Name
9418
Title
The Sight-line toward PHL 1811: A Rare Chance to Probe a Lyman Limit System at Very Low Redshift
URL
https://hst.esac.esa.int/ehst/#/pages/search;proposal=9418;TAPCLIENT=DOI
DOI
https://doi.org/10.5270/esa-6uv8e1v
Author
Jenkins, Edward B.
Description
This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9418&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 Near-Solar Metallicity, Nitrogen-deficient Lyman Limit Absorber Associated with Two S0 Galaxies 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 A Survey of Analogs to Weak Mg II Absorbers in the Present Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-line Spectroscopy Characterizing Transition Temperature Gas in the Galactic Corona Cosmic Filaments in Superclusters Highly Ionized High-Velocity Clouds: Hot Intergalactic Medium or Galactic Halo? 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 history of enrichment of the intergalactic medium using cosmological simulations The impact of satellite trails on Hubble Space Telescope observations The Last Eight-billion Years of Intergalactic Si IV Evolution The Low-redshift Intergalactic Medium as Seen in Archival Legacy HST/STIS and FUSE Data The Low-z Intergalactic Medium. III. H I and Metal Absorbers at z < 0.4 The Low-z Intergalactic Medium. II. Lyb, O VI, and C III Forest 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 origins and evolution of weak low ionization quasar absorption line systems The Properties of Low Redshift Intergalactic O VI Absorbers Determined from High S/N Observations of 14 QSOs with the Cosmic Origins Spectrograph The properties of the extended warm ionised gas around low-redshift QSOs and the lack of extended high-velocity outflows The z = 0.0777 CIII absorber towards PHL 1811 as a case study of a low-redshift weak metal line absorber
Instrument
ACS, ACS/HRC, ACS/WFC, STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2002-10-07T14:07:12Z/2003-07-09T06:50:15Z
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
2004-07-09T06:50:15Z
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, Jenkins comma Edward B., 2004, 'The Sight-line toward PHL 1811: A Rare Chance to Probe a Lyman Limit System at Very Low Redshift', 1.0, European Space Agency, https://doi.org/10.5270/esa-6uv8e1v Copy Example
