TABLE
2
Summary of Sky Survey Telescopes
SurveyStatusAperture (m)f/noField-of-view (degree2 )Magnitude limitSpeed (degree2
per hour)Ref.CSS – Mt. Lemmonoperational1.52.01.321201CSS – Catalina Schmidtoperational0.681.9819.51501CSS – Siding Spring Uppsala Schmidtoperational0.53.54.219.5751LINEARoperational2
×1.02.22.019.412002LONEOS (Schmidt)operational0.441.98.319.31063LONEOS (USNO)in development1.32.41.321.4153NEAT (Palomar)operational1.21.59.522.5854NEAT (MSSS)operational1.23.02.319.740.54NEAT (Schmidt)in development1.22.59.4∼20.0504Spacewatch (Mosaic)operational0.933.02.921.51605Spacewatch (1.8 m)operational1.822.70.3222.58.95Pan-STARRS (Hawaii)in development4
×1.843.024.07006Discovery Channel Telescope (Lowell)in development4.02.23.121.81107Large Synoptic Survey Telescopeproposed6.91.257.024.025008References: (1) Catalina Sky Survey, http://www.lpl.arizona.edu/css/, (2) Lincoln Near Earth Asteroid Research, http://www.ll.mit.edu/LINEAR/, (3) Lowell Observatory Near-Earth-Object Search,http://asteroid.lowell.edu/asteroid/loneos/loneos1.html, (4) Near-Earth Asteroid Tracking, http://neat.jpl.nasa.gov/, (5) http://spacewatch.lpl.arizona.edu/, (6) Panoramic Survey Telescope & Rapid ResponseSystem, http://pan-starrs.ifa.hawaii.edu/public/, (7) http://www.lowell.edu/DCT/, (8) http://www.lsst.org/1. Field-of-view is the area of sky covered in a single exposure.2. Magnitude limit is the faintest star recorded at visible wavelengths.3. Speed is the rate at which observations can be carried out. One can see that of the operational facilities, LINEAR covers the most sky per hour (1200 degree2 /hour) but the faintest stars it can observe at thisspeed is 19.4 mag. The Spacewatch (1.8 m) telescope can observe stars that are 3 magnitudes fainter but at a speed of only 8.9 degree2 /hour).732