Submission uncertainty - Get NEOCP orbits

00001sS

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-10 02:14:13 UTC	3	3	327 — Peking Observatory, Xinglong Station	5.850′	fitted

6JC2221

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 02:50:05 UTC	3	3	W94 — MAPS, San Pedro de Atacama	7.367′	fitted
2026-09-13 03:20:04 UTC	3	6	W97 — Atacama Desert Observatory, San Pedro de Atacama	0.797′	fitted
2026-09-13 03:40:23 UTC	2	8	X09 — Deep Random Survey, Rio Hurtado	0.055′	fitted
2026-09-13 04:40:04 UTC	3	11	W97 — Atacama Desert Observatory, San Pedro de Atacama	0.077′	fitted
2026-09-14 00:17:18 UTC	3	14	807 — Cerro Tololo Observatory, La Serena	0.021′	fitted
2026-09-14 18:36:10 UTC	3	17	M49 — IAS Remote Observatory, Hakos	0.010′	fitted

6JD1C21

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 06:35:05 UTC	3	3	W94 — MAPS, San Pedro de Atacama	4.267′	fitted
2026-09-14 06:45:05 UTC	3	6	W97 — Atacama Desert Observatory, San Pedro de Atacama	0.682′	fitted
2026-09-15 05:20:26 UTC	3	9	W97 — Atacama Desert Observatory, San Pedro de Atacama	0.018′	fitted

6JD4321

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 05:20:05 UTC	3	3	W94 — MAPS, San Pedro de Atacama	3.683′	fitted
2026-09-14 05:25:07 UTC	3	6	W97 — Atacama Desert Observatory, San Pedro de Atacama	0.295′	fitted
2026-09-14 19:04:04 UTC	3	9	M49 — IAS Remote Observatory, Hakos	0.004′	fitted
2026-09-15 00:16:51 UTC	3	12	807 — Cerro Tololo Observatory, La Serena	0.004′	fitted
2026-09-15 05:25:06 UTC	3	15	W97 — Atacama Desert Observatory, San Pedro de Atacama	0.005′	fitted
2026-09-15 05:25:23 UTC	3	18	W97 — Atacama Desert Observatory, San Pedro de Atacama	0.004′	fitted

6JE1921

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-15 04:40:22 UTC	3	3	W94 — MAPS, San Pedro de Atacama	1.540′	fitted
2026-09-15 06:17:46 UTC	3	6	734 — Farpoint Observatory, Eskridge	0.075′	fitted

8NFG001

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 04:46:54 UTC	3	3	K19 — PASTIS Observatory, Banon	1,320.000′	fitted
2026-09-14 23:16:49 UTC	3	6	K19 — PASTIS Observatory, Banon	36.567′	fitted

A11FPxB

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-08-19 19:56:00 UTC	4	4	M22 — ATLAS South Africa, Sutherland	1.578′	fitted
2026-08-20 22:58:01 UTC	3	7	Y05 — SONEAR Wykrota-CEAMIG, Serra da Piedade	0.041′	fitted
2026-08-21 18:23:55 UTC	2	9	M49 — IAS Remote Observatory, Hakos	0.007′	fitted
2026-08-22 18:46:56 UTC	2	11	M49 — IAS Remote Observatory, Hakos	0.005′	fitted
2026-08-23 16:03:49 UTC	2	13	Q64 — Siding Spring-LCO B	0.006′	fitted
2026-08-23 16:20:05 UTC	3	16	Q62 — iTelescope Observatory, Siding Spring	0.004′	fitted
2026-08-24 18:46:32 UTC	2	18	M49 — IAS Remote Observatory, Hakos	0.004′	fitted
2026-08-26 16:04:26 UTC	2	20	X28 — Station name unavailable	0.016′	fitted
2026-08-28 08:00:18 UTC	3	23	E42 — AUSTRALIA1/SRI, Swan Reach	—	fit-error
2026-08-28 22:33:43 UTC	2	25	E62 — Slooh.com Australia, Coonabarabran	0.004′	fitted
2026-08-31 22:09:45 UTC	2	27	E62 — Slooh.com Australia, Coonabarabran	0.005′	fitted
2026-09-03 20:07:37 UTC	3	30	M49 — IAS Remote Observatory, Hakos	0.003′	fitted
2026-09-04 14:09:31 UTC	3	33	194 — Tivoli	0.002′	fitted
2026-09-05 16:51:23 UTC	3	36	M49 — IAS Remote Observatory, Hakos	0.003′	fitted
2026-09-09 20:31:38 UTC	3	39	194 — Tivoli	0.004′	fitted
2026-09-09 20:50:54 UTC	2	41	M21 — Schiaparelli Southern Observatory, Hakos	0.004′	fitted
2026-09-12 04:45:05 UTC	5	46	Q63 — Siding Spring-LCO A	0.003′	fitted
2026-09-12 18:52:05 UTC	3	49	M49 — IAS Remote Observatory, Hakos	0.002′	fitted

A11GP9t

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 14:12:20 UTC	3	3	W68 — ATLAS Chile, Rio Hurtado	247.000′	fitted

ABC0199

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 14:41:11 UTC	4	4	122 — Pises Observatory	910.000′	fitted

AFS700

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 22:04:53 UTC	3	3	R48 — Centro Astronomico Alto Turia 2	2.167′	fitted

C1G1VQ5

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-05 08:43:01 UTC	4	4	V00 — Kitt Peak-Bok	4.250′	fitted
2026-09-05 09:41:14 UTC	4	8	V00 — Kitt Peak-Bok	1.108′	fitted
2026-09-06 07:00:10 UTC	3	11	V00 — Kitt Peak-Bok	0.059′	fitted

C1G8TZ5

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-06 08:55:28 UTC	4	4	V00 — Kitt Peak-Bok	3.233′	fitted
2026-09-08 05:10:05 UTC	3	7	H21 — Astronomical Research Observatory, Westfield	0.081′	fitted
2026-09-09 04:55:23 UTC	2	9	H21 — Astronomical Research Observatory, Westfield	0.031′	fitted

C1GCU65

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-08 03:40:04 UTC	4	4	V00 — Kitt Peak-Bok	2.983′	fitted
2026-09-09 04:30:05 UTC	3	7	H21 — Astronomical Research Observatory, Westfield	0.085′	fitted
2026-09-11 05:36:23 UTC	4	11	H01 — Magdalena Ridge Observatory, Socorro	0.003′	fitted
2026-09-13 04:35:05 UTC	2	13	H21 — Astronomical Research Observatory, Westfield	0.004′	fitted

C1LT29P

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 22:30:34 UTC	4	4	G96 — University of Arizona Mt. Lemmon Survey	535.000′	fitted

C1LT2DP

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 22:53:34 UTC	4	4	G96 — University of Arizona Mt. Lemmon Survey	15.433′	fitted

C46K1R1

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 04:04:35 UTC	4	4	703 — University of Arizona Catalina Sky Survey	3.533′	fitted
2026-09-14 04:21:00 UTC	4	8	703 — University of Arizona Catalina Sky Survey	1.100′	fitted
2026-09-14 18:56:13 UTC	3	11	595 — Farra d'Isonzo	0.046′	fitted
2026-09-14 19:04:56 UTC	3	14	M26 — Zen Observatory, Scandicci	0.037′	fitted
2026-09-14 19:08:14 UTC	2	16	126 — Monte Viseggi L. Zannoni Observatory	0.046′	fitted
2026-09-14 19:14:39 UTC	4	20	033 — Karl Schwarzschild Observatory, Tautenburg	0.046′	fitted
2026-09-14 19:17:16 UTC	2	22	126 — Monte Viseggi L. Zannoni Observatory	0.025′	fitted
2026-09-14 19:47:49 UTC	3	25	K74 — Muensterschwarzach Observatory, Schwarzach	0.021′	fitted
2026-09-14 19:50:06 UTC	2	27	L06 — Sormano 2 Observatory, Bellagio Via Lattea	0.015′	fitted
2026-09-14 20:20:06 UTC	3	30	G34 — Oberfrauendorf	0.047′	fitted
2026-09-14 20:26:59 UTC	3	33	R48 — Centro Astronomico Alto Turia 2	0.006′	fitted
2026-09-14 20:29:10 UTC	2	35	M38 — Harsona Observatory, Nyiregyhaza	0.004′	fitted
2026-09-14 20:38:21 UTC	3	38	R59 — Camarasa Observatory, Astrocamp Nerpio	0.004′	fitted
2026-09-14 20:50:22 UTC	3	41	J87 — La Canada	0.006′	fitted
2026-09-14 20:53:42 UTC	3	44	A71 — Stixendorf	0.005′	fitted
2026-09-14 21:00:51 UTC	2	46	D31 — Osservatorio Aldebaran, Rivalba	0.005′	fitted
2026-09-14 21:17:12 UTC	3	49	R93 — Sanse Observatory, San Sebastiano Curone	0.005′	fitted
2026-09-14 21:24:27 UTC	3	52	R85 — Telescope Leonard de Vinci, GAPRA, Antibes	0.004′	fitted
2026-09-14 21:52:47 UTC	4	56	C23 — Olmen	0.003′	fitted
2026-09-14 22:25:17 UTC	2	58	970 — Chelmsford	0.004′	fitted
2026-09-15 00:01:24 UTC	3	61	P13 — Baihuashan Observatory, Beijing	0.004′	fitted
2026-09-15 05:05:17 UTC	3	64	215 — Buchloe	0.012′	fitted
2026-09-15 05:05:53 UTC	6	70	L27 — 29PREMOTE Observatory, Dauban	0.012′	fitted

C98FG8Z

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 09:03:24 UTC	4	4	V00 — Kitt Peak-Bok	3,300.000′	fitted

CERCZM2

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-06 07:35:20 UTC	4	4	G96 — University of Arizona Mt. Lemmon Survey	6.350′	fitted
2026-09-06 08:53:36 UTC	4	8	V06 — Catalina Sky Survey-Kuiper	1.950′	fitted

CERUX32

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 06:33:01 UTC	3	3	G96 — University of Arizona Mt. Lemmon Survey	1.933′	fitted
2026-09-11 07:48:14 UTC	2	5	673 — Table Mountain Observatory, Wrightwood	0.243′	fitted
2026-09-11 08:04:27 UTC	3	8	I52 — Steward Observatory, Mt. Lemmon Station	0.058′	fitted
2026-09-11 10:17:56 UTC	3	11	I52 — Steward Observatory, Mt. Lemmon Station	0.078′	fitted
2026-09-12 04:41:38 UTC	2	13	673 — Table Mountain Observatory, Wrightwood	0.004′	fitted
2026-09-12 20:31:33 UTC	3	16	R48 — Centro Astronomico Alto Turia 2	0.004′	fitted
2026-09-13 02:10:22 UTC	3	19	H21 — Astronomical Research Observatory, Westfield	0.003′	fitted
2026-09-13 03:49:46 UTC	5	24	I41 — Palomar Mountain--ZTF	0.004′	fitted
2026-09-13 04:50:24 UTC	2	26	673 — Table Mountain Observatory, Wrightwood	0.004′	fitted

CERWPH2

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 07:03:57 UTC	4	4	G96 — University of Arizona Mt. Lemmon Survey	3.517′	fitted
2026-09-13 08:10:11 UTC	3	7	G96 — University of Arizona Mt. Lemmon Survey	1.330′	fitted
2026-09-13 23:10:05 UTC	3	10	Z84 — Calar Alto-Schmidt	0.011′	fitted

CERXY22

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 07:59:28 UTC	4	4	G96 — University of Arizona Mt. Lemmon Survey	4.617′	fitted
2026-09-13 09:06:19 UTC	4	8	G96 — University of Arizona Mt. Lemmon Survey	0.973′	fitted
2026-09-14 09:52:30 UTC	3	11	J04 — ESA Optical Ground Station, Tenerife	0.017′	fitted
2026-09-14 22:00:32 UTC	2	13	I41 — Palomar Mountain--ZTF	0.026′	fitted

KVCD1ME

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 16:12:22 UTC	12	12	W84 — Cerro Tololo-DECam	9.650′	fitted

LA0D3nK

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 16:57:17 UTC	6	6	P07 — Space Surveillance Telescope, HEH Station	0.842′	fitted

LA0D3nL

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 16:57:17 UTC	4	4	P07 — Space Surveillance Telescope, HEH Station	1.063′	fitted

P12pBfG

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-04 11:10:10 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	3.517′	fitted
2026-09-04 22:11:14 UTC	2	5	F52 — Pan-STARRS 2, Haleakala	1.238′	fitted
2026-09-05 05:36:18 UTC	3	8	807 — Cerro Tololo Observatory, La Serena	0.009′	fitted

P12pEFf

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-05 12:00:51 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	1.143′	fitted

P12pEFg

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-05 12:00:56 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	1.575′	fitted
2026-09-05 16:46:07 UTC	2	6	F52 — Pan-STARRS 2, Haleakala	0.805′	fitted
2026-09-08 11:44:53 UTC	3	9	474 — Mount John Observatory, Lake Tekapo	0.019′	fitted

P12pEuy

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-05 07:38:53 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	3.400′	fitted
2026-09-05 17:03:14 UTC	1	4	F51 — Pan-STARRS 1, Haleakala	2.533′	fitted
2026-09-08 23:45:05 UTC	2	6	J04 — ESA Optical Ground Station, Tenerife	0.026′	fitted

P12pHLa

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-05 16:14:17 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	1.480′	fitted
2026-09-06 13:57:08 UTC	3	7	T14 — Canada-France-Hawaii Telescope, Maunakea	0.053′	fitted
2026-09-08 07:05:21 UTC	2	9	Q62 — iTelescope Observatory, Siding Spring	0.233′	fitted
2026-09-10 03:00:05 UTC	4	13	K91 — Sutherland-LCO A	0.002′	fitted
2026-09-11 09:25:00 UTC	2	15	S15 — Station name unavailable	0.009′	fitted
2026-09-12 21:17:06 UTC	3	18	E42 — AUSTRALIA1/SRI, Swan Reach	0.007′	fitted

P12pKZG

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-05 18:18:36 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	4.033′	fitted

P12pRCw

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 12:51:10 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	4.117′	fitted
2026-09-14 23:31:21 UTC	2	5	I41 — Palomar Mountain--ZTF	0.038′	fitted

P12pRIj

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 13:19:46 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	2.367′	fitted
2026-09-11 16:38:14 UTC	2	5	F51 — Pan-STARRS 1, Haleakala	1.105′	fitted
2026-09-13 08:05:05 UTC	2	7	H21 — Astronomical Research Observatory, Westfield	0.009′	fitted

P12pRQk

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 15:55:46 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	16.633′	fitted
2026-09-13 09:10:05 UTC	2	5	H21 — Astronomical Research Observatory, Westfield	0.092′	fitted

P12pRQl

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 15:55:49 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	1.967′	fitted
2026-09-13 09:00:05 UTC	3	7	H21 — Astronomical Research Observatory, Westfield	0.057′	fitted
2026-09-14 23:29:12 UTC	3	10	I41 — Palomar Mountain--ZTF	0.014′	fitted

P12pRQm

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 15:55:54 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	1.800′	fitted
2026-09-13 09:25:38 UTC	2	6	H21 — Astronomical Research Observatory, Westfield	0.041′	fitted

P12pRQn

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 15:55:58 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	1.750′	fitted
2026-09-13 08:40:05 UTC	3	7	H21 — Astronomical Research Observatory, Westfield	0.060′	fitted
2026-09-14 23:27:33 UTC	4	11	I41 — Palomar Mountain--ZTF	0.010′	fitted

P12pWPI

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 15:41:32 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	1.597′	fitted
2026-09-14 09:00:05 UTC	3	7	Z84 — Calar Alto-Schmidt	0.091′	fitted
2026-09-14 16:48:37 UTC	2	9	F51 — Pan-STARRS 1, Haleakala	0.012′	fitted

P12pWTl

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 15:49:57 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	0.973′	fitted
2026-09-14 16:41:34 UTC	3	6	T14 — Canada-France-Hawaii Telescope, Maunakea	0.063′	fitted

P12pZCA

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 14:38:04 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	1.700′	fitted
2026-09-14 01:55:04 UTC	3	7	958 — Observatoire de Dax	0.060′	fitted
2026-09-14 05:06:35 UTC	3	10	807 — Cerro Tololo Observatory, La Serena	0.012′	fitted
2026-09-14 08:30:05 UTC	2	12	H21 — Astronomical Research Observatory, Westfield	0.002′	fitted

P12pZCy

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 14:37:58 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	1.525′	fitted
2026-09-14 21:46:17 UTC	1	5	I41 — Palomar Mountain--ZTF	0.265′	fitted

P12pZb6

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 11:21:52 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	3.550′	fitted
2026-09-13 17:16:47 UTC	2	5	F52 — Pan-STARRS 2, Haleakala	0.890′	fitted
2026-09-14 06:30:26 UTC	3	8	H21 — Astronomical Research Observatory, Westfield	0.000′	fitted
2026-09-14 09:00:05 UTC	2	10	Z84 — Calar Alto-Schmidt	0.003′	fitted

P12pZnp

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 11:30:43 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	0.763′	fitted
2026-09-13 17:17:50 UTC	2	6	F52 — Pan-STARRS 2, Haleakala	0.457′	fitted
2026-09-14 06:05:06 UTC	3	9	H21 — Astronomical Research Observatory, Westfield	0.007′	fitted

P12pZnq

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 11:32:08 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	0.908′	fitted
2026-09-13 17:18:55 UTC	2	6	F52 — Pan-STARRS 2, Haleakala	0.413′	fitted
2026-09-14 05:20:25 UTC	2	8	H21 — Astronomical Research Observatory, Westfield	0.004′	fitted

P12pZnr

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 11:32:59 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	2.067′	fitted
2026-09-13 17:19:59 UTC	2	5	F52 — Pan-STARRS 2, Haleakala	1.030′	fitted
2026-09-14 05:40:25 UTC	3	8	H21 — Astronomical Research Observatory, Westfield	0.001′	fitted
2026-09-14 09:52:30 UTC	3	11	J04 — ESA Optical Ground Station, Tenerife	0.004′	fitted

P12pZns

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 11:34:05 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	0.617′	fitted
2026-09-13 17:21:18 UTC	3	6	F52 — Pan-STARRS 2, Haleakala	0.317′	fitted
2026-09-15 05:30:06 UTC	3	9	H21 — Astronomical Research Observatory, Westfield	0.005′	fitted

P12pZsW

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 12:37:28 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	0.488′	fitted
2026-09-13 17:22:46 UTC	2	6	F51 — Pan-STARRS 1, Haleakala	0.622′	fitted

P12pwoA

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-02 10:25:01 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	1.800′	fitted
2026-09-05 11:27:53 UTC	3	7	T14 — Canada-France-Hawaii Telescope, Maunakea	0.074′	fitted
2026-09-06 00:05:40 UTC	3	10	807 — Cerro Tololo Observatory, La Serena	0.004′	fitted
2026-09-09 03:15:05 UTC	2	12	Q62 — iTelescope Observatory, Siding Spring	0.006′	fitted

P12q6aM

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 09:37:57 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	3.517′	fitted
2026-09-14 16:49:48 UTC	2	5	F52 — Pan-STARRS 2, Haleakala	1.320′	fitted

P12q6iW

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 11:34:36 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	2.350′	fitted

P12qbdP

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 17:12:57 UTC	4	4	F51 — Pan-STARRS 1, Haleakala	3.817′	fitted

P12qbdQ

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 17:13:16 UTC	3	3	F51 — Pan-STARRS 1, Haleakala	6.017′	fitted

P22oLCM

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-08-03 12:10:42 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	0.500′	fitted
2026-08-04 00:13:24 UTC	2	6	F51 — Pan-STARRS 1, Haleakala	0.640′	fitted
2026-08-04 06:10:06 UTC	2	8	H21 — Astronomical Research Observatory, Westfield	0.017′	fitted
2026-08-04 13:05:52 UTC	4	12	F52 — Pan-STARRS 2, Haleakala	0.007′	fitted
2026-08-06 13:55:01 UTC	3	15	T14 — Canada-France-Hawaii Telescope, Maunakea	0.000′	fitted
2026-08-08 16:49:06 UTC	2	17	F51 — Pan-STARRS 1, Haleakala	0.003′	fitted
2026-08-14 03:15:12 UTC	2	19	Q62 — iTelescope Observatory, Siding Spring	0.005′	fitted
2026-09-04 21:19:35 UTC	3	22	M57 — Wide-field Mufara Telescope, Isnello	0.003′	fitted
2026-09-06 05:10:02 UTC	3	25	G00 — AZM Martinsberg, Oed	0.002′	fitted

P22oVrz

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-08-06 18:42:50 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	14.117′	fitted
2026-08-07 13:04:03 UTC	3	6	T14 — Canada-France-Hawaii Telescope, Maunakea	0.042′	fitted
2026-08-07 19:05:05 UTC	2	8	L01 — Visnjan Observatory, Tican	0.017′	fitted
2026-08-07 19:26:28 UTC	2	10	J95 — Great Shefford	0.006′	fitted
2026-08-07 19:38:57 UTC	4	14	F51 — Pan-STARRS 1, Haleakala	0.005′	fitted
2026-08-08 12:15:51 UTC	3	17	T14 — Canada-France-Hawaii Telescope, Maunakea	0.008′	fitted
2026-08-15 16:10:06 UTC	2	19	Q62 — iTelescope Observatory, Siding Spring	0.004′	fitted
2026-09-04 11:32:33 UTC	3	22	T14 — Canada-France-Hawaii Telescope, Maunakea	0.001′	fitted

P22pKXS

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-05 17:35:01 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	5.200′	fitted
2026-09-06 06:45:37 UTC	3	6	807 — Cerro Tololo Observatory, La Serena	0.042′	fitted
2026-09-07 05:05:05 UTC	3	9	H21 — Astronomical Research Observatory, Westfield	0.002′	fitted
2026-09-11 06:46:50 UTC	3	12	R48 — Centro Astronomico Alto Turia 2	0.003′	fitted

P22pKXT

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-05 17:35:57 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	4.083′	fitted

P22pKZA

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-05 18:14:23 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	4.100′	fitted
2026-09-10 17:22:45 UTC	3	6	J04 — ESA Optical Ground Station, Tenerife	0.742′	fitted
2026-09-11 12:51:51 UTC	2	8	691 — Steward Observatory, Kitt Peak-Spacewatch	0.003′	fitted

P22pKZB

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-05 18:14:28 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	2.700′	fitted
2026-09-10 17:22:45 UTC	3	7	J04 — ESA Optical Ground Station, Tenerife	0.562′	fitted

P22pL3T

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-09 10:30:45 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	4.683′	fitted

P22pL3Z

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-09 10:43:35 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	2.917′	fitted
2026-09-10 03:16:10 UTC	4	7	V06 — Catalina Sky Survey-Kuiper	0.083′	fitted

P22pL40

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-09 10:45:11 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	1.667′	fitted
2026-09-12 21:05:22 UTC	3	7	R48 — Centro Astronomico Alto Turia 2	0.024′	fitted
2026-09-13 03:10:05 UTC	2	9	H21 — Astronomical Research Observatory, Westfield	0.014′	fitted

P22pL41

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-09 10:46:22 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	0.086′	fitted
2026-09-09 11:47:26 UTC	2	6	H01 — Magdalena Ridge Observatory, Socorro	0.053′	fitted

P22pL44

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-09 10:48:06 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	1.867′	fitted

P22pP3n

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-10 15:34:07 UTC	2	2	F52 — Pan-STARRS 2, Haleakala	—	insufficient-observations
2026-09-10 16:07:03 UTC	1	3	F52 — Pan-STARRS 2, Haleakala	948.000′	fitted

P22pRQ8

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 15:54:14 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	3.633′	fitted
2026-09-13 07:35:05 UTC	3	6	H21 — Astronomical Research Observatory, Westfield	0.043′	fitted

P22pRjP

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 12:42:35 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	3.200′	fitted
2026-09-11 16:43:05 UTC	2	5	F51 — Pan-STARRS 1, Haleakala	0.807′	fitted
2026-09-14 09:30:05 UTC	3	8	Z84 — Calar Alto-Schmidt	0.123′	fitted

P22pRjQ

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 12:42:58 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	10.050′	fitted
2026-09-11 16:44:19 UTC	2	5	F51 — Pan-STARRS 1, Haleakala	1.217′	fitted

P22pRlF

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 12:45:17 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	3.150′	fitted
2026-09-11 16:46:24 UTC	2	6	F51 — Pan-STARRS 1, Haleakala	0.563′	fitted

P22pWJA

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 11:48:34 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	1.392′	fitted
2026-09-12 18:20:08 UTC	2	5	F51 — Pan-STARRS 1, Haleakala	2.400′	fitted
2026-09-13 07:10:05 UTC	2	7	H21 — Astronomical Research Observatory, Westfield	0.035′	fitted

P22pWJB

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 11:48:52 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	2.733′	fitted
2026-09-12 18:21:19 UTC	4	7	F51 — Pan-STARRS 1, Haleakala	1.620′	fitted
2026-09-13 06:00:05 UTC	3	10	H21 — Astronomical Research Observatory, Westfield	0.006′	fitted

P22pWJx

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 11:47:47 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	4.433′	fitted
2026-09-12 18:23:43 UTC	2	5	F51 — Pan-STARRS 1, Haleakala	2.333′	fitted
2026-09-13 06:35:04 UTC	3	8	H21 — Astronomical Research Observatory, Westfield	0.052′	fitted

P22pWRV

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 15:45:43 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	0.843′	fitted
2026-09-12 22:42:27 UTC	3	7	R48 — Centro Astronomico Alto Turia 2	0.047′	fitted
2026-09-13 01:28:30 UTC	2	9	I41 — Palomar Mountain--ZTF	0.017′	fitted
2026-09-14 07:55:05 UTC	3	12	H21 — Astronomical Research Observatory, Westfield	0.002′	fitted

P22pZ20

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 19:29:36 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	13.733′	fitted
2026-09-15 03:15:05 UTC	3	6	L01 — Visnjan Observatory, Tican	0.037′	fitted

P22pZAB

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 14:24:40 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	1.817′	fitted

P22pZAD

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 14:26:10 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	1.717′	fitted
2026-09-14 07:10:06 UTC	3	7	H21 — Astronomical Research Observatory, Westfield	0.032′	fitted
2026-09-14 09:15:05 UTC	3	10	Z84 — Calar Alto-Schmidt	0.025′	fitted
2026-09-14 16:53:08 UTC	2	12	F51 — Pan-STARRS 1, Haleakala	0.013′	fitted

P22pZAE

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 14:26:12 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	2.350′	fitted
2026-09-13 17:28:00 UTC	1	4	F52 — Pan-STARRS 2, Haleakala	2.100′	fitted
2026-09-14 09:30:05 UTC	3	7	Z84 — Calar Alto-Schmidt	0.202′	fitted
2026-09-14 16:54:32 UTC	2	9	F51 — Pan-STARRS 1, Haleakala	0.013′	fitted

P22pZAF

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 14:26:16 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	0.668′	fitted

P22pZcc

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 11:24:50 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	2.367′	fitted
2026-09-13 17:32:25 UTC	2	6	F51 — Pan-STARRS 1, Haleakala	1.097′	fitted
2026-09-14 09:15:05 UTC	3	9	Z84 — Calar Alto-Schmidt	0.110′	fitted

P22pZo5

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 11:35:38 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	1.767′	fitted
2026-09-13 17:34:54 UTC	2	6	F51 — Pan-STARRS 1, Haleakala	0.782′	fitted
2026-09-13 22:10:05 UTC	3	9	J04 — ESA Optical Ground Station, Tenerife	0.029′	fitted
2026-09-14 03:11:41 UTC	4	13	I52 — Steward Observatory, Mt. Lemmon Station	0.008′	fitted
2026-09-14 03:30:05 UTC	2	15	H21 — Astronomical Research Observatory, Westfield	0.005′	fitted
2026-09-14 21:55:17 UTC	3	18	I41 — Palomar Mountain--ZTF	0.014′	fitted
2026-09-15 05:52:53 UTC	2	20	204 — Schiaparelli Observatory	0.003′	fitted

P22pZoy

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 11:38:18 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	5.817′	fitted
2026-09-13 17:35:53 UTC	2	5	F51 — Pan-STARRS 1, Haleakala	2.033′	fitted
2026-09-14 09:52:30 UTC	2	7	J04 — ESA Optical Ground Station, Tenerife	0.092′	fitted
2026-09-14 16:57:42 UTC	2	9	F51 — Pan-STARRS 1, Haleakala	0.014′	fitted
2026-09-15 05:05:05 UTC	2	11	H21 — Astronomical Research Observatory, Westfield	0.003′	fitted

P22pZoz

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 11:40:10 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	1.133′	fitted
2026-09-13 17:36:58 UTC	2	5	F51 — Pan-STARRS 1, Haleakala	0.565′	fitted

P22pZwK

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 13:08:27 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	1.130′	fitted
2026-09-13 17:39:01 UTC	2	6	F51 — Pan-STARRS 1, Haleakala	0.725′	fitted

P22pZwL

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 13:08:29 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	2.000′	fitted
2026-09-13 17:40:07 UTC	2	6	F51 — Pan-STARRS 1, Haleakala	0.643′	fitted

P22pZzV

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 13:31:18 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	0.813′	fitted
2026-09-15 04:35:39 UTC	3	7	H21 — Astronomical Research Observatory, Westfield	0.019′	fitted

P22pZzW

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 13:31:21 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	1.332′	fitted

P22q64z

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 19:58:44 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	769.000′	fitted
2026-09-14 17:00:09 UTC	2	5	F51 — Pan-STARRS 1, Haleakala	0.272′	fitted

P22q67Q

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 09:03:20 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	0.132′	fitted
2026-09-14 17:01:28 UTC	2	6	F52 — Pan-STARRS 2, Haleakala	0.842′	fitted
2026-09-15 03:25:05 UTC	4	10	H21 — Astronomical Research Observatory, Westfield	0.007′	fitted

P22q6aC

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 09:06:40 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	1.267′	fitted
2026-09-14 17:05:54 UTC	2	5	F52 — Pan-STARRS 2, Haleakala	1.833′	fitted

P22q6aD

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 09:06:44 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	0.168′	fitted
2026-09-14 17:06:56 UTC	2	6	F52 — Pan-STARRS 2, Haleakala	0.715′	fitted
2026-09-14 20:21:37 UTC	2	8	G96 — University of Arizona Mt. Lemmon Survey	0.118′	fitted
2026-09-15 03:40:22 UTC	3	11	H21 — Astronomical Research Observatory, Westfield	0.009′	fitted

P22q6aE

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 09:06:47 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	0.795′	fitted
2026-09-14 17:08:01 UTC	2	5	F52 — Pan-STARRS 2, Haleakala	1.453′	fitted

P22q6ca

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 10:30:42 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	0.588′	fitted
2026-09-14 17:09:18 UTC	2	5	F52 — Pan-STARRS 2, Haleakala	0.847′	fitted
2026-09-14 22:22:11 UTC	3	8	R48 — Centro Astronomico Alto Turia 2	0.020′	fitted

P22q6nE

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 12:14:38 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	1.157′	fitted
2026-09-14 17:10:47 UTC	2	6	F51 — Pan-STARRS 1, Haleakala	0.948′	fitted
2026-09-14 21:45:19 UTC	4	10	106 — Crni Vrh	0.025′	fitted
2026-09-14 22:32:12 UTC	2	12	595 — Farra d'Isonzo	0.025′	fitted
2026-09-14 22:40:06 UTC	3	15	958 — Observatoire de Dax	0.024′	fitted
2026-09-14 23:55:05 UTC	3	18	K51 — Osservatorio del Celado, Castello Tesino	0.021′	fitted
2026-09-15 01:15:06 UTC	3	21	L01 — Visnjan Observatory, Tican	0.005′	fitted
2026-09-15 03:50:57 UTC	3	24	807 — Cerro Tololo Observatory, La Serena	0.003′	fitted
2026-09-15 04:47:14 UTC	3	27	W62 — Comet Hunter Observatory2, New Ringgold	0.001′	fitted

P22qbe3

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 21:39:59 UTC	3	3	F52 — Pan-STARRS 2, Haleakala	729.000′	fitted

P22qblY

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 22:06:40 UTC	4	4	F52 — Pan-STARRS 2, Haleakala	3.883′	fitted

PDOB866

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-13 17:20:05 UTC	3	3	Z84 — Calar Alto-Schmidt	3.250′	fitted
2026-09-13 21:20:22 UTC	4	7	Z84 — Calar Alto-Schmidt	0.014′	fitted

RJT002

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-09 21:02:59 UTC	3	3	194 — Tivoli	6.183′	fitted

S06001

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 22:52:57 UTC	10	10	S06 — ASTRIS Osservatorio Astronomico Claudio Del Sole	2,760.000′	fitted

SE000AI

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-15 03:11:38 UTC	4	4	R43 — TransAstra TKO at e-EYE	8.283′	fitted

SWAN26Q

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-05 02:39:20 UTC	8	8	249 — SOHO	—	fit-error
2026-09-06 01:55:49 UTC	4	12	247 — Roving Observer	—	fit-error
2026-09-06 18:50:16 UTC	5	17	C49 — STEREO-A	—	fit-error
2026-09-08 00:10:33 UTC	2	19	247 — Roving Observer	—	fit-error

Sar2913

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-15 03:30:06 UTC	3	3	K88 — GINOP-KHK, Piszkesteto	0.165′	fitted

ZTF10Fo

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-10 13:35:32 UTC	4	4	I41 — Palomar Mountain--ZTF	387.000′	fitted

ZTF10Fp

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-10 13:47:52 UTC	4	4	I41 — Palomar Mountain--ZTF	2,400.000′	fitted

ZTF10Fq

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 04:26:13 UTC	2	2	I41 — Palomar Mountain--ZTF	—	insufficient-observations

ZTF10Fr

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 04:26:39 UTC	4	4	I41 — Palomar Mountain--ZTF	2,280.000′	fitted

ZTF10Fv

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 21:33:56 UTC	4	4	I41 — Palomar Mountain--ZTF	2,760.000′	fitted

ZTF10Fw

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 21:34:16 UTC	4	4	I41 — Palomar Mountain--ZTF	3,420.000′	fitted
2026-09-12 23:57:11 UTC	2	6	I41 — Palomar Mountain--ZTF	528.000′	fitted

ZTF10Fx

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 21:34:31 UTC	4	4	I41 — Palomar Mountain--ZTF	2,820.000′	fitted

ZTF10Fy

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 21:35:03 UTC	4	4	I41 — Palomar Mountain--ZTF	2,880.000′	fitted

ZTF10G2

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 03:59:16 UTC	4	4	I41 — Palomar Mountain--ZTF	4,020.000′	fitted

ZTF10G3

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 03:59:40 UTC	4	4	I41 — Palomar Mountain--ZTF	1,680.000′	fitted

ZTF10G6

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 16:49:15 UTC	4	4	I41 — Palomar Mountain--ZTF	1,440.000′	fitted
2026-09-14 20:46:44 UTC	2	6	I41 — Palomar Mountain--ZTF	6.600′	fitted
2026-09-14 21:51:52 UTC	3	9	595 — Farra d'Isonzo	0.016′	fitted
2026-09-14 23:45:20 UTC	2	11	I41 — Palomar Mountain--ZTF	0.014′	fitted
2026-09-15 01:00:10 UTC	3	14	L01 — Visnjan Observatory, Tican	0.011′	fitted
2026-09-15 01:05:52 UTC	2	16	L04 — ROASTERR-1 Observatory, Cluj-Napoca	0.010′	fitted

ZTF10G8

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 21:36:18 UTC	4	4	I41 — Palomar Mountain--ZTF	970.000′	fitted

ZTF10G9

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 21:37:07 UTC	4	4	I41 — Palomar Mountain--ZTF	2,880.000′	fitted

jdq0079

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-06 22:23:33 UTC	3	3	B67 — Sternwarte Mirasteilas, Falera	1.767′	fitted

oRc0136

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-10 07:31:32 UTC	10	10	O18 — WFST, Lenghu	2.983′	fitted
2026-09-13 05:40:07 UTC	3	13	H21 — Astronomical Research Observatory, Westfield	0.004′	fitted

oRc0205

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-10 07:31:32 UTC	3	3	O18 — WFST, Lenghu	11.650′	fitted

oRc0346

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-10 07:31:32 UTC	4	4	O18 — WFST, Lenghu	7.367′	fitted

oRe0171

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-11 19:41:35 UTC	3	3	O18 — WFST, Lenghu	691.000′	fitted

oRh0119

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-14 19:42:59 UTC	3	3	O18 — WFST, Lenghu	3.783′	fitted

orA5256

Purpose: shows how this object’s independently reconstructed orbit uncertainty changed after each actual observation submission. Read: lower points are more precise; the vertical scale is logarithmic.

Submission UTC	New observations	Cumulative observations	Stations	Uncertainty at submission	Fit status
2026-09-12 03:54:42 UTC	3	3	J43 — Oukaimeden Observatory, Marrakech	5.033′	fitted
2026-09-12 21:32:58 UTC	3	6	R48 — Centro Astronomico Alto Turia 2	0.108′	fitted
2026-09-13 00:17:41 UTC	3	9	185 — Observatoire Astronomique Jurassien-Vicques	0.013′	fitted
2026-09-13 01:40:42 UTC	3	12	I41 — Palomar Mountain--ZTF	0.012′	fitted
2026-09-13 05:07:28 UTC	3	15	807 — Cerro Tololo Observatory, La Serena	0.002′	fitted
2026-09-13 07:14:07 UTC	2	17	J43 — Oukaimeden Observatory, Marrakech	0.001′	fitted
2026-09-15 03:05:02 UTC	3	20	807 — Cerro Tololo Observatory, La Serena	0.004′	fitted

Orbit uncertainty after observation submissions