Last NEOCP objects for station O75 in reverse order.

Created at 2024-04-12 09:11:17 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 O75. 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 O75. 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 O75. |res| is the mean absolute residual (in arc secs) for this station O75. max res is the maximum residual (in arc secs) for this station O75 (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 O75
NEOCPDesignationMPECPublicationMOIDDate 1st obs O75R.A.DecMagMotion
res|res|max res
ELGBA202024 GF2024-G035Apr. 3.930.01042024-04-02.7662312:56:32-06:14:1519.021,95382811%0,760,761,30
ELEJA112024 EB32024-E147Mar. 12.040.03022024-03-10.6619111:27:52+01:52:5217.440,94512579%0,950,981,90
EXCIA01does not existFeb. 9.782024-02-09.5477410:07:35+27:42:3418.736,11313100%   
Sar27382024 CK12024-C079Feb. 8.050.00142024-02-07.8066208:26:34+37:16:4418.076,1537378%0,640,851,71
C42XMN12024 CT2024-C055Feb. 5.930.00372024-02-05.7833109:41:40+26:25:0117.324,84317923%0,400,430,61
A1134Tw2024 BC32024-B153Jan. 30.050.04612024-01-29.8242708:10:04+09:15:3316.719,373241093%0,070,380,50
ELE07412023 QM52023-Q133Aug. 25.130.00682023-08-23.7219223:39:44-00:19:4818.615,56672722%0,230,631,20
C8VJ6522023 CA2023-C014Feb. 2.100.00372023-02-01.7203909:46:32+30:37:3718.217,34311486%0,110,250,30
A10Qx8M2022 WF2022-W035Nov. 17.740.00962022-11-16.8462705:37:59+28:52:1719.17,82210316%0,491,111,30
C8EDED22022 WA2022-W020Nov. 17.120.00322022-11-16.6663603:46:42+16:14:4618.619,87313526%0,490,490,71
C3ALL012022 VH22022-V164Nov. 14.970.02122022-11-14.5487102:25:52+38:52:5919.121,2938398%0,540,841,57
ELE06752022 VG22022-V163Nov. 14.970.00572022-11-14.5125501:19:59+06:59:1018.349,586125212%0,971,153,14
A10PcHv2022 UA102022-U266Oct. 26.550.02172022-10-25.8795122:39:08+82:37:1718.619,80382811%0,240,761,08
TMG00752022 UQ62022-U200Oct. 22.670.00352022-10-20.7823503:47:23-11:50:3319.0162,38341817%0,360,761,30
C38AZV12022 UA62022-U185Oct. 22.620.00362022-10-21.5835502:49:09+18:29:5719.052,23372413%0,540,601,08
A10iynG2019 XR12019-X073Dec. 6.200.00362019-12-05.8406207:31:27+45:17:4616.264,70964321%0,170,560,94
A10ifCP2019 WR32019-W170Nov. 29.570.03502019-11-27.6542504:36:21+61:18:0117.47,05311457%0,090,380,57
A10ifCL2019 WQ32019-W169Nov. 29.570.02512019-11-27.6474702:41:46+80:06:1016.528,88311625%0,831,071,48
C0RVN712019 WS22019-W154Nov. 27.130.07812019-11-26.5255102:16:06+10:26:0218.915,3139349%0,500,570,81
A10i6ZR2019 WK22019-W144Nov. 26.210.00512019-11-25.7578104:36:50-07:45:1118.418,26311457%0,500,590,81

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.