Evaluating the Accuracy of Non-parametric Galaxy Morphological Indicator Measurements in the CSST Imaging Survey
Identification of High-redshift Galaxy Overdensities in GOODS-N and GOODS-S
Not Just a Dot: The Complex UV Morphology and Underlying Properties of Little Red Dots
The First Photometric Evidence of a Transient/Variable Source at z > 5 with JWST
The impact of satellite trails on Hubble Space Telescope observations
The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z = 3.5
The z 9 Galaxy UV Luminosity Function from the JWST Advanced Deep Extragalactic Survey: Insights into Early Galaxy Evolution and Reionization
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2005-11-26T23:34:32Z/2005-11-28T05:06:56Z
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, Sirianni et al., 2005, 'CTE and QE measurement for ACS CCDs at three different temperatures', 1.0, European Space Agency, https://doi.org/10.5270/esa-tit6646
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.