SIMBAD references

2020AJ....160...74H - Astron. J., 160, 74-74 (2020/August-0)

OGLE-2017-BLG-0406: Spitzer microlens parallax reveals Saturn-mass planet orbiting M-dwarf host in the inner Galactic disk.

HIRAO Y., BENNETT D.P., RYU Y.-H., KOSHIMOTO N., UDALSKI A., YEE J.C., SUMI T., BOND I.A., SHVARTZVALD Y., ABE F., BARRY R.K., BHATTACHARYA A., DONACHIE M., FUKUI A., ITOW Y., KONDO I., LI M.C.A., MATSUBARA Y., MATSUO T., MIYAZAKI S., MURAKI Y., NAGAKANE M., RANC C., RATTENBURY N.J., SUEMATSU H., SHIBAI H., SUZUKI D., TRISTRAM P.J., YONEHARA A. (The MOA Collaboration), SKOWRON J., POLESKI R., MROZ P., SZYMANSKI M.K., SOSZYNSKI I., KOZLOWSKI S., PIETRUKOWICZ P., ULACZYK K., RYBICKI K., IWANEK P. (The OGLE Collaboration), ALBROW M.D., CHUNG S.-J., GOULD A., HAN C., HWANG K.-H., JUNG Y.K., SHIN I.-G., ZANG W., CHA S.-M., KIM D.-J., KIM H.-W., KIM S.-L., LEE C.-U., LEE D.-J., LEE Y., PARK B.-G., POGGE R.W. (The KMTNet Collaboration), BEICHMAN C.A., BRYDEN G., NOVATI S.C., CAREY S., GAUDI B.S., HENDERSON C.B., ZHU W. (The Spitzer Team), BACHELET E., BOLT G., CHRISTIE G., HUNDERTMARK M., NATUSCH T., MAOZ D., McCORMICK J., STREET R.A., TAN T.-G., TSAPRAS Y. (The LCO and mFUN Follow-up Teams), JORGENSEN U.G., DOMINIK M., BOZZA V., SKOTTFELT J., SNODGRASS C., CICERI S., FIGUERA JAIMES R., EVANS D.F., PEIXINHO N., HINSE T.C., BURGDORF M.J., SOUTHWORTH J., RAHVAR S., SAJADIAN S., RABUS M., VON ESSEN C., FUJII Y.I., CAMPBELL-WHITE J., LOWRY S., HELLING C., MANCINI L., HAIKALA L. (The MiNDSTEp Collaboration), KANDORI R. (The IRSF Team)

Abstract (from CDS):

We report the discovery and analysis of the planetary microlensing event OGLE-2017-BLG-0406, which was observed both from the ground and by the Spitzer satellite in a solar orbit. At high magnification, the anomaly in the light curve was densely observed by ground-based-survey and follow-up groups, and it was found to be explained by a planetary lens with a planet/host mass ratio of q=7.0×10–4 from the light-curve modeling. The ground-only and Spitzer-"only" data each provide very strong one-dimensional (1D) constraints on the 2D microlens parallax vector πE. When combined, these yield a precise measurement of πE and of the masses of the host Mhost=0.56±0.07M☉ and planet Mplanet = 0.41 ± 0.05 MJup. The system lies at a distance DL = 5.2 ± 0.5 kpc from the Sun toward the Galactic bulge, and the host is more likely to be a disk population star according to the kinematics of the lens. The projected separation of the planet from the host is a⊥=3.5±0.3au (i.e., just over twice the snow line). The Galactic-disk kinematics are established in part from a precise measurement of the source proper motion based on OGLE-IV data. By contrast, the Gaia proper-motion measurement of the source suffers from a catastrophic 10σ error.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Gravitational microlensing - Gravitational microlensing exoplanet detection

VizieR on-line data: <Available at CDS (J/AJ/160/74): auckland.dat ctioh.dat ctioi.dat ctiov.dat irsfh.dat irsfj.dat irsfk.dat kmtc02i.dat kmtc42i.dat kmts02i.dat kmts42i.dat lcoctio.dat lcosso.dat moar.dat moav.dat ogle.dat spitzer.dat>

CDS comments: EWS 2012-BLG-0265 is a misprint for EWS 2011-BLG-0265.

Simbad objects: 29

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