A dataset provided by the European Space Agency

Name 014198
Title Deep XMM-Newton survey of M33


DOI 10.5270/esa-9o2jpyq
Author Dr Wolfgang Pietsch
Description In a GT raster observation of the bright local group spiral galaxy M33 we study the population of X-ray sources (SNRs, XRBs, supershells) down to a 0.1-2.4 keV luminosity limit of 10E35erg-s - a factor of 10 deeper than earlier ROSAT observations. EPIC spectra and hardness ratios are used to separate between different source classes. We search for short term time variability, pulsations of the order of 1 to few 100 s and long term variability, i.e. binary light curves, transients. We spectrally characterize the diffuse component that is correlated with the inner spiral arms. Here, we re-propose observations that were dominated by high EPIC background or used EPIC with the thick filter.
Publication The eclipsing massive X-ray binary M 33 X-7: New X-ray observations and optical identification . Pietsch, W., Mochejska, B. J., et all. . A&A . 413-879 . 2004 . 2004A&A...413..879P ,
Identifying XMM-Newton observations affected by solar wind charge exchange - Part II . Carter, J. A., Sembay, S., . A&A . 527-115 . 2011 . 2011A&A...527A.115C ,
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 ,
Soft X-ray emission from the inner disc of M33 . Owen, R. A., Warwick, R. S., . MNRAS . 403-558 . 2010 . 2010MNRAS.403..558O ,
XMM-Newton survey of the Local Group galaxy M 33 . Pietsch, W., Misanovic, Z., et all. . A&A . 426-11 . 2004 . 2004A&A...426...11P ,
An XMM-Newton survey of the Local Group galaxy M 33 - variability of the detected sources . Misanovic, Z., Pietsch, W., et all. . A&A . 448-1247 . 2006 . 2006A&A...448.1247M , ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-01-22T19:14:47Z/2003-07-25T12:44:34Z
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 2004-09-03T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-09-03T00:00:00Z, 014198, 17.56_20190403_1200. https://doi.org/10.5270/esa-9o2jpyq