F
F. Schönebeck
Researcher at Heidelberg University
Publications - 20
Citations - 740
F. Schönebeck is an academic researcher from Heidelberg University. The author has contributed to research in topics: Gravitational microlensing & Light curve. The author has an hindex of 16, co-authored 20 publications receiving 701 citations.
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Journal ArticleDOI
Radial constraints on the initial mass function from TiO features and Wing–Ford band in early-type galaxies
Francesco La Barbera,Alexandre Vazdekis,Alexandre Vazdekis,Ignacio Ferreras,Anna Pasquali,Michele Cappellari,Ignacio Martín-Navarro,Ignacio Martín-Navarro,F. Schönebeck,Jesús Falcón-Barroso,Jesús Falcón-Barroso +10 more
TL;DR: In this paper, the authors combine various TiO-based, IMF-sensitive indicators in the optical and NIR spectral windows, along with the FeH-based Wing-Ford band to break this degeneracy.
Journal ArticleDOI
The transiting system GJ1214: high-precision defocused transit observations and a search for evidence of transit timing variation
K. B. W. Harpsøe,S. Hardis,Tobias C. Hinse,U. G. Jørgensen,Luigi Mancini,John Southworth,Khalid Al-Subai,Valerio Bozza,P. Browne,Martin Burgdorf,S. Calchi Novati,Peter N. Dodds,Martin Dominik,X.-S. Fang,François Finet,T. Gerner,Shenghong Gu,M. Hundertmark,Jens Jessen-Hansen,N. Kains,Eamonn Kerins,Hans Kjeldsen,C. Liebig,Mikkel N. Lund,M. Lundkvist,M. Mathiasen,David Nesvorný,Nikolay Nikolov,Matthew T. Penny,S. Proft,Sohrab Rahvar,Davide Ricci,Kailash C. Sahu,Gaetano Scarpetta,Sebastian Schafer,F. Schönebeck,Colin Snodgrass,Jesper Skottfelt,Jean Surdej,J. Tregloan-Reed,Olivier Wertz +40 more
TL;DR: In this paper, the authors used a Bayesian approach to investigate the ephemeris for possible signs of transit timing variations (TTVs) using a high-precision photometric transitobservations of the transiting super-Earth planet GJ 1214 b.
Journal ArticleDOI
The Transiting System GJ1214: High-Precision Defocused Transit Observations and a Search for Evidence of Transit Timing Variation
K. B. W. Harpsøe,S. Hardis,Tobias C. Hinse,U. G. Jørgensen,Luigi Mancini,John Southworth,Khalid Al-Subai,Valerio Bozza,P. Browne,Martin Burgdorf,S. Calchi Novati,Peter N. Dodds,Martin Dominik,X.-S. Fang,François Finet,T. Gerner,Shenghong Gu,M. Hundertmark,N. Kains,Eamonn Kerins,H. Kjeldsen,C. Liebig,Mikkel N. Lund,M. Lundkvist,M. Mathiasen,David Nesvorný,Nikolay Nikolov,Matthew T. Penny,S. Proft,Sohrab Rahvar,Davide Ricci,Kailash C. Sahu,Gaetano Scarpetta,Sebastian Schafer,F. Schönebeck,Colin Snodgrass,Jesper Skottfelt,Jean Surdej,J. Tregloan-Reed,Olivier Wertz +39 more
TL;DR: In this article, a Bayesian analysis reveals that it is highly improbable that the observed transit times is explained by TTV, when compared with the simpler alternative of a linear ephemeris.
Journal ArticleDOI
MOA-2010-BLG-477Lb: constraining the mass of a microlensing planet from microlensing parallax, orbital motion and detection of blended light
Etienne Bachelet,In-Gu Shin,C. Han,P. Fouque,Andrew Gould,J. W. Menzies,J. P. Beaulieu,David P. Bennett,Ian A. Bond,Subo Dong,David Heyrovský,J. B. Marquette,Jennifer L. Marshall,Jan Skowron,R. A. Street,Takahiro Sumi,Andrzej Udalski,L. Abe,K. Agabi,Michael D. Albrow,William H. Allen,E. Bertin,M. Bos,D. M. Bramich,J. Chavez,G. W. Christie,Andrew A. Cole,Nicolas Crouzet,S. Dieters,Martin Dominik,Jack D. Drummond,J. G. Greenhill,Tristan Guillot,Calen B. Henderson,F. V. Hessman,Keith Horne,M. Hundertmark,John Asher Johnson,U. G. Jørgensen,Ryo Kandori,C. Liebig,D. Mekarnia,Jennie McCormick,D. Moorhouse,Takahiro Nagayama,David M. Nataf,Tim Natusch,Shogo Nishiyama,J. P. Rivet,Kailash C. Sahu,Yossi Shvartzvald,G. Thornley,Adam Tomczak,Yiannis Tsapras,Jennifer C. Yee,V. Batista,C. S. Bennett,Stephane Brillant,J. A. R. Caldwell,Arnaud Cassan,E. Corrales,C. Coutures,D. Dominis Prester,J. Donatowicz,D. Kubas,R. M. Martin,Andrew Williams,M. Zub,L. Andrade de Almeida,Darren L. DePoy,B. S. Gaudi,Li-Wei Hung,Francisco Jablonski,Shai Kaspi,N. Klein,C.-U. Lee,Young Sun Lee,J.-R. Koo,D. Maoz,J. A. Muñoz,R. W. Pogge,David Polishook,Avi Shporer,Fumio Abe,C. S. Botzler,Paul Chote,M. Freeman,Akihiko Fukui,K. Furusawa,P. Harris,Yoshitaka Itow,S. Kobara,C. H. Ling,Kimiaki Masuda,Yutaka Matsubara,N. Miyake,Kantaro Ohmori,K. Ohnishi,Nicholas J. Rattenbury,To. Saito,Denis J. Sullivan,Daisuke Suzuki,Winston L. Sweatman,P. J. Tristram,K. Wada,Philip Yock,Michał K. Szymański,Igor Soszyński,M. Kubiak,Radosław Poleski,K. Ulaczyk,Grzegorz Pietrzyński,Łukasz Wyrzykowski,N. Kains,Colin Snodgrass,Iain A. Steele,Khalid Al-Subai,Valerio Bozza,P. Browne,Martin Burgdorf,S. Calchi Novati,Peter N. Dodds,S. Dreizler,F. Finet,T. Gerner,S. Hardis,Kasper Harpsøe,Tobias C. Hinse,Eamonn Kerins,Luigi Mancini,M. Mathiasen,Matthew T. Penny,S. Proft,Sohrab Rahvar,Davide Ricci,Gaetano Scarpetta,Sebastian Schafer,F. Schönebeck,John Southworth,Jean Surdej,Joachim Wambsganss +140 more
TL;DR: In this article, the authors reported the discovery of a giant planet detected from the analysis of the light curve of a high-magnification microlensing event MOA-2010-BLG-477.
Journal ArticleDOI
MOA 2010-BLG-477Lb: Constraining the Mass of a Microlensing Planet from Microlensing Parallax, Orbital Motion, and Detection of Blended Light
Etienne Bachelet,In-Gu Shin,C. Han,Pascal Fouqué,Andrew Gould,J. W. Menzies,J. P. Beaulieu,David P. Bennett,Ian A. Bond,Subo Dong,Subo Dong,David Heyrovský,J. B. Marquette,Jennifer L. Marshall,Jan Skowron,Rachel Street,Takahiro Sumi,Takahiro Sumi,Andrzej Udalski,L. Abe,K. Agabi,Michael D. Albrow,William H. Allen,Emmanuel Bertin,M. Bos,D. M. Bramich,J. Chavez,G. W. Christie,Andrew A. Cole,Nicolas Crouzet,S. Dieters,Martin Dominik,Martin Dominik,Jack D. Drummond,J. G. Greenhill,Tristan Guillot,Calen B. Henderson,Frederic V. Hessman,Keith Horne,M. Hundertmark,M. Hundertmark,Jennifer A. Johnson,U. G. Jørgensen,U. G. Jørgensen,Ryo Kandori,C. Liebig,C. Liebig,D. Mekarnia,Jennie McCormick,D. Moorhouse,Takahiro Nagayama,David M. Nataf,Tim Natusch,Shogo Nishiyama,J. P. Rivet,Kailash C. Sahu,Yossi Shvartzvald,G. Thornley,Adam Tomczak,Yiannis Tsapras,Yiannis Tsapras,Jennifer C. Yee,V. Batista,V. Batista,C. S. Bennett,S. Brillant,J. A. R. Caldwell,Arnaud Cassan,E. Corrales,C. Coutures,D. Dominis Prester,J. Donatowicz,D. Kubas,D. Kubas,R. M. Martin,Andrew Williams,M. Zub,L. Andrade de Almeida,Darren L. DePoy,B. S. Gaudi,Li-Wei Hung,Francisco Jablonski,Shai Kaspi,N. Klein,C.-U. Lee,Young Sun Lee,J.-R. Koo,D. Maoz,J. A. Muñoz,R. W. Pogge,David Polishook,Avi Shporer,Avi Shporer,Fumio Abe,C. S. Botzler,Paul Chote,M. Freeman,Akihiko Fukui,K. Furusawa,P. Harris,Yoshitaka Itow,S. Kobara,C. H. Ling,Kimiaki Masuda,Yutaka Matsubara,N. Miyake,Kantaro Ohmori,K. Ohnishi,Nicholas J. Rattenbury,To. Saito,Denis J. Sullivan,Daisuke Suzuki,Winston L. Sweatman,P. J. Tristram,K. Wada,Philip Yock,Michał K. Szymański,Igor Soszyński,M. Kubiak,Radosław Poleski,Krzysztof Ulaczyk,Grzegorz Pietrzyński,Grzegorz Pietrzyński,Łukasz Wyrzykowski,Łukasz Wyrzykowski,N. Kains,N. Kains,Colin Snodgrass,Iain A. Steele,Khalid Al-Subai,Valerio Bozza,P. Browne,Martin Burgdorf,Martin Burgdorf,S. Calchi Novati,Peter N. Dodds,Stefan Dreizler,F. Finet,T. Gerner,S. Hardis,K. B. W. Harpsøe,K. B. W. Harpsøe,Tobias C. Hinse,Eamonn Kerins,Luigi Mancini,Luigi Mancini,M. Mathiasen,Matthew T. Penny,S. Proft,Sohrab Rahvar,Davide Ricci,Gaetano Scarpetta,Sebastian Schafer,F. Schönebeck,John Southworth,Jean Surdej,Joachim Wambsganss +156 more
TL;DR: In this article, the authors reported the discovery of a giant planet detected from the analysis of the light curve of a high-magnification microlensing event MOA 2010-BLG-477.