FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3098491639> ?p ?o ?g. }

• W3098491639 endingPage "A44" @default.
• W3098491639 startingPage "A44" @default.
• W3098491639 abstract "Context: GeV gamma-ray pulsations from over 140 pulsars have been characterized using the Fermi Large Area Telescope, enabling improved understanding of the emission regions within the neutron star magnetospheres, and the contributions of pulsars to high energy electrons and diffuse gamma rays in the Milky Way. The first gamma-ray pulsars to be detected were the most intense and/or those with narrow pulses. Aims: As the Fermi mission progresses, progressively fainter objects can be studied. In addition to more distant pulsars (thus probing a larger volume of the Galaxy), or ones in high background regions (thus improving the sampling uniformity across the Galactic plane), we detect pulsars with broader pulses or lower luminosity. Adding pulsars to our catalog with inclination angles that are rare in the observed sample, and/or with lower spindown power, will reduce the bias in the currently known gamma-ray pulsar population. Methods: We use rotation ephemerides derived from radio observations to phase-fold gamma rays recorded by the Fermi Large Area Telescope, to then determine the pulse profile properties. Spectral analysis provides the luminosities and, when the signal-to-noise ratio allows, the cutoff energies. We constrain the pulsar distances by different means in order to minimize the luminosity uncertainties. Results: We present six new gamma-ray pulsars with an eclectic mix of properties. Three are young, and three are recycled. They include the farthest, the lowest power, two of the highest duty-cycle pulsars seen, and only the fourth young gamma-ray pulsar with a radio interpulse. We discuss the biases existing in the current gamma-ray pulsar catalog, and steps to be taken to mitigate the bias." @default.
• W3098491639 created "2020-11-23" @default.
• W3098491639 creator A5003133702 @default.
• W3098491639 creator A5006134581 @default.
• W3098491639 creator A5016391781 @default.
• W3098491639 creator A5020716271 @default.
• W3098491639 creator A5030103540 @default.
• W3098491639 creator A5034510030 @default.
• W3098491639 creator A5037300172 @default.
• W3098491639 creator A5045533942 @default.
• W3098491639 creator A5047474127 @default.
• W3098491639 creator A5054081345 @default.
• W3098491639 creator A5058309297 @default.
• W3098491639 creator A5065846192 @default.
• W3098491639 creator A5077493826 @default.
• W3098491639 creator A5091186797 @default.
• W3098491639 date "2014-10-01" @default.
• W3098491639 modified "2023-10-18" @default.
• W3098491639 title "Six faint gamma-ray pulsars seen with theFermiLarge Area Telescope" @default.
• W3098491639 cites W1523127772 @default.
• W3098491639 cites W1564915826 @default.
• W3098491639 cites W1607720132 @default.
• W3098491639 cites W1891457057 @default.
• W3098491639 cites W1895340151 @default.
• W3098491639 cites W1968304054 @default.
• W3098491639 cites W1973285267 @default.
• W3098491639 cites W1973820399 @default.
• W3098491639 cites W1975382763 @default.
• W3098491639 cites W1989894077 @default.
• W3098491639 cites W1996788380 @default.
• W3098491639 cites W1999892386 @default.
• W3098491639 cites W2010835546 @default.
• W3098491639 cites W2016178642 @default.
• W3098491639 cites W2019741049 @default.
• W3098491639 cites W2028991506 @default.
• W3098491639 cites W2029623000 @default.
• W3098491639 cites W2030974231 @default.
• W3098491639 cites W2044661517 @default.
• W3098491639 cites W2052270969 @default.
• W3098491639 cites W2052926897 @default.
• W3098491639 cites W2057634812 @default.
• W3098491639 cites W2058610559 @default.
• W3098491639 cites W2071024667 @default.
• W3098491639 cites W2074148045 @default.
• W3098491639 cites W2089679482 @default.
• W3098491639 cites W2091836325 @default.
• W3098491639 cites W2100696415 @default.
• W3098491639 cites W2106662526 @default.
• W3098491639 cites W2109942349 @default.
• W3098491639 cites W2110614149 @default.
• W3098491639 cites W2112353369 @default.
• W3098491639 cites W2112494265 @default.
• W3098491639 cites W2128609127 @default.
• W3098491639 cites W2137533160 @default.
• W3098491639 cites W2147288423 @default.
• W3098491639 cites W2148103048 @default.
• W3098491639 cites W2155930460 @default.
• W3098491639 cites W2167277890 @default.
• W3098491639 cites W2167727712 @default.
• W3098491639 cites W2170852626 @default.
• W3098491639 cites W3098380171 @default.
• W3098491639 cites W3099830973 @default.
• W3098491639 cites W3102749679 @default.
• W3098491639 cites W3102926480 @default.
• W3098491639 cites W3103290940 @default.
• W3098491639 cites W3105430980 @default.
• W3098491639 cites W3106110599 @default.
• W3098491639 cites W3106263174 @default.
• W3098491639 cites W3121848060 @default.
• W3098491639 cites W4292403095 @default.
• W3098491639 doi "https://doi.org/10.1051/0004-6361/201424294" @default.
• W3098491639 hasPublicationYear "2014" @default.
• W3098491639 type Work @default.
• W3098491639 sameAs 3098491639 @default.
• W3098491639 citedByCount "19" @default.
• W3098491639 countsByYear W30984916392015 @default.
• W3098491639 countsByYear W30984916392016 @default.
• W3098491639 countsByYear W30984916392017 @default.
• W3098491639 countsByYear W30984916392018 @default.
• W3098491639 countsByYear W30984916392019 @default.
• W3098491639 countsByYear W30984916392020 @default.
• W3098491639 countsByYear W30984916392021 @default.
• W3098491639 countsByYear W30984916392023 @default.
• W3098491639 crossrefType "journal-article" @default.
• W3098491639 hasAuthorship W3098491639A5003133702 @default.
• W3098491639 hasAuthorship W3098491639A5006134581 @default.
• W3098491639 hasAuthorship W3098491639A5016391781 @default.
• W3098491639 hasAuthorship W3098491639A5020716271 @default.
• W3098491639 hasAuthorship W3098491639A5030103540 @default.
• W3098491639 hasAuthorship W3098491639A5034510030 @default.
• W3098491639 hasAuthorship W3098491639A5037300172 @default.
• W3098491639 hasAuthorship W3098491639A5045533942 @default.
• W3098491639 hasAuthorship W3098491639A5047474127 @default.
• W3098491639 hasAuthorship W3098491639A5054081345 @default.
• W3098491639 hasAuthorship W3098491639A5058309297 @default.
• W3098491639 hasAuthorship W3098491639A5065846192 @default.
• W3098491639 hasAuthorship W3098491639A5077493826 @default.
• W3098491639 hasAuthorship W3098491639A5091186797 @default.

• next