A dataset provided by the European Space Agency

Name: X-Rays, Dust, Ice, and Gas in Time (X-DIGIT)
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
Last Update	2025-01-27
Keywords	"chemical conditions", "xray impact", "xmm newton", "extensive investigation", "tauri stars", "potential impact", "XMM", "xray data", "key role", "infrared spectroscopy", "model physical", "planet formation", "chemical processing", "stellar xray", "XMM-Newton", "time key project", "circumstellar dis", "time x digit", "herschel spectral range", "x rays", "water plays", "xray tracers"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Manuel Guedel, 2012, 'X-Rays, Dust, Ice, and Gas in Time (X-DIGIT)', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-t6fj0h7