A dataset provided by the European Space Agency

Name: The most sensitive search for pulsations in a Central Compact Object
Published: 2011-05-05T00:00:00Z

Proposal ID	060628
Title	The most sensitive search for pulsations in a Central Compact Object
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606280101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606280201
DOI	https://doi.org/10.5270/esa-01uw58e
Principal Investigator, PI	Dr Andrea De Luca
Abstract	Central Compact Objects (CCOs) in SNR are a handful of puzzling sources supposedto be young, radio-quiet Isolated Neutron Stars (INSs). Recent X-ray timingresults unveiled the nature of a few individual CCOs and showed hat such aclass. is a heterogeneous group of dramatically different objects, possiblyincluding both weakly magnetized INSs and peculiar magnetars. Assessing thenature of CCOs would be crucial in order to get a view of the birth propertiesof neutron stars, which will have important implications for our overallunderstanding of INSs and of their evolutionary pathways. We selected the mostpromising source, RX J0822-4300 inside Puppis A, to perform a definitive searchfor pulsations.
Publications	A time-variable, phase-dependent emission line in the X-ray spectrum of the isolated neutron star RX J0822-4300 \|de Luca, A., Salvetti, D., et al. \| MNRAS \| 421-72 \| 2012 \| 2012MNRAS.421L..72D \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.421L..72D 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 The most complete and detailed X-ray view of the SNR Puppis A \|Dubner, G., Loiseau, N., et al. \| A&A \| 555-9 \| 2013 \| 2013A&A...555A...9D \| http://ui.adsabs.harvard.edu/#abs/2013A&A...555A...9D Unifying the observational diversity of isolated neutron stars via magneto-thermal evolution models \|Vigano, D., Rea, N., et al. \| MNRAS \| 434-123 \| 2013 \| 2013MNRAS.434..123V \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.434..123V 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 Magnetic fields in neutron stars \|Vigano, Daniele, \| PhDT \| 0-7 \| 2013 \| 2013PhDT.........7V \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.........7V Intermediate-mass Elements in Young Supernova Remnants Reveal Neutron Star Kicks by Asymmetric Explosions \|Katsuda, Satoru, Morii, Mikio, et al. \| ApJ \| 856-18 \| 2018 \| 2018ApJ...856...18K \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...856...18K 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 Rectangular core-collapse supernova remnants: application to Puppis A \|Meyer, D. M. -A., Vel\\u00e1zquez, P. F., et al. \| MNRAS \| 515-594 \| 2022 \| 2022MNRAS.515..594M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515..594M Progenitors and explosion properties of supernova remnants hosting central compact objects: II. A global systematic study with a comparison to nucleosynthesis models \|Braun, C., Safi-Harb, S., et al. \| MNRAS \| 525-6257 \| 2023 \| 2023MNRAS.525.6257B \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.525.6257B
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2009-12-17T19:31:50Z/2010-04-05T22:35:04Z
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	2011-05-05T00:00:00Z
Keywords	"neutron stars", "supernova remnant", "definitive search", "evolutionary pathways", "weakly magnetized inss", "sources supposed", "central compact object", "birth properties", "promising source", "individual ccos", "sensitive search"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Andrea De Luca, 2011, 'The most sensitive search for pulsations in a Central Compact Object', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-01uw58e