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, Mowla, Lamiya A.,van der Wel, Arjen,van Dokkum, Pieter, The Astrophysical Journal, 872, 2019-02-01 00:00:00, 2019ApJ...872L..13M||A quantitative assessment of completeness correction methods and public release of a versatile simulation code, Leethochawalit, Nicha,Trenti, Michele,Morishita, Takahiro, Monthly Notices of the Royal Astronomical Society, 509, 2022-02-01 00:00:00, 2022MNRAS.509.5836L||A Stellar Velocity Dispersion for a Strongly-lensed, Intermediate-mass Quiescent Galaxy at z=2.8, Hill, Allison. R.,Muzzin, Adam,Franx, Marijn, The Astrophysical Journal, 819, 2016-03-01 00:00:00, 2016ApJ...819...74H||COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation since z ∼ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D-HST, Mowla, Lamiya A.,van Dokkum, Pieter,Brammer, Gabriel, The Astrophysical Journal, 880, 2019-07-01 00:00:00, 2019ApJ...880...57M||Dusty Starbursts and the Formation of Elliptical Galaxies: A SCUBA-2 Survey of a z = 1.46 Cluster, Ma, C.-J.,Smail, Ian,Swinbank, A. M., The Astrophysical Journal, 806, 2015-06-01 00:00:00, 2015ApJ...806..257M||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, Marsan, Z. Cemile,Marchesini, Danilo,Muzzin, Adam, The Astrophysical Journal, 871, 2019-02-01 00:00:00, 2019ApJ...871..201M||Near-infrared Spectroscopy of Five Ultra-massive Galaxies at 1.7 < z < 2.7, Kado-Fong, Erin,Marchesini, Danilo,Marsan, Z. Cemile, The Astrophysical Journal, 838, 2017-03-01 00:00:00, 2017ApJ...838...57K||Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z = 3.35: a Detailed Look at an Early Progenitor of Local Giant Ellipticals, Marsan, Z. Cemile,Marchesini, Danilo,Brammer, Gabriel, The Astrophysic...al Journal, 801, 2015-03-01 00:00:00, 2015ApJ...801..133M||The Hubble Legacy Field GOODS-S Photometric Catalog, Whitaker, Katherine E.,Ashas, Mohammad,Illingworth, Garth, The Astrophysical Journal Supplement Series, 244, 2019-09-01 00:00:00, 2019ApJS..244...16W||The mean Hα EW and Lyman-continuum photon production efficiency for faint z ≈ 4-5 galaxies, Lam, Daniel,Bouwens, Rychard J.,Labbé, Ivo, Astronomy and Astrophysics, 627, 2019-07-01 00:00:00, 2019A&A...627A.164L||The missing light of the Hubble Ultra Deep Field, Borlaff, Alejandro,Trujillo, Ignacio,Román, Javier, Astronomy and Astrophysics, 621, 2019-01-01 00:00:00, 2019A&A...621A.133B
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.
European Space Agency, 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
