V* V607 Lyr , the SIMBAD biblio

V* V607 Lyr , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST20:01:10


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Bibcode/DOI Score in Title|Abstract|
Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2003A&A...410..323B 51 34 A search for planets in the old open cluster NGC 6791. BRUNTT H., GRUNDAHL F., TINGLEY B., et al.
2005AJ....129.2856M viz 107 41 Planets in stellar clusters extensive search. III. A search for transiting planets in the metal-rich open cluster NGC 6791. MOCHEJSKA B.J., STANEK K.Z., SASSELOV D.D., et al.
2006IBVS.5721....1K viz 1754 36 The 78th name-list of variable stars. KAZAROVETS E.V., SAMUS N.N., DURLEVICH O.V., et al.
2007A&A...471..515D viz 74           X         2 127 34 Variable stars in the open cluster NGC 6791 and its surrounding field. DE MARCHI F., PORETTI E., MONTALTO M., et al.
2013A&A...557L..10N viz 15       D               1 12151 189 Rotation periods of 12000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations. NIELSEN M.B., GIZON L., SCHUNKER H., et al.
2014ApJS..211...24M viz 15       D               1 34022 573 Rotation periods of 34,030 Kepler main-sequence stars: the full autocorrelation sample. McQUILLAN A., MAZEH T. and AIGRAIN S.
2014AJ....148..123H 518       D S   X C       12 19 8 Kepler and the long-period variables. HARTIG E., CASH J., HINKLE K.H., et al.
2015ApJ...809....8B viz 16       D               1 112329 282 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
2020MNRAS.499.3481A viz 16       D               1 28505 24 Evidence for metallicity-dependent spin evolution in the Kepler field. AMARD L., ROQUETTE J. and MATT S.P.
2020JAVSO..48..218C         O           3 ~ Kepler Observations of Three SRS: StarsoV616 Lyrae, V607 Lyrae, and V621 Lyrae. CASH J., WALTER D., RED W., et al.
2021AJ....161..189L viz 17       D               1 29956 19 Gyro-kinematic ages for around 30,000 Kepler stars. LU Y., ANGUS R., CURTIS J.L., et al.

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