Planet Hunters TESS II: findings from the first two years of TESS

Author:

Eisner N L1ORCID,Barragán O1,Lintott C1ORCID,Aigrain S1,Nicholson B12,Boyajian T S3,Howell S4,Johnston C56ORCID,Lakeland B1,Miller G1,McMaster A1,Parviainen H7,Safron E J3,Schwamb M E89,Trouille L10,Vaughan S1,Zicher N1,Allen C1,Allen S10,Bouslog M10,Johnson C10,Simon M N10,Wolfenbarger Z10,Baeten E M L11,Bundy D M11,Hoffman T11

Affiliation:

1. Department of Physics, University of Oxford, Keble Rd, Oxford OX1 3RH, UK

2. University of Southern Queensland, Centre for Astrophysics, West Street, Toowoomba, QLD 4350, Australia

3. Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803, USA

4. NASA Ames Research Center, Moffett Field, CA 94035, USA

5. Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium

6. Department of Astrophysics, IMAPP, Radboud University Nijmegen, P.O. Box 9010, NL-6500 GL Nijmegen, the Netherlands

7. Instituto de Astrofisica de Canarias (IAC), Via Lactea s/n, 38205 E-La Laguna, Tenerife, Spain

8. Gemini Observatory, Northern Operations Center, 670 North A’ohoku Place, Hilo, HI 96720, USA

9. Astrophysics Research Centre, Queen’s University Belfast, Belfast BT7 1NN, UK

10. Department of Citizen Science, The Adler Planetarium, Chicago, IL 60605, USA

11. Planet Hunters TESS Citizen Scientist, University of Oxford, Keble Road, Oxford OX1 3RH, UK

Abstract

ABSTRACT We present the results from the first two years of the Planet Hunters TESS (PHT) citizen science project, which identifies planet candidates in the TESS (Transiting Exoplanet Survey Satellite) data by engaging members of the general public. Over 22 000 citizen scientists from around the world visually inspected the first 26 sectors of TESS data in order to help identify transit-like signals. We use a clustering algorithm to combine these classifications into a ranked list of events for each sector, the top 500 of which are then visually vetted by the science team. We assess the detection efficiency of this methodology by comparing our results to the list of TESS Objects of Interest (TOIs) and show that we recover 85 per cent of the TOIs with radii greater than 4 R⊕ and 51 per cent of those with radii between 3 and 4 R⊕. Additionally, we present our 90 most promising planet candidates that had not previously been identified by other teams, 73 of which exhibit only a single-transit event in the TESS light curve, and outline our efforts to follow these candidates up using ground-based observatories. Finally, we present noteworthy stellar systems that were identified through the Planet Hunters TESS project.

Funder

NASA

NSF

National Research Council Canada

European Union

Horizon 2020

Brinson Foundation

Moore Foundation

European Research Council

Research Foundation Flanders

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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