Last NEOCP objects for station 198 in reverse order.

Created at 2024-07-15 01:50:05 UTC. This site will be recalculated about each 3 hours. Only objects with a MPEC are all complete in this list. Other objects are only in this list, if my crawler works fine (most time). Unfortunately there are sometime several day(s) lost, when my machine needs service. Designation links to objects works mostly not on recent comets. Also the data for asteroids, are only uptodate, when the MPEC has just been published.

This list is only for the last months, not for all time. The order and the data are from NEOCP archive and the NEOCP list.

Explanations: NEOCP is the NEOCP identification. Designation is provisional object ID, mostly a provisional designation. But it can also be a message (mostly 'in observing'), a comet or another NEOCP ID. Link goes to the MPC database. MPEC is the MPEC for this object (if existent) and link is to this MPEC. Publication is the time for identifaction in UT. MOID is the MOID for this object (if given) in AU. Dat 1st obs is the time of the first observation of this station 198. R.A, Dec, Mag and Moltion are the same for this date. Obs stat is the number of observations for this object by this station 198. Stats is the number of all involved stations for this object. Obs total is the number nof all observations for this object. Obs part is the percentage of station observation to all observations. res is the mean residual (in arc sec) for this station 198. |res| is the mean absolute residual (in arc secs) for this station 198. max res is the maximum residual (in arc secs) for this station 198 (outlier alarm).

You can download (test mode) a CSV file with all data in the table below (slightly other formatted).

Notice: Sometimes the MPC links the latest NEOCP ID not to a MPEC. This can need some hours, so you will see the link as soon, as it will be published in the html code of the MPC page.

NEOCP objects for station 198
NEOCPDesignationMPECPublicationMOIDDate 1st obs 198R.A.DecMagMotion
res|res|max res
C2ED6J22020 FB52020-F141Mar. 25.970.01212020-03-24.7987113:08:36+17:25:4618.636,089241128%0,500,531,25
C13EU312020 FV42020-F134Mar. 25.830.00962020-03-24.9575812:58:08+37:31:1419.326,575145110%0,070,280,45
X680912013 AO272020-F123Mar. 25.580.05822020-03-24.9913815:19:55-05:41:2319.61,95410528%0,600,661,30
P10XTaq2020 FR32020-F109Mar. 24.870.00992020-03-23.8170609:24:12+14:16:2120.32,556125511%0,420,611,10
P20XZMB2020 FH32020-F100Mar. 24.190.01432020-03-23.8896011:40:58-11:09:5720.112,3138368%1,121,151,97
A10iY9L2019 YX62020-A111Jan. 10.740.02582019-12-29.8890404:37:45+28:53:0420.91,443382341%0,240,450,50
A10jgpj2019 YK42019-Y131Dec. 31.150.09992019-12-30.8104507:44:55+13:45:4617.39,3410241109%0,090,210,60
A10jdfg2019 YA42019-Y123Dec. 30.810.02322019-12-29.8550304:38:40-00:05:5718.39,68412479%0,280,290,36
P20VI2y2019 YV32019-Y120Dec. 30.610.07302019-12-29.9413605:22:31-07:19:4119.72,35493113%0,130,270,71
A10j7GU2019 YS32019-Y115Dec. 29.900.01292019-12-29.8026502:32:09+11:34:1719.319,62416686%0,170,230,42
ZW01220Comet A/2018 W12018-X014Dec. 1.822018-11-16.7962802:21:55+46:12:3019.41,436291364%   
ZTF01na2008 WS622018-W005Nov. 17.140.01322018-11-16.7693903:21:51+36:49:4418.018,95694015%0,200,270,57
ZL1ECBE2018 LJ 2018-L010June 5.450.13092018-06-04.8762116:16:38+37:36:0219.115,65314645%0,200,430,82
ZJ1030F2018 JQ1 2018-J049May 10.830.18382018-05-08.9050614:56:57-14:43:0319.03,04418726%0,400,471,08
ZJ993132018 JW 2018-J030May 9.750.01652018-05-07.9156713:37:54+19:18:2319.236,53693816%0,220,350,58
ZH06DE62018 HU 2018-H059Apr. 21.810.02052018-04-20.8281113:37:00+20:06:2318.529,84821978%0,180,200,50
ZGB86432018 GM 2018-G033Apr. 8.480.01512018-04-06.8719411:26:44+41:13:3419.29,897211017%0,180,641,00
ZG32E732018 GL 2018-G032Apr. 8.480.14302018-04-06.8965715:16:49+57:40:0619.64,736221135%0,190,280,45
ZG333F02018 GG 2018-G028Apr. 7.880.00562018-04-06.8331511:33:27+28:42:2719.48,26518737%0,550,560,63

Jost Jahn, Amrum, Germany, Made with 'previousneo' program. This research has made use of data and/or services provided by the International Astronomical Union's Minor Planet Center.