J/ApJS/270/7ivo://CDS.VizieR/J/ApJS/270/7doi:10.26093/cds/vizier.22700007CDSWeaver J.R.Cutler S.E.Pan R.Whitaker K.E.Labbe I.Price S.H.,Bezanson R.Brammer G.Marchesini D.Leja J.Wang B.Furtak L.J.,Zitrin A.Atek H.Chemerynska I.Coe D.Dayal P.van Dokkum P.,Feldmann R.Forster Schreiber N.M.Franx M.Fujimoto S.Fudamoto Y.,Glazebrook K.de Graaff A.Greene J.E.Juneau S.Kassin S.Kriek M.,Khullar G.Maseda M.V.Mowla L.A.Muzzin A.Nanayakkara T.,Nelson E.J.Oesch P.A.Pacifici C.Papovich C.Setton D.J.,Shapley A.E.Shipley H.V.Smit R.Stefanon M.Taylor E.N.Weibel A.,Williams C.C.2026-05-13T20:05:54Z2024-05-13T11:41:52ZCDS support team

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

cds-question@unistra.frgalaxy-clustershst-photometryinfrared-photometryvisible-astronomyredshiftedastronomical-object-identificationgravitational-lensingIn 2022 November, the James Webb Space Telescope (JWST) returned deep near-infrared images of A2744-a powerful lensing cluster capable of magnifying distant, incipient galaxies beyond it. Together with existing Hubble Space Telescope (HST) imaging, this publicly available data set opens a fundamentally new discovery space to understand the remaining mysteries of the formation and evolution of galaxies across cosmic time. In this work, we detect and measure some 60000 objects across the 49arcmin^2^ JWST footprint down to a 5{sigma} limiting magnitude of ~30mag in 0.32" apertures. Photometry is performed using circular apertures on images matched to the point-spread function (PSF) of the reddest NIRCam broad band, F444W, and cleaned of bright cluster galaxies and the related intracluster light. To give an impression of the photometric performance, we measure photometric redshifts and achieve a {sigma}NMAD~0.03 based on known, but relatively small, spectroscopic samples. With this paper, we publicly release our HST and JWST PSF-matched photometric catalog with optimally assigned aperture sizes for easy use, along with single aperture catalogs, photometric redshifts, rest-frame colors, and individual magnification estimates. These catalogs will set the stage for efficient and deep spectroscopic follow up of some of the first JWST-selected samples in summer of 2023.2024ApJS..270....7Whttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/270/7CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/hst : HST Archived Exposures Catalog (STScI, 2007)II/261 : GOODS initial results (Giavalisco+, 2004)III/334 : VISTA Deep Extragalactic Observations (VIDEO) (Jarvis+, 2013)I/337 : Gaia DR1 (Gaia Collaboration, 2016)II/357 : The Dark Energy Survey (DES): Data Release 1 (Abbott+, 2018)J/AJ/112/1335 : Hubble Deep Field observations (Williams+ 1996)J/AJ/125/1107 : Ultra-deep near-IR observation in HDF-S (Labbe+, 2003)J/AJ/132/1729 : HUDF BVI-dropout sources (Beckwith+, 2006)J/ApJS/164/334 : ACS Virgo Cluster Survey. VI (Ferrarese+, 2006)J/ApJ/663/320 : IR-through-UV extinction curve (Fitzpatrick+, 2007)J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014)J/ApJ/810/71 : UV mag of galaxies at 3~<z~<8.5 (Finkelstein+, 2015)J/MNRAS/452/1437 : Abell 2744 strong-lensing analysis (Jauzac+, 2015)J/ApJ/812/114 : Grism Lens-Amplified Survey from Space. I. (Treu+, 2015)J/ApJ/835/113 : Gal. >~6 from the Hubble Frontier Fields (Livermore+, 2017)J/ApJS/235/14 : HFF-DeepSpace phot. cat. of 12 HFF fields (Shipley+, 2018)J/ApJ/884/85 : RELICS: Reionization Lensing Cluster Survey (Coe+, 2019)J/ApJS/244/16 : HLF photometric catalog in GOODS-S v2.0 (Whitaker+, 2019)J/ApJ/889/189 : Brightest high-z galaxies in RELICS clusters (Salmon+, 2020)J/ApJS/247/12 : Strong lens models for 37 clusters from SGAS (Sharon+, 2020)J/A+A/646/A83 : 12 massive lensing clusters MUSE obs. (Richard+, 2021)J/ApJ/910/135 : RELICS 6<~z<=8 gal. with Spitzer & HST obs. (Strait+, 2021)J/ApJ/928/87 : Strongest cluster lenses (Fox+, 2022)J/ApJS/258/11 : The COSMOS2020 catalog (Weaver+, 2022)J/ApJS/270/12 : UNCOVER SPS cat. for robust sources up to z~15 (Wang+, 2024)http://jwst-uncover.github.io/ : JWST UNCOVER program home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/270/7https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/270/7http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/270/7https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/270/7https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/270/7http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/270/7GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/270/7/catalog (The UNCOVER DR2 "SUPER" photometric catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/270/7/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/270/7/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/270/7/catalog?GETtext/xml+votable180.050000true3.61533009655-30.461230316550.0055555555555555566/164864.0428963483234324e-20 4.75565502943315e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/270/7?format=asciiOpticalInfrareddefaultJ/ApJS/270/7/catalogThe UNCOVER DR2 "SUPER" photometric catalogSeq[1/61648] Object identification number (id)meta.id;meta.mainintUsePhot[0/1]? 1 if photometry is reliable (f444w SNR>3, not a star, not likely a bad pixel) (use_phot)meta.codeintnullablelowsnr[0/1]? 1 if S/N < 3 in the f277W+f356w+f444w stack (flag_lowsnr)meta.codeintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintXposCentroid position in X image frame (x)pixpos.cartesian.x;instr.det;obs.fielddoubleYposCentroid position in Y image frame (y)pixpos.cartesian.y;obs.fielddoubleRAJ2000[3.4/3.7] Centroid position in right ascension (J2000) (ra)degpos.eq.ra;meta.mainindexedDEJ2000[-30.5/-30.2] Centroid position in declination (J2000) (dec)degpos.eq.dec;meta.mainindexedE(B-V)[0.01/0.012] MW attenuation correction in E(B-V) computed from Schlafly & Finkbeiner (2011ApJ...737..103S) (ebv_mw)phot.color.excessdoubleFaper[-2.7/13198]? Flux computed in circular aperture of size corresponding to filename, in 10*nJy (Fnu) corresponding to ABMag zpt=28.9 (faper_f277w+f356w+f444w)10nJyphot.flux.density;em.IRdoublenullablee_Faper[0.03/4.1]? Flux error computed from empty apertures (same size as above), scaled by local weight / median weight (eaper_f277w+f356w+f444w)10nJystat.errorfloatnullableFauto[-2.7/34184]? Flux computed in Kron ellipse on the F444W-matched LW stack (Fv, zero-point=28.9) (fauto_f277w+f356w+f444w)10nJyphot.flux.density;em.IRdoublenullableWeight[0.008/1.2] Weight at the position of the source relative to the maximum weight (i.e. large values-->deep regions) (w_f277w+f356w+f444w)stat.weight;phys.atmol.weightfloatf435w[-16/35940]? Total HST/ACS F435W flux (f_f435w) (1)10nJyphot.mag;em.opt.Bdoublenullablee_f435w[0.1/34]? f435w uncertainty (e_f435w)10nJystat.errorfloatnullablew_f435w[0.003/1.1]? F435W weight at the position of the source relative to the maximum weight (w_f435w)stat.weightfloatnullablef606w[-59/61399]? Total HST/ACS F606W flux (f_f606w) (1)10nJyphot.mag;em.opt.Rdoublenullablee_f606w[0.1/111]? f606w uncertainty (e_f606w)10nJystat.errorfloatnullablew_f606w[5e-6/1.1]? f606w weight (w_f606w)stat.weightdoublenullablef814w[-26/62611]? Total HST/ACS F814W flux (f_f814w) (1)10nJyphot.mag;em.opt.Idoublenullablee_f814w[0.1/1313]? f814w uncertainty (e_f814w)10nJystat.errorfloatnullablew_f814w[3e-8/1.1]? f814w weight (w_f814w)stat.weightdoublenullablef090w[-4/29795]? Total JWST/NIRCam F090W flux (f_f090w) (1)10nJyphot.flux.density;em.opt.Idoublenullablee_f090w[0.1/12]? f090w uncertainty (e_f090w)10nJystat.errorfloatnullablew_f090w[0.04/1.1]? f090w weight (w_f090w)stat.weightfloatnullablef105w[-33/37122]? Total HST/WFC3 F105W flux (f_f105w) (1)10nJyphot.mag;em.IR.Jdoublenullablee_f105w[0.1/120]? f105w uncertainty (e_f105w)10nJystat.errorfloatnullablew_f105w[9e-6/1.1]? f105w weight (w_f105w)stat.weightdoublenullablef115w[-62/41559]? Total JWST/NIRCam F115W flux (f_f115w) (1)10nJyphot.flux.density;em.IR.Jdoublenullablee_f115w[0.1/47]? f115w uncertainty (e_f115w)10nJystat.errorfloatnullablew_f115w[0.008/1.2]? f115w weight (w_f115w)stat.weightfloatnullablef125w[-88/45394]? Total HST/WFC3 F125W flux (f_f125w) (1)10nJyphot.flux.density;em.IR.Jdoublenullablee_f125w[0.2/380]? f125w uncertainty (e_f125w)10nJystat.errorfloatnullablew_f125w[2e-6/1.1]? f125w weight (w_f125w)stat.weightdoublenullablef140w[-40/23772]? Total HST/WFC3 F140W flux (f_f140w) (1)10nJyphot.flux.density;em.IR.Hdoublenullablee_f140w[0.2/30]? f140w uncertainty (e_f140w)10nJystat.errorfloatnullablew_f140w[0.001/1]? f140w weight (w_f140w)stat.weightfloatnullablef150w[-28/55104]? Total JWST/NIRCam F150W flux (f_f150w) (1)10nJyphot.flux.density;em.IR.Hdoublenullablee_f150w[0.1/41]? f150w uncertainty (e_f150w)10nJystat.errorfloatnullablew_f150w[0.001/1.2]? f150w weight (w_f150w)stat.weightfloatnullablef160w[-349/56971]? Total HST/WFC3 F160W flux (f_f160w) (1)10nJyphot.flux.density;em.IR.Hdoublenullablee_f160w[0.2/258]? f160w uncertainty (e_f160w)10nJystat.errorfloatnullablew_f160w[1e-5/1.1]? f160w weight (w_f160w)stat.weightdoublenullablef200w[-6/65821]? Total JWST/NIRCam F200W flux (f_f200w) (1)10nJyphot.mag;em.IR.Kdoublenullablee_f200w[0.1/42]? f200w uncertainty (e_f200w)10nJystat.errorfloatnullablew_f200w[0.005/1.3]? f200w weight (w_f200w)stat.weightfloatnullablef277w[-8/40519]? Total JWST/NIRCam F277W flux (f_f277w) (1)10nJyphot.mag;em.IR.Kdoublenullablee_f277w[0.08/42]? f277w uncertainty (e_f277w)10nJystat.errorfloatnullablew_f277w[4.7e-6/1.2]? f277w weight (w_f277w)stat.weightdoublenullablef356w[-11/29066]? Total JWST/NIRCam F356W flux (f_f356w) (1)10nJyphot.flux.density;em.IR.3-4umdoublenullablee_f356w[0.08/31]? f356w uncertainty (e_f356w)10nJystat.errorfloatnullablew_f356w[0.0002/1.2]? f356w weight (w_f356w)stat.weightdoublenullablef410m[-10/31456]? Total JWST/NIRCam F410W flux (f_f410m) (1)10nJyphot.mag;em.IR.4-8umdoublenullablee_f410m[0.1/108]? f410m uncertainty (e_f410m)10nJystat.errorfloatnullablew_f410m[8.4e-5/1.2]? f410m weight (w_f410m)stat.weightdoublenullablef444w[-10/29395]? Total JWST/NIRCam F444W flux (f_f444w) (1)10nJyphot.mag;em.IR.4-8umdoublenullablee_f444w[0.07/48]? f444w uncertainty (e_f444w)10nJystat.errorfloatnullablew_f444w[0.004/1.1]? f444w weight (w_f444w)stat.weightfloatnullableCorr[1/119] Aperture to total correction based on circularized kron radius (tot_cor)phot.flux;arith.ratiofloatkronRad[1/12]? Kron radius factor (Source Extractor-like, unit-less) (kron_radius)phys.size.radiusfloatnullablekronRadc[0.1/7]? Circularized Kron radius (kron_radius_circ)arcsecphys.size.radiusfloatnullableUseCirc[0/1]? 1 for objects without Kron correction (faint and/or blended) (use_circle)meta.codeintnullablef_kron[0/1]? 1 when kron radius is not robust, in which case total photometry assumes point-like light distribution (flag_kron)meta.codeintnullableArea[0.001/176] Isophotal area based on the source segment (iso_area)arcsec**2phys.areadoubleUseAper[0.3/1.4] Indicates arcsec diameter adopted for color aperture (use_aper)arcsecphys.angSizefloataimg[0.5/183] Semi-major axis (a_image)pixphys.size.smajAxisfloatbimg[0.2/59] Semi-minor axis (b_image)pixphys.size.sminAxisfloattheta2000[-1.57/1.57] Position angle clockwise from the first image axis (along y) (theta_J2000)degpos.posAngfloatR50[0/34] Radius containing 50% of the flux (flux_radius)arcsecphys.angSize;srcfloatnophot[0]? 1 if the object has no viable photometry in any band at this aperture size (flag_nophot)meta.codeintnullablestar[0/1]? Stellarity flag (1=star; 113 occurrences; see Section 4.5) (flag_star)meta.codeintnullableartifact[0/1]? 1 if bad pixel, bCG-subtraction residual, or image artifact; see Section 4.6 (flag_artifact)meta.codeintnullablenearbcg[0/1]? 1 if source is within 3" of a subtracted bCG (likely a residual artifact; see Section 4.6) (flag_nearbcg)meta.codeintnullablezsp[2e-6/6.4]? Spectroscopic redshift (matched within 0.3" radius); see Section 2.4 (z_spec)src.redshiftdoublenullableIDDR1[1/50365]? ID of the source in the DR1 catalog release (all within <0.08" radius) (id_DR1)meta.id.crossintnullablesepDR1[7.8e-5/0.08]? Radius to DR1 catalog release match (match_radius_DR1)arcsecpos.angDistancedoublenullableMSA[2008/60157]? ID of the source in the team internal MSA catalog (Price+ 2023arXiv231002500P ; all within <0.24" radius) (id_msa)meta.id.crossintnullablesepMSA[4.6e-5/0.3]? Radius to team internal msa catalog match (match_radius_msa)arcsecpos.angDistancedoublenullableALMA[1/69]? ID of ALMA source from Fujimoto+ 2023, in prep. (id_alma)meta.id.crossintnullableFalma[15000/304100]? ALMA flux (NaN for non-detections), in 10*nJy (Fnu) corresponding to ABMag zpt=28.9 (f_alma)10nJyphot.flux.density;em.radiointnullablee_Falma[3270/24200]? Falma uncertainty (e_alma)10nJystat.errorfloatnullablesepALMA[0.01/0.7]? Radius to this catalog (nearest within 1" radius) (match_radius_alma)arcsecpos.angDistancefloatnullableNfilt[2/14]? Number of filters used in the fit (nusefilt)meta.numberintnullablezph[0.01/20]? Best-fit photometric redshift (maximum likelihood)src.redshiftdoublenullableChi2zph[-1/87991]? Total chi-squared at zph (z_phot_chi2)stat.fit.chi2doublenullablez025[0.01/19.4]? 0.25% of P(z) (redshift posterior) (z025)meta.notedoublenullablez160[0.01/19.7]? 16% of P(z) (redshift posterior) (z160)meta.notedoublenullablez500[0.01/19.8]? 50% of P(z) (redshift posterior) (z500)meta.notedoublenullablez840[0.01/19.9]? 84% of P(z) (redshift posterior) (z840)meta.notedoublenullablez975[0.02/19.9]? 97.5% of P(z) (redshift posterior) (z975)meta.notedoublenullablerestU[-7360/30483]? Rest-frame U-band flux (restU)10nJyphot.flux.density;em.opt.Udoublenullablee_restU[0/88629]? restU uncertainty (restU_err)10nJystat.errordoublenullablerestB[-1480/49455]? Rest-frame B-band flux (restB)10nJyphot.flux.density;em.opt.Bdoublenullablee_restB[0/69338]? restB uncertainty (restB_err)10nJystat.errordoublenullablerestV[-551/50407]? Rest-frame V-band flux (restV)10nJyphot.flux.density;em.opt.Vdoublenullablee_restV[0/202608]? restV uncertainty (restV_err)10nJystat.errordoublenullablerestJ[-939/57899]? Rest-frame J-band flux (restJ)10nJyphot.flux.density;em.IR.Jdoublenullablee_restJ[0/348812]? restJ uncertainty (restJ_err)10nJystat.errordoublenullablerestus[-7210/22681]? Rest-frame synth. u-band flux (restus)10nJyphot.flux.density;em.opt.Udoublenullablee_restus[0/105399]? restus uncertainty (restus_err)10nJystat.errordoublenullablerestgs[-2353/50513]? Rest-frame synth. g-band flux (restgs)10nJyphot.flux.density;em.opt.Bdoublenullablee_restgs[0/56108]? restgs uncertainty (restgs_err)10nJystat.errordoublenullablerestis[-57/33181]? Rest-frame synth. i-band flux (restis)10nJyphot.flux.density;em.opt.Idoublenullablee_restis[0/17021]? restis uncertainty (restis_err)10nJystat.errordoublenullableChi2min[1.5e-15/2677]? Chi2 of best-fit stellar template (star_min_chi2)stat.fit.chi2doublenullableeazy[0/1]? 1 if fit is reliable (flag_eazy)meta.codeintnullablezUse[2e-6/20]? Redshift used to compute magnification (z_phot unless is_zspec == 1) (z_use)meta.codedoublenullablef_zsp[0/1]? 1 if the redshift comes from zsp, 0 otherwise (is_zspec)meta.codeintnullablemu[0.02/12151]? Magnification (best-fit; = 1 for foreground objects) (mu)phot.mag;arith.ratiodoublenullablemu025[0.01/177]? Magnification uncertainty (mu025)stat.errordoublenullablemu160[0.01/207]? 16% magnification uncertainty (mu160)stat.errorfloatnullablemu840[0.03/1909]? 84% magnification uncertainty (mu840)stat.errordoublenullablemu975[0.03/24095]? Magnification uncertainty (mu975)stat.errordoublenullablemur[-599/7091]? Radial magnification (best-fit; = 1 for foreground objects) (mu_r)phot.mag;arith.ratiodoublenullablemur025[-155/26]? Radial magnification (mu_r025)phot.mag;arith.ratiodoublenullablemur160[-13/401]? 16% radial magnification (mu_r160)phot.mag;arith.ratiofloatnullablemur840[-1167/14]? 84% radial magnification (mu_r840)phot.mag;arith.ratiodoublenullablemur975[-7/1842]? Radial magnification (mu_r975)phot.mag;arith.ratiodoublenullablemut[-2597/2399]? Tangential magnification (best-fit; = 1 for foreground objects) (mu_t)phot.mag;arith.ratiodoublenullablemut025[-324/37]? Tangential magnification (mu_t025)phot.mag;arith.ratiodoublenullablemut160[-55/358]? 16% tangential magnification (mu_t160)phot.mag;arith.ratiofloatnullablemut840[-4217/27]? 84% tangential magnification (mu_t840)phot.mag;arith.ratiodoublenullablemut975[-38/6307]? Tangential magnification (mu_t975)phot.mag;arith.ratiodoublenullableshearone[-1.5/2.5]? Shear gamma_1 (best-fit; = 1 for foreground objects) (shearone)stat.fit.paramfloatnullableshearone025? Shear gamma_1 (shearone025)stat.fit.paramfloatnullableshearone160? 16% Shear gamma_1 (shearone160)stat.fit.paramfloatnullableshearone840? 84% Shear gamma_1 (shearone840)stat.fit.paramfloatnullableshearone975? Shear gamma_1 (shearone975)stat.fit.paramfloatnullablesheartwo[-5.5/1]? Shear gamma_2 (best-fit; = 1 for foreground objects) (sheartwo)stat.fit.paramfloatnullablesheartwo025? Shear gamma_2 (sheartwo025)stat.fit.paramfloatnullablesheartwo160? 16% Shear gamma_2 (sheartwo160)stat.fit.paramfloatnullablesheartwo840? 84% Shear gamma_2 (sheartwo840)stat.fit.paramfloatnullablesheartwo975? Shear gamma_2 (sheartwo975)stat.fit.paramfloatnullable