Infrared detectors and telescopes


Recall the thermal background we noted before:

[ir bkgd]

Image from McLean, I., Electronic Imaging in Astronomy, © 1997 John Wiley & Sons

 

Design of optical vs. infrared-optimized telescopes:

The 4-meter telescopes at Kitt Peak and Cerro Tololo are both classically-designed (i.e. not IR-optimized) telescopes.

The Mayall 4-meter telescope at Kitt Peak National Observatory:

[Mayall 4m]

The Blanco 4-meter telescope at CTIO:

[Blanco 4m]

[CTIO 4-meter telescope]


UKIRT, the United Kingdom Infrared Telescope:

[ukirt]


Note the lack of large sky baffles and the relatively open design:

[ukirt]


Note the thin supports holding up the very small secondary mirror:

[ukirt]


A schematic of the telescope design:

[ukirt schematic]


An infrared array, showing the composite structure:

[ir array]

Image © 1997 McLean, I., Electronic Imaging in Astronomy, John Wiley & Sons


A basic schematic of a bolometer:

Image © 1994 Rieke, G., Detection of Light from the Ultraviolet to the Submillimeter, Cambridge University Press


Next: An example: the young star DQ Tau


Eric Jensen <ejensen1@swarthmore.edu>
Last modified: June 12, 2006