activity
19942025
most citedThe Nuclear Spectroscopic Telescope Array (NuSTAR) Mission

2.3k citations · 10.7k across the 219 of their papers we have counts for

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Showing 1997Show all

6 papers · 1 filter

astro-ph1997★ 1 cited

Balloon-Borne Hard X-Ray Imaging and Future Surveys

Jonathan E. Grindlay

Several payloads for hard X-ray (20-600 keV) imaging with coded aperture telescopes have been developed for balloon flight observations of cosmic x-ray sources. We briefly review t…

astro-ph1997★ 2 cited

Simulations and Measurements of the Background Encountered by a High-Altitude Balloon-Borne Experiment for Hard X-ray Astronomy

Kenneth S. K. Lum, Joseph J. Mohr, Didier Barret +2

We have modelled the hard X-ray background expected for a high-altitude balloon flight of the Energetic X-ray Telescope Experiment (EXITE2), an imaging phoswich detector/telescope…

astro-ph1997

Kilo-hertz QPO and X-ray Bursts in 4U 1608-52 in Low Intensity State

W. Yu, S. N. Zhang, B . A. Harmon +8

We present the results from RXTE/PCA observations of 4U 1608-52 in its island state on March 15, 18 and 22 of 1996. Three type I X-ray bursts were detected in one RXTE orbit on Mar…

astro-ph1997

Kilo-hertz QPO in Island State of 4U1608-52 as Observed with RXTE/PCA

W. Yu, S. N. Zhang, B . A. Harmon +8

We report RXTE/PCA observations of 4U 1608-52 on March 15, 18 and 22 immediately after the outburst in early 1996. The persistent count rates ranged from 190 to 450 cps (1-60 keV).…

astro-ph1997★ 55 cited

Energy Spectra and High Frequency Oscillations in 4U 0614+091

Eric C. Ford, Philip Kaaret, Kaiyou Chen +7

We investigate the behavior of the high frequency quasi-periodic oscillations (QPOs) in 4U 0614+091, combining timing and spectral analysis of RXTE observations. The energy spectra…

astro-ph1997★ 428 cited

Advection-Dominated Accretion Model of Sagittarius A*: Evidence for a Black Hole at the Galactic Center

Ramesh Narayan, Rohan Mahadevan, Jonathan E. Grindlay +2

Sgr A* at the Galactic Center is a puzzling source. It has a mass M=(2.5+/-0.4) x 10^6 solar masses which makes it an excellent black hole candidate. Observations of stellar winds…