A dataset provided by the European Space Agency

Name: OM UV Photometric calibration using BPM16274
Published: 2016-05-16T22:00:00Z

Proposal ID	070158
Title	OM UV Photometric calibration using BPM16274
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701580101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701581101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701581201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701581301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701581601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701581701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701581801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701581901
DOI	https://doi.org/10.5270/esa-sr2lyl7
Principal Investigator, PI	Dr Fred Jansen XMM-Newton MM
Abstract	Routine calibration observation for OM photometry - BPM16274Every 6 months, two different EPIC setup01: MOS1/2: SW+LW diagnostic// pn: ff closed noise (18ks)11: all in FF Diagnostic12: MOS1/2: Diagnostic 1x1, pn Noise (18ks)13: MOS1/2: SW+LW diagnostic// pn: ff closed noise (18ks)15: MOS1/2: Diagnostic 1x1, pn Noise16/18: MOS1/2: Diagnostic 1x1, pn Noise17/19: MOS1/2: SW+LW diagnostic// pn: ff closed noise (18ks)
Publications	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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Complex optical/UV and X-ray variability of the Seyfert 1 galaxy 1H 0419-577 \|Pal, Main, Dewangan, Gulab C., et al. \| MNRAS \| 473-3584 \| 2018 \| 2018MNRAS.473.3584P \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.473.3584P
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-11-10T02:16:11Z/2016-05-11T09:39:46Z
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	2016-05-16T22:00:00Z
Keywords	"epic setup 01", "ff diagnostic", "om photometry bpm16274", "ff closed noise", "pn noise", "diagnostic 1x1", "EPIC", "routine calibration"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton MM, 2016, 'OM UV Photometric calibration using BPM16274', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-sr2lyl7