M.P.E.C. statistics for L06

Observed objects

Nr.	Object	Discovery	Stations	Obs all	Obs L06	Obs percent	Note
1	`K18C02Y`	`*`	25	164	2	1 %
2	`K18U02C`		36	278	3	1 %
3	`K19O01U`		19	74	3	4 %
4	`K19Q04V`		34	212	3	1 %
5	`K19X00S`		98	1612	5	0 %
6	`K20G02D`		45	416	2	0 %
7	`K21F00B`	`*`	23	149	3	2 %
8	`K21G00C`	`*`	25	112	3	3 %
9	`K21G00F`	`*`	38	212	3	1 %
10	`K21G00G`	`*`	15	66	3	5 %
11	`K21G01D`		36	196	3	2 %
12	`K21G01J`	`*`	23	110	3	3 %
13	`K21G02V`		18	91	3	3 %
14	`K21G03E`	`*`	31	150	3	2 %
15	`K21G03Y`	`*`	16	88	2	2 %
16	`K21G04M`	`*`	25	253	2	1 %
17	`K21G05P`	`*`	13	73	3	4 %
18	`K21J02F`	`*`	10	51	3	6 %
19	`K21K00J`	`*`	14	66	4	6 %
20	`K21K02Q`		13	62	3	5 %
21	`K21K02X`	`*`	12	54	3	6 %
22	`K21L05C`	`*`	30	112	2	2 %
23	`K21M01K`		50	309	6	2 %
24	`K21P10C`	`*`	23	135	3	2 %
25	`K21P10E`	`*`	30	195	3	2 %
26	`K21P24A`	`*`	18	113	2	2 %
27	`K21R07U`		18	97	3	3 %
28	`K21R09U`	`*`	11	44	2	5 %
29	`K21R10U`	`*`	20	77	3	4 %
30	`K21R12G`	`*`	19	67	3	4 %
31	`K21S01Y`	`*`	11	35	3	9 %
32	`K21S01Z`	`*`	12	53	3	6 %
33	`K21S02O`	`*`	19	82	3	4 %
34	`K21S02P`	`*`	9	24	3	13 %
35	`K21S02V`	`*`	15	61	2	3 %
36	`K21S02W`	`*`	7	29	3	10 %
37	`K21T09U`	`*`	10	32	2	6 %
38	`K21T10K`	`*`	9	32	2	6 %
39	`K21U01E`	`*`	11	57	3	5 %
40	`K21U01F`	`*`	16	71	3	4 %
41	`K21U01P`	`*`	11	58	3	5 %
42	`K21W00H`	`*`	19	88	3	3 %
43	`K21W06T`	`*`	11	39	4	10 %
44	`K21W08C`		34	223	3	1 %
45	`K21X03H`	`*`	26	113	4	4 %
46	`K21X04Q`		6	32	3	9 %
47	`K21X04V`	`*`	4	19	7	37 %
48	`K21X04Y`	`*`	23	108	4	4 %
49	`K21X05D`	`*`	8	27	2	7 %
50	`K21X05E`	`*`	13	44	2	5 %
51	`K21Y00Q`	`*`	21	149	3	2 %
52	`K21Y00R`	`*`	17	106	5	5 %
53	`K21Y00S`	`*`	22	160	4	3 %
54	`K22A00Y`		4	25	2	8 %
55	`K22A01B`	`*`	17	84	4	5 %
56	`K22A01C`	`*`	19	94	2	2 %
57	`K22A01D`	`*`	12	50	3	6 %
58	`K22A01E`	`*`	17	88	3	3 %
59	`K22A01F`	`*`	10	48	3	6 %
60	`K22A01K`	`*`	6	34	2	6 %
61	`K22A02B`	`*`	13	55	3	5 %
62	`K22A02C`	`*`	29	160	3	2 %
63	`K22A03M`	`*`	7	24	2	8 %
64	`K22A04A`	`*`	8	35	4	11 %
65	`K22A04B`	`*`	12	51	3	6 %
66	`K22A04C`	`*`	11	40	3	8 %
67	`K22A04D`	`*`	10	46	5	11 %
68	`K22A05E`	`*`	14	72	6	8 %
69	`K22A05V`	`*`	19	103	4	4 %
70	`K22A05Y`		8	27	3	11 %
71	`K22A05Z`	`*`	6	41	4	10 %
72	`K22A06G`	`*`	18	118	2	2 %
73	`K22A08B`	`*`	20	64	4	6 %
74	`K22B00A`	`*`	31	137	3	2 %
75	`K22B00B`	`*`	26	112	2	2 %
76	`K22B00C`	`*`	12	51	3	6 %
77	`K22B00D`	`*`	9	36	3	8 %
78	`K22D00T`		12	48	3	6 %
79	`K22D00U`	`*`	20	96	3	3 %
80	`K22E04V`	`*`	8	33	2	6 %
81	`K22E04W`	`*`	13	44	3	7 %
82	`K22E05J`	`*`	6	23	2	9 %
83	`K22F00C`	`*`	26	117	2	2 %
84	`K22F00F`	`*`	31	130	3	2 %
85	`K22F01H`		16	107	2	2 %
86	`K22F01O`	`*`	12	68	3	4 %
87	`K22F01X`	`*`	15	69	4	6 %
88	`K22F01Y`	`*`	14	60	3	5 %
89	`K22F02C`	`*`	11	51	3	6 %
90	`K22F02D`	`*`	24	170	4	2 %
91	`K22G01N`	`*`	19	75	3	4 %
92	`K22G01Q`	`*`	8	45	3	7 %
93	`K22G01T`	`*`	15	74	4	5 %
94	`K22G01U`	`*`	11	49	3	6 %
95	`K22G01X`	`*`	16	77	2	3 %
96	`K22H02A`	`*`	23	105	3	3 %
97	`K22H02B`	`*`	20	87	4	5 %
98	`K22H02D`	`*`	14	76	2	3 %
99	`K22H02J`	`*`	16	91	3	3 %
100	`K22H03A`	`*`	19	78	3	4 %
101	`K22H03D`	`*`	16	64	3	5 %
102	`K22H03E`	`*`	11	61	3	5 %
103	`K22H03L`	`*`	16	108	3	3 %
104	`AK18W010`	`*`	29	136	4	3 %	comet
105	`CK15E61R`		107	2878	3	0 %	comet
106	`CK16N060`		116	3141	3	0 %	comet
107	`CK16R020`		135	4509	6	0 %	comet
108	`CK17K020`	`*`	173	7900	14	0 %	comet
109	`CK17O010`		105	2901	6	0 %	comet
110	`CK17T010`		75	1073	10	1 %	comet
111	`CK18D04O`	`*`	51	808	6	1 %	comet
112	`CK18N020`	`*`	134	4636	6	0 %	comet
113	`CK18V010`	`*`	39	1410	6	0 %	comet
114	`CK18W010`	`*`	45	308	4	1 %	comet
115	`CK18W020`	`*`	98	2358	22	1 %	comet
116	`CK19D010`	`*`	56	1282	10	1 %	comet
117	`CK19F020`	`*`	74	1199	6	1 %	comet
118	`CK19H010`	`*`	29	307	2	1 %	comet
119	`CK19J020`	`*`	27	491	2	0 %	comet
120	`CK19K080`	`*`	53	1837	6	0 %	comet
121	`CK19L030`		162	5288	3	0 %	comet
122	`CK19M030`	`*`	50	530	6	1 %	comet
123	`CK19Q040`	`*`	52	550	6	1 %	comet
124	`CK19U050`		80	1900	3	0 %	comet
125	`CK19Y040`	`*`	121	4205	12	0 %	comet
126	`CK20A020`		56	546	4	1 %	comet
127	`CK20K010`	`*`	68	1276	2	0 %	comet
128	`CK20K030`	`*`	38	234	3	1 %	comet
129	`CK20M030`		94	1984	3	0 %	comet
130	`CK20Q010`	`*`	42	320	3	1 %	comet
131	`CK20R040`		101	2490	2	0 %	comet
132	`CK20V020`		85	2020	6	0 %	comet
133	`CK20X020`	`*`	35	229	4	2 %	comet
134	`CK20X040`	`*`	19	113	3	3 %	comet
135	`CK20Y030`	`*`	41	388	3	1 %	comet
136	`CK21A010`	`*`	105	2529	9	0 %	comet
137	`CK21A040`	`*`	72	730	3	0 %	comet
138	`CK21D010`		33	379	4	1 %	comet
139	`CK21E030`	`*`	80	945	3	0 %	comet
140	`CK21L030`	`*`	27	166	3	2 %	comet
141	`CK21P040`	`*`	70	697	4	1 %	comet
142	`CK21S010`	`*`	42	356	4	1 %	comet
143	`CK21S040`	`*`	15	67	4	6 %	comet
144	`CK21T010`	`*`	29	117	3	3 %	comet
145	`CK21T020`	`*`	40	183	3	2 %	comet
146	`CK21T040`	`*`	26	158	2	1 %	comet
147	`CK21Y010`	`*`	56	271	3	1 %	comet
148	`CK22A010`	`*`	52	313	4	1 %	comet
149	`CK22A020`	`*`	32	371	4	1 %	comet
150	`CK22A030`	`*`	27	151	4	3 %	comet
151	`PK13PA4A`		17	143	2	1 %	comet
152	`PK18C010`		27	162	2	1 %	comet
153	`PK18H020`	`*`	32	171	3	2 %	comet
154	`PK19A020`	`*`	54	440	6	1 %	comet
155	`PK19B020`	`*`	30	315	6	2 %	comet
156	`PK19L04M`		38	219	2	1 %	comet
157	`PK19R010`	`*`	18	97	3	3 %	comet
158	`PK19Y020`	`*`	60	792	6	1 %	comet
159	`PK20F040`		16	92	2	2 %	comet
160	`PK20G010`	`*`	51	526	3	1 %	comet
161	`PK20W020`	`*`	19	94	2	2 %	comet
162	`PK21L020`	`*`	23	135	2	1 %	comet
163	`PK21N010`	`*`	15	85	4	5 %	comet
164	`PK21N020`	`*`	64	758	4	1 %	comet
165	`PK21Q050`	`*`	41	266	8	3 %	comet
166	`PK21R060`	`*`	18	105	3	3 %	comet
167	`PK21U030`	`*`	42	279	4	1 %	comet
168	`PK22E010`	`*`	15	76	5	7 %	comet
169	`0002I`	`*`	105	2549	15	1 %
170	`0004P`		206	6568	3	0 %	comet
171	`0029P`	`*`	429	37727	3	0 %	comet
172	`0038P`	`*`	113	3102	7	0 %	comet
173	`0046P`	`*`	224	9241	6	0 %	comet
174	`0060P`	`*`	89	1502	3	0 %	comet
175	`0064P`		127	3597	3	0 %	comet
176	`0101P`	`*`	78	1333	3	0 %	comet
177	`0260P`	`*`	161	6590	9	0 %	comet
178	`03200`		225	8985	9	0 %
179	`0398P`		86	1366	5	0 %	comet
180	`0409P`		78	1128	3	0 %	comet
181	`04660`		86	2965	5	0 %
182	`66391`		91	4767	3	0 %
183	`88254`		46	1144	3	0 %
184	`99942`		189	9710	3	0 %
Sum	`184 objects`			184590	701	0 %	75 comets

Stations are all stations in all MPECs, which observed this object. Object is the short name and an asteriks appears for objects, which have been announced in the MPECs as NEO. A discovery by this station is named as Discovery. Obs all are all observations in all MPECs for this object. Obs L06 are all observations in all MPECs for this station. Obs percent is the percentage of stations observation to all observations.

L06 has discovered 0 objects. It has made 701 of all 184590 observations (0 %) at 184 objects in all MPECs with involved station L06. There are 498 of all 42858 observations (1 %) at 143 objects in all discovery MPECs with involved station L06.

All MPECs for station L06

Discovery MPEC for station L06

All observations for station L06

Created with MPECSGET.