A
András Pál
Researcher at Hungarian Academy of Sciences
Publications - 38
Citations - 1105
András Pál is an academic researcher from Hungarian Academy of Sciences. The author has contributed to research in topics: Light curve & Stars. The author has an hindex of 16, co-authored 38 publications receiving 936 citations. Previous affiliations of András Pál include Konkoly Thege Miklós Astronomical Institute & Eötvös Loránd University.
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Journal ArticleDOI
The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation
Jose Luis Ortiz,Pablo Santos-Sanz,Bruno Sicardy,G. Benedetti-Rossi,Diane Berard,Nicolás Morales,Rene Duffard,Felipe Braga-Ribas,Ulrich Hopp,C. Ries,Valerio Nascimbeni,Valerio Nascimbeni,Francesco Marzari,V. Granata,V. Granata,András Pál,Cs. Kiss,Theodor Pribulla,R. Komžík,Kamil Hornoch,Petr Pravec,Paolo Bacci,Martina Maestripieri,L. Nerli,L. Mazzei,Mauro Bachini,F. Martinelli,Giacomo Succi,F. Ciabattari,Herman Mikuz,A. Carbognani,B. Gaehrken,Stefano Mottola,S. Hellmich,F. L. Rommel,Estela Fernández-Valenzuela,A. Campo Bagatin,Stefan Cikota,Aleksandar Cikota,J. Lecacheux,Roberto Vieira-Martins,Julio Camargo,Marcelo Assafin,François Colas,Raoul Behrend,Josselin Desmars,E. Meza,Alvaro Alvarez-Candal,W. Beisker,A. R. Gomes-Júnior,B. E. Morgado,Françoise Roques,Frédéric Vachier,Jérôme Berthier,T. G. Mueller,José M. Madiedo,Ozan Ünsalan,Eda Sonbas,N. Karaman,O. Erece,D. T. Koseoglu,T. Ozisik,S. Kalkan,Yavuz Güney,Mohammad Shameoni Niaei,O. Satir,Cahit Yeşilyaprak,Ç. Püsküllü,Afşar Kabaş,Osman Demircan,J. Alikakos,Vassilis Charmandaris,Giuseppe Leto,J. M. Ohlert,J. M. Christille,Róbert Szakáts,A. Takácsné Farkas,E. Varga-Verebélyi,Gábor Marton,A. Marciniak,Przemyslaw Bartczak,Toni Santana-Ros,M. Butkiewicz-Bąk,Grzegorz Dudziński,Victor Ali-Lagoa,Kosmas Gazeas,L. Tzouganatos,N. Paschalis,V. Tsamis,Agustín Sánchez-Lavega,Santiago Pérez-Hoyos,Ricardo Hueso,J. C. Guirado,V. Peris,R. Iglesias-Marzoa +94 more
TL;DR: Observations from multiple Earth-based observatories of Haumea passing in front of a distant star (a multi-chord stellar occultation) report the presence of a ring with an opacity of 0.5, which constrains the three-dimensional orientation of Haumesa and its triaxial shape, which is inconsistent with a homogeneous body in hydrostatic equilibrium.
Journal ArticleDOI
“TNOs are Cool”: A survey of the trans-Neptunian region - IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel-PACS
Pablo Santos-Sanz,Emmanuel Lellouch,Sonia Fornasier,Cs. Kiss,András Pál,T. G. Müller,Esa Vilenius,John Stansberry,Michael Mommert,Audrey Delsanti,Audrey Delsanti,Michael Mueller,Nuno Peixinho,Florence Henry,Jose Luis Ortiz,Audrey Thirouin,S. Protopapa,Rene Duffard,N. Szalai,T. L. Lim,C. Ejeta,Paul Hartogh,Alan W. Harris,Miriam Rengel +23 more
TL;DR: In this article, a set of 15 scattered disk (SDOs) and detached objects, in terms of their size, albedo, and thermal properties, were characterized using a Monte-Carlo approach.
Journal ArticleDOI
TNOs are cool: A survey of the trans-Neptunian region. V. Physical characterization of 18 Plutinos using Herschel-PACS observations
Michael Mommert,Alan W. Harris,Cs. Kiss,András Pál,Pablo Santos-Sanz,John Stansberry,Audrey Delsanti,Audrey Delsanti,Esa Vilenius,T. G. Müller,Nuno Peixinho,Emmanuel Lellouch,N. Szalai,Florence Henry,Rene Duffard,Sonia Fornasier,Paul Hartogh,Michael Mueller,Michael Mueller,J. L. Ortiz,Silvia Protopapa,Miriam Rengel,Audrey Thirouin +22 more
TL;DR: In this article, the authors present a photometry of 18 Plutinos and determine sizes and albedos for these objects using thermal modeling, and analyze their results for correlations, draw conclusions on the Plutino size distribution, and compare to earlier results.
Journal ArticleDOI
Spin–orbit resonance, transit duration variation and possible secular perturbations in KOI‐13
Gy. M. Szabó,Gy. M. Szabó,András Pál,András Pál,Aliz Derekas,A. E. Simon,A. E. Simon,Tamás Szalai,László L. Kiss,László L. Kiss +9 more
TL;DR: In this paper, the authors analyzed publicly available Kepler Q2-Q3 short-cadence observations, revealing a continuous light variation with a period of Prot = 25.43 ± 0.05 h and a half-amplitude of 21 ppm, which is linked to stellar rotation.
Journal ArticleDOI
Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations
Wenxiong Li,Wenxiong Li,Xiaofeng Wang,Jozsef Vinko,Jozsef Vinko,Jun Mo,Griffin Hosseinzadeh,Griffin Hosseinzadeh,Griffin Hosseinzadeh,David J. Sand,Jujia Zhang,Han Lin,Tianmeng Zhang,Long Wang,Long Wang,Zhihao Chen,Danfeng Xiang,Liming Rui,Fang Huang,Fang Huang,Xue Li,Xiaojia Zhang,Linyi Li,E. Baron,James M. DerKacy,Xulin Zhao,Hanna Sai,Kaicheng Zhang,Kaicheng Zhang,Dale Andrew Howell,Dale Andrew Howell,Curtis McCully,Iair Arcavi,Iair Arcavi,Iair Arcavi,Stefano Valenti,Daichi Hiramatsu,Daichi Hiramatsu,J. Burke,J. Burke,A. Rest,A. Rest,Peter M. Garnavich,Brad E. Tucker,Gautham Narayan,Edward J. Shaya,S. Margheim,A. Zenteno,A. Villar,Georgios Dimitriadis,R. J. Foley,Yen-Chen Pan,David A. Coulter,Ori D. Fox,Saurabh Jha,D. O. Jones,Dan Kasen,Dan Kasen,Charles D. Kilpatrick,Anthony L. Piro,Adam G. Riess,Adam G. Riess,César Rojas-Bravo,Benjamin J. Shappee,Thomas W.-S. Holoien,Krzysztof Z. Stanek,Maria R. Drout,Katie Auchettl,Christopher S. Kochanek,J. S. Brown,Subhash Bose,D. Bersier,J. Brimacombe,Ping Chen,Subo Dong,S. Holmbo,J. A. Muñoz,Robert L. Mutel,R. S. Post,J. L. Prieto,J. V. Shields,D. Tallon,Todd A. Thompson,Patrick J. Vallely,Steven Villanueva,Stephen J. Smartt,K. W. Smith,K. C. Chambers,H. Flewelling,Mark E. Huber,E. A. Magnier,C. Z. Waters,A. S. B. Schultz,Joanna Bulger,T. B. Lowe,Mark Willman,Krisztián Sárneczky,András Pál,John C Wheeler,John C Wheeler,Attila Bódi,Zs. Bognár,B. Csák,B. Cseh,G. Csörnyei,O. Hanyecz,Bernadett Ignácz,Cs. Kalup,Réka Könyves-Tóth,Levente Kriskovics,A. Ordasi,I. Rajmon,Ádám Sódor,R. Szabó,Róbert Szakáts,G. Zsidi,Peter A. Milne,Jennifer E. Andrews,Nathan Smith,Christopher Bilinski,Peter J. Brown,Jakob Nordin,Steven Williams,Lluís Galbany,J. Palmerio,Isobel Hook,Cosimo Inserra,Kate Maguire,Régis Cartier,A. Razza,A. Razza,Claudia P. Gutiérrez,J. J. Hermes,Joshua S. Reding,B. C. Kaiser,John L. Tonry,A. N. Heinze,L. Denneau,H. Weiland,B. Stalder,Geert Barentsen,Jessie L. Dotson,Thomas Barclay,Thomas Barclay,Michael Gully-Santiago,Christina Hedges,Ann Marie Cody,Steve B. Howell,Jeffrey L. Coughlin,Jeffrey L. Coughlin,J. Van Cleve,J. Van Cleve,J. Vinicius de Miranda Cardoso,J. Vinicius de Miranda Cardoso,K. A. Larson,K. M. McCalmont-Everton,C. A. Peterson,S. E. Ross,L. H. Reedy,D. Osborne,C. McGinn,L. Kohnert,L. Migliorini,A. Wheaton,B. Spencer,C. Labonde,G. Castillo,G. Beerman,K. Steward,M. Hanley,R. M. Larsen,R. Gangopadhyay,R. Kloetzel,T. Weschler,V. Nystrom,J. Moffatt,M. Redick,Kim Griest,M. Packard,M. Muszynski,J. Kampmeier,R. Bjella,S. Flynn,B. Elsaesser +183 more
TL;DR: The first spectroscopically confirmed type Ia supernova (ASASSN-18bt) was observed in the Kepler field by Dimitriadis et al. as mentioned in this paper.