A dataset provided by the European Space Agency

Name 080425
Title Understanding the emission geometry of rotation-powered pulsars
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804250101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804250201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804250301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804250401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804250501

DOI 10.5270/esa-u3tw640
Author Dr Martino Marelli
Description We propose deep EPIC observations of 5 X-ray-emitting rotation-powered pulsars to obtain detailed view of their light curves and phase-resolved spectra, available so far for only three (not representative) sources. Our sample spans 4 decades of energetics, including RPPs with different properties and radio-gamma- ray light curves. shapes. We.ll investigate how RPP emission depends on energetics, age and geometry. X-ray data will be aligned in phase with contemporaneous gamma-ray and radio data and fitted, constraining the RPP emission 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.
Publication Characterization of the Particle-induced Background of XMM-Newton EPIC-pn: Short- and Long-term Variability . Bulbul, Esra, Kraft, Ralph, et all. . ApJ . 891-13 . 2020 . 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 all. . A&A . 637-7 . 2020 . 2020A&A...637L...7K ,
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2019-05-04T22:00:00Z, 080425, 17.56_20190403_1200. https://doi.org/10.5270/esa-u3tw640