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TCP J05074264+2447555 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.02.03CET14:36:16 |
Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
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 ![]() |
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 ![]() |
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 ![]() |
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 ![]() |
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 ![]() |
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 ![]() |
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. |
2022MNRAS.514.5952Z | 47 | X | 1 | 20 | ~ | OGLE-2018-BLG-0799Lb: a q ∼ 2.7 x 10–3 planet with Spitzer parallax. | ZANG W., SHVARTZVALD Y., UDALSKI A., 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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