LATTE: Lightcurve Analysis Tool for Transiting Exoplanets

Journal of Open Source Software, 5(49), 2101,

Authors:

Nora L. Eisner, Chris J. Lintott and Suzanne Aigrain

Abstract:

Book Review: Barbara L. Wheeler and Kathleen Murphy (eds), Music Therapy Research

British Journal of Music Therapy SAGE Publications 34:1 (2020) 61-66

Authors:

Claire Molyneux, Alisa Apreleva Kolomeytseva, Laura Blauth, Jodie Bloska, Veronica Austin

Planet Hunters TESS I: TOI 813, a subgiant hosting a transiting Saturn-sized planet on an 84-day orbit

Monthly Notices of the Royal Astronomical Society, Volume 494, Issue 1, May 2020, Pages 750–763,

Authors:

N L Eisner, O Barragán, S Aigrain, C Lintott, G Miller, N Zicher, T S Boyajian, C Briceño, E M Bryant, J L Christiansen, A D Feinstein, L M Flor-Torres, M Fridlund, D Gandolfi, J Gilbert, N Guerrero, J M Jenkins, K Jones, M H Kristiansen, A Vanderburg, N Law, A R López-Sánchez, A W Mann, E J Safron, M E Schwamb, K G Stassun, H P Osborn, J Wang, A Zic, C Ziegler, F Barnet, S J Bean, D M Bundy, Z Chetnik, J L Dawson, J Garstone, A G Stenner, M Huten, S Larish, L D Melanson, T Mitchell, C Moore, K Peltsch, D J Rogers, C Schuster, D S Smith, D J Simister, C Tanner, I Terentev, A Tsymbal

Abstract:

We report on the discovery and validation of TOI 813 b (TIC 55525572 b), a transiting exoplanet identified by citizen scientists in data from NASA’s Transiting Exoplanet Survey Satellite (TESS) and the first planet discovered by the Planet Hunters TESS project. The host star is a bright (V = 10.3 mag) subgiant (⁠R⋆=1.94R⊙⁠, M⋆=1.32M⊙⁠). It was observed almost continuously by TESS during its first year of operations, during which time four individual transit events were detected. The candidate passed all the standard light curve-based vetting checks, and ground-based follow-up spectroscopy and speckle imaging enabled us to place an upper limit of 2MJup (99 per cent confidence) on the mass of the companion, and to statistically validate its planetary nature. Detailed modelling of the transits yields a period of 83.8911+0.0027−0.0031 d, a planet radius of 6.71 ± 0.38 R⊕ and a semimajor axis of 0.423+0.031−0.037 AU. The planet’s orbital period combined with the evolved nature of the host star places this object in a relatively underexplored region of parameter space. We estimate that TOI 813 b induces a reflex motion in its host star with a semi-amplitude of ∼6 m s−1, making this a promising system to measure the mass of a relatively long-period transiting planet.

LATTE: Lightcurve Analysis Tool for Transiting Exoplanets

The Journal of Open Source Software The Open Journal 5:49 (2020) 2101

Authors:

Nora Eisner, Chris Lintott, Suzanne Aigrain

Defining the Really Habitable Zone

(2020)

Authors:

Marven F Pedbost, Trillean Pomalgu, Chris Lintott, Nora Eisner, Belinda Nicholson