Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.arcetri.astro.it/irlab/instr/firt/firt.php
Дата изменения: Unknown
Дата индексирования: Mon Feb 4 01:51:40 2013
Кодировка:

Поисковые слова: astro-ph
Arcetri Infrared Activities THE FIRT NEAR INFRARED PHOTOMETER


Main Sections
LabIR main page
Instrument page
Documentation
Science Publications

Special Sections
Software Page
Inside the Lab
LabIR staff

Companion Pages
Skysoft Home
Tirgo Page
Tirgo Archive
LabIR Hotlist
Lunar occultations
AO star finder
Simple calculator




Labir logo

The FIRT Near Infrared Photometer

The TIRGO NIR photometer uses a single InSb detector with cooled low-noise amplification electronics. Detector, filters, and diaphragms are cryogenically cooled to solid nitrogen temperature. The TIRGO NIR filter system closely approximates that of CalTech, although work is needed to better establish a color transformation between the two systems. The limiting magnitudes reported below are average values (roughly for a 4 mm diaphragm) and, since broad-band NIR observations are background-limited, will vary with observing aperture. FIRT gives the following choice of filters and diaphragms:

More information on following topics:

  • "Results of the TIRGO calibration program: 1986-1987" L.K. Hunt, G.Calamai, and E. Oliva Arcetri Technical Report No. 5/87
  • "Near-infrared photometry at the Gornergrat Infrared Telescope" L.K. Hunt Arcetri Technical Report No. 15/91
  • "Manuale del nuovo sistema di controllo del Fotometro del TIRGO" C.Baffa Arcetri Technical Report No. 8/92 Parti 1 e 2

Last Modified:
28/Jul/2005


Back one page Write Us Labir Home
Please select the LabIR Main Page or an item in the left menu.