Observations of Gamma-ray Bursts with the Rossi X-ray Timing Explorer

Kavli Affiliate: Edmund Bertschinger | Summary:The role of the Rossi X-ray Timing Explorer (RXTE) in the study of Gamma-ray Bursts (GRBs) is reviewed. Through April 2001, the All-Sky Monitor (ASM) and the Proportional Counter Array (PCA) instruments have detected 30 GRBs. In 16 cases, an early celestial position was released to the community, sometimes in […]


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Highlights of RXTE Studies of Compact Objects after ~5 Years

Kavli Affiliate: Edmund Bertschinger | Summary:Observations with the Rossi X-ray Timing Explorer (RXTE) have led to fundamental progress in the study of compact objects, in particular neutron stars and black holes. In this paper we present briefly some highlights from ~5 years of RXTE operations. | Search Query: arXiv Query: search_query=au:”Bradt Hale”&id_list=&start=0&max_results=10Read More


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An All-sky Advanced X-ray Monitor (AXM) Mission

Kavli Affiliate: Edmund Bertschinger | Summary:A concept for an all-sky monitor mission substantially more powerful than the RXTE ASM is presented in brief. It makes use of 31 Gas Electron Multiplier (GEM) proportional counters to provide continuous monitoring of the entire x-ray sky, except for earth occultations and a small region around the sun. This […]


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X-ray Transients Monitored by the All-Sky Monitor on RXTE: A Tabulation

Kavli Affiliate: Edmund Bertschinger | Summary:We present a tabulation of 46 transient x-ray sources monitored with the All-Sky Monitor (ASM) on the Rossi X-ray Timing Explorer (RXTE). They fall into four broad categories: short (~d), intermediate, and long (>500 d) duration of outbursts, and long period binary systems that flare up at periastron (e.g., Be […]


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Transient X–Ray Sources Observed with the Rxte All-Sky Monitor after 3.5 Years

Kavli Affiliate: Edmund Bertschinger | Summary:We present light curves of a sample of "transient" sources observed with the All-Sky Monitor (ASM) of the Rossi X-ray Timing Explorer (RXTE). The light curves extend over 3.5 years. They are presented in three groups: six neutron-star systems, eight black-hole-candidate systems, and an additional diverse set of six objects […]


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