Periodicity Search of Possible X-ray Counterparts to Radio-quiet Gamma-ray Pulsar Candidates

dc.creatorLin, Lupin Chun-Che
dc.creatorChang, Hsiang-Kuang
dc.date2008-05-01
dc.date.accessioned2026-07-07T09:36:23Z
dc.date.available2026-07-07T09:36:23Z
dc.descriptionPeriodicity search in gamma-ray data is usually difficult because of the small number of detected photons. A periodicity in the timing signal at other energy bands from the counterpart to the gamma-ray source may help to establish the periodicity in the gamma-ray emission and strengthen the identification of the source in different energy bands. It may, however, still be difficult to find the period directly from X-ray data because of limited exposure. We developed a procedure, by cross-checking two X-ray data sets, to find candidate periods for X-ray sources which are possible counterparts to gamma-ray pulsar candidates. Here we report the results of this method obtained with all the currently available X-ray data of 8 X-ray sources. Some tempting periodicity features were found. Those candidate periods can serve as the target periods for future search when new data become available so that a blind search with a huge number of trials can be avoided.
dc.description7 pages, 6 figures and 2 tables
dc.identifierhttps://arxiv.org/abs/0805.0072
dc.identifierhttp://arxiv.org/abs/0805.0072
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/160104
dc.subjectAstrophysics
dc.titlePeriodicity Search of Possible X-ray Counterparts to Radio-quiet Gamma-ray Pulsar Candidates
dc.typetext

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