Status of the Thirty Meter Telescope site selection program

The Thirty Meter Telescope (TMT) project has been collecting data on five candidate sites since 2003. This paper describes the site testing portion of the TMT site selection program and the process and standards employed by it. This includes descriptions of the candidate sites, the process by which they were identified, the site characterization instrument suite and its calibration and the available results, which will be published shortly.

[1]  S. G. Els,et al.  Temporal variability of the seeing of TMT sites , 2008, Astronomical Telescopes + Instrumentation.

[2]  Edison Bustos,et al.  Monitoring the night sky with the Cerro Tololo All-Sky camera for the TMT and LSST projects , 2006, SPIE Astronomical Telescopes + Instrumentation.

[3]  J. Seguel,et al.  Study on the precision of the MASS turbulence profiler employed in the site testing campaign for the Thirty Meter Telescope , 2008 .

[4]  Brooke Gregory,et al.  An analysis of light pollution at the Thirty Meter Telescope candidate sites , 2008, Astronomical Telescopes + Instrumentation.

[5]  T. Travouillon,et al.  The Multi Aperture Scintillation Sensor (MASS) used in the site selection of the Thirty Meter Telescope (TMT) , 2008, Astronomical Telescopes + Instrumentation.

[6]  Ka-Ming Lau,et al.  Does a Monsoon Climate Exist over South America , 1998 .

[7]  T. Travouillon SODAR calibration for turbulence profiling in TMT site testing , 2006, SPIE Astronomical Telescopes + Instrumentation.

[8]  Reed L. Riddle,et al.  The Thirty Meter Telescope site testing robotic computer system , 2006, SPIE Astronomical Telescopes + Instrumentation.

[9]  Reed Riddle,et al.  Evaluation of sonic anemometers as highly sensitive optical turbulence measuring devices for the Thirty Meter Telescope site testing campaign , 2006, SPIE Astronomical Telescopes + Instrumentation.

[10]  Jerry Nelson,et al.  CELT site testing program , 2003, SPIE Astronomical Telescopes + Instrumentation.

[11]  David A. Naylor,et al.  Initial operations of a water vapour monitor (IRMA) at Gemini South, Las Campanas Observatories, and in the TMT site testing role , 2006, SPIE Astronomical Telescopes + Instrumentation.

[12]  Brooke Gregory,et al.  Using All Sky Cameras to determine cloud statistics for the Thirty Meter Telescope candidate sites , 2008, Astronomical Telescopes + Instrumentation.

[13]  K. Vogiatzis,et al.  TMT studies on the influence of short term changes of local thermodynamic conditions on the seeing: CFD vs. observations , 2006, SPIE Astronomical Telescopes + Instrumentation.

[14]  Sebastian G. Els,et al.  Status of the tmt site evaluation process , 2007 .

[15]  Edison Bustos,et al.  High-accuracy differential image motion monitor measurements for the Thirty Meter Telescope site testing program. , 2007, Applied optics.

[16]  Victor Kornilov,et al.  MASS: a monitor of the vertical turbulence distribution , 2003, SPIE Astronomical Telescopes + Instrumentation.

[17]  M. Sarazin,et al.  The ESO differential image motion monitor , 1990 .