Periodicity search for possible X-ray counterparts to radio-quiet gamma-ray pulsar candidates
Abstract
A periodicity search of 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. However, it may still be difficult to find the period directly from X-ray data because of limited exposure. We have developed a procedure, by cross-checking two X-ray data sets, to find candidate periods for X-ray sources that are possible counterparts to gamma-ray pulsar candidates. Here, we report on the results of this method obtained with all the currently available X-ray data of eight X-ray sources. Some attractive periodicity features were found. These candidate periods can serve as the target periods for a future search when new data become available, so that a blind search with a huge number of trials can be avoided.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- June 2008
- DOI:
- 10.1111/j.1365-2966.2008.13256.x
- Bibcode:
- 2008MNRAS.387..729L
- Keywords:
-
- stars: neutron;
- pulsars: general;
- gamma-rays: observations;
- X-rays: general