Monitoring of the wavelength calibration lamps for the Hubble Space Telescope

Ilaria Pascucci, Charles Proffitt, Parviz Ghavamian, David Sahnow, Cristina Oliveira, Alessandra Aloisi, Tony Keyes, Steven V. Penton

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The Space Telescope Imaging Spectrograph (STIS) and the Cosmic Origins Spectrograph (COS) are the two optical-UV spectrographs on board the Hubble Space Telescope. To determine the wavelength scale for individual science observations, internal arc lamp spectra accompany most observations of external targets. Here we present a detailed analysis of the changes in the COS and STIS internal lamp fluxes and spectra over time, and also compare our results to pre-launch ground testing, and to laboratory accelerated aging testing of similar lamps. Most of the analysis presented here focuses on the behaviour of the lamps in the far-UV (FUV). We find that the STIS LINE lamp has faded by a factor of ∼15 in the very short FUV wavelengths (1150-1200Å) over the 13-year period on which STIS was in space, a much steeper fading than predicted from accelerated aging tests in the laboratory. We also find that all STIS lamps have faded during the period in which the spectrograph was not operational (2004-2009) thus pointing to on-orbit conditions as an additional and important cause of lamp fading. We report that the COS P1 lamp output appears to decline with usage with a similar slope as the LINE and HITM1 lamps on STIS. Finally, we recommend switching from the LINE to the HITM2 lamp for a more efficient wavelength calibration of the STIS settings covering the very short FUV wavelengths.

Original languageEnglish (US)
Title of host publicationSpace Telescopes and Instrumentation 2010
Subtitle of host publicationOptical, Infrared, and Millimeter Wave
DOIs
StatePublished - Oct 27 2010
Externally publishedYes
EventSpace Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave - San Diego, CA, United States
Duration: Jun 27 2010Jul 2 2010

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume7731
ISSN (Print)0277-786X

Other

OtherSpace Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave
CountryUnited States
CitySan Diego, CA
Period6/27/107/2/10

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Keywords

  • Cosmic origins spectrograph
  • Hollow cathod lamps
  • Hubble space telescope
  • Space Telescope imaging spectrograph
  • Wavelength calibration

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

Cite this

Pascucci, I., Proffitt, C., Ghavamian, P., Sahnow, D., Oliveira, C., Aloisi, A., Keyes, T., & Penton, S. V. (2010). Monitoring of the wavelength calibration lamps for the Hubble Space Telescope. In Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave [77313B] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7731). https://doi.org/10.1117/12.857465