A dataset provided by the European Space Agency

Name 050423
Title Searching For Thermal Emission in Two Nearby High Magnetic Field Radio Pulsars
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504230201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504230301

DOI 10.5270/esa-ij0oto7
Author Prof Victoria Kaspi
Description We propose to observe the nearby, high magnetic field radio pulsars PSRs B1916+14 and B1845-19 in order to search for thermal emission from their surface. Models of thermal emission from neutron stars predict that these pulsars can have detectable emission arising from cooling of their interior or decay of their magnetic field. The pulsars are located at distances less than 2 kpc and in regions of low interstellar absorption, offering us a rare opportunity to place strong constraints on the presence of any anomalous thermal X-ray emission from possible radio pulsar-magnetar transition objects.
Publication Xmm-Newton X-Ray Detection of the High-Magnetic-Field Radio Pulsar PSR B1916+14 . Zhu, Weiwei, Kaspi, Victoria M., et all. . ApJ . 704-1321 . 2009 . 2009ApJ...704.1321Z ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
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 ,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
The XMM Cluster Survey: Present status and latest results . Viana, P. ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-03-25T12:50:05Z/2008-03-25T22:12:24Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2009-04-11T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-04-11T00:00:00Z, 050423, 17.56_20190403_1200. https://doi.org/10.5270/esa-ij0oto7