A dataset provided by the European Space Agency

Name: EPIC Effective area vs. Energy openPar3C58closePar
Published: 2000-03-09T00:00:00Z

Proposal ID	010258
Title	EPIC Effective area vs. Energy (3C58)
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102580601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102580801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0102581001
DOI	https://doi.org/10.5270/esa-q822aqh
Principal Investigator, PI	Dr Fred Jansen XMM-Newton PS
Abstract	CAL- we will observe the Crab-like SNR 3C58 to measure the spectrum to revealdepartures from a simple power-law fit that may be caused by groundcalibration inaccuracies. This object is not subject to pile-up effects so that we can be sure that spectral residuals will be more likely due to calibrationerrors in the response matrices. In addition, offset pointings are made tomeasure the energy dependent vignetting (in y direction to ensure we miss abright star on the planned dates). Epic overheads of 4 ksec per exposure havebeen assumed.
Publications	The X-ray nebula of the filled center supernova remnant 3C 58 and its interaction with the environment \|Bocchino, F., Warwick, R. S., et al. \| A&A \| 369-1078 \| 2001 \| 2001A&A...369.1078B \| http://ui.adsabs.harvard.edu/#abs/2001A&A...369.1078B The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca, A., Molendi, S., \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D 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 The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F The Spectrum of the Universe \|Hill, Ryley, Masui, Kiyoshi W., \| ApSpe \| 72-663 \| 2018 \| 2018ApSpe..72..663H \| http://ui.adsabs.harvard.edu/#abs/2018ApSpe..72..663H Spectral energy distribution modeling of broadband emission in the pulsar wind nebula 3C 58 \|Kim, Seungjong, An, Hongjun, \| AN \| 341-170 \| 2020 \| 2020AN....341..170K \| http://ui.adsabs.harvard.edu/#abs/2020AN....341..170K Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z 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 Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2000-03-11T09:55:52Z/2000-03-12T17:07:56Z
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	2000-03-09T00:00:00Z
Keywords	"epic effective", "energy 3c58", "epic overheads", "spectral residuals", "supernova remnant 3c58", "planned dates", "calibration errors", "bright star", "ground calibration inaccuracies", "energy dependent vignetting", "offset pointings", "EPIC", "response matrices"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton PS, 2000, 'EPIC Effective area vs. Energy openPar3C58closePar', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-q822aqh