D
David L. Kaplan
Researcher at University of Wisconsin–Milwaukee
Publications - 620
Citations - 29455
David L. Kaplan is an academic researcher from University of Wisconsin–Milwaukee. The author has contributed to research in topics: Pulsar & Murchison Widefield Array. The author has an hindex of 82, co-authored 590 publications receiving 25400 citations. Previous affiliations of David L. Kaplan include California Institute of Technology & Massachusetts Institute of Technology.
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Journal ArticleDOI
The Murchison widefield array: The square kilometre array precursor at low radio frequencies
Steven Tingay,Robert F. Goeke,Judd D. Bowman,David Emrich,Stephen M. Ord,Daniel A. Mitchell,Miguel F. Morales,T. Booler,Brian Crosse,Randall B. Wayth,Colin J. Lonsdale,S. E. Tremblay,D. Pallot,T. Colegate,Andreas Wicenec,Nadia Kudryavtseva,W. Arcus,David G. Barnes,Gianni Bernardi,Frank H. Briggs,S. Burns,John D. Bunton,Roger J. Cappallo,Brian E. Corey,Avinash A. Deshpande,Ludi deSouza,Bryan Gaensler,Lincoln J. Greenhill,Peter J. Hall,Bryna J. Hazelton,David Herne,Jacqueline N. Hewitt,Melanie Johnston-Hollitt,David L. Kaplan,Justin C. Kasper,B. B. Kincaid,R. Koenig,Eric Kratzenberg,Mervyn J. Lynch,Benjamin McKinley,Stephen R. McWhirter,Edward H. Morgan,Divya Oberoi,Joseph Pathikulangara,Thiagaraj Prabu,Ron Remillard,Alan E. E. Rogers,A. Roshi,Joseph E. Salah,Robert J. Sault,N. Udaya-Shankar,F. Schlagenhaufer,K. S. Srivani,Jamie Stevens,Ravi Subrahmanyan,M. Waterson,Rachel L. Webster,Alan R. Whitney,Andrew Williams,Christopher L. Williams,J. S. B. Wyithe +60 more
TL;DR: The Murchison Widefield Array (MWA) as discussed by the authors is one of three Square Kilometre Array Precursor telescopes and is located at the MUR-astronomy Observatory in Western Australia, a location chosen for its extremely low levels of radio frequency interference.
Journal ArticleDOI
The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies
Steven Tingay,Robert F. Goeke,Judd D. Bowman,David Emrich,Stephen M. Ord,Daniel A. Mitchell,Miguel F. Morales,Tom Booler,Brian Crosse,D. Pallot,Andreas Wicenec,W. Arcus,David G. Barnes,Gianni Bernardi,Frank H. Briggs,S. Burns,John D. Bunton,Roger J. Cappallo,T. Colegate,Brian E. Corey,Avinash A. Deshpande,L. deSouza,Bryan Gaensler,Lincoln J. Greenhill,J. Hall,Bryna J. Hazelton,David Herne,Jacqueline N. Hewitt,Melanie Johnston-Hollitt,David L. Kaplan,Justin C. Kasper,B. B. Kincaid,R. Koenig,Eric Kratzenberg,Colin J. Lonsdale,Mervyn J. Lynch,Benjamin McKinley,Stephen R. McWhirter,Edward H. Morgan,Divya Oberoi,Joseph Pathikulangara,Thiagaraj Prabu,Ron Remillard,Alan E. E. Rogers,A. Roshi,Joseph E. Salah,Robert J. Sault,N. Udaya-Shankar,F. Schlagenhaufer,K. S. Srivani,Jamie Stevens,Ravi Subrahmanyan,S. E. Tremblay,Randall B. Wayth,M. Waterson,Rachel L. Webster,Alan R. Whitney,Andrew Williams,Christopher L. Williams,J. S. B. Wyithe +59 more
TL;DR: The Murchison Widefield Array (MWA) as mentioned in this paper is one of three Square Kilometre Array Precursor telescopes and is located at the MUR-astronomy Observatory in Western Australia, a location chosen for its extremely low levels of radio frequency interference.
Journal ArticleDOI
Illuminating gravitational waves: A concordant picture of photons from a neutron star merger
Mansi M. Kasliwal,Ehud Nakar,Leo Singer,Leo Singer,David L. Kaplan,David O. Cook,A. Van Sistine,R. M. Lau,Christoffer Fremling,Ore Gottlieb,Jacob E. Jencson,Scott M. Adams,U. Feindt,Kenta Hotokezaka,Sourav Ghosh,Daniel A. Perley,Po-Chieh Yu,Tsvi Piran,James R. Allison,James R. Allison,G. C. Anupama,Arvind Balasubramanian,Keith W. Bannister,John Bally,Jennifer Barnes,Sudhanshu Barway,Eric C. Bellm,Varun Bhalerao,Deb Sankar Bhattacharya,Nadejda Blagorodnova,Joshua S. Bloom,Joshua S. Bloom,Patrick Brady,Chris Cannella,Deep Chatterjee,S. B. Cenko,S. B. Cenko,B. E. Cobb,Chris M. Copperwheat,A. Corsi,Kaushik De,Dougal Dobie,Dougal Dobie,Dougal Dobie,S. W. K. Emery,Phil Evans,Ori D. Fox,Dale A. Frail,C. Frohmaier,C. Frohmaier,Ariel Goobar,Gregg Hallinan,Fiona A. Harrison,George Helou,Tanja Hinderer,Anna Y. Q. Ho,Assaf Horesh,Wing-Huen Ip,Ryosuke Itoh,Daniel Kasen,Hyesook Kim,N. P. M. Kuin,Thomas Kupfer,Christene Lynch,Christene Lynch,K. K. Madsen,Paolo A. Mazzali,Paolo A. Mazzali,Adam A. Miller,Adam A. Miller,Kunal Mooley,Tara Murphy,Tara Murphy,Chow-Choong Ngeow,David A. Nichols,Samaya Nissanke,Peter Nugent,Peter Nugent,Eran O. Ofek,H. Qi,Robert M. Quimby,Robert M. Quimby,Stephan Rosswog,Florin Rusu,Elaine M. Sadler,Elaine M. Sadler,Patricia Schmidt,Jesper Sollerman,Iain A. Steele,A. R. Williamson,Y. Xu,Lin Yan,Yoichi Yatsu,C. Zhang,Weijie Zhao +94 more
TL;DR: It is demonstrated that merging neutron stars are a long-sought production site forging heavy elements by r-process nucleosynthesis, which is dissimilar to classical short gamma-ray bursts with ultrarelativistic jets.
Journal ArticleDOI
wsclean: an implementation of a fast, generic wide-field imager for radio astronomy
A. R. Offringa,Benjamin McKinley,Natasha Hurley-Walker,Frank H. Briggs,Randall B. Wayth,Randall B. Wayth,David L. Kaplan,Martin Bell,Martin Bell,Lu Feng,Abraham R. Neben,J. D. Hughes,J. Rhee,Tara Murphy,Tara Murphy,N. D. R. Bhat,Gianni Bernardi,Judd D. Bowman,Roger J. Cappallo,Brian E. Corey,Avinash A. Deshpande,David Emrich,Aaron Ewall-Wice,Bryan Gaensler,Bryan Gaensler,Robert F. Goeke,Lincoln J. Greenhill,Bryna J. Hazelton,Luke Hindson,Melanie Johnston-Hollitt,Daniel C. Jacobs,Justin C. Kasper,Justin C. Kasper,Eric Kratzenberg,Emil Lenc,Emil Lenc,Colin J. Lonsdale,Mervyn J. Lynch,Stephen R. McWhirter,Daniel A. Mitchell,Daniel A. Mitchell,Miguel F. Morales,Edward H. Morgan,Nadia Kudryavtseva,Divya Oberoi,Stephen M. Ord,Stephen M. Ord,Bartosz Pindor,Pietro Procopio,Thiagaraj Prabu,J. Riding,D. A. Roshi,N. Udaya Shankar,K. S. Srivani,Ravi Subrahmanyan,Ravi Subrahmanyan,Steven Tingay,Steven Tingay,Mark Waterson,Mark Waterson,Rachel L. Webster,Rachel L. Webster,Alan R. Whitney,Andrew Williams,Christopher L. Williams +64 more
TL;DR: In this article, the authors present a wide-field interferometric imager that uses the w-stacking algorithm and can make use of the W-snapshot algorithm, which is an order of magnitude faster than w-projection, as well as being capable of full-sky imaging at full resolution with correct polarization correction.
Journal ArticleDOI
The Zwicky Transient Facility: Science Objectives
Matthew J. Graham,Shrinivas R. Kulkarni,Eric C. Bellm,Scott M. Adams,Cristina Barbarino,Nadejda Blagorodnova,Dennis Bodewits,Bryce Bolin,Patrick Brady,S. Bradley Cenko,Chan-Kao Chang,Michael W. Coughlin,Kaushik De,Gwendolyn Eadie,Tony L. Farnham,Ulrich Feindt,Anna Franckowiak,Christoffer Fremling,Avishay Gal-Yam,Suvi Gezari,Sourav Ghosh,Daniel A. Goldstein,V. Zach Golkhou,Ariel Goobar,Anna Y. Q. Ho,Daniela Huppenkothen,Zeljko Ivezic,R. Lynne Jones,Mario Juric,David L. Kaplan,Mansi M. Kasliwal,Michael S. P. Kelley,Thomas Kupfer,Chien-De Lee,Hsing Wen Lin,Ragnhild Lunnan,Ashish Mahabal,Adam A. Miller,Chow-Choong Ngeow,Peter Nugent,Eran O. Ofek,Thomas A. Prince,L. Rauch,Jan van Roestel,Steve Schulze,Leo Singer,Jesper Sollerman,Francesco Taddia,Lin Yan,Quanzhi Ye,Po-Chieh Yu,Igor Andreoni,Tom A. Barlow,James M. Bauer,Ron Beck,Justin Belicki,Rahul Biswas,V. Brinnel,Tim Brooke,Brian D. Bue,Mattia Bulla,Kevin B. Burdge,Rick Burruss,Andrew J. Connolly,John Cromer,Virginia Cunningham,Richard Dekany,Alex Delacroix,Vandana Desai,Dmitry A. Duev,Eugean Hacopians,David Hale,George Helou,John Henning,David Hover,Lynne A. Hillenbrand,Justin Howell,Tiara Hung,David Imel,Wing-Huen Ip,Edward Jackson,Shai Kaspi,Stephen Kaye,Marek Kowalski,Emily Kramer,Michael A. Kuhn,Walter Landry,Russ R. Laher,Peter H. Mao,Frank J. Masci,Serge Monkewitz,Patrick J. Murphy,J. Nordin,Maria T. Patterson,Bryan E. Penprase,Michael Porter,Umaa Rebbapragada,Daniel J. Reiley,Reed Riddle,Mickael Rigault,Hector P. Rodriguez,Ben Rusholme,J. V. Santen,David L. Shupe,Roger M. H. Smith,Maayane T. Soumagnac,Robert Stein,Jason Surace,Paula Szkody,Scott Terek,Angela Van Sistine,Sjoert van Velzen,W. Thomas Vestrand,Richard Walters,Charlotte Ward,Chaoran Zhang,Jeffry Zolkower +116 more
TL;DR: The Zwicky Transient Facility (ZTF) as discussed by the authors is a new time domain survey employing a dedicated camera on the Palomar 48-inch Schmidt telescope with a 47 deg$^2$ field of view and 8 second readout time.