activity
20012018
most citedThe Large Observatory for X-ray Timing (LOFT)

214 citations · 492 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2018★ 72 cited

Observatory science with eXTP

Jean J. M. in 't Zand, Enrico Bozzo, Jinlu Qu +181

In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring s…

astro-ph.IM2011★ 214 cited

The Large Observatory for X-ray Timing (LOFT)

M. Feroci, the LOFT Consortium

High-time-resolution X-ray observations of compact objects provide direct access to strong-field gravity, to the equation of state of ultra-dense matter and to black hole masses an…

astro-ph2007★ 22 cited

Non-Detection of Gravitationally Redshifted Absorption Lines in the X-ray Burst Spectra of GS 1826-24

Albert K. H. Kong, Jon M. Miller, Mariano Mendez +6

During a 200 ks observation with the XMM-Newton Reflection Grating Spectrometer, we detected 16 type-I X-ray bursts from GS 1826-24. We combined the burst spectra in an attempt to…

astro-ph2007★ 20 cited

Investigating the nature of absorption lines in the Chandra X-ray spectra of the neutron star binary 4U 1820-30

E. M. Cackett, J. M. Miller, J. Raymond +5

We use four Chandra gratings spectra of the neutron star low-mass X-ray binary 4U 1820-30 to better understand the nature of certain X-ray absorption lines in X-ray binaries, inclu…

astro-ph2006★ 35 cited

Intensity-hardness correlation and deep infrared observation of the anomalous X-ray pulsar 1RXS J170849-400910

N. Rea, G. L. Israel, T. Oosterbroek +6

We report here on X-ray and IR observations of the Anomalous X-ray Pulsar 1RXS J170849-400910. First, we report on new XMM-Newton, Swift-XRT and Chandra observations of this AXP, w…

astro-ph2006★ 60 cited

High-frequency Quasi-Periodic Oscillations from GRS 1915+105 in its C state

T. Belloni, P. Soleri, P. Casella +2

We report the results of a systematic timing analysis of RXTE observations of GRS 1915+105 when the source was in its variability class theta, characterized by alternating soft and…