A dataset provided by the European Space Agency

Name 014687
Title XMM-Newton monitoring of the binary x-ray pulsar SAX J0635+0533
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0146870101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0146870201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0146870301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0146870401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0146870501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0146870901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0146871001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0146871101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0146871201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0146871301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0146871501
...

DOI 10.5270/esa-cv4q2p7
Author Dr giancarlo cusumano
Description Modulations detected in the observed spin period of the 34~ms x-ray pulsar SAX J0635+0533 confirm that the pulsar is in a binary system with a massive star and place a lower bound on the intrinsic period derivative of the pulsar of 4x10^-13 ss^-1. The high spin-down rate would require a very high accretion rate if produced by accretion and suggests, instead, that the pulsar is rotation powered with a characteristic age of less than 1400 yr. We propose a set of XMM-Newton observations to accurately measure the position of the source, to search for extended emission from the system, and to accurately measure the orbital parameters of the system. The latter is mandatory to fold gamma-ray data to identify SAX J0635 + 0533 as x-ray counterpart of 2EG~J0635 + 0521.
Publication The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
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 ,
A low luminosity state in the massive X-ray binary SAX J0635+0533 . Mereghetti, S., La Palombara, N., . A&A . 504-181 . 2009 . 2009A&A...504..181M ,
A new search strategy for microquasar candidates using NVSS-2MASS and XMM-Newton data . Combi, J. A., Albacete-Colombo, J. F., . A&A . 477-125 . 2008 . 2008A&A...477..125C ,
A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations . Muno, M. P., Gaensler, B. M., et all. . ApJ . 680-639 . 2008 . 2008ApJ...680..639M ,
An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 . Henley, David B., Shelton, Robin L., . ApJS . 187-388 . 2010 . 2010ApJS..187..388H ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . ...,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
A systematic cross-search for radio-infrared counterparts of XMM- Newton sources . Combi, J. A., Albacete Colombo, J. F., et all. . Ap&SS . 331-53 . 2011 . 2011Ap&SS.331...53C ,
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 ,
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 ,
Revealing the broad iron Kalpha line in Cygnus X-1 through simultaneous XMM-Newton, RXTE, and INTEGRAL observations . Duro, Refiz, Dauser, Thomas, et all. . A&A . 589-14 . 2016 . 2016A&A...589A..14D ,
The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . 2016ApJ...829....9M ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals . Sibeck, David G., Allen, R., et all. . SSRv . 214-79 . 2018 . 2018SSRv..214...79S ,
The XMM Cluster Survey: Present status and latest results . Viana, P. T. P., Mehrtens, N., et all. . AN . 334-462 . 2013 . 2013AN....334..462V ,
Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 2019ApJS..244...22H ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-09-11T13:40:12Z/2004-04-14T10:18:01Z
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 2005-05-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-05-15T00:00:00Z, 014687, 17.56_20190403_1200. https://doi.org/10.5270/esa-cv4q2p7