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JCMT Newsletter No. 11 (Early Start)
JACH | JCMT | UKIRT | Computer Services | Local server

An Early Start to the Evening Shift

Studies over the past few months show that changing ambient temperature effects on the antenna surface during the early evening can be significantly reduced if the carousel is opened well in advance of the commencement of observing. A closed building tends to exaggerate the distortions to the surface and when the building is finally opened. These effects persist well into evening shift, making it necessary for more frequent pointing, focus and efficiency checks.

Therefore, wherever possible, the TSS will open the building early to allow the antenna to stabilise well in advance of the nominal 17:30 start of evening shift. However, the daycrew leave the telescope at 16:00 sharp and if nobody is remaining to buddy the TSS then the TSS must also leave. This means that the building will be closed and the software systems run down.

If would be extremely helpful, to both the TSS and to the observers, if the evening shift observers at HP telephoned the TSS at no later than 15:30 to discuss the weather conditions, the state of the instruments and thus make preliminary plans for their evening shift.

Observers can, if they want to get a good start, drive to the telescope prior to the daycrew leaving at 16:00. The TSS will be able to leave the carousel open and make most, if not all, of the startup checks and tests (including the first run through pointing, focus and calibration) well in advance of the 17:30 nominal shift start time.

If observers are not particularly worried about an early start then at least the TSS is aware of this and can come down to HP for dinner without having to immediately turn around and drive back up with observers. Or, as is often the case, the TSS meets the observers on the way down to HP and has to turn around and go up again, having just completely shut down the carousel and the observing system.


JACH | JCMT | UKIRT | Computer Services | Local server

Modification Author: Graeme Watt (gdw)
Contact: Jonathan Kemp. Updated: Tue Aug 17 17:32:04 HST 2004

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