PILOT: design and capabilities (2008)
Saunders, W., Gillingham, P. R., McGrath, A. J., Storey, J. W. V., Lawrence, J. S.
The proposed design for PILOT is a general-purpose, wide-field 1 degree 2.4m, f/10 Ritchey-Chretien telescope, with fast tip-tilt guiding, for use 0.5-25 microns. The design allows both wide-field...
Telescope and instrument robotization at Dome C (2007)
Strassmeier, K. G., Agabi, K., Agnoletto, L., Allan, A., Andersen, M. I., Ansorge, W., ...
This article reviews the situation for robotization of telescopes and instruments at the Antarctic station Concordia on Dome C. A brain-storming meeting was held in Tenerife in March 2007 from which...
Atmospheric scintillation at Dome C, Antarctica: implications for photometry and astrometry (2006)
Kenyon, S. L., Lawrence, J. S., Ashley, M. C. B., Storey, J. W. V., Tokovinin, A., Fossat, E.
We present low-resolution turbulence profiles of the atmosphere above Dome C, Antarctica, measured with the MASS instrument during 25 nights in March-May 2004. Except for the lowest layer, Dome C has...
Burton, Michael G., Lawrence, J. S., Ashley, M. C. B., Bailey, J. A., Blake, Chris, Bedding, T. R., ...
The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....
Burton, M. G., Lawrence, J., Ashley, M. C. B., Bailey, J. A., Blake, C., Bedding, T. R., ...
The cold, dry and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-mm wavelengths to be found on the Earth. PILOT is a...
The Trumpler 14 photodissociation region in the Carina Nebula (2003)
Brooks, K. J., Cox, P., Schneider, N., Storey, J. W. V., Poglitsch, A., Geis, N., ...
Photodissociation regions and star formation in the Carina Nebula (2001)
Rathborne, J. M., Burton, M. G., Brooks, K. J., Cohen, M., Ashley, M. C. B., Storey, J. W. V.
We have obtained wide-field thermal infrared (IR) images of the Carina Nebula, using the SPIREX/Abu telescope at the South Pole. Emission from poly-cyclic aromatic hydrocarbons (PAHs) at 3.29um, a...
H110alpha recombination-line emission and 4.8-GHz continuum emission in the Carina Nebula (2001)
Brooks, K. J., Storey, J. W. V., Whiteoak, J. B.
We present results from observations of H110alpha recombination-line emission at 4.874 GHz and the related 4.8-GHz continuum emission towards the Carina Nebula using the Australia Telescope Compact...
Unlocking the Keyhole - H2 and PAH emission from molecular clumps in the Keyhole Nebula (2000)
Brooks, K. J., Burton, M. G., Rathborne, J. M., Ashley, M. C. B., Storey, J. W. V.
To better understand the environment surrounding CO emission clumps in the Keyhole Nebula, we have made images of the region in H2 1-0 S(1) (2.122 um) emission and polycyclic aromatic hydrocarbon...
Brooks, K. J., Whiteoak, J. B., Storey, J. W. V.
The Carina Nebula is an extremely bright southern HII region embedded in a giant molecular cloud and contains some of the most massive stars known in our Galaxy. We are undertaking a multi-wavelength...
Mid-infrared [NeII] line emission from the nucleus of NGC 253 (1998)
Boeker, T., Krabbe, A., Storey, J. W. V.
We report on mid-infrared (MIR) continuum and line emission mapping of the nucleus of NGC 253. The data, with a resolution of 1\as.4, reveal a double-peaked arc-like [NeII] emission region....
Molecular Hydrogen Line Emission from the Reflection Nebula Parsamyan 18 (1997)
Ryder, S. D., Allen, L. E., Burton, M. G., Ashley, M. C. B., Storey, J. W. V.
The newly-commissioned University of New South Wales Infrared Fabry-Perot (UNSWIRF) has been used to image molecular hydrogen emission at 2.12 and 2.25 microns in the reflection nebula Parsamyan 18....