activity
20072026
most citedFollow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

212 citations · 876 across the 28 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

13 papers · 1 filter

astro-ph.HE2020★ 9 cited

Grandma: a network to coordinate them all

S. Agayeva, S. Alishov, S. Antier +75

GRANDMA is an international project that coordinates telescope observations of transient sources with large localization uncertainties. Such sources include gravitational wave even…

astro-ph.HE2017★ 192 cited

The SUrvey for Pulsars and Extragalactic Radio Bursts II: New FRB discoveries and their follow-up

S. Bhandari, E. F. Keane, E. D. Barr +47

We report the discovery of four Fast Radio Bursts (FRBs) in the ongoing SUrvey for Pulsars and Extragalactic Radio Bursts (SUPERB) at the Parkes Radio Telescope: FRBs 150610, 15120…

astro-ph.HE2017★ 212 cited

Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

I. Andreoni, K. Ackley, J. Cooke +122

The discovery of the first electromagnetic counterpart to a gravitational wave signal has generated follow-up observations by over 50 facilities world-wide, ushering in the new era…

astro-ph.HE2016★ 12 cited

The Zadko Telescope: Exploring the transient Universe

D. M. Coward, B. Gendre, P. Tanga +11

The Zadko Telescope is a 1 m f/4 Cassegrain telescope, situated in the state of Western Australia about 80 km north of Perth. The facility plays a niche role in Australian astronom…

astro-ph.HE2015★ 9 cited

Hunting Gravitational Waves with Multi-Messenger Counterparts: Australia's Role

E. J. Howell, A. Rowlinson, D. M. Coward +12

The first observations by a worldwide network of advanced interferometric gravitational wave detectors offer a unique opportunity for the astronomical community. At design sensitiv…

astro-ph.HE2015★ 24 cited

Optical and X-ray early follow-up of ANTARES neutrino alerts

S. Adrian-Martinez, M. Ageron, A. Albert +137

High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. Even with the recent detection of extr…

astro-ph.HE2013★ 28 cited

Fall back accretion and energy injections in gamma-ray bursts

Y. B. Yu, X. F. Wu, Y. F. Huang +4

Intense flares that occur at late times relative to the prompt phase have been observed by the satellite in the X-ray afterglows of gamma-ray bursts (GRBs). Here, we presen…

astro-ph.HE2013★ 18 cited

The Potential for Detecting Gamma-Ray Burst Afterglows from Population III Stars with the Next Generation of Infrared Telescopes

Damien Macpherson, D. M. Coward, M. G. Zadnik

We investigate the detectability of a proposed population of Gamma-Ray Bursts (GRBs) from the collapse of Population III (Pop III) stars. The James Webb Space Telescope (JWST) and…

astro-ph.HE2013★ 34 cited

Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +875

Long gamma-ray bursts (GRBs) have been linked to extreme core-collapse supernovae from massive stars. Gravitational waves (GW) offer a probe of the physics behind long GRBs. We inv…

astro-ph.HE2013★ 1 cited

The diversity of progenitors and emission mechanisms for ultra-long bursts

B. Gendre, G. Stratta, J. L. Atteia +10

GRB 111209A is the longest ever recorded burst. This burst was detected by Swift and Konus-Wind, and we obtained TOO time from XMM-Newton as well as prompt data from TAROT. We made…

astro-ph.HE2013★ 91 cited

The ultra-long GRB 111209A - II. Prompt to afterglow and afterglow properties

G. Stratta, B. Gendre, J. L. Atteia +7

The "ultra-long" Gamma Ray Burst GRB 111209A at redshift z=0.677, is so far the longest GRB ever observed, with rest frame prompt emission duration of ~4 hours. In order to explain…

astro-ph.HE2010★ 1 cited

Using temporal distributions of transient events to characterize cosmological source populations

E. Howell, D. Coward, R. Burman +1

The brightest events in a time series of cosmological transients obey an observation time dependence which is often overlooked. This dependence can be exploited to probe the global…

astro-ph.HE2009★ 6 cited

Are GRB optical afterglows relatively brighter at high z?

A. Imerito, D. M. Coward, R. R. Burman +1

The redshift distribution of gamma-ray bursts (GRBs) is strongly biased by selection effects. We investigate, via Monte Carlo simulations, one possible selection effect that may be…