sameAs
Ly α EMISSION FROM A LUMINOUS z = 8.68 GALAXY: IMPLICATIONS FOR GALAXIES AS TRACERS OF COSMIC REIONIZATIONA tentative detection of an emission line at 1.6 {mu}m for the z ~ 12 candidate UDFj-39546284A magnified young galaxy from about 500 million years after the Big Bang.Rapid evolution of the most luminous galaxies during the first 900 million years.A large population of 'Lyman-break' galaxies in a protocluster at redshift z approximately 4.1.Rotation in [C ii]-emitting gas in two galaxies at a redshift of 6.8.Astronomy: Quasars signpost massive galaxies.CLASH: three strongly lensed images of a candidate z {approx} 11 galaxyA mature cluster with X-ray emission atz= 2.07The Science Case for PILOT I: Summary and OverviewALMA spectroscopic survey in the Hubble Ultra Deep Field: survey descriptionThe ALMA spectroscopic survey in the Hubble Ultra Deep Field: molecular gas reservoirs in high-redshift galaxiesAGN Feedback Causes DownsizingModels of Disk Evolution: Confrontation with ObservationsCloning Hubble Deep Fields. I. A Model‐independent Measurement of Galaxy EvolutionCloning Hubble Deep Fields. II. Models for Evolution by Bright Galaxy Image TransformationCLASH: the concentration-mass relation of galaxy clustersNot in our backyard: spectroscopic support for the CLASH z=11 candidate MACS 0647-JDThe MUSIC of CLASH: predictions on the concentration-mass relationCLASH-x: a comparison of lensing and X-ray techniques for measuring the mass profiles of galaxy clustersCLASH: a census of magnified star-forming galaxies at z ~ 6-8CLASH: extending galaxy strong lensing to small physical scales with distant sources highly magnified by galaxy cluster membersThree gravitationally lensed supernovae behind CLASH galaxy clustersCLASH: Photometric redshifts with 16 HST bands in galaxy cluster fieldsCLASH: z ∼ 6 young galaxy candidate quintuply lensed by the frontier field cluster RXC J2248.7−4431CLASH: complete lensing analysis of the largest cosmic lens MACS J0717.5+3745 and surrounding structuresThe contribution of halos with different mass ratios to the overall growth of cluster-sized halosCLASH: the enhanced lensing efficiency of the highly elongated merging cluster MACS J0416.1-2403CLASH: PRECISE NEW CONSTRAINTS ON THE MASS PROFILE OF THE GALAXY CLUSTER A2261CLASH: mass distribution in and around MACS J1206.2-0847 from a full cluster lensing analysisThe Cluster Lensing And Supernova survey with Hubble: an overviewCLASH: discovery of a bright z =~ 6.2 dwarf galaxy quadruply lensed by MACS J0329.6-0211The MUSE Hubble Ultra Deep Field Survey I. Survey description, data reduction, and source detectionThe evolution of mass-size relation for Lyman break galaxies from z = 1 to z = 7z∼ 7 GALAXY CANDIDATES FROM NICMOS OBSERVATIONS OVER THE HDF-SOUTH AND THE CDF-SOUTH AND HDF-NORTH GOODS FIELDSThe Environment of M85 Optical Transient 2006‐1: Constraints on the Progenitor Age and MassStrong‐Lensing Analysis of A1689 from Deep Advanced Camera ImagesFaint Galaxies in Deep Advanced Camera for Surveys ObservationsDiscovery of Two Distant Type Ia Supernovae in the Hubble Deep Field–North with the Advanced Camera for SurveysAdvanced Camera for Surveys Observations of Young Star Clusters in the Interacting Galaxy UGC 10214
P50
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astrofísico estadounidense
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astrónomu estauxunidense
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