Kepler-427b , the SIMBAD biblio

Kepler-427b , the SIMBAD biblio (22 results)

C.D.S. - SIMBAD4 rel 1.7 - 2021.01.18CET13:18:44

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Bibcode/DOI	Score	in Title\|Abstract\| Keywords	in a table	in teXt, Caption, ...	Nb occurence	Nb objects in ref	Citations (from ADS)	Title	First 3 Authors
`2020A&A...634A..43O`	`65`		`D`	`X`	`2`	`141`	`~`	Revisited mass-radius relations for exoplanets below 120 M_⊕.	OTEGI J.F., BOUCHY F. and HELLED R.
`2020A&A...638A.143A`	`19`		`D`		`1`	`193`	`~`	Variability of transit light curves of Kepler objects of interest.	ARKHYPOV O.V., KHODACHENKO M.L. and HANSLMEIER A.
`2020AJ....159...41T`	`19`		`D`		`1`	`564`	`~`	Estimating planetary mass with deep learning.	TASKER E.J., LANEUVILLE M. and GUTTENBERG N.
`2020AJ....160..233A`	`47`			`X`	`1`	`9`	`~`	WASP-117 b: an eccentric hot Saturn as a future complex chemistry laboratory.	ANISMAN L.O., EDWARDS B., CHANGEAT Q., et al.
`2020MNRAS.497.3484A`	`47`			`X`	`1`	`4`	`~`	Constraining the oblateness of transiting planets with photometry and spectroscopy.	AKINSANMI B., BARROS S.C.C., SANTOS N.C., et al.
`2019A&A...630A.135U`	`18`		`D`		`1`	`501`	`~`	Beyond the exoplanet mass-radius relation.	ULMER-MOLL S., SANTOS N.C., FIGUEIRA P., et al.
`2019ApJ...874L..31T`	`18`		`D`		`1`	`403`	`~`	Connecting giant planet atmosphere and interior modeling: constraints on atmospheric metal enrichment.	THORNGREN D. and FORTNEY J.J.
`2018AJ....155..206A`	`17`		`D`		`3`	`183`	`~`	Systematic search for rings around Kepler planet candidates: constraints on ring size and occurrence rate.	AIZAWA M., MASUDA K., KAWAHARA H., et al.
`2018ApJ...866...99B`	`17`		`D`		`1`	`7129`	`101`	Revised radii of Kepler stars and planet's using Gaia Data Release 2.	BERGER T.A., HUBER D., GAIDOS E., et al.
`2017A&A...602A.107B`	`17`		`D`		`3`	`476`	`14`	The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets.	BONOMO A.S., DESIDERA S., BENATTI S., et al.
`2017AJ....154..164B`	`1379`		`D`	`S X C`	`31`	`8`	`2`	Determining exoplanetary oblateness using transit depth variations.	BIERSTEKER J. and SCHLICHTING H.
`2017ApJ...834...17C`	`17`		`D`		`1`	`289`	`84`	Probabilistic forecasting of the masses and radii of other worlds.	CHEN J. and KIPPING D.
`2017MNRAS.465.3693H`	`43`			`X`	`1`	`35`	`17`	WASP-South transiting exoplanets: WASP-130b, WASP-131b, WASP-132b, WASP-139b, WASP-140b, WASP-141b and WASP-142b.	HELLIER C., ANDERSON D.R., COLLIER CAMERON A., et al.
`2016AJ....152...18B`	`17`		`D`		`1`	`1167`	`34`	Robo-AO Kepler planetary candidate survey. II. Adaptive optics imaging of 969 Kepler exoplanet candidate host stars.	BARANEC C., ZIEGLER C., LAW N.M., et al.
`2016AJ....152..158T`	`17`		`D`		`1`	`4386`	`18`	Detection of potential transit signals in 17 quarters of Kepler data: results of the final Kepler mission transiting planet search (DR25).	TWICKEN J.D., JENKINS J.M., SEADER S.E., et al.
`2016AJ....152..181H`	`17`		`D`		`1`	`9278`	`9`	SETI observations of exoplanets with the Allen Telescope Array.	HARP G.R., RICHARDS J., TARTER J.C., et al.
`2016ApJ...825...98H`	`17`		`D`		`1`	`166`	`45`	Warm jupiters are less lonely than hot jupiters: close neighbors.	HUANG C., WU Y. and TRIAUD A.H.M.J.
`2015ApJ...809....8B`	`16`		`D`		`1`	`112329`	`139`	Terrestrial planet occurrence rates for the Kepler GK dwarf sample.	BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
`2015ApJS..217...16R`	`16`		`D`		`1`	`8625`	`84`	Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months).	ROWE J.F., COUGHLIN J.L., ANTOCI V., et al.
`2014A&A...572A..93H`	`715`	`T A`		`X C`	`16`	`29`	`9`	Characterization of the four new transiting planets KOI-188b, KOI-195b, KOI-192b, and KOI-830b.	HEBRARD G., SANTERNE A., MONTAGNIER G., et al.
`2014ApJS..210...19B`	`16`		`D`		`1`	`5860`	`162`	Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months).	BURKE C.J., BRYSON S.T., MULLALLY F., et al.
`2013ApJS..204...24B`	`16`		`D`		`1`	`3274`	`779`	Planetary candidates observed by Kepler. III. Analysis of the first 16 months of data.	BATALHA N.M., ROWE J.F., BRYSON S.T., et al.

View the references in ADS