A dataset provided by the European Space Agency

Name: Measuring the Spin-Down and Magnetic Field Strength of the CCO Pulsar in PuppisA
Published: 2013-04-28T00:00:00Z

Proposal ID	065760
Title	Measuring the Spin-Down and Magnetic Field Strength of the CCO Pulsar in PuppisA
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0657600101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0657600201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0657600301
DOI	https://doi.org/10.5270/esa-zzawpag
Principal Investigator, PI	Prof Jules Halpern
Abstract	This proposal is the second element of our two-year plan to measure thespin-downrate of the pulsar in Puppis A by obtaining a phase-coherent timing solution. Ifit is a weakly magnetized neutron star like the other CCO pulsars, this is theonly practical way of measuring its spin-down. Our sensitivity to P-dot willcorrespond to a surface dipole B-field as small as 3.e10 G, comparable to ourmeasured value for the CCO pulsar PSR J1852+0040 in Kes 79. Such a result wouldprovide important support for the anti-magnetar model of CCOs. In addition,we will explore possible reasons for the unexplained surface hot spots using theenergy-dependent pulse profiles and phase-resolved spectra.
Publications	The Spin-down of PSR J0821-4300 and PSR J1210-5226: Confirmation of Central Compact Objects as Anti-magnetars \|Gotthelf, E. V., Halpern, J. P., \| ApJ \| 765-58 \| 2013 \| 2013ApJ...765...58G \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...765...58G 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 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 Measuring the Nonaxially Symmetric Surface Temperature Distribution of the Central Compact Object in Puppis A \|Alford, J. A. J., Gotthelf, E. V., et al. \| ApJ \| 927-233 \| 2022 \| 2022ApJ...927..233A \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...927..233A
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2011-05-18T22:05:00Z/2012-04-10T10:18:44Z
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	2013-04-28T00:00:00Z
Keywords	"magnetic field strength", "phase resolved spectra", "cco pulsars", "phase coherent", "kes 79", "surface dipole", "anti magnetar", "cco pulsar"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Jules Halpern, 2013, 'Measuring the Spin-Down and Magnetic Field Strength of the CCO Pulsar in PuppisA', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zzawpag