A bright, dust-obscured, millimetre-selected galaxy beyond the Bullet Cluster (1E0657-56), Wilson, G. W.,Hughes, D. H.,Aretxaga, I., Monthly Notices of the Royal Astronomical Society, 390, 2008-11-01 00:00:00, 2008MNRAS.390.1061W||A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters, Shu, X. W.,Yang, Lei,Liu, Daizhong, The Astrophysical Journal, 926, 2022-02-01 00:00:00, 2022ApJ...926..155S||A Direct Empirical Proof of the Existence of Dark Matter, Clowe, Douglas,Bradač, Maruša,Gonzalez, Anthony H., The Astrophysical Journal, 648, 2006-09-01 00:00:00, 2006ApJ...648L.109C||A Multiply Imaged Luminous Infrared Galaxy Behind the Bullet Cluster (1E0657-56), Gonzalez, Anthony H.,Clowe, Douglas,Bradač, Maruša, The Astrophysical Journal, 691, 2009-01-01 00:00:00, 2009ApJ...691..525G||Constraints on the Self-Interaction Cross Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-56, Randall, Scott W.,Markevitch, Maxim,Clowe, Douglas, The Astrophysical Journal, 679, 2008-06-01 00:00:00, 2008ApJ...679.1173R||Deep luminosity functions and colour-magnitude relations for cluster galaxies at 0.2 < z < 0.6, De Propris, R.,Phillipps, S.,Bremer, M. N., Monthly Notices of the Royal Astronomical Society, 434, 2013-10-01 00:00:00, 2013MNRAS.434.3469D||Evolution of the observed Lyα luminosity function from z = 6.5 to z = 7.7: evidence for the epoch of reionization?, Clément, B.,Cuby, J.-G.,Courbin, F., Astronomy and Astrophysics, 538, 2012-02-01 00:00:00, 2012A&A...538A..66C||Little change in the sizes of the most massive galaxies since z = 1, Stott, J. P.,Collins, C. A.,Burke, C., Monthly Notices of the Royal Astronomical Society, 414, 2011-06-01 00:00:00, 2011MNRAS.414..445S||Looking for dark matter trails in colliding galaxy clusters, Harvey, David,Robertson, Andrew,Massey, Richard, Monthly Notices of the Royal Astronomical Society, 464, ...2017-02-01 00:00:00, 2017MNRAS.464.3991H||Lyman Break Galaxies under a Microscope: The Small-Scale Dynamics and Mass of an Arc in the Cluster 1E 0657-56, Nesvadba, N. P. H.,Lehnert, M. 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Instrument
ACS, ACS/WFC
Temporal Coverage
2004-10-21T14:10:42Z/2004-10-21T21:19:07Z
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, 2005, Dark Matter Constraints From The Merging Cluster 1E0657-56, 1.0, European Space Agency, https://doi.org/10.5270/esa-ft6exjz
