A dataset provided by the European Space Agency

Name 060066
Title Resolving short supersoft source states of optical novae in the core of M31
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600660201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600660301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600660401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600660501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600660601

DOI 10.5270/esa-1zqzwdf
Author Dr Wolfgang Pietsch
Description We propose to continue the monitoring of the M31 core with five 18.4ks XMM EPIC and five 20ks Chandra HRC-I observations equally distributed from Nov 2009 to mid Feb2010 to determine additional light curves for short supersoft source (SSS) states of optical novae. SSS states with <100d duration indicate accreting massive white dwarfs. They are proposed as SNIa progenitors. Determining their frequency is very important. We will correlate detected sources with novae from optical monitoring. With a nova rate in the field of ~25-yr and SSS states last- ing from weeks to years we will follow light curves of many novae. Durations of the nova SSS state will allow us to constrain envelope and white dwarf masses. We also will monitor time variability of ~200 M31 X-ray sources (mostly XRBs).
Publication CXOM31 J004253.1+411422: the first ultraluminous X-ray transient in M 31 . Kaur, A., Henze, M., et all. . A&A . 538-49 . 2012 . 2012A&A...538A..49K ,
The missing link: a low-mass X-ray binary in M31 seen as an ultraluminous X-ray source . Middleton, Matthew J., Sutton, Andrew D., et all. . MNRAS . 420-2969 . 2012 . 2012MNRAS.420.2969M ,
Light curves of six bright soft X-ray transients in M31 . Nooraee, Nakisa, . MNRAS . 428-205 . 2013 . 2013MNRAS.428..205N ,
The effect of advection at luminosities close to Eddington: The ULX in M 31 . Straub, O., Done, C., . A&A . 553-61 . 2013 . 2013A&A...553A..61S ,
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 ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog: Objects of Special Interest . Lin, Dacheng, Webb, Natalie A., . ApJ . 780-39 . 2014 . 2014ApJ...780...39L ,
X-ray monitoring of classical novae in the central region of M 31 III. Autumn and winter 2009-10, 2010-11, and 2011-12 . Henze, M., Pietsch, W., et all. . A&A . 563-2 . 2014 . 2014A&A...563A...2H ,
Unidentified Line in X-Ray Spectra of the Andromeda Galaxy and Perseus Galaxy Cluster . Boyarsky, A., Ruchayskiy, O., et all. . PhRvL . 113-251301 . 2014 . ...,
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 ,
Detection of a Compact Nuclear Radio Source in the Local Group Elliptical Galaxy M32 . Yang, Yang, Li, Zhiyuan, et all. . ApJ . 807-19 . 2015 . 2015ApJ...807L..19Y ,
Non-detection of X-ray emission from sterile neutrinos in stacked galaxy spectra . Anderson, Michael E., Churazov, Eugene, . MNRAS . 452-3905 . 2015 . 2015MNRAS.452.3905A ,
A novel scenario for the possible X-ray line feature at ~3.5 keV. Charge exchange with bare sulfur ions . Gu, L., Kaastra, J., et all. . A&A . 584-11 . 2015 . 2015A&A...584L..11G ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Crossing the Eddington Limit: Examining Disk Spectra at High Accretion Rates . Sutton, Andrew D., Swartz, Douglas A., et all. . ApJ . 836-48 . 2017 . 2017ApJ...836...48S ,
The Slowest Spinning X-Ray Pulsar in an Extragalactic Globular Cluster . Zolotukhin, Ivan Yu., Bachetti, Matteo, et all. . ApJ . 839-125 . 2017 . 2017ApJ...839..125Z ,
Discovery of Periodic Dips in the Brightest Hard X-Ray Source of M31 with EXTraS . Marelli, Martino, Tiengo, Andrea, et all. . ApJ . 851-27 . 2017 . 2017ApJ...851L..27M ,
X-Ray Lines from Dark Matter Annihilation at the keV Scale . Brdar, Vedran, Kopp, Joachim, et all. . PhRvL . 120-61301 . 2018 . 2018PhRvL.120f1301B ,
Astrophysical Accretion and Feedback: The Bayesian Linchpin of Theory and Observation . Roberts, Shawn R., . PhDT . 0-81 . 2017 . 2017PhDT........81R ,
WIMP dark matter candidates and searches---current status and future prospects . Roszkowski, Leszek, Sessolo, Enrico Maria, . RPPh . 81-66201 . 2018 . 2018RPPh...81f6201R ,
Creation of the X-ray sky maps and their application for a search of the dark matter decay line . Yakubovskyi, D. A., Savchenko, D. O., . KosNT . 21-90 . 2015 . 2015KosNT..21e..90Y ,
Resonant Scattering Effect on the Soft X-Ray Line Emission from the Hot Interstellar Medium. I. Galactic Bulges . Chen, Yang, Wang, Q. Daniel, et all. . ApJ . 861-138 . 2018 . 2018ApJ...861..138C ,
XMM-Newton RGS Spectroscopy of the M31 Bulge. I. Evidence for a Past AGN Half a Million Years Ago . Zhang, Shuinai, Wang, Q. Daniel, et all. . ApJ . 885-157 . 2019 . 2019ApJ...885..157Z ,
Deep XMM-Newton observations of the northern disc of M31. II. Tracing the hot interstellar medium . Kavanagh, Patrick J., Sasaki, Manami, et all. . A&A . 637-12 . 2020 . 2020A&A...637A..12K ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-12-28T12:18:42Z/2010-02-02T07:06:03Z
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 2011-03-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-03-02T00:00:00Z, 060066, 17.56_20190403_1200. https://doi.org/10.5270/esa-1zqzwdf