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19982019
most citedLong gamma-ray bursts and core-collapse supernovae have different environments

843 citations · 5.1k across the 45 of their papers we have counts for

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astro-ph2008★ 61 cited

GRB 070714B - Discovery of the Highest Spectroscopically Confirmed Short Burst Redshift

J. F. Graham, A. S. Fruchter, A. J. Levan +10

We detect the optical afterglow and host galaxy of GRB 070714B. Our observations of the afterglow show an initial plateau in the lightcurve for approximately the first 5 to 25 minu…

astro-ph2008★ 116 cited

High resolution spectroscopy for Cepheids distance determination. I. Line asymmetry

N. Nardetto, D. Mourard, P. Kervella +3

The ratio of pulsation to radial velocity (the projection factor) is currently limiting the accuracy of the interferometric Baade-Wesselink method. This work aims at establishing a…

astro-ph2008★ 1 cited

A large-scale survey for variable stars in M33

D. Bersier, J. D. Hartman, K. Z. Stanek +6

We have started a survey of M 33 in order to find variable stars and Cepheids in particular. We have obtained more than 30 epochs of g'r'i' data with the CFHT and the one-square-de…

astro-ph2008★ 3 cited

GRB 070714B - Discovery of the Highest Spectroscopically Confirmed Short Burst Redshift

J. F. Graham, A. S. Fruchter, A. J. Levan +5

Gemini Nod & Shuffle spectroscopy on the host of the short GRB 070714B shows a single emission line at 7167 angstroms which, based on a grizJHK photometric redshift, we conclude is…

astro-ph2008★ 4 cited

LOFAR-UK White Paper: A Science case for UK involvement in LOFAR

P. N. Best, the LOFAR-UK Consortium

LOFAR, the Low-Frequency Array, is a next-generation software-driven radio telescope operating between 30 and 240MHz, currently under construction by ASTRON in the Netherlands. Thi…

astro-ph2006

A Review of Early-Time Optical Follow-ups with 2-m Robotic Telescopes

A. Gomboc, C. Guidorzi, C. G. Mundell +9

We summarise recent deep, rapid GRB follow-up observations using the RoboNet-1.0 network which comprises three fully-robotic 2-m telescopes, the Liverpool Telescope and the Faulkes…

astro-ph2006★ 143 cited

The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33

A. Z. Bonanos, K. Z. Stanek, R. P. Kudritzki +12

We present the first direct distance determination to a detached eclipsing binary in M33, which was found by the DIRECT Project. Located in the OB 66 association at coordinates (al…

astro-ph2006★ 12 cited

The first Swift X-ray Flash: The faint afterglow of XRF 050215B

A. J. Levan, J. P. Osborne, N. R. Tanvir +17

We present the discovery of XRF 050215B and its afterglow. The burst was detected by the Swift BAT during the check-out phase and observations with the X-ray telescope began approx…

astro-ph2006★ 66 cited

Deep CFHT Photometric Survey of the Entire M33 Galaxy I: Catalogue of 36000 Variable Point Sources

J. D. Hartman, D. Bersier, K. Z. Stanek +4

We have conducted a variability survey of the local group galaxy M33 using g', r', and i' observations from 27 nights spanning 17 months made with the MegaPrime/MegaCam instrument…

astro-ph2006★ 843 cited

Long gamma-ray bursts and core-collapse supernovae have different environments

A. S. Fruchter, A. J. Levan, L. Strolger +30

When massive stars exhaust their fuel they collapse and often produce the extraordinarily bright explosions known as core-collapse supernovae. On occasion, this stellar collapse al…

astro-ph2006★ 67 cited

Evidence for a Supernova Associated with the X-ray Flash 020903

D. Bersier, A. S. Fruchter, L. -G. Strolger +24

We present ground-based and Hubble Space Telescope optical observations of the X-ray flash (XRF) 020903, covering 300 days. The afterglow showed a very rapid rise in the first day,…

astro-ph2005★ 119 cited

Discovery and identification of the very high redshift afterglow of GRB 050904

J. Haislip, M. Nysewander, D. Reichart +39

In 2000, Lamb and Reichart predicted that gamma-ray bursts (GRBs) and their afterglows occur in sufficient numbers and at sufficient brightnesses at very high redshifts (z > 5) to…

astro-ph2004★ 37 cited

Cepheid distances from infrared long-baseline interferometry - II. Calibration of the Period-Radius and Period-Luminosity relations

P. Kervella, D. Bersier, D. Mourard +2

Using our interferometric observations of seven classical Cepheids reported in Kervella et al. (2003, Paper I), complemented by previously existing measurements, we derive new cali…

astro-ph2002★ 69 cited

The Strongly Polarized Afterglow of GRB 020405

D. Bersier, B. McLeod, P. M. Garnavich +12

We report polarization measurements and photometry for the optical afterglow of the gamma-ray burst GRB 020405. We measured a highly significant 9.9% polarization (in V band) 1.3 d…

astro-ph2000★ 33 cited

The distance to the Fornax dwarf galaxy using red clump stars, and the discrepancy between red clump and tip of the red giant branch distances

D. Bersier

I determine a distance to the Fornax dwarf galaxy using stars in the red clump and at the tip of the red giant branch. They are in very good agreement, with . Comp…

astro-ph1998★ 47 cited

The MACHO Project Large Magellanic Cloud Variable Star Inventory. VIII. The Recent Star Formation History of the LMC from the Cepheid Period Distribution

C. Alcock, R. A. Allsman, D. R. Alves +20

We present an analysis of the period distribution of Cepheids in the Large Magellanic Cloud, based on data obtained by the MACHO microlensing experiment and on a previo…