activity
20172023
most citedOptical observations of NEA 3200 Phaethon (1983 TB) during the 2017 apparition

20 citations · 59 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2023★ 1 cited

Photometry of the Didymos system across the DART impact apparition

Nicholas Moskovitz, Cristina Thomas, Petr Pravec +78

On 26 September 2022, the Double Asteroid Redirection Test (DART) spacecraft impacted Dimorphos, the satellite of binary near-Earth asteroid (65803) Didymos. This demonstrated the…

astro-ph.EP2023★ 2 cited

Physical properties of the slow-rotating near-Earth asteroid (2059) Baboquivari from one apparition

Orhan Erece, Irek Khamitov, Murat Kaplan +6

In this study, we carried out photometric, spectroscopic, and for the first time, polarimetric observations of the Amor-type near-Earth asteroid (2059) Baboquivari. Our findings re…

astro-ph.EP2020★ 11 cited

Spin Change of Asteroid 2012 TC4 probably by Radiation Torques

Hee-Jae Lee, Josef Ďurech, David Vokrouhlický +9

Asteroid 2012 TC4 is a small (10 m) near-Earth object that was observed during its Earth close approaches in 2012 and 2017. Earlier analyses of light curves revealed its exci…

astro-ph.EP2018★ 12 cited

Investigation of surface homogeneity of (3200) Phaethon

Hee-Jae Lee, Myung-Jin Kim, Dong-Heun Kim +7

Time-series multi-band photometry and spectrometry were performed in Nov.-Dec. 2017 to investigate the homogeneity of the surface of asteroid (3200) Phaethon. We found that Phaetho…

astro-ph.EP2018★ 20 cited

Optical observations of NEA 3200 Phaethon (1983 TB) during the 2017 apparition

Myung-Jin Kim, Hee-Jae Lee, Sang-Min Lee +24

The near-Earth asteroid 3200 Phaethon (1983 TB) is an attractive object not only from a scientific viewpoint but also because of JAXA's DESTINY+ target. The rotational lightcurve a…

astro-ph.EP2017★ 13 cited

Confirmation of Large Super-Fast Rotator (144977) 2005 EC127

Chan-Kao Chang, Hsing-Wen Lin, Wing-Huen Ip +7

(144977) 2005 EC127 is an V-/A-type inner-main-belt asteroid with a diameter of 0.6 +- 0.1 km. Asteroids of this size are believed to have rubble-pile structure, and, therefore, ca…