A dataset provided by the European Space Agency

Name: Fundamental properties of novae outburst
Published: 2014-12-05T23:00:00Z

Proposal ID	072820
Title	Fundamental properties of novae outburst
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728200201
DOI	https://doi.org/10.5270/esa-jmxt629
Principal Investigator, PI	Dr Gregory Schwarz
Abstract	We propose non-disruptive ToO observations of two optically bright Galacticnovae in outburst to observe their temporal UV evolution using the HST/STISechelle. One ToO will target a Carbon-Oxygen type nova and the other ToO will bereserved for the next high energy gamma-ray detected nova. The Fermi/LATdetection of high energy gamma-rays is a recent and unexpected discovery whosemechanism in classical novae is not currently understood. In both cases, UVspectroscopy is essential for determining elemental abundances, mass, dynamics,and structure. Each nova target would also be observed with a single, highresolution XMM/RGS exposure obtained while X-ray luminous (as determined by ourSwift X-ray monitoring).
Publications	Short-period X-ray oscillations in super-soft novae and persistent super-soft sources \|Ness, J.-U., Beardmore, A. P., et al. \| A&A \| 578-39 \| 2015 \| 2015A&A...578A..39N \| http://ui.adsabs.harvard.edu/#abs/2015A&A...578A..39N 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 Multiwavelength Modeling of the SED of Nova V339 Del: Stopping the Wind and Long-lasting Super-Eddington Luminosity with Dust Emission \|Skopal, Augustin, \| ApJ \| 878-28 \| 2019 \| 2019ApJ...878...28S \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...878...28S 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 The first nova eruption in a novalike variable: YZ Ret as seen in X-rays and \\u03b3-rays \|Sokolovsky, Kirill V., Li, Kwan-Lok, et al. \| MNRAS \| 514-2239 \| 2022 \| 2022MNRAS.514.2239S \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514.2239S 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	2013-11-21T13:11:10Z/2013-11-21T22:34:50Z
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	2014-12-05T23:00:00Z
Keywords	"resolution xmm", "temporal uv evolution", "XMM", "stis echelle", "xray luminous", "classical novae", "energy gamma ray", "fundamental properties", "determining elemental abundance", "novae outburst", "uv spectroscopy", "nova target", "lat detection", "rgs exposure", "swift xray", "HST", "energy gamma rays"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gregory Schwarz, 2014, 'Fundamental properties of novae outburst', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jmxt629