Publication Details


Toward a Galactic Distribution of Planets. I. Methodology and Planet Sensitivities of the 2015 High-cadence Spitzer Microlens Sample


Zhu, Wei and Udalski, A. and Calchi Novati, S. and Chung, S. -J. and Jung, Y. K. and Ryu, Y. -H. and Shin, I. -G. and Gould, A. and Lee, C. -U. and Albrow, M. D. and Yee, J. C. and Han, C. and Hwang, K. -H. and Cha, S. -M. and Kim, D. -J. and Kim, H. -W. and Kim, S. -L. and Kim, Y. -H. and Lee, Y. and Park, B. -G. and Pogge, R. W. and Poleski, R. and Mróz, P. and Pietrukowicz, P. and Skowron, J. and Szymański, M. K. and KozLowski, S. and Ulaczyk, K. and Pawlak, M. and Beichman, C. and Bryden, G. and Carey, S. and Fausnaugh, M. and Gaudi, B. S. and Henderson, C. B. and Shvartzvald, Y. and Wibking, B.



, 2017, 154, 210

Data Sets Used

Note: A "More Missions" icon indicates one or more data sets from among: COSMOS, BLAST, BOLOCAM, IRTS, MSX, SWAS, BRAVA, MUSYC, GPIPS, HERON. Follow the icon link for data set descriptions.

A best-effort attempt was made to match publications with data sets actually used given available resources. It is possible that in some cases data sets were missed or the publication's use of the data set was indirect or incidental.