A dataset provided by the European Space Agency

Name: Supersoft X-ray source states of optical novae in the disk of M 31
Published: 2013-02-09T00:00:00Z

Proposal ID	065562
Title	Supersoft X-ray source states of optical novae in the disk of M 31
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655620301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655620401
DOI	https://doi.org/10.5270/esa-ft18pgw
Principal Investigator, PI	Mr Martin Henze
Abstract	We propose Target of Opportunity (ToO) observations to characterise thesupersoft X-ray emission of optical novae in the disk of M 31 with four 20 ksXMM-Newton EPIC observations during July 2010 to mid-August 2010 and January2011 to mid-February 2011. These observations will allow to perform spectralanalysis of M 31 disk novae during their supersoft X-ray source state (SSS) andto determine effective temperatures and luminosities. The probability oftriggering all four observations on four different novae is high. Ourobservations will double the number of M 31 disk novae with known SSS spectra.This will help to study the differences between bulge novae and disk novae inthe X-ray regime.
Publications	M31N 2008-05d: a M 31 disk nova with a dipping supersoft X-ray light curve \|Henze, M., Pietsch, W., et al. \| A&A \| 544-44 \| 2012 \| 2012A&A...544A..44H \| http://ui.adsabs.harvard.edu/#abs/2012A&A...544A..44H 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 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 An XMM-Newton View of the Andromeda Galaxy as Explored in a Legacy Survey (New-ANGELS). I. The X-Ray Source Catalog \|Huang, Rui, Li, Jiang-Tao, et al. \| ApJS \| 268-36 \| 2023 \| 2023ApJS..268...36H \| http://ui.adsabs.harvard.edu/#abs/2023ApJS..268...36H 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	2011-08-01T05:27:15Z/2012-01-22T03:10:46Z
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	2013-02-09T00:00:00Z
Keywords	"xmm newton epic", "effective temperatures", "bulge novae", "XMM", "sss spectra", "xray regime", "disk novae", "M 31", "XMM-Newton", "perform spectral analysis", "EPIC", "supersoft xray source", "supersoft xray emission", "optical novae"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Martin Henze, 2013, 'Supersoft X-ray source states of optical novae in the disk of M 31', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ft18pgw