57 datasets found

Keywords: intergalactic medium

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  • Hydra I cluster study with H I emission

    We present results from our analysis of the Hydra I cluster observed in neutral atomic hydrogen (H I) as part of the Widefield ASKAP L-band Legacy All-sky Blind Survey...
  • Thermal parameters of the IGM at 2 <= z <= 4

    We characterize the thermal state of the intergalactic medium (IGM) in 10 redshift bins in the range 2 <= z <= 4 with a sample of 103 high-resolution, high S/N Ly{alpha}...
  • Lyman limit systems in large quasar surveys

    We present a pipeline based on a random forest classifier for the identification of high column density clouds of neutral hydrogen (i.e. the Lyman limit systems, LLSs) in...
  • Quasar Sightline and Galaxy Evolution Survey I

    We present the first results from a study of OVI absorption around galaxies at z<1.44 using data from a near-infrared grism spectroscopic Hubble Space Telescope Large...
  • HI enhancement in proto-cluster

    In the SSA22 field which exhibits a large-scale proto-cluster at z=3.1, we carried out a spectroscopic survey for Lyman Break Galaxies (LBGs) with the VLT/VIMOS and identified...
  • Void catalogs from SDSS DR7

    We produce several public void catalogs using a volume-limited subsample of the Sloan Digital Sky Survey Data Release 7 (SDSS DR7). Using new implementations of three different...
  • CLAMATO DR2 redshift catalog

    We present the second data release of the COSMOS Ly{alpha} Mapping And Tomography Observations Survey conducted with the Low Resolution Imaging Spectrometer on the Keck I...
  • Damped Ly{alpha} systems from SDSS DR16Q

    We present the characteristics of the damped Ly{alpha} (DLA) systems found in data release DR16 of the extended Baryon Oscillation Spectroscopic Survey of the Sloan Digital Sky...
  • CLAMATO DR1: 3D Ly{alpha} forest tomography

    Faint star-forming galaxies at z~2-3 can be used as alternative background sources to probe the Ly{alpha} forest in addition to quasars, yielding high sightline densities that...
  • Gal. redshift survey near HST/COS AGN sight lines

    To establish the connection between galaxies and UV-detected absorption systems in the local universe, a deep (g<=20) and wide (~20' radius) galaxy redshift survey is...
  • 2<zobs<4 quasars stacked spectrum

    We investigate the metal species associated with the Ly{alpha} forest in eBOSS quasar spectra. Metal absorption lines are revealed in stacked spectra from cross-correlating the...
  • CGM2 galaxy-OVI absorber pairs

    We combine 126 new galaxy-OVI absorber pairs from the CGM^2^ survey with 123 pairs drawn from the literature to examine the simultaneous dependence of the column density of OVI...
  • Compilation of double radio sources

    The origin of magnetic fields in clusters of galaxies is still a matter of debate. Observations for intracluster magnetic fields over a wide range of redshifts are crucial to...
  • Milky Way SiIV and CIV kinematics from HST/COS

    We compose a 265-sight-line Milky Way CIV line-shape sample using the Hubble Space Telescope/Cosmic Origins Spectrograph archive, which is complementary to the existing SiIV...
  • Galaxy-absorber pairs for low-z QSO sightlines

    We present a study of candidate galaxy-absorber pairs for 43 low-redshift QSO sightlines (0.06<z<0.85) observed with the Hubble Space Telescope/Cosmic Origins Spectrograph...
  • VLT/X-SHOOTER & Keck/ESI spectra of z~5 QSOs

    We present a new investigation of the intergalactic medium (IGM) near the end of reionization using "dark gaps" in the Ly{alpha} forest. Using spectra of 55 QSOs at...
  • 18 UV bright QSOs obs. with HST (COS-IGrM survey)

    We present the results of the Cosmic Origins Spectrograph-Intragroup Medium (COS-IGrM) Survey that used the COS on the Hubble Space Telescope to observe a sample of 18 UV bright...
  • A large sample of FR II radio sources

    The dynamical evolution and radiative properties of luminous radio galaxies and quasars of the FR II type, are well understood. As a result, through the use of detailed modeling...
  • WALLABY pilot survey: HI gas in Hydra cluster

    This study uses HI image data from the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) pilot survey with the Australian Square Kilometre Array Pathfinder (ASKAP)...
  • Ly{alpha} emitters and QSOs in COMSOS and EGS fields

    We present cosmological (30-400Mpc) distributions of neutral hydrogen (HI) in the intergalactic medium (IGM) traced by Ly{alpha} emitters (LAEs) and QSOs at z=2.1-2.5, selected...
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