K
K. S. Wood
Researcher at United States Naval Research Laboratory
Publications - 128
Citations - 23132
K. S. Wood is an academic researcher from United States Naval Research Laboratory. The author has contributed to research in topics: Fermi Gamma-ray Space Telescope & Pulsar. The author has an hindex of 69, co-authored 128 publications receiving 21224 citations.
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Journal ArticleDOI
The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission
W. B. Atwood,A. A. Abdo,A. A. Abdo,Markus Ackermann,W. Althouse,Brandon Anderson,Magnus Axelsson,Luca Baldini,Jean Ballet,David L. Band,Guido Barbiellini,Guido Barbiellini,J. Bartelt,Denis Bastieri,Denis Bastieri,B. M. Baughman,Keith Bechtol,D. Bédérède,F. Bellardi,Ronaldo Bellazzini,B. Berenji,Giovanni F. Bignami,Dario Bisello,Dario Bisello,Elisabetta Bissaldi,Roger Blandford,E. D. Bloom,J. R. Bogart,Emanuele Bonamente,Emanuele Bonamente,Jerry T. Bonnell,A. W. Borgland,A. Bouvier,Johan Bregeon,Alessandro Brez,M. Brigida,M. Brigida,P. Bruel,T. H. Burnett,G. Busetto,G. Busetto,G. A. Caliandro,G. A. Caliandro,R. A. Cameron,P. A. Caraveo,Staffan Carius,P. Carlson,J. M. Casandjian,E. Cavazzuti,M. Ceccanti,C. Cecchi,C. Cecchi,Eric Charles,A. Chekhtman,A. Chekhtman,C. C. Cheung,James Chiang,R. Chipaux,A. N. Cillis,Stefano Ciprini,Stefano Ciprini,R. Claus,Johann Cohen-Tanugi,S. Condamoor,Jan Conrad,Jan Conrad,Robin H. D. Corbet,L. Corucci,L. Costamante,S. Cutini,David S. Davis,David S. Davis,D. Decotigny,M. Deklotz,Charles D. Dermer,A. De Angelis,Seth Digel,E. Do Couto E Silva,Persis S. Drell,R. Dubois,D. Dumora,D. Dumora,Y. Edmonds,D. Fabiani,Christian Farnier,C. Favuzzi,C. Favuzzi,D. L. Flath,P. Fleury,W. B. Focke,Stefan Funk,P. Fusco,P. Fusco,F. Gargano,Dario Gasparrini,Neil Gehrels,Neil Gehrels,F.-X. Gentit,S. Germani,S. Germani,B. Giebels,Nicola Giglietto,Nicola Giglietto,Paolo Giommi,F. Giordano,F. Giordano,T. Glanzman,G. Godfrey,I. A. Grenier,M.-H. Grondin,M.-H. Grondin,J. E. Grove,L. Guillemot,L. Guillemot,S. Guiriec,Gunther Haller,Alice K. Harding,P. A. Hart,E. Hays,S. E. Healey,M. Hirayama,M. Hirayama,L. Hjalmarsdotter,R. Horn,R. E. Hughes,Gudlaugur Johannesson,G. Johansson,A. S. Johnson,R. P. Johnson,Tyrel J. Johnson,Tyrel J. Johnson,W. N. Johnson,T. Kamae,Hideaki Katagiri,Jun Kataoka,A. Kavelaars,Nobuyuki Kawai,H. Kelly,Matthew Kerr,Wlodzimierz Klamra,Jürgen Knödlseder,Martin Kocian,N. Komin,N. Komin,F. Kuehn,M. Kuss,D. Landriu,Luca Latronico,B. Lee,Shiu-Hang Lee,Marianne Lemoine-Goumard,Marianne Lemoine-Goumard,Andrea Lionetto,Andrea Lionetto,Francesco Longo,Francesco Longo,F. Loparco,F. Loparco,Benoit Lott,Benoit Lott,M. N. Lovellette,P. Lubrano,P. Lubrano,G. M. Madejski,A. Makeev,A. Makeev,B. Marangelli,B. Marangelli,M.M. Massai,M. N. Mazziotta,Julie McEnery,N. Menon,C. Meurer,Peter F. Michelson,Massimo Minuti,N. Mirizzi,N. Mirizzi,W. Mitthumsiri,Tsunefumi Mizuno,A. A. Moiseev,C. Monte,C. Monte,M. E. Monzani,Elena Moretti,Elena Moretti,A. Morselli,A. Morselli,Igor V. Moskalenko,S. Murgia,Takeshi Nakamori,Sho Nishino,P. L. Nolan,J. P. Norris,Eric Nuss,Masanori Ohno,T. Ohsugi,Nicola Omodei,E. Orlando,J. F. Ormes,Alessandro Paccagnella,Alessandro Paccagnella,David Paneque,J. H. Panetta,D. Parent,D. Parent,Mark Pearce,M. Pepe,M. Pepe,A. Perazzo,Melissa Pesce-Rollins,P. Picozza,P. Picozza,L. Pieri,Michele Pinchera,F. Piron,T. A. Porter,L. Poupard,S. Rainò,S. Rainò,Robert R. Rando,Robert R. Rando,E. Rapposelli,M. Razzano,A. Reimer,Olaf Reimer,T. Reposeur,T. Reposeur,L. C. Reyes,S. Ritz,S. Ritz,L. S. Rochester,A. Y. Rodriguez,Roger W. Romani,M. Roth,J. J. Russell,Felix Ryde,S. Sabatini,S. Sabatini,Hartmut Sadrozinski,David Sanchez,A. Sander,L. Sapozhnikov,P. M. Saz Parkinson,Jeffrey D. Scargle,T. L. Schalk,G. Scolieri,Carmelo Sgrò,Gerald H. Share,Gerald H. Share,M. S. Shaw,Takashi Shimokawabe,Chris Shrader,Agnieszka Sierpowska-Bartosik,E. J. Siskind,David A. Smith,David A. Smith,P. D. Smith,Gloria Spandre,P. Spinelli,P. Spinelli,Jean-Luc Starck,T. E. Stephens,M. S. Strickman,Andrew W. Strong,D. J. Suson,Hiroyasu Tajima,Hiromitsu Takahashi,Tadayuki Takahashi,Takaaki Tanaka,A. Tenze,S. Tether,J. B. Thayer,J. G. Thayer,D. J. Thompson,L. Tibaldo,L. Tibaldo,O. Tibolla,Diego F. Torres,Diego F. Torres,Gino Tosti,Gino Tosti,A. Tramacere,M. Turri,T. L. Usher,N. Vilchez,V. Vitale,V. Vitale,P. Wang,K. Watters,Brian L Winer,K. S. Wood,T. Ylinen,M. Ziegler +292 more
TL;DR: The Large Area Telescope (Fermi/LAT) as mentioned in this paper is the primary instrument on the Fermi Gamma-ray Space Telescope, which is an imaging, wide field-of-view, high-energy gamma-ray telescope, covering the energy range from below 20 MeV to more than 300 GeV.
Journal ArticleDOI
The second catalog of active galactic nuclei detected by the Fermi Large Area Telescope
Markus Ackermann,Marco Ajello,Alice Allafort,Elisa Antolini,Elisa Antolini,W. B. Atwood,Magnus Axelsson,Magnus Axelsson,Luca Baldini,Jean Ballet,Guido Barbiellini,Guido Barbiellini,Denis Bastieri,Denis Bastieri,Keith Bechtol,Ronaldo Bellazzini,B. Berenji,Roger Blandford,E. D. Bloom,Emanuele Bonamente,Emanuele Bonamente,A. W. Borgland,Eugenio Bottacini,A. Bouvier,Johan Bregeon,M. Brigida,M. Brigida,P. Bruel,R. Buehler,T. H. Burnett,S. Buson,S. Buson,G. A. Caliandro,R. A. Cameron,P. A. Caraveo,J. M. Casandjian,E. Cavazzuti,C. Cecchi,C. Cecchi,Eric Charles,C. C. Cheung,C. C. Cheung,James Chiang,Stefano Ciprini,R. Claus,Johann Cohen-Tanugi,Jan Conrad,Jan Conrad,L. Costamante,S. Cutini,A. De Angelis,F. de Palma,F. de Palma,Charles D. Dermer,Seth Digel,E. Do Couto E Silva,Persis S. Drell,R. Dubois,L. Escande,C. Favuzzi,C. Favuzzi,Stephen Fegan,Elizabeth C. Ferrara,Justin D. Finke,W. B. Focke,P. Fortin,M. Frailis,Yasushi Fukazawa,Stefan Funk,P. Fusco,P. Fusco,F. Gargano,Dario Gasparrini,Neil Gehrels,S. Germani,S. Germani,B. Giebels,Nicola Giglietto,Nicola Giglietto,Paolo Giommi,F. Giordano,F. Giordano,Marcello Giroletti,T. Glanzman,G. Godfrey,I. A. Grenier,J. E. Grove,Sylvain Guiriec,Mats Gustafsson,Daniela Hadasch,M. Hayashida,M. Hayashida,E. Hays,S. E. Healey,D. Horan,Xian Hou,R. E. Hughes,G. Iafrate,Gudlaugur Johannesson,A. S. Johnson,W. N. Johnson,T. Kamae,Hideaki Katagiri,Jun Kataoka,Jürgen Knödlseder,Jürgen Knödlseder,M. Kuss,J. Lande,S. Larsson,Luca Latronico,Francesco Longo,Francesco Longo,F. Loparco,F. Loparco,Benoit Lott,M. N. Lovellette,P. Lubrano,P. Lubrano,G. M. Madejski,M. N. Mazziotta,W. McConville,W. McConville,Julie McEnery,Julie McEnery,Peter F. Michelson,W. Mitthumsiri,Tsunefumi Mizuno,A. A. Moiseev,A. A. Moiseev,C. Monte,C. Monte,M. E. Monzani,E. Moretti,E. Moretti,A. Morselli,Igor V. Moskalenko,S. Murgia,Takeshi Nakamori,M. Naumann-Godo,P. L. Nolan,Jay P. Norris,E. Nuss,M. Ohno,T. Ohsugi,Akira Okumura,Nicola Omodei,M. Orienti,E. Orlando,J. F. Ormes,M. Ozaki,David Paneque,David Paneque,D. Parent,D. Parent,Melissa Pesce-Rollins,M. Pierbattista,Silvia Piranomonte,F. Piron,G. Pivato,T. A. Porter,S. Rainò,S. Rainò,Riccardo Rando,Riccardo Rando,M. Razzano,M. Razzano,Soebur Razzaque,A. Reimer,Olaf Reimer,Steven Ritz,L. S. Rochester,Roger W. Romani,M. Roth,Daniel Sánchez,C. Sbarra,Jeffrey D. Scargle,T. L. Schalk,Carmelo Sgrò,M. S. Shaw,E. J. Siskind,Gloria Spandre,P. Spinelli,P. Spinelli,Andrew W. Strong,D. J. Suson,Hiroyasu Tajima,Hiroyasu Tajima,Hiromitsu Takahashi,Tadayuki Takahashi,Takaaki Tanaka,J. G. Thayer,J. B. Thayer,D. J. Thompson,L. Tibaldo,L. Tibaldo,M. Tinivella,Diego F. Torres,Diego F. Torres,Gino Tosti,Gino Tosti,Eleonora Troja,Yasunobu Uchiyama,Justin Vandenbroucke,V. Vasileiou,Giacomo Vianello,V. Vitale,V. Vitale,A. P. Waite,E. Wallace,P. Wang,Brian L Winer,D. L. Wood,D. L. Wood,K. S. Wood,Stephan Zimmer +214 more
TL;DR: The second catalog of active galactic nuclei (AGNs) detected by the Fermi Large Area Telescope (LAT) in two years of scientific operation is presented in this article, which includes 1017 γ-ray sources located at high Galactic latitudes (|b| > 10°) that are detected with a test statistic (TS) greater than 25 and associated statistically with AGNs.
Journal ArticleDOI
Measurement of the Cosmic Ray e+ + e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope.
A. A. Abdo,Markus Ackermann,Marco Ajello,Magnus Axelsson,Luca Baldini,Jean Ballet,Guido Barbiellini,Denis Bastieri,M. Battelino,M. Battelino,B. M. Baughman,Keith Bechtol,Ronaldo Bellazzini,B. Berenji,Roger Blandford,Elliott D. Bloom,G. Bogaert,Emanuele Bonamente,A. W. Borgland,Johan Bregeon,A. Brez,M. Brigida,P. Bruel,T. H. Burnett,G. A. Caliandro,R. A. Cameron,P. A. Caraveo,P. Carlson,P. Carlson,J. M. Casandjian,Claudia Cecchi,E. Charles,A. Chekhtman,A. Chekhtman,C. C. Cheung,James Chiang,Stefano Ciprini,R. Claus,Johann Cohen-Tanugi,L. R. Cominsky,Jan Conrad,Jan Conrad,Jan Conrad,S. Cutini,Charles D. Dermer,A. De Angelis,F. de Palma,Seth Digel,G. Di Bernardo,E. Do Couto E Silva,Persis S. Drell,Richard Dubois,D. Dumora,Y. Edmonds,C. Farnier,C. Favuzzi,W. B. Focke,Marco Frailis,Yasushi Fukazawa,Stefan Funk,P. Fusco,Daniele Gaggero,F. Gargano,Dario Gasparrini,Neil Gehrels,Neil Gehrels,S. Germani,B. Giebels,Nicola Giglietto,F. Giordano,T. Glanzman,G.L. Godfrey,Dario Grasso,I. A. Grenier,M.-H. Grondin,J. E. Grove,L. Guillemot,Sylvain Guiriec,Y. Hanabata,Alice K. Harding,R. C. Hartman,M. Hayashida,E. Hays,R. E. Hughes,Gudlaugur Johannesson,A. S. Johnson,R. P. Johnson,W. N. Johnson,T. Kamae,Hideaki Katagiri,Jun Kataoka,N. Kawai,Matthew Kerr,Jürgen Knödlseder,Daniel Kocevski,F. Kuehn,M. Kuss,J. Lande,Luca Latronico,M. Lemoine-Goumard,Francesco Longo,F. Loparco,B. Lott,M. N. Lovellette,P. Lubrano,Grzegorz Madejski,A. Makeev,A. Makeev,M.M. Massai,M. N. Mazziotta,W. McConville,W. McConville,Julie McEnery,C. Meurer,Peter F. Michelson,W. Mitthumsiri,Tsunefumi Mizuno,A. A. Moiseev,A. A. Moiseev,C. Monte,M. E. Monzani,Elena Moretti,A. Morselli,Igor V. Moskalenko,S. Murgia,P. L. Nolan,J. P. Norris,E. Nuss,T. Ohsugi,Nicola Omodei,E. Orlando,J. F. Ormes,M. Ozaki,David Paneque,J. H. Panetta,D. Parent,V. Pelassa,M. Pepe,Melissa Pesce-Rollins,F. Piron,Martin Pohl,T. A. Porter,Stefano Profumo,S. Rainò,Riccardo Rando,M. Razzano,A. Reimer,Olaf Reimer,T. Reposeur,S. Ritz,S. Ritz,L.S. Rochester,A. Y. Rodriguez,Roger W. Romani,M. Roth,Felix Ryde,Felix Ryde,H. F.W. Sadrozinski,David Sánchez,A. Sander,P. M. Saz Parkinson,Jeffrey D. Scargle,T. Schalk,A. Sellerholm,Carmelo Sgrò,David Smith,P. D. Smith,Gloria Spandre,P. Spinelli,Jean-Luc Starck,T. E. Stephens,M. S. Strickman,Andrew W. Strong,D. J. Suson,H. Tajima,Hiromitsu Takahashi,Tadayuki Takahashi,Takaaki Tanaka,J. B. Thayer,J. G. Thayer,D. J. Thompson,L. Tibaldo,O. Tibolla,Diego F. Torres,G. Tosti,A. Tramacere,Yasunobu Uchiyama,T. L. Usher,A. van Etten,V. Vasileiou,V. Vasileiou,N. Vilchez,V. Vitale,A. P. Waite,E. Wallace,Paul J. Wang,Brian L Winer,K. S. Wood,T. Ylinen,T. Ylinen,T. Ylinen,M. Ziegler +201 more
TL;DR: In this article, the Fermi Large Area Telescope (Fermi LAT) was used to detect the electron spectrum up to 1 TeV using a diffusive model and a potential local extra component.
Journal ArticleDOI
The spectral energy distribution of fermi bright blazars
A. A. Abdo,A. A. Abdo,Markus Ackermann,Ivan Agudo,Marco Ajello,Hugh D. Aller,Margo F. Aller,Emmanouil Angelakis,A. A. Arkharov,Magnus Axelsson,Magnus Axelsson,Uwe Bach,Luca Baldini,Jean Ballet,Guido Barbiellini,Denis Bastieri,B. M. Baughman,Keith Bechtol,Ronaldo Bellazzini,Erika Benítez,Andrei Berdyugin,B. Berenji,Roger Blandford,E. D. Bloom,Markus Boettcher,Emanuele Bonamente,A. W. Borgland,Johan Bregeon,A. Brez,M. Brigida,P. Bruel,T. H. Burnett,David N. Burrows,S. Buson,G. A. Caliandro,L. Calzoletti,R. A. Cameron,M. Capalbi,P. A. Caraveo,D. Carosati,J. M. Casandjian,E. Cavazzuti,C. Cecchi,Omer Celik,Omer Celik,E. Charles,Sylvain Chaty,A. Chekhtman,A. Chekhtman,Wen Ping Chen,James Chiang,G. Chincarini,Stefano Ciprini,R. Claus,Johann Cohen-Tanugi,S. Colafrancesco,L. R. Cominsky,Jan Conrad,Jan Conrad,L. Costamante,S. Cutini,F. D'Ammando,R. Deitrick,V. D'Elia,Charles D. Dermer,A. De Angelis,F. de Palma,Seth Digel,I. Donnarumma,E. Do Couto E Silva,Persis S. Drell,R. Dubois,Deborah Dultzin,D. Dumora,A. D. Falcone,C. Farnier,C. Favuzzi,S. J. Fegan,W. B. Focke,E. Forné,P. Fortin,Marco Frailis,Lars Fuhrmann,Yasushi Fukazawa,Stefan Funk,P. Fusco,José L. Gómez,F. Gargano,Dario Gasparrini,Neil Gehrels,S. Germani,B. Giebels,Nicola Giglietto,Paolo Giommi,F. Giordano,A. Giuliani,T. Glanzman,G. Godfrey,I. A. Grenier,Caryl Gronwall,J. E. Grove,L. Guillemot,L. Guillemot,Sylvain Guiriec,Mark Gurwell,D. Hadasch,Y. Hanabata,Alice K. Harding,M. Hayashida,E. Hays,S. E. Healey,Jochen Heidt,David Hiriart,D. Horan,E. A. Hoversten,R. E. Hughes,Ryosuke Itoh,Miranda Jackson,Miranda Jackson,Gudlaugur Johannesson,A. S. Johnson,W. N. Johnson,Svetlana G. Jorstad,Matthias Kadler,T. Kamae,Hideaki Katagiri,Jun Kataoka,Nobuyuki Kawai,J. A. Kennea,Matthew Kerr,Givi N. Kimeridze,Jürgen Knödlseder,M. L. Kocian,E. N. Kopatskaya,Ekaterina Koptelova,Tatiana S. Konstantinova,Yuri Y. Kovalev,Yu. A. Kovalev,Omar M. Kurtanidze,M. Kuss,J. Lande,Valeri M. Larionov,Luca Latronico,Paolo Leto,Elina Lindfors,Francesco Longo,F. Loparco,Benoit Lott,M. N. Lovellette,P. Lubrano,Grzegorz Madejski,A. Makeev,A. Makeev,P. Marchegiani,Alan P. Marscher,F. E. Marshall,Walter Max-Moerbeck,M. N. Mazziotta,W. McConville,W. McConville,Julie McEnery,Julie McEnery,C. Meurer,Peter F. Michelson,W. Mitthumsiri,Tsunefumi Mizuno,A. A. Moiseev,A. A. Moiseev,C. Monte,M. E. Monzani,A. Morselli,Igor V. Moskalenko,S. Murgia,I. Nestoras,K. Nilsson,N. A. Nizhelsky,P. L. Nolan,J. P. Norris,E. Nuss,T. Ohsugi,Roopesh Ojha,Nicola Omodei,E. Orlando,Jonathan F. Ormes,J. P. Osborne,M. Ozaki,L. Pacciani,Paolo Padovani,C. Pagani,K. L. Page,David Paneque,J. H. Panetta,D. Parent,M. Pasanen,Vasiliki Pavlidou,V. Pelassa,M. Pepe,M. Perri,Melissa Pesce-Rollins,S. Piranomonte,F. Piron,C. Pittori,T. A. Porter,Simonetta Puccetti,Farid Rahoui,S. Rainò,C. M. Raiteri,Robert R. Rando,M. Razzano,A. Reimer,A. Reimer,Olaf Reimer,Olaf Reimer,T. Reposeur,Joseph L. Richards,Steven Ritz,L.S. Rochester,A. Y. Rodriguez,Roger W. Romani,J. A. Ros,M. Roth,P. Roustazadeh,Felix Ryde,Felix Ryde,H. F.W. Sadrozinski,A. C. Sadun,David Sánchez,A. Sander,P. M. Saz Parkinson,Jeffrey D. Scargle,A. Sellerholm,Carmelo Sgrò,M. S. Shaw,Lorand A. Sigua,E. J. Siskind,David A. Smith,P. D. Smith,Gloria Spandre,P. Spinelli,Jean-Luc Starck,Mark Stevenson,G. Stratta,M. S. Strickman,D. J. Suson,H. Tajima,Hiromitsu Takahashi,Tadayuki Takahashi,L. O. Takalo,Takaaki Tanaka,J. B. Thayer,J. G. Thayer,D. J. Thompson,L. Tibaldo,Diego F. Torres,Gino Tosti,A. Tramacere,A. Tramacere,Yasunobu Uchiyama,T. L. Usher,V. Vasileiou,V. Vasileiou,F. Verrecchia,N. Vilchez,M. Villata,V. Vitale,A. P. Waite,Paul J. Wang,Brian L Winer,K. S. Wood,T. Ylinen,T. Ylinen,J. A. Zensus,G. V. Zhekanis,M. Ziegler +273 more
Abstract: We have conducted a detailed investigation of the broadband spectral properties of the gamma-ray selected blazars of the Fermi LAT Bright AGN Sample (LBAS). By combining our accurately estimated Fermi gamma-ray spectra with Swift, radio, infra-red, optical, and other hard X-ray/gamma-ray data, collected within 3 months of the LBAS data taking period, we were able to assemble high-quality and quasi-simultaneous spectral energy distributions (SED) for 48 LBAS blazars. The SED of these gamma-ray sources is similar to that of blazars discovered at other wavelengths, clearly showing, in the usual log nu-log nu F-nu representation, the typical broadband spectral signatures normally attributed to a combination of low-energy synchrotron radiation followed by inverse Compton emission of one or more components. We have used these SED to characterize the peak intensity of both the low-and the high-energy components. The results have been used to derive empirical relationships that estimate the position of the two peaks from the broadband colors (i.e., the radio to optical, alpha(ro), and optical to X-ray, alpha(ox), spectral slopes) and from the gamma-ray spectral index. Our data show that the synchrotron peak frequency (nu(S)(peak)) is positioned between 10(12.5) and 10(14.5) Hz in broad-lined flat spectrum radio quasars (FSRQs) and between 10(13) and 10(17) Hz in featureless BL Lacertae objects. We find that the gamma-ray spectral slope is strongly correlated with the synchrotron peak energy and with the X-ray spectral index, as expected at first order in synchrotron-inverse Compton scenarios. However, simple homogeneous, one-zone, synchrotron self-Compton (SSC) models cannot explain most of our SED, especially in the case of FSRQs and low energy peaked (LBL) BL Lacs. More complex models involving external Compton radiation or multiple SSC components are required to reproduce the overall SED and the observed spectral variability. While more than 50% of known radio bright high energy peaked (HBL) BL Lacs are detected in the LBAS sample, only less than 13% of known bright FSRQs and LBL BL Lacs are included. This suggests that the latter sources, as a class, may be much fainter gamma-ray emitters than LBAS blazars, and could in fact radiate close to the expectations of simple SSC models. We categorized all our sources according to a new physical classification scheme based on the generally accepted paradigm for Active Galactic Nuclei and on the results of this SED study. Since the LAT detector is more sensitive to flat spectrum gamma-ray sources, the correlation between nu(S)(peak) and gamma-ray spectral index strongly favors the detection of high energy peaked blazars, thus explaining the Fermi overabundance of this type of sources compared to radio and EGRET samples. This selection effect is similar to that experienced in the soft X-ray band where HBL BL Lacs are the dominant type of blazars.
Journal ArticleDOI
PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
M. C. Miller,Frederick K. Lamb,Alexander J. Dittmann,Slavko Bogdanov,Zaven Arzoumanian,Keith C. Gendreau,Sebastien Guillot,Alice K. Harding,Wynn C. G. Ho,Wynn C. G. Ho,James M. Lattimer,Renee M. Ludlam,Simin Mahmoodifar,Simin Mahmoodifar,Sharon M. Morsink,Paul S. Ray,Tod E. Strohmayer,K. S. Wood,Teruaki Enoto,R. S. Foster,Takashi Okajima,Gregory Y. Prigozhin,Yang Soong +22 more
TL;DR: In this paper, the mass and radius of the isolated 205.53 Hz millisecond pulsar PSR J0030+0451 were estimated using a Bayesian inference approach to analyze its energy-dependent thermal X-ray waveform, which was observed using the Neutron Star Interior Composition Explorer (NICER).