A dataset provided by the European Space Agency

Name: The old
Published: 2012-10-15T00:00:00Z

Proposal ID	067444
Title	The old
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674440101
DOI	https://doi.org/10.5270/esa-8au2rux
Principal Investigator, PI	Dr Andrea De Luca
Abstract	The Fermi mission opened a new era for pulsar astronomy, detecting gamma-raypulsations from more than 60 pulsars, 30% of which are not seen at radiowavelengths. One of the most interesting Fermi pulsars is PSR J0357+32, aradio-quiet source standing out as the gamma-ray pulsar with the smallestspin-down luminosity (Erotvirgul1e33 erg/s) known so far. We observed PSR J0357+32with Chandra and we detected its X-ray counterpart, but we could not constrainits emission properties. Chandra data unveiled the existence of a huge (9 arcminlong) extended feature apparently protruding from the pulsar, with a peculiarphenomenology. We ask for a deep observation with XMM in order to assess thepulsar emission properties as well as the nature of the extended feature.
Publications	PSR J0357+3205: The Tail of the Turtle \|Marelli, M., De Luca, A., et al. \| ApJ \| 765-36 \| 2013 \| 2013ApJ...765...36M \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...765...36M Deep optical observations of the gamma-ray pulsar J0357+3205 \|Kirichenko, A., Danilenko, A., et al. \| A&A \| 564-81 \| 2014 \| 2014A&A...564A..81K \| http://ui.adsabs.harvard.edu/#abs/2014A&A...564A..81K 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 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 Pulsar-Wind Nebulae and Magnetar Outflows: Observations at Radio, X-Ray, and Gamma-Ray Wavelengths \|Reynolds, Stephen P., Pavlov, George G., et al. \| SSRv \| 207-175 \| 2017 \| 2017SSRv..207..175R \| http://ui.adsabs.harvard.edu/#abs/2017SSRv..207..175R Spectral characterization of the non-thermal X-ray emission of gamma-ray pulsars \|Coti Zelati, Francesco, Torres, Diego F., et al. \| MNRAS \| 492-1025 \| 2020 \| 2020MNRAS.492.1025C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.492.1025C 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	2011-09-15T02:08:08Z/2011-09-16T11:34:08Z
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	2012-10-15T00:00:00Z
Keywords	"psr j0357", "1e33 erg", "emission properties", "fermi mission", "XMM", "radio wavelengths", "chandra data unveiled", "pulsar emission properties", "luminosity erot", "xray counterpart", "gamma ray pulsar", "apparently protruding", "pulsar astronomy", "fermi pulsars", "gamma ray pulsations"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Andrea De Luca, 2012, 'The old', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8au2rux