A dataset provided by the European Space Agency

Name: Unveiling the timing behaviour of the radio-quiet Vela-like pulsar J1826-1256
Published: 2015-11-04T23:00:00Z

Proposal ID	074442
Title	Unveiling the timing behaviour of the radio-quiet Vela-like pulsar J1826-1256
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744420101
DOI	https://doi.org/10.5270/esa-2gs92wi
Principal Investigator, PI	Dr Massimiliano Razzano
Abstract	The radio-quiet gamma-ray pulsars discovered by Fermi Large Area Telescope arecrucial to understand pulsar magnetospheres and the Galactic neutron starpopulation. We propose a deep XMM observation of PSR J1826-1256, the young,energetic radio-quiet pulsar in the Eel nebula. Its timing parameters andgamma-ray properties are similar to those of the Vela pulsar. Comparing its Xand gamma-ray emission with other Vela-like, but radio-loud, pulsars will helpto probe the nature of radio quietness/loudness in pulsars. We will exploit XMMto search for X-ray pulsations of the X-ray bright PSR J1826-1256, detail itstiming and spectral behaviour, and discriminate the pulsar emission from that ofits nebula by using archival Chandra data.
Publications	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 Theoretically Motivated Search and Detection of Non-thermal Pulsations from PSRs J1747-2958 J2021+3651 and J1826-1256 \|Li Jian Torres Diego F. et al. \| ApJ \| 868-29 \| 2018 \| 2018ApJ...868L..29L \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...868L..29L A new study towards PSR J1826-1334 and PSR J1826-1256 in the region of HESS J1825-137 and HESS J1826-130 \|Duvidovich L. Giacani E. et al. \| A&A \| 623-115 \| 2019 \| 2019A&A...623A.115D \| http://ui.adsabs.harvard.edu/#abs/2019A&A...623A.115D X-ray studies of the gamma-ray pulsar J1826-1256 and its pulsar wind nebula with Chandra and XMM-Newton \|Karpova Anna V. Zyuzin Dmitry A. \| MNRAS \| 487-1964 \| 2019 \| 2019MNRAS.487.1964K \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487.1964K 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 The Eel Pulsar Wind Nebula: A PeVatron-candidate Origin for HAWC J1826-128 and HESS J1826-130 \|Burgess Daniel A. Mori Kaya et al. \| ApJ \| 930-148 \| 2022 \| 2022ApJ...930..148B \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930..148B 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	2014-10-11T16:23:16Z/2014-10-13T07:18:16Z
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	2015-11-04T23:00:00Z
Last Update	2025-01-27
Keywords	"archival chandra data", "vela pulsar", "gamma ray properties", "pulsar magnetosphere", "pulsar emission", "psr j1826 1256", "pulsar j1826 1256", "radio quiet vela", "radio quietness", "xray pulsations", "radio loud", "gamma ray emission", "deep xmm", "XMM", "exploit xmm"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Massimiliano Razzano, 2015, 'Unveiling the timing behaviour of the radio-quiet Vela-like pulsar J1826-1256', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2gs92wi