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2017AJ....154..210Z - Astron. J., 154, 210-210 (2017/November-0)
Toward a Galactic distribution of planets. I. Methodology and planet sensitivities of the 2015 high-cadence Spitzer microlens sample.
ZHU W., UDALSKI A., CALCHI NOVATI S., CHUNG S.-J., JUNG Y.K., RYU Y.-H., SHIN I.-G., GOULD A., LEE C.-U., ALBROW M.D., YEE J.C., HAN C., HWANG K.-H., CHA S.-M., KIM D.-J., KIM H.-W., KIM S.-L., KIM Y.-H., LEE Y., PARK B.-G., POGGE R.W. (The KMTNet Collaboration), POLESKI R., MROZ P., PIETRUKOWICZ P., SKOWRON J., SZYMANSKI M.K., KOZLOWSKI S., ULACZYK K., PAWLAK M. (The OGLE Collaboration), BEICHMAN C., BRYDEN G., CAREY S., FAUSNAUGH M., GAUDI B.S., HENDERSON C.B., SHVARTZVALD Y., WIBKING B. (The Spitzer Team)
Abstract (from CDS):
Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.
Journal keyword(s): gravitational lensing: micro - methods: statistical - planetary systems - planets and satellites: dynamical evolution and stability - planets and satellites: dynamical evolution and stability
VizieR on-line data: <Available at CDS (J/AJ/154/210): table1.dat table2.dat>
Simbad objects: 75
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