A dataset provided by the European Space Agency

Name: Searching for XRBs in the Dwarf Irregular Phoenix Galaxy
Published: 2010-08-18T00:00:00Z

Proposal ID	060135
Title	Searching for XRBs in the Dwarf Irregular Phoenix Galaxy
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0601350101
DOI	https://doi.org/10.5270/esa-tjquwct
Principal Investigator, PI	Prof Malcolm Coe
Abstract	Dwarf galaxies, both irregular and elliptical/spirals represent a key stage inthe formation of galactic structures - possibly one of the earliest phases.Studies of such objects, and the formation of stars therein, is r^ant toresearch on stellar evolution, primordial abundances and the chemical evolutionof galaxies in general. Through the X-ray channel it is possible to gainsignificant insight into the formation of evolved binary systems and hence theunderlying star formation rates (SFR) over recent epochs. In this proposal weplan to extend out previous Chandra and XMM work on the SMC to another similargalaxy - Phoenix.
Publications	The search for high-mass X-ray binaries in the Phoenix dwarf galaxy \|Bartlett E. S. Coe M. J. et al. \| MNRAS \| 422-2302 \| 2012 \| 2012MNRAS.422.2302B \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.422.2302B 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 High mass X-ray binaries in the MilkyWay and beyond: a multiwavelength temporal and spectroscopic study \|Bartlett Elizabeth \| PhDT \| 0-107 \| 2013 \| 2013PhDT.......107B \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......107B 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2009-07-07T08:13:08Z/2009-07-07T21:30:06Z
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	2010-08-18T00:00:00Z
Last Update	2025-01-27
Keywords	"dwarf galaxy", "galactic structures", "key stage", "evolved binary systems", "stars therein", "earliest phases", "chemical evolution", "stellar evolution", "XMM", "primordial abundance", "xray channel", "galaxy phoenix"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Malcolm Coe, 2010, 'Searching for XRBs in the Dwarf Irregular Phoenix Galaxy', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-tjquwct