TCP J05074264+2447555 , the SIMBAD biblio

TCP J05074264+2447555 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2022.11.29CET14:33:33


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Title First 3 Authors
2017ATel10919....1M 82 T         X         1 2 ~ High-dispersion spectroscopy of the probable microlensing event
TCP J05074264+2447555.
MAEHARA H.
2017ATel10921....1S 165 T         X         3 1 ~ Swift observations of the bright microlensing event
TCP J05074264+2447555.
SOKOLOVSKY K.
2017ATel10923....1J 247 T         X         5 1 ~ ASAS-SN Confirmation of the Bright Microlensing Event
TCP J05074264+2447555.
JAYASINGHE T., DONG S., STANEK K.Z., et al.
2017ATel10926....1K 165 T         X         3 1 ~ Follow-up Photometry of the Microlensing Event
TCP J05074264+2447555.
KONYVES-TOTH R., PAL A., ORDASI A., et al.
2017ATel10934....1N 206 T         X         4 2 ~
TCP J05074264+2447555 as a bright microlensing event due to a binary system with very low mass ratio component: hint for a new planetary system?
NUCITA A.A., LICCHELLI D., DE PAOLIS F., et al.
2018MNRAS.476.2962N 293     A D     X   F     7 8 4 Discovery of a bright microlensing event with planetary features towards the Taurus region: a super-Earth planet. NUCITA A.A., LICCHELLI D., DE PAOLIS F., et al.
2019ApJ...871...70D 596           X C       13 3 ~ First resolution of microlensed images. DONG S., MERAND A., DELPLANCKE-STROBELE F., et al.
2019ApJ...876...81H 43           X         1 6 ~ OGLE-2018-BLG-0022: first prediction of an astrometric microlensing signal from a photometric microlensing event. HAN C., BOND I.A., UDALSKI A., et al.
2019MNRAS.487.4603T 43           X         1 4 ~ An analysis of binary microlensing event OGLE-2015-BLG-0060. TSAPRAS Y., CASSAN A., RANC C., et al.
2019AJ....158..206F 621     A     X C       14 6 ~
Kojima-1Lb is a mildly cold Neptune around the brightest microlensing host star.
FUKUI A., SUZUKI D., KOSHIMOTO N., et al.
2020A&A...633A..98W viz 44           X         1 8 ~ Full orbital solution for the binary system in the northern Galactic disc microlensing event Gaia16aye. WYRZYKOWSKI L., MROZ P., RYBICKI K.A., et al.
2020ApJ...890...23L viz 17       D               1 4935 ~ Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2020ApJ...891....3Z viz 87           X         2 13 ~ Spitzer microlensing parallax reveals two isolated stars in the Galactic bulge. ZANG W., SHVARTZVALD Y., WANG T., et al.
2020ApJ...897..180Z viz 505     A     X C       11 6 ~ Spitzer + VLTI-GRAVITY measure the lens mass of a nearby microlensing event. ZANG W., DONG S., GOULD A., et al.
2020ApJS..249...16M viz 44           X         1 471 ~ Microlensing optical depth and event rate in the OGLE-IV Galactic plane fields. MROZ P., UDALSKI A., SZYMANSKI M.K., et al.
2020AJ....160...74H viz 87           X         2 27 ~ 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., et al.
2020RNAAS...4...13M 44           X         1 33 ~ Gravitational Microlensing Events from the First Year of the Northern Galactic Plane Survey by the Zwicky Transient Facility. MROZ P., STREET R.A., BACHELET E., et al.
2022NatAs...6..121C 280     A D     X C       6 115 ~ Microlensing mass measurement from images of rotating gravitational arcs. CASSAN A., RANC C., ABSIL O., et al.
2022NatAs...6..782Z 93             C       1 31 ~ A ubiquitous unifying degeneracy in two-body microlensing systems. ZHANG K., GAUDI B.S. and BLOOM J.S.

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2022.11.29-14:33:33

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