A dataset provided by the European Space Agency

Name: Probing the Environments of Young Supernovae with XMM-Newton
Published: 2008-06-23T00:00:00Z

Proposal ID	030186
Title	Probing the Environments of Young Supernovae with XMM-Newton
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301860101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301860301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301860401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301860501
DOI	https://doi.org/10.5270/esa-erky4nj
Principal Investigator, PI	Dr Stefan Immler
Abstract	By observing the X-ray emission properties of young supernovae (SNe), physicalkey parameters such as the circumstellar matter (CSM) density, the mass-lossrate of the progenitor, and the temperature of the outgoing and reverse shockcan be studied as a function of time. We propose follow-up observations of thebrightest known X-ray emitting SNe (1978K, 1979C, 2004dj) to study thetemperature evolution, establish the physical parameters of the ambient CSM outto radii of E18cm from the sites of the explosions, and to monitor the mass-lossrates over 10^4 years in the progenitors stellar wind history. Studying thesekey parameters as a function of time has never been done before.
Publications	Spectral variability of ultraluminous X-ray sources \|Kajava, Jari J. E., Poutanen, Juri, \| MNRAS \| 398-1450 \| 2009 \| 2009MNRAS.398.1450K \| http://ui.adsabs.harvard.edu/#abs/2009MNRAS.398.1450K X-ray spectral states and metallicity in the ultraluminous X-ray sources NGC 1313 X-1 and X-2 \|Pintore, Fabio, Zampieri, Luca, \| MNRAS \| 420-1107 \| 2012 \| 2012MNRAS.420.1107P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.420.1107P 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 XMM-Newton discovery of transient X-ray pulsar in NGC 1313 \|Trudolyubov, S. P., \| MNRAS \| 387-36 \| 2008 \| 2008MNRAS.387L..36T \| http://ui.adsabs.harvard.edu/#abs/2008MNRAS.387L..36T Multiwavelength Monitoring of the Unusual Ultraluminous Supernova SN 1978K in NGC 1313 and the Search for an Associated Gamma-Ray Burst \|Smith, I. A., Ryder, S. D., et al. \| ApJ \| 669-1130 \| 2007 \| 2007ApJ...669.1130S \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...669.1130S Six years of XMM-Newton observations of NGC 1313 X-1 and X-2 \|Pintore, F., Zampieri, L., \| AN \| 332-337 \| 2011 \| 2011AN....332..337P \| http://ui.adsabs.harvard.edu/#abs/2011AN....332..337P Associated spectral and temporal state transition of the bright ULXNGC1313 X-1 \|Dewangan, G. C., Misra, R., et al. \| MNRAS \| 407-291 \| 2010 \| 2010MNRAS.407..291D \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.407..291D 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 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 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 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 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 ultraluminous state revisited: fractional variability and spectral shape as diagnostics of super-Eddington accretion \|Sutton, Andrew D., Roberts, Timothy P., \| MNRAS \| 435-1758 \| 2013 \| 2013MNRAS.435.1758S \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.435.1758S Super-Eddington Accretion in the Ultraluminous X-Ray Source NGC 1313 X-2: An Ephemeral Feast \|Weng, Shan-Shan, Zhang, Shuang-Nan, \| ApJ \| 780-147 \| 2014 \| 2014ApJ...780..147W \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...780..147W 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 Irradiated, colour-temperature-corrected accretion discs in ultraluminous X-ray sources \|Sutton, Andrew D., Done, Chris, \| MNRAS \| 444-2415 \| 2014 \| 2014MNRAS.444.2415S \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.444.2415S A spectral-timing model for ULXs in the supercritical regime \|Middleton, Matthew J., Heil, Lucy, et al. \| MNRAS \| 447-3243 \| 2015 \| 2015MNRAS.447.3243M \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.447.3243M 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 Evidence for High-frequency QPOs with a 3:2 Frequency Ratio from a 5000 Solar Mass Black Hole \|Pasham, Dheeraj R., Cenko, S. Bradley, et al. \| ApJ \| 811-11 \| 2015 \| 2015ApJ...811L..11P \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...811L..11P The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 The X-ray decay of the ultraluminous supernova SN 1978K in NGC 1313 \|Zhao, Hai-Hui, Weng, Shan-Shan, \| MNRAS \| 468-1551 \| 2017 \| 2017MNRAS.468.1551Z \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468.1551Z 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 Recurrent Outbursts Revealed in 3XMM J031820.8-663034 \|Zhao, Hai-Hui, Weng, Shan-Shan, \| ApJ \| 859-106 \| 2018 \| 2018ApJ...859..106Z \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...859..106Z 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 A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw, H. P., Roberts, T. P., et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E 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 A new possible accretion scenario for ultra-luminous X-ray sources \|Kobayashi, Shogo B., Nakazawa, K., \| MNRAS \| 489-366 \| 2019 \| 2019MNRAS.489..366K \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489..366K Thermal stability of winds driven by radiation pressure in super-Eddington accretion discs \|Pinto, C., Mehdipour, M., et al. \| MNRAS \| 491-5702 \| 2020 \| 2020MNRAS.491.5702P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491.5702P 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 X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M First detection of X-ray line emission from Type IIn supernova 1978K with XMM-Newton.s RGS \|Chiba, Yuki, Katsuda, Satoru, et al. \| PASJ \| 72-25 \| 2020 \| 2020PASJ...72...25C \| http://ui.adsabs.harvard.edu/#abs/2020PASJ...72...25C Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Broadband X-ray spectral variability of the pulsing ULX NGC 1313 X-2 \|Robba, A., Pinto, C., et al. \| A&A \| 652-118 \| 2021 \| 2021A&A...652A.118R \| http://ui.adsabs.harvard.edu/#abs/2021A&A...652A.118R The impact of precession on the observed population of ULXs \|Khan, Norman, Middleton, Matthew J., et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows, R., Comerford, Julia M., et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S Winds in ultraluminous X\\u2011ray sources: New challenges \|Pinto, C., Kosec, P., \| AN \| 344-20220134 \| 2023 \| 2023AN....34420134P \| http://ui.adsabs.harvard.edu/#abs/2023AN....34420134P NGC 2403 XMM4: evidence for a super-Eddington neutron star with a possible transient pulsation \|Luangtip, Wasutep, Roberts, Timothy P., \| MNRAS \| 528-418 \| 2024 \| 2024MNRAS.528..418L \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.528..418L The XMM-Newton Line Emission Analysis Program (X-LEAP). 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 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	2005-10-11T01:02:53Z/2006-03-06T22:46:41Z
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	2008-06-23T00:00:00Z
Keywords	"reverse shock", "mass loss rates", "XMM", "ambient csm", "xray emission properties", "physical key parameters", "key parameters", "XMM-Newton", "supernova sne", "mass loss rate", "temperature evolution", "xmm newton", "physical parameters"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Stefan Immler, 2008, 'Probing the Environments of Young Supernovae with XMM-Newton', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-erky4nj