PSABA
Photometry > 2017
| Telescope code | Telescope | Mount | f ratio | focuser | Camera | "/pix | observatory |
| B14 | SCT 0.35m | Paramount MX | 5.9 | TCFs | ST8XME | 0.98 | Q68 |
| B14Edge | SCT 0.35m | Paramount MX+ | 11 | Optec fast focus | U6M | 1.28 | Q68 |
| B24 | CDK 0.61m | MI-1250 Fork | 6.8 | Planewave | U42 | 0.70 | Q68 |
| Telescope code | Telescope | Mount | f ratio | focuser | Camera | "/pix | observatory |
| JBL02 | RCOS 0.32 | Paramount MX+ | Robofocus | STL 11000 | 1.28 | ||
| JBL04 | TAK 0.18D | Paramount ME | Robofocus | STL 11000 | |||
| JBL01 | RCOS 0.40 | Paramount ME | Robofocus | STL 11000 | 1.07 |
| Telescope code | Telescope | Mount | f ratio | focuser | Camera | "/pix | observatory |
| P12 Groom | SCT 0.35m | Paramount ME | ST 8XME | ||||
| P14 PO | SCT 0.35 | Paramount ME | ST 10XME |
(10498) Bobgent
dual periodic light curve but no events detected
P1=3.455h
P2=5.708h
JBL02

(32621) 1996 PA
PSABA target


(23621) 1996 PA
D. Pray, Sugarloaf Mountain Observatory, South Deerfield, MA, U.S.A.;
J. Oey, Blue Mountains Observatory, Leura, NSW, Australia; P. Pravec, H.
Kucakova, and K. Hornoch, Ondrejov Observatory; V. Benishek, Belgrade
Astronomical Observatory; and A. Marchini, R. Papini, and F. Salvaggio,
Dipartimento di Scienze Fisiche, Della Terra e Dell'Ambiente, University of
Siena, report that photometric observations obtained with a 0.50-m telescope
at the Sugarloaf Mountain Observatory, a 0.35-m telescope at the Blue
Mountains Observatory, a 0.65-m telescope at the Ondrejov Observatory,
a 0.35-m telescope at the Sopot Observatory in Serbia, and a 0.30-m
telescope at the Astronomical Observatory of the University of Siena during
July 16-Sept. 25 reveal that minor planet (23621), whose orbit crosses that
of Mars, is a binary system with an orbital period of 20.60 ± 0.03 hr.
The primary shows a period of 2.6649 ± 0.0005 hr and has a lightcurve
amplitude of 0.07 mag at solar phases 1-4 degrees, suggesting a nearly
spheroidal shape. Mutual eclipse/occultation events that are 0.04- to
0.12-magnitude deep indicate a lower limit on the secondary-to-primary
mean-diameter ratio of 0.27.
2017 October 4 (CBET 4436) Daniel W. E. Green
(15590) 2000 GH82
PSABA target

(16815) 1997 UA9
Paired asteroid. Taken 1 night per lunation
1829 Dawson
PSABA target
33 Data points







2859 Paganini
PSABA target.
the last night was linked using same comparison stars since 2859 was in a stationaly position as viewed from earth.
it confirm the low amplitude nature and longish period of 32.4h
3892 Deszo
Probable binary target for PSABA target.
4718 Araki
PSABA target
5887 Yauza
PSABA target
This asteroid show a long period bimodal light curve.
will continue to observe.
Data obtained from BMO 14Edge
5859 Ostozhenka
PSABA target
very low amplitude target .
shown the period spectrum for 6.89h
4760 Jia-Xiang
PSABA target.
initially target appear to have synch binary characteristic however after more data was collected, it appear to be a large amplitude asteroid.
telescope used..
JBL02 and DRO
4760 Jia-Xiang
Unusual light curve. possible synch binary but unconfirmed.






7368 Haldancohn
PSABA target
data taken with 24" CDK reflector with U42 (2015 Shoemaker NEO grant)
7368 Haldancohn
PSABA target from DRO
(14950) 1996 BE2
PSABA target
May target was taken with JBL02 and 24"



(14950) 1996 BE2
Data collected for the month of June. Amplitude is larger due to the usual Phase-Amplitude relation ship.
June data was taken with 14Edge
(15590) 2000 GH82
PSABA target 3 multiple coverage to arrive at a period of 3.7901h
(22766) 1999 AE7
PSABA target
24410 Juliewalker
PSABA target
(27005) 1998 DR35
PSABA target




31170 1997 WO58
PSABA target
This one turned out to be a tough target. It was not such long period as I
thought it might have been originally and the poor weather condition here meant I
couldn't get long sessions .
The Jan and Feb data pointed to a shorter 13.7h period and
0.3mag amplitude. However I have to adjust 12/09 and 01/20 by as much a
0.5mag. which I concluded to be stray . Once adjusted, the curve fit well into the 13.7h light curve
(35404) 1997 YV5
PSABA target
Unique period





94346 2001 QU88
PSABA target
54355 2000 KJ33
PSABA target
data taken with 24" CDK reflector with U42 (2015 Shoemaker NEO grant)
27005 1998 DR35
PSABA target
6707 Shigeru
PSABA target
data taken with 24" CDK reflector with U42 (2015 Shoemaker NEO grant)
4750 Mukai
PSABA target
Long period but showing signs of tumbling at 38.3h
data taken with 24" CDK reflector with U42 (2015 Shoemaker NEO grant)


1401 Lavonne
PSABA target
