Table A.1
Observing setup and circumstances for VIS spectra.
| Asteroid | Telescope | Grism | Slit width | Observing | Phase | Air | Solar Analog | Airm | Ref. | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|
| (arcsec) | night | angle (deg) | mass | mass | VIS | NIR | ||||
| 1914 Hartbeespoortdam | NOT | 11 | 1.3 | 2019-04-22 | 14.3 | 1.32 | SA 110-361 | 1.34 | (1) | (2) |
| 2704 Julian Loewe | NOT | 11 | 1.3 | 2019-06-09 | 6.7 | 1.60 | HD 133011 | 1.47 | (3) | |
| 2798 Vergilius | NOT | 11 | 1.3 | 2019-04-22 | 5.0 | 1.67 | SA102-1081 | 1.66 | ||
| 2823 Van der Laan | NOT | 11 | 1.3 | 2019-06-09 | 6.2 | 1.59 | HD 140990 | 1.60 | (4) | |
| 3302 Schliemann | NOT | 11 | 1.3 | 2019-06-09 | 26.1 | 1.49 | HD 203311 | 1.50 | ||
| 3331 Kvitasberg | NOT | 11 | 1.3 | 2019-04-22 | 17.3 | 1.06 | HD 77730 | 1.08 | ||
| 4434 Nikulin | NOT | 12 | 1.3 | 2018-04-03 | 9.0 | 1.26 | Land 107-998 | 1.24 | (3) | (5) |
| 5037 Habing | NOT | 11 | 1.3 | 2018-09-16 | 14.7 | 1.41 | HD 210078 | 1.36 | (6) | |
| 5235 Jean-Loup | NOT | 11 | 1.3 | 2018-09-16 | 19.2 | 1.06 | 51 Peg | 1.13 | (7) | |
| 5525 (1991 TS4) | NOT | 11 | 1.3 | 2018-09-16 | 25.4 | 1.35 | Hyades 64 | 1.21 | (6) | |
| 5560 Amytis | NOT | 11 | 1.3 | 2018-09-16 | 7.4 | 1.51 | HIP 11915 | 1.41 | (6) | (7) |
| 5754 (1992 FR2) | SALT | PG0300 | 3.0 | 2017-11-27 | 17.5 | 1.22 | HD 11532 | 1.2 | (8) | |
| 6819 McGarvey | NOT | 11 | 1.3 | 2018-09-16 | 17.9 | 1.58 | 51 Peg | 1.34 | ||
| 7558 Yurlov | NOT | 12 | 1.3 | 2018-04-03 | 27.2 | 1.32 | Land 102-1081 | 1.18 | (9) | |
| 8645 (1988 TN) | LDT | 150 1/mm | 3 | 2020-01-08 | 7.1 | 1.01 | SA 102-1081 | 1.43 | ||
| LDT | PRISM | 1.34 | 2020-01-08 | 7.1 | 1.05 | SA 102-1081 | 1.4 | |||
| 9652 (1996 AF2) | NOT | 11 | 1.3 | 2019-04-22 | 9.3 | 1.43 | HD 117860 | 1.44 | ||
| 17057 (1999 GS4) | NOT | 11 | 1.3 | 2018-09-16 | 15.5 | 1.32 | HD 209847 | 1.36 |
Notes. Columns are: asteroid designation, telescope, grisms, slit width, observing night, asteroid phase angle, asteroid air mass at the start of exposures, solar analogs used, air masses of the solar analogs at the start of exposures. References are given for the first publication of each asteroid spectrum.
References. (1) Alvarez-Candal et al. (2006), (2) Fulvio et al. (2016), (3) Bus & Binzel (2002), (4) Moskovitz et al. (2010), (5) Duffard et al. (2004), (6) Solontoi et al. (2012), (7) Hardersen et al. (2014b), (8) Hardersen et al. (2018), (9) Moskovitz et al. (2008b).
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