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2020MNRAS.493..973D - Mon. Not. R. Astron. Soc., 493, 973-985 (2020/March-3)
TOI-132 b: A short-period planet in the Neptune desert transiting a V = 11.3 G-type star.
DIAZ M.R., JENKINS J.S., GANDOLFI D., LOPEZ E.D., SOTO M.G., CORTES-ZULETA P., BERDINAS Z.M., STASSUN K.G., COLLINS K.A., VINES J.I., ZIEGLER C., FRIDLUND M., JENSEN E.L.N., MURGAS F., SANTERNE A., WILSON P.A., ESPOSITO M., HATZES A.P., JOHNSON M.C., LAM K.W.F., LIVINGSTON J.H., VAN EYLEN V., NARITA N., BRICENO C., COLLINS K.I., CSIZMADIA S., FAUSNAUGH M., GAN T., GARCIA R.A., GEORGIEVA I., GLIDDEN A., GONZALEZ-CUESTA L., JENKINS J.M., LATHAM D.W., LAW N.M., MANN A.W., MATHUR S., MIRELES I., MORRIS R., PALLE E., PERSSON C.M., RICKER G., RINEHART S., ROSE M.E., SEAGER S., SMITH J.C., TAN T.-G., TOKOVININ A., VANDERBURG A., VANDERSPEK R., WINN J.N. and YAHALOMI D.A.
Abstract (from CDS):
Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): techniques: photometric - techniques: radial velocities - planets and satellites: fundamental parameters - planetary systems
Simbad objects: 7
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