A dataset provided by the European Space Agency

Name 041298
Title EPIC Gain, contamination and CTI monitoring-1ES0102
URL

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DOI 10.5270/esa-fxne1uz
Author Dr Fred Jansen XMM-Newton MM
Description EPIC ROUTINE CAL - The AXAF standard candle source, 1ES0102-72 in the SMC region will be observed periodically. The strong emission lines at low energies will be measured to determine the CCD gain and CTI at the boresight location. In addition, apparent secular changes in various emission line strengths may be used to track contamination build-up. (was proposal 13572)
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Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
A new super-soft X-ray source in the Small Magellanic Cloud: Discovery of the first Be-white dwarf system in the SMC? . Sturm, R., Haberl, F., et all. . A&A . 537-76 . 2012 . 2012A&A...537A..76S ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
XMM-Newton observations of the Small Magellanic Cloud: RX J0105.9-7203, a 726 s Be-X-ray binary pulsar . Eger, P., Haberl, F., . A&A . 485-807 . 2008 . 2008A&A...485..807E ,
XMM-Newton observations of the Small Magellanic Cloud: Long term evolution of frequently observed Be-X-ray binaries . Eger, P., Haberl, F., . A&A . 491-841 . 2008 . 2008A&A...491..841E ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . ...,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
The XMM-Newton survey of the Small Magellanic Cloud . Haberl, F., Sturm, R., et all. . A&A . 545-128 . 2012 . 2012A&A...545A.128H ,
Supernova remnants: the X-ray perspective . Vink, Jacco, . A&ARv . 20-49 . 2012 . 2012A&ARv..20...49V ,
A systematic cross-search for radio-infrared counterparts of XMM- Newton sources . Combi, J. A., Albacete Colombo, J. F., et all. . Ap&SS . 331-53 . 2011 . 2011Ap&SS.331...53C ,
The XMM-Newton survey of the Small Magellanic Cloud: The X-ray point-source catalogue . Sturm, R., Haberl, F., et all. . A&A . 558-3 . 2013 . 2013A&A...558A...3S ,
Active galactic nuclei behind the SMC selected from radio and X-ray surveys . Sturm, R., Draskovic, D., et all. . A&A . 558-101 . 2013 . 2013A&A...558A.101S ,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 2014 . 2014ApJ...786...20L ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
Revealing the broad iron Kalpha line in Cygnus X-1 through simultaneous XMM-Newton, RXTE, and INTEGRAL observations . Duro, Refiz, Dauser, Thomas, et all. . A&A . 589-14 . 2016 . 2016A&A...589A..14D ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
SNR 1E 0102.2-7219 as an X-ray calibration standard in the 0.5-1.0 keV bandpass and its application to the CCD instruments aboard Chandra, Suzaku, Swift and XMM-Newton . Plucinsky, Paul P., Beardmore, Andrew P., et all. . A&A . 597-35 . 2016 . 2016A&A...597A..35P ,
SNR 1E 0102.2-7219 as an X-ray calibration standard in the 0.5-1.0 keV bandpass and its application to the CCD instruments aboard Chandra, Suzaku, Swift and XMM-Newton . Plucinsky, Paul P., Beardmore, Andrew P., et all. . A&A . 597-35 . 2017 . 2017A&A...597A..35P ,
Discovery of a 26.2 day period in the long-term X-ray light curve of SXP 1323: a very short orbital period for a long spin period pulsar . Carpano, S., Haberl, F., . A&A . 602-81 . 2017 . 2017A&A...602A..81C ,
A Comprehensive Library of X-Ray Pulsars in the Small Magellanic Cloud: Time Evolution of Their Luminosities and Spin Periods . Yang, J., Laycock, S. G. T., et all. . ApJ . 839-119 . 2017 . 2017ApJ...839..119Y ,
Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
The XMM Cluster Survey: Present status and latest results . Viana, P. T. P., Mehrtens, N., et all. . AN . 334-462 . 2013 . 2013AN....334..462V ,
Identification of AGN in the XMM-Newton X-ray survey of the SMC . Maitra, Chandreyee, Haberl, Frank, et all. . A&A . 622-29 . 2019 . 2019A&A...622A..29M ,
Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 2019ApJS..244...22H ,
Anticorrelation between X-ray luminosity and pulsed fraction in the Small Magellanic Cloud pulsar SXP 1323 . Yang, Jun, Zezas, Andreas, et all. . MNRAS . 479-1 . 2018 . 2018MNRAS.479L...1Y ,
The supernova remnant population of the Small Magellanic Cloud . Maggi, Pierre, Filipoviu0107, Miroslav D., et all. . A&A . 631-127 . 2019 . 2019A&A...631A.127M ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
New optically identified supernova remnants in the Large Magellanic Cloud . Yew, Miranda, Filipoviu0107, Miroslav D., et all. . MNRAS . 500-2336 . 2021 . 2021MNRAS.500.2336Y ,
Instrument EPN, RGS1, OM, RGS2, EMOS1, EMOS2
Temporal Coverage 2006-11-05T00:54:41Z/2017-11-05T00:35:34Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2017-11-09T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2017-11-09T23:00:00Z, 041298, 17.56_20190403_1200. https://doi.org/10.5270/esa-fxne1uz