A dataset provided by the European Space Agency

Name 050214
Title SGR 1627-41: a transient Soft Gamma-ray Repeater


DOI 10.5270/esa-sxsqhwz
Author Dr Sandro Mereghetti
Description Soft Gamma-ray Repeaters were the first class of X-ray sources believed to host magnetars, i.e. isolated neutron stars with surface magnetic fields of 10^14-10^15 G. SGR 1627-41 is the only known SGR with a transient X-ray counterpart. After a single bursting episode, its persistent X-ray luminosity monotonically decreased from 1998 to 2004 with an overall variation of a factor greater than 20, the largest ever observed in a SGR. We propose to observe again SGR 1627-41 with XMM-Newton EPIC to establish whether the flux has reached a stable level and to obtain the best quality spectrum for a SGR in an unique low luminosity state.
Publication The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
X-ray spectra from magnetar candidates - III. Fitting SGR-AXP soft X-ray emission with non-relativistic Monte Carlo models . Zane, S., Rea, N., et all. . MNRAS . 398-1403 . 2009 . 2009MNRAS.398.1403Z ,
Two magnetars: SGR 1627-41 and 1E 1547-5408 . Mereghetti, S., Tiengo, A., et all. . AdSpR . 47-1312 . 2011 . 2011AdSpR..47.1312M ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The 2008 May burst activation of SGR1627-41 . Esposito, P., Israel, G. L., et all. . MNRAS . 390-34 . 2008 . 2008MNRAS.390L..34E ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 201...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-02-12T15:41:12Z/2008-02-13T19:09:44Z
Version 17.56_20190403_1200
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.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2009-03-12T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-03-12T00:00:00Z, 050214, 17.56_20190403_1200. https://doi.org/10.5270/esa-sxsqhwz