A dataset provided by the European Space Agency

Name: X-Rays comma Dust comma Ice comma and Gas in Time openParX-DIGITclosePar
Published: 2012-03-04T00:00:00Z

Proposal ID	065235
Title	X-Rays, Dust, Ice, and Gas in Time (X-DIGIT)
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652350201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652350301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652350401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652350501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652350601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652350801
DOI	https://doi.org/10.5270/esa-t6fj0h7
Principal Investigator, PI	Dr Manuel Guedel
Abstract	We propose an extensive investigation of the impact of stellar X-rays on theplanet-forming molecular environments of T Tauri stars by combining X-ray datafrom XMM-Newton with novel far-infrared spectroscopy from our Herschel OpenTime Key Project and complementary mid-infrared spectroscopy from Spitzer. Theprincipal goals are, i) to identify X-ray tracers in the Herschel spectralrange, ii) to study the potential impact of X-rays on circumstellar disks, andiii) to model physical and chemical conditions in the regions where the X-rayimpact is significant. We wish to understand how X-ray radiation influencesstar- and planet formation through physical and chemical processing of disks.Understanding the distribution of the astrobiologically important water plays a key role.
Publications	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 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 Consistent dust and gas models for protoplanetary disks. IV. A panchromatic view of protoplanetary disks \|Dionatos, O., Woitke, P., et al. \| A&A \| 625-66 \| 2019 \| 2019A&A...625A..66D \| http://ui.adsabs.harvard.edu/#abs/2019A&A...625A..66D 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 ESASky SSOSS: Solar System Object Search Service and the case of Psyche \|Racero, E., Giordano, F., et al. \| A&A \| 659-38 \| 2022 \| 2022A&A...659A..38R \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..38R The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2010-08-10T01:39:21Z/2011-02-15T02:09:22Z
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	2012-03-04T00:00:00Z
Keywords	"chemical processing", "water plays", "circumstellar dis", "XMM-Newton", "chemical conditions", "time x digit", "xmm newton", "xray data", "key role", "x rays", "tauri stars", "stellar xray", "model physical", "XMM", "extensive investigation", "herschel spectral range", "potential impact", "xray impact", "xray tracers", "time key project", "planet formation", "infrared spectroscopy"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Manuel Guedel, 2012, 'X-Rays comma Dust comma Ice comma and Gas in Time openParX-DIGITclosePar', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-t6fj0h7