A dataset provided by the European Space Agency

Name: PSR J1119-6127 and the Physics of High-Magnetic-Field Neutron Stars
Published: 2012-07-30T00:00:00Z

Proposal ID	067279
Title	PSR J1119-6127 and the Physics of High-Magnetic-Field Neutron Stars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672790101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672790201
DOI	https://doi.org/10.5270/esa-tcu2ywo
Principal Investigator, PI	Prof Victoria Kaspi
Abstract	We propose a follow-up XMM observation of the young, high-magnetic-field radiopulsar PSR J1119-6127. A previous XMM observation revealed X-ray pulsations withunusual properties: a thermal spectrum with high temperature, narrow pulseprofile and high pulsed fraction. These characteristics, together with the lackof pulsations at high energies, are unlike those of most other radio pulsarsdetected at X-ray energies; the requested observation is required to confirmthem with high confidence. The fact that such emission is present in one of theyoungest radio pulsars which also has a magnetic field close to those ofmagnetars is intriguing, and likely signals phenomena important to our physicalunderstanding of high-magnetic-field neutron stars.
Publications	Deep X-Ray Observations of the Young High-magnetic-field Radio Pulsar J1119-6127 and Supernova Remnant G292.2-0.5 \|Ng, C.-Y., Kaspi, V. M., et al. \| ApJ \| 761-65 \| 2012 \| 2012ApJ...761...65N \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...761...65N Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y SOAR Optical and Near-infrared Spectroscopic Survey of Newly Discovered Massive Stars in the Periphery of Galactic Massive Star Clusters I-NGC 3603 \|Roman-Lopes, A., Franco, G. A. P., \| ApJ \| 823-96 \| 2016 \| 2016ApJ...823...96R \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...823...96R 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 The Fermi-LAT detection of magnetar-like pulsar PSR J1846-0258 at high-energy gamma-rays \|Kuiper, L., Hermsen, W., \| MNRAS \| 475-1238 \| 2018 \| 2018MNRAS.475.1238K \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.1238K 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 The EXTraS project: Exploring the X-ray transient and variable sky \|De Luca, A., Salvaterra, R., et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D 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	2011-06-13T18:12:51Z/2011-06-30T16:22:52Z
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	2012-07-30T00:00:00Z
Keywords	"xray energies", "XMM", "xray pulsations", "psr j1119 6127", "signals phenomena", "thermal spectrum", "narrow pulse profile", "pulsed fraction", "magnetic field close", "radio pulsars"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Victoria Kaspi, 2012, 'PSR J1119-6127 and the Physics of High-Magnetic-Field Neutron Stars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-tcu2ywo