The K2-OjOS Project: New and revisited planets and candidates in K2 campaigns 5, 16, & 18

Author:

Castro-González A1ORCID,Díez Alonso E1,Menéndez Blanco J1,Livingston J2ORCID,de Leon J P2ORCID,Lillo-Box J3ORCID,Korth J4ORCID,Fernández Menéndez S1,Recio J M5ORCID,Izquierdo-Ruiz F6ORCID,Coya Lozano A7,García de la Cuesta F7,Gómez Hernández N7,Vidal Blanco J R7,Hevia Díaz R7,Pardo Silva R7,Pérez Acevedo S7,Polancos Ruiz J7,Padilla Tijerín P7,Vázquez García D7,Suárez Gómez S L1,García Riesgo F1,González Gutiérrez C1,Bonavera L1ORCID,González-Nuevo J1ORCID,Rodríguez Pereira C1,Sánchez Lasheras F1,Sánchez Rodríguez M L1,Muñiz R1ORCID,Santos Rodríguez J D1,de Cos Juez F J1

Affiliation:

1. Instituto Universitario de Ciencias y Tecnologías Espaciales de Asturias (ICTEA), C. Independencia 13, E-33004 Oviedo, Spain

2. Department of Astronomy, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

3. Centro de Astrobiología (CSIC-INTA), ESAC campus, Villanueva de la Cañada, E-28692 Madrid, Spain

4. Department of Space, Earth and Environment, Astronomy and Plasma Physics, Chalmers University of Technology, SE-412 96 Gothenburg, Sweden

5. Malta-Consolider Team and Departmento de Química Física y Analítica, Universidad de Oviedo, E-33006 Oviedo, Spain

6. Malta-Consolider Team and Department of Chemistry and Chemical Engineering, Chalmers University of Technology, SE-412 96 Gothenburg, Sweden

7. Sociedad Astronómica Asturiana Omega, C. Alegría 45, E-33209 Gijón, Spain

Abstract

ABSTRACT We present the first results of K2-OjOS, a collaborative project between professional and amateur astronomers primarily aimed to detect, characterize, and validate new extrasolar planets. For this work, 10 amateur astronomers looked for planetary signals by visually inspecting the 20 427 light curves of K2 campaign 18 (C18). They found 42 planet candidates, of which 18 are new detections and 24 had been detected in the overlapping C5 by previous works. We used archival photometric and spectroscopic observations, as well as new high-spatial resolution images in order to carry out a complete analysis of the candidates found, including a homogeneous characterization of the host stars, transit modelling, search for transit timing variations and statistical validation. As a result, we report four new planets (K2-355 b, K2-356 b, K2-357 b, and K2-358 b) and 14 planet candidates. Besides, we refine the transit ephemeris of the previously published planets and candidates by modelling C5, C16 (when available) and C18 photometric data jointly, largely improving the period and mid-transit time precision. Regarding individual systems, we highlight the new planet K2-356 b and candidate EPIC 211537087.02 being near a 2:1 period commensurability, the detection of significant TTVs in the bright star K2-184 (V = 10.35), the location of K2-103 b inside the habitable zone according to optimistic models, the detection of a new single transit in the known system K2-274, and the disposition reassignment of K2-120 b, which we consider as a planet candidate as the origin of the signal cannot be ascertained.

Funder

MINECO

MICINN

FEDER

Swedish National Space Agency

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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