A dataset provided by the European Space Agency

Name: A Deep Observation of V1118 Ori in Outburst with XMM-Newton
Published: 2007-05-23T00:00:00Z

Proposal ID	040320
Title	A Deep Observation of V1118 Ori in Outburst with XMM-Newton
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0403200101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0403200201
DOI	https://doi.org/10.5270/esa-0m5yon9
Principal Investigator, PI	Dr Marc Audard
Abstract	We propose to observe the young accreting star V1118 Ori with XMM-Newton for100ks during AO5. We aim to obtain a high signal-to-noise ratio CCD spectrum toquantify the X-ray properties of V1118 Ori in outburst in detail. Our goal is todetect additional spectral components than the dominant plasma detected in theCCD spectra obtained during previous short observations. The long exposure willhelp us to study the short-term variability of V1118 Ori in the X-rays, and tocorrelate it with the optical and near-infrared light curves. The XMM-Newtondata will complement our approved Chandra X-ray monitoring that will continue in2006. The X-ray data will help us to understand the interplay between theaccretion disk and the magnetosphere and photosphere of an accreting young star.
Publications	A multi-wavelength study of the young star V1118 Orionis in outburst \|Audard M. Stringfellow G. S. et al. \| A&A \| 511-63 \| 2010 \| 2010A&A...511A..63A \| http://ui.adsabs.harvard.edu/#abs/2010A&A...511A..63A 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 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 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 Orion revisited. I. The massive cluster in front of the Orion nebula cluster \|Alves J. Bouy H. \| A&A \| 547-97 \| 2012 \| 2012A&A...547A..97A \| http://ui.adsabs.harvard.edu/#abs/2012A&A...547A..97A Hot stars observed by XMM-Newton. I. The catalog and the properties of OB stars \|Naze Y. \| A&A \| 506-1055 \| 2009 \| 2009A&A...506.1055N \| http://ui.adsabs.harvard.edu/#abs/2009A&A...506.1055N Young Stellar Objects in Lynds 1641: Disks Accretion and Star Formation History \|Fang Min Kim Jinyoung Serena et al. \| ApJS \| 207-5 \| 2013 \| 2013ApJS..207....5F \| http://ui.adsabs.harvard.edu/#abs/2013ApJS..207....5F Transitional Disks and Their Origins: An Infrared Spectroscopic Survey of Orion A \|Kim K. H. Watson Dan M. et al. \| ApJ \| 769-149 \| 2013 \| 2013ApJ...769..149K \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...769..149K A New Halpha Emission-line Survey in the Orion Nebula Cluster \|Szegedi-Elek E. Kun M. et al. \| ApJS \| 208-28 \| 2013 \| 2013ApJS..208...28S \| http://ui.adsabs.harvard.edu/#abs/2013ApJS..208...28S 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 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 Disruption of the Orion molecular core 1 by wind from the massive star theta1 Orionis C \|Pabst C. Higgins R. et al. \| Natur \| 565-618 \| 2019 \| 2019Natur.565..618P \| http://ui.adsabs.harvard.edu/#abs/2019Natur.565..618P 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 Exploring X-ray variability with unsupervised machine learning. I. Self-organizing maps applied to XMM-Newton data \|Kovau010deviu0107 M. Pasquato M. et al. \| A&A \| 659-66 \| 2022 \| 2022A&A...659A..66K \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..66K From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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	2006-03-02T15:16:53Z/2006-03-03T21:06:28Z
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	2007-05-23T00:00:00Z
Last Update	2025-01-27
Keywords	"accretion disk", "xray data", "short term variability", "dominant plasma", "approved chandra xray", "xmm newton", "XMM-Newton", "xray properties", "xmm newton data", "infrared light curves", "XMM", "ccd spectra", "v1118 ori", "additional spectral components"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marc Audard, 2007, 'A Deep Observation of V1118 Ori in Outburst with XMM-Newton', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0m5yon9