M.P.E.C. statistics for G37

Observed objects

Nr.	Object	Discovery	Stations	Obs all	Obs G37	Obs percent	Note
1	`K00K43W`		26	144	2	1 %
2	`K00L00K`		16	90	3	3 %
3	`K06A04N`		16	112	1	1 %
4	`K07BA2P`		2	43	2	5 %
5	`K10E45W`		15	148	2	1 %
6	`K11O16D`		6	22	3	14 %
7	`K12F62P`		12	77	2	3 %
8	`K12P26D`		6	20	5	25 %
9	`K13N15J`		9	40	1	3 %
10	`K13S87A`		2	10	2	20 %
11	`K14F43P`		1	4	4	100 %
12	`K14F61U`		1	4	4	100 %
13	`K14F62B`		1	4	4	100 %
14	`K14Qh3L`		19	213	4	2 %
15	`K14SU3R`		4	11	2	18 %
16	`K14UM5B`		1	4	4	100 %
17	`K14Wo9M`		2	67	2	3 %
18	`K14X40Z`		1	2	2	100 %
19	`K15A45K`		8	44	11	25 %
20	`K15Bp5F`		1	5	5	100 %
21	`K15C00M`		13	73	5	7 %
22	`K15C00S`	`*`	13	62	5	8 %
23	`K15C01B`	`*`	8	41	13	32 %
24	`K15C01D`	`*`	7	29	3	10 %
25	`K15E00K`	`*`	10	56	8	14 %
26	`K15E00P`	`*`	11	55	4	7 %
27	`K15FB7W`	`*`	20	162	4	2 %
28	`K15FB7Z`		1	5	5	100 %
29	`K15Q00B`	`*`	16	57	7	12 %
30	`K15S16U`	`*`	9	68	8	12 %
31	`K15Tc7G`	`*`	3	22	5	23 %
32	`K15VI4X`	`*`	3	20	10	50 %
33	`K16B01F`	`*`	6	28	5	18 %
34	`K16CW3N`	`*`	3	25	14	56 %
35	`K16F00A`	`*`	18	156	10	6 %
36	`K16GD5D`		11	113	3	3 %
37	`K16J18D`	`*`	22	248	16	6 %
38	`K16J18E`	`*`	8	67	9	13 %
39	`K16M00A`	`*`	8	85	17	20 %
40	`K16S46S`		1	2	2	100 %
41	`K16W01J`		44	450	2	0 %
42	`K17B93Q`		15	125	2	2 %
43	`K17C33X`		6	29	2	7 %
44	`K17DC1M`	`*`	2	10	8	80 %
45	`K17DC1N`	`*`	2	9	7	78 %
46	`K17DC1P`	`*`	3	10	2	20 %
47	`K17E02Z`	`*`	26	124	11	9 %
48	`K17E03A`	`*`	19	88	3	3 %
49	`K17E03E`	`*`	11	65	3	5 %
50	`K17E03K`	`*`	7	33	3	9 %
51	`K17E04H`	`*`	17	123	7	6 %
52	`K17FG1O`	`*`	3	11	6	55 %
53	`K17FG1P`	`*`	3	10	2	20 %
54	`K17FG1Q`	`*`	3	10	2	20 %
55	`K17FG3D`	`*`	3	13	5	38 %
56	`K17FH3E`	`*`	3	15	4	27 %
57	`K17G07M`		15	118	2	2 %
58	`K17M04E`	`*`	5	31	5	16 %
59	`K17O69F`	`*`	3	10	4	40 %
60	`K17O69G`	`*`	3	12	4	33 %
61	`K17O69K`	`*`	3	11	7	64 %
62	`K17Q18G`	`*`	9	42	13	31 %
63	`K17W14W`		2	9	2	22 %
64	`K17W30H`	`*`	3	22	12	55 %
65	`K18A02V`		12	104	2	2 %
66	`K18A12B`		10	75	5	7 %
67	`K18A18O`		10	79	2	3 %
68	`K18C02N`	`*`	8	60	14	23 %
69	`K18G12T`	`*`	3	8	4	50 %
70	`K18L01B`		13	136	10	7 %
71	`K18L01C`		11	91	9	10 %
72	`K18L01J`		6	45	9	20 %
73	`K18L02Q`		36	471	6	1 %
74	`K18L02V`		6	44	9	20 %
75	`K18R07Y`		8	97	9	9 %
76	`K18T06G`		15	142	3	2 %
77	`K19A13M`		7	42	2	5 %
78	`K19G22N`		2	35	2	6 %
79	`K19P02R`		30	269	20	7 %
80	`K19Q06R`		18	144	23	16 %
81	`K19R03T`		23	133	2	2 %
82	`K19R04O`		1	2	2	100 %
83	`K19S03P`		9	36	2	6 %
84	`K19S04L`		8	25	1	4 %
85	`K19S07N`		3	12	2	17 %
86	`K19S08W`		6	22	2	9 %
87	`K19T00B`		9	46	2	4 %
88	`K19T00W`		8	37	2	5 %
89	`K19T02T`		6	24	6	25 %
90	`K19T07B`		9	30	4	13 %
91	`K19T07X`		5	20	2	10 %
92	`K19U00H`		12	62	5	8 %
93	`K19U00J`	`*`	5	19	2	11 %
94	`K19U00P`	`*`	7	37	6	16 %
95	`K19U02J`	`*`	21	174	5	3 %
96	`K19U02K`		5	15	2	13 %
97	`K19U02U`		5	25	3	12 %
98	`K19U03G`		8	33	2	6 %
99	`K19U03L`		6	25	2	8 %
100	`K19U06Y`		6	24	2	8 %
101	`K19U08P`		5	16	2	13 %
102	`K19U09H`		10	39	2	5 %
103	`K19U10F`		8	38	2	5 %
104	`K19U12H`		12	50	2	4 %
105	`K19U12X`		5	21	3	14 %
106	`K19U14C`		10	56	2	4 %
107	`K19V00K`		15	62	4	6 %
108	`K19V00V`		16	103	2	2 %
109	`K19V04E`		3	15	2	13 %
110	`K20B12F`		5	22	2	9 %
111	`K20B12T`		7	54	5	9 %
112	`K20C01Q`		12	48	3	6 %
113	`K20C02K`		6	30	3	10 %
114	`K20C03D`		10	63	3	5 %
115	`K20C03M`		1	3	3	100 %
116	`K20D03F`		20	84	5	6 %
117	`K20D04G`		9	42	6	14 %
118	`K20F01A`		16	83	4	5 %
119	`K20F06U`	`*`	8	43	6	14 %
120	`K20F06V`	`*`	14	95	5	5 %
121	`K20F06X`	`*`	11	35	4	11 %
122	`K20P02C`		4	13	2	15 %
123	`K20P06G`		6	32	2	6 %
124	`K20Q01N`		11	61	4	7 %
125	`K20Q04D`		3	11	2	18 %
126	`K20Q05R`		14	54	2	4 %
127	`K20R00K`		25	110	4	4 %
128	`K20R02J`		7	34	5	15 %
129	`K20R02O`		6	20	4	20 %
130	`K20S04P`	`*`	5	32	10	31 %
131	`K20S04U`		7	43	2	5 %
132	`K20S05W`		4	18	2	11 %
133	`K20S06P`		6	30	7	23 %
134	`K20S06X`		7	43	5	12 %
135	`K20T00W`		12	77	5	6 %
136	`K20T01T`		8	37	3	8 %
137	`K20T01Y`		20	125	5	4 %
138	`K20T03Z`		7	31	7	23 %
139	`K20T04Y`		11	60	5	8 %
140	`K20T05K`		16	109	3	3 %
141	`K20T07D`		8	31	5	16 %
142	`K20T08D`		16	82	4	5 %
143	`K20U00E`		25	132	7	5 %
144	`K20U00H`		12	71	3	4 %
145	`K20U02K`		5	28	5	18 %
146	`K20U03L`		13	118	5	4 %
147	`K20U03Q`		8	32	7	22 %
148	`K20U04O`		15	69	2	3 %
149	`K20V00V`		12	79	9	11 %
150	`K20V00W`		7	20	2	10 %
151	`K20V02U`		3	13	3	23 %
152	`K20V04A`		12	63	4	6 %
153	`K20Y03R`	`*`	11	117	5	4 %
154	`CK13X010`		133	3320	14	0 %	comet
155	`CK14Od2G`	`*`	10	201	6	3 %	comet
156	`CK18E09F`	`*`	25	191	2	1 %	comet
157	`CK18P050`	`*`	16	82	9	11 %	comet
158	`CK20B020`	`*`	18	106	4	4 %	comet
159	`PK16B14A`		90	1873	14	1 %	comet
160	`PK20Y010`	`Discovery`	2	6	4	67 %	comet
161	`SK17J040`	`*`	3	20	6	30 %
162	`SK18J010`	`*`	4	17	2	12 %
163	`0010P`		165	3703	9	0 %	comet
164	`0012P`		1	8	8	100 %	comet
165	`0046P`	`*`	225	9213	104	1 %	comet
166	`0071P`		110	1883	7	0 %	comet
167	`0073P`		58	1230	6	0 %	comet
168	`0114P`	`*`	93	1841	7	0 %	comet
169	`0252P`		81	1676	16	1 %	comet
170	`0313P`	`*`	15	84	3	4 %	comet
171	`0322P`		4	32	8	25 %	comet
172	`0332P`		1	3	3	100 %	comet
173	`65803`		59	959	7	1 %
174	`E1531`		32	605	2	0 %
175	`c8185`		5	17	3	18 %
176	`j1397`		5	44	3	7 %
Sum	`176 objects`			36372	978	3 %	17 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 G37 are all observations in all MPECs for this station. Obs percent is the percentage of stations observation to all observations.

G37 has discovered 1 objects. It has made 978 of all 36372 observations (3 %) at 176 objects in all MPECs with involved station G37. There are 385 of all 9557 observations (4 %) at 55 objects in all discovery MPECs with involved station G37.

All MPECs for station G37

Discovery MPEC for station G37

All observations for station G37

Created with MPECSGET.