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相关论文: The Metallicity of Intergalactic Gas in Cosmic Voi…

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We investigate the association between galaxies and metal-enriched and metal-deficient absorbers in the local universe ($z < 0.16$) using a large compilation of FUV spectra of bright AGN targets observed with the Cosmic Origins Spectrograph…

星系天体物理 · 物理学 2018-03-14 C. T. Pratt , J. T. Stocke , B. A. Keeney , C. W. Danforth

We conduct an ultraviolet (HST and FUSE) spectroscopic survey of HI (Lyman lines) and seven metal ions (OVI, NV, CIV, CIII, SiIV, SiIII, FeIII) in the low-redshift intergalactic medium (IGM) at z<0.4. We analyzed 650 Lya absorbers over…

天体物理学 · 物理学 2009-11-13 Charles W. Danforth , J. Michael Shull

We present high-resolution UV spectra of absorption-line systems toward the low-z QSO HS0624+6907 (z=0.3700). Coupled with spectroscopic galaxy redshifts, we find that many of these absorbers are integalactic gas clouds distributed within…

We search for weak O VI absorption in the low-redshift intergalactic medium (IGM) using 82 high signal-to-noise quasar spectra obtained with the Cosmic Origins Spectrograph on board the Hubble Space Telescope. From this dataset, we compile…

星系天体物理 · 物理学 2025-12-12 Sapna Mishra , Vikram Khaire , Romeo Pallikkara , Anand Narayanan , Andrew J. Fox

We analyze the association of galaxies to Lya and OVI absorption, the most commonly detected transitions in the low-z intergalactic medium (IGM), in the fields of 14 quasars with z_em = 0.06-0.57. Confirming previous studies, we observe a…

宇宙学与河外天体物理 · 物理学 2015-05-27 J. Xavier Prochaska , B. Weiner , H. -W. Chen , J. S. Mulchaey , K. L. Cooksey

The intergalactic medium (IGM) is believed to contain the majority of baryons in the universe and to trace the same dark matter structure as galaxies, forming filaments and sheets. Lya absorbers, which sample the neutral component of the…

宇宙学与河外天体物理 · 物理学 2021-03-31 Sietske J. D. Bouma , Philipp Richter , Martin Wendt

We combine a FUSE sample of OVI absorbers (z < 0.15) with a database of 1.07 million galaxy redshifts to explore the relationship between absorbers and galaxy environments. All 37 absorbers with N(OVI) > 10^{13.2} cm^-2 lie within 800…

We create stacked composite absorption spectra from Hubble Space Telescope Faint Object Spectrograph data from four quasi-stellar objects to search for absorption lines in the extreme ultraviolet wavelength region associated with LyA forest…

天体物理学 · 物理学 2009-11-07 R. C. Telfer , G. A. Kriss , W. Zheng , A. F. Davidsen , D. Tytler

In this paper, we use large-angle, nearby galaxy redshift surveys to investigate the relationship between the 81 low-redshift Lya absorbers in our HST/GHRS survey and galaxies, superclusters, and voids. In a subsample of 46 Lya absorbers…

天体物理学 · 物理学 2009-11-07 Steven V. Penton , John T. Stocke , J. Michael Shull

We present a detailed analysis of the intergalactic metal-line absorption systems in the archival HST/STIS and FUSE ultraviolet spectra of the low-redshift quasar PKS1302-102 (z_QSO = 0.2784). We supplement the archive data with CLOUDY…

We use high-resolution UV spectra of the radio-quiet QSO H1821+643 (z_em = 0.297), obtained with STIS and FUSE, to study the ionization and metallicity of an intervening O VI absorption line system at z(abs) = 0.1212. This absorber has the…

天体物理学 · 物理学 2009-11-07 Todd M. Tripp , Mark L. Giroux , John T. Stocke , Jason Tumlinson , William R. Oegerle

We present a detailed study of the physical properties of absorbers associated with $z\approx3.3$ \lya\ emitters (LAEs) from the MUSEQuBES survey. Using \HI\ and ionic column densities derived from Voigt profile fitting, we determine the…

星系天体物理 · 物理学 2026-01-14 Eshita Banerjee , Sowgat Muzahid , Joop Schaye , Sean D. Johnson , Sebastiano Cantalupo

We present an ultraviolet quasar absorption line analysis of metal lines associated with three strong intervening H I absorbers (with $N$(H I) $>$ 10$^{16.5}$ cm$^{-2}$) detected in the outskirts of Sunyaev-Zel'dovich (SZ) effect-selected…

We present the KODIAQ-Z survey aimed to characterize the cool, photoionized gas at 2.2<z<3.6 in 202 HI-selected absorbers with 14.6<log N(HI)<20, i.e., the gaseous interface between galaxies and the intergalactic medium (IGM). We find that…

Low ionization metal absorption due to OI has been identified as an important probe of the physical state of the inter-/circumgalactic medium at the tail-end of reionization. We use here high-resolution hydrodynamic simulations to interpret…

宇宙学与河外天体物理 · 物理学 2015-06-17 Laura C. Keating , Martin G. Haehnelt , George D. Becker , James S. Bolton

We have conducted pointed redshift surveys for galaxies in the direction of bright AGN whose HST far-UV spectra contain nearby (cz <~ 30,000 kms), low column density (12.5 <= log N_{HI} (cm s^{-2}) <= 14.5) Ly-alpha forest absorption…

天体物理学 · 物理学 2009-11-07 Kevin M. McLin , John T. Stocke , R. J. Weymann , Steven V. Penton , J. Micheal Shull

We investigate the impact of environment on the metallicity of the diffuse intergalactic medium. We use pixel correlation techniques to search for weak CIV and OVI absorption in the spectrum of quasar Q1422+231 in regions of the spectrum…

天体物理学 · 物理学 2009-11-13 Matthew M. Pieri , Joop Schaye , Anthony Aguirre

(Abridged) We study metal absorption around 854 $z\approx$2.4 star-forming galaxies taken from the Keck Baryonic Structure Survey (KBSS). The galaxies examined in this work lie in the fields of 15 hyper-luminous background QSOs, with galaxy…

宇宙学与河外天体物理 · 物理学 2015-02-10 Monica L. Turner , Joop Schaye , Charles C. Steidel , Gwen C. Rudie , Allison L. Strom

We characterize the metallicities and physical properties of cool, photoionized gas in a sample of 152 z<1 strong Lya forest systems (SLFSs, absorbers with 15<log N(HI)<16.2). The sample is drawn from our COS circumgalactic medium (CGM)…

We present a sample of 34 weak metal line absorbers at $z< 0.3$ complied via the simultaneous detections ($3\sigma$) of the SiII$\lambda1260$ and CII$\lambda1334$ absorption lines, with $W_{r}$(SiII)$<0.2$ \AA\ and $W_{r}$(CII)$<0.3$ \AA,…

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