Analysis of Breit-Pauli Transition Probabilities for Lines in O III
Fe VII lines in the spectrum of RR Telescopii
Forbidden and Intercombination Lines of RR Telescopii: Wavelength Measurements and Energy Levels
On the effect of emission lines on UBVR photometry
O VI Recombination Lines in Ultraviolet and Visible Spectra of RR Telescopii
Revised Analysis of Fe VII
The calibration of read-out-streak photometry in the XMM-Newton Optical Monitor and the construction of a bright-source catalogue
The HeII Fowler lines and the OIII and NIII Bowen fluorescence lines in the symbiotic nova RR Telescopii
The O I 1641 A line as a probe of symbiotic star winds
The OIV and SIV intercombination lines in the ultraviolet spectra of astrophysical sources
XMM-Newton observations of RR Telescopii: evidence for wind signatures and shocked gas emission
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2000-10-18T15:08:37Z/2000-10-18T19:05:54Z
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, Keenan comma Francis, 2001, 'Fe II emission lines as a chronometer for high-redshift quasars', 1.0, European Space Agency, https://doi.org/10.5270/esa-auninfl