A dataset provided by the European Space Agency

Name 010686
Title X-Ray Supernovae in Nearby Galaxies
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0106860101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0106860201

DOI 10.5270/esa-a4ebesg
Author Dr Bernd Aschenbach
Description GT- In this proposal we address various questions related to the X-ray emission processes of type II SNe in nearby spiral galaxies at different stages of their evolution. The programmatic search for X-ray emission from young type II SNe in nearby galaxies will lead to a detailed study of the X-ray turn-on phase of SNe and the long-term X-ray lightcurve behavior. The expected high-quality X-ray spectra of young SNe will give us the opportunity to determine with unprecedented accuracy the physical conditions of the ejecta and the ambient ISM in terms of the shock-reverse-shock model.
Publication Elemental Abundances of Nearby Galaxies through High Signal-to-Noise Ratio XMM-Newton Observations of Ultraluminous X-Ray Sources . Winter, Lisa M., Mushotzky, Richard F., . ApJ . 655-163 . 2007 . 2007ApJ...655..163W ,
X-Ray and Optical Variability of the Ultraluminous X-Ray Source NGC 1313 X-2 . Mucciarelli, P., Zampieri, L., et all. . ApJ . 658-999 . 2007 . 2007ApJ...658..999M ,
Spectral variability of ultraluminous X-ray sources . Kajava, Jari J. E., Poutanen, Juri, . MNRAS . 398-1450 . 2009 . 2009MNRAS.398.1450K ,
The scaling of X-ray variability with luminosity in ultra-luminous X-ray sources . Gonzalez-Martin, O., Papadakis, I., et all. . A&A . 526-132 . 2011 . 2011A&A...526A.132G ,
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 ,
An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . Levan, A. J., Tanvir, N. R., et all. . Sci . 333-199 . 2011 . 2011Sci...333..199L ,
The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project . Fassbender, R., Bohringer, H., et all. . NJPh . 13-125014 . 2011 . 2011NJPh...13l5014F ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-10-17T00:59:18Z/2001-12-29T08:51:47Z
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 2003-01-25T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-01-25T00:00:00Z, 010686, 17.56_20190403_1200. https://doi.org/10.5270/esa-a4ebesg