Observations, compositional, and physical characterization of near-Earth and Mars-crosser asteroids from a spectroscopic survey

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Table 1:

Solar analogue stars used to obtain the reflectance spectra of the asteroids of this survey.
Star	$\alpha$ (J2000)	$\delta$ (J2000)	V	B-V	V-K	J-H	H-K	Spectral type
Hyades 64^a	04:26:40.1	+16:44:49	8.090	0.657	1.543	0.250	0.096	G2 V
Landolt SA 93-101	01:53:18.0	+00:22:25	9.720^b	0.650^b	1.548	0.309	0.098	G5
Landolt SA 98-978	06:51:34.0	-00:11:28	10.570^c	0.609^c	1.399	0.255	0.084	F8
Landolt SA 102-1081	10:57:04.4	-00:13:10	9.903^c	0.664^c				G2^b
Landolt SA 107-684	15:37:18.1	-00:09:50	8.433^d	0.619^d	1.603	0.263	0.122	G0
Landolt SA 107-998	15:38:16.4	+00:15:23	10.440^b	0.630^b	1.600	0.255	0.117	G3^b
Landolt SA 110-361	18:42:45.0	+00:08:04	12.425^c	0.632^c	1.565	0.285	0.066
Landolt SA 112-1333	20:43:11.8	+00:26:15	9.990^b	0.620^b	1.526	0.248	0.115	F8
Landolt SA 115-271	23:42:41.8	+00:45:10	9.695^c	0.615^c	1.557	0.258	0.121	F8
P330E	16:31:33.8	+30:08:47	13.010	0.620	1.500	0.280	0.060	G0 V
Hardorp^e	-	-	-	0.663	1.490	0.310	0.060
Sun^f								G2 V
C85	-	-	-	-	1.486	0.310	0.060
C96	-	-	-26.75	0.630	1.500	0.310	0.060
HD02	-	-	-	0.641	1.486	0.230	0.060
H80	-	-	-26.71	0.665	-	-	-

Notes. ^(a) Solar analogue star Hyades 64 belongs to class 1 following Hardorp (1978), i.e., it is considered as perfect solar analogue. V magnitude and B-V colour for this star were taken from that paper; ^(b) data extracted from Landolt (1973); ^(c) colours extracted from Landolt (1992); ^(d) colours extracted from Landolt (1983); ^(e) mean values from the list of Campins et al. (1985) of solar analogue stars belonging to Hardorp's class 1; ^(f) colours of the Sun following different authors: C85 $\equiv$ Campins et al. (1985); C96 $\equiv$ Colina et al. (1996); H02 $\equiv$ Hainaut & Delsanti (2002); H80 $\equiv$ Hardorp (1980).

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