A dataset provided by the European Space Agency

Name: High Resolution Spectroscopy of Knots in the Puppis A Supernova Remnant
Published: 2004-09-17T00:00:00Z

Proposal ID	015015
Title	High Resolution Spectroscopy of Knots in the Puppis A Supernova Remnant
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150150101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150150201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0150150301
DOI	https://doi.org/10.5270/esa-f2rhjhc
Principal Investigator, PI	Dr Una Hwang
Abstract	We propose observations of two prominent knots in the Puppis A supernova remnantusing the XMM gratings. These knots are comparable in extent to sources thathave been successfully observed with the RGS, and have relatively high surfacebrightness compared to their surroundings. They are believed to be interstellarclouds in different density environments that are interacting with the remnant.sforward shock. Puppis A.s rich O, Ne, and Fe emission line spectrum iswell-matched to the bandpass of the XMM gratings. High resolution spectra arethe only way to directly measure line fluxes that would provide importantdiagnostics of the nonequilibrium ionization state of each element, and theirrelative abundances, including signatures of possible enrichment by the ejecta.
Publications	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 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 Chandra X-Ray Observation of a Mature Cloud-Shock Interaction in the Bright Eastern Knot Region of Puppis A \|Hwang, Una, Flanagan, Kathryn A., \| ApJ \| 635-355 \| 2005 \| 2005ApJ...635..355H \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...635..355H A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations \|Muno, M. P., Gaensler, B. M., et al. \| ApJ \| 680-639 \| 2008 \| 2008ApJ...680..639M \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...680..639M 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 Discovery of X-ray-emitting O-Ne-Mg-rich Ejecta in the Galactic Supernova Remnant Puppis A \|Katsuda, Satoru, Hwang, Una, et al. \| ApJ \| 714-1725 \| 2010 \| 2010ApJ...714.1725K \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...714.1725K 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 High-resolution X-Ray Spectroscopy of the Galactic Supernova Remnant Puppis A with XMM-Newton/RGS \|Katsuda, Satoru, Tsunemi, Hiroshi, et al. \| ApJ \| 756-49 \| 2012 \| 2012ApJ...756...49K \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...49K 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 The most complete and detailed X-ray view of the SNR Puppis A \|Dubner, G., Loiseau, N., et al. \| A&A \| 555-9 \| 2013 \| 2013A&A...555A...9D \| http://ui.adsabs.harvard.edu/#abs/2013A&A...555A...9D 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 Feature-tailored spectroscopic analysis of the supernova remnant Puppis A in X-rays \|Luna, G. J. M., Smith, M. J. S., et al. \| A&A \| 590-70 \| 2016 \| 2016A&A...590A..70L \| http://ui.adsabs.harvard.edu/#abs/2016A&A...590A..70L 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 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 Intermediate-mass Elements in Young Supernova Remnants Reveal Neutron Star Kicks by Asymmetric Explosions \|Katsuda, Satoru, Morii, Mikio, et al. \| ApJ \| 856-18 \| 2018 \| 2018ApJ...856...18K \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...856...18K 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 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 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 Wide-field X-ray observations of the supernova remnant Puppis A with the SRG/ART-XC telescope \|Krivonos, R., Arefiev, V., et al. \| MNRAS \| 510-3113 \| 2022 \| 2022MNRAS.510.3113K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.510.3113K Rectangular core-collapse supernova remnants: application to Puppis A \|Meyer, D. M. -A., Vel\\u00e1zquez, P. F., et al. \| MNRAS \| 515-594 \| 2022 \| 2022MNRAS.515..594M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515..594M Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Puppis A \|Aruga, M., Sano, H., et al. \| ApJ \| 938-94 \| 2022 \| 2022ApJ...938...94A \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...938...94A Progenitors and explosion properties of supernova remnants hosting central compact objects: II. A global systematic study with a comparison to nucleosynthesis models \|Braun, C., Safi-Harb, S., et al. \| MNRAS \| 525-6257 \| 2023 \| 2023MNRAS.525.6257B \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.525.6257B The Peculiar Ejecta Rings in the O-Rich Supernova Remnant Puppis A: Evidence of a Binary Interaction? \|Ghavamian, Parviz, Seitenzahl, Ivo R., et al. \| ApJ \| 960-7 \| 2024 \| 2024ApJ...960....7G \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...960....7G 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	2003-04-17T07:20:12Z/2003-06-25T22:19:08Z
Version	17.56_20190403_1200
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	2004-09-17T00:00:00Z
Keywords	"resolution spectroscopy", "supernova remnant", "XMM", "surface brightness", "forward shock", "line fluxes", "xmm gratings", "relative abundance", "density environments", "prominent knots", "interstellar clouds", "resolution spectra", "nonequilibrium ionization"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Una Hwang, 2004, 'High Resolution Spectroscopy of Knots in the Puppis A Supernova Remnant', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-f2rhjhc