A decrease of the gas exchanges between galaxies and the intergalactic medium, from 12 to 6 billion years ago
An infrared view of the coevolution of massive blackholes and galaxies
A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z 4
Combining weak and strong cluster lensing: applications to simulations and MS 2137
Revealing the formation histories of the first stars with the cosmic near-infrared background
The MUSE Hubble Ultra Deep Field Survey. XVI. The angular momentum of low-mass star-forming galaxies: A cautionary tale and insights from TNG50
The UV 2175A attenuation bump and its correlation with PAH emission at z 2
Instrument
WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
2003-09-24T08:34:15Z/2004-01-15T07:50:55Z
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, Beckwith comma Steven, 2004, 'The Ultra Deep Field - WFPC2 Parallels', 1.0, European Space Agency, https://doi.org/10.5270/esa-9w1tywk