Dictionary of Nomenclature of Celestial Objects
(Last update: 07-Nov-2018)

Result of query: info cati KOI-7016$



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Details on Acronym:   KOI
   KOI (Kepler Object of Interest) Write:<<KOI -NNNN>>
<<KOI -NNNNa>>
<<KOI -NNNN.NN>> N: ? Object:Unknown  (SIMBAD class: Unknown = Object of unknown nature) Note:The Kepler Mission list of "Objects of Interest".
Format -NNNN.NN: The two digits beyond the decimal provide identification of the candidates when more than one is found for a given star. For a multi-candidate system these digits beyond the decimal indicate the order in which the candidates were identified by the analysis pipelines and are not necessarily in order of orbital period. It should be noted that the KOI list is not contiguous and not all integers have an associated KOI.
KOI numbers are always cross-referenced to a KIC ID.
(See documentation: http://archive.stsci.edu/kepler/planet_candidates.html) Ref:=2011ApJ...728..117B byBORUCKI W.J. , KOCH D.G., BASRI G., BATALHA N., BOSS A., BROWN T.M., CALDWELL D., CHRISTENSEN-DALSGAARD J., COCHRAN W.D., DEVORE E., DUNHAM E.W., DUPREE A.K., GAUTIER III T.N., GEARY J.C., GILLILAND R., GOULD A., HOWELL S.B., JENKINS J.M., KJELDSEN H., LATHAM D.W., LISSAUER J.J., MARCY G.W., MONET D.G., SASSELOV D., TARTER J., CHARBONNEAU D., DOYLE L., FORD E.B., FORTNEY J., HOLMAN M.J., SEAGER S., STEFFEN J.H., WELSH W.F., ALLEN C., BRYSON S.T., BUCHHAVE L., CHANDRASEKARAN H., CHRISTIANSEN J.L., CIARDI D., CLARKE B.D., DOTSON J.L., ENDL M., FISCHER D., FRESSIN F., HAAS M., HORCH E., HOWARD A., ISAACSON H., KOLODZIEJCZAK J., LI J., MacQUEEN P., MEIBOM S., PRSA A., QUINTANA E.V., ROWE J., SHERRY W., TENENBAUM P., TORRES G., TWICKEN J.D., VAN CLEVE J., WALKOWICZ L., WU H. Astrophys. J., 728, 117 (2011) Characteristics of Kepler planetary candidates based on the first data set. Ref:=2011ApJ...736...19B byBORUCKI W.J. , KOCH D.G., BASRI G., BATALHA N., BROWN T.M., BRYSON S.T., CALDWELL D., CHRISTENSEN-DALSGAARD J., COCHRAN W.D., DEVORE E., DUNHAM E.W., GAUTIER T.N., GEARY J.C., GILLILAND R., GOULD A., HOWELL S.B., JENKINS J.M., LATHAM D.W., LISSAUER J.J., MARCY G.W., ROWE J., SASSELOV D., BOSS A., CHARBONNEAU D., CIARDI D., DOYLE L., DUPREE A.K., FORD E.B., FORTNEY J., HOLMAN M.J., SEAGER S., STEFFEN J.H., TARTER J., WELSH W.F., ALLEN C., BUCHHAVE L.A., CHRISTIANSEN J.L., CLARKE B.D., DAS S., DESERT J.-M., ENDL M., FABRYCKY D., FRESSIN F., HAAS M., HORCH E., HOWARD A., ISAACSON H., KJELDSEN H., KOLODZIEJCZAK J., KULESA C., LI J., LUCAS P.W., MACHALEK P., McCARTHY D., MacQUEEN P., MEIBOM S., MIQUEL T., PRSA A., QUINN S.N., QUINTANA E.V., RAGOZZINE D., SHERRY W., SHPORER A., TENENBAUM P., TORRES G., TWICKEN J.D., VAN CLEVE J., WALKOWICZ L., WITTEBORN F.C., STILL M. Astrophys. J., 736, 19 (2011) Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data. =E=Catalogue in electronic form as J/ApJ/728/117 =E=Catalogue in electronic form as J/ApJ/736/19 Originof the Acronym: L = Found in the literature

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