J/ApJS/234/5ivo://CDS.VizieR/J/ApJS/234/5doi:10.26093/cds/vizier.22340005CDSYang M.Wu H.Yang F.Lam M.I.Cao T.-W.Wu C.-J.Zhao P.-S.,Zhang T.-M.Zhou Z.-M.Wu X.-B.Zhang Y.-X.Shao Z.-Y.Jing Y.-P.,Shen S.-Y.Zhu Y.-N.Du W.Lei F.-J.He M.Jin J.-J.Shi J.-R.,Zhang W.Wang J.-L.Wu Y.-Z.Zhang H.-T.Luo A.-L.Yuan H.-L.,Bai Z.-R.Kong X.Gu Q.-S.Zhou X.Ma J.Hu Z.Nie J.-D.Wang J.-L.,Zhang Y.Hou Y.-H.Zhao Y.-H.2021-01-25T10:47:30Z2018-04-17T11:46:42ZCDS support team

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

cds-question@unistra.frgalaxiescatalogsredshiftedspectroscopysurveysvisible-astronomysloan-photometryultraviolet-photometryinfrared-photometryWe present a spectroscopic redshift catalog from the LAMOST Complete Spectroscopic Survey of Pointing Area (LaCoSSPAr) in the Southern Galactic Cap (SGC), which is designed to observe all sources (Galactic and extragalactic) by using repeating observations with a limiting magnitude of r=18.1mag in two 20deg^2^ fields. The project is mainly focusing on the completeness of LAMOST ExtraGAlactic Surveys (LEGAS) in the SGC, the deficiencies of source selection methods, and the basic performance parameters of the LAMOST telescope. In both fields, more than 95% of galaxies have been observed. A post-processing has been applied to the LAMOST 1D spectrum to remove the majority of remaining sky background residuals. More than 10000 spectra have been visually inspected to measure the redshift by using combinations of different emission/absorption features with an uncertainty of {sigma}_z_/(1+z)<0.001. In total, 1528 redshifts (623 absorption and 905 emission line galaxies) in Field A and 1570 redshifts (569 absorption and 1001 emission line galaxies) in Field B have been measured. The results show that it is possible to derive redshift from low S/N galaxies with our post-processing and visual inspection. Our analysis also indicates that up to one-fourth of the input targets for a typical extragalactic spectroscopic survey might be unreliable. The multi-wavelength data analysis shows that the majority of mid-infrared-detected absorption (91.3%) and emission line galaxies (93.3%) can be well separated by an empirical criterion of W2-W3=2.4. Meanwhile, a fainter sequence paralleled to the main population of galaxies has been witnessed both in Mr/W2-W3 and M*/W2-W3 diagrams, which could be the population of luminous dwarf galaxies but contaminated by the edge-on/highly inclined galaxies (~30%).2018ApJS..234....5Yhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/234/5CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVII/110 : Rich Clusters of Galaxies (Abell+ 1989)II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)V/139 : The SDSS Photometric Catalog, Release 9 (Adelman- McCarthy+, 2012)II/328 : AllWISE Data Release (Cutri+ 2013)V/147 : The SDSS Photometric Catalog, Release 12 (Alam+, 2015)V/146 : LAMOST DR1 catalogs (Luo+, 2015)V/149 : LAMOST DR2 catalogs (Luo+, 2016)J/ApJ/384/404 : Redshifts of nearby rich clusters of gal. (Postman+ 1992)J/PASP/111/438 : Updated Zwicky catalog (UZC) (Falco+, 1999)J/ApJS/167/1 : Galaxy groups and clusters from SDSS (Berlind+, 2006)J/MNRAS/406/1583 : Quasar from SDSS and UKIDSS (Wu+, 2010)J/AJ/144/49 : QSOs from SDSS-DR7, WISE and UKIDSS surveys (Wu+, 2012)J/other/RAA/15.1424 : LAMOST luminous infrared galaxies (Lam+, 2015)J/other/RAA/15.1414 : E+A galaxy candidates in LAMOST DR2 (Yang+, 2015)J/other/RAA/16.C7 : LAMOST-SDSS galaxy pairs (Shen+, 2016)J/AJ/151/24 : LAMOST quasar survey: QSOs from the DR1 (Ai+, 2016)J/other/RAA/17.41 : LAMOST metal-poor galaxies sample (Gao+, 2017)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/234/5https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/234/5http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/234/5https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/234/5https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/234/5http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/234/5GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/234/5/zspcat (The spectroscopic redshift catalog of LAMOST Complete Spectroscopic Survey of Pointing Area (LaCoSSPAr) (tables 2 and 3))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/234/5/zspcat?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/234/5/zspcat?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/234/5/zspcat?GETtext/xml+votable180.050000true36.856688892.105210.0055555555555555565/4411 4412 4414 4415 4446 4447 4468 4469 4500 4501 6/40 42 128 130 17637 17638 17639 17652 17654 17655 17767 17773 17775 17778 17779 17782 17783 17832 17834 17861 17863 17880 17881 17884 17885 179898.157980699529898e-21 1.4134638842407062e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/234/5?format=asciiUVOpticalInfrareddefaultJ/ApJS/234/5/zspcatThe spectroscopic redshift catalog of LAMOST Complete Spectroscopic Survey of Pointing Area (LaCoSSPAr) (tables 2 and 3)SimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFieldobs.fieldcharSeqRunning sequence numbermeta.id;meta.mainintRAJ2000Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainType[ae] Galaxy type (1)meta.codecharzspec[0.006/3.2] Spectroscopic redshiftsrc.redshiftfloatFUVmag[16.5/24.4]? GALEX FUV magnitude (2)magphot.mag;em.UVdoublenullablee_FUVmag[0.006/0.8]? GALEX FUV magnitude error (2)magstat.error;phot.magdoublenullableNUVmag[16/24.7]? GALEX NUV magnitude (2)magphot.mag;em.UVdoublenullablee_NUVmag[0.003/1.2]? GALEX NUV magnitude error (2)magstat.error;phot.magdoublenullableumag[14.6/34]? SDSS u-band Petrosian magnitude (2)magphot.mag;em.opt.Udoublenullablee_umag[0.005/66]? umag error (2)magstat.error;phot.magdoublenullablegmag[14/34]? SDSS g-band Petrosian magnitude (2)magphot.mag;em.opt.Bdoublenullablee_gmag[0.002/144]? gmag error (2)magstat.error;phot.magdoublenullablermag[14/20.5]? SDSS r-band Petrosian magnitude (2)magphot.mag;em.opt.Rdoublenullablee_rmag[0.002/7.6]? rmag error (2)magstat.error;phot.magdoublenullableimag[13.6/35]? SDSS i-band Petrosian magnitude (2)magphot.mag;em.opt.Idoublenullablee_imag[0.002/1557]? imag error (2)magstat.error;phot.magdoublenullablezmag[13.3/31.1]? SDSS z-band Petrosian magnitude (2)magphot.mag;em.opt.Idoublenullablee_zmag[0.004/518]? zmag error (2)magstat.error;phot.magdoublenullableJmag[13.2/17.4]? 2MASS J-band magnitude (2)magphot.mag;em.IR.Jdoublenullablee_Jmag[0.02/0.3]? Jmag error (2)magstat.error;phot.magdoublenullableHmag[12.5/16.8]? 2MASS H-band magnitude (2)magphot.mag;em.IR.Hdoublenullablee_Hmag[0.02/0.3]? Hmag error (2)magstat.error;phot.magdoublenullableKsmag[12/16]? 2MASS Ks-band magnitude (2)magphot.mag;em.IR.Kdoublenullablee_Ksmag[0.03/0.3]? Ksmag error (2)magstat.error;phot.magdoublenullableW1mag[10.8/17.8]? ALLWISE W1 band magnitude (2)magphot.mag;em.IR.3-4umdoublenullablee_W1mag[0.02/0.2]? W1mag error (2)magstat.error;phot.magdoublenullableW1snr[5.8/50]? ALLWISE W1-band Signal-to-Noise Ratio (2)meta.notedoublenullableW2mag[9.9/17.1]? ALLWISE W2 band magnitude (2)magphot.mag;em.IR.4-8umdoublenullablee_W2mag[0.02/0.4]? W2mag error (2)magstat.error;phot.magdoublenullableW2snr[1/55]? ALLWISE W2-band Signal-to-Noise Ratio (2)meta.notedoublenullableW3mag[6.6/13]? ALLWISE W3 band magnitude (2)magphot.flux.density;em.IR.8-15umdoublenullablee_W3mag[0.01/0.6]? W3mag error (2)magstat.error;phot.magdoublenullableW3snr[-2.5/68.4]? ALLWISE W3-band Signal-to-Noise Ratio (2)meta.notedoublenullableW4mag[3.7/9.6]? ALLWISE W4 band magnitude (2)magphot.flux.density;em.IR.15-30umdoublenullablee_W4mag[0.02/0.6]? W4mag error (2)magstat.error;phot.magdoublenullableW4snr[-3/47]? ALLWISE W4-band Signal-to-Noise Ratio (2)meta.notedoublenullableFUVmag0[10.5/24.4]? GALEX FUV, rest frame magnitude (2)magphot.mag;em.UVdoublenullableNUVmag0[15.8/24]? GALEX NUV, rest frame magnitude (2)magphot.mag;em.UVdoublenullableumag0[14.7/35]? SDSS u-band, rest frame magnitude (2)magphot.mag;em.opt.Udoublenullablegmag0[14.3/34]? SDSS g-band, rest frame magnitude (2)magphot.mag;em.opt.Bdoublenullablermag0[13.8/20.3]? SDSS r-band, rest frame magnitude (2)magphot.mag;em.opt.Rdoublenullableimag0[13.5/35]? SDSS i-band, rest frame magnitude (2)magphot.mag;em.opt.Idoublenullablezmag0[13.2/31.1]? SDSS z-band, rest frame magnitude (2)magphot.mag;em.opt.IdoublenullableCommComments for peculiar targets (3)src.classcharWISEADisplay the AllWISE data (Cutri+ 2013, II/328) within 3.5"meta.ref.urlcharLAMOSTDisplay the LAMOST -DR1 (V/146) and -DR2 data (V/149) within 0.5"meta.ref.urlcharSloanDisplay the online SDSS data for the nearest objectmeta.ref.urlchar2MDisplay the 2MASS data (Cutri+ 2003, II/246) within 3"meta.ref.urlchar