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

28 papers

astro-ph.EP2026★ 1 cited

High-Speed Observations of Lunar Impact Flashes

Dale P. Giancono, Hadrien A. R. Devillepoix, Robert M. Howie +7

Lunar impact flashes provide a direct means of estimating the flux of centimetre-sized meteoroids impacting the lunar surface. However, 25-60 frames per second imaging typical of m…

astro-ph.IM2024

The impact of the site quality of the Zadko Observatory on its scientific results

Bruce Gendre, Richard Tonello, Mitchell Studdert +5

We present the site quality of the Zadko Observatory, focusing on the brightness of the sky and the effects of the weather on the efficiency of the Observatory. We discuss these ef…

astro-ph.IM2024

Management of a Multi-User Robotic Observatory

John Moore, Bruce Gendre, David Coward +2

The Zadko Observatory located approximately 70 kilometres north of Perth in the Yeal nature reserve within the Shire of Gingin, Western Australia, initially housed the 1.0 metre f/…

astro-ph.IM2020

The Zadko Observatory

J. A. Moore, B. Gendre, D. M. Coward +2

The 1.0 metre f/4 fast-slew Zadko Telescope was installed in June 2008 approximately seventy kilometres north of Perth at Yeal, in the Shire of Gingin, Western Australia. Since the…

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.IM2020

The Zadko telescope results: ten years of science

B. Gendre, D. Coward, J. Moore +5

The 1.0 meter f/4 fast-slew Zadko telescope is located in Western Australia, approximately seventy kilometers north of Perth at Yeal in the Shire of Gingin in a dedicated "low-lumi…

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.IM2014

HEIDI: An Automated Process for the Identification and Extraction of Photometric Light Curves from Astronomical Images

M. Todd, H. U. Wallon Pizarro, P. Tanga +2

The production of photometric light curves from astronomical images is a very time-consuming task. Larger data sets improve the resolution of the light curve, however, the time req…

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.EP2013★ 5 cited

Predictions for the Detection of Earth and Mars Trojan Asteroids by the Gaia satellite

M. Todd, P. Tanga, D. M. Coward +1

The European Space Agency Gaia satellite, planned for launch in late 2013, will perform systematic astrometric observations of the whole sky over a five year period. During this mi…

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…

gr-qc2013★ 160 cited

Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network

the LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +801

Compact binary systems with neutron stars or black holes are one of the most promising sources for ground-based gravitational wave detectors. Gravitational radiation encodes rich i…

astro-ph.IM2012★ 1 cited

Australian participation in the Gaia Follow-Up Network for Solar System Objects

M. Todd, D. M. Coward, P. Tanga +1

The Gaia satellite, planned for launch by the European Space Agency (ESA) in 2013, is the next generation astrometry mission following Hipparcos. Gaia's primary science goal is to…

astro-ph.EP2012★ 13 cited

An optimal Mars Trojan asteroid search strategy

M. Todd, P. Tanga, D. M. Coward +1

Trojan asteroids are minor planets that share the orbit of a planet about the Sun and librate around the L4 or L5 Lagrangian points of stability. Although only three Mars Trojans h…

astro-ph.EP2011★ 13 cited

An optimal Earth Trojan asteroid search strategy

M. Todd, P. Tanga, D. M. Coward +1

Trojan asteroids are minor planets that share the orbit of a planet about the Sun and librate around the L4 or L5 Lagrangian points of stability. They are important solar-system fo…

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.IM2010★ 30 cited

The Zadko Telescope: A Southern Hemisphere Telescope for Optical Transient Searches, Multi-Messenger Astronomy and Education

D. M. Coward, M. Todd, T. P. Vaalsta +17

The new 1-m f/4 fast-slew Zadko Telescope was installed in June 2008 about 70 km north of Perth, Western Australia. It is the only metre-class optical facility at this southern lat…