A multi-epoch spectroscopic study of the BAL quasar APM 08279+5255. I. C IV absorption variability
A multi-epoch spectroscopic study of the BAL quasar APM 08279+5255. II. Emission- and absorption-line variability time lags
An old quasar in a young dark energy-dominated universe?
Imaging The Molecular Gas in a z = 3.9 Quasar Host Galaxy at 0farcs3 Resolution: A Central, Sub-Kiloparsec Scale Star Formation Reservoir in APM 08279+5255
Restframe UV-to-optical spectroscopy of APM 08279+5255. BAL classification and black hole mass estimates
Spatially resolved STIS spectra of the gravitationally lensed broad absorption line quasar APM08279+5255: the nature of component C and evidence for microlensing
The sizes and kinematic structure of absorption systems towards the lensed quasar APM08279+5255
Instrument
STIS/CCD, WFPC2, WFPC2/PC
Temporal Coverage
2001-05-11T00:44:14Z/2001-05-11T08:54:34Z
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, ELLISON SARA, 2003, 'Spatially Resolved Spectroscopy of APM08279+5255', 1.0, European Space Agency, https://doi.org/10.5270/esa-ag2j5r0