A dataset provided by the European Space Agency

Name 050649
Title Probing a new super-giant fast X-ray transient
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506490101

DOI 10.5270/esa-ytawa49
Author Mr Jean-Christophe Leyder
Description The newly discovered Super-giant Fast X-ray Transients (SFXT) IGR J08408-4503 is an interesting member of this class that is expected to rapidly grow. Indeed, it is one of the few sources for which the optical association with an O-type super-giant (HD 74194) has been confirmed, making it a perfect target for a detailed X-ray investigation. This source has been recently detected in the X-ray domain by two Swift ToO observations, but these observations were too short to allow more than a better determination of the position. Therefore, we request one observation of IGR J08408-4503 with XMM-Newton, in order to perform an in-depth analysis of the spectral properties and of the X-ray variability study of our target.
Publication The supergiant fast X-ray transients XTE J1739-302 and IGR J08408-4503 in quiescence with XMM-Newton . Bozzo, E., Stella, L., et all. . A&A . 519-6 . 2010 . 2010A&A...519A...6B ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The longest observation of a low-intensity state from a supergiant fast X-ray transient: Suzaku observes IGRJ08408-4503 . Sidoli, L., Esposito, P., . MNRAS . 409-611 . 2010 . 2010MNRAS.409..611S ,
Investigating the Structure of Vela X . Slane, P., Lovchinsky, I., et all. . ApJ . 865-86 . 2018 . 2018ApJ...865...86S ,
Supergiant Fast X-ray Transients uncovered by the EXTraS project: flares reveal the development of magnetospheric instability in accreting neutron stars . Sidoli, Lara, Postnov, Konstantin A., et all. . MNRAS . 487-420 . 2019 . 2019MNRAS.487..420S ,
Accretion disc by Roche lobe overflow in the supergiant fast X-ray transient IGR J08408-4503 . Ducci, L., Romano, P., et all. . A&A . 631-135 . 2019 . 2019A&A...631A.135D ,
Instrument EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage 2007-05-29T09:21:24Z/2007-05-29T22:03:32Z
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 2008-06-22T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-06-22T00:00:00Z, 050649, 17.56_20190403_1200. https://doi.org/10.5270/esa-ytawa49