Summary of OSCIR Engineering/Commissioning (June 2000)
OSCIR, the visiting University of Florida 10um imager and spectrograph, has just completed its first commissioning run on Gemini North. This period saw several engineering firsts for Gemini: the first use of chopping synchronised to an instrument, the first test of the Visitor Instrument Interface (used to exchange commands and status information between OSCIR and the Telescope Control System), the first chopping and nodding of the telescope, the first attempts at simultaneous chopping and fast guiding and, of course, the first 10um images.
|The image (at right) is of the young planetary nebula NGC7027 and consists
of 1 minute chopped integration using a 10 arcsec chop throw at 3Hz taken through the
broad-band 10um filter. It has been smoothed with a 3 pixel (0.26 arcsec) Gaussian. The
excellent image quality is evident, for example, in the emission peak to the far left
(north-west on the sky) that has a full-width at half maximum of slighly less than 0.4
The bulk of the emission in this waveband is from dust particles and large hydrocarbon molecules, which can only survive outside of the ionized central region. There is also some emission from ionized atoms within the hot central region.
Planetary nebulae are large luminous shells of material ejected from dying stars. The material of this particular PN was ejected about a thousand years ago and is currently about 100 times the size of our Solar System.
Some notable results from this highly successful engineering run include:
We are extremely grateful for the hard work put in by the OSCIR team (Charlie Telesco,
Robert Pina, Kevin Hanna, Jeff Julian, Scott Fisher, Chris Packham, Naibi Marinas and
David Ciardi), Chris Mayer (Observatory Sciences Ltd., for the VII) and the Gemini support
Last update July 5, 2000; Phil Puxley