|Title||XMM-Newton observation of the new SGR 0501+4516 in its return to in quiescence|
|Author||Dr Nanda Rea|
|Description||We ask for a 50ks XMM-Newton observation of the newly discovered Soft Gamma Repeater SGR 0501+4516, aimed at a deep study of the source in its return to quiescence state. The transient X-ray behaviour of SGR0501+4516 was caught from the beginning of the outburst by our AO7 XMM-Newton ToO monitoring program, allowing us to study in unprecedented detail the timing and spectral evolution of the outburst decay of a SGR. We now request a further pointing in order to complete the study of the evolution of the source to characterize its quiescent state, and single out permanent spectral-timing changes induced by the outburst.|
|Publication||Unifying the observational diversity of isolated neutron stars via magneto-thermal evolution models . Vigano, D., Rea, N., et all. . MNRAS . 434-123 . 2013 . 2013MNRAS.434..123V ,
Quiescent state and outburst evolution of SGR 0501+4516 . Camero, A., Papitto, A., et all. . MNRAS . 438-3291 . 2014 . 2014MNRAS.438.3291C ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
The Short Bursts in SGR-1806 20, 1E 1048-5937, and SGR 0501+4516 . Qu, Zhijie, Li, Zhaosheng, et all. . PASP . 127-211 . 2015 . 2015PASP..127..211Q ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Magnetic fields in neutron stars . Vigano, Daniele, . PhDT . 0-7 . 2013 . 2013PhDT.........7V ,
Systematic study of magnetar outbursts . Coti Zelati, Francesco, Rea, Nanda, et all. . MNRAS . 474-961 . 2018 . 2018MNRAS.474..961C ,
X-Ray Observations of Magnetar SGR 0501+4516 from Outburst to Quiescence . Mong, Y.-L., Ng, C.-Y., . ApJ . 852-86 . 2018 . 2018ApJ...852...86M ,
|Instrument||EMOS1, EMOS2, EPN, OM, RGS1, RGS2|
|Mission Description||The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2010-09-12T00:00:00Z, 060422, 17.56_20190403_1200. https://doi.org/10.5270/esa-s7spyp8|