170 citations · 316 across the 8 of their papers we have counts for
8 papers
Femtosecond X-ray Laser induced transient electronic phase change observed in fullerene C60
Brian Abbey, Ruben A. Dilanian, Connie Darmanin +17
X-ray Free-Electron Lasers (XFELs) deliver X-ray pulses with a coherent flux that is approximately eight orders of magnitude greater than that available from a modern third generat…
Coherence Properties of Individual Femtosecond Pulses of an X-ray Free-Electron Laser
I. A. Vartanyants, A. Singer, A. P. Mancuso +33
Measurements of the spatial and temporal coherence of single, femtosecond x-ray pulses generated by the first hard x-ray free-electron laser (FEL), the Linac Coherent Light Source…
4U2206+54 - an Unusual High Mass X-ray Binary with a 9.6 Day Orbital Period but No Strong Pulsations
Robin H. D. Corbet, Andrew G. Peele
Rossi X-ray Timing Explorer All-Sky Monitor observations of the X-ray source 4U2206+54, previously proposed to be a Be star system, show the X-ray flux to be modulated with a perio…
The Orbital Period of the Be/Neutron Star Binary RX J0812.4-3114
Robin H. D. Corbet, Andrew G. Peele
We present the results of Rossi X-ray Timing Explorer observations of the Be star X-ray binary system RX J0812.4-3114. A light curve obtained with the RXTE All-Sky Monitor shows th…
RXTE Observations of the X-ray Pulsar XTE J1855-026 - a Possible New Supergiant System
R. H. D. Corbet, F. E. Marshall, A. G. Peele +1
A new X-ray source, XTE J1855-026, was discovered during RXTE scans along the galactic plane. The source shows pulsations at a period of 361 s and also modulation at a period of 6.…
Evidence for a very slow X-ray pulsar in 2S0114+650 from RXTE All-Sky Monitor Observations
Robin H. D. Corbet, John P. Finley, Andrew G. Peele
Rossi X-ray Timing Explorer (RXTE) All-Sky Monitor (ASM) observations of the X-ray binary 2S0114+650 show modulations at periods close to both the optically derived orbital period…
RXTE Observations of the Be star X-ray Transient X0726-260 (4U0728-25) - Orbital and Pulse Periods
Robin H. D. Corbet, Andrew G. Peele
Rossi X-ray Timing Explorer (RXTE) All Sky Monitor observations of the transient Be star X-ray source X0726-260 suggest a 34.5 day period. This is apparently confirmed by a serendi…
A Broad Band and Large Area X-Ray Omni Sky Monitor (BLOSM)
W. Zhang, R. Petre, A. N. Peele +4
We present a conceptual design for a new X-ray all sky monitor (ASM). Compared with previous ASMs, its salient features are: (1) it has a focusing capability that increases the sig…