A dataset provided by the European Space Agency

Name: X-ray emission and star formation history in Spitzer-selected ETGs
Published: 2013-03-01T00:00:00Z

Proposal ID	067170
Title	X-ray emission and star formation history in Spitzer-selected ETGs
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671700101
DOI	https://doi.org/10.5270/esa-kykvyhb
Principal Investigator, PI	Dr Ginevra Trinchieri
Abstract	With this proposal we focus on a well selected sample of nearby ellipticals forwhich we reliably determine the star formation history from high S/N Spitzer andGALEX observations. We aim at determining the incidence and where possible theproperties of the hot ISM in light of the detailed characteristics of theirstellar population. Chosen galaxies are passively evolving systems, at most witha small episode of recent star formation. In light of current scenario we expectthem to have a sizable hot ISM. We request high quality X-ray data to determinethe ISM parameters, such as luminosity, spatial distribution, temperature wherepossible, to explore whether gas properties are homogeneous or whether evensmall perturbations in the SF history can alter the hot gas content.
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 Investigating early-type galaxy evolution with a multiwavelength approach - I. X-ray properties of 12 galaxies observed with Swift and XMM-Newton \|Trinchieri G. Rampazzo R. et al. \| MNRAS \| 449-3021 \| 2015 \| 2015MNRAS.449.3021T \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.449.3021T Non-detection of X-ray emission from sterile neutrinos in stacked galaxy spectra \|Anderson Michael E. Churazov Eugene \| MNRAS \| 452-3905 \| 2015 \| 2015MNRAS.452.3905A \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.452.3905A 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 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	2012-02-11T21:16:29Z/2012-02-13T01:45:17Z
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	2013-03-01T00:00:00Z
Last Update	2025-01-27
Keywords	"spatial distribution", "sizable hot ism", "nearby ellipticals", "star formation", "passively evolving systems", "hot ism", "quality xray data", "x ray emission", "gas properties", "star formation history", "stellar population", "sf history", "chosen galaxy", "ism parameters", "hot gas content"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ginevra Trinchieri, 2013, 'X-ray emission and star formation history in Spitzer-selected ETGs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-kykvyhb