17 September 2012 Evaluations of new atmospheric windows at thirty micron wavelengths for astronomy
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Abstract
Thirty micron has remained one of unexplored frontiers of ground-based astronomical observations. Recent developments of extreme high sites including the Chajnantor TAO site (5,640m) enable us to access the this wavelengths from the ground. The expected transmittance seems clear enough for astronomical observations, but practical evaluations based on astronomical data has not been carried out yet. We have analyzed images obtained at the 31.7 micron with a mid-infrared camera MAX38 attached on a mini-TAO 1.0-meter telescope. 109 images of a star IRC+10420 and 11,114 images of the sky have been reduced. Clear relationship between the measured photocurrents and the perceptible water vapor has been found. Simple estimation of the photocurrents with of the ATRAN model gives good agreements with the measurements, indicating that the ATRAN model reproduce the atmospheric transmittance reasonably well. This also supports our assumption that the scaling factor 0.85 of the PVW at the Chajnantor TAO site to the PWV at the APEX. The average transmittance in the 31.7 micron is achieved to be over 20% when the PWV below 0.6 mm. In some cases clear degradation up to 10% in the transmittance is found. It may be caused by droplets of liquid or iced water with a size over 10 micron although the causes are not exactly specified. Diurnal time variations of the sky photocurrents are also investigated. The sky is sometimes bright and usually unstable in the twilight time. On the other hand the sky around the noontime does not show clear difference from the night sky. It may suggest that the observing condition at the thirty micron windows remain good even in the daytime.
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Takashi Miyata, Takashi Miyata, Shigeyuki Sako, Shigeyuki Sako, Takafumi Kamizuka, Takafumi Kamizuka, Tomohiko Nakamura, Tomohiko Nakamura, Kentaro Asano, Kentaro Asano, Mizuho Uchiyama, Mizuho Uchiyama, Masahiro Konishi, Masahiro Konishi, Mizuki Yoneda, Mizuki Yoneda, Naruhisa Takato, Naruhisa Takato, Yuzuru Yoshii, Yuzuru Yoshii, Mamoru Doi, Mamoru Doi, Kotaro Kohno, Kotaro Kohno, Kimiaki Kawara, Kimiaki Kawara, Masuo Tanaka, Masuo Tanaka, Kentaro Motohara, Kentaro Motohara, Takeo Minezaki, Takeo Minezaki, Toshihiko Tanabe, Toshihiko Tanabe, Tomoki Morokuma, Tomoki Morokuma, Yoichi Tamura, Yoichi Tamura, Tsutomu Aoki, Tsutomu Aoki, Takao Soyano, Takao Soyano, Ken'ichi Tarusawa, Ken'ichi Tarusawa, Hidenori Takahashi, Hidenori Takahashi, Shintaro Koshida, Shintaro Koshida, Natsuko M. Kato, Natsuko M. Kato, } "Evaluations of new atmospheric windows at thirty micron wavelengths for astronomy", Proc. SPIE 8444, Ground-based and Airborne Telescopes IV, 84446B (17 September 2012); doi: 10.1117/12.925258; https://doi.org/10.1117/12.925258
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