A dataset provided by the European Space Agency

Name 12990
Title Size Growth at the Top: WFC3 Imaging of Ultra-Massive Galaxies at 1.5 < z < 3
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12990;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-9twunvp
Author Muzzin, Adam
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12990&mission=hst
Publication
  • A Mass-dependent Slope of the Galaxy Size-Mass Relation out to z ~ 3: Further Evidence for a Direct Relation between Median Galaxy Size and Median Halo Mass
  • A quantitative assessment of completeness correction methods and public release of a versatile simulation code
  • A Stellar Velocity Dispersion for a Strongly-lensed, Intermediate-mass Quiescent Galaxy at z=2.8
  • Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys
  • COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation since z ~ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D-HST
  • Dusty Starbursts and the Formation of Elliptical Galaxies: A SCUBA-2 Survey of a z = 1.46 Cluster
  • HST F160W Imaging of Very Massive Galaxies at 1.5 < z < 3.0: Diversity of Structures and the Effect of Close Pairs on Number Density Estimates
  • MIDIS: JWST NIRCam and MIRI Unveil the Stellar Population Properties of Lya Emitters and Lyman-break Galaxies at z 3-7
  • MIDIS: Strong (Hb+O III) and Ha Emitters at Redshift z 7-8 Unveiled with JWST NIRCam and MIRI Imaging in the Hubble eXtreme Deep Field
  • Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
  • Near-infrared Spectroscopy of Five Ultra-massive Galaxies at 1.7 < z < 2.7
  • Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. I. Point-spread Function Modeling and Systematics
  • Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z = 3.35: a Detailed Look at an Early Progenitor of Local Giant Ellipticals
  • The hidden side of cosmic star formation at z > 3. Bridging optically dark and Lyman-break galaxies with GOODS-ALMA
  • The Hubble Legacy Field GOODS-S Photometric Catalog
  • The mean Ha EW and Lyman-continuum photon production efficiency for faint z 4-5 galaxies
  • The missing light of the Hubble Ultra Deep Field
  • The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
  • The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
Instrument WFC3, WFC3/IR
Temporal Coverage 2012-10-12T23:26:30Z/2013-11-08T16:04:37Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2014-11-09T05:28:09Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Muzzin comma Adam, 2014, 'Size Growth at the Top: WFC3 Imaging of Ultra-Massive Galaxies at 1.5 < z < 3', 1.0, European Space Agency, https://doi.org/10.5270/esa-9twunvp