J/A+A/708/A104ivo://CDS.VizieR/J/A+A/708/A104CDSEuclid Coll.Zalesky L.Weaver J.R.McPartland C.J.R.Murphree G.,Valdes I.Jespersen C.K.Taamoli S.Chartab N.Allen N.Barrow S.W.J.,Sanders D.B.Toft S.Mobasher B.Szapudi I.Altieri B.Amara A.,Andreon S.Auricchio N.Baccigalupi C.Baldi M.Bardelli S.,Battaglia P.Biviano A.Bonino D.Branchini E.Brescia M.,Brinchmann J.Caillat A.Camera S.Canas-Herrera G.Capobianco V.,Carbone C.Carretero J.Casas S.Castander F.J.Castellano M.,Castignani G.Cavuoti S.Chambers K.C.Cimatti A.Colodro-Conde C.,Congedo G.Conselice C.J.Conversi L.Copin Y.Courbin F.,Courtois H.M.Da Silva A.Degaudenzi H.De Lucia G.Di Giorgio A.M.,Dole H.Dubath F.Duncan C.A.J.Dupac X.Dusini S.Ealet A.,Escoffier S.Farina M.Farinelli R.Farrens S.Faustini F.,Ferriol S.Finelli F.Fosalba P.Fotopoulou S.Frailis M.,Franceschi E.Fumana M.George K.Gillis B.Giocoli C.,Gracia-Carpio J.Grazian A.Grupp F.Gwyn S.Haugan S.V.H.Holmes W.,Hook I.Hormuth F.Hornstrup A.Jahnke K.Jhabvala M.Joachimi B.,Keihanen E.Kermiche S.Kiessling A.Kubik B.Kuijken K.Kummel M.,Kunz M.Kurki-Suonio H.Le Brun A.M.C.Le Mignant D.Ligori S.,Lilje P.B.Lindholm V.Lloro I.Mainetti G.Maino D.Maiorano E.,Mansutti O.Marggraf O.Markovic K.Martinelli M.Martinet N.,Marulli F.Massey R.Maurogordato S.McCracken H.J.Medinaceli E.,Mei S.Mellier Y.Meneghetti M.Merlin E.Meylan G.Mora A.,Moresco M.Moscardini L.Nakajima R.Neissner C.Niemi S.-M.,Nightingale J.W.Padilla C.Paltani S.Pasian F.Pedersen K.,Pettorino V.Polenta G.Poncet M.Popa L.A.Pozzetti L.Raison F.,Rebolo R.Renzi A.Rhodes J.Riccio G.Romelli E.Roncarelli M.,Saglia R.Sakr Z.Sapone D.Sartoris B.Schewtschenko J.A.,Schirmer M.Schneider P.Schrabback T.Secroun A.Sefusatti E.,Seidel G.Serrano S.Simon P.Sirignano C.Sirri G.Stanco L.,Starck J.-L.Steinwagner J.Tallada-Crespi P.Tavagnacco D.,Taylor A.N.Teplitz H.I.Tereno I.Toledo-Moreo R.Torradeflot F.,Tsyganov A.Tutusaus I.Valenziano L.Valiviita J.Vassallo T.,Verdoes Kleijn G.Veropalumbo A.Wang Y.Weller J.Zacchei A.,Zamorani G.Zucca E.Bolzonella M.Bozzo E.Burigana C.Calabrese M.,Di Ferdinando D.Escartin Vigo J.A.Gabarra L.Matthew S.Mauri N.,Pezzotta A.Pontinen M.Porciani C.Scottez V.Tenti M.Viel M.,Wiesmann M.Akrami Y.Allevato V.Andika I.T.Anselmi S.,Archidiacono M.Atrio-Barandela F.Ballardini M.Bertacca D.,Bethermin M.Blanchard A.Blot L.Borgani S.Brown M.L.Bruton S.,Cabanac R.Calabro A.Camacho Quevedo B.Cappi A.Caro F.,Carvalho C.S.Castro T.Chary R.Cogato F.Contini T.Cooray A.R.,Cucciati O.Davini S.De Paolis F.Desprez G.Diaz-Sanchez A.,Di Domizio S.Diego J.M.Ferrari A.G.Finoguenov A.Ganga K.,Garcia-Bellido J.Gasparetto T.Gaztanaga E.Giacomini F.Gianotti F.,Gozaliasl G.Gregorio A.Guidi M.Gutierrez C.M.Hall A.,Hartley W.G.Hemmati S.Hildebrandt H.Hjorth J.Huertas-Company M.,Ilbert O.Kajava J.J.E.Kang Y.Kansal V.Karagiannis D.,Kirkpatrick C.C.Kruk S.Lattanzi M.Le Graet J.Legrand L.Lembo M.,Leroy G.Lesgourgues J.Liaudat T.I.Loureiro A.Macias-Perez J.,Maggio G.Magliocchetti M.Mancini C.Mannucci F.Maoli R.,Martin-Fleitas J.Martins C.J.A.P.Maurin L.Metcalf R.B.Miluzio M.,Monaco P.Moretti C.Morgante G.Murray C.Naidoo K.Natoli P.,Navarro-Alsina A.Nesseris S.Paterson K.Patrizii L.Pisani A.,Potter D.Risso I.Rocci P.-F.Sahlen M.Sarpa E.Schaye J.,Schneider A.Schultheis M.Sciotti D.Sellentin E.Sereno M.,Shankar F.Smith L.C.Stanford S.A.Tanidis K.Tao C.Testera G.,Teyssier R.Tosi S.Troja A.Tucci M.Valieri C.Venhola A.,Vergani D.Verza G.Vielzeuf P.Walton N.A.2026-05-04T07:43:19Z2026-03-30T11:26:35ZCDS support team

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

cds-question@unistra.frgalaxiescatalogssurveysredshiftedphotometryspectroscopyThe Cosmic Dawn Survey Pre-Launch (PL) catalogues cover an effective 10.13deg^2^ area with uniform deep Spitzer/IRAC data (m~25mag, 5{sigma}), the largest area covered to these depths at infrared wavelengths. These data are used to gain new insight into the growth of stellar mass across cosmic history by characterising the evolution of the galaxy stellar mass function through 0.2<z<=6.5. The total volume (0.62Gpc^3^) represents an order of magnitude increase compared to previous works that have explored z>3 and significantly reduces cosmic variance, thus yielding strong constraints on the abundance of galaxies above the characteristic stellar mass (M*) across this ten billion year time period. The evolution of the galaxy stellar mass function is generally consistent with results from the literature but now provide firm estimates of number density where only upper limits were previously available. Contrasting the galaxy stellar mass function with the dark matter halo mass function suggests that massive galaxies (M~>10^11^M_{Sun}_) at z>3.5 required integrated star-formation efficiencies of M/(M_h_*f_b_)~>0.25-0.5, in excess of the commonlyheld view of 'universal peak efficiency' from studies on the stellar-to-halo mass relation. Such increased efficiencies imply an evolving peak in the stellar-to-halo mass relation at z>3.5 which can be maintained if feedback mechanisms from active galactic nuclei and stellar processes are ineffective at early times. In addition, a significant fraction of the most massive quiescent galaxies are observed to be in place already by z~2.5-3. The apparent lack in change of their number density by z~0.2 is consistent with relatively little mass growth from mergers. Utilising the unique volume, evidence for an environmental dependence of the galaxy stellar mass function is found all the way through z~3.5 for the first time, though a more careful characterisation of the density field is ultimately required for confirmation.2026A&A...708A.104Ehttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/708/A104CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/830/51 : FourStar galaxy evolution survey (ZFOURGE) (Straatman+, 2016)J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)J/ApJ/735/86 : NEWFIRM MBS: photometric catalogs (Whitaker+, 2011)J/A+A/695/A229 : DAWN Survey PL (Euclid Coll.+, 2025)J/A+A/647/A150 : VANDELS ESO public spectroscopic survey. DR4 (Garilli+, 2021)J/A+A/556/A55 : Multi-color photometry of star-forming galaxies (Ilbert+,2013)J/ApJS/258/11 : The COSMOS2020 catalog (Weaver+, 2022)J/ApJS/237/39 : Spitzer survey of UltraVISTA deep Stripes (SMUVS)J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)J/ApJS/172/70 : zCOSMOS-bright catalog, DR3 (Lilly+, 2007)I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)II/388 : Euclid final merged catalog. Q1 data releaseII/373 : The fourth UltraVISTA data release (DR4) (Moneti+, 2019)II/261 : GOODS initial results (Giavalisco+, 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/708/A104https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/708/A104http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/708/A104https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/708/A104https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/708/A104http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/708/A104GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/708/A104/totsamp (selection of reliable objects in the DAWN PL Catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/708/A104/totsamp?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/708/A104/totsamp?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/708/A104/totsamp?GETtext/xml+votable180.050000true274.004822632316863.905151540102240.0055555555555555565/2559 2901 2903 3839 4010-4011 8983 6/10229-10231 15353-15355 35956-35957 35959 36106 36128https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/708/A104?format=asciidefaultJ/A+A/708/A104/totsampselection of reliable objects in the DAWN PL CataloguerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDRaw identifier source number (ID)meta.id;meta.mainintRAJ2000Right ascension (J2000) (ALPHA_J2000)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (DELTA_J2000)degpos.eq.dec;meta.mainindexedflagField flag for edfn or edffmeta.code.errorchartotCategory boolean for the total samplemeta.codecharsfCategory boolean for the star-forming samplemeta.codecharqCategory boolean for the quiescent samplemeta.codecharJ/A+A/708/A104/table1Redshift bin informations on volumes, stellar mass limits for N_gal_ with M*>MlimrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbinRedshift bin (redshift_bin)src.redshift.phot;arith.diffcharVTotal comoving volume (volume)1e+06Mpc**3meta.bib.volumefloatlog(Mlim)Stellar mass limit for the total sample (mlim)log(solMass)phys.massfloatNgalNumber of galaxies with stellar masses above the stellar mass limit (ngal)meta.numberintJ/A+A/708/A104/table2Schechter parameters ranges derived for the total mass complete samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbinRedshift bin (redshift_bin)src.redshift.phot;arith.diffcharaminMinimum allowed value of alpha (alpha_min)stat.param;meta.modelledfloatamaxMaximum allowed value of alpha (alpha_max)stat.param;meta.modelledfloatRefLiterature reference (literature) (1)meta.ref;pos.framecharJ/A+A/708/A104/table3Double (z<=2) and single (z>2) Schechter parameters for the total mass complete samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbinRedshift bin from MCMC fit (redshift_bin)src.redshift.phot;arith.diffcharlogM*Schechter function knee (log10_mstar)solMassphys.massfloata1? First slope (alpha1)stat.param;meta.modelledfloatnullablelogphi1? First normalization (log10_phi1)log(Mpc**-3)phys.mass;meta.modelled;arithfloatnullablea2? Second slope (alpha2)stat.param;meta.modelledfloatnullablelogphi2? Second normalization (log10_phi2)log(Mpc**-3)phys.mass;meta.modelled;arithfloatnullableJ/A+A/708/A104/table4Double (z<=2) and single (z>2) Schechter parameters for star-forming complete subsamplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbinRedshift bin from MCMC fit (redshift_bin)src.redshift.phot;arith.diffcharlogM*Schechter function knee (log10_mstar)solMassphys.massfloata1? First slope (alpha1)stat.param;meta.modelledfloatnullablelogphi1? First normalization (log10_phi1)log(Mpc**-3)phys.mass;meta.modelled;arithfloatnullablea2? Second slope (alpha2)stat.param;meta.modelledfloatnullablelogphi2? Second normalization (log10_phi2)log(Mpc**-3)phys.mass;meta.modelled;arithfloatnullableJ/A+A/708/A104/table5Double (z<=0.8) and single (z>0.8) Schechter parameters for quiescent mass complete subsamplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbinRedshift bin from MCMC fit (redshift_bin)src.redshift.phot;arith.diffcharlogM*Schechter function knee (log10_mstar)solMassphys.massfloata1? First slope (alpha1)stat.param;meta.modelledfloatnullablelogphi1? First normalization (log10_phi1)log(Mpc**-3)phys.mass;meta.modelled;arithfloatnullablea2? Second slope (alpha2)stat.param;meta.modelledfloatnullablelogphi2? Second normalization (log10_phi2)log(Mpc**-3)phys.mass;meta.modelled;arithfloatnullableJ/A+A/708/A104/qz0205Observed mass function for the quiescent sample in redshift range of 0.2 to 0.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/qz0508Observed mass function for the quiescent sample in redshift range of 0.5 to 0.8recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/qz0811Observed mass function for the quiescent sample in redshift range of 0.8 to 1.1recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/qz1115Observed mass function for the quiescent sample in redshift range of 1.1 to 1.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/qz1520Observed mass function for the quiescent sample in redshift range of 1.5 to 2.0recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/qz2025Observed mass function for the quiescent sample in redshift range of 2.0 to 2.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/qz2530Observed mass function for the quiescent sample in redshift range of 2.5 to 3.0zbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/sfz0205Observed mass function for the star-forming in redshift range of 0.2 to 0.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/sfz0508Observed mass function for the star-forming in redshift range of 0.5 to 0.8recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/sfz0811Observed mass function for the star-forming in redshift range of 0.8 to 1.1recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/sfz1115Observed mass function for the star-forming in redshift range of 1.1 to 1.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/sfz1520Observed mass function for the star-forming in redshift range of 1.5 to 2.0zbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/sfz2025Observed mass function for the star-forming in redshift range of 2.0 to 2.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/sfz2530Observed mass function for the star-forming in redshift range of 2.5 to 3.0recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/tz0205Observed mass function for the total sample in redshift range of 0.2 to 0.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/tz0508Observed mass function for the total sample in redshift range of 0.5 to 0.8recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/tz0811Observed mass function for the total sample in redshift range of 0.8 to 1.1recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/tz1115Observed mass function for the total sample in redshift range of 1.1 to 1.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/tz1520Observed mass function for the total sample in redshift range of 1.5 to 2.0recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/tz2025Observed mass function for the total sample in redshift range of 2.0 to 2.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/tz2530Observed mass function for the total sample in redshift range of 2.5 to 3.0recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/tz3035Observed mass function for the total sample in redshift range of 3.0 to 3.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/tz3545Observed mass function for the total sample in redshift range of 3.5 to 4.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/tz4555Observed mass function for the total sample in redshift range of 4.5 to 5.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullableJ/A+A/708/A104/tz5565Observed mass function for the total sample in redshift range of 5.5 to 6.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbcRedshift bin center (bin_center)src.redshift.photdoublezbwRedshift bin width (bin_width)src.redshift.phot;arith.diffdoublelogphi? Mass function for the total 'tot', star-forming 'sf', and quiescent 'q' (log_phi)phys.mass;meta.modelled;arithdoublenullablee_logphi? Lower uncertainty of logphi (log_phi_lo)stat.errordoublenullableE_logphi? Upper uncertainty of logphi (log_phi_hi)stat.error;stat.maxdoublenullable