A dataset provided by the European Space Agency

Name 055208
Title Optical Monitor Observations of Extended UV Disks
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552080101

DOI 10.5270/esa-0eiytvt
Author Dr K.D. Kuntz
Description One of the early results from the Galaxy Evolution Explorer (GALEX) Nearby Galaxies Survey (NGS) is the discovery of conspicuous UV emission extending significantly beyond the optical disks of some spiral galaxies, into regions where the gas density was believed to be too low to support star formation. We propose to use the high angular resolution and large FOV of the XMM Optical Monitor to resolve the star-forming regions responsible for this UV emission in a small sample of extended UV disk galaxies. The simultaneous X-ray observations may provide valuable constraints on the mass function of the star clusters and provide valuable insight into star-forming processes at such low surface densities.
Publication An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The Birth of an Ultraluminous X-Ray Source in M83 . Soria, Roberto, Kuntz, K. D., et all. . ApJ . 750-152 . 2012 . 2012ApJ...750..152S ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
X-ray source population study of the starburst galaxy M 83 with XMM-Newton . Ducci, L., Sasaki, M., et all. . A&A . 553-7 . 2013 . 2013A&A...553A...7D ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-08-16T07:50:34Z/2008-08-16T16:07:28Z
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 2009-09-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-09-27T00:00:00Z, 055208, 17.56_20190403_1200. https://doi.org/10.5270/esa-0eiytvt