A dataset provided by the European Space Agency

Name: Star formation in the NGC7000/IC5070 complex
Published: 2012-12-17T00:00:00Z

Proposal ID	067958
Title	Star formation in the NGC7000/IC5070 complex
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0679580101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0679580201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0679580301
DOI	https://doi.org/10.5270/esa-3v8lb08
Principal Investigator, PI	Dr Francesco Damiani
Abstract	We propose a joint Chandra ACIS-I and XMM-Newton EPIC/pn observing program todiscover the still unknown population of the star-forming region NGC7000/IC5070,at 600 pc. Recent Spitzer data have shown this region to host 2000 or moreYoung Stellar Objects of Classes 0 to II, but missed Class III stars, whichare expected to be numerous as well. The requested combination of high-spatialresolution ACIS data (3 pointings, total exposure: 144 ks), and wider-fieldEPIC data (3 pointings, total exposure: 73.5 ks) optimizes coverage of bothclustered and diffuse YSO populations. These data will permit studies of thestar formation history, early cluster evolution, mass spectrum and segregation,with unprecedented accuracy for this rich region.
Publications	X-ray and UV observations of V751 Cygni in an optical high state \|Page K. L. Osborne J. P. et al. \| A&A \| 570-37 \| 2014 \| 2014A&A...570A..37P \| http://ui.adsabs.harvard.edu/#abs/2014A&A...570A..37P 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 X-ray survey of the North-America and Pelican star-forming complex (NGC 7000/IC 5070) \|Damiani Francesco Pillitteri Ignazio \| A&A \| 602-115 \| 2017 \| 2017A&A...602A.115D \| http://ui.adsabs.harvard.edu/#abs/2017A&A...602A.115D 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 X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions \|Ortiz R. Guerrero M. A. \| ApJ \| 912-93 \| 2021 \| 2021ApJ...912...93O \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...912...93O 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	2011-11-23T23:50:39Z/2011-11-25T02:27:32Z
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	2012-12-17T00:00:00Z
Last Update	2025-01-27
Keywords	"ic5070 complex", "rich region", "EPIC", "star formation", "NGC7000", "xmm newton epic", "mass spectrum", "requested combination", "XMM-Newton", "stellar objects", "chandra acis", "star formation history", "optimizes coverage", "XMM", "cluster evolution", "spitzer data", "diffuse yso populations", "total exposure"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Francesco Damiani, 2012, 'Star formation in the NGC7000/IC5070 complex', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-3v8lb08