Table A.2
Asteroids found as a match to the powder and raw slab samples of EC 002 with a curve-matching method.
Asteroid | Acceptance | Notes | Type | Method | Ref. |
---|---|---|---|---|---|
(6853) Silvanomassaglia | 1 | - | V | Phot. NIR | 17 |
(10156) 1994 VQ7 | 1 | - | V | Phot. VIS | 24 |
(13743) Rivkin | 0 | shorter band I centre | V | Phot. VIS | 24 |
(16856) Banach | 1 | - | S | Phot. VIS | 24 |
(17056) Boschetti | 1 | - | S | Phot. VIS | 24 |
(20289) Nettimi | 0 | noisy and unclear band I | - | - | - |
(20454) Pedrajo | 1 | - | S | Phot. VIS | 24 |
(23522) 1992 WC9 | 0 | shorter band I centre | V | Phot. NIR | 17 |
(24143) 1999 VY124 | 0 | noisy | C | Phot. VIS | 24 |
(24892) 1997 AD3 | 1 | - | - | - | - |
(26399) Rileyennis | 0 | shorter band I centre | - | - | - |
(26420) 1999 XL103 | 0 | shorter band I centre | V | Phot. VIS | 23 |
(27106) Jongoldman | 0 | shorter band I centre | V | Phot. VIS | 24 |
(27627) 2038 P-L | 0 | shorter band I centre | V | Phot. VIS | 24 |
(30000) Camenzind | 0 | shallow slope | V | Phot. VIS | 10, 23, 24 |
(30081) Zarinrahman | 0 | shorter band I centre | S | Phot. VIS | 24 |
(38690) 2000 QS29 | 0 | unclear band I | S | Phot. VIS | 24 |
(40693) 1999 RX229 | 0 | unclear band I | C | Phot. VIS | 24 |
(44691) 1999 RF221 | 0 | shallow slope | C | Phot. VIS | 24 |
(47327) 1999 XZ25 | 0 | shorter band I centre | V | Phot. VIS | 10, 23 |
(48632) 1995 SV29 | 0 | shorter band I centre | V | Phot. VIS | 10 |
(50488) 2000 DA86 | 0 | shallow slope | - | - | - |
(51659) Robohachi | 0 | noisy | S | Phot. VIS | 24 |
(51688) 2001 KW12 | 0 | shorter band I centre | S | Phot. VIS | 24 |
(53561) 2000 CM22 | 0 | noisy and unclear band I | S | Phot. VIS | 24 |
(54062) 2000 GX135 | 1 | noisy but plausible | C | Phot. VIS | 24 |
(55549) 2001 XC59 | 1 | S | Phot. VIS | 24 | |
(55866) 1997 PV4 | 0 | shallow slope | V | Phot. VIS | 24 |
(59686) 1999 JS108 | 0 | shorter band I centre | - | - | - |
(61169) 2000 NY20 | 0 | band red and blue parts | X | Phot. VIS | 24 |
(63653) 2001 QQ109 | 1 | - | - | - | - |
(64181) 2001 TS64 | 0 | shorter band I centre | V | Phot. VIS | 23 |
(68814) 2002 GP66 | 0 | shallow slope | - | - | - |
(77147) 2001 EV6 | 1 | bad two last points | S | Phot. VIS | 24 |
(77590) 2001 KM17 | 0 | shorter band I centre | V | Phot. NIR | 17 |
(77935) 2002 GM54 | 1 | noisy but plausible | V | Phot. VIS | 24 |
(78034) 2002 JF82 | 0 | shorter band I centre | V | Phot. VIS | 7 |
(80924) 2000 DJ73 | 0 | noisy and unclear band I | C | Phot. VIS | 24 |
(81448) 2000 GV123 | 0 | shallow slope | S | Phot. VIS | 24 |
(87010) 2000 JR55 | 0 | shallow slope | C | Phot. VIS | 24, 24 |
(88955) 2001 TW42 | 1 | - | S | Phot. VIS | 24 |
(89556) 2001 XS98 | 1 | except for last points | - | - | - |
(93893) 2000 WL141 | 0 | unclear band I | S | Phot. VIS | 10, 23, 24 |
(96353) 1997 VF3 | 0 | flatter spectrum | C | Phot. VIS | 24 |
(99722) 2002 JW46 | 0 | flatter spectrum | S | Phot. VIS | 24 |
(102107) 1999 RL164 | 0 | shorter band I centre | V | Phot. VIS | 10 |
(103308) 2000 AH55 | 0 | unclear band I | - | - | - |
(119144) 2001 PH32 | 0 | unclear band I | V | Phot. VIS | 10, 23 |
(123113) 2000 SH361 | 1 | - | V | Phot. VIS | 23 |
(124884) 2001 TE41 | 1 | - | V | Phot. VIS | 10, 23 |
(130988) 2000 WT141 | 0 | NEA | V | Spec. VIS | 13 |
(147124) 2002 TH129 | 0 | less pronounced band | - | - | - |
(149372) 2002 XC71 | 0 | bad agreement before 700 nm | - | - | - |
(153408) 2001 QV137 | 0 | shorter band I centre | - | - | - |
(164121) 2003 YT1 | 1 | RP noisy but plausible | V | Spec. VISNIR | 12 |
(194248) 2001 TA199 | 0 | flatter spectrum | - | - | - |
(205560) 2001 SC282 | 1 | noisy but plausible | - | - | - |
(310436) 2000 AB169 | 1 | noisy but plausible | - | - | - |
Note: The information in the table are the number and name of the 58 asteroids, if they are accepted or not as a good match for EC 002 (1 if accepted, 0 if not), some notes about the visual inspection, the spectral type of the asteroid if determined and the method and relevant references associated (Ref. column). The taxonomic scheme used for the type of each asteroid is the one used in the reference papers associated. Spec. stands for Spectroscopy and Phot. for Photometry.
Note: The references are (1) Xu et al. (1995), (2) Bus & Binzel (2002), (3) Lazzaro et al. (2004), (4) Alvarez-Candal et al. (2006), (5) DeMeo et al. (2009), (6) Moskovitz et al. (2010), (7) Carvano et al. (2010), (8) de Sanctis et al. (2011), (9) Solontoi et al. (2012), (10) DeMeo & Carry (2013), (11) Jasmim et al. (2013), (12) Sanchez et al. (2013), (13) Ribeiro et al. (2014), (14) Lindsay et al. (2015), (15) Carry et al. (2016), (16) Hardersen et al. (2018), (17) Popescu et al. (2018), (18) Medeiros et al. (2019), (19) DeMeo et al. (2019), (20) Binzel et al. (2019), (21) Matlovič et al. (2020), (22) Migliorini et al. (2021), (23) Sergeyev & Carry (2021), (24) Sergeyev et al. (2022), (25) Mahlke et al. (2022)
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