Cross-correlation of Lyman a absorbers with gas-rich galaxies
Far-Ultraviolet Spectroscopy of the Intergalactic and Interstellar Absorption toward 3C 273
New Observations with the HST Goddard High Resolution Spectrograph of the Low-Redshift Lyman-Alpha Clouds in the 3C 273 Line of Sight
Observations of 3C273 with the Goddard High Resolution Spectrograph on the Hubble Space Telescope. II.
ORFEUS II Far-Ultraviolet Observations of 3C 273: Interstellar and Intergalactic Absorption Lines
O VI, N V, and C IV in the Galactic Halo. II. Velocity-Resolved Observations with the Hubble Space Telescope and Far Ultraviolet Spectroscopic Explorer
The Galaxy Environment of O VI Absorption Systems
The Local Lya Forest. II. Distribution of H I Absorbers,Doppler Widths, and Baryon Content
The Local Lya Forest. I. Observations with the GHRS/G160M on the Hubble Space Telescope
The Search for Intergalactic Hydrogen Clouds in Voids
Instrument
HRS, HRS/2
Temporal Coverage
1993-11-26T21:26:11Z/1993-11-27T00:32:21Z
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, Weymann comma Ray J., 1994, 'WEAK ABSORPTION LINES IN 3C273: CYCLE 2 OBSERVATIONS', 1.0, European Space Agency, https://doi.org/10.5270/esa-d2zwe4k
