A dataset provided by the European Space Agency

Name 8421
Title STIS Spectroscopic Sensitivity for MAMA and CCD
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=8421;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-9isb74y
Author Leitherer, Claus
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=8421&mission=hst
Publication
  • A Comparative Study of the Atmospheric Composition of the DA White Dwarfs Feige 24 and G191-B2B
  • A comprehensive near- and far-ultraviolet spectroscopic study of the hot DA white dwarf G191-B2B
  • Constraining the magnetic field on white dwarf surfaces; Zeeman effects and fine structure constant variation
  • Discovery of Photospheric Germanium in Hot DA White Dwarfs
  • Hot DA white dwarf model atmosphere calculations: including improved Ni PI cross-sections
  • Hubble Space Telescope Flux Calibration. I. STIS and CALSPEC
  • Limits on the Dependence of the Fine-Structure Constant on Gravitational Potential from White-Dwarf Spectra
  • Measuring chemical evolution and gravitational dependence of a using ultraviolet Fe v and Ni v transitions in white-dwarf spectra
  • Measuring the fine-structure constant on a white dwarf surface; a detailed analysis of Fe V absorption in G191-B2B
  • Stellar laboratories. III. New Ba v, Ba vi, and Ba vii oscillator strengths and the barium abundance in the hot white dwarfs G191-B2B and RE 0503-289
  • Stellar laboratories. II. New Zn iv and Zn v oscillator strengths and their validation in the hot white dwarfs G191-B2B and RE 0503-289
  • Stellar laboratories . VIII. New Zr iv-vii, Xe iv-v, and Xe vii oscillator strengths and the Al, Zr, and Xe abundances in the hot white dwarfs G191-B2B and RE 0503-289
  • Stellar laboratories. VI. New Mo iv-vii oscillator strengths and the molybdenum abundance in the hot white dwarfs G191-B2B and RE 0503-289
  • Stellar laboratories. X. New Cu IV-VII oscillator strengths and the first detection of copper and indium in hot white dwarfs
  • The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
  • The Structure of the Local Interstellar Medium. II. Observations of D I, C II, N I, O I, Al II, and Si II toward Stars within 100 Parsecs
  • The virtual observatory service TheoSSA: Establishing a database of synthetic stellar flux standards. I. NLTE spectral analysis of the DA-type white dwarf G191-B2B
Instrument STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage 2000-01-30T17:04:24Z/2000-03-19T06:49:06Z
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.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2000-03-19T20:16:56Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Leitherer comma Claus, 2000, 'STIS Spectroscopic Sensitivity for MAMA and CCD', 1.0, European Space Agency, https://doi.org/10.5270/esa-9isb74y