A dataset provided by the European Space Agency

Name: EPIC Effective Area vs. Energy openParG21.5-09closePar
Published: 2003-08-08T00:00:00Z

Proposal ID	012270
Title	EPIC Effective Area vs. Energy (G21.5-09)
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122700801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122701001
DOI	https://doi.org/10.5270/esa-8f9d9e9
Principal Investigator, PI	Dr Fred Jansen XMM-Newton PS
Abstract	CAL- Supplementing the 3C58 calibration, we use the SNR G21.5-09 which has a slightly steeper slope, but similar count rate. Offsets in theZ-direction are used to complement the 3C58 vignetting data, while avoidingbright stars.
Publications	Timing analysis of the core of the Crab-like SNR G21.5-0.9 \|La Palombara, N., Mereghetti, S., \| A&A \| 383-916 \| 2002 \| 2002A&A...383..916L \| http://ui.adsabs.harvard.edu/#abs/2002A&A...383..916L The nature of the X-ray halo of the plerion G21.5-0.9 unveiled by XMM-Newton and Chandra \|Bocchino, F., van der Swaluw, E., et al. \| A&A \| 442-539 \| 2005 \| 2005A&A...442..539B \| http://ui.adsabs.harvard.edu/#abs/2005A&A...442..539B Cross-calibration of the X-ray instruments onboard the Chandra, INTEGRAL, RXTE, Suzaku, Swift, and XMM-Newton observatories using G21.5-0.9 \|Tsujimoto, M., Guainazzi, M., et al. \| A&A \| 525-25 \| 2011 \| 2011A&A...525A..25T \| http://ui.adsabs.harvard.edu/#abs/2011A&A...525A..25T The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M The missing link: a low-mass X-ray binary in M31 seen as an ultraluminous X-ray source \|Middleton, Matthew J., Sutton, Andrew D., et al. \| MNRAS \| 420-2969 \| 2012 \| 2012MNRAS.420.2969M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.420.2969M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M A Multiwavelength Study on the High-energy Behavior of the Fermi/LAT Pulsars \|Marelli, Martino, De Luca, Andrea, \| ApJ \| 733-82 \| 2011 \| 2011ApJ...733...82M \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...733...82M The extended X-ray halo of the Crab-like SNR G21.5-0.9 \|Warwick, R. S., Bernard, J.-P., et al. \| A&A \| 365-248 \| 2001 \| 2001A&A...365L.248W \| http://ui.adsabs.harvard.edu/#abs/2001A&A...365L.248W The XMM-Newton Serendipitous Survey. I. The role of XMM-Newton Survey Science Centre \|Watson, M. G., Augueres, J.-L., et al. \| A&A \| 365-51 \| 2001 \| 2001A&A...365L..51W \| http://ui.adsabs.harvard.edu/#abs/2001A&A...365L..51W Discovery of an absorbed cluster of galaxies (XMMU J183225.4-103645) close to the Galactic plane with XMM-Newton \|Nevalainen, J., Lumb, D., et al. \| A&A \| 374-66 \| 2001 \| 2001A&A...374...66N \| http://ui.adsabs.harvard.edu/#abs/2001A&A...374...66N A new search strategy for microquasar candidates using NVSS/2MASS and XMM-Newton data \|Combi, J. A., Albacete-Colombo, J. F., \| A&A \| 477-125 \| 2008 \| 2008A&A...477..125C \| http://ui.adsabs.harvard.edu/#abs/2008A&A...477..125C A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations \|Muno, M. P., Gaensler, B. M., et al. \| ApJ \| 680-639 \| 2008 \| 2008ApJ...680..639M \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...680..639M The source content of low galactic latitude XMM-Newton surveys \|Motch, C., Herent, O., \| AN \| 324-61 \| 2003 \| 2003AN....324...61M \| http://ui.adsabs.harvard.edu/#abs/2003AN....324...61M The X-ray halo of G21.5 - 0.9 \|Bandiera, R., Bocchino, F., \| AdSpR \| 33-398 \| 2004 \| 2004AdSpR..33..398B \| http://ui.adsabs.harvard.edu/#abs/2004AdSpR..33..398B In-Orbit Vignetting Calibrations of XMM-Newton Telescopes \|Lumb, D. H., Finoguenov, A., et al. \| ExA \| 15-89 \| 2003 \| 2003ExA....15...89L \| http://ui.adsabs.harvard.edu/#abs/2003ExA....15...89L The Galactic plane at faint X-ray fluxes - I. Properties and characteristics of the X-ray source population \|Warwick, R. S., Perez-Ramirez, D., \| MNRAS \| 413-595 \| 2011 \| 2011MNRAS.413..595W \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.413..595W An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog \|Georgakakis, A. E., Chavushyan, V., et al. \| MNRAS \| 367-1017 \| 2006 \| 2006MNRAS.367.1017G \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367.1017G The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L Hot stars observed by XMM-Newton. I. The catalog and the properties of OB stars \|Naze, Y., \| A&A \| 506-1055 \| 2009 \| 2009A&A...506.1055N \| http://ui.adsabs.harvard.edu/#abs/2009A&A...506.1055N A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi, J. A., Albacete Colombo, J. F., et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C The XMM-Newton serendipitous source catalogue \|Watson, M. G., Pye, J. P., et al. \| AN \| 324-89 \| 2003 \| 2003AN....324...89W \| http://ui.adsabs.harvard.edu/#abs/2003AN....324...89W 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 The XMM-Newton SSC survey of the Galactic plane \|Nebot Gomez-Moran, A., Motch, C., et al. \| A&A \| 553-12 \| 2013 \| 2013A&A...553A..12N \| http://ui.adsabs.harvard.edu/#abs/2013A&A...553A..12N The effect of advection at luminosities close to Eddington: The ULX in M 31 \|Straub, O., Done, C., \| A&A \| 553-61 \| 2013 \| 2013A&A...553A..61S \| http://ui.adsabs.harvard.edu/#abs/2013A&A...553A..61S The Second Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars \|Abdo, A. A., Ajello, M., et al. \| ApJS \| 208-17 \| 2013 \| 2013ApJS..208...17A \| http://ui.adsabs.harvard.edu/#abs/2013ApJS..208...17A Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S An XMM-Newton view of FeKalpha in high-mass X-ray binaries \|Gimenez-Garcia, A., Torrejon, J. M., et al. \| A&A \| 576-108 \| 2015 \| 2015A&A...576A.108G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...576A.108G In orbit calibrations of XMM-Newton telescopes \|Lumb, David H., Finoguenov, A., et al. \| SPIE \| 4851-255 \| 2003 \| 2003SPIE.4851..255L \| http://ui.adsabs.harvard.edu/#abs/2003SPIE.4851..255L Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X Detection of thermal X-ray emission in the halo of the plerionic supernova remnant G21.5-0.9 \|Bocchino, F., \| AdSpR \| 35-1003 \| 2005 \| 2005AdSpR..35.1003B \| http://ui.adsabs.harvard.edu/#abs/2005AdSpR..35.1003B 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 Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz, Tobias, \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P X-ray lags in PDS 456 revealed by Suzaku observations \|Chiang, Chia-Ying, Cackett, E. M., et al. \| MNRAS \| 472-1473 \| 2017 \| 2017MNRAS.472.1473C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.472.1473C Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V 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 Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P 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 SRG/ART-XC Galactic Plane Survey near Galactic Longitude L 20\\u00b0: Catalog of Sources \|Karasev, D. I., Semena, A. N., et al. \| AstL \| 49-662 \| 2023 \| 2023AstL...49..662K \| http://ui.adsabs.harvard.edu/#abs/2023AstL...49..662K 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	2000-04-07T12:36:39Z/2001-04-09T22:25:05Z
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	2003-08-08T00:00:00Z
Keywords	"z direction", "epic effective", "energy g21", "3c58 vignetting data", "G21.5", "supernova remnant g21", "3c58 calibration", "bright stars", "EPIC", "count rate"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton PS, 2003, 'EPIC Effective Area vs. Energy openParG21.5-09closePar', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8f9d9e9