| Автор | R C Rannot |
| Автор | C L Bhat |
| Автор | V K Senecha |
| Автор | M L Sapru |
| Автор | A K Tickoo |
| Автор | R K Kaul |
| Дата выпуска | 1994-01-01 |
| dc.description | An analysis of 47 hours of data, collected by the Gulmarg gamma-ray telescope during the period 27 September-30 October 1989, indicates the absence of a statistically significant DC signal from the X-ray binary pulsar, 4UO115+63, at photon energies >or=4 TeV. An independent search, carried out for a pulsed signal in the same database, using the well known Rayleigh power test, also does not yield evidence for any episodic, or persistent-pulsed, gamma-ray emission from the source. An upper limit of 2.33*10<sup>-11</sup> photons cm<sup>-2</sup> s<sup>-1</sup> is placed at 99% confidence level on the steady gamma-ray flux from this transient X-ray binary system at photon energies >4 TeV. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | 4UO115+63 revisited - a search for TeV photons during 1989 |
| Тип | paper |
| DOI | 10.1088/0954-3899/20/1/022 |
| Electronic ISSN | 1361-6471 |
| Print ISSN | 0954-3899 |
| Журнал | Journal of Physics G: Nuclear and Particle Physics |
| Том | 20 |
| Первая страница | 223 |
| Последняя страница | 228 |
| Аффилиация | R C Rannot; Nucl. Res. Lab., Bhabha Atomic Res. Centre, Bombay, India |
| Аффилиация | C L Bhat; Nucl. Res. Lab., Bhabha Atomic Res. Centre, Bombay, India |
| Аффилиация | V K Senecha; Nucl. Res. Lab., Bhabha Atomic Res. Centre, Bombay, India |
| Аффилиация | M L Sapru; Nucl. Res. Lab., Bhabha Atomic Res. Centre, Bombay, India |
| Аффилиация | A K Tickoo; Nucl. Res. Lab., Bhabha Atomic Res. Centre, Bombay, India |
| Аффилиация | R K Kaul; Nucl. Res. Lab., Bhabha Atomic Res. Centre, Bombay, India |
| Выпуск | 1 |
