M.P.E.C. statistics for W05

Observed objects

Nr.	Object	Discovery	Stations	Obs all	Obs W05	Obs percent	Note
1	`K04H12F`		39	303	3	1 %
2	`K06Q57Z`		17	89	5	6 %
3	`K11V09G`		22	123	3	2 %
4	`K21X06B`		30	141	3	2 %
5	`K24P05T`		44	410	2	0 %
6	`K24U00W`		8	63	26	41 %
7	`K24U11T`		18	144	80	56 %
8	`K24W00B`	`*`	54	448	4	1 %
9	`K24W01P`		16	54	10	19 %
10	`K24X00H`		17	66	8	12 %
11	`K24Y01U`		29	159	3	2 %
12	`K24Y04S`		9	72	3	4 %
13	`K25A00B`	`*`	21	95	2	2 %
14	`K25A02O`		11	40	2	5 %
15	`K25C04H`	`*`	39	210	3	1 %
16	`K25D00E`	`*`	47	228	3	1 %
17	`K25D01D`	`*`	41	217	2	1 %
18	`K25D07U`		16	84	2	2 %
19	`K25E00L`	`*`	9	53	4	8 %
20	`K25E00X`	`*`	37	180	3	2 %
21	`K25E01A`		42	205	3	1 %
22	`K25E01S`	`*`	58	339	3	1 %
23	`K25E02F`		19	68	3	4 %
24	`K25E03V`	`*`	14	59	3	5 %
25	`K25E04A`	`*`	13	69	7	10 %
26	`K25E04F`	`*`	36	308	16	5 %
27	`K25E04K`	`*`	12	50	4	8 %
28	`K25F00A`	`*`	47	327	3	1 %
29	`K25F15A`		13	51	6	12 %
30	`K25F18F`	`*`	12	34	2	6 %
31	`K25F28K`	`*`	8	44	3	7 %
32	`K25G00D`	`*`	44	268	3	1 %
33	`K25G00N`	`*`	32	129	2	2 %
34	`K25G01D`		23	113	4	4 %
35	`K25G01H`	`*`	9	38	3	8 %
36	`K25G01Q`	`*`	24	126	18	14 %
37	`K25H00A`		22	75	3	4 %
38	`K25H00B`	`*`	19	69	9	13 %
39	`K25H00C`	`*`	18	66	10	15 %
40	`K25H00G`	`*`	9	26	3	12 %
41	`K25H00U`	`*`	10	46	9	20 %
42	`K25H04P`	`*`	22	80	3	4 %
43	`K25H06Z`	`*`	18	64	2	3 %
44	`K25J00A`	`*`	37	159	6	4 %
45	`K25J00C`	`*`	30	118	3	3 %
46	`K25J01B`	`*`	30	126	3	2 %
47	`K25K00D`	`*`	40	205	3	1 %
48	`K25K01B`	`*`	38	150	3	2 %
49	`K25M00H`	`*`	22	84	3	4 %
50	`K25M02A`		19	63	3	5 %
51	`K25M89L`	`*`	22	80	3	4 %
52	`K25N00M`	`*`	13	47	3	6 %
53	`K25O04R`		21	105	3	3 %
54	`K25O04T`		28	139	3	2 %
55	`K25O04V`		17	62	3	5 %
56	`K25O05Q`		29	121	9	7 %
57	`K25P00M`		20	80	3	4 %
58	`K25P01O`	`*`	6	20	6	30 %
59	`K25P01Q`	`*`	11	38	3	8 %
60	`K25P01Y`		25	85	6	7 %
61	`K25P02B`		10	36	3	8 %
62	`K25Q00A`		25	106	3	3 %
63	`K25Q00D`	`*`	10	29	3	10 %
64	`K25Q01K`	`*`	16	74	3	4 %
65	`K25Q04V`	`*`	28	98	3	3 %
66	`K25Q04X`	`*`	16	54	3	6 %
67	`K25Q04Y`	`*`	28	94	3	3 %
68	`K25Q05A`	`*`	10	42	6	14 %
69	`K25Q05B`	`*`	22	85	3	4 %
70	`K25Q05C`	`*`	10	34	3	9 %
71	`K25Q07K`	`*`	26	94	3	3 %
72	`K25Q09M`	`*`	9	31	3	10 %
73	`K25Q09W`	`*`	10	39	3	8 %
74	`K25Q12R`	`*`	34	172	3	2 %
75	`K25Q13G`	`*`	22	72	3	4 %
76	`K25Q16E`	`*`	46	195	3	2 %
77	`K25Q21B`	`*`	35	181	3	2 %
78	`K25R00K`	`*`	25	85	2	2 %
79	`K25R01R`	`*`	22	112	3	3 %
80	`K25R01W`	`*`	13	58	3	5 %
81	`K25R01Y`	`*`	30	148	3	2 %
82	`K25R01Z`	`*`	15	66	3	5 %
83	`K25R02D`	`*`	21	87	3	3 %
84	`K25R02N`	`*`	15	47	3	6 %
85	`K25S01O`	`*`	27	110	12	11 %
86	`K25S01Z`	`*`	18	64	3	5 %
87	`K25S04F`	`*`	24	117	3	3 %
88	`K25S05T`	`*`	11	41	3	7 %
89	`K25S15G`	`*`	30	156	6	4 %
90	`K25S15J`	`*`	25	104	3	3 %
91	`K25S20N`	`*`	25	80	3	4 %
92	`K25T02O`	`*`	14	52	5	10 %
93	`K25T05O`	`*`	34	126	3	2 %
94	`K25T05P`	`*`	29	109	3	3 %
95	`K25T05Q`	`*`	26	82	3	4 %
96	`K25T10Q`	`*`	28	97	3	3 %
97	`K25U00E`	`*`	9	49	3	6 %
98	`K25U03J`	`*`	6	45	2	4 %
99	`K25U05J`	`*`	19	62	2	3 %
100	`K25U06G`	`*`	6	52	6	12 %
101	`K25U12F`	`*`	17	68	6	9 %
102	`K25V00D`	`*`	16	51	3	6 %
103	`K25V00P`	`*`	31	112	6	5 %
104	`K25V00Q`	`*`	10	35	3	9 %
105	`K25V02P`	`*`	26	111	3	3 %
106	`K25V03J`	`*`	25	106	3	3 %
107	`K25V03L`		9	40	2	5 %
108	`K25V04Y`	`*`	9	37	2	5 %
109	`K25V04Z`	`*`	9	35	3	9 %
110	`K25V05D`	`*`	10	36	2	6 %
111	`K25V05M`	`*`	13	83	5	6 %
112	`K25W00K`	`*`	10	37	2	5 %
113	`K25W01T`	`*`	13	45	3	7 %
114	`K25W02C`	`*`	14	53	2	4 %
115	`K25W04J`	`*`	39	170	3	2 %
116	`K25W06J`	`*`	18	64	3	5 %
117	`K25W06M`	`*`	7	26	2	8 %
118	`K25W19W`	`*`	4	24	3	13 %
119	`K25Y03C`	`*`	11	37	3	8 %
120	`K25Y03D`	`*`	9	44	3	7 %
121	`K25Y03J`	`*`	16	73	3	4 %
122	`K25Y05F`	`*`	22	78	3	4 %
123	`K25Y05T`	`*`	14	64	3	5 %
124	`K25Y09S`	`*`	10	33	3	9 %
125	`K26A00E`	`*`	34	124	5	4 %
126	`K26A00N`	`*`	16	54	3	6 %
127	`K26A01O`	`*`	20	222	3	1 %
128	`K26A02L`	`*`	8	37	3	8 %
129	`K26A02M`	`*`	10	30	4	13 %
130	`K26A02W`	`*`	27	116	6	5 %
131	`K26A04E`	`*`	12	44	3	7 %
132	`K26A04H`	`*`	20	118	3	3 %
133	`K26B00U`	`*`	10	44	3	7 %
134	`K26B02H`	`*`	15	65	3	5 %
135	`K26B02N`	`*`	23	101	3	3 %
136	`K26B03V`	`*`	17	88	2	2 %
137	`K26B04W`	`*`	16	56	2	4 %
138	`K26C00C`	`*`	27	118	6	5 %
139	`K26C00G`	`*`	34	183	3	2 %
140	`K26C01W`	`*`	5	20	3	15 %
141	`K26C02A`	`*`	8	26	2	8 %
142	`K26D00D`	`*`	20	68	3	4 %
143	`K26D00L`	`*`	53	209	3	1 %
144	`K26D05L`	`*`	13	48	3	6 %
145	`K26D07B`	`*`	24	91	3	3 %
146	`K26D14F`	`*`	16	56	3	5 %
147	`K26D14M`	`*`	15	64	3	5 %
148	`K26D14U`	`*`	32	180	3	2 %
149	`K26D14X`	`*`	24	93	3	3 %
150	`K26D15M`	`*`	27	171	2	1 %
151	`K26D16K`		12	73	2	3 %
152	`K26D27F`	`*`	18	83	3	4 %
153	`K26E00C`	`*`	40	172	3	2 %
154	`K26E00F`	`*`	17	63	3	5 %
155	`K26E00G`	`*`	30	122	3	2 %
156	`K26E01Q`	`*`	19	60	2	3 %
157	`K26E02Z`	`*`	18	90	3	3 %
158	`K26F00B`	`*`	28	114	3	3 %
159	`K26F00S`	`*`	35	161	2	1 %
160	`K26F03E`	`*`	44	179	3	2 %
161	`K26F03Q`	`*`	12	82	3	4 %
162	`K26F05K`	`*`	15	70	3	4 %
163	`K26F12Q`		35	140	3	2 %
164	`K26G00B`	`*`	38	190	2	1 %
165	`K26G01T`	`*`	19	94	3	3 %
166	`K26H02F`	`*`	14	67	2	3 %
167	`K26H03A`	`*`	10	40	3	8 %
168	`K26H04J`	`*`	32	146	3	2 %
169	`K26J00A`	`*`	12	70	3	4 %
170	`K26J03K`	`*`	8	29	3	10 %
171	`K26J04U`	`*`	16	47	3	6 %
172	`K26L00E`		18	87	6	7 %
173	`K26M00F`	`*`	42	229	3	1 %
174	`K26M03S`	`*`	19	69	3	4 %
175	`AK25Y010`		51	422	9	2 %	comet
176	`CK25J010`	`*`	68	922	8	1 %	comet
177	`CK25M020`	`*`	29	334	3	1 %	comet
178	`CK25O020`	`*`	17	88	6	7 %	comet
179	`CK25Q030`	`*`	118	1443	3	0 %	comet
180	`CK25R030`	`*`	86	910	5	1 %	comet
181	`CK25T010`	`*`	73	826	3	0 %	comet
182	`CK25V010`	`*`	27	117	3	3 %	comet
183	`CK25V020`	`*`	49	563	3	1 %	comet
184	`CK25Y010`		86	1292	9	1 %	comet
185	`CK26A010`	`*`	77	1067	14	1 %	comet
186	`CK26A020`		55	519	8	2 %	comet
187	`CK26B020`	`*`	31	191	6	3 %	comet
188	`CK26B030`	`*`	57	476	3	1 %	comet
189	`CK26C010`	`*`	100	865	3	0 %	comet
190	`CK26H020`	`*`	52	356	3	1 %	comet
191	`PK25UA9X`	`*`	18	127	8	6 %	comet
192	`PK26C020`	`*`	39	186	5	3 %	comet
193	`0003I`		337	8518	5	0 %
194	`0128P`		77	865	3	0 %	comet
195	`L9071`		95	2903	12	0 %
Sum	`195 objects`			40255	845	2 %	19 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 W05 are all observations in all MPECs for this station. Obs percent is the percentage of stations observation to all observations.

W05 has discovered 0 objects. It has made 845 of all 40255 observations (2 %) at 195 objects in all MPECs with involved station W05. There are 566 of all 10943 observations (5 %) at 158 objects in all discovery MPECs with involved station W05.

All MPECs for station W05

Discovery MPEC for station W05

All observations for station W05

Created with MPECSGET.