K2-45 , the SIMBAD biblio

K2-45 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.06.03CEST18:12:07


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Title First 3 Authors
2015A&A...579A..19A viz 16       D               1 8375 75 K2 Variable Catalogue: Variable stars and eclipsing binaries in K2 campaigns 1 and 0. ARMSTRONG D.J., KIRK J., LAM K.W.F., et al.
2016ApJS..222...14V viz 16       D               1 209 177 Planetary candidates from the first year of the K2 mission. VANDERBURG A., LATHAM D.W., BUCHHAVE L.A., et al.
2016ApJS..226....7C viz 16       D               2 400 165 197 candidates and 104 validated planets in K2's first five fields. CROSSFIELD I.J.M., CIARDI D.R., PETIGURA E.A., et al.
2017ApJ...836..167D viz 16       D               1 144 30 Characterizing K2 candidate planetary systems orbiting low-mass stars. I. Classifying low-mass host stars observed during Campaigns 1-7. DRESSING C.D., NEWTON E.R., SCHLIEDER J.E., et al.
2017MNRAS.465.2634A viz 16       D               4 5400 21 Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. ARMSTRONG D.J., POLLACCO D. and SANTERNE A.
2017AJ....154..207D viz 16       D               1 118 78 Characterizing K2 candidate planetary systems orbiting low-mass stars. II. Planetary systems observed during campaigns 1-7. DRESSING C.D., VANDERBURG A., SCHLIEDER J.E., et al.
2018AJ....156...99L 173           X C       3 15 126 An update to the EVEREST K2 pipeline: short cadence, saturated stars, and Kepler-like photometry down to Kp = 15. LUGER R., KRUSE E., FOREMAN-MACKEY D., et al.
2019AJ....157..124K viz 142       D     X C       3 603 7 Discovery and Vetting of Exoplanets. I. Benchmarking K2 vetting tools. KOSTOV V.B., MULLALLY S.E., QUINTANA E.V., et al.
2019ApJS..244...11K viz 17       D               1 2119 48 Detection of hundreds of new planet candidates and eclipsing binaries in K2 campaigns 0-8. KRUSE E., AGOL E., LUGER R., et al.
2020ApJ...890...23L viz 17       D               1 4935 35 Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2022ApJS..259...50S viz 18       D               1 1632 9 New Pulsating Stars Detected in EA-type Eclipsing-binary Systems Based on TESS Data. SHI X.-D., QIAN S.-B. and LI L.-J.

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