activity
19972020
most citedThe bright Gamma-Ray Burst of February 10, 2000: a case study of an optically dark GRB

112 citations · 755 across the 30 of their papers we have counts for

collaborators

30 papers

astro-ph.EP2020★ 27 cited

A multi-chord stellar occultation by the large trans-Neptunian object (174567) Varda

D. Souami, F. Braga-Ribas, B. Sicardy +41

We present results from the first recorded stellar occultation by the large trans-Neptunian object (174567) Varda that was observed on September 10, 2018. Varda belongs…

astro-ph.SR2019★ 34 cited

First stellar spectroscopy in Leo P

C. J. Evans, N. Castro, O. A. Gonzalez +11

We present the first stellar spectroscopy in the low-luminosity (M_V ~-9.3 mag), dwarf galaxy Leo P. Its significantly low oxygen abundance (3% solar) and relative proximity (~1.6…

astro-ph.SR2018

ELT Spectroscopy of Extragalactic Massive Stars

C. J. Evans, O. H. Ramirez-Agudelo, M. Garcia +2

Quantitative spectroscopy of O-type stars in galaxies beyond 1 Mpc requires the unprecedented sensitivity of the so-called Extremely Large Telescopes. Visible spectroscopy with the…

astro-ph.GA2016★ 9 cited

Probing the Dragonfish star-forming complex: the ionizing population of the young massive cluster Mercer 30

D. de la Fuente, F. Najarro, J. Borissova +11

The Dragonfish Nebula has been recently claimed to be powered by a superluminous but elusive OB association. Instead, systematic searches in near-infrared photometric surveys have…

astro-ph.HE2015

Chandra, XMM-Newton and HST observations of a transient in M31 with a possible asymmetric, precessing disk

R. Barnard, M. R. Garcia, S. S. Murray

The transient X-ray source CXOM31 004205.77+411330.43 exhibited several outbursts during our long-term monitoring campaign of ~monthly observations of the M31 center with Chandra.…

astro-ph.HE2015★ 1 cited

XMM-Newton and Chandra observations of the M31 globular cluster black hole candidate XB135: a heavyweight contender cut down to size

R. Barnard, F. Primini, M. R. Garcia +2

CXOM31 J004252.030+413107.87 is one of the brightest X-ray sources within the D_25 region of M31, and associated with a globular cluster (GC) known as B135; we therefore call this…