참고문헌
- Batista, V., Gould, A., Dieters, S. et al. 2011, MOA-2009-BLG-387Lb: A Massive Planet Orbiting an M Dwarf, A&A, 529, 102
- Calchi Novati, S., Gould, A., Udalski, A., et al., 2015, Pathway to the Galactic Distribution of Planets: Combined Spitzer and Ground-Based Microlens Parallax Measurements of 21 Single-Lens Events, ApJ, 804, 20 https://doi.org/10.1088/0004-637X/804/1/20
- Gould, A. 1992, Extending the MACHO Search to about 106 Solar Masses, ApJ, 392, 442 https://doi.org/10.1086/171443
- Gould, A. 1994, MACHO Velocities from Satellite-based Parallaxes, ApJL, 421, L75 https://doi.org/10.1086/187191
- Gould, A. 2000, A Natural Formalism for Microlensing, ApJ, 542, 785 https://doi.org/10.1086/317037
- Gould, A. 2019, Osculating Versus Intersecting Circles in Space-Based Microlens Parallax Degeneracies, JKAS, 52, 121
- Han, C. & Gould, A. 1995, The Mass Spectrum of MACHOs From Parallax Measurements, ApJ, 447, 53 https://doi.org/10.1086/175856
- Koshimoto, N. & Bennett, D.P., 2019, Evidence of Systematic Errors in Spitzer Microlens Parallax Measurements, AJ, in press, arXiv:1905.05794
- Refsdal, S. 1966, On the Possibility of Determining the Distances and Masses of Stars from the Gravitational Lens Effect, MNRAS, 134, 315 https://doi.org/10.1093/mnras/134.3.315
- Udalski, A., Yee, J.C., Gould, A., et al. 2015, Spitzer as a Microlens Parallax Satellite: Mass Measurement for the OGLE-2014-BLG-0124L Planet and its Host Star, ApJ, 799, 237 https://doi.org/10.1088/0004-637X/799/2/237
- Yee, J.C., Udalski, A., Calchi Novati, S., et al., 2015a, First Space-based Microlens Parallax Measurement of an Isolated Star: Spitzer Observations of OGLE-2014-BLG-0939, ApJ, 802, 76 https://doi.org/10.1088/0004-637X/802/2/76
- Zang, W., Dong, S., Gould, A. et al. 2020, Spitzer + VLTIGRAVITY Measure the Lens Mass of a Nearby Microlensing Event, ApJ, 897, 180 https://doi.org/10.3847/1538-4357/ab9749
- Zhu, W., Udalski, A., Calchi Novati, S., et al. 2017, Toward a Galactic Distribution of Planets. I. Methodology & Planet Sensitivities of the 2015 High-Cadence Spitzer Microlens Sample, AJ, 154, 210 https://doi.org/10.3847/1538-3881/aa8ef1