A dataset provided by the European Space Agency

Name 7345
Title ORIGIN AND PHYSICAL CONDITIONS IN THE LOCAL Ly-alpha FOREST
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=7345;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-jq9kr7s
Author Stocke, John Thomas
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=7345&mission=hst
Publication
  • A Survey of Far Ultraviolet Spectroscopic Explorer and Hubble Space Telescope Sight Lines through High-Velocity Cloud Complex C
  • Characterizing Transition Temperature Gas in the Galactic Corona
  • Cosmic Filaments in Superclusters
  • Cosmic Voids and Void Properties
  • Cross-correlation of Lyman a absorbers with gas-rich galaxies
  • Discovery of a fast, broad, transient outflow in NGC 985
  • Discovery of a multiphase O VI and O VII absorber in the circumgalactic/intergalactic transition region
  • Diverse metallicities of Fermi bubble clouds indicate dual origins in the disk and halo
  • Does the Milky Way Produce a Nuclear Galactic Wind?
  • Do starburst winds escape? Insights from QSO absorption lines
  • Highly Ionized Gas Surrounding High-Velocity Cloud Complex C
  • Highly Ionized High-Velocity Clouds: Hot Intergalactic Medium or Galactic Halo?
  • Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
  • Lya Absorption around Nearby Galaxies
  • Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
  • Metallicity and Ionization in High-Velocity Cloud Complex C
  • Mid-Infrared and CO Observations of the Infrared/X-Ray Luminous Seyfert 1 Galaxy NGC 985: The Making or Breaking of a ULIRG?
  • Origins of highly ionized gas in high-velocity clouds
  • O VI, N V, and C IV in the Galactic Halo. II. Velocity-Resolved Observations with the Hubble Space Telescope and Far Ultraviolet Spectroscopic Explorer
  • Probing the chemical composition of the Z < 1 intergalactic medium with observations and simulations
  • Probing the Intergalactic Medium/Galaxy Connection. V. On the Origin of Lya and O VI Absorption at z < 0.2
  • The Last Eight-Billion Years of Intergalactic C IV Evolution
  • The Local Lya Forest. IV. Space Telescope Imaging Spectrograph G140M Spectra and Results on the Distribution and Baryon Content of H I Absorbers
  • The Properties and Evolution of the Highly Ionized Gas in MR 2251-178
  • The Relationship Between Baryons and Dark Matter in Extended Galaxy Halos
  • Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies
  • Ultraviolet characteristics, outflow properties and variability of active galactic nucleus Markarian 1513
  • Warm Gas in the Virgo Cluster. I. Distribution of Lya Absorbers
Instrument STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage 1997-11-08T13:55:14Z/2000-08-02T06:03:00Z
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 2002-05-20T00:00:00Z
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, Stocke comma John Thomas, 2002, 'ORIGIN AND PHYSICAL CONDITIONS IN THE LOCAL Ly-alpha FOREST', 1.0, European Space Agency, https://doi.org/10.5270/esa-jq9kr7s