A polarimetric study of asteroids in comet-like orbits

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Volume 658 (February 2022)

A&A, 658 (2022) A158

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Table B.1

Observation circumstance of photometric data

Date	UT	Telescope	Filter	Exptime^a	N^b	r^c	Δ^d	α^e
				(sec)		(au)	(au)	(deg)
2016-May-26	12:33–13:09	IAO	g′, R_C, I_C	30	76	0.88	0.29	108.6
2016-May-27	11:15–14:03	IAO	g′, R_C, I_C	20	476	0.90	0.28	105.0
2016-Jun-02	11:39–17:48	OAO	g′, R_C, I_C	120	320	1.01	0.28	82.1
2016-Jun-02	13:05–14:17	IAO	g′, R_C, I_C	20	18	1.01	0.28	82.2
2016-Jun-03	11:14–17:43	OAO	g′, R_C, I_C	120	350	1.03	0.29	78.5
2016-Jun-03	11:47–17:16	IAO	g′, R_C, I_C	20	384	1.03	0.29	78.5
2016-Jun-04	13:34–16:58	IAO	g′, R_C, I_C	20	222	1.05	0.29	75.1
2016-Jun-05	11:47–16:20	OAO	g′, R_C, I_C	120	164	1.07	0.30	72.0
2016-Jun-08	13:34–15:52	IAO	g′, R_C, I_C	20	262	1.12	0.33	63.4
2016-Jun-12	13:31–14:55	IAO	g′, R_C, I_C	20	82	1.19	0.38	54.8
2016-Aug-01	20:50	OHP	R_C	300	1	1.90	1.39	31.3
2016-Aug-02	20:23–20:29	OHP	R_C	300	2	1.91	1.41	31.2
2016-Aug-03	20:09–20:19	OHP	R_C	300	3	1.92	1.43	31.0

Notes. The observation circumstance of light curve data taken at Okayama Astrophysical Observatory (OAO) and Ishigakijima Astrophysical Observatory(IAO). We used the web-based JPL Horizons system (http://ssd.jpl.nasa.gov/?horizons) to obtain these quantities. ^(a) Exposure time in sec, ^(b) Number of data obtained, ^(c) Median heliocentric distance in au, ^(d)Median geocentric distance in au, ^(e)Median solar phase angle in deg.

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