A dataset provided by the European Space Agency

Name 010546
Title New ROSAT discovered Intermediate Polars in the Galactic Plane TS_30
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0105460801

DOI 10.5270/esa-vd8c7y9
Author Dr Bernd Aschenbach
Description GT-XMM observations of newly discovered intermediate polars (IPs) are proposed. Broad band pulse phase resolved spectroscopy will allow to investigate the different emission components observed in the X-ray spectra of IPs. The large collecting area and high spectral resolution of the EPIC detectors will provide high quality spectra for a detailed modeling to get insight into the accretion process close to the surface of the white dwarf. RXJ1914.4+2456 is of particular interest. It was proposed as candidate for a soft IP or might be the first double-degenerate polar in which case the 569 s period would indicate the orbital period. We propose a 2nd observation about one year after that of K. Mason to follow the period history.
Publication X-ray and optical observations of 1RXS J154814.5-452845: A new intermediate polar with soft X-ray emission . Haberl, F., Motch, C., . A&A . 387-201 . 2002 . 2002A&A...387..201H ,
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 ,
XMM-Newton and Chandra observations of the ultra-compact binary RX J1914 + 24 . Ramsay, Gavin, Cropper, Mark, . MNRAS . 367-62 . 2006 . 2006MNRAS.367L..62R ,
The X-ray spectrum of RX J1914.4+2456 revisited . Ramsay, Gavin, . MNRAS . 384-687 . 2008 . 2008MNRAS.384..687R ,
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 ,
Identifying XMM-Newton observations affected by solar wind charge exchange. Part I . Carter, J. A., Sembay, S., . A&A . 489-837 . 2008 . 2008A&A...489..837C , ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-09-07T10:02:37Z/2004-10-02T06:21:54Z
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 2005-11-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-11-01T00:00:00Z, 010546, 17.56_20190403_1200. https://doi.org/10.5270/esa-vd8c7y9