A dataset provided by the European Space Agency

Name 060585
Title Prompt study of magnetar outbursts with XMM-Newton
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605851901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605852001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605852101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605852201

DOI 10.5270/esa-kz83evc
Author Dr Sandro Mereghetti
Description Magnetars (AXPs and SGRs) go through long stretches of quiescence, interrupted by periods of activity, characterized by bursts and significant variability in flux, spectral shape, pulse shape, and pulsed fraction; they also exhibit glitches. Observations performed during, or immediately after such periods of high activity yield the largest amount of information, allowing to test the theoretical models on a variety of phenomena and source states. We propose a rapid ToO program aimed at gathering new physical insight on these sources, through the study of the very initial phases (within 10 days) of the outbursts of known or newly discovered magnetars.
Publication A Low-Magnetic-Field Soft Gamma Repeater . Rea, N., Esposito, P., et all. . Sci . 330-944 . 2010 . 2010Sci...330..944R ,
Long-term spectral and timing properties of the soft gamma-ray repeater SGR 1833-0832 and detection of extended X-ray emission around the radio pulsar PSR B1830-08 . Esposito, P., Israel, G. L., et all. . MNRAS . 416-205 . 2011 . 2011MNRAS.416..205E ,
Search for the Optical Counterpart to SGR 0418+5729 . Durant, Martin, Kargaltsev, Oleg, . ApJ . 742-77 . 2011 . 2011ApJ...742...77D ,
The Outburst Decay of the Low Magnetic Field Magnetar SGR 0418+5729 . Rea, N., Israel, G. L., et all. . ApJ . 770-65 . 2013 . 2013ApJ...770...65R ,
Chasing the Identification of ASCA Galactic Objects (ChIcAGO): An X-Ray Survey of Unidentified Sources in the Galactic Plane. I. Source Sample and Initial Results . Anderson, Gemma E., Gaensler, B. M., et all. . ApJS . 212-13 . 2014 . 2014ApJS..212...13A ,
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 ,
Suzaku observations of two diffuse hard X-ray source regions, G22.0+0.0 and G23.5+0.1 . Yamauchi, Shigeo, Sumita, Mayu, . PASJ . 68-6 . 2016 . 2016PASJ...68S...6Y ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . ...,
Pulsar-Wind Nebulae and Magnetar Outflows: Observations at Radio, X-Ray, and Gamma-Ray Wavelengths . Reynolds, Stephen P., Pavlov, George G., et all. . SSRv . 207-175 . 2017 . 2017SSRv..207..175R ,
Systematic study of magnetar outbursts . Coti Zelati, Francesco, Rea, Nanda, et all. . MNRAS . 474-961 . 2018 . 2018MNRAS.474..961C ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-03-23T12:37:25Z/2010-09-24T11:24:44Z
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 2011-10-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-10-01T00:00:00Z, 060585, 17.56_20190403_1200. https://doi.org/10.5270/esa-kz83evc