| Proposal ID | 041538 |
| Title | OM photometric calibration: observing standard UBV fields |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0415380101 |
| DOI | https://doi.org/10.5270/esa-j7vns2q |
| Principal Investigator, PI | Dr Arvind Parmar XMM-Newton MM |
| Abstract | standard UBV fields:SA 101SA 104SA 110aSA 110b |
| Publications |
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| 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 Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 |
| Keywords | "om photometric calibration", "standard ubv fields" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Arvind Parmar XMM-Newton MM, 2007, 'OM photometric calibration: observing standard UBV fields', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-j7vns2q |