activity
20102019
most citedGROWTH on S190425z: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR

131 citations · 215 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2019★ 131 cited

GROWTH on S190425z: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR

Michael W. Coughlin, Tomás Ahumada, Shreya Anand +76

The third observing run by LVC has brought the discovery of many compact binary coalescences. Following the detection of the first binary neutron star merger in this run (LIGO/Virg…

astro-ph.HE2013★ 29 cited

Discovery of periodic dips in the light curve of GX 13+1: the X-ray orbital ephemeris of the source

R. Iaria, T. Di Salvo, L. Burderi +3

The bright low-mass X-ray binary (LMXB) GX 13+1 is one of the most peculiar Galactic binary systems. A periodicity of 24.27 d with a formal statistical error of 0.03 d was observed…

astro-ph.HE2010

Timing of the accreting millisecond pulsar IGR~J17511--3057

A. Riggio, A. Papitto, L. Burderi +5

{Timing analysis of Accretion-powered Millisecond Pulsars (AMPs) is a powerful tool to probe the physics of compact objects. The recently discovered \newigrj is the 12 discovered o…

astro-ph.HE2010★ 55 cited

New ephemeris of the ADC source 2A 1822-371: a stable orbital-period derivative over 30 years

L. Burderi, T. Di Salvo, A. Riggio +4

We report on a timing of the eclipse arrival times of the low mass X-ray binary and X-ray pulsar 2A 1822-371 performed using all available observations of the Proportional Counter…

astro-ph.HE2010

The X-ray spectrum of the newly discovered accreting millisecond pulsar IGR J17511-3057

A. Papitto, A. Riggio, T. Di Salvo +5

We report on an XMM-Newton observation of the accreting millisecond pulsar, IGR J17511-3057. Pulsations at 244.8339512(1) Hz are observed with an RMS pulsed fraction of 14.4(3)%. A…