activity
20022010
most citedHigh-Redshift Starbursting Dwarf Galaxies Revealed by GRB Afterglows

97 citations · 251 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2010★ 35 cited

Improving the identification of high-z Herschel sources with position priors and optical/NIR and FIR/mm photometric redshifts

P. G. Pérez-González, E. Egami, M. Rex +36

We present preliminary results about the detection of high redshift (U)LIRGs in the Bullet cluster field by the PACS and SPIRE instruments within the Herschel Lensing Survey (HLS)…

astro-ph.CO2010★ 31 cited

Deep Herschel view of obscured star formation in the Bullet cluster

T. D. Rawle, S. M. Chung, D. Fadda +33

We use deep, five band (100-500um) data from the Herschel Lensing Survey (HLS) to fully constrain the obscured star formation rate, SFR_FIR, of galaxies in the Bullet cluster (z=0.…

astro-ph2008★ 97 cited

High-Redshift Starbursting Dwarf Galaxies Revealed by GRB Afterglows

Hsiao-Wen Chen, Daniel A. Perley, Lindsey K. Pollack +7

We present a study of 15 long-duration gamma-ray burst (GRB) host galaxies at z>2. The GRBs are selected with available early-time afterglow spectra in order to compare interstella…

astro-ph2006★ 49 cited

On the absence of Wind Signatures in GRB Afterglow Spectra: Constraints on the Wolf-Rayet Winds of GRB Progenitors

Hsiao-Wen Chen, Jason X. Prochaska, Enrico Ramirez-Ruiz +3

We investigate available constraints on the circumstellar medium (CSM) around long-duration gamma-ray burst (GRB) progenitors from afterglow spectra. We first establish a statistic…

astro-ph2006★ 39 cited

Temporal Variation in Excited Fe^+ Near a GRB Afterglow

Miroslava Dessauges-Zavadsky, Hsiao-Wen Chen, Jason X. Prochaska +2

Excited Si^+ and Fe^+ species are routinely observed in the host environment of gamma-ray burst (GRB) afterglows, but are not commonly seen in other extragalactic locations. Their…

astro-ph2002

H2, D/H and the CMBR Temperature at z = 3.025 Toward QSO 0347-3819

S. A. Levshakov, P. Molaro, M. Dessauges-Zavadsky +1

A new molecular hydrogen cloud has been identified at z = 3.025 in the absorption-line spectrum of the quasar 0347-3819 observed with the UVES spectrograph at the VLT/Kueyen telesc…