A dataset provided by the European Space Agency

Name 050386
Title XMM Monitoring of the Evolving AXP 4U 0142+61
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503860101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503860201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503860301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503860401

DOI 10.5270/esa-zfmheju
Author Prof Victoria Kaspi
Description 4U 0142+61 is a 8.7-s "anomalous X-ray pulsar" (AXP) which, in data from our RXTE monitoring program, recently showed pulsations that were slowly but steadily getting brighter (24% increase in 6 yr), in concert with a slow evolution of its soft X-ray pulse profile. Such behavior is unprecedented for an AXP and challenges the current magnetar model. We request XMM observations of the source in Cycle 6 in order to monitor its phase-averaged flux and its spectrum, to try to shed light on the physical origin of this surprising behavior, as well as to better characterize recent and apparently ongoing bursting activity in the source.
Publication Long-term X-ray Changes in the Emission from the Anomalous X-ray Pulsar 4U 0142+61 . Gonzalez, M. E., Dib, R., et all. . ApJ . 716-1345 . 2010 . 2010ApJ...716.1345G ,
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 ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
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 ,
Phase-resolved X-Ray Spectra of Magnetars and the Coronal Outflow Model . Hascoet, Romain, Beloborodov, Andrei M., . ApJ . 786-1 . 2014 . 2014ApJ...786L...1H ,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
The XMM Cluster Survey: Present status and latest results . Viana, P. T...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-01-27T16:45:13Z/2008-03-07T03:49:40Z
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 2009-04-03T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-04-03T00:00:00Z, 050386, 17.56_20190403_1200. https://doi.org/10.5270/esa-zfmheju