.typecharLTypeLuminosity type in terms of B-band absolute magnitude (4)meta.codecharT2indicates galaxy with data in table2meta.ref.urlchargmagg-band magnitude measured on the sky-subtracted images of galaxies within the automatic aperture by SExtractor (1)magphot.mag;em.opt.Bfloate_gmagError on gmagmagstat.error;phot.magfloatrmagr-band magnitude measured on the sky-subtracted images of galaxies within the automatic aperture by SExtractor (1)magphot.mag;em.opt.Rfloate_rmagError on rmagmagstat.error;phot.magfloatBmagB-band auto magnitude converted from the combination of auto magnitudes in both g and r bands (2)magphot.mag;em.opt.Bfloate_BmagError on Bmagmagstat.error;phot.magfloatb/ag-band major-to-minor axis ratio (b/a) derived from fitting the sky-subtracted image of the galaxy with a single exponential profile using GALFITphys.angSize;arith.ratiofloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintW50Velocity width of the HI line profile measured at the 50 per cent level of the peak (stemed from the {alpha}.40 catalogue)km/sspect.line.widthinte_W50Error on W50km/sstat.errorint_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainNameGalaxy name as it appears in the ALFALFA ({alpha}.40) catalogue (AGC NNNNNNA)meta.id;meta.maincharprimaryJ/MNRAS/483/1754/table2The subLSBGs for optical and NIR Tully-Fisher relation studiesiInclination angledegsrc.orbital.inclination;pos.posAngfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameGalaxy name as it appears in the ALFALFA ({alpha}.40) catalogue (AGC NNNNNNA)meta.id;meta.maincharW50corCorrected velocity width of the HI line profile measured at the 50 per cent level of the peakkm/sspect.line.widthfloate_W50corError on W50corkm/sstat.errorfloatDistDistance from the released entire ALFALFA catalogueMpcpos.distancefloate_DistError on DistMpcstat.errorfloatBmagB-band absolute magnitude that has been corrected for Galactic and internal extinctionmagphot.mag;em.opt.Bfloate_BmagError on Bmagmagstat.error;phot.magfloatJmag? J-band absolute magnitude corrected only for Galactic extinction (1)magphot.mag;em.IR.Jfloatnullablee_Jmag? Error on Jmag (1)magstat.error;phot.magfloatnullableHmag? H-band absolute magnitude corrected only for Galactic extinction (1)magphot.mag;em.IR.Hfloatnullablee_Hmag? Error on Hmag (1)magstat.error;phot.magfloatnullableKmag? K-band absolute magnitude corrected only for Galactic extinction (1)magphot.mag;em.IR.Kfloatnullablee_Kmag? Error on Kmag (1)magstat.error;phot.magfloatnullable