A dataset provided by the European Space Agency

Name: Point Spread Function Comparison with AXAF-PKS0312-770
Published: 2001-10-06T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	012252
Title	Point Spread Function Comparison with AXAF-PKS0312-770
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122520201
DOI	https://doi.org/10.5270/esa-byse8em
Principal Investigator, PI	Dr Fred Jansen XMM-Newton PS
Abstract	CAL- The PSF of the EPIC MOS is checked against the AXAF PSF calibration targetPKS0312-770, which has a source flux sufficiently low to avoid pile-up. A modestexposure allows the core of the PSF in MOS to be well-studied and provides areference against the PSF obtained with brighter sources, and with the higherresolution CHANDRA cameras. In the current plan only one off-axis pointing isscheduled because PSF cores at various field angles is covered eitherserendipitously or via other CAL observations.
Publications	An XMM-Newton view of the serendipitous sources in the PKS0312-770 field \|Lumb D. H. Guainazzi M. \| A&A \| 376-387 \| 2001 \| 2001A&A...376..387L \| http://ui.adsabs.harvard.edu/#abs/2001A&A...376..387L The HELLAS2XMM survey. III. Multiwavelength observations of hard X-ray selected sources in the PKS 0312-77 field \|Brusa M. Comastri A. et al. \| A&A \| 409-65 \| 2003 \| 2003A&A...409...65B \| http://ui.adsabs.harvard.edu/#abs/2003A&A...409...65B An XMM-Newton study of the hard X-ray sky \|Piconcelli E. Cappi M. et al. \| A&A \| 412-689 \| 2003 \| 2003A&A...412..689P \| http://ui.adsabs.harvard.edu/#abs/2003A&A...412..689P Exploring the X-ray sky with the XMM-Newton bright serendipitous survey \|Della Ceca R. Maccacaro T. et al. \| A&A \| 428-383 \| 2004 \| 2004A&A...428..383D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...428..383D High-precision multi-band measurements of the angular clustering of X-ray sources \|Ebrero J. Mateos S. et al. \| A&A \| 500-749 \| 2009 \| 2009A&A...500..749E \| http://ui.adsabs.harvard.edu/#abs/2009A&A...500..749E 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 Normal galaxies in the XMM-Newton fields. X-rays as a star formation indicator \|Rovilos E. Georgantopoulos I. et al. \| A&A \| 502-85 \| 2009 \| 2009A&A...502...85R \| http://ui.adsabs.harvard.edu/#abs/2009A&A...502...85R The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project \|Fassbender R. Bohringer H. et al. \| NJPh \| 13-125014 \| 2011 \| 2011NJPh...13l5014F \| http://ui.adsabs.harvard.edu/#abs/2011NJPh...13l5014F 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 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 The HELLAS2XMM survey. XI. Unveiling the nature of X-ray bright optically normal galaxies \|Civano F. Mignoli M. et al. \| A&A \| 476-1223 \| 2007 \| 2007A&A...476.1223C \| http://ui.adsabs.harvard.edu/#abs/2007A&A...476.1223C Exploring the spectral properties of faint hard X-ray sources with XMM-Newton \|Piconcelli E. Cappi M. et al. \| A&A \| 394-835 \| 2002 \| 2002A&A...394..835P \| http://ui.adsabs.harvard.edu/#abs/2002A&A...394..835P The HELLAS2XMM survey. IV. Optical identifications and the evolution of the accretion luminosity in the Universe \|Fiore F. Brusa M. et al. \| A&A \| 409-79 \| 2003 \| 2003A&A...409...79F \| http://ui.adsabs.harvard.edu/#abs/2003A&A...409...79F The XMM-Newton HBS28 sample: Studying the obscuration in hard X-ray selected AGNs \|Caccianiga A. Severgnini P. et al. \| A&A \| 416-901 \| 2004 \| 2004A&A...416..901C \| http://ui.adsabs.harvard.edu/#abs/2004A&A...416..901C The HELLAS2XMM survey. V. Near-Infrared observations of X-ray sources with extreme X/O ratios \|Mignoli M. Pozzetti L. et al. \| A&A \| 418-827 \| 2004 \| 2004A&A...418..827M \| http://ui.adsabs.harvard.edu/#abs/2004A&A...418..827M The HELLAS2XMM survey. VI. X-ray absorption in the 1df AGN sample through a spectral analysis \|Perola G. C. Puccetti S. et al. \| A&A \| 421-491 \| 2004 \| 2004A&A...421..491P \| http://ui.adsabs.harvard.edu/#abs/2004A&A...421..491P XMM-Newton data processing for faint diffuse emission. Proton flares exposure maps and report on EPIC MOS1 bright CCDs contamination \|Pradas J. 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Mignoli M. et al. \| ApJ \| 571-771 \| 2002 \| 2002ApJ...571..771C \| http://ui.adsabs.harvard.edu/#abs/2002ApJ...571..771C The Resolved Fraction of the Cosmic X-Ray Background \|Moretti A. Campana S. et al. \| ApJ \| 588-696 \| 2003 \| 2003ApJ...588..696M \| http://ui.adsabs.harvard.edu/#abs/2003ApJ...588..696M The XMM-Newton serendipitous survey. VI. The X-ray luminosity function \|Ebrero J. Carrera F. J. et al. \| A&A \| 493-55 \| 2009 \| 2009A&A...493...55E \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493...55E An XMM-Newton study of hard X-ray sources \|Piconcelli E. Bassani L. et al. \| AN \| 324-161 \| 2003 \| 2003AN....324..161P \| http://ui.adsabs.harvard.edu/#abs/2003AN....324..161P Breaking the sigma8-Omega m Degeneracy Using the Clustering of High-z X-ray Active Galactic Nuclei \|Basilakos Spyros Plionis Manolis \| ApJ \| 714-185 \| 2010 \| 2010ApJ...714L.185B \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...714L.185B The X-ray spectral properties of the AGN population in the XMM-Newton bright serendipitous survey \|Corral A. Della Ceca R. et al. \| A&A \| 530-42 \| 2011 \| 2011A&A...530A..42C \| http://ui.adsabs.harvard.edu/#abs/2011A&A...530A..42C 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 Fe Kalpha line profile in AGNs: average shape and redshift dependence \|Mao Wei-Ming Hu Chen et al. \| RAA \| 10-905 \| 2010 \| 2010RAA....10..905M \| http://ui.adsabs.harvard.edu/#abs/2010RAA....10..905M 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 The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc N. Sadibekova T. et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H Properties of the integrated spectrum of serendipitous 2XMM catalog sources \|Chaudhary P. Brusa M. et al. \| A&A \| 518-58 \| 2010 \| 2010A&A...518A..58C \| http://ui.adsabs.harvard.edu/#abs/2010A&A...518A..58C Rest-frame stacking of 2XMM catalog sources. Properties of the Fe Kalpha line \|Chaudhary P. 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Brusa M. et al. \| AN \| 324-28 \| 2003 \| 2003AN....324...28C \| http://ui.adsabs.harvard.edu/#abs/2003AN....324...28C Studying Cosmic Evolution with the XMM-Newton Distant Cluster Project: X-ray Luminous Galaxy Clusters at z>~1 and their Galaxy Populations \|Fassbender Rene \| PhDT \| 0-116 \| 2008 \| 2008PhDT.......116F \| http://ui.adsabs.harvard.edu/#abs/2008PhDT.......116F The close environments of accreting massive black holes are shaped by radiative feedback \|Ricci Claudio Trakhtenbrot Benny et al. \| Natur \| 549-488 \| 2017 \| 2017Natur.549..488R \| http://ui.adsabs.harvard.edu/#abs/2017Natur.549..488R BAT AGN Spectroscopic Survey (BASS) - VI. The GammaX-L/LEdd relation \|Trakhtenbrot Benny Ricci Claudio et al. \| MNRAS \| 470-800 \| 2017 \| 2017MNRAS.470..800T \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470..800T BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog \|Ricci C. 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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 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage	2000-03-31T10:56:11Z/2000-03-31T23:41:31Z
Version	21.51_20241115_1113
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	2001-10-06T00:00:00Z
Last Update	2026-07-09
Keywords	"modest exposure allows", "resolution chandra cameras", "psf cores", "brighter sources", "EPIC", "spread function comparison", "source flux", "epic mos", "field angles", "avoid pile", "axaf p0312 770"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton PS, 2001, 'Point Spread Function Comparison with AXAF-PKS0312-770', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-byse8em
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.