Two faces of L-type asteroids - Evidence from UV-VisNIR spectra and CO/CV chondrites

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Table 1

Observational conditions during target acquisition.

Name	Obs. Date	V	α	AM	S	SA
Riviera	2024-04-19	13.8	6.9	1.61	0.8	HD 117939
Welther	2024-09-06	14.4	22.8	1.85	1.1	HD 197027
1987 VT	2024-09-07	16.0	18.2	1.12	1.5	HD 4391
Heco	2024-04-21	17.1	0.9	1.13	0.8	HD 117939
1992 OB	2024-05-11	16.8	2.9	1.08	1.3	18 Sco
Molaro	2024-07-26	16.5	3.4	1.15	0.5	HD 197027
1997 AK₁₇	2024-07-26	17.1	5.8	1.25	0.5	HD 197027
2001 SD₃₁₆	2024-08-15	16.9	10.8	1.61	1.1	HD 197027
2001 CD₄₂	2024-05-02	17.2	2.4	1.15	0.5	HD 117939

Notes. For each target, we provide the date of observation, its visual magnitude V and phase angle α in degrees at the time of observation, the airmass (AM), the seeing (S) in arcseconds, and the solar analogue (SA) used for the calibration.

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