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2XMM J010247.4-720449 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST04:19:50 |
Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
---|---|---|---|---|---|---|---|---|---|
2013PASJ...65L...2W | 78 | T | 1 | 4 | 2 |
Detection of a 522 s Pulsation from the Transient X-Ray Source Suzaku J0102.8-7204 ( SXP 523) in the Small Magellanic Cloud. |
WADA Q., TSUJIMOTO M., EBISAWA K., et al. | ||
2013A&A...558A...3S | 16 | D | 2 | 3092 | 73 | The XMM-Newton survey of the Small Magellanic Cloud: the X-ray point-source catalogue. | STURM R., HABERL F., PIETSCH W., et al. | ||
2011ATel.3761....1S | 115 | T | X | 2 | 2 | 2 |
2XMM J010247.4-720449 is a Be/X-ray binary, detected in outburst with Swift. |
STURM R., HABERL F., PIETSCH W., et al. | |
2012ATel.4628....1W | 77 | T | 1 | 3 | 3 |
Discovery of a new X-ray transient pulsar Suzaku J0102-7204 in the SMC. |
WADA Q., TSUJIMOTO M. and EBISAWA K. | ||
2012ATel.4648....1H | 155 | T | X | 3 | 3 | 2 |
SXP 523 = Suzaku J0102-7204 = 2XMM J010247.4-720449, a Be/X-ray binary pulsar in the SMC. |
HABERL F., STURM R., TSUJIMOTO M., et al. | |
2013ATel.4719....1S | 273 | T | X | 6 | 3 | 2 | Confirmation of the spin period and coordinates of SXP 523 with XMM-Newton. | STURM R., HABERL F., FREYBERG M., et al. | |
2015MNRAS.452..969C | 16 | D | 3 | 69 | 33 | Catalogue of Be/X-ray binary systems in the Small Magellanic Cloud: X-ray, optical and IR properties. | COE M.J. and KIRK J. | ||
2016A&A...586A..81H | 96 | D | C | 3 | 180 | 112 | High-mass X-ray binaries in the Small Magellanic Cloud. | HABERL F. and STURM R. | |
2017ApJ...839..119Y | 16 | D | 2 | 66 | 27 | A comprehensive library of X-ray pulsars in the Small Magellanic Cloud: time evolution of their luminosities and spin periods. | YANG J., LAYCOCK S.G.T., CHRISTODOULOU D.M., et al. | ||
2022A&A...661A..25H | 690 | D | S X C | 14 | 52 | 10 | eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds. | HABERL F., MAITRA C., CARPANO S., et al. |