A dataset provided by the European Space Agency

Name: Understanding the emission geometry of rotation-powered pulsars
Published: 2019-05-04T22:00:00Z

Proposal ID	080425
Title	Understanding the emission geometry of rotation-powered pulsars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804250101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804250201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804250301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804250401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804250501
DOI	https://doi.org/10.5270/esa-u3tw640
Principal Investigator, PI	Dr Martino Marelli
Abstract	We propose deep EPIC observations of 5 X-ray-emitting rotation-powered pulsarsto obtain detailed view of their light curves and phase-resolved spectra,available so far for only three (not representative) sources. Our sample spans 4decades of energetics, including RPPs with different properties and radio/gamma-ray light curves shapes. Well investigate how RPP emission depends onenergetics, age and geometry. X-ray data will be aligned in phase withcontemporaneous gamma-ray and radio data and fitted, constraining the RPPemission models and geometry in these bands. Studying the multiband, phase-resolved spectra will reveal properties and physics of the pair distribution.Overall, our project will result in a decisive step forward in our understanding of RPP emissions.
Publications	Characterization of the Particle-induced Background of XMM-Newton EPIC-pn: Short- and Long-term Variability \|Bulbul Esra Kraft Ralph et al. \| ApJ \| 891-13 \| 2020 \| 2020ApJ...891...13B \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...891...13B A deep X-ray spectral imaging of the bow-shock pulsar wind nebula associated with PSR B1929+10 \|Kim S. I. Hui C. Y. et al. \| A&A \| 637-7 \| 2020 \| 2020A&A...637L...7K \| http://ui.adsabs.harvard.edu/#abs/2020A&A...637L...7K 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 ESASky SSOSS: Solar System Object Search Service and the case of Psyche \|Racero E. Giordano F. et al. \| A&A \| 659-38 \| 2022 \| 2022A&A...659A..38R \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..38R Mitigating the effects of particle background on the Athena Wide Field Imager \|Miller Eric D. Grant Catherine E. et al. \| JATIS \| 8-18001 \| 2022 \| 2022JATIS...8a8001M \| http://ui.adsabs.harvard.edu/#abs/2022JATIS...8a8001M X-Ray Studies of the Pulsar PSR J1420-6048 and Its TeV Pulsar Wind Nebula in the Kookaburra Region \|Park Jaegeun Kim Chanho et al. \| ApJ \| 945-33 \| 2023 \| 2023ApJ...945...33P \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...945...33P Extreme accretion events: TDEs and changingu2011look AGN \|Komossa S. Grupe D. \| AN \| 344-20230015 \| 2023 \| 2023AN....34430015K \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430015K 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	2017-04-06T22:18:59Z/2018-04-15T14:14:18Z
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	2019-05-04T22:00:00Z
Last Update	2025-01-27
Keywords	"rpp emission", "rpp emissions", "rotation powered pulsars", "pair distribution", "EPIC", "xray data", "light curves", "decisive step forward", "deep epic", "sample spans", "emission geometry", "phase resolved spectra", "rpp emission models", "gamma ray", "radio data"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Martino Marelli, 2019, 'Understanding the emission geometry of rotation-powered pulsars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-u3tw640