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Announcement of the Swift/BAT Hard X-ray Transient Monitor
The Swift/Burst Alert Telescope (BAT) hard X-ray transient monitor provides near real-time coverage of the X-ray sky in the energy range 15-50 keV. The BAT observes 88% of the sky each day with aExpand
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The Three Types of High Mass X-Ray Pulsator
High mass X-ray pulsators are shown to be divisible into three distinct groups on the basis of their observational properties: 1) the Be star systems, 2) non-Be star systems with long pulse periods,Expand
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A Systematic Search for Periodicities in RXTE ASM Data
We present the results of a systematic search in 8.5 years of Rossi X-ray Timing Explorer All-Sky Monitor data for evidence of periodicities. The search was conducted by application of theExpand
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Evidence for a Very Slow X-Ray Pulsar in 2S 0114+650 from Rossi X-Ray Timing Explorer All-Sky Monitor Observations
Rossi X-Ray Timing Explorer (RXTE) all-sky monitor (ASM) observations of the X-ray binary 2S 0114+650 show modulations at periods close to both the optically derived orbital period (11.591 days) andExpand
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AN EXTENDED AND MORE SENSITIVE SEARCH FOR PERIODICITIES IN ROSSI X-RAY TIMING EXPLORER/ALL-SKY MONITOR X-RAY LIGHT CURVES
We present the results of a systematic search in {approx}14 years of Rossi X-ray Timing Explorer All-Sky Monitor (ASM) data for evidence of periodicities. Two variations of the commonly used FourierExpand
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Ginga observations of Centaurus X-3
A series of observations of Centaurus X-3 was made with Ginga on 1989 March 22-24, over a complete orbital cycle. The data set includes a pre-eclipse dip, the eclipse ingress and egress, the eclipseExpand
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LONG-TERM MONITORING OF THE HIGH-ENERGY γ -RAY EMISSION FROM LS I +61 ◦ 303 AND LS 5039
The Fermi Large Area Telescope (LAT) reported the first definitive GeV detections of the binaries LS I +61°303 and LS 5039 in the first year after its launch in 2008 June. These detections wereExpand
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CAL 83: a 1-day period low-mass X-ray binary in the LMC
La campagne d'observation internationale de CAL 83, en 1984, a permis la determination sans aucune ambiguite de la periode de cette binaire RX. Elle est de 1.04 jours avec une modulation sinusoidaleExpand
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A giant radio flare from Cygnus X-3 with associated γ-ray emission
With frequent flaring activity of its relativistic jets, Cygnus X-3 (Cyg X-3) is one of the most active microquasars and is the only Galactic black hole candidate with confirmed high-energy γ-rayExpand
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