BD+26 2091B , the SIMBAD biblio

BD+26 2091B , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST00:55:52


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Title First 3 Authors
2016AJ....151...45E 1282     A     X C       32 26 26 KELT-4Ab: an inflated hot Jupiter transiting the bright (V ∼ 10) component of a hierarchical triple. EASTMAN J.D., BEATTY T.G., SIVERD R.J., et al.
2017ApJ...834...17C viz 16       D               1 290 454 Probabilistic forecasting of the masses and radii of other worlds. CHEN J. and KIPPING D.
2017AJ....154...25B 40           X         1 5 6 Determining empirical stellar masses and radii from transits and Gaia parallaxes as illustrated by Spitzer observations of KELT-11b. BEATTY T.G., STEVENS D.J., COLLINS K.A., et al.
2018MNRAS.474.4264M 16       D               1 36 4 A survey of eight hot Jupiters in secondary eclipse using WIRCam at CFHT. MARTIOLI E., COLON K.D., ANGERHAUSEN D., et al.
2018AJ....155...27C 40           X         1 58 ~ A search for binary star companions to the KELT planet hosts and a comparison sample. I. Results of DSSI observations. COKER C.T., GAUDI B.S., POGGE R.W., et al.
2023MNRAS.521.2969B 17       D               1 87 2 Planet engulfment detections are rare according to observations and stellar modelling. BEHMARD A., DAI F., BREWER J.M., et al.
2024ApJS..270...14W viz 18       D               1 333 ~ Long-term Variations in the Orbital Period of Hot Jupiters from Transit-timing Analysis Using TESS Survey Data. WANG W., ZHANG Z., CHEN Z., et al.
2024MNRAS.529.4768S viz 18       D               1 66 ~ Search for Stellar Companions of Exoplanet Host Stars with AstraLux/CAHA 2.2 m. SCHLAGENHAUF S., MUGRAUER M., GINSKI C., et al.
2024A&A...690A.379K 134           X         3 72 ~ Obliquities of exoplanet host stars Nineteen new and updated measurements, and trends in the sample of 205 measurements. KNUDSTRUP E., ALBRECHT S.H., WINN J.N., et al.
2026ApJ...996L...7W 120       D       C       2 48 ~ Unified Kraft Break at ∼6500 K: A Newly Identified Single-star Obliquity Transition Matches the Classical Rotation Break. WANG X.-Y., WANG S. and ONG J.M.J.

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