A dataset provided by the European Space Agency

Name 011088
Title A deep X-ray study of the starforming region IC348 SSC_44
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0110880101

DOI 10.5270/esa-mj99gsf
Author Dr Michael Watson
Description We propose XMM pointings towards the star-forming region IC348. A large number of X-ray sources have already been found by ROSAT in this cluster. The XMM data will be considerably more sensitive, especially for the young objects still embedded in the molecular cloud. XMM will allow us to find the population of pre main sequence stars with a much higher degree of completeness than the previous ROSAT observations. Furthermore, we can investigate the X-ray spectra and the temporal variability of a large number of T Tauri stars. Finally, these observations will allow us to ''X-ray.. the dense cloud cores and to search for X-ray emission from deeply embedded protostars.
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 ,
X-ray emission of brown dwarfs: towards constraining the dependence on age, luminosity, and temperature . Stelzer, B., Micela, G., et all. . A&A . 448-293 . 2006 . 2006A&A...448..293S ,
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 study of the very young stellar cluster IC 348 . Preibisch, T., Zinnecker, H., . A&A . 422-1001 . 2004 . 2004A&A...422.1001P ,
General X-ray properties of hot, massive stars . Naze, Yael, . BSRSL . 80-109 . 2011 . 2011BSRSL..80..109N ,
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 ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-02-02T19:07:47Z/2003-02-03T08:07:00Z
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 2004-03-06T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-03-06T00:00:00Z, 011088, 17.56_20190403_1200. https://doi.org/10.5270/esa-mj99gsf