4.1 ANÁLISIS CUANTITATIVO DE LOS DATOS
4.1.1 Análisis de la reforma No023-2014
For most of the history of our field, other solar systems were often assumed to exist, but astronomers had to make do with only dreams of their discovery and exploration. Twenty years ago that dream finally came true, and began an astronomical revolution, marked by an exponential increase in the number and diversity of planets found around distant stars since then. And with new missions and improved technology, that explosion looks set to continue well into the 21st century.
Transiting planetary systems offer the most detailed look at an exoplanet, with mea- surements of bulk density, orbital dynamics and even atmospheric composition possible. But, with classical detection methods and short-duration surveys such as K2 and TESS, such planets are limited to only the hot inner regions of extrasolar systems. The techniques developed in this thesis help push those current boundaries towards cooler planets and the eye-catching planet candidates detected in K2 photometry will, if confirmed, provide bench- mark systems for future transit surveys. The signals of many more key long-period planets may have already been recorded by ground- and space-based transit surveys, which future analyses based on methods presented by this thesis may reveal. Eventually, such methods will unlock planets capable of being directly imaged by future giant telescopes and, with high-precision transit missions, may even offer a new way of detecting Earth-like planets around sunlike stars.
Chapter 8
Full Author Publication List
-1 :Andrew J Rushby, Mark W Claire, Hugh Osborn, and Andrew J Watson. Habit-
able zone lifetimes of exoplanets around main sequence stars.Astrobiology, 13(9):833–849, 2013
2 :David J Armstrong, Hugh P Osborn, DJA Brown, Francesca Faedi, Y Gómez Maqueo
Chew, David V Martin, Don Pollacco, and S Udry. On the abundance of circumbinary plan- ets. Monthly Notices of the Royal Astronomical Society, 444(2):1873–1883, 2014a
3 : AMS Smith, DR Anderson, David J Armstrong, SCC Barros, AS Bonomo,
F Bouchy, DJA Brown, A Collier Cameron, Laetitia Delrez, Francesca Faedi, et al. Wasp- 104b and wasp-106b: two transiting hot jupiters in 1.75-day and 9.3-day orbits.Astronomy
&Astrophysics, 570:A64, 2014
4 : DJ Armstrong, HP Osborn, DJA Brown, J Kirk, KWF Lam, DL Pollacco,
J Spake, and SR Walker. K2 variable catalogue i: A catalogue of variable stars from k2 field 0. arXiv preprint arXiv:1411.6830, 2014b
5 : David J Armstrong, Alexandre Santerne, Dimitri Veras, Susana CC Barros,
Olivier Demangeon, Jorge Lillo-Box, James McCormac, Hugh P Osborn, Maria Tsantaki, José-Manuel Almenara, et al. One of the closest exoplanet pairs to the 3: 2 mean motion resonance: K2-19b and c. Astronomy&Astrophysics, 582:A33, 2015b
6 : David J Armstrong, J Kirk, KWF Lam, J McCormac, SR Walker, DJA Brown,
Hugh P Osborn, DL Pollacco, and J Spake. K2 variable catalogue: Variable stars and eclipsing binaries in k2 campaigns 1 and 0.Astronomy&Astrophysics, 579:A19, 2015a
7 : SCC Barros, JM Almenara, O Demangeon, M Tsantaki, A Santerne, David J
Armstrong, D Barrado, D Brown, M Deleuil, J Lillo-Box, et al. Photodynamical mass de- termination of the multiplanetary system k2-19.Monthly Notices of the Royal Astronomical Society, 454(4):4267–4276, 2015
8 : F Faedi, Y Chew, D Pollacco, DJA Brown, G Hébrard, B Smalley, KWF Lam, D Veras, D Anderson, AP Doyle, et al. Wasp-86b and wasp-102b: super-dense versus bloated planets.arXiv preprint arXiv:1608.04225, 2016
9 : David J Armstrong, J Kirk, KWF Lam, J McCormac, HP Osborn, J Spake,
S Walker, DJA Brown, MH Kristiansen, Don Pollacco, et al. K2 variable catalogue–ii. machine learning classification of variable stars and eclipsing binaries in k2 fields 0–4.
Monthly Notices of the Royal Astronomical Society, 456(2):2260–2272, 2016a
10 : J Lillo-Box, O Demangeon, A Santerne, SCC Barros, D Barrado, G Hébrard,
Hugh P Osborn, David J Armstrong, J-M Almenara, I Boisse, et al. K2-30 b and k2-34 b: Two inflated hot jupiters around solar-type stars. Astronomy&Astrophysics, 594:A50, 2016
11 :Jessica J Spake, David JA Brown, Amanda P Doyle, Guillaume Hébrard, James
McCormac, David J Armstrong, Don Pollacco, Y Gómez Maqueo Chew, David R Ander- son, Susana CC Barros, et al. Wasp-135b: a highly irradiated, inflated hot jupiter orbiting a g5v star. Publications of the Astronomical Society of the Pacific, 128(960):024401, 2016
12 : D Bayliss, S Hojjatpanah, A Santerne, D Dragomir, G Zhou, A Shporer,
KD Colón, J Almenara, DJ Armstrong, D Barrado, et al. Epic 201702477b: A transiting brown dwarf from k2 in a 41 day orbit. The Astronomical Journal, 153(1):15, 2016
13 :David J Armstrong, CE Pugh, A-M Broomhall, DJA Brown, MN Lund, Hugh P
Osborn, and DL Pollacco. The host stars of kepler’s habitable exoplanets: superflares,
rotation and activity. Monthly Notices of the Royal Astronomical Society, 455(3):3110–
3125, 2016b
14 :A Santerne, G Hébrard, J Lillo-Box, David J Armstrong, SCC Barros, O De-
mangeon, D Barrado, A Debackere, M Deleuil, E Delgado Mena, et al. K2-29 b/wasp-152
b: an aligned and inflated hot jupiter in a young visual binary. The Astrophysical Journal, 824(1):55, 2016
15 : DJ Armstrong, E de Mooij, J Barstow, HP Osborn, J Blake, and N Fereshteh
Saniee. Variability in the atmosphere of the hot giant planet hat-p-7 b. Nature Astronomy, 1:0004, 2016c
16 :Joseph E Rodriguez, George Zhou, Phillip A Cargile, Daniel J Stevens, Hugh P Osborn, Benjamin J Shappee, Phillip A Reed, Michael B Lund, Howard M Relles, David W
Latham, et al. The mysterious dimmings of the t tauri star v1334 tau. arXiv preprint
arXiv:1701.03044, 2017
17 : KWF Lam, F Faedi, DJA Brown, DR Anderson, Laetitia Delrez, Michaël
Gillon, G Hébrard, M Lendl, L Mancini, J Southworth, et al. From dense hot jupiter to
low-density neptune: The discovery of wasp-127b, wasp-136b, and wasp-138b.Astronomy
18 : HP Osborn, JE Rodriguez, MA Kenworthy, GM Kennedy, EE Mamajek, CE Robinson, CC Espaillat, DJ Armstrong, BJ Shappee, A Bieryla, DW Latham, DR An- derson, TG Beatty, P Berlind, ML Calkins, GA Esquerdo, BS Gaudi, C Hellier, TW-S Holoien, D James, CS Kochanek, RB Kuhn, MB Lund, J Pepper, DL Pollacco, JL Pri- eto, RJ Siverd, KG Stassun, DJ Stevens, KZ Stanek, and RG West. Periodic eclipses of
the young star pds 110 discovered with wasp and kelt photometry. Monthly Notices of the
Royal Astronomical Society, page stx1249, 2017a
19 :HP Osborn, A Santerne, SCC Barros, NC Santos, X Dumusque, L Malavoltac-
nmsep, DJ Armstrong, S Hojjatpanah, O Demangeon, V Adibekyan, J-M Almenara, D Bar- rado, D Bayliss, I Boisse, F Bouchy, DJA Brown, AC Cameron, D Charbonneau, M Deleuil, E DelgadoMena, R Diaz, G H’ebrard, J Kirk, GW King, KWF Lam, D Latham, J Lillo-Box, TM Louden, C Lovis, M Marmier, J McCormac, E Molinari, F Pepe, D Pollacco, SG Sousa, S Udry, and SR Walker. K2-110 b: a massive mini-neptune exoplanet.Astronomy&Astro- physics, 604:A19, 2017b
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