A dataset provided by the European Space Agency

Name: OM Routine Calibration Observations
Published: 2007-06-20T00:00:00Z

Proposal ID	021228
Title	OM Routine Calibration Observations
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212282001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212282201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212282301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212282401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212282501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212282601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212282701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212282801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212283001
DOI	https://doi.org/10.5270/esa-56sjpr3
Principal Investigator, PI	Dr Fred Jansen XMM-Newton PS
Abstract	RCOs 2005:GD 153 OM throughputHD 13499 OM UV grism wavelength Hz 2 OM optical grism wavelengthHD 5980 OM photometry
Publications	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 X-ray spectra from magnetar candidates - III. Fitting SGR/AXP soft X-ray emission with non-relativistic Monte Carlo models \|Zane, S., Rea, N., et al. \| MNRAS \| 398-1403 \| 2009 \| 2009MNRAS.398.1403Z \| http://ui.adsabs.harvard.edu/#abs/2009MNRAS.398.1403Z XMM-Newton Observations of CXOU J010043.1-721134: The First Deep Look at the Soft X-Ray Emission of a Magnetar \|Tiengo, A., Esposito, P., \| ApJ \| 680-133 \| 2008 \| 2008ApJ...680L.133T \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...680L.133T IKT 16: a composite supernova remnant in the Small Magellanic Cloud \|Owen, R. A., Filipovic, M. D., et al. \| A&A \| 530-132 \| 2011 \| 2011A&A...530A.132O \| http://ui.adsabs.harvard.edu/#abs/2011A&A...530A.132O Optical and UV monitor (OM) on-board XMM-Newton \|Talavera, Antonio, \| Ap&SS \| 320-177 \| 2009 \| 2009Ap&SS.320..177T \| http://ui.adsabs.harvard.edu/#abs/2009Ap&SS.320..177T 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 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 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 The XMM-Newton survey of the Small Magellanic Cloud \|Haberl, F., Sturm, R., et al. \| A&A \| 545-128 \| 2012 \| 2012A&A...545A.128H \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A.128H The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page, M. J., Brindle, C., et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P 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 10 Years of the optical & UV monitor (OM) on-board XMM-Newton \|Talavera, Antonio, \| Ap&SS \| 335-291 \| 2011 \| 2011Ap&SS.335..291T \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.335..291T The XMM-Newton survey of the Small Magellanic Cloud: The X-ray point-source catalogue \|Sturm, R., Haberl, F., et al. \| A&A \| 558-3 \| 2013 \| 2013A&A...558A...3S \| http://ui.adsabs.harvard.edu/#abs/2013A&A...558A...3S Active galactic nuclei behind the SMC selected from radio and X-ray surveys \|Sturm, R., Draskovic, D., et al. \| A&A \| 558-101 \| 2013 \| 2013A&A...558A.101S \| http://ui.adsabs.harvard.edu/#abs/2013A&A...558A.101S 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 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 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 XMM-Newton publication statistics \|Ness, J.-U., Parmar, A. N., et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti, F., Middei, R., et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V Tracing the Lowest Propeller Line in Magellanic High-mass X-Ray Binaries \|Christodoulou, Dimitris M., Laycock, Silas G. T., et al. \| ApJ \| 829-30 \| 2016 \| 2016ApJ...829...30C \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829...30C SXP 7.92: a recently rediscovered Be/X-ray binary in the Small Magellanic Cloud, viewed edge on \|Bartlett, E. S., Coe, M. J., et al. \| MNRAS \| 466-4659 \| 2017 \| 2017MNRAS.466.4659B \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.466.4659B 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 al. \| ApJ \| 839-119 \| 2017 \| 2017ApJ...839..119Y \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...839..119Y Retrograde accretion discs in high-mass Be/X-ray binaries \|Christodoulou, D. M., Laycock, S. G. T., \| MNRAS \| 470-21 \| 2017 \| 2017MNRAS.470L..21C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470L..21C A Changing Wind Collision \|Naze, Yael, Koenigsberger, Gloria, et al. \| ApJ \| 853-164 \| 2018 \| 2018ApJ...853..164N \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...853..164N 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 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 The supernova remnant population of the Small Magellanic Cloud \|Maggi, Pierre, Filipovi\\u0107, Miroslav D., et al. \| A&A \| 631-127 \| 2019 \| 2019A&A...631A.127M \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P New optically identified supernova remnants in the Large Magellanic Cloud \|Yew, Miranda, Filipovi\\u0107, Miroslav D., et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y 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 Long-term XMM-Newton view of magnetar CXOU J010043.1-721134: comprehensive spectral and temporal results \|Chatterjee, Rwitika, Agrawal, Vivek K., \| MNRAS \| 505-3785 \| 2021 \| 2021MNRAS.505.3785C \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.505.3785C Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud \|Matsuura, Mikako, Ayley, Victoria, et al. \| MNRAS \| 513-1154 \| 2022 \| 2022MNRAS.513.1154M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.1154M The MeerKAT 1.3 GHz Survey of the Small Magellanic Cloud \|Cotton, W. D., Filipovi\\u0107, M. D., et al. \| MNRAS \| 529-2443 \| 2024 \| 2024MNRAS.529.2443C \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.529.2443C 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	2005-01-07T05:33:15Z/2006-02-16T20:40:44Z
Version	PPS_NOT_AVAILABLE
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	2007-06-20T00:00:00Z
Keywords	"om routine calibration", "rcos 2005"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton PS, 2007, 'OM Routine Calibration Observations', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-56sjpr3