M
Martin Dominik
Researcher at University of St Andrews
Publications - 414
Citations - 17326
Martin Dominik is an academic researcher from University of St Andrews. The author has contributed to research in topics: Gravitational microlensing & Planet. The author has an hindex of 62, co-authored 399 publications receiving 16221 citations. Previous affiliations of Martin Dominik include Max Planck Society & University of Groningen.
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Journal ArticleDOI
The complete catalogue of light curves in equal-mass binary microlensing
TL;DR: In this article, the authors presented a paper supported by NPRP grant NPRP-09-476-1-78 from the Qatar National Research Fund (QNF), a member of Qatar Foundation.
Journal Article
Detecting planets around stars in nearby galaxies
TL;DR: In this article, the capability of photometric µL extends to the detection of signals caused by planets around stars in nearby galaxies (e.g. M31) and that there is no other method that can achieve this.
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Larger and faster: revised properties and a shorter orbital period for the WASP-57 planetary system from a pro-am collaboration
John Southworth,Luigi Mancini,J. Tregloan-Reed,S. Calchi Novati,Simona Ciceri,Giuseppe D'Ago,Laetitia Delrez,Martin Dominik,Daniel F. Evans,Michaël Gillon,Emmanuel Jehin,U. G. Jørgensen,Troels Haugbølle,Monika Lendl,C. Arena,L. Barbieri,M. Barbieri,Giorgio Corfini,C. Lopresti,Andrea Marchini,Gennaro Marino,Khalid Al-Subai,Valerio Bozza,D. M. Bramich,R. Figuera Jaimes,Tobias C. Hinse,Th. Henning,M. Hundertmark,Diana Juncher,Heidi Korhonen,A. Popovas,Markus Rabus,Sohrab Rahvar,R. W. Schmidt,Jesper Skottfelt,Colin Snodgrass,D. A. Starkey,Jean Surdej,Olivier Wertz +38 more
TL;DR: In this paper, a new and precise orbital ephemeris of the WASP-57 planetary system has been determined, and the physical properties of the system were measured using 10 transit light curves from amateur telescopes, on which this discovery was based, 13 transit light curve from professional facilities which confirm and refine this finding, and high-resolution imaging which show no evidence for nearby companions.
Journal ArticleDOI
Flux and color variations of the doubly imaged quasar UM673
Davide Ricci,Davide Ricci,Davide Ricci,Andrii Elyiv,François Finet,Olivier Wertz,Khalid Al-Subai,Timo Anguita,Valerio Bozza,P. Browne,Martin Burgdorf,Martin Burgdorf,S. Calchi Novati,Peter N. Dodds,Martin Dominik,Stefan Dreizler,T. Gerner,M. Glitrup,F. Grundahl,S. Hardis,K. B. W. Harpsøe,Tobias C. Hinse,Tobias C. Hinse,Allan Hornstrup,M. Hundertmark,U. G. Jørgensen,N. Kains,Eamonn Kerins,C. Liebig,C. Liebig,Gernot Maier,Luigi Mancini,Luigi Mancini,Luigi Mancini,G. Masi,M. Mathiasen,Matthew T. Penny,S. Proft,Sohrab Rahvar,Sohrab Rahvar,Gaetano Scarpetta,Kailash C. Sahu,S. Schäfer,F. Schönebeck,R. W. Schmidt,Jesper Skottfelt,Colin Snodgrass,Colin Snodgrass,John Southworth,Christina C. Thöne,Christina C. Thöne,Joachim Wambsganss,F. Zimmer,M. Zub,Jean Surdej +54 more
TL;DR: In this article, the authors performed multi-epoch and multi-band photometric observations with the Danish 1.54m telescope at the La Silla Observatory during four seasons (2008-2011) using the PSF (Point Spread Function) photometric technique as well as aperture photometry.
Journal ArticleDOI
High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). II. Lucky Imaging results from 2015 and 2016
Daniel F. Evans,John Southworth,Barry Smalley,U. G. Jørgensen,Martin Dominik,Michael I. Andersen,Valerio Bozza,Valerio Bozza,D. M. Bramich,Martin Burgdorf,Simona Ciceri,Giuseppe D'Ago,R. Figuera Jaimes,R. Figuera Jaimes,Shenghong Gu,Tobias C. Hinse,Th. Henning,M. Hundertmark,N. Kains,Eamonn Kerins,Heidi Korhonen,Rosita Kokotanekova,Rosita Kokotanekova,M. Kuffmeier,Penélope Longa-Peña,Luigi Mancini,Luigi Mancini,Luigi Mancini,J. MacKenzie,A. Popovas,Markus Rabus,Markus Rabus,Sohrab Rahvar,Sedighe Sajadian,Colin Snodgrass,Jesper Skottfelt,Jean Surdej,René Tronsgaard,Eduardo Unda-Sanzana,C. von Essen,Yi-Bo Wang,Olivier Wertz +41 more
TL;DR: In this article, the authors search for binary companions to known transiting exoplanet host stars, in order to determine the multiplicity properties of hot Jupiter host stars and characterise unassociated stars along the line of sight, allowing photometric and spectroscopic observations to be corrected for contaminating light.