A dataset provided by the European Space Agency

Name 012234
Title GX13+1: RGS effective area calibrations
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122340101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122340201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122340401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122340501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122340601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122340701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122340901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0122341001

DOI 10.5270/esa-m98q74x
Author Dr Fred Jansen XMM-Newton PS
Description CAL-RGS effective area calibrations
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XMM-Newton observations of GX 13 + 1: correlation between photoionised absorption and broad line emission . Diaz Trigo, M., Sidoli, L., et all. . A&A . 543-50 . 2012 . ...,
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The XMM-Newton serendipitous source catalogue . Watson, M. G., Pye, J. P., et all. . AN . 324-89 . 2003 . 2003AN....324...89W ,
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The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Testing rate-dependent corrections on timing mode EPIC-pn spectra of the accreting neutron star GX 13+1 . Pintore, F., Sanna, A., et all. . MNRAS . 445-3745 . 2014 . 2014MNRAS.445.3745P ,
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 ,
Interstellar Dust Properties from a Survey of X-Ray Halos . Valencic, Lynne A., Smith, Randall K., . ApJ . 809-66 . 2015 . 2015ApJ...809...66V ,
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A Study of Low-mass X-Ray Binaries in the Low-luminosity Regime . Sonbas, E., Dhuga, K. S., . ApJ . 853-150 . 2018 . 2018ApJ...853..150S ,
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 ,
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 ,
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 ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-03-30T14:11:34Z/2000-04-11T10:49:07Z
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 2002-01-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-01-09T00:00:00Z, 012234, 17.56_20190403_1200. https://doi.org/10.5270/esa-m98q74x