NAME 118 Tau group , the SIMBAD biblio

NAME 118 Tau group , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST17:36:57

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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
2017ApJ...836L..15C 1 16 20 Subaru/SCExAO first-light direct imaging of a young debris disk around HD 36546. CURRIE T., GUYON O., TAMURA M., et al.
2018ApJ...853...75T 82             C       1 40 1 2MASS J11151597+1937266 a young, dusty, isolated, planetary-mass object with a potential wide stellar companion. THEISSEN C.A., BURGASSER A.J., BARDALEZ GAGLIUFFI D.C., et al.
2018ApJ...856...23G viz 428       D     X C       10 1601 367 BANYAN. XI. The BANYAN Σ multivariate Bayesian algorithm to identify members of young associations with 150 pc. GAGNE J., MAMAJEK E.E., MALO L., et al.
2018ApJ...860...43G viz 181       D     X C       4 739 55 BANYAN. XII. New members of nearby young associations from Gaia-Tycho data. GAGNE J., ROY-LOUBIER O., FAHERTY J.K., et al.
2018ApJ...862..138G viz 99       D       C       3 943 100 BANYAN. XIII. A first look at nearby young associations with Gaia Data Release 2. GAGNE J. and FAHERTY J.K.
2018ApJ...863...91F 305       D     X C       7 289 47 New and known moving groups and clusters identified in a Gaia comoving catalog. FAHERTY J.K., BOCHANSKI J.J., GAGNE J., et al.
2018ApJ...865..136G 82             C       2 99 9 Volans-Carina: a new 90 Myr old stellar association at 85 pc. GAGNE J., FAHERTY J.K. and MAMAJEK E.E.
2018AJ....156..302D 82           X         2 117 10 Discovery of a transiting adolescent sub-Neptune exoplanet with K2. DAVID T.J., MAMAJEK E.E., VANDERBURG A., et al.
2019ApJ...877...60B viz 42           X         1 658 26 The elusive majority of young moving groups. I. Young binaries and lithium-rich stars in the solar neighborhood. BOWLER B.P., HINKLEY S., ZIEGLER C., et al.
2019AJ....157..247R 42           X         1 71 ~ Radial velocities, space motions, and nearby young moving group memberships of eleven candidate young brown dwarfs. RIEDEL A.R., DITOMASSO V., RICE E.L., et al.
2020ApJ...896..173P 255           X C       5 46 3 2MASS J04435686+3723033 B: a young companion at the substellar boundary with potential membership in the β Pictoris moving group. PHILLIPS C.L., BOWLER B.P., MACE G., et al.
2021ApJS..254...20L viz 131           X         3 632 15 The old moving groups in the field of Taurus. LIU J., FANG M., TIAN H., et al.
2021AJ....161..271F 174           X         4 41 23 A detailed characterization of HR 8799's debris disk with ALMA in Band 7. FARAMAZ V., MARINO S., BOOTH M., et al.
2021AJ....161..277K viz 17       D               1 88 24 Calibration of the Hα age-activity relation for M dwarfs. KIMAN R., FAHERTY J.K., CRUZ K.L., et al.
2021ApJ...915L..29G 131           X         3 34 27 A number of nearby moving groups may be fragments of dissolving open clusters. GAGNE J., FAHERTY J.K., MORANTA L., et al.
2021ApJ...917...20H 61       D     X         2 27 13 Evidence suggesting that 'Oumuamua is the ∼30 Myr old product of a molecular cloud. HSIEH C.-H., LAUGHLIN G. and ARCE H.G.
2021ApJ...917...23K viz 104       D     X         3 90 57 Stars with photometrically young Gaia luminosities around the solar system (SPYGLASS). I. Mapping Young stellar structures and their star formation histories. KERR R.M.P., RIZZUTO A.C., KRAUS A.L., et al.
2021AJ....162..293L 44           X         1 9 4 Multiband imaging of the HD 36546 debris disk: a refined view from SCExAO/CHARIS. LAWSON K., CURRIE T., WISNIEWSKI J.P., et al.
2022AJ....164..151L 90           X         2 60 4 A Census of the 32 Ori Association with Gaia. LUHMAN K.L.
2022ApJ...939...94M 466       D     X C       10 132 6 New Coronae and Stellar Associations Revealed by a Clustering Analysis of the Solar Neighborhood. MORANTA L., GAGNE J., COUTURE D., et al.
2023AJ....166..175F 19       D               1 33 ~ Using Photometrically Derived Properties of Young Stars to Refine TESS's Transiting Young Planet Survey Completeness. FERNANDES R.B., HARDEGREE-ULLMAN K.K., PASCUCCI I., et al.

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