Gaia and IRTF abundance of A-type main-belt asteroids

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Table B.1

Forty-four main belt and Mars-crosser asteroids classified as A-types in the literature using their VIS and NIR part of the spectrum that are also incl

Asteroid	Family	a	e	sin(i)	p_V	σ p_V	Reference
113 Amalthea	Flora	2.37786	0.08556	0.08785	0.235	0.0092	1
246 Asporina	-	2.69391	0.10849	0.26928	0.166	0.0088	2,3
289 Nenetta	-	2.87556	0.20191	0.11634	0.270	0.0369	2
354 Eleonora	-	2.79959	0.11149	0.31501	0.192	0.0093	2,3
446 Aeternitas	-	2.78836	0.12512	0.18423	0.269	0.0076	2
863 Benkoela	-	3.20099	0.02764	0.42912	0.367	0.0052	2
984 Gretia	-	2.80521	0.19537	0.15804	0.346	0.0191	1
1122 Neith	-	2.60807	0.25508	0.08248	0.371	0.0204	4
1709 Ukraina	-	2.37907	0.21338	0.13146	0.160	0.0198	1
2501 Lohja	-	2.42118	0.19785	0.05753	0.244	0.0317	2
3819 Robinson	-	2.77292	0.14012	0.19279	0.358	0.2982	5
4125 LewAllen	-	1.92131	0.11818	0.34926	0.160	0.0216	6
4142 Dersu-Uzala	-	1.91166	0.15111	0.44611	0.224	0.0288	7
4402 Tsunemori	-	2.89017	0.02267	0.13426	0.367	0.0760	1
4490 Bambery	-	1.93084	0.09229	0.44028	0.205	0.0055	6
5641 McCleese	-	1.81995	0.12622	0.37782	0.185	0.0208	7
6067 1990 QR11	-	3.16302	0.04871	0.18186	0.256	0.0605	5
7468 Anfimov	Anfimov	3.04235	0.12040	0.07634	0.257	0.0391	5
7579 1990TN1	Hungaria	1.97822	0.06583	0.29201	0.518	0.1150	8
8838 1989 UW2	-	3.14202	0.00745	0.19324	0.246	0.0195	5,6
9983 Rickfienberg	-	2.70619	0.11650	0.14464	0.165	0.0328	5
10715 Nagler	-	2.63329	0.27376	0.30364	0.309	0.0399	5,6
10977 Mathlener	-	2.23745	0.02405	0.02413	0.327	0.0922	6
16520 1990 WO3	Flora	2.27497	0.16065	0.08567	0.325	0.1776	5,6
17818 1998 FE118	-	2.77003	0.05269	0.15903	0.217	0.0400	5,6
17889 Liechty	-	2.40783	0.10558	0.08096	0.460	0.0524	5,6
18853 1999 RO92	Anfimov	3.06203	0.09723	0.06893	0.302	0.0494	5,6
19652 Saris	Hoffmeister	2.77542	0.06044	0.07191	0.242	0.0100	5,6
21809 1999 TG19	-	2.69442	0.01652	0.06401	0.168	0.0356	5,6
23615 1996 FK12	-	1.96056	0.10049	0.38565	0.223	0.0230	5
31393 1998 YG8	-	2.19463	0.01918	0.06153	0.467	0.1164	5,6
33763 1999 RB84	1999 XT17	2.94534	0.07571	0.18242	-	-	9
34969 4108T-2	Flora	2.26635	0.09135	0.08256	-	-	6
35925 1999 JP104	-	2.43812	0.10853	0.19865	0.176	0.0201	5,6
36256 1999 XT17	1999 XT17	2.93727	0.12373	0.19056	0.186	0.0330	5,6
52228 Protos	-	3.20469	0.12401	0.46842	0.271	0.1763	6
52726 1998 GY6		2.84758	0.03831	0.30342	-	-	5
60631 2000 FC26	-	2.71579	0.11666	0.18269	0.218	0.0736	5,6
75810 2000 AX244	-	2.47639	0.10275	0.06741	0.275	0.0674	5,6
92516 2000 ND25	-	2.18750	0.07058	0.10843	-	-	5,6
95560 2002 EX98	-	2.64959	0.11952	0.38285	0.294	0.0754	5,6
105840 2000 SK155	-	3.07764	0.23761	0.10689	-	-	5,6
139045 2001 EQ9	-	2.30958	0.13943	0.07845	-	-	6
142040 2002 QE15	-	1.66706	0.34452	0.47337	0.340	0.0400	10,11

Notes. The reported semimajor axis (a), eccentricity (e), sin of the inclination (i) as well as the uncertainty-weighted geometric visible albedo (p_V) with this uncertainty were retrieved from Minor Planet Physical Properties Catalogue. The family membership is taken from Nesvorný et al. (2015). The reference corresponds to the study that reported the A-type classification as follows: (1) Mahlke et al. (2022), (2) DeMeo et al. (2009), (3) Gietzen et al. (2012), (4) Fornasier et al. (2011), (5) Hasegawa et al. (2024), (6) DeMeo et al. (2019), (7) Binzel et al. (2004), (8) Fornasier et al. (2008), (9) Galinier et al. (2024), (10) de León et al. (2010), (11) Lazzarin et al. (2005).

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