Publication:
Einstein@Home discovers a radio-quiet gamma-ray millisecond pulsar

Simple item page
dc.contributor.authorColin J. Clarken_US
dc.contributor.authorHolger J. Pletschen_US
dc.contributor.authorJason Wuen_US
dc.contributor.authorLucas Guillemoten_US
dc.contributor.authorMatthew Kerren_US
dc.contributor.authorTyrel J. Johnsonen_US
dc.contributor.authorFernando Camiloen_US
dc.contributor.authorDavid Salvettien_US
dc.contributor.authorBruce Allenen_US
dc.contributor.authorDavid Andersonen_US
dc.contributor.authorCarsten Aulberten_US
dc.contributor.authorChristian Beeren_US
dc.contributor.authorOliver Bocken_US
dc.contributor.authorAndres Cuéllaren_US
dc.contributor.authorHeinz Bernd Eggensteinen_US
dc.contributor.authorHenning Fehrmannen_US
dc.contributor.authorMichael Krameren_US
dc.contributor.authorShawn A. Kwangen_US
dc.contributor.authorBernd MacHenschalken_US
dc.contributor.authorLars Niederen_US
dc.contributor.authorMarkus Ackermannen_US
dc.contributor.authorMarco Ajelloen_US
dc.contributor.authorLuca Baldinien_US
dc.contributor.authorJean Balleten_US
dc.contributor.authorGuido Barbiellinien_US
dc.contributor.authorDenis Bastierien_US
dc.contributor.authorRonaldo Bellazzinien_US
dc.contributor.authorElisabetta Bissaldien_US
dc.contributor.authorRoger D. Blandforden_US
dc.contributor.authorElliott D. Bloomen_US
dc.contributor.authorRaffaella Boninoen_US
dc.contributor.authorEugenio Bottacinien_US
dc.contributor.authorTerri J. Brandten_US
dc.contributor.authorJohan Bregeonen_US
dc.contributor.authorPhilippe Bruelen_US
dc.contributor.authorRolf Buehleren_US
dc.contributor.authorToby H. Burnetten_US
dc.contributor.authorSara Busonen_US
dc.contributor.authorRob A. Cameronen_US
dc.contributor.authorRegina Caputoen_US
dc.contributor.authorPatrizia A. Caraveoen_US
dc.contributor.authorElisabetta Cavazzutien_US
dc.contributor.authorClaudia Cecchien_US
dc.contributor.authorEric Charlesen_US
dc.contributor.authorAlexandre Chekhtmanen_US
dc.contributor.authorStefano Ciprinien_US
dc.contributor.authorLynn R. Cominskyen_US
dc.contributor.authorDenise Costantinen_US
dc.contributor.authorSara Cutinien_US
dc.contributor.authorFilippo D'Ammandoen_US
dc.contributor.authorAndrea De Lucaen_US
dc.contributor.authorRachele Desianteen_US
dc.contributor.authorLeonardo Di Venereen_US
dc.contributor.authorMattia Di Mauroen_US
dc.contributor.authorNiccolò Di Lallaen_US
dc.contributor.authorSeth W. Digelen_US
dc.contributor.authorCecilia Favuzzien_US
dc.contributor.authorElizabeth C. Ferraraen_US
dc.contributor.authorAnna Franckowiaken_US
dc.contributor.authorYasushi Fukazawaen_US
dc.contributor.authorStefan Funken_US
dc.contributor.authorPiergiorgio Fuscoen_US
dc.contributor.authorFabio Garganoen_US
dc.contributor.authorDario Gasparrinien_US
dc.contributor.authorNico Gigliettoen_US
dc.contributor.authorFrancesco Giordanoen_US
dc.contributor.authorMarcello Girolettien_US
dc.contributor.authorGermán A. Gomez-Vargasen_US
dc.contributor.authorDavid Greenen_US
dc.contributor.authorIsabelle A. Grenieren_US
dc.contributor.authorSylvain Guiriecen_US
dc.contributor.authorAlice K. Hardingen_US
dc.contributor.authorJohn W. Hewitten_US
dc.contributor.authorDeirdre Horanen_US
dc.contributor.authorGuolaugur Jóhannessonen_US
dc.contributor.authorShiki Kenseien_US
dc.contributor.authorMichael Kussen_US
dc.contributor.authorGiovanni La Muraen_US
dc.contributor.authorStefan Larssonen_US
dc.contributor.authorLuca Latronicoen_US
dc.contributor.authorJian Lien_US
dc.contributor.authorFrancesco Longoen_US
dc.contributor.authorFrancesco Loparcoen_US
dc.contributor.authorMichael N. Lovelletteen_US
dc.contributor.authorPasquale Lubranoen_US
dc.contributor.authorJeffrey D. Magillen_US
dc.contributor.authorSimone Malderaen_US
dc.contributor.authorAlberto Manfredaen_US
dc.contributor.authorMario N. Mazziottaen_US
dc.contributor.authorJulie E. McEneryen_US
dc.contributor.authorPeter F. Michelsonen_US
dc.contributor.authorNestor Mirabalen_US
dc.contributor.authorWarit Mitthumsirien_US
dc.contributor.authorTsunefumi Mizunoen_US
dc.contributor.authorMaria Elena Monzanien_US
dc.contributor.authorAldo Morsellien_US
dc.contributor.authorIgor V. Moskalenkoen_US
dc.contributor.authorEric Nussen_US
dc.contributor.authorTakashi Ohsugien_US
dc.contributor.authorNicola Omodeien_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Triesteen_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Perugiaen_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Barien_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergataen_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Torinoen_US
dc.contributor.otherIstituto Nazionale di Fisica Nucleare, Sezione di Pisaen_US
dc.contributor.otherSquare Kilometre Array, South Africaen_US
dc.contributor.otherIstituto Nazionale Di Fisica Nucleare, Sezione di Padovaen_US
dc.contributor.otherLaboratoire Univers et Particules de Montpellieren_US
dc.contributor.otherLaboratoire Leprince-Ringueten_US
dc.contributor.otherScuola Universitaria Superiore IUSS di Paviaen_US
dc.contributor.otherKavli Institute for Particle Astrophysics and Cosmologyen_US
dc.contributor.otherINAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milanen_US
dc.contributor.otherUniversity Science Institute Reykjaviken_US
dc.contributor.otherAgenzia Spaziale Italianaen_US
dc.contributor.otherHiroshima Universityen_US
dc.contributor.otherDeutsches Elektronen-Synchrotron (DESY)en_US
dc.contributor.otherUniversite d'Orleansen_US
dc.contributor.otherPontificia Universidad Católica de Chileen_US
dc.contributor.otherSpace Sciences Laboratory at UC Berkeleyen_US
dc.contributor.otherUniversità di Pisaen_US
dc.contributor.otherAlma Mater Studiorum Università di Bolognaen_US
dc.contributor.otherNaval Research Laboratoryen_US
dc.contributor.otherClemson Universityen_US
dc.contributor.otherNordisk Institut for Teoretisk Atomtysiken_US
dc.contributor.otherUniversità degli Studi di Udineen_US
dc.contributor.otherUniversitat Autònoma de Barcelonaen_US
dc.contributor.otherUniversità degli Studi di Barien_US
dc.contributor.otherUniversity of Marylanden_US
dc.contributor.otherUniversity of Wisconsin-Milwaukeeen_US
dc.contributor.otherInstitut National des Sciences de l'Universen_US
dc.contributor.otherUniversità degli Studi di Triesteen_US
dc.contributor.otherGeorge Mason University, Fairfax Campusen_US
dc.contributor.otherUniversity of Washington, Seattleen_US
dc.contributor.otherSonoma State Universityen_US
dc.contributor.otherMahidol Universityen_US
dc.contributor.otherIstituto Di Radioastronomia, Bolognaen_US
dc.contributor.otherUniversità degli Studi di Torinoen_US
dc.contributor.otherMax Planck Institute for Gravitational Physics (Albert Einstein Institute)en_US
dc.contributor.otherNASA Goddard Space Flight Centeren_US
dc.contributor.otherUniversite Paris 7- Denis Dideroten_US
dc.contributor.otherGottfried Wilhelm Leibniz Universitäten_US
dc.contributor.otherUniversity of Manchesteren_US
dc.contributor.otherGeorge Washington Universityen_US
dc.contributor.otherUniversità degli Studi di Perugiaen_US
dc.contributor.otherThe Royal Institute of Technology (KTH)en_US
dc.contributor.otherMax Planck Institut für Radioastronomieen_US
dc.contributor.otherFriedrich-Alexander-Universität Erlangen-Nürnbergen_US
dc.contributor.otherUniversità degli Studi di Padovaen_US
dc.contributor.otherUniversity of North Floridaen_US
dc.contributor.otherOskar Klein Centre for Cosmoparticle Physicsen_US
dc.date.accessioned2019-08-28T07:13:39Z
dc.date.available2019-08-28T07:13:39Z
dc.date.issued2018-02-28en_US
dc.description.abstract© 2018 The Authors,some rights reserved. Millisecond pulsars (MSPs) are old neutron stars that spin hundreds of times per second and appear to pulsate as their emission beams cross our line of sight. To date,radio pulsations have been detected from all rotation-powered MSPs. In an attempt to discover radio-quiet gamma-ray MSPs,we used the aggregated power from the computers of tens of thousands of volunteers participating in the Einstein@Home distributed computing project to search for pulsations from unidentified gamma-ray sources in Fermi Large Area Telescope data. This survey discovered two isolated MSPs,one of which is the only known rotation-powered MSP to remain undetected in radio observations. These gamma-ray MSPs were discovered in completely blind searches without prior constraints from other observations,raising hopes for detecting MSPs from a predicted Galactic bulge population.en_US
dc.identifier.citationScience Advances. Vol.4, No.2 (2018)en_US
dc.identifier.doi10.1126/sciadv.aao7228en_US
dc.identifier.issn23752548en_US
dc.identifier.other2-s2.0-85044781385en_US
dc.identifier.urihttps://repository.li.mahidol.ac.th/handle/20.500.14594/47531
dc.rightsMahidol Universityen_US
dc.rights.holderSCOPUSen_US
dc.source.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85044781385&origin=inwarden_US
dc.subjectMultidisciplinaryen_US
dc.titleEinstein@Home discovers a radio-quiet gamma-ray millisecond pulsaren_US
dc.typeArticleen_US
dspace.entity.typePublication
mu.datasource.scopushttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85044781385&origin=inwarden_US

Files

Collections

Scopus 2018