A dataset provided by the European Space Agency

Name 8651
Title STIS UV Spectroscopy in the Magellanic Bridge: A Typical QSO Absorption Line System?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=8651;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-0eddns2
Author Kobulnicky, Henry A.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=8651&mission=hst
Publication
  • A census of quasar-intrinsic absorption in the Hubble Space Telescope archive: systems from high-resolution echelle spectra
  • A High-Resolution Survey of Low-Redshift QSO Absorption Lines: Statistics and Physical Conditions of O VI Absorbers
  • A Population of Weak Metal-Line Absorbers Surrounding the Milky Way
  • A Space Telescope Imaging Spectrograph Survey for O VI Absorption Systems at 0.12 < z lesssim 0.5. II. Physical Conditions of the Ionized Gas
  • A STIS Survey for O VI Absorption Systems at 0.12 < z lesssim 0.5. I. The Statistical Properties of Ionized Gas
  • Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-line Spectroscopy. II. Methods and Models
  • Characterizing Transition Temperature Gas in the Galactic Corona
  • Cosmic Voids and Void Properties
  • Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
  • Mining circumgalactic baryons in the low-redshift universe
  • Probing the Intergalactic Medium/Galaxy Connection. V. On the Origin of Lya and O VI Absorption at z < 0.2
  • The Connection Between a Lyman Limit System, a Very Strong O VI Absorber, and Galaxies at z ~ 0.203
  • The history of enrichment of the intergalactic medium using cosmological simulations
  • The Last Eight-billion Years of Intergalactic Si IV Evolution
  • The Low-z Intergalactic Medium. III. H I and Metal Absorbers at z < 0.4
  • The Magellanic Bridge as a Damped Lyman Alpha System: Physical Properties of Cold Gas Toward PKS 0312-770
  • The Milky Way halo as a QSO absorption-line system. New results from an HST/STIS absorption-line catalogue of Galactic high-velocity clouds
  • The Nature of Weak Mg II Absorbing Structures
Instrument STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage 2001-03-07T19:25:47Z/2001-10-16T10:45:04Z
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 2006-12-08T05:51:36Z
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, Kobulnicky comma Henry A., 2006, 'STIS UV Spectroscopy in the Magellanic Bridge: A Typical QSO Absorption Line System?', 1.0, European Space Agency, https://doi.org/10.5270/esa-0eddns2