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BD+73 323 , the SIMBAD biblio (18 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST19:31:55 |
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 |
---|---|---|---|---|---|---|---|---|---|
2017AJ....153...94C | 1316 | D | S X C | 31 | 33 | 15 | Discovery of XO-6b: a hot Jupiter transiting a fast rotating F5 star on an oblique orbit. | CROUZET N., McCULLOUGH P.R., LONG D., et al. | |
2017A&A...603A..30S | 16 | D | 2 | 2500 | 58 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al. | ||
2018ApJS..239...14J | 16 | D | 1 | 1561 | 6 | Revised exoplanet radii and habitability using Gaia data release 2. | JOHNS D., MARTI C., HUFF M., et al. | ||
2019AJ....158..190H | 17 | D | 1 | 343 | 61 | Hot Jupiters are destroyed by tides while their host stars are on the main sequence. | HAMER J.H. and SCHLAUFMAN K.C. | ||
2020MNRAS.491.2760G | 877 | A | X C | 20 | 19 | ~ |
Periodic transit timing variations and refined system parameters of the exoplanet XO-6b. |
GARAI Z., PRIBULLA T., KOMZIK R., et al. | |
2020ApJ...890...23L | 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. | ||
2020AJ....160..249R | 213 | X | 5 | 7 | ~ | TESS observations of the hot Jupiter exoplanet XO-6b: no evidence of transit timing variations. | RIDDEN-HARPER A., TURNER J.D. and JAYAWARDHANA R. | ||
2021A&A...645A...7K | 17 | D | 1 | 1569 | 17 | Determining the true mass of radial-velocity exoplanets with Gaia. Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets. | KIEFER F., HEBRARD G., LECAVELIER DES ETANGS A., et al. | ||
2021ApJ...909..115C | 17 | D | 1 | 2175 | 13 | Planets Across Space and Time (PAST). I. Characterizing the memberships of Galactic components and stellar ages: revisiting the kinematic methods and applying to planet host stars. | CHEN D.-C., XIE J.-W., ZHOU J.-L., et al. | ||
2021ApJ...916L...1A | 17 | D | 1 | 57 | 40 | A preponderance of perpendicular planets. | ALBRECHT S.H., MARCUSSEN M.L., WINN J.N., et al. | ||
2021ApJS..256...33T | 17 | D | 3 | 56 | 23 | The Magellan-TESS Survey. I. Survey description and midsurvey results. | TESKE J., WANG S.X., WOLFGANG A., et al. | ||
2022AJ....163..104F | 18 | D | 2 | 61 | 7 | The Breakthrough Listen search for intelligent life: technosignature search of Transiting TESS Targets of Interest. | FRANZ N., CROFT S., SIEMION A.P.V., et al. | ||
2022ApJS..259...62I | 18 | D | 1 | 395 | 24 | TESS Transit Timing of Hundreds of Hot Jupiters. | IVSHINA E.S. and WINN J.N. | ||
2022AJ....164..104R | 18 | D | 1 | 105 | 10 | A Tendency Toward Alignment in Single-star Warm-Jupiter Systems. | RICE M., WANG S., WANG X.-Y., et al. | ||
2022PASP..134h2001A | 18 | D | 1 | 366 | 39 | Stellar Obliquities in Exoplanetary Systems. | ALBRECHT S.H., DAWSON R.I. and WINN J.N. | ||
2022AcA....72....1M | 12 | 3 | Search for planets in hot Jupiter systems with multi-sector TESS photometry. II. Constraints on planetary companions in 12 systems. | MACIEJEWSKI G. | |||||
2023AJ....166...72S | 47 | X | 1 | 23 | ~ | Variability of Known Exoplanet Host Stars Observed by TESS. | SIMPSON E.R., FETHEROLF T., KANE S.R., et al. | ||
2024AJ....167...48M | 20 | D | 1 | 72 | ~ | Signs of Similar Stellar Obliquity Distributions for Hot and Warm Jupiters Orbiting Cool Stars. | MORGAN M., BOWLER B.P., TRAN Q.H., et al. |