J/ApJS/199/25ivo://CDS.VizieR/J/ApJS/199/25doi:10.26093/cds/vizier.21990025CDSPostman M.Coe D.Benitez N.Bradley L.Broadhurst T.Donahue M.,Ford H.Graur O.Graves G.Jouvel S.Koekemoer A.Lemze D.,Medezinski E.Molino A.Moustakas L.Ogaz S.Riess A.Rodney S.,Rosati P.Umetsu K.Zheng W.Zitrin A.Bartelmann M.Bouwens R.,Czakon N.Golwala S.Host O.Infante L.Jha S.Jimenez-Teja Y.,Kelson D.Lahav O.Lazkoz R.Maoz D.McCully C.Melchior P.,Meneghetti M.Merten J.Moustakas J.Nonino M.Patel B.Regos E.,Sayers J.Seitz S.Van der Wel A.2017-06-20T13:16:00Z2012-08-22T09:07:56ZCDS support team

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

cds-question@unistra.frgalaxy-clustersgalaxiesphotometryhst-photometryredshiftedsurveysThe Cluster Lensing And Supernova survey with Hubble (CLASH) is a 524-orbit Multi-Cycle Treasury Program to use the gravitational lensing properties of 25 galaxy clusters to accurately constrain their mass distributions. The survey, described in detail in this paper, will definitively establish the degree of concentration of dark matter in the cluster cores, a key prediction of structure formation models. The CLASH cluster sample is larger and less biased than current samples of space-based imaging studies of clusters to similar depth, as we have minimized lensing-based selection that favors systems with overly dense cores. Specifically, 20 CLASH clusters are solely X-ray selected. The X-ray-selected clusters are massive (kT>5keV) and, in most cases, dynamically relaxed. Five additional clusters are included for their lensing strength ({theta}_Ein_>35" at z_s_=2) to optimize the likelihood of finding highly magnified high-z (z>7) galaxies. A total of 16 broadband filters, spanning the near-UV to near-IR, are employed for each 20-orbit campaign on each cluster. These data are used to measure precise ({sigma}_z_~0.02(1+z)) photometric redshifts for newly discovered arcs. Observations of each cluster are spread over eight epochs to enable a search for Type Ia supernovae at z>1 to improve constraints on the time dependence of the dark energy equation of state and the evolution of supernovae. We present newly re-derived X-ray luminosities, temperatures, and Fe abundances for the CLASH clusters as well as a representative source list for MACS1149.6+2223 (z=0.544).2012ApJS..199...25Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/199/25CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/hst : HST Archived Exposures Catalog (STScI, 2007)J/ApJ/736/21 : Galaxy clusters optical catalog from AMF on SDSS DR6 (Szabo+J/ApJS/150/1 : VV29 and NGC 4676 HST photometry (Benitez+, 2004)http://archive.stsci.edu/prepds/clash/ : CLASH home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/199/25https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/199/25http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/199/25https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/199/25https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/199/25http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/199/25GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/199/25/table7 (Sample of CLASH source list for MACS1149.6+2223)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/199/25/table7?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/199/25/table7?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/199/25/table7?GETtext/xml+votable180.050000true177.381422322.38029040.0055555555555555566/284481.1796835550914393e-19 9.254243743779334e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/199/25?format=asciiOpticaldefaultJ/ApJS/199/25/table7Sample of CLASH source list for MACS1149.6+2223l_F160WLimit flag on F160Wmeta.code.errorcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[1/9664] Object ID Numbermeta.id;meta.mainintRAJ2000[177.35/177.444] Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000[22.35/22.443] Declination (J2000)degpos.eq.dec;meta.mainXpix[20.168/4779.85] The X pixel coordinatepixpos.cartesian.xdoubleYpix[208.663/4804.08] The Y pixel coordinatepixpos.cartesian.ydoubleFWHM[-0.012/18.929] Full width at half maximumarcsecspect.line.widthfloatArea[0/36560] Isophotal aperture areapixel**2phys.angSize;instr.fovintStel[0/1] SExtractor "stellarity"; 1=star; 0=galaxysrc.class.starGalaxyfloatEll[0/1] Ellipticity=1-b/asrc.ellipticityfloatf5s[0] Significance flag (0: probably real) (1)meta.codeintNf5s[1/17] Number of filters with a 5{sigma} detectionmeta.numberintNfcr5s[0/12] Number of CR(cosmic rays)-vulnerable filters with a 5{sigma} detectionmeta.numberintNfobs[2/17] Number of filters observed; not in chip gap, etc.meta.numberintl_F225WLimit flag on F225Wmeta.code.errorcharF225W? HST/WFC3 F225W isophotal AB mag. (2)magphot.mag;em.UV.200-300nmdoublenullablee_F225W? Uncertainty in F225W (2)magstat.errorfloatnullableF225Wf[-8.903/90.1419] F225W isophotal flux (3)ct/sphot.count;em.UVfloate_F225Wf? Uncertainty in F225Wf (3)ct/sstat.errordoublenullableF225Wsig[-19.82/60.48] F225W detection significancestat.likelihood;obsfloatl_F275WLimit flag on F275Wmeta.code.errorcharF275W? HST/WFC3 F275W isophotal AB mag. (2)magphot.mag;em.UV.200-300nmdoublenullablee_F275W? Uncertainty in F275W (2)magstat.errorfloatnullableF275Wf[-16.2184/49.8871] F275W isophotal flux (3)ct/sphot.count;em.UVdoublee_F275Wf? Uncertainty in F275Wf (3)ct/sstat.errordoublenullableF275Wsig[-11.55/121.45] F275W detection significancestat.likelihood;obsfloatl_F336WLimit flag on F336Wmeta.code.errorcharF336W? HST/WFC3 F336W isophotal AB mag. (2)magphot.mag;em.opt.Udoublenullablee_F336W? Uncertainty in F336W (2)magstat.errorfloatnullableF336Wf[-3818.88/1413.53] F336W isophotal flux (3)ct/sphot.count;em.UVdoublee_F336Wf? Uncertainty in F336Wf (3)ct/sstat.errordoublenullableF336Wsig[-7.24/1612.91] F336W detection significancestat.likelihood;obsfloatl_F390WLimit flag on F390Wmeta.code.errorcharF390W? HST/WFC3 F390W isophotal AB mag. (2)magphot.mag;em.opt.Udoublenullablee_F390W? Uncertainty in F390W (2)magstat.errorfloatnullableF390Wf[-44.57/57346.04] F390W isophotal flux (3)ct/sphot.countdoublee_F390Wf? Uncertainty in F390Wf (3)ct/sstat.errordoublenullableF390Wsig[-80.08/1438] F390W detection significancestat.likelihood;obsfloatl_F435WLimit flag on F435Wmeta.code.errorcharF435W? HST/ACS F435W isophotal AB mag. (2)magphot.mag;em.opt.Bdoublenullablee_F435W? Uncertainty in F435W (2)magstat.errorfloatnullableF435Wf[-0.2294/5117.84] F435W isophotal flux (3)ct/sphot.countdoublee_F435Wf? Uncertainty in F435Wf (3)ct/sstat.errordoublenullableF435Wsig[-3.19/1491.93] F435W detection significancestat.likelihood;obsfloatl_F475WLimit flag on F475Wmeta.code.errorcharF475W? HST/WFC3 F475W isophotal AB mag. (2)magphot.mag;em.opt.Bdoublenullablee_F475W? Uncertainty in F475W (2)magstat.errorfloatnullableF475Wf[-0.312/7724.97] F475W isophotal flux (3)ct/sphot.countdoublee_F475Wf? Uncertainty in F475Wf (3)ct/sstat.errordoublenullableF475Wsig[-2.74/3233.47] F555W detection significancestat.likelihood;obsfloatl_F555WLimit flag on F555Wmeta.code.errorcharF555W? HST/WFC3 F555W isophotal AB mag. (2)magphot.mag;em.opt.Vdoublenullablee_F555W? Uncertainty in F555W (2)magstat.errorfloatnullableF555Wf[-0.2152/7308.11] F555W isophotal flux (3)ct/sphot.countdoublee_F555Wf? Uncertainty in F555Wf (3)ct/sstat.errordoublenullableF555Wsig[-2.47/2032.41] F555W detection significancestat.likelihood;obsfloatl_F606WLimit flag on F606Wmeta.code.errorcharF606W? HST/WFC3 F606W isophotal AB mag. (2)magphot.mag;em.opt.Rdoublenullablee_F606W? Uncertainty in F606W (2)magstat.errorfloatnullableF606Wf[-1.6315/12022.1] F606W isophotal flux (3)ct/sphot.countdoublee_F606Wf? Uncertainty in F606Wf (3)ct/sstat.errordoublenullableF606Wsig[-2.24/1949.76] F625W detection significancestat.likelihood;obsfloatl_F625WLimit flag on F625Wmeta.code.errorcharF625W? HST/WFC3 F625W isophotal AB mag. (2)magphot.mag;em.opt.Rdoublenullablee_F625W? Uncertainty in F625W (2)magstat.errorfloatnullableF625Wf[-0.39/8634.72] F625W isophotal flux (3)ct/sphot.countdoublee_F625Wf? Uncertainty in F625Wf (3)ct/sstat.errordoublenullableF625Wsig[-2.85/1489.83] F625W detection significancestat.likelihood;obsfloatl_F775WLimit flag on F775Wmeta.code.errorcharF775W? HST/WFC3 F775W isophotal AB mag. (2)magphot.mag;em.opt.Idoublenullablee_F775W? Uncertainty in F775W (2)magstat.errorfloatnullableF775Wf[-0.2508/8157.78] F775W isophotal flux (3)ct/sphot.countdoublee_F775Wf? Uncertainty in F775Wf (3)ct/sstat.errordoublenullableF775Wsig[-2.19/2004.02] F775W detection significancestat.likelihood;obsfloatl_F814WLimit flag on F814Wmeta.code.errorcharF814W? HST/WFC3 F814W isophotal AB mag. (2)magphot.mag;em.opt.Idoublenullablee_F814W? Uncertainty in F814W (2)magstat.errorfloatnullableF814Wf[-0.309/11081.44] F814W isophotal flux (3)ct/sphot.countdoublee_F814Wf? Uncertainty in F814Wf (3)ct/sstat.errordoublenullableF814Wsig[-1.73/2611.36] F814W detection significancestat.likelihood;obsfloatl_F850LPLimit flag on F850LPmagmeta.code.errorcharF850LP? HST/WFC3 F850LP isophotal AB mag. (2)magphot.mag;em.opt.Idoublenullablee_F850LP? Uncertainty in F850LPmag (2)magstat.errorfloatnullableF850LPf[-0.1143/6326.15] F850LP isophotal flux (3)ct/sphot.countdoublee_F850LPf? Uncertainty in F850LPf (3)ct/sstat.errordoublenullableF850LPsig[-2.21/2624.73] F850LP detection significancestat.likelihood;obsfloatl_F105WLimit flag on F105Wmeta.code.errorcharF105W? HST/WFC3 F105W isophotal AB mag. (2)magphot.mag;em.IR.Hdoublenullablee_F105W? Uncertainty in F105W (2)magstat.errorfloatnullableF105Wf[-957.665/44447.6] F105W isophotal flux (3)ct/sphot.count;em.UVdoublee_F105Wf? Uncertainty in F105Wf (3)ct/sstat.errordoublenullableF105Wsig[-0.97/9561.83] F105W detection significancestat.likelihood;obsfloatl_F110WLimit flag on F110Wmeta.code.errorcharF110W? HST/WFC3 F110W isophotal AB mag. (2)magphot.mag;em.IR.Jdoublenullablee_F110W? Uncertainty in F110W (2)magstat.errorfloatnullableF110Wf[-5427.58/76700.12] F110W isophotal flux (3)ct/sphot.count;em.UVdoublee_F110Wf? Uncertainty in F110Wf (3)ct/sstat.errordoublenullableF110Wsig[-1.27/8778.04] F110W detection significancestat.likelihood;obsfloatl_F125WLimit flag on F125Wmeta.code.errorcharF125W? HST/WFC3 F125W isophotal AB mag. (2)magphot.mag;em.IR.Hdoublenullablee_F125W? Uncertainty in F125W (2)magstat.errorfloatnullableF125Wf[-2.701/40609.6] F125W isophotal flux (3)ct/sphot.count;em.UVdoublee_F125Wf? Uncertainty in F125Wf (3)ct/sstat.errordoublenullableF125Wsig[-2.08/7830.46] F125W detection significancestat.likelihood;obsfloatl_F140WLimit flag on F140Wmeta.code.errorcharF140W? HST/WFC3 F140W isophotal AB mag. (2)magphot.mag;em.IR.Hdoublenullablee_F140W? Uncertainty in F140W (2)magstat.errorfloatnullableF140Wf[-2.7066/46638.8] F140W isophotal flux (3)ct/sphot.count;em.UVdoublee_F140Wf? Uncertainty in F140Wf (3)ct/sstat.errordoublenullableF140Wsig[-2.1/7898.04] F140W detection significancestat.likelihood;obsfloatF160W? HST/WFC3 F160W isophotal AB mag. (2)magphot.mag;em.UV.100-200nmdoublenullablee_F160W? Uncertainty in F160W (2)magstat.errorfloatnullableF160Wf[-2.8516/29292.5] F160W isophotal flux (3)ct/sphot.count;em.UVdoublee_F160Wf? Uncertainty in F160Wf (3)ct/sstat.errordoublenullableF160Wsig[-1.09/12352.1] F140W detection significancestat.likelihood;obsdoublezb[0.014/9.989] Bayesian Photometric z (BPZ) most likely redshiftsrc.redshift.photfloate_zb[0.01/9.91] Lower 95% confidence limit on zbstat.errorfloatE_zb[0.02/10] Upper 95% confidence limit on zbstat.error;stat.maxfloattb[1/11] BPZ most likely spectral typesrc.spTypefloatOdds[0.041/1] P(z) contained within zb+/-2*0.02*(1+z) (4)stat.fit.goodnessfloatchisq[0/156] Poorness of BPZ fit: observed vs. model fluxesstat.fit.chi2floatchisq2[0/2204] Modified chisq: model fluxes given error barsstat.fit.chi2doubleM0? AB magnitude used as a priormagphot.mag;meta.modelleddoublenullablezml[0.01/10] Maximum Likelihood most likely redshiftsrc.redshiftfloattml[1/11] Maximum Likelihood most likely spectral typestat.likelihood;src.spTypefloatSEDSimbad column added by the CDSmeta.ref.urlchar