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Photometry > 2017

Obs Code	Name	Longitude	Latitude	Altitude	Time (UT)
Q68	BMO	150d 20' 30"	-33d 42' 22"	950m	+10h

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
P12 Groom	SCT 0.35m	Paramount ME			ST 8XME
P14 PO	SCT 0.35	Paramount ME			ST 10XME
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

393 Lampetia

Collaboration with Frederick Pilcher and Anna Marciniak to arrive a period of 38.455h.

Data published .

4058 Cecilgreen

Target of opportunity in the same fov as 24410 on 23/04/17

5859 Ostozhenka

Asteroid happened to be in the stationary movement in the sky allowing 6 nights linkages using same comparison stars. This method is very reliable and allowing accurate links to 0.01 magnitude over many nights. Giving a good light curve determination even with a low amplitude problem as in this case.

9671 Hemera

Observation started by Alessandro Marchini et al. from Italy and analysed by Petr Pravec shown that the light curve is double periodic indicating a probable binary scenario.

BMO _ JBL02 intend to observe the target until events found.

13958 1991 DY

Target of opportunity in the same Fov as 6097 Koishikawa

data taken with 24" CDK reflector with U42 (2015 Shoemaker NEO grant)

92545 2000 OV30

Object of opportunity within the same fov as 6707 Shigeru.

68 Data points

data taken with 24" CDK reflector with U42 (2015 Shoemaker NEO grant)

6199 Yoshiokayayoi

CALL target . favourable apparition . full moon target to start of .

No.

Asteroid

2015/mm/dd

LPAB

BPAB

Period

Amplitude

Diameter

Telescope

31170

1997 WO58

B14,B24,B14E