A dataset provided by the European Space Agency

Name: 3C273: XMM-Newton routine cross-calibration
Published: 2024-01-16T00:00:00Z

Proposal ID	081082
Title	3C273: XMM-Newton routine cross-calibration
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810820101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810821501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810821601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810821701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810821801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810821901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810822001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810822101
DOI	https://doi.org/10.5270/esa-k3hrikv
Principal Investigator, PI	Dr Peter Kretschmar XMM-Newton MM
Abstract	Routine Cal. (copied from 13655)NRCO-114 on 1ES 0229+200
Publications	X-ray intraday variability and power spectral density profiles of the blazar 3C 273 with XMM-Newton during 2000-2021 \|Pavana Gowtami, G. S., Gaur, Haritma, et al. \| MNRAS \| 511-3101 \| 2022 \| 2022MNRAS.511.3101P \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.511.3101P Study of Intra-Day Flux Distributions of Blazars Using XMM-Newton Satellite \|Wani, Kiran, Gaur, Haritma, \| Univ \| 8-578 \| 2022 \| 2022Univ....8..578W \| http://ui.adsabs.harvard.edu/#abs/2022Univ....8..578W Constraining X-Ray Variability of the Blazar 3C 273 Using XMM-Newton Observations over Two Decades \|Dinesh, Adithiya, Bhatta, Gopal, et al. \| ApJ \| 955-121 \| 2023 \| 2023ApJ...955..121D \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...955..121D The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2019-07-02T17:16:32Z/2024-01-08T10:13:20Z
Version	21.23_20231215_1101
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	2024-01-16T00:00:00Z
Keywords	"13655 nrco 114", "routine cal", "XMM", "1es 0229", "XMM-Newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Peter Kretschmar XMM-Newton MM, 2024, '3C273: XMM-Newton routine cross-calibration', 21.23_20231215_1101, European Space Agency, https://doi.org/10.5270/esa-k3hrikv