A dataset provided by the European Space Agency

Name: X-rays from young open clusters in the Gaia-ESO Survey: completing the sample
Published: 2014-05-11T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	069473
Title	X-rays from young open clusters in the Gaia-ESO Survey: completing the sample
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694730101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694730301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694730401
DOI	https://doi.org/10.5270/esa-s1502f1
Principal Investigator, PI	Dr Elena Franciosini
Abstract	The Gaia-ESO Survey will provide the first homogeneous spectroscopic study ofthe kinematics and elemental abundances of open clusters. Combined with X-raydata, it will allow a complete characterization of the cluster populations andof magnetic activity as a function of age, metallicity, ambient environment anddynamical evolution, improving our understanding of the activity-rotation-agerelationship. Here we propose to observe the four young open clusters IC 4665,NGC 2451, NGC 6504 and NGC 6716, to complete the sample of nearby clusters inthe Survey observed with modern X-ray telescopes, and to fill the gaps in thecrucial 30-100 Myr age range where the transition from pre-main sequence to mainsequence X-ray activity regime occurs.
Publications	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 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 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-04-11T06:48:05Z/2013-04-25T23:36:40Z
Version	21.51_20241115_1113
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	2014-05-11T00:00:00Z
Last Update	2026-07-09
Keywords	"pre main sequence", "complete characterization", "x rays", "myr age range", "homogeneous spectroscopic", "gaia eso survey", "ngc 6504", "cluster ic 4665", "NGC 2451", "ngc 2451", "elemental abundance", "magnetic activity", "nearby cluster", "dynamical evolution", "ngc 6716", "xray data", "cluster populations", "modern xray telescopes"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Elena Franciosini, 2014, 'X-rays from young open clusters in the Gaia-ESO Survey: completing the sample', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-s1502f1
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.