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`		5	37	6	16 %
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	`K12B85X`	`Discovery`	1	31	31	100 %
55	`K12D85S`	`Discovery`	1	45	45	100 %
56	`K12L09K`		12	177	3	2 %
57	`K12V85U`		1	13	13	100 %
58	`K12X16H`	`Discovery`	2	122	113	93 %
59	`K12X17E`		32	446	9	2 %
60	`K12X93S`		12	84	3	4 %
61	`K12Y08J`		6	44	12	27 %
62	`K13A20N`		15	127	9	7 %
63	`K13A27R`		10	59	9	15 %
64	`K13A27S`		25	370	9	2 %
65	`K13A53G`		8	51	12	24 %
66	`K13A60Q`		16	178	9	5 %
67	`K13A60R`		7	60	12	20 %
68	`K13A76S`		6	54	12	22 %
69	`K13A91J`		13	99	12	12 %
70	`K13B18N`		4	65	9	14 %
71	`K13B18P`		7	115	12	10 %
72	`K13B19E`		28	429	3	1 %
73	`K13B70D`		9	91	3	3 %
74	`K13R53Z`		5	38	6	16 %
75	`K13TB7L`		16	190	18	9 %
76	`K13W44A`		16	157	2	1 %
77	`K13X08Y`	`*`	26	428	8	2 %
78	`K13X20Y`		14	85	6	7 %
79	`K14A51E`	`*`	10	88	9	10 %
80	`K14B03A`		11	124	11	9 %
81	`K14C13H`		3	21	5	24 %
82	`K15FB8P`		38	1070	3	0 %
83	`K15G13Z`		19	296	3	1 %
84	`K15N13K`		35	739	7	1 %
85	`K15VA5L`		8	287	3	1 %
86	`K15X00T`		15	238	3	1 %
87	`K15X01R`		5	61	6	10 %
88	`K15X02B`		10	257	3	1 %
89	`K15XQ1F`		10	94	3	3 %
90	`K16E85U`		10	73	2	3 %
91	`K16V03V`		17	379	3	1 %
92	`K16W09W`		22	161	4	2 %
93	`K16W10F`		6	46	4	9 %
94	`K16X02A`		17	131	4	3 %
95	`K17R12B`		6	36	2	6 %
96	`K18X05D`		10	69	12	17 %
97	`K19V04L`		21	139	3	2 %
98	`K19V06F`		13	94	3	3 %
99	`K19W03F`		13	126	3	2 %
100	`K19W04X`		7	71	3	4 %
101	`K19X00F`		8	48	6	13 %
102	`K19X00X`		30	223	3	1 %
103	`K19X01E`		12	66	3	5 %
104	`K21T03K`		14	108	3	3 %
105	`K21U20P`		6	44	3	7 %
106	`K21U70F`		9	56	4	7 %
107	`K21V09C`		7	36	4	11 %
108	`K21V12O`		16	63	4	6 %
109	`K21V26Q`		19	140	3	2 %
110	`K21W01T`		8	63	4	6 %
111	`K21X02T`		6	35	3	9 %
112	`K21X05H`		8	34	3	9 %
113	`K21X05J`		22	148	4	3 %
114	`K21X05Y`		6	45	3	7 %
115	`K21X06L`		14	75	4	5 %
116	`K21X07D`		2	32	29	91 %
117	`K21Y00C`		13	67	4	6 %
118	`K21Y00D`		10	42	4	10 %
119	`K22B06S`		9	85	3	4 %
120	`K22C05G`		15	81	3	4 %
121	`K22C07K`		8	41	3	7 %
122	`K22E04E`		8	34	3	9 %
123	`K22E05R`		14	94	4	4 %
124	`K22R05Q`		19	86	4	5 %
125	`K22T04S`		5	20	3	15 %
126	`K22U01N`		5	17	3	18 %
127	`K22U05E`		5	22	4	18 %
128	`K22U05K`		15	55	3	5 %
129	`K22U06L`		9	58	4	7 %
130	`K22U08T`		8	68	3	4 %
131	`K22U11U`		9	29	3	10 %
132	`K22U14S`		10	54	3	6 %
133	`K22U14V`		5	40	3	8 %
134	`K22U16H`		7	39	4	10 %
135	`K22U16R`		11	55	3	5 %
136	`K22U20V`		8	30	4	13 %
137	`K22U21N`		8	37	8	22 %
138	`K22U21Q`		7	32	3	9 %
139	`K22U21R`		7	32	3	9 %
140	`K22U21S`		17	65	4	6 %
141	`K22U21X`		15	96	7	7 %
142	`K22U22C`		25	155	4	3 %
143	`K22U24Y`		11	39	4	10 %
144	`K22U28C`		10	51	3	6 %
145	`K22U28P`		4	23	4	17 %
146	`K22U34A`		5	45	3	7 %
147	`K22V00A`		8	26	3	12 %
148	`K22V00C`		10	41	4	10 %
149	`K22V00E`		7	28	4	14 %
150	`K22V00F`		18	98	4	4 %
151	`K22V00J`		10	51	3	6 %
152	`K23G00O`		5	44	3	7 %
153	`K23H02H`		10	55	4	7 %
154	`K23H04P`		9	44	7	16 %
155	`K23H07J`		11	44	3	7 %
156	`K23H18O`		43	360	4	1 %
157	`K23J01M`		8	56	7	13 %
158	`K23J02O`		10	55	3	5 %
159	`K23J02R`		9	71	3	4 %
160	`K23K02M`		5	34	4	12 %
161	`K23K04A`		10	44	3	7 %
162	`K23K05H`		6	38	6	16 %
163	`K23K05L`		9	43	4	9 %
164	`K23K05N`		5	26	4	15 %
165	`CK01K050`		93	3305	2	0 %	comet
166	`CK04P42Y`		2	6	4	67 %	comet
167	`CK06S030`		212	6501	16	0 %	comet
168	`CK09P010`		183	9156	8	0 %	comet
169	`CK10R010`		85	1619	7	0 %	comet
170	`CK11UU5F`		101	2304	4	0 %	comet
171	`CK12K010`		185	7892	26	0 %	comet
172	`CK12S010`		201	6754	21	0 %	comet
173	`CK12T050`		63	699	3	0 %	comet
174	`CK12V020`		70	1108	4	0 %	comet
175	`CK12X010`		105	2669	7	0 %	comet
176	`CK13A010`		136	3614	8	0 %	comet
177	`CK14Q020`		159	7961	10	0 %	comet
178	`CK22E030`		192	8208	7	0 %	comet
179	`PK01J010`		7	33	3	9 %	comet
180	`PK05Q040`		25	221	5	2 %	comet
181	`PK13TB7L`		50	912	18	2 %	comet
182	`0026P`		46	453	3	1 %	comet
183	`0032P`		186	3656	6	0 %	comet
184	`0063P`		103	1891	4	0 %	comet
185	`0168P`		140	3539	4	0 %	comet
186	`0175P`		53	666	6	1 %	comet
187	`05645`		57	1460	3	0 %
188	`07350`		73	2203	6	0 %
189	`10115`		57	1981	3	0 %
190	`12711`		97	3623	3	0 %
191	`22753`		62	1630	3	0 %
192	`29075`		40	1037	23	2 %
193	`68216`		106	3959	4	0 %
194	`68278`		48	2284	6	0 %
195	`87684`		50	1949	3	0 %
196	`99942`		192	11048	21	0 %
197	`A1955`		20	580	4	1 %
198	`D6793`		28	527	7	1 %
199	`D6993`		34	894	3	0 %
200	`D8911`		37	975	32	3 %
201	`E4411`		48	1203	3	0 %
202	`F3220`		6	159	3	2 %
203	`F3958`		38	795	3	0 %
204	`G2004`		50	1698	3	0 %
205	`G2783`		5	46	3	7 %
206	`G3249`		61	2163	24	1 %
207	`G3364`		36	718	3	0 %
208	`S5263`		81	3103	7	0 %
209	`U3262`		24	605	3	0 %
210	`X7558`		8	69	4	6 %
211	`X9714`		23	267	3	1 %
212	`Y1050`		13	334	33	10 %
213	`Z0713`		14	237	7	3 %
Sum	`213 objects`			141875	1400	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 1400 of all 141875 observations (1 %) at 213 objects in all MPECs with involved station 290. There are 144 of all 4424 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.