A dataset provided by the European Space Agency

Name 13398
Title A Breakaway from Incremental Science: Full Characterization of the z<1 CGM and Testing Galaxy Evolution Theory
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=13398;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-oodljfr
Author Churchill, Christopher W.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=13398&mission=hst
Publication
  • An Extreme Metallicity, Large-scale Outflow from a Star-forming Galaxy at z ~ 0.4
  • An HST/COS survey of molecular hydrogen in DLAs & sub-DLAs at z < 1: molecular fraction and excitation temperature
  • Cloud-by-cloud multiphase investigation of the circumgalactic medium of low-redshift galaxies
  • COS-Weak: probing the CGM using analogues of weak Mg II absorbers at z < 0.3
  • Discovery of extremely low-metallicity circumgalactic gas at z = 0.5 towards Q0454-220
  • Disentangling the multiphase circumgalactic medium shared between a dwarf and a massive star-forming galaxy at z~0.4
  • Evidence for galaxy quenching in the green valley caused by a lack of a circumgalactic medium
  • Halo Mass Dependence of H I and O VI Absorption: Evidence for Differential Kinematics
  • Kinematics of the O VI Circumgalactic Medium: Halo Mass Dependence and Outflow Signatures
  • Low-mass Group Environments Have No Substantial Impact on the Circumgalactic Medium Metallicity
  • MAGIICAT VI. The Mg II Intragroup Medium Is Kinematically Complex
  • Molecular Hydrogen Absorption from the Halo of a z ~ 0.4 Galaxy
  • MUSE-ALMA haloes VI: coupling atomic, ionized, and molecular gas kinematics of galaxies
  • Relationship between the Metallicity of the Circumgalactic Medium and Galaxy Orientation
  • Spatial Distribution of O VI Covering Fractions in the Simulated Circumgalactic Medium
  • The Azimuthal Dependence of Outflows and Accretion Detected Using O VI Absorption
  • The Extent of Chemically Enriched Gas around Star-forming Dwarf Galaxies
  • The extreme ultraviolet spectra of low-redshift radio-loud quasars
  • The Highly Ionized Circumgalactic Medium is Kinematically Uniform around Galaxies
  • The Impact of the Group Environment on the O VI Circumgalactic Medium
  • The Relation between Galaxy ISM and Circumgalactic O VI Gas Kinematics Derived from Observations and LCDM Simulations
  • The Relationship between Galaxy ISM and Circumgalactic Gas Metallicities
  • The Signature of the Northern Galactic Center Region in Low-velocity UV Absorption
Instrument COS, COS/FUV, COS/NUV
Temporal Coverage 2013-10-30T18:10:00Z/2014-11-27T22:09:43Z
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 2014-11-28T00:38:27Z
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, Churchill comma Christopher W., 2014, 'A Breakaway from Incremental Science: Full Characterization of the z<1 CGM and Testing Galaxy Evolution Theory', 1.0, European Space Agency, https://doi.org/10.5270/esa-oodljfr