A dataset provided by the European Space Agency

Name 011278
Title Search for Cyclotron Line Features in the Spectra of Pulsating X-ray Binaries
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112780101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112780201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112780301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112780401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112780501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112780601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112780801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112781001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112781101

DOI 10.5270/esa-6ak5vbe
Author Dr Martin Turner
Description GT-A sample of X-ray binaries containing neutron stars with a supposed intermediate magnetic field strength (10**10 to 10**12 Gauss) is to be observed. The X-ray spectra will be analysed with the particular aim to search for cyclotron absorption lines in the energy range accessible to XMM. It is to be noted that observation 1 (4U 0115+63) will have to be a target of opportunity (TOO) observation, with a trigger to come from CGRO-BATSE and-or RXTE-ASM.
Publication The anomalous X-ray pulsar 1E 1048.1-5937: Phase resolved spectroscopy with the XMM-Newton satellite . Tiengo, A., Gohler, E., et all. . A&A . 383-182 . 2002 . 2002A&A...383..182T ,
The Likely Near-Infrared Counterpart to the Anomalous X-Ray Pulsar 1E 1048.1-5937 . Wang, Zhongxiang, Chakrabarty, Deepto, . ApJ . 579-33 . 2002 . 2002ApJ...579L..33W ,
Detailed high-energy characteristics of AXP 4U 0142+61. Multi-year observations with INTEGRAL, RXTE, XMM-Newton, and ASCA . den Hartog, P. R., Kuiper, L., et all. . A&A . 489-245 . 2008 . 2008A&A...489..245D ,
Extinction and Distance to Anomalous X-ray Pulsars from X-ray Scattering Halos . Rivera-Ingraham, A., van Kerkwijk, M. H., . ApJ . 710-797 . 2010 . 2010ApJ...710..797R ,
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-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 ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-09-13T18:06:20Z/2003-01-24T23:52:31Z
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 2005-01-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-01-01T00:00:00Z, 011278, 17.56_20190403_1200. https://doi.org/10.5270/esa-6ak5vbe