• Bulletin of the Korean Space Science Society
• /
• 2000.10a
• /
• pp.19-19
• /
• 2000

No Abstract, See Full Text

• Bulletin of the Korean Space Science Society
• /
• 1998.10a
• /
• pp.73-82
• /
• 1998

• Bulletin of the Korean Space Science Society
• /
• 1998.10a
• /
• pp.16.2-16
• /
• 1998

No Abstract.See Full-text

• The Bulletin of The Korean Astronomical Society
• /
• v.29 no.2
• /
• pp.62.1-62.1
• /
• 2004

• The Bulletin of The Korean Astronomical Society
• /
• v.22
• /
• pp.33.2-34
• /
• 1997

• The Bulletin of The Korean Astronomical Society
• /
• v.24 no.1
• /
• pp.57-57
• /
• 1999

• The Bulletin of The Korean Astronomical Society
• /
• v.30 no.1
• /
• pp.51.2-51.2
• /
• 2005

• The Bulletin of The Korean Astronomical Society
• /
• v.23
• /
• pp.47-47
• /
• 1998

• The Bulletin of The Korean Astronomical Society
• /
• v.25 no.1
• /
• pp.31-31
• /
• 2000

• The Bulletin of The Korean Astronomical Society
• /
• v.40 no.2
• /
• pp.57.4-58
• /
• 2015

Thanks to high cadence monitoring and high photometric accuracy of Korea Microlensing Telescope Network (KMTNet), we expect the detection of many events caused by wide-separation planets and free-floating planets, which is not easy due to the short event duration. Thus, it is important to understand wide-separation planetary lensing events. Several studies on the wide-separation events have been reported, but events caused by wide-separation planetary systems with a moon have not yet been studied. In this paper, we study the properties of events caused by planetary systems where wide-separation planets host a moon. We also study the effect of a finite background source star on the moon feature in the wide planetary-lensing events.