ATO J067.3755+22.6542 , the SIMBAD biblio

ATO J067.3755+22.6542 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST07:13:38


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Title First 3 Authors
2018AJ....156..241H viz 16       D               1 311114 199 A first catalog of variable stars measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS). HEINZE A.N., TONRY J.L., DENNEAU L., et al.
2018AJ....156..271L viz 16       D               1 630 108 The stellar membership of the Taurus star-forming region. LUHMAN K.L.
2018A&A...620A.172Z viz 16       D               1 127607 99 3D mapping of young stars in the solar neighbourhood with Gaia DR2. ZARI E., HASHEMI H., BROWN A.G.A., et al.
2019AJ....158...54E viz 100       D         F     3 633 47 A survey for new members of Taurus from stellar to planetary masses. ESPLIN T.L. and LUHMAN K.L.
2019A&A...630A.137G viz 17       D               1 560 78 Structure and kinematics of the Taurus star-forming region from Gaia-DR2 and VLBI astrometry. GALLI P.A.B., LOINARD L., BOUY H., et al.
2020AJ....159..273R viz 17       D               1 269 55 Rotation of low-mass stars in Taurus with K2. REBULL L.M., STAUFFER J.R., CODY A.M., et al.
2020MNRAS.495.1252Z viz 17       D               2 1120 18 Magnetic activity based on LAMOST medium-resolution spectra and the Kepler survey. ZHANG L.-Y., LONG L., SHI J., et al.
2020A&A...638A..85R viz 17       D               2 320 31 A 3D view of the Taurus star-forming region by Gaia and Herschel. Multiple populations related to the filamentary molecular cloud. ROCCATAGLIATA V., FRANCIOSINI E., SACCO G.G., et al.
2021ApJS..254...20L viz 17       D               1 632 15 The old moving groups in the field of Taurus. LIU J., FANG M., TIAN H., et al.
2021AJ....162..110K viz 17       D               1 605 44 Gaia EDR3 reveals the substructure and complicated star formation history of the greater Taurus-Auriga star-forming complex. KROLIKOWSKI D.M., KRAUS A.L. and RIZZUTO A.C.
2021ApJ...920..132P viz 17       D               1 5441 33 Quantifying variability of young stellar objects in the mid-infrared over 6 years with the Near-Earth Object Wide-field Infrared Survey Explorer. PARK W., LEE J.-E., CONTRERAS PENA C., et al.

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