A dataset provided by the European Space Agency

Name: Searching for thermal emission from nearby high magnetic field radio pulsars
Published: 2010-04-02T00:00:00Z

Proposal ID	055414
Title	Searching for thermal emission from nearby high magnetic field radio pulsars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554140401
DOI	https://doi.org/10.5270/esa-xwzubn7
Principal Investigator, PI	Dr Marjorie Gonzalez
Abstract	A major open issue in neutron star astrophysics is the connection between highmagnetic field radio pulsars (HBRP), isolated neutron stars (INS), andmagnetars. It is unclear why young HBRPs do not exhibit magnetar-like emission,and how INSs are related to both populations. We propose to observe threenearby, HBRPs to search for thermal emission from their surface. This emissionis predicted to be observable if dominated by magnetic field decay. The pulsarshave small distances and are regions of low interstellar absorption, offering usa rare opportunity to detect this emission or place strong constraints on itspresence. We will then be able to test whether there are overlapping radiativeproperties from the HBRPs to magnetars, or whether they really are two distinct classes.
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 Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz, Tobias, \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2009-03-15T21:34:59Z/2009-03-16T05:00:13Z
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	2010-04-02T00:00:00Z
Keywords	"overlapping radiative properties", "distinct classes", "magnetic field decay", "neutron star astrophysics", "exhibit magnetar", "low interstellar absorption", "thermal emission"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marjorie Gonzalez, 2010, 'Searching for thermal emission from nearby high magnetic field radio pulsars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xwzubn7