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19942023
most citedHerwig 7.0 / Herwig++ 3.0 Release Note

1.2k citations · 13.1k across the 150 of their papers we have counts for

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44 papers · 1 filter

astro-ph2008★ 105 cited

High Redshift Metals I.: The Decline of C IV at z > 5.3

George D. Becker, Michael Rauch, Wallace L. W. Sargent

We present the results from our search for C IV in the intergalactic medium at redshifts z=5.3-6.0. We have observed four z~6 QSOs with Keck/NIRSPEC in echelle mode. The data are t…

astro-ph2007★ 234 cited

A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems

Michael Rauch, Martin Haehnelt, Andrew Bunker +10

We have conducted a long slit search for low surface brightness Lyman-alpha emitters at redshift 2.67 < z < 3.75. A 92 hour long exposure with VLT/FORS2 down to a 1-sigma surface b…

astro-ph2007★ 207 cited

How cold is cold dark matter? Small scales constraints from the flux power spectrum of the high-redshift Lyman-alpha forest

M. Viel, G. D. Becker, J. S. Bolton +3

We present constraints on the mass of warm dark matter (WDM) particles derived from the Lyman-alpha flux power spectrum of 55 high- resolution HIRES spectra at 2.0 < z < 6.4. From…

astro-ph2007★ 40 cited

Galactic Wind Signatures around High Redshift Galaxies

Daisuke Kawata, Michael Rauch

We carry out cosmological chemodynamical simulations with different strengths of supernova (SN) feedback and study how galactic winds from star-forming galaxies affect the features…

astro-ph2006★ 227 cited

The Evolution of Optical Depth in the Ly-alpha Forest: Evidence Against Reionization at z~6

George D. Becker, Michael Rauch, Wallace L. W. Sargent

We examine the evolution of the IGM Ly-alpha optical depth distribution using the transmitted flux probability distribution function (PDF) in a sample of 63 QSOs spanning absorptio…

astro-ph2006★ 67 cited

A Spectacular Radio Flare from XRF 050416a at 40 days and Implications for the Nature of X-ray Flashes

A. M. Soderberg, E. Nakar, S. B. Cenko +26

We present detailed optical, near-infrared, and radio observations of the X-ray flash 050416a obtained with Palomar and Siding Springs Observatories as well as HST and the VLA, pla…

astro-ph2005★ 77 cited

Discovery of excess O I absorption towards the z = 6.42 QSO SDSS J1148+5251

George D. Becker, Wallace L. W. Sargent, Michael Rauch +1

We present a search for O I in the spectra of nine 4.9 < z_qso < 6.4 QSOs taken with Keck/HIRES. We detect six systems with N(O I) > 10^13.7 cm^{-2} in the redshift intervals where…

astro-ph2005★ 503 cited

The afterglow of GRB050709 and the nature of the short-hard gamma-ray bursts

D. B. Fox, D. A. Frail, P. A. Price +33

The final chapter in the long-standing mystery of the gamma-ray bursts (GRBs) centres on the origin of the short-hard class, suspected on theoretical grounds to result from the coa…

astro-ph2005★ 40 cited

Expansion and Collapse in the Cosmic Web

Michael Rauch, George D. Becker, Matteo Viel +5

We study the kinematics of the gaseous cosmic web at high redshift with Lyman alpha forest absorption in multiple QSO sightlines. Using a simple analytic model and a cosmological h…

astro-ph2005★ 144 cited

Observations of Chemically Enriched QSO Absorbers near z ~ 2.3 Galaxies: Galaxy-Formation Feedback Signatures in the IGM

Robert A. Simcoe, Wallace L. W. Sargent, Michael Rauch +1

We present a study of galaxies and intergalactic gas toward the z=2.73 quasar HS1700+6416, to explore the effects of galaxy formation feedback on the IGM. Our observations and ioni…

astro-ph2005★ 49 cited

Tightening Constraints from the Lyman Alpha Forest with the Flux Probability Distribution Function

Adam Lidz, Katrin Heitmann, Lam Hui +3

The analysis of the Lyman-alpha forest of absorption lines in quasar spectra has emerged as a potentially powerful technique to constrain the linear matter power spectrum. In most…

astro-ph2005★ 71 cited

An HST Study of the Supernovae Accompanying GRB 040924 and GRB 041006

A. M. Soderberg, S. R. Kulkarni, P. A. Price +23

We present the results from a {\it Hubble Space Telescope/ACS} study of the supernovae associated with gamma-ray bursts 040924 () and 041006 (). We find evidence th…

astro-ph2005★ 98 cited

An HST Search for Supernovae Accompanying X-ray Flashes

A. M. Soderberg, S. R. Kulkarni, D. B. Fox +24

We present the results from an Hubble Space Telescope/ACS search for supernovae associated with X-ray flashes 020903, 040701, 040812 and 040916. We find strong evidence that XRF 02…

astro-ph2004★ 140 cited

Abundance Profiles and Kinematics of Damped Lyman-alpha Absorbing Galaxies at z < 0.65

Hsiao-Wen Chen, Robert C. Kennicutt, Michael Rauch

We present a spectroscopic study of six damped Lya absorption (DLA) systems at z<0.65, based on moderate-to-high resolution spectra of the galaxies responsible for the absorbers. C…

astro-ph2004★ 25 cited

Large-Scale Correlations in the Lyman-alpha Forest at z = 3-4

George D. Becker, Wallace L. W. Sargent, Michael Rauch

We present a study of the spatial coherence of the intergalactic medium toward two pairs of high-redshift quasars with moderate angular separations observed with Keck/ESI, Q1422+23…

astro-ph2004★ 228 cited

The Distribution of Metallicity in the IGM at z~2.5: OVI and CIV Absorption in the Spectra of 7 QSOs

Robert A. Simcoe, Wallace L. W. Sargent, Michael Rauch

We present a direct measurement of the metallicity distribution function for the high redshift intergalactic medium. We determine the shape of this function using survival statisti…

astro-ph2003★ 116 cited

Metallicity of the intergalactic medium using pixel statistics: III. Silicon

Anthony Aguirre, Joop Schaye, Tae-Sun Kim +3

(Modified) We study the abundance of silicon in the intergalactic medium by analyzing the statistics of SiIV, CIV, and HI pixel optical depths in a sample of 19 high-quality quasar…

astro-ph2002★ 100 cited

Characterizing the Warm-Hot IGM at High Redshift: A High Resolution Survey for O VI at z = 2.5

Robert A. Simcoe, Wallace L. W. Sargent, Michael Rauch

We describe a survey for OVI absorption in the spectra of 5 high redshift quasars (2.2 < z < 2.8). We identify 12 cosmological systems, and 6 systems that are either ejected from t…

astro-ph2002★ 68 cited

Small Scale Structure at High Redshift: IV. Low Ionization Gas Intersecting Three Lines of Sight to Q2237+0305

M. Rauch, W. L. W. Sargent, T. A. Barlow +1

We have obtained Keck HIRES spectra of three images of the gravitationally lensed QSO 2237+0305 to study low ionization absorption systems and their differences in terms of project…

astro-ph2001★ 56 cited

Small Scale Structure at High Redshift: III. The Clumpiness of the Intergalactic Medium on Sub-kpc Scales

Michael Rauch, Wallace L. W. Sargent, Thomas A. Barlow +1

Spectra from the Keck HIRES instrument of the Lyman alpha forests in the lines of sight to the A and C components of the gravitationally lensed QSO Q1422+231 were used to investiga…

astro-ph2001★ 109 cited

Small Scale Structure at High Redshift: II. Physical Properties of the CIV Absorbing Clouds

Michael Rauch, Wallace L. W. Sargent, Thomas A. Barlow

Keck HIRES spectra were obtained of the separate images of three gravitationally lensed QSOs (UM 673, Q1104-1804, and Q1422+2309). We studied the velocity and column density differ…

astro-ph2000★ 169 cited

A Measurement of the Temperature-Density Relation in the Intergalactic Medium Using a New Lyman-alpha Absorption Line Fitting Method

Patrick McDonald, Jordi Miralda-Escude, Michael Rauch +3

The evolution of the temperature in the intergalactic medium is related to the reionization of hydrogen and helium, and has important consequences for our understanding of the Lya…

astro-ph2000

Constraining reionization using the thermal history of the baryons

Joop Schaye, Tom Theuns, Michael Rauch +2

The thermal evolution of the intergalactic medium (IGM) depends on the reionization history of the universe. Numerical simulations indicate that the low density IGM, which is respo…

astro-ph1999★ 397 cited

The thermal history of the intergalactic medium

Joop Schaye, Tom Theuns, Michael Rauch +2

At redshifts z >~ 2, most of the baryons reside in the smooth intergalactic medium which is responsible for the low column density Lyman-alpha forest. This photoheated gas follows…