... We had a unique diagnostic tool for determining whether or not the secondary was fractured during the dark run in that we had 3 sets of focus sweep data for the imaging camera taken on the nights of 05 October 1999, 11 October 1999, and 14 October 1999. ... Figure: 05 October 1999, CCD g1 . ... Surface plot. ... Figure 32 plots the same data but for CCD g3. ... Figure: Comparison of normalised brighness for the out-of-focus doughnuts for the nights of 05, 11, and 14 October 1999 for CCD g1. ...

... Talks . Integral field spectroscopy of AGN host galaxies . Talk at the Research School of Astronomy and Astrophysics, The Australian National University, October 17th, 2011, in Canberra, Australia . ... Talk at the Centre for Astrophysics Supercomputing, Swinburne University of Technology, February 25th, 2010, in Melbourne, Australia . ... Talk at the Research School of Astronomy and Astrophysics of the Australian National University, May 28th, 2009, in Canberra, Australia . ...

... Detector - Machine Data Flow · Detector - Machine diagnostic info (slow) · Detector - Machine feedback inputs (fast) · Machine - Detector information Eric Torrence 2/8 July 2004 Polarimeter 532 nm Frequency Doubled YAG Laser e­ Mirror Box Pockels Cell Left or Right Circularly Polarized Photons Focusing and ... Eric Torrence 7/8 July 2004 Putting it all together Beam Instrumentation historically runs in a semi-autonomous manner from either machine or detector. ...

12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 Mode switch Idle mode Initalise hand-shake FTT mode Seeing estimates Acquisition mode Seeing estimates Acq check mode Dark frame mode Dk xfer to ISS Use of dk frame Flat field mode FF xfer to ISS Use of ff frame Coordinate xform Sensor wavelength Space envelope ...

... The two-faced Whirlpool Galaxy . Probing a galaxy's dust structure serves as an important diagnostic tool for astronomers, providing invaluable information on how gas and dust collapse to form stars. ... The image at left, taken in visible light, highlights the attributes of a typical spiral galaxy, including graceful, curving arms, pink star-forming regions, and brilliant blue strands of star clusters. ... The visible-light image captured only some of the light; dust obscured the rest. ...

CFITSIO Interface Library CFITSIO is a library of ANSI C routines for reading and writing FITS format data files. ... The CFITSIO library is built on Unix systems by typing: > ./configure [--prefix=/target/installation/path] > make (or 'make shared') > make install (this step is optional) at the operating system prompt. The configure command customizes the Makefile for the particular system, then the `make' command compiles the source files and builds the library. ...

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