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D. Coward

28 papers hereh-index 492 citations10 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author2
  • first author2
  • middle author15

Across the 19 of 28 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE13
  • astro-ph.IM7
  • astro-ph.EP4
  • astro-ph3
  • gr-qc1
same name
  • D. Coward — 107 papers, h 82
  • D. Coward — 97 papers, h 45
  • D. Coward — 41 papers, h 44
  • D. Coward — 23 papers
  • D. Coward — 1 paper
  • D. Coward — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

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-phShow all

3 papers · 1 filter

astro-ph2008★ 8 cited

GRB optical afterglow and redshift selection effects: The learning curve effect at work

D. M. Coward

We show how the observed gamma ray burst (GRB) optical afterglow (OA) and redshift distributions are changing in time from selection effects. For a subset of {\it Swift} triggered…

astro-ph2008★ 1 cited

Observation time to first detection of double neutron star mergers by gravitational wave observatories

D. M. Coward

We constrain the uncertainty in waiting times for detecting the first double-neutron-star (DNS) mergers by gravitational wave observatories. By accounting for the Poisson fluctuati…

astro-ph2007★ 7 cited

An improved method for estimating source densities using the temporal distribution of Cosmological Transients

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

It has been shown that the observed temporal distribution of transient events in the cosmos can be used to constrain their rate density. Here we show that the peak flux--observatio…

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