maclega scsivo://org.gavo.dc/maclega/q/coneThe GAVO DC teamDobrycheva, D.GAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837galaxiessurveys We present a sample of 317,018 galaxies at the redshifts 0.003 < z < 0.1 from SDSS DR9. We arrived at the current selection by limiting z as computed by SDSS, filtering out non-galaxy objects, and finally checking for faulty and duplicate objects. This yielded 724,000 objects. Further cleaning steps included removal of quasars and star-like objects, removal of duplicate images using the SDSS DR9 Image List Tool as well as proprietary code. By visual inspection, we selected the best image of each galaxy, which led to a sample of about 360,000 galaxies. Using the SDSS recommendation to avoid typical statistical errors near the spectroscopic flux limit we restricted the sample by stellar magnitude in r-band (modelMag_r < 17.7).2013OAP...26..187Dhttps://dc.g-vo.org/maclega/q/cone/infoCatalogResearchSDSS1/5,8,10,27 2/16-17,19,25,28,36,38,103,107 3/72-73,75,97,116,176-178,184,407,409-411,423,427,491,494 4/296-297,299,399,468-469,472,592,594,600,602,624,716,718,724,740,744-746,773-774,1109-1110,1114,1125-1126,1129-1130,1216,1367,1373,1375,1599,1621-1623,1625-1627,1685-1687,1690-1691,1701,1703,1707,1961-1963,1980,1982-1983,2027 5/0,10,136,138,267,295,419,425,1192-1193,1195,1540-1541,1543,1549,1585,1588-1589,1591,1684-1685,1728-1729,1732-1733,1880-1882,1896-1898,1900-1901,2372,2374,2380-2381,2504,2506,2515,2518,2521,2523-2524,2526,2528,2530,2536,2545,2547-2548,2550,2553,2555-2556,2868,2870,2876,2878,2968-2970,2988,3077,3089-3090,3100-3101,3136-3138,3153,4223,4287,4303,4307-4310,4312-4314,4323,4325-4326,4328-4330,4350-4351,4373-4375,4377-4380,4387-4390,4392-4394,4415-4416,4423,4433,4444,4450,4453-4455,4460-4461,4463,4466-4468,4472-4473,4475,4495,4498-4499,4508-4509,4513-4515,4524,4533,4544-4545,4547-4548,4550-4551,4556,4560,4562,4566,4569,4574-4575,4582,4596-4598,4601-4602,4629-4631,4633-4636,4645,4647,4651-4652,4654,4656,4672,4685,4687,4693-4698,4700-4701,4706,4709-4714,4716-4717,4719-4720,4736-4738,4750-4751,4757-4759,4761-4762,4764,4766,4773-4774,4776-4778,4782-4783,4788-4790,4792,4794-4798,4800,4802,4831,4835,4838,4842,4845-4847,4850-4854,4856,4858,4872,4917-4919,4921-4924,4933-4935,4937-4940,4944,4960,4995,4997-5002,5008,5461-5463,5491,5588-5589,5591,5597,5621,5623,5679,5761-5765,5768,5786,5795,5797-5798,5801-5802,6391,6461-6463,6477-6479,6481-6483,6497-6499,6541-6543,6735,6737-6739,6757-6759,6809-6811,6821-6823,6825-6827,7508-7510,7786,7823,7829-7831,7833-7834,7839,7841-7843,7882-7883,7886,7924,7926-7927,8099,8102-8103,8105-8107,8114-8115,8120-8122,8125,8127,8170-8171,9179,9181-9183,9191,9194-9196,9200-9202,11261-11263,12247,12253-12254,12271,12273-12276,12280,12282 6/4,8-9,12,14-15,26,32,34-36,38,521-524,526-527,538,548-550,556,640,723,993,1043-1045,1049,1051-1053,1055,1061-1063,1065,1067,1072,1075,1082,1086,1090,1153,1156-1157,1169,1171-1172,1174-1177,1205,1218,1224,1226-1227,1248,1690,1697,1712,1714,4776-4777,4779,6148-6150,6168-6169,6205,6337,6339,6348-6349,6360-6361,6363,6976-6977,6980-6981,6992-6993,6996-6997,7532-7533,7536-7538,7568-7570,7572,7576,7579,7582-7583,7596-7597,7608-7609,7612,7680-7681,7684-7685,7696-7697,7700-7701,8165,9494,9500,9503,9528,9530,9532,9616,9618,9624-9626,9648,9650,9656,9658,10000,10020-10022,10028,10030,10067,10070,10116,10118,10124,10152-10154,10177,10179,10185,10187,10209,10211,10217,10219,10232-10234,11476-11478,11484,11486,11508,11520,11522,11528,11530,11551-11552,11572-11573,11600,11602,11608,11610,11616-11617,11620-11621,11856,11858,11864,11884,11956,11960,11968-11970,12288-12290,12304-12305,12307,12313,12316-12317,12319,12341,12343,12352,12354-12355,12364,12408-12410,12480-12481,12484,12556-12558,12560-12561,12564,12568,12576,12609,12621,12632,15918,16887,16891,17207,17211,17223,17227,17244-17246,17260-17262,17264-17265,17287,17297-17299,17308-17310,17324-17326,17328-17330,17344,17346,17374-17375,17389,17391,17396-17397,17399,17469-17471,17485-17487,17490-17491,17505-17507,17524,17528,17547,17564-17566,17580-17582,17584-17586,17600-17602,17631,17647,17649-17650,17652-17654,17656-17658,17668-17670,17672-17673,17681-17683,17686,17689,17716,17718-17719,17723,17725-17727,17729,17731,17738,17741-17743,17780,17782-17786,17788,17790-17791,17794-17795,17798-17799,17805-17807,17809-17811,17848-17849,17851,17856-17858,17876-17878,17880-17881,17883-17884,17896-17898,17904-17905,17907-17908,17910-17911,17913-17916,17920-17922,17949,17951,17966-17967,17972,17974,17976,17978,17986,17989,17991,18040-18041,18043-18044,18046-18047,18049-18051,18100-18102,18104-18106,18109,18112-18114,18118-18120,18122-18125,18128,18130-18131,18136-18137,18139,18144-18145,18148-18150,18197-18199,18210,18212-18213,18215-18216,18221,18229-18231,18233-18238,18244-18245,18247,18253-18255,18258,18272-18274,18281-18285,18287-18288,18290-18292,18294-18295,18317,18319,18341,18352,18365-18367,18372-18373,18375,18381-18383,18396,18398,18401-18403,18412-18414,18416-18418,18495,18509-18511,18513-18515,18529-18531,18548,18552,18575,18579,18585-18587,18597-18599,18601-18603,18612-18614,18628,18632-18634,18653,18655,18677,18679,18683,18685-18687,18719,18744-18745,18747,18762,18765-18767,18769-18771,18796-18798,18808,18829-18831,18833-18835,18860-18862,18872-18873,18875,18886-18887,18889-18894,18906,18914,18916-18917,18920,18922-18923,18956,18958,18960,18976,18978,18989,18991,19021-19023,19025-19027,19041-19043,19052-19054,19061-19063,19068,19071,19080,19082-19083,19085-19087,19089-19091,19100-19102,19116-19118,19120-19122,19125,19127,19136-19138,19140-19141,19143-19144,19147,19149-19151,19164-19165,19167,19173-19175,19196-19197,19199,19204,19206,19213-19214,19216,19218-19222,19225-19228,19232-19233,19236,19238,19241-19242,19244,19264,19319,19322-19323,19334-19338,19347,19356,19358-19360,19362-19365,19367,19373-19377,19379,19397-19399,19420,19428-19430,19436,19438,19440,19472,19492-19494,19583,19645-19647,19661-19663,19665-19667,19681-19683,19700,19704,19725-19727,19729,19731,19747,19764,19768,19780,19784,19844,19848,19979,19985-19987,20012-20014,20016-20018,20036,20040,20096,21783,21839,21843,21959,21963,21988,21991,21997,21999,22351,22360-22361,22363,22384-22385,22396-22397,22399,22517,22519,22710-22711,22713-22715,22760,22762-22763,22875,23043,23064-23066,23076-23077,23080,23101-23104,23138,23150,23179,23185-23187,23196-23198,23201-23203,23212-23214,23216-23218,23224,23232-23234,25559,25575,25579,25581-25583,25821-25823,25837-25839,25841-25843,25885-25887,25901-25903,25905-25907,25922-25923,25985-25987,26135,26139,26141-26143,26155,26157-26159,26161-26163,26877-26879,26903,26909-26911,26933,26935,26945-26947,27015,27019,27021-27023,27025-27027,27197-27199,27213-27215,27233-27235,27278-27279,27281-27283,27297,27299,29973,30016,30029-30031,30044-30046,30064-30065,30067-30068,30973-30975,31138-31139,31148,31150,31286,31289-31291,31307,31309-31311,31313-31315,31329-31331,31340-31342,31344-31346,31351,31353-31355,31363,31488-31490,31548,31550-31551,31594,31598-31599,31611,31702,32104,32386-32387,32390-32392,32394-32395,32402-32403,32406-32407,32417-32419,32451,32471-32472,32474-32475,32477-32479,32492,32494-32495,32497-32499,32505-32507,32642,32650,32672,32674,32696,36607,36703,36715,36721-36723,36759,36761-36763,36771,36773-36775,36788-36790,36792-36794,36799,36812,36814,36816-36818,36832,36842,36846,36858-36859,36861-36863,40957,40959,45023,45039,45043,48983,49005,49007,49009-49011,49020-49022,49077-49079,49081,49091,49108,49112,49114,49119,49124-49125,49141,49147,49149-49151https://dc.g-vo.org/maclega/q/cone/coverageOpticalmaclega We present a sample of 317,018 galaxies at the redshifts 0.003 < z < 0.1 from SDSS DR9. We arrived at the current selection by limiting z as computed by SDSS, filtering out non-galaxy objects, and finally checking for faulty and duplicate objects. This yielded 724,000 objects. Further cleaning steps included removal of quasars and star-like objects, removal of duplicate images using the SDSS DR9 Image List Tool as well as proprietary code. By visual inspection, we selected the best image of each galaxy, which led to a sample of about 360,000 galaxies. Using the SDSS recommendation to avoid typical statistical errors near the spectroscopic flux limit we restricted the sample by stellar magnitude in r-band (modelMag_r < 17.7).maclega.main We present a sample of 317,018 galaxies at the redshifts 0.003 < z < 0.1 from SDSS DR9. We arrived at the current selection by limiting z as computed by SDSS, filtering out non-galaxy objects, and finally checking for faulty and duplicate objects. This yielded 724,000 objects. Further cleaning steps included removal of quasars and star-like objects, removal of duplicate images using the SDSS DR9 Image List Tool as well as proprietary code. By visual inspection, we selected the best image of each galaxy, which led to a sample of about 360,000 galaxies. Using the SDSS recommendation to avoid typical statistical errors near the spectroscopic flux limit we restricted the sample by stellar magnitude in r-band (modelMag_r < 17.7).idMain identifier for this object; this is the objID column from SDSS DR9's photoTag tablemeta.id;meta.maincharnullableraICRS right ascension for this object from SDSSpos.eq.ra;meta.maindoubleindexednullabledecICRS declination for this object from SDSSpos.eq.dec;meta.maindoubleindexednullabledlLuminosity distance. This was calculated it with the LUMDIST program.Mpcpos.distancefloatnullablezRedshift taken from SDSSsrc.redshiftfloatnullableabs_mrAbsolute stellar magnitude in the SDSS r band, calculated as Mr = modelMag_r - 5*log10(DL) - 25 - Extinction_r - kcorrect_r, where modelMag_r - the model magnitudes in a r-band; DL - luminosity distance; Extinction_r - Galactic extinction in r-band; kcorrect_r - k- correction in r-band.magphys.magabsfloatnullablemorphMorphological type, E, S, or Isrc.morph.typeESIcharnullablemodelmag_uModel magnitude in the u band from SDSS DR9magphot.mag;em.opt.Ufloatnullableext_uExtinction in the u band following 1998wfsc.conf..297S, taken from SDSS DR9.magphys.absorption;em.opt.Ufloatnullablekcorrect_uTBDTBDfloatnullablemodelmag_gModel magnitude in the g band from SDSS DR9magphot.mag;em.opt.Vfloatnullableext_gExtinction in the g band following 1998wfsc.conf..297S, taken from SDSS DR9.magphys.absorption;em.opt.Vfloatnullablekcorrect_gTBDTBDfloatnullablemodelmag_rModel magnitude in the r band from SDSS DR9magphot.mag;em.opt.Rfloatnullableext_rExtinction in the r band following 1998wfsc.conf..297S, taken from SDSS DR9.magphys.absorption;em.opt.Rfloatnullablekcorrect_rTBDTBDfloatnullablemodelmag_iModel magnitude in the i band from SDSS DR9magphot.mag;em.opt.Ifloatnullableext_iExtinction in the i band following 1998wfsc.conf..297S, taken from SDSS DR9.magphys.absorption;em.opt.Ifloatnullablekcorrect_iTBDTBDfloatnullablemodelmag_zModel magnitude in the z band from SDSS DR9magphot.mag;em.opt.Ifloatnullableext_zExtinction in the z band following 1998wfsc.conf..297S, taken from SDSS DR9.magphys.absorption;em.opt.Ifloatnullablekcorrect_zTBDTBDfloatnullablepetror50_rRadius containing 50% of the Petrosian flux in the r-band.arcsecphys.angsize;srcfloatnullablepetror90_rRadius containing 90% of the Petrosian flux in the r-band.arcsecphys.angsize;srcfloatnullable