A dataset provided by the European Space Agency

Name 041538
Title OM photometric calibration: observing standard UBV fields
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0415380101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0415380201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0415380301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0415380401

DOI 10.5270/esa-j7vns2q
Author Dr Arvind Parmar XMM-Newton MM
Description standard UBV fields: SA 101 SA 104 SA 110a SA 110b
Publication Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-03-24T13:35:30Z/2007-06-11T21:58:12Z
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 2007-06-12T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-06-12T00:00:00Z, 041538, 17.56_20190403_1200. https://doi.org/10.5270/esa-j7vns2q