TOI-942b , the SIMBAD biblio

TOI-942b , the SIMBAD biblio (33 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST06:55:47

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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
2021AJ....161....2Z 879     A D     X C       21 27 38 Two young planetary systems around field stars with ages between 20 and 320 Myr from TESS. ZHOU G., QUINN S.N., IRWIN J., et al.
2021A&A...645A..71C 1672     A D     X C F     39 33 24 The GAPS Programme at TNG. XXVIII. A pair of hot-Neptunes orbiting the young star TOI-942. CARLEO I., DESIDERA S., NARDIELLO D., et al.
2021A&A...650A..66B viz 42           X         1 45 28 Constraints on the mass and on the atmospheric composition and evolution of the low-density young planet DS Tucanae A b. BENATTI S., DAMASSO M., BORSA F., et al.
2021ApJS..254...39G viz 17       D               1 2206 165 The TESS Objects of Interest Catalog from the TESS Prime Mission. GUERRERO N.M., SEAGER S., HUANG C.X., et al.
2021ApJ...917L..34W 1046 T   A D     X C       24 8 9
TOI-942b: a prograde Neptune in a ∼ 60 Myr old multi-transiting system. 		WIRTH C.P., ZHOU G., QUINN S.N., et al.
2021ApJ...922L...1H 84           X         2 14 8 The obliquity of HIP 67522 b: a 17 Myr old transiting hot, Jupiter-sized planet. HEITZMANN A., ZHOU G., QUINN S.N., et al.
2022MNRAS.510.2111K 1549       D     X C F     35 15 6 Atmospheric mass-loss and stellar wind effects in young and old systems - I. Comparative 3D study of TOI-942 and TOI-421 systems. KUBYSHKINA D., VIDOTTO A.A., VILLARREAL D'ANGELO C., et al.
2022MNRAS.510.3039K 766       S   X C F     15 9 3 Atmospheric mass loss and stellar wind effects in young and old systems - II. Is TOI-942 the past of TOI-421 system? KUBYSHKINA D., VIDOTTO A.A., VILLARREAL D'ANGELO C., et al.
2022AJ....163..247J viz 85           X         2 16 9 An Aligned Orbit for the Young Planet V1298 Tau b. JOHNSON M.C., DAVID T.J., PETIGURA E.A., et al.
2022AJ....163..284H 45           X         1 10 21 The unpopular Package: A Data-driven Approach to Detrending TESS Full-frame Image Light Curves. HATTORI S., FOREMAN-MACKEY D., HOGG D.W., et al.
2022PASP..134h2001A viz 17       D               2 366 39 Stellar Obliquities in Exoplanetary Systems. ALBRECHT S.H., DAWSON R.I. and WINN J.N.
2022ApJ...939...24A 102       D     X         3 20 1 Detecting Magnetospheric Radio Emission from Giant Exoplanets. ASHTARI R., SCIOLA A., TURNER J.D., et al.
2022A&A...666A.183K 43           X         1 15 5 A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N. KONIG P.-C., DAMASSO M., HEBRARD G., et al.
2023ApJ...944L..41F viz 44           X         1 19 2 NEID Reveals That the Young Warm Neptune TOI-2076 b Has a Low Obliquity. FRAZIER R.C., STEFANSSON G., MAHADEVAN S., et al.
2023AJ....165..121H 44           X         1 24 1 TOI-4562b: A Highly Eccentric Temperate Jupiter Analog Orbiting a Young Field Star. HEITZMANN A., ZHOU G., QUINN S.N., et al.
2023AJ....165..250S 87             C       1 11 ~ Updated Planetary Mass Constraints of the Young V1298 Tau System Using MAROON-X. SIKORA J., ROWE J., BARAT S., et al.
2023A&A...674A.120A 17       D               1 189 1 DREAM II. The spin-orbit angle distribution of close-in exoplanets under the lens of tides. ATTIA O., BOURRIER V., DELISLE J.-B., et al.
2023A&A...675A.158D 87           X         2 27 ~ TOI-179: A young system with a transiting compact Neptune-mass planet and a low-mass companion in outer orbit. DESIDERA S., DAMASSO M., GRATTON R., et al.
2023AJ....166..266R viz 17       D               1 54 ~ Evidence for Low-level Dynamical Excitation in Near-resonant Exoplanet Systems. RICE M., WANG X.-Y., WANG S., et al.
2024MNRAS.528.2834B 45           X         1 7 ~ Hot Jupiter formation in dense star clusters. BENKENDORFF L., FLAMMINI DOTTI F., STOCK K., et al.
2024A&A...684L..17M viz 45           X         1 25 ~ Orbital obliquity of the young planet TOI-5398 b and the evolutionary history of the system. MANTOVAN G., MALAVOLTA L., LOCCI D., et al.
2024A&A...685A.143M viz 18       D               1 535 ~ Planets similar in size are often dissimilar in interior. MAMONOVA E., SHAN Y., HATALOVA P., et al.
2024NatAs...8..899B 90               F     1 21 ~ The metal-poor atmosphere of a potential sub-Neptune progenitor. BARAT S., DESERT J.-M., VAZAN A., et al.
2024MNRAS.532.4752D 45           X         1 130 ~ The SHERLOCK pipeline: new exoplanet candidates in the WASP-16, HAT-P-27, HAT-P-26, and TOI-2411 systems. DEVORA-PAJARES M., POZUELOS F.J., THUILLIER A., et al.
2024AJ....168..194T 314           X   F     6 6 ~ The ∼50 Myr Old TOI-942c is Likely on an Aligned, Coplanar Orbit and Losing Mass. TENG H.-Y., DAI F., HOWARD A.W., et al.
2024AJ....168..196L viz 90           X         2 27 ~ The HD 191939 Exoplanet System is Well Aligned and Flat. LUBIN J., PETIGURA E.A., VAN ZANDT J., et al.
2024AJ....168..239D 45           X         1 37 ~ The Prevalence of Resonance Among Young, Close-in Planets. DAI F., GOLDBERG M., BATYGIN K., et al.
2025MNRAS.536.1538A 47           X         1 32 ~ NGTS-33b: a young super-Jupiter hosted by a fast-rotating massive hot star. ALVES D.R., JENKINS J.S., VINES J.I., et al.
2025MNRAS.536.2046Y 93               F     1 11 ~ A possible misaligned orbit for the young planet AU Mic c. YU H., GARAI Z., CRETIGNIER M., et al.
2025AJ....170..182P 19       D               1 58 ~ An Aligned Sub-Neptune Revealed with MAROON-X and a Tendency Toward Alignment for Small Planets. POLANSKI A.S., CROSSFIELD I.J.M., SEIFAHRT A., et al.
2025AJ....170..275Y 47           X         1 13 ~ The Polar Orbit of TOI-2374 b, a Planet in the Neptunian Ridge. YEE S.W., TAMBURO P., STEFANSSON G., et al.
2025ApJ...994L..55B 19       D               1 18 ~ Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape (SOYSAUCE): A Likely Aligned Orbit for the 3 Myr Planet TIDYE-1 b. BARBER M.G., MANN A.W., JOHNSON M.C., et al.
2026A&A...705A.142R viz 20       D               1 55 ~ True spin-orbit obliquity distribution: Data-driven confirmation of no clustering of misaligned planets. ROSSI A.M., RAINER M., BORSA F., et al.

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