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Production of Millisecond Dips in Sco X-1 Count Rates by Dead Time Effects

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© 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation T. A. Jones et al 2008 ApJ 677 1241 DOI 10.1086/533581

0004-637X/677/2/1241

Abstract

Chang and coworkers reported millisecond duration dips in the X-ray intensity of Sco X-1 and attributed them to occultations of the source by small trans-Neptunian objects (TNOs). We have found multiple lines of evidence that these dips are not astronomical in origin, but rather the result of high-energy charged particle events in the RXTE PCA detectors. Our analysis of the RXTE data indicates that at most 10% of the observed dips in Sco X-1 could be due to occultations by TNOs, and, furthermore, we find no positive or supporting evidence for any of them being due to TNOs. We therefore believe that it is a mistake to conclude that any TNOs have been detected via occultation of Sco X-1.

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10.1086/533581