A dataset provided by the European Space Agency

Name: NRCO EPIC main proposal
Published: 2016-05-04T22:00:00Z

Proposal ID	079158
Title	NRCO EPIC main proposal
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791580101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791580201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791580301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791580401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791580501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791580601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791580701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791580801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791580901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791581001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791581101 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0791581201
DOI	https://doi.org/10.5270/esa-z92aiss
Principal Investigator, PI	Dr Fred Jansen XMM-Newton PS
Abstract	NRCO - proposal to store all EPIC requests as separate observations:obs1-6:RXJ1856.6-3754obs7-12: 1E 0102-72.2
Publications	Discovery of a 26.2 day period in the long-term X-ray light curve of SXP 1323: a very short orbital period for a long spin period pulsar \|Carpano, S., Haberl, F., \| A&A \| 602-81 \| 2017 \| 2017A&A...602A..81C \| http://ui.adsabs.harvard.edu/#abs/2017A&A...602A..81C Identification of AGN in the XMM-Newton X-ray survey of the SMC \|Maitra, Chandreyee, Haberl, Frank, et al. \| A&A \| 622-29 \| 2019 \| 2019A&A...622A..29M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...622A..29M Hard X-Ray Excess from the Magnificent Seven Neutron Stars \|Dessert, Christopher, Foster, Joshua W., \| ApJ \| 904-42 \| 2020 \| 2020ApJ...904...42D \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904...42D Axion Emission Can Explain a New Hard X-Ray Excess from Nearby Isolated Neutron Stars \|Buschmann, Malte, Co, Raymond T., et al. \| PhRvL \| 126-21102 \| 2021 \| 2021PhRvL.126b1102B \| http://ui.adsabs.harvard.edu/#abs/2021PhRvL.126b1102B 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 Two decades of X-ray observations of the isolated neutron star RX J1856.5 - 3754: detection of thermal and non-thermal hard X-rays and refined spin-down measurement \|De Grandis, Davide, Rigoselli, Michela, et al. \| MNRAS \| 516-4932 \| 2022 \| 2022MNRAS.516.4932D \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.516.4932D 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 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	2016-04-16T16:42:40Z/2016-04-27T15:30:36Z
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	2016-05-04T22:00:00Z
Keywords	"epic requests", "EPIC", "1e 0102 72", "3754 obs7", "nrco epic main"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton PS, 2016, 'NRCO EPIC main proposal', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-z92aiss