Marta Burgay

Dr. Marta Burgay

INAF – Osservatorio Astronomico di Cagliari, Via della Scienza 5, I-09047 Selargius (CA), Italy
orcid

Research Focus & Metrics

Academic Career Length

26Years (2001-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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3 October 2023 in Astronomy & Astrophysics
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Journal Article
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JAJ. Antoniadis
J. Antoniadis
SBS. Babak
S. Babak
ANA.-S. Bak Nielsen
A.-S. Bak Nielsen
AAAl. Al.
Al. Al.
ECEPTA Collaboration and InPTA Collaboration:
EPTA Collaboration and InPTA Collaboration:
ZWZ. Wu
Z. Wu
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysics

5 July 2013 in Science
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Journal Article
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DTD. Thornton
D. Thornton
BSB. Stappers
B. Stappers
MBM. Bailes
M. Bailes
BBB. Barsdell
B. Barsdell
SBS. Bates
S. Bates
WSW. van Straten
W. van Straten
Mysterious Radio Bursts: It has been uncertain whether single, short, and bright bursts of radio emission that have been observed are celestial or terrestrial in origin. Thornton et al. (p. 53 ; see the Perspective by Cordes ) report the detection of four nonrepeating radio transient events with millisecond duration in data from the 64-meter Parkes radio telescope in Australia. The properties of these radio bursts indicate that they had their origin outside our galaxy, but it is not possible to tell what caused them. Because the intergalactic medium affects the characteristics of the bursts, it will be possible to use them to study its properties.

6 October 2006 in Science
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MKMichael Kramer
Michael Kramer
ISI. H. Stairs
I. H. Stairs
RMR. N. Manchester
R. N. Manchester
MMM. A. McLaughlin
M. A. McLaughlin
ALA. G. Lyne
A. G. Lyne
FCF. Camilo
F. Camilo
The double pulsar system PSR J0737-3039A/B is unique in that both neutron stars are detectable as radio pulsars. They are also known to have much higher mean orbital velocities and accelerations than those of other binary pulsars. The system is therefore a good candidate for testing Einstein's theory of general relativity and alternative theories of gravity in the strong-field regime. We report on precision timing observations taken over the 2.5 years since its discovery and present four independent strong-field tests of general relativity. These tests use the theory-independent mass ratio of the two stars. By measuring relativistic corrections to the Keplerian description of the orbital motion, we find that the “post-Keplerian” parameter s agrees with the value predicted by general relativity within an uncertainty of 0.05%, the most precise test yet obtained. We also show that the transverse velocity of the system's center of mass is extremely small. Combined with the system's location near the Sun, this result suggests that future tests of gravitational theories with the double pulsar will supersede the best current solar system tests. It also implies that the second-born pulsar may not have formed through the core collapse of a helium star, as is usually assumed.

1 December 2003 in Nature
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MBMarta Burgay
Marta Burgay
NDN. D'Amico
N. D'Amico
APA. Possenti
A. Possenti
RMR. N. Manchester
R. N. Manchester
ALA. G. Lyne
A. G. Lyne
DLD. R. Lorimer
D. R. Lorimer

19 September 2013 in The Astrophysical Journal Supplement Series
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AAA. A. Abdo
A. A. Abdo
MAM. Ajello
M. Ajello
AAA. Allafort
A. Allafort
LBL. Baldini
L. Baldini
JBJ. Ballet
J. Ballet
ZYZ. Yang
Z. Yang

6 April 2010 in Classical and Quantum Gravity
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Journal Article
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GHG Hobbs
G Hobbs
AAA Archibald
A Archibald
ZAZ Arzoumanian
Z Arzoumanian
DBD Backer
D Backer
MBM Bailes
M Bailes
XYX P You
X P You