A dataset provided by the European Space Agency

Name: Unveiling the pulsating behaviour of J1813, a very energetic radio-quiet pulsar
Published: 2014-04-10T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	069396
Title	Unveiling the pulsating behaviour of J1813, a very energetic radio-quiet pulsar
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693960101
DOI	https://doi.org/10.5270/esa-bh24i9k
Principal Investigator, PI	Dr Martino Marelli
Abstract	After 3 years of all-sky scanning, Fermi has discovered dozens of new g-ray onlypulsars. Such a discovery has far reaching implications for our overallunderstanding of pulsar physics. We propose a joint XMM-Chandra observation ofJ1813-1246, one of the most energetic g-ray selected pulsar. J1813 rotates asfast as the Crab and its Erot is similar to that of Vela, thus we expect thepulsar to be embedded in a bright PWN. Among RQ pulsars, J1813 shows the highestX-ray flux but no deep X-ray observations have ever been performed on thistarget. Exploiting both XMM and Chandra capabilities we ll be able to (i)discriminate J1813 from its pulsar wind nebula (ii) study its X-ray timingbehaviour (iii) obtain accurate phase-averaged and phase-resolved spectra (iv) constrain the source distance.
Publications	On the Puzzling High-Energy Pulsations of the Energetic Radio-Quiet gamma-Ray Pulsar J1813-1246 \|Marelli M. Harding A. et al. \| ApJ \| 795-168 \| 2014 \| 2014ApJ...795..168M \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...795..168M 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 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 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-03-10T08:37:15Z/2013-03-11T14:52:34Z
Version	21.51_20241115_1113
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	2014-04-10T00:00:00Z
Last Update	2026-07-09
Keywords	"sky scanning", "discriminate j1813", "bright pwn", "phase averaged", "xray flux", "source distance", "XMM", "pulsar physics", "xmm chandra", "deep xray", "rq pulsars", "j1813 1246", "j1813 rotates"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Martino Marelli, 2014, 'Unveiling the pulsating behaviour of J1813, a very energetic radio-quiet pulsar', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-bh24i9k
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.