Prof. David Alonso: Publications

Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD

JOURNAL OF LOW TEMPERATURE PHYSICS 193:5-6 (2018) 841-850

Authors:

T Hasebe, S Kashima, PAR Ade, Y Akiba, D Alonso, K Arnold, J Aumont, C Baccigalupi, D Barron, S Basak, S Beckman, J Borrill, F Boulanger, M Bucher, E Calabrese, Y Chinone, H-M Cho, A Cukierman, DW Curtis, T de Haan, M Dobbs, A Dominjon, T Dotani, L Duband, A Ducout, J Dunkley, JM Duval, T Elleflot, HK Eriksen, J Errard, J Fischer, T Fujino, T Funaki, U Fuskeland, K Ganga, N Goeckner-Wald, J Grain, NW Halverson, T Hamada, M Hasegawa, K Hattori, M Hattori, L Hayes, M Hazumi, N Hidehira, CA Hill, G Hilton, J Hubmayr, K Ichiki, T Iida, H Imada, M Inoue, Y Inoue, KD Irwin, H Ishino, O Jeong, H Kanai, D Kaneko, N Katayama, T Kawasaki, SA Kernasovskiy, R Keskitalo, A Kibayashi, Y Kida, K Kimura, T Kisner, K Kohri, E Komatsu, K Komatsu, CL Kuo, NA Kurinsky, A Kusaka, A Lazarian, AT Lee, D Li, E Linder, B Maffei, A Mangilli, M Maki, T Matsumura, S Matsuura, D Meilhan, S Mima, Y Minami, K Mitsuda, L Montier, M Nagai, T Nagasaki, R Nagata, M Nakajima, S Nakamura, T Namikawa, M Naruse, H Nishino, T Nitta, T Noguchi, H Ogawa, S Oguri, N Okada, A Okamoto, T Okamura, C Otani, G Patanchon, G Pisano, G Rebeiz, M Remazeilles, PL Richards, S Sakai, Y Sakurai, Y Sato, N Sato, M Sawada, Y Segawa, Y Sekimoto, U Seljak, BD Sherwin, T Shimizu, K Shinozaki, R Stompor, H Sugai, H Sugita, A Suzuki, J Suzuki, O Tajima, S Takada, R Takaku, S Takakura, S Takatori, D Tanabe, E Taylor, KL Thompson, B Thorne, T Tomaru, T Tomida, N Tomita, M Tristram, C Tucker, P Turin, M Tsujimoto, S Uozumi, S Utsunomiya, Y Uzawa, F Vansyngel, IK Wehus, B Westbrook, M Willer, N Whitehorn, Y Yamada, R Yamamoto, N Yamasaki, T Yamashita, M Yoshida

The effect on cosmological parameter estimation of a parameter dependent covariance matrix

(2018)

Authors:

Darsh Kodwani, David Alonso, Pedro Ferreira

Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts

(2018)

Authors:

Square Kilometre Array Cosmology Science Working Group, David J Bacon, Richard A Battye, Philip Bull, Stefano Camera, Pedro G Ferreira, Ian Harrison, David Parkinson, Alkistis Pourtsidou, Mario G Santos, Laura Wolz, Filipe Abdalla, Yashar Akrami, David Alonso, Sambatra Andrianomena, Mario Ballardini, Jose Luis Bernal, Daniele Bertacca, Carlos AP Bengaly, Anna Bonaldi, Camille Bonvin, Michael L Brown, Emma Chapman, Song Chen, Xuelei Chen, Steven Cunnington, Tamara M Davis, Clive Dickinson, Jose Fonseca, Keith Grainge, Stuart Harper, Matt J Jarvis, Roy Maartens, Natasha Maddox, Hamsa Padmanabhan, Jonathan R Pritchard, Alvise Raccanelli, Marzia Rivi, Sambit Roychowdhury, Martin Sahlen, Dominik J Schwarz, Thilo M Siewert, Matteo Viel, Francisco Villaescusa-Navarro, Yidong Xu, Daisuke Yamauchi, Joe Zuntz

Transit timing analysis of the exoplanet TrES-5 b. Possible existence of the exoplanet TrES-5 c

Monthly Notices of the Royal Astronomical Society 480:1 (2018) 291-301

Authors:

EN Sokov, IA Sokova, VV Dyachenko, DA Rastegaev, A Burdanov, SA Rusov, P Benni, S Shadick, VP Hentunen, M Salisbury, N Esseiva, J Garlitz, M Bretton, Y Ogmen, Y Karavaev, A Ayiomamitis, O Mazurenko, D Alonso, SF Velichko

Abstract:

In this work, we present transit timing variations detected for the exoplanet TrES-5b. To obtain the necessary amount of photometric data for this exoplanet, we have organized an international campaign to search for exoplanets based on the transit-timing variation (TTV) method and as a result of this we collected 30 new light curves, 15 light curves from the Exoplanet Transit Database (ETD) and 8 light curves from the literature for the timing analysis of the exoplanet TrES-5b. We have detected timing variations with a semi-amplitude of A≈ 0.0016 d and a period of P≈ 99 d. We carried out the N-body modelling based on the three-body problem. The detected perturbation of TrES-5b may be caused by a second exoplanet in the TrES-5 system. We have calculated the possible mass and resonance of the object: M ≈ 0.24MJup at a 1:2 Resonance.

A unified pseudo-$C_\ell$ framework

(2018)

Authors:

David Alonso, Javier Sanchez, Anže Slosar

91̽��