A new determination of theINTEGRAL/IBIS point source location accuracy
(2010)
Journal Article
Scaringi, S., Bird, A., Hill, A., Clark, D., McBride, V., Dean, A., …Stephen, J. (2010). A new determination of theINTEGRAL/IBIS point source location accuracy. Astronomy & Astrophysics, 516, https://doi.org/10.1051/0004-6361/201014209
Dr Simone Scaringi's Outputs (5)
Hard X-ray properties of magnetic cataclysmic variables (2010)
Journal Article
Scaringi, S., Bird, A., Norton, A., Knigge, C., Hill, A., Clark, D., …Landi, R. (2010). Hard X-ray properties of magnetic cataclysmic variables. Monthly Notices of the Royal Astronomical Society, 401(4), https://doi.org/10.1111/j.1365-2966.2009.15826.x
Discovery of the 51.47-d orbital period in the supergiant fast X-ray transient XTE J1739−302 with INTEGRAL (2010)
Journal Article
Drave, S., Clark, D., Bird, A., McBride, V., Hill, A., Sguera, V., …Bazzano, A. (2010). Discovery of the 51.47-d orbital period in the supergiant fast X-ray transient XTE J1739−302 with INTEGRAL. Monthly Notices of the Royal Astronomical Society, 409(3), https://doi.org/10.1111/j.1365-2966.2010.17383.x
Searching for the signature of radiative line driving: on the absence of Lyα-N v line-locking features in a large sample of BALQSOs (2010)
Journal Article
Cottis, C., Goad, M., Knigge, C., & Scaringi, S. (2010). Searching for the signature of radiative line driving: on the absence of Lyα-N v line-locking features in a large sample of BALQSOs. Monthly Notices of the Royal Astronomical Society, 406(3), 2094–2112. https://doi.org/10.1111/j.1365-2966.2010.16839.x
The orbital period in the supergiant fast X-ray transient IGR J16465−4507 (2010)
Journal Article
Clark, D., Sguera, V., Bird, A., McBride, V., Hill, A., Scaringi, S., Drave, S., Bazzano, A., & Dean, A. (2010). The orbital period in the supergiant fast X-ray transient IGR J16465−4507. Monthly Notices of the Royal Astronomical Society: Letters, 406(1), L75–L79. https://doi.org/10.1111/j.1745-3933.2010.00885.xTiming analysis of the INTEGRAL-IBIS and Swift-BAT light curves of the supergiant fast X-ray transient (SFXT) IGR J16465−4507 has identified a period of 30.32 ± 0.02 d which we interpret as the orbital period of the binary system. In addition 11 outb... Read More about The orbital period in the supergiant fast X-ray transient IGR J16465−4507.