A dataset provided by the European Space Agency

Name 11598
Title How Galaxies Acquire their Gas: A Map of Multiphase Accretion and Feedback in Gaseous Galaxy Halos
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=11598;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-es17jc9
Author Tumlinson, Jason
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=11598&mission=hst
Publication
  • A Budget and Accounting of Metals at z ~ 0: Results from the COS-Halos Survey
  • A Deep Search for Faint Galaxies Associated with Very Low Redshift C IV Absorbers. III. The Mass- and Environment-dependent Circumgalactic Medium
  • A Deep Search For Faint Galaxies Associated With Very Low-redshift C IV Absorbers. II. Program Design, Absorption-line Measurements, and Absorber Statistics
  • Ambient Column Densities of Highly Ionized Oxygen in Precipitation-limited Circumgalactic Media
  • An HST/COS survey of molecular hydrogen in DLAs & sub-DLAs at z < 1: molecular fraction and excitation temperature
  • An Ultraviolet Survey of Low-redshift Partial Lyman-limit Systems with the HST Cosmic Origins Spectrograph
  • A Universal Density Structure for Circumgalactic Gas
  • Baryon cycling in the low-redshift circumgalactic medium: a comparison of simulations to the COS-Halos survey
  • Bimodality of low-redshift circumgalactic O VI in non-equilibrium EAGLE zoom simulations
  • CGM2 + CASBaH: The Mass Dependence of H I Lya-Galaxy Clustering and the Extent of the CGM
  • CGM2 I: The Extent of the Circumgalactic Medium Traced by Neutral Hydrogen
  • Characterizing circumgalactic gas around massive ellipticals at z ~ 0.4 - I. Initial results
  • Characterizing circumgalactic gas around massive ellipticals at z ~ 0.4 - II. Physical properties and elemental abundances
  • Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-line Spectroscopy. II. Methods and Models
  • Cloud-by-cloud multiphase investigation of the circumgalactic medium of low-redshift galaxies
  • Constraining UV Continuum Slopes of Active Galactic Nuclei with CLOUDY Models of Broad-line Region Extreme-ultraviolet Emission Lines
  • Cool circumgalactic gas of passive galaxies from cosmological inflow
  • COS-burst: Observations of the Impact of Starburst-driven Winds on the Properties of the Circum-galactic Medium
  • COS-Weak: probing the CGM using analogues of weak Mg II absorbers at z < 0.3
  • Detection of a Multiphase Intragroup Medium: Results from the COS-IGrM Survey
  • Empirically Constrained Predictions for Metal-line Emission from the Circumgalactic Medium
  • Entropy-driven winds: Outflows and fountains lifted gently by buoyancy
  • Extreme Circumgalactic H I and C III Absorption around the Most Massive, Quenched Galaxies
  • Fast winds drive slow shells: a model for the circumgalactic medium as galactic wind-driven bubbles
  • High-velocity clouds as streams of ionized and neutral gas in the halo of the Milky Way
  • HST/COS Observations of Thirteen New He II Quasars
  • Hubble Asteroid Hunter. I. Identifying asteroid trails in Hubble Space Telescope images
  • Hubble Asteroid Hunter. III. Physical properties of newly found asteroids
  • Ha Distances to the Leading Arm of the Magellanic Stream
  • Implications of the Large O VI Columns around Low-redshift L * Galaxies
  • Interpreting Observations of Absorption Lines in the Circumgalactic Medium with a Turbulent Medium
  • Kinematics of Circumgalactic Gas: Feeding Galaxies and Feedback
  • Kinematics of the Magellanic Stream and Implications for Its Ionization
  • Kinematics of the O VI Circumgalactic Medium: Halo Mass Dependence and Outflow Signatures
  • Low-metallicity Absorbers Account for Half of the Dense Circumgalactic Gas at z 1
  • MAGIICAT VI. The Mg II Intragroup Medium Is Kinematically Complex
  • Massive Warm/Hot Galaxy Coronae as Probed by UV/X-Ray Oxygen Absorption and Emission. I. Basic Model
  • Massive Warm/Hot Galaxy Coronae. II. Isentropic Model
  • Mining circumgalactic baryons in the low-redshift universe
  • Modeling Photoionized Turbulent Material in the Circumgalactic Medium. II. Effect of Turbulence within a Stratified Medium
  • Molecular hydrogen from z = 0.0963 DLA towards the QSO J1619+3342
  • Most of the cool CGM of star-forming galaxies is not produced by supernova feedback
  • Multiphase Gas in Galaxy Halos: The O VI Lyman-limit System toward J1009+0713
  • MUSEQuBES: characterizing the circumgalactic medium of redshift 3.3 Ly a emitters
  • Not Dead Yet: Cool Circumgalactic Gas in the Halos of Early-type Galaxies
  • Not So Heavy Metals: Black Hole Feedback Enriches the Circumgalactic Medium
  • On the CGM Fundamental Plane: The Halo Mass Dependency of Circumgalactic H I
  • On the connection between the intergalactic medium and galaxies: the H I-galaxy cross-correlation at z 1
  • On the connection between the metal-enriched intergalactic medium and galaxies: an O VI-galaxy cross-correlation study at z < 1
  • On the possible environmental effect in distributing heavy elements beyond individual gaseous haloes
  • O VI traces photoionized streams with collisionally ionized boundaries in cosmological simulations of z ~ 1 massive galaxies
  • Physical conditions and redshift evolution of optically thin C III>absorbers: low-z sample
  • Probing Large Galaxy Halos at Z ~ 0 with Automated Lya-absorption Matching
  • Probing the CGM of low-redshift dwarf galaxies using FIRE simulations
  • Relationship between the Metallicity of the Circumgalactic Medium and Galaxy Orientation
  • Role of cosmic rays in the circumgalactic medium
  • The abundance, distribution, and physical nature of highly ionized oxygen O VI, O VII, and O VIII in IllustrisTNG
  • The Azimuthal Dependence of Outflows and Accretion Detected Using O VI Absorption
  • The baryon cycle of Seven Dwarfs with superbubble feedback
  • The Bimodal Absorption System Imaging Campaign (BASIC). I. A Dual Population of Low-metallicity Absorbers at z < 1
  • The Bimodal Metallicity Distribution of the Cool Circumgalactic Medium at z <~ 1
  • The CGM2 Survey: Circumgalactic O VI from Dwarf to Massive Star-forming Galaxies
  • The CGM2 Survey: Quenching and the Transformation of the Circumgalactic Medium
  • The Circumgalactic Medium of eBOSS Emission Line Galaxies: Signatures of Galactic Outflows in Gas Distribution and Kinematics
  • The Cool Circumgalactic Medium of Low-redshift Star-forming Galaxies. I. Empirical Model and Mean Properties
  • The COS Absorption Survey of Baryon Harbors: The Galaxy Database and Cross-correlation Analysis of O VI Systems
  • The COS CGM Compendium. III. Metallicity and Physical Properties of the Cool Circumgalactic Medium at z 1
  • The COS CGM Compendium. I. Survey Design and Initial Results
  • The COS-Dwarfs Survey: The Carbon Reservoir around Sub-L* Galaxies
  • The COS-Halos Survey: An Empirical Description of Metal-line Absorption in the Low-redshift Circumgalactic Medium
  • The COS-Halos Survey: Keck LRIS and Magellan MagE Optical Spectroscopy
  • The COS-Halos Survey: Metallicities in the Low-redshift Circumgalactic Medium
  • The COS-Halos Survey: Origins of the Highly Ionized Circumgalactic Medium of Star-Forming Galaxies
  • The COS-Halos Survey: Physical Conditions and Baryonic Mass in the Low-redshift Circumgalactic Medium
  • The COS-Halos Survey: Rationale, Design, and a Census of Circumgalactic Neutral Hydrogen
  • The Cosmic Ultraviolet Baryon Survey: Empirical Characterization of Turbulence in the Cool Circumgalactic Medium
  • The COS/UVES Absorption Survey of the Magellanic Stream. III. Ionization, Total Mass, and Inflow Rate onto the Milky Way
  • The Dispersion of Fast Radio Bursts from a Structured Intergalactic Medium at Redshifts z < 1.5
  • The Extended Distribution of Baryons around Galaxies
  • The Extreme Ultraviolet Variability of Quasars
  • The First Observations of Low-redshift Damped Lya Systems with the Cosmic Origins Spectrograph
  • The First Observations of Low-redshift Damped Lya Systems with the Cosmic Origins Spectrograph: Chemical Abundances and Affiliated Galaxies
  • The Formation and Physical Origin of Highly Ionized Cooling Gas
  • The Galaxys veil of excited hydrogen
  • The gas and stellar mass of low-redshift damped Lyman-a absorbers
  • The Gas-Galaxy Connection at z abs = 0.35: O VI and H I Absorption toward J 0943+0531
  • The High-ion Content and Kinematics of Low-redshift Lyman Limit Systems
  • The Highly Ionized Circumgalactic Medium is Kinematically Uniform around Galaxies
  • The impact of satellite trails on Hubble Space Telescope observations
  • The Impact of the Group Environment on the O VI Circumgalactic Medium
  • The Large, Oxygen-Rich Halos of Star-Forming Galaxies Are a Major Reservoir of Galactic Metals
  • The Mass and Absorption Column Densities of Galactic Gaseous Halos. II. The High Ionization State Ions
  • The Properties of the Circumgalactic Medium in Red and Blue Galaxies: Results from the COS-GASS+COS-Halos Surveys
  • The Relation between Galaxy ISM and Circumgalactic O VI Gas Kinematics Derived from Observations and LCDM Simulations
  • The Signature of the Northern Galactic Center Region in Low-velocity UV Absorption
  • Where do Galaxies End?
  • X-Ray Detection of the Galaxys Missing Baryons in the Circumgalactic Medium of L* Galaxies
Instrument COS, COS/FUV, COS/NUV, WFC3, WFC3/UVIS
Temporal Coverage 2010-03-06T05:51:39Z/2011-08-04T14:59:01Z
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 2012-08-04T18:33:41Z
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, Tumlinson et al., 2012, 'How Galaxies Acquire their Gas: A Map of Multiphase Accretion and Feedback in Gaseous Galaxy Halos', 1.0, European Space Agency, https://doi.org/10.5270/esa-es17jc9