activity
19962023
most citedINTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817

916 citations · 7.9k across the 163 of their papers we have counts for

collaborators
Showing 2003Show all

12 papers · 1 filter

astro-ph2003★ 47 cited

Detection of hard X-ray emission from the Galactic nuclear region with INTEGRAL

G. Belanger, A. Goldwurm, P. Goldoni +13

This letter presents the first results of an observational campaign to study the Galactic Centre with INTEGRAL. The mosaicked images obtained with the IBIS/ISGRI coded aperture ins…

astro-ph2003★ 64 cited

The observers' view of (very) long X-ray bursts: they are super!

Erik Kuulkers

In many X-ray point sources on the sky, the X-ray emission arises because hydrogen and/or helium is accreted onto a neutron star from a nearby donor star. When this matter settles…

astro-ph2003★ 70 cited

A superburst from 4U 1254-690

J. J. M. in 't Zand, E. Kuulkers, F. Verbunt +2

We report the detection with the BeppoSAX Wide Field Cameras of a superburst from 4U 1254-690. The superburst is preceded by a normal type-I X-ray burst, has a decay time that is t…

astro-ph2003★ 125 cited

Periodic Thermonuclear X-ray Bursts from GS 1826-24 and the Fuel Composition as a Function of Accretion Rate

D. K. Galloway, A. Cumming, E. Kuulkers +3

We analyze 24 type I X-ray bursts from GS 1826-24 observed by the Rossi X-ray Timing Explorer between 1997 November and 2002 July. The bursts observed between 1997-98 were consiste…

astro-ph2003★ 11 cited

The INTEGRAL ground segment and its science operations centre

R. Much, P. Barr, L. Hansson +10

The INTEGRAL ground segment is divided into operational and scientific components. The operational component consists of the Mission Operations Centre, the ground stations and comm…

astro-ph2003★ 7 cited

First INTEGRAL Observations of Eight Persistent Neutron Star Low Mass X-ray Binaries

A. Paizis, V. Beckmann, T. J. -L. Courvoisier +16

Early results from the INTEGRAL Core Program, for a sample of eight persistently bright neutron star low mass X-ray binaries in the energy range from 5 keV to 200 keV are presented…