M.P.E.C. statistics for 290

Observed objects

Nr.	Object	Discovery	Stations	Obs all	Obs 290	Obs percent	Note
1	`J94L00Y`		11	84	5	6 %
2	`J99T05B`		18	165	4	2 %
3	`J99U00Q`		20	141	3	2 %
4	`K00O67M`		2	10	2	20 %
5	`K00O67N`		3	8	2	25 %
6	`K00Y02B`		2	8	2	25 %
7	`K01K54F`	`*`	14	126	3	2 %
8	`K01K66U`	`*`	10	53	3	6 %
9	`K01K66Y`	`*`	18	109	3	3 %
10	`K01K66Z`	`*`	27	240	3	1 %
11	`K01K68D`	`*`	5	20	3	15 %
12	`K01S73Q`		3	13	2	15 %
13	`K02G31W`		4	9	2	22 %
14	`K02G32P`		4	9	2	22 %
15	`K02V85O`		15	96	3	3 %
16	`K03V01E`		20	133	15	11 %
17	`K03V01F`		26	323	16	5 %
18	`K03V01G`		34	370	12	3 %
19	`K03YB8G`		42	527	11	2 %
20	`K04A00E`		11	87	3	3 %
21	`K04A00M`	`*`	5	40	4	10 %
22	`K04B11F`	`*`	8	58	3	5 %
23	`K04B11G`	`*`	31	224	4	2 %
24	`K04B11K`	`*`	8	59	3	5 %
25	`K04E20P`	`*`	29	433	4	1 %
26	`K04F04U`		34	528	6	1 %
27	`K04G00Y`		27	175	6	3 %
28	`K04G02E`	`*`	19	155	5	3 %
29	`K04P02J`		19	218	2	1 %
30	`K04V00B`		51	782	24	3 %
31	`K04V17D`		63	1299	4	0 %
32	`K04Y35J`	`*`	16	129	5	4 %
33	`K05A13D`	`*`	60	704	7	1 %
34	`K05A14H`	`*`	16	162	4	2 %
35	`K05E70N`		25	157	6	4 %
36	`K05Q11Q`		13	100	3	3 %
37	`K05Q30E`		24	179	3	2 %
38	`K05R24V`		12	105	3	3 %
39	`K05S19H`		19	195	3	2 %
40	`K05S26G`		2	26	3	12 %
41	`K05T00C`		6	47	3	6 %
42	`K05T00L`		8	42	3	7 %
43	`K05T15B`		26	207	3	1 %
44	`K05T15E`		22	129	3	2 %
45	`K05T15S`		30	262	4	2 %
46	`K06C10T`		10	80	4	5 %
47	`K06E01B`	`*`	13	71	5	7 %
48	`K06H51Y`		24	262	3	1 %
49	`K06H51Z`		18	115	5	4 %
50	`K06Y00F`		16	182	6	3 %
51	`K07D41M`		25	273	12	4 %
52	`K09A16H`		26	785	3	0 %
53	`K09SA4Q`		33	443	3	1 %
54	`K11V09G`		22	123	3	2 %
55	`K12B01N`		10	88	3	3 %
56	`K12B85X`	`Discovery`	1	31	31	100 %
57	`K12D85S`	`Discovery`	1	45	45	100 %
58	`K12L09K`		12	177	3	2 %
59	`K12V85U`		1	13	13	100 %
60	`K12X16H`	`Discovery`	2	122	113	93 %
61	`K12X17E`		32	450	9	2 %
62	`K12X93S`		21	160	3	2 %
63	`K12Y08J`		6	44	12	27 %
64	`K13A20N`		15	127	9	7 %
65	`K13A27R`		10	59	9	15 %
66	`K13A27S`		25	373	9	2 %
67	`K13A53G`		8	51	12	24 %
68	`K13A60Q`		16	178	9	5 %
69	`K13A60R`		7	60	12	20 %
70	`K13A76S`		6	54	12	22 %
71	`K13A91J`		14	106	12	11 %
72	`K13B18N`		4	65	9	14 %
73	`K13B18P`		7	115	12	10 %
74	`K13B19E`		28	429	3	1 %
75	`K13B70D`		9	91	3	3 %
76	`K13R53Z`		5	38	6	16 %
77	`K13TB7L`		16	190	18	9 %
78	`K13W44A`		16	157	2	1 %
79	`K13X08Y`	`*`	26	428	8	2 %
80	`K13X20Y`		14	95	6	6 %
81	`K14A51E`	`*`	10	88	9	10 %
82	`K14B03A`		11	124	11	9 %
83	`K14C13H`		3	21	5	24 %
84	`K15FB8P`		38	1070	3	0 %
85	`K15G13Z`		19	296	3	1 %
86	`K15N13K`		35	739	7	1 %
87	`K15VA5L`		8	287	3	1 %
88	`K15X00T`		15	238	3	1 %
89	`K15X01R`		5	61	6	10 %
90	`K15X02B`		10	257	3	1 %
91	`K15XQ1F`		11	100	3	3 %
92	`K16E85U`		10	73	2	3 %
93	`K16V03V`		18	387	3	1 %
94	`K16W09W`		22	161	4	2 %
95	`K16W10F`		6	46	4	9 %
96	`K16X02A`		17	131	4	3 %
97	`K17R12B`		6	36	2	6 %
98	`K18B06Y`		4	29	6	21 %
99	`K18X05D`		10	69	12	17 %
100	`K19V04L`		21	139	3	2 %
101	`K19V06F`		14	101	3	3 %
102	`K19W03F`		14	129	3	2 %
103	`K19W04X`		7	71	3	4 %
104	`K19X00F`		8	48	6	13 %
105	`K19X00X`		31	235	3	1 %
106	`K19X01E`		12	66	3	5 %
107	`K21T03K`		14	108	3	3 %
108	`K21U20P`		6	44	3	7 %
109	`K21U70F`		9	56	4	7 %
110	`K21V09C`		7	36	4	11 %
111	`K21V12O`		16	63	4	6 %
112	`K21V26Q`		19	140	3	2 %
113	`K21W01T`		8	63	4	6 %
114	`K21X02T`		6	35	3	9 %
115	`K21X05H`		8	34	3	9 %
116	`K21X05J`		22	148	4	3 %
117	`K21X05Y`		6	45	3	7 %
118	`K21X06L`		14	75	4	5 %
119	`K21X07D`		2	32	29	91 %
120	`K21Y00C`		13	67	4	6 %
121	`K21Y00D`		10	46	4	9 %
122	`K22B06S`		9	85	3	4 %
123	`K22C05G`		15	81	3	4 %
124	`K22C07K`		8	41	3	7 %
125	`K22E04E`		8	34	3	9 %
126	`K22E05R`		14	94	4	4 %
127	`K22R05Q`		19	86	4	5 %
128	`K22T04S`		5	20	3	15 %
129	`K22U01N`		5	17	3	18 %
130	`K22U05E`		5	22	4	18 %
131	`K22U05K`		15	55	3	5 %
132	`K22U06L`		9	58	4	7 %
133	`K22U08T`		8	68	3	4 %
134	`K22U11U`		9	29	3	10 %
135	`K22U14S`		10	54	3	6 %
136	`K22U14V`		5	40	3	8 %
137	`K22U16H`		7	39	4	10 %
138	`K22U16R`		11	55	3	5 %
139	`K22U20V`		8	30	4	13 %
140	`K22U21N`		8	37	8	22 %
141	`K22U21Q`		7	32	3	9 %
142	`K22U21R`		7	32	3	9 %
143	`K22U21S`		17	69	4	6 %
144	`K22U21X`		16	98	7	7 %
145	`K22U22C`		25	155	4	3 %
146	`K22U24Y`		11	39	4	10 %
147	`K22U28C`		10	51	3	6 %
148	`K22U28P`		4	23	4	17 %
149	`K22U34A`		5	45	3	7 %
150	`K22V00A`		8	26	3	12 %
151	`K22V00C`		10	41	4	10 %
152	`K22V00E`		7	28	4	14 %
153	`K22V00F`		18	98	4	4 %
154	`K22V00J`		10	51	3	6 %
155	`K23G00O`		5	44	3	7 %
156	`K23H02H`		10	55	4	7 %
157	`K23H04P`		9	44	7	16 %
158	`K23H07J`		11	44	3	7 %
159	`K23H18O`		43	363	4	1 %
160	`K23J01M`		8	56	7	13 %
161	`K23J02O`		10	64	3	5 %
162	`K23J02R`		9	71	3	4 %
163	`K23K02M`		5	34	4	12 %
164	`K23K04A`		10	44	3	7 %
165	`K23K05H`		6	38	6	16 %
166	`K23K05L`		9	43	4	9 %
167	`K23K05N`		5	26	4	15 %
168	`K23Y02B`		11	79	3	4 %
169	`K24A03L`		15	68	3	4 %
170	`K24B00F`		14	82	3	4 %
171	`K24B00J`		21	86	3	3 %
172	`K24B00R`		5	19	3	16 %
173	`K24B02S`		9	25	3	12 %
174	`K24B02U`		8	44	3	7 %
175	`K25F04G`		14	56	3	5 %
176	`K25F05U`		12	119	3	3 %
177	`K25F16S`		7	33	3	9 %
178	`K25F22Y`		7	29	7	24 %
179	`K25G00X`		11	62	4	6 %
180	`K25G01K`		6	32	7	22 %
181	`CK01K050`		93	3305	2	0 %	comet
182	`CK04P42Y`		2	6	4	67 %	comet
183	`CK06S030`		212	6501	16	0 %	comet
184	`CK09P010`		183	9156	8	0 %	comet
185	`CK10R010`		85	1619	7	0 %	comet
186	`CK11UU5F`		101	2304	4	0 %	comet
187	`CK12K010`		185	7892	26	0 %	comet
188	`CK12S010`		201	6754	21	0 %	comet
189	`CK12T050`		63	699	3	0 %	comet
190	`CK12V020`		70	1108	4	0 %	comet
191	`CK12X010`		105	2669	7	0 %	comet
192	`CK13A010`		136	3614	8	0 %	comet
193	`CK14Q020`		159	7961	10	0 %	comet
194	`CK22E030`		193	8265	7	0 %	comet
195	`PK01J010`		7	33	3	9 %	comet
196	`PK05Q040`		25	221	5	2 %	comet
197	`PK13TB7L`		50	912	18	2 %	comet
198	`0026P`		52	538	3	1 %	comet
199	`0032P`		227	5093	6	0 %	comet
200	`0063P`		103	1891	4	0 %	comet
201	`0168P`		140	3539	4	0 %	comet
202	`0175P`		53	666	6	1 %	comet
203	`05645`		66	1831	3	0 %
204	`07350`		79	2542	6	0 %
205	`10115`		62	2450	3	0 %
206	`12711`		97	3623	3	0 %
207	`22753`		63	1750	3	0 %
208	`29075`		43	1135	23	2 %
209	`68216`		113	4406	4	0 %
210	`68278`		50	2457	6	0 %
211	`87684`		51	2517	3	0 %
212	`99942`		193	11058	21	0 %
213	`A1955`		22	598	4	1 %
214	`D6793`		32	737	7	1 %
215	`D6993`		34	894	3	0 %
216	`D8911`		37	975	32	3 %
217	`E4411`		49	1278	3	0 %
218	`F3220`		7	187	3	2 %
219	`F3958`		44	876	3	0 %
220	`G2004`		58	2062	3	0 %
221	`G2783`		5	49	3	6 %
222	`G3249`		61	2231	24	1 %
223	`G3364`		36	718	3	0 %
224	`S5263`		81	3107	7	0 %
225	`U3262`		26	613	3	0 %
226	`X7558`		8	83	4	5 %
227	`X9714`		23	267	3	1 %
228	`Y1050`		13	334	33	10 %
229	`Z0713`		14	255	7	3 %
Sum	`229 objects`			148192	1460	1 %	22 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 290 are all observations in all MPECs for this station. Obs percent is the percentage of stations observation to all observations.

290 has discovered 3 objects. It has made 1460 of all 148192 observations (1 %) at 229 objects in all MPECs with involved station 290. There are 144 of all 4748 observations (3 %) at 20 objects in all discovery MPECs with involved station 290.

All MPECs for station 290

Discovery MPEC for station 290

All observations for station 290

Created with MPECSGET.