S
Subo Dong
Researcher at Peking University
Publications - 334
Citations - 18263
Subo Dong is an academic researcher from Peking University. The author has contributed to research in topics: Gravitational microlensing & Light curve. The author has an hindex of 71, co-authored 318 publications receiving 16344 citations. Previous affiliations of Subo Dong include Princeton University & Ohio State University.
Papers
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Journal ArticleDOI
The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0
Christopher S. Kochanek,Benjamin J. Shappee,Krzysztof Z. Stanek,Thomas W.-S. Holoien,Todd A. Thompson,J. L. Prieto,J. L. Prieto,Subo Dong,J. V. Shields,D. Will,C. A. Britt,D. Perzanowski,G. Pojmanski +12 more
TL;DR: In this paper, the authors describe a web interface that provides an up-to-date aperture photometry light curve for any user-selected sky coordinate, which can only be used for small samples of objects.
Journal ArticleDOI
Frequency of solar-like systems and of ice and gas giants beyond the snow line from high-magnification microlensing events in 2005-2008
Andrew Gould,Subo Dong,B. S. Gaudi,Andrzej Udalski,Ian A. Bond,J. G. Greenhill,Rachel Street,Martin Dominik,Takahiro Sumi,Michał K. Szymański,C. Han,William H. Allen,Greg Bolt,M. Bos,G. W. Christie,Darren L. DePoy,Jack D. Drummond,Jason D. Eastman,Avishay Gal-Yam,D. Higgins,J. Janczak,Shai Kaspi,Szymon Kozłowski,C.-U. Lee,F. Mallia,Anaëlle Maury,D. Maoz,Jennie McCormick,L. A. G. Monard,D. Moorhouse,N. D. Morgan,Tim Natusch,Eran O. Ofek,Byeong-Gon Park,Richard W. Pogge,David Polishook,R. Santallo,Avi Shporer,O. Spector,G. Thornley,Jennifer C. Yee,M. Kubiak,Grzegorz Pietrzyński,Igor Soszyński,O. Szewczyk,Łukasz Wyrzykowski,Krzysztof Ulaczyk,Radosław Poleski,Fumio Abe,David P. Bennett,C. S. Botzler,D. Douchin,M. Freeman,Akihiko Fukui,K. Furusawa,John B. Hearnshaw,S. Hosaka,Yoshitaka Itow,K. Kamiya,P. M. Kilmartin,A. Korpela,W. Lin,C. H. Ling,S. Makita,Kimiaki Masuda,Yutaka Matsubara,N. Miyake,Yasushi Muraki,M. Nagaya,K. Nishimoto,Kouji Ohnishi,Teppei Okumura,Y. C. Perrott,L. Philpott,Nicholas J. Rattenbury,To. Saito,Takashi Sako,Denis J. Sullivan,W. L. Sweatman,P. J. Tristram,E. von Seggern,P. C. M. Yock,Michael D. Albrow,V. Batista,J. P. Beaulieu,S. Brillant,J. Caldwell,J. J. Calitz,Arnaud Cassan,Andrew A. Cole,K. W. Cook,C. Coutures,S. Dieters,D. Dominis Prester,J. Donatowicz,Pascal Fouqué,K. Hill,M. Hoffman,Francisco Jablonski,Stephen R. Kane,N. Kains,D. Kubas,J.-B. Marquette,R. M. Martin,Eder Martioli,P. J. Meintjes,J. Menzies,Ettore Pedretti,K. R. Pollard,K. C. Sahu,C. Vinter,J. Wambsganss,R. A. Watson,Andrew Williams,M. Zub,Alasdair Allan,M. F. Bode,D. M. Bramich,Martin Burgdorf,N. Clay,S. Fraser,E. Hawkins,Keith Horne,E. Kerins,T. A. Lister,C. Mottram,E. S. Saunders,Colin Snodgrass,Iain A. Steele,Yiannis Tsapras,U. G. Jørgensen,Timo Anguita,Valerio Bozza,S. Calchi Novati,K. Harpsøe,Tobias C. Hinse,M. Hundertmark,P. Kjærgaard,C. Liebig,C. Liebig,Luigi Mancini,G. Masi,M. Mathiasen,Sohrab Rahvar,Davide Ricci,Gaetano Scarpetta,John Southworth,Jean Surdej,Christina C. Thöne,Christina C. Thöne +149 more
TL;DR: In this paper, the authors presented the first measurement of the planet frequency beyond the "snow line," for the planet-to-star mass-ratio interval during 2005-2008 microlensing events during the survey-plus-follow-up high-magnification channel.
Journal ArticleDOI
Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing
B. S. Gaudi,David P. Bennett,Andrzej Udalski,Andrew Gould,G. W. Christie,D. Maoz,Subo Dong,Jennie McCormick,Michał K. Szymański,P. J. Tristram,S. Nikolaev,Bohdan Paczynski,M. Kubiak,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Igor Soszyński,O. Szewczyk,Krzysztof Ulaczyk,Łukasz Wyrzykowski,Łukasz Wyrzykowski,Darren L. DePoy,C. Han,Shai Kaspi,C.-U. Lee,F. Mallia,Tim Natusch,Richard W. Pogge,Byeong-Gon Park,Fumio Abe,Ian A. Bond,C. S. Botzler,Akihiko Fukui,John B. Hearnshaw,Yoshitaka Itow,Kisaku Kamiya,A. V. Korpela,P. M. Kilmartin,W. Lin,Kimiaki Masuda,Yutaka Matsubara,M. Motomura,Yasushi Muraki,Shota Nakamura,Teppei Okumura,Kouji Ohnishi,Nicholas J. Rattenbury,Takashi Sako,To. Saito,Shuji Sato,L. Skuljan,Denis J. Sullivan,Takahiro Sumi,Winston L. Sweatman,Philip Yock,Michael D. Albrow,Alasdair Allan,J.-P. Beaulieu,Martin Burgdorf,K. H. Cook,C. Coutures,Martin Dominik,S. Dieters,Pascal Fouqué,J. G. Greenhill,Keith Horne,Iain A. Steele,Yiannis Tsapras,Brian Chaboyer,A. Crocker,Stephan Frank,Bruce Macintosh +70 more
TL;DR: Two planets with masses that could not have been detected with other techniques are identified; their discovery from only six confirmed microlensing planet detections suggests that solar system analogs may be common.
Journal ArticleDOI
Six months of multiwavelength follow-up of the tidal disruption candidate asassn-14li and implied tde rates from asas-sn
Thomas W.-S. Holoien,Christopher S. Kochanek,J. L. Prieto,J. L. Prieto,Krzysztof Z. Stanek,Subo Dong,Benjamin J. Shappee,Dirk Grupe,J. S. Brown,U. Basu,John F. Beacom,D. Bersier,J. Brimacombe,A. B. Danilet,E. E. Falco,Zhen Guo,Jessy Jose,Gregory J. Herczeg,Feng Long,G. Pojmanski,G. V. Simonian,D. M. Szczygiel,Todd A. Thompson,John R. Thorstensen,R. M. Wagner,R. M. Wagner,Przemysław Woźniak +26 more
TL;DR: In this article, ground-based and Swift photometric and spectroscopic observations of the candidate tidal disruption event (TDE) ASASSN-14li, found at the center of PGC043234 (d'90 Mpc) by the All-Sky Automated Survey for SuperNovae (ASAS-SN).
Journal ArticleDOI
Microlens OGLE-2005-BLG-169 Implies That Cool Neptune-like Planets Are Common
Andrew Gould,Andrzej Udalski,Deokkeun An,David P. Bennett,A. Y. Zhou,Subo Dong,Nicholas J. Rattenbury,B. S. Gaudi,P. C. M. Yock,Ian A. Bond,G. W. Christie,Keith Horne,Joseph M. Anderson,Krzysztof Z. Stanek,Darren L. DePoy,C. Han,Jennie McCormick,Byeong-Gon Park,Richard W. Pogge,Shawn Poindexter,Igor Soszyński,Michał K. Szymański,M. Kubiak,Grzegorz Pietrzyński,O. Szewczyk,Łukasz Wyrzykowski,K. Ulaczyk,Bohdan Paczynski,D. M. Bramich,Colin Snodgrass,Iain A. Steele,Martin Burgdorf,M. F. Bode,C. S. Botzler,Shude Mao,S. C. Swaving +35 more
TL;DR: In this paper, the authors detect a Neptune mass ratio (q 8? 10-5) planetary companion to the lens star in the extremely high magnification (A ~ 800) microlensing event OGLE-2005-BLG-169.