000203187 001__ 203187
000203187 005__ 20181203023649.0
000203187 0247_ $$2doi$$a10.1093/mnras/stu1395
000203187 022__ $$a0035-8711
000203187 02470 $$2ISI$$a000342925100021
000203187 037__ $$aARTICLE
000203187 245__ $$aMass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high-redshift studies
000203187 260__ $$aOxford$$bWiley-Blackwell$$c2014
000203187 269__ $$a2014
000203187 300__ $$a22
000203187 336__ $$aJournal Articles
000203187 520__ $$aExtending over three Hubble Space Telescope (HST) cycles, the Hubble Frontier Fields (HFF) initiative constitutes the largest commitment ever of HST time to the exploration of the distant Universe via gravitational lensing by massive galaxy clusters. Here, we present models of the mass distribution in the six HFF cluster lenses, derived from a joint strong-and weak-lensing analysis anchored by a total of 88 multiple-image systems identified in existing HST data. The resulting maps of the projected mass distribution and of the gravitational magnification effectively calibrate the HFF clusters as gravitational telescopes. Allowing the computation of search areas in the source plane, these maps are provided to the community to facilitate the exploitation of forthcoming HFF data for quantitative studies of the gravitationally lensed population of background galaxies. Our models of the gravitational magnification afforded by the HFF clusters allow us to quantify the lensing-induced boost in sensitivity over blank-field observations and predict that galaxies at z > 10 and as faint as m(AB) = 32 will be detectable, up to 2 mag fainter than the limit of the Hubble Ultra Deep Field.
000203187 6531_ $$agalaxies clusters: individual: Abell 370
000203187 6531_ $$agalaxies clusters: individual: A1063S
000203187 6531_ $$agalaxies clusters: individual: Abell 2744
000203187 6531_ $$agalaxies clusters: individual: MACS J0416.1-2403
000203187 6531_ $$agalaxies clusters: individual: MACS J0717.5+3745
000203187 6531_ $$agalaxies clusters: individual: MACS J1149.5+2223
000203187 700__ $$aRichard, Johan$$uUniv Lyon 1, Observ Lyon, CRAL, F-69561 St Genis Laval, France
000203187 700__ $$aJauzac, Mathilde$$uUniv Durham, Inst Computat Cosmol, Durham DH1 3LE, England
000203187 700__ $$aLimousin, Marceau$$uUniv Aix Marseille, CNRS, Lab Astrophys Marseille, F-13388 Marseille 13, France
000203187 700__ $$aJullo, Eric$$uUniv Aix Marseille, CNRS, Lab Astrophys Marseille, F-13388 Marseille 13, France
000203187 700__ $$aClement, Benjamin$$uUniv Arizona, Steward Observ, Tucson, AZ 85721 USA
000203187 700__ $$aEbeling, Harald$$uUniv Hawaii, Inst Astron, Honolulu, HI 96822 USA
000203187 700__ $$0246614$$aKneib, Jean-Paul$$g222189$$uEcole Polytech Fed Lausanne, Observ Sauverny, Astrophys Lab, CH-1290 Versoix, Switzerland
000203187 700__ $$0246906$$aAtek, Hakim$$g230964$$uEcole Polytech Fed Lausanne, Observ Sauverny, Astrophys Lab, CH-1290 Versoix, Switzerland
000203187 700__ $$aNatarajan, Priya$$uYale Univ, Dept Astron, New Haven, CT 06511 USA
000203187 700__ $$aEgami, Eiichi$$uUniv Arizona, Steward Observ, Tucson, AZ 85721 USA
000203187 700__ $$aLivermore, Rachael
000203187 700__ $$aBower, Richard$$uUniv Durham, Inst Computat Cosmol, Durham DH1 3LE, England
000203187 773__ $$j444$$k1$$q268-289$$tMonthly Notices Of The Royal Astronomical Society
000203187 909C0 $$0252365$$pLASTRO$$xU10933
000203187 909CO $$ooai:infoscience.tind.io:203187$$pSB$$particle
000203187 917Z8 $$x103317
000203187 937__ $$aEPFL-ARTICLE-203187
000203187 973__ $$aEPFL$$rREVIEWED$$sPUBLISHED
000203187 980__ $$aARTICLE