Chandra Observations of the cl1604 Supercluster at z = 0.9: Evidence for an Overdensity of Active Galactic Nuclei, Kocevski, Dale D.,Lubin, Lori M.,Gal, Roy, The Astrophysical Journal, 690, 2009-01-01 00:00:00, 2009ApJ...690..295K||Environmental Impact on Star-forming Galaxies in a z ∼ 0.9 Cluster during the Course of Galaxy Accretion, Asano, Tetsuro,Kodama, Tadayuki,Motohara, Kentaro, The Astrophysical Journal, 899, 2020-08-01 00:00:00, 2020ApJ...899...64A||Evolution of galaxy scaling relations in clusters at 0.5 < z < 1.5, Pérez-Martínez, J. M.,Ziegler, B.,Dannerbauer, H., Astronomy and Astrophysics, 646, 2021-02-01 00:00:00, 2021A&A...646A..53P||Obscured Starburst Activity in High-redshift Clusters and Groups, Kocevski, Dale D.,Lemaux, Brian C.,Lubin, Lori M., The Astrophysical Journal, 736, 2011-07-01 00:00:00, 2011ApJ...736...38K||Properties of Galaxies Hosting X-ray-selected Active Galactic Nuclei in the CL1604 Supercluster at z = 0.9, Kocevski, Dale D.,Lubin, Lori M.,Lemaux, Brian C., The Astrophysical Journal, 700, 2009-08-01 00:00:00, 2009ApJ...700..901K||Searching for environmental effects on galaxy kinematics in groups and clusters at z ∼ 1 from the ORELSE survey, Pelliccia, Debora,Lemaux, Brian C.,Tomczak, Adam, Monthly Notices of the Royal Astronomical Society, 482, 2019-01-01 00:00:00, 2019MNRAS.482.3514P||Serendipitous Discovery of an Overdensity of Lyα Emitters at z ~ 4.8 in the CL1604 Supercluster Field, Lemaux, B. C.,Lubin, L. M.,Sawicki, M., The Astrophysical Journal, 700, 2009-07-01 00:00:00, 2009ApJ...700...20L||Star Formation Quenching in High-redshift Large-scale Structure: Post-starburst Galaxies in the Cl 1604 Supercluster at z ~ 0.9, Wu, Po-Feng,Gal, Roy R.,Lemaux, Brian C., The Astrophysical Journal, 792, 2014-09-01 00:00:00, 2014ApJ...792...16W||The Assembly of the Red Sequence at z ~ 1: The Color and Spectral Properties of Galaxies in the Cl1604 Supercluster, Lemaux, B. C.,Gal, R. R....,Lubin, L. M., The Astrophysical Journal, 745, 2012-02-01 00:00:00, 2012ApJ...745..106L||The Complex Structure of the Cl 1604 Supercluster at z ~ 0.9, Gal, R. R.,Lemaux, B. C.,Lubin, L. M., The Astrophysical Journal, 684, 2008-09-01 00:00:00, 2008ApJ...684..933G||The violent youth of bright and massive cluster galaxies and their maturation over 7 billion years, Ascaso, B.,Lemaux, B. C.,Lubin, L. M., Monthly Notices of the Royal Astronomical Society, 442, 2014-07-01 00:00:00, 2014MNRAS.442..589A||X-ray-emitting active galactic nuclei from z = 0.6 to 1.3 in the intermediate- and high-density environments of the ORELSE survey, Rumbaugh, N.,Lemaux, B. C.,Tomczak, A., Monthly Notices of the Royal Astronomical Society, 466, 2017-04-01 00:00:00, 2017MNRAS.466..496R
Instrument
ACS, ACS/WFC
Temporal Coverage
2006-11-23T10:48:49Z/2006-12-03T21:59:05Z
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, 2007, Mixing It Up : Gas, Stars, Starbirth, And Agn In A Supercluster At Z = 0.9, 1.0, European Space Agency, https://doi.org/10.5270/esa-5p86fuk
