A 7 deg2 survey for galaxy-scale gravitational lenses with the HST imaging archive, Pawase, R. S.,Courbin, F.,Faure, C., Monthly Notices of the Royal Astronomical Society, 439, 2014-02-01 00:00:00, 2014MNRAS.439.3392P||Assembly of the Red Sequence in Infrared-selected Galaxy Clusters from the IRAC Shallow Cluster Survey, Snyder, Gregory F.,Brodwin, Mark,Mancone, Conor M., The Astrophysical Journal, 756, 2012-09-01 00:00:00, 2012ApJ...756..114S||First Weak-lensing Results from “See Change”: Quantifying Dark Matter in the Two z ≳ 1.5 High-redshift Galaxy Clusters SPT-CL J2040-4451 and IDCS J1426+3508, Jee, M. James,Ko, Jongwan,Perlmutter, Saul, The Astrophysical Journal, 847, 2017-10-01 00:00:00, 2017ApJ...847..117J||Hα Star Formation Rates of z > 1 Galaxy Clusters in the IRAC Shallow Cluster Survey, Zeimann, Gregory R.,Stanford, S. A.,Brodwin, Mark, The Astrophysical Journal, 779, 2013-12-01 00:00:00, 2013ApJ...779..137Z||IDCS J1426.5+3508: Cosmological Implications of a Massive, Strong Lensing Cluster at z = 1.75, Gonzalez, Anthony H.,Stanford, S. Adam,Brodwin, Mark, The Astrophysical Journal, 753, 2012-07-01 00:00:00, 2012ApJ...753..163G||IDCS J1426.5+3508: Discovery of a Massive, Infrared-selected Galaxy Cluster at z = 1.75, Stanford, S. A.,Brodwin, M.,Gonzalez, Anthony H., The Astrophysical Journal, 753, 2012-07-01 00:00:00, 2012ApJ...753..164S||IDCS J1426.5+3508: Sunyaev-Zel'dovich Measurement of a Massive Infrared-selected Cluster at z = 1.75, Brodwin, M.,Gonzalez, A. H.,Stanford, S. A., The Astrophysical Journal, 753, 2012-07-01 00:00:00, 2012ApJ...753..162B||IDCS J1426.5+3508: The Most Massive Galaxy Cluster at z > 1.5, Brodwin, Mark,McDonald, Michael,Gonzalez, Anthony H., The Astrophysical Journal, 817, 2016-02-01 00:00:00, 2016ApJ...817..122B||IDCS J1426.5+3508: Weak Lensing Analysis of a Massive Galaxy Cluster at z = 1.75, Mo, Wenli,Gonzalez, Anthony,Jee, M. James, The Astrophysical Journal..., 818, 2016-02-01 00:00:00, 2016ApJ...818L..25M||IDCS J1433.2+3306: An Infrared-selected Galaxy Cluster at z = 1.89, Zeimann, Gregory R.,Stanford, S. A.,Brodwin, Mark, The Astrophysical Journal, 756, 2012-09-01 00:00:00, 2012ApJ...756..115Z||Measuring the total infrared light from galaxy clusters at z = 0.5-1.6: connecting stellar populations to dusty star formation, Alberts, Stacey,Lee, Kyoung-Soo,Pope, Alexandra, Monthly Notices of the Royal Astronomical Society, 501, 2021-02-01 00:00:00, 2021MNRAS.501.1970A||Molecular gas in two companion cluster galaxies at z = 1.2, Castignani, G.,Combes, F.,Salomé, P., Astronomy and Astrophysics, 617, 2018-09-01 00:00:00, 2018A&A...617A.103C||PyGFit: A Tool for Extracting PSF Matched Photometry, Mancone, Conor L.,Gonzalez, Anthony H.,Moustakas, Leonidas A., Publications of the Astronomical Society of the Pacific, 125, 2013-12-01 00:00:00, 2013PASP..125.1514M||Star Formation in High-redshift Cluster Ellipticals, Wagner, Cory R.,Brodwin, Mark,Snyder, Gregory F., The Astrophysical Journal, 800, 2015-02-01 00:00:00, 2015ApJ...800..107W||The Era of Star Formation in Galaxy Clusters, Brodwin, M.,Stanford, S. A.,Gonzalez, Anthony H., The Astrophysical Journal, 779, 2013-12-01 00:00:00, 2013ApJ...779..138B||The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries, Hayden, B.,Rubin, D.,Boone, K., The Astrophysical Journal, 912, 2021-05-01 00:00:00, 2021ApJ...912...87H||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||The Morphology-Density Relationship in 1 < z < 2 Clusters, Sazonova, Elizaveta,Alatalo, Katey,Lotz, Jennifer M., The Astrophysical Journal, 899, 2020-08-01 00:00:00, 2020ApJ...899...85S||X-ray Emission from Two Infrared-selected Galaxy Clusters at z > 1.4 in the IRAC Shallow Cluster Survey, Brodwin, M.,Stern, D.,Vikhlinin, A., The Astrophysical Journal, 732, 2011-05-01 00:00:00, 2011ApJ...732...33B
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2010-03-06T02:57:46Z/2010-11-21T15:11:42Z
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, 2011, Formation And Evolution Of Massive Galaxies In The Richest Environments At 1.5 < Z < 2.0, 1.0, European Space Agency, https://doi.org/10.5270/esa-dsleqze
