activity
19992026
most citedThe Cosmic Baryon and Metal Cycles

321 citations · 6.3k across the 122 of their papers we have counts for

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12 papers · 1 filter

astro-ph.CO2024★ 9 cited

Extragalactic 85Rb/87Rb and 6Li/7Li ratios in the Small Magellanic Cloud

P. Molaro, P. Bonifacio, G. Cupani +1

The line of sight toward Sk 143 (AzV 456), an O9.5 Ib star in the Small Magellanic Cloud (SMC), shows significant absorption from neutral atoms and molecules. We report a new study…

astro-ph.CO2020★ 12 cited

The Third Data Release of the KODIAQ Survey

John M. O'Meara, Nicolas Lehner, J. Christopher Howk +1

We present and make publicly available the third data release (DR3) of the Keck Observatory Database of Ionized Absorption toward Quasars (KODIAQ) survey. KODIAQ DR3 consists of a…

astro-ph.CO2015★ 87 cited

The First Data Release of the KODIAQ Survey

J. M. O'Meara, N. Lehner, J. C. Howk +6

We present and make publicly available the first data release (DR1) of the Keck Observatory Database of Ionized Absorption toward Quasars (KODIAQ) survey. The KODIAQ survey is aime…

astro-ph.CO2014★ 117 cited

Galactic and Circumgalactic OVI and its Impact on the Cosmological Metal and Baryon Budgets at 2<z<3.5

Nicolas Lehner, John M. O'Meara, Andrew J. Fox +4

We present the first results from our NASA Keck Observatory Database of Ionized Absorbers toward Quasars (KODIAQ) survey which aims to characterize the properties of the highly ion…

astro-ph.CO2013★ 41 cited

The High-Ion Content and Kinematics of Low-Redshift Lyman Limit Systems

Andrew J. Fox, Nicolas Lehner, Jason Tumlinson +9

We study the high-ionization phase and kinematics of the circumgalactic medium around low-redshift galaxies using a sample of 23 Lyman Limit Systems (LLSs) at 0.08<z<0.93 observed…

astro-ph.CO2013★ 220 cited

The Bimodal Metallicity Distribution of the Cool Circumgalactic Medium at z<1

N. Lehner, J. C. Howk, T. M. Tripp +7

We assess the metal content of the cool (10^4 K) circumgalactic medium (CGM) about galaxies at z<1 using an H I-selected sample of 28 Lyman limit systems (LLS, defined here as abso…

astro-ph.CO2012★ 2 cited

Project Lyman: Quantifying 11 Gyrs of Metagalactic Ionizing Background Evolution

Stephan R. McCandliss, B-G Andersson, Nils Bergvall +23

The timing and duration of the reionization epoch is crucial to the emergence and evolution of structure in the universe. The relative roles that star-forming galaxies, active gala…

astro-ph.CO2012★ 82 cited

QSO Absorption Systems Detected in Ne VIII: High-Metallicity Clouds with a Large Effective Cross Section

Joseph D. Meiring, Todd M. Tripp, Jessica K. Werk +5

Using high resolution, high signal-to-noise ultraviolet spectra of the z = 0.9754 quasar PG1148+549 obtained with the Cosmic Origins Spectrograph (COS) on the Hubble Space Telescop…

astro-ph.CO2011★ 158 cited

The Hidden Mass and Large Spatial Extent of a Poststarburst Galaxy Outflow

Todd M. Tripp, Joseph D. Meiring, J. Xavier Prochaska +9

Outflowing winds of multiphase plasma have been proposed to regulate the buildup of galaxies, but key aspects of these outflows have not been probed with observations. Using ultrav…

astro-ph.CO2010★ 41 cited

The Interstellar Medium and Star Formation in Edge-On Galaxies. I. NGC 891

Kijeong Yim, Tony Wong, J. Christopher Howk +1

We analyze images of BIMA 12CO (J = 1 --> 0), VLA HI, and Spitzer 3.6 and 24 \mum emission toward the edge-on galaxy NGC 891 and derive the radial and vertical distributions of gas…

astro-ph.CO2009★ 96 cited

Wavelength Accuracy of the Keck HIRES Spectrograph and Measuring Changes in the Fine Structure Constant

Kim Griest, Jonathan B. Whitmore, Arthur M. Wolfe +3

We report on an attempt to accurately wavelength calibrate four nights of data taken with the Keck HIRES spectrograph on QSO PHL957, for the purpose of determining whether the fine…

astro-ph.CO2009★ 1 cited

Strong z~0.5 O VI Absorption Toward PKS 0405-123: Implications for Ionization and Metallicity of the Cosmic Web

J. Christopher Howk, Joseph S. Ribaudo, Nicolas Lehner +2

We present observations of the O VI system at z_abs = 0.495096 toward PKS 0405-123 (z_em = 0.5726) obtained with FUSE and STIS. In addition to strong O VI, with log N(O VI) = 14.47…