2011
DOI: 10.1017/s1743921312010630
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Spitzer observations of planetary nebulae

Abstract: Abstract. The Spitzer Space Telescope has three science instruments (IRAC, MIPS, and IRS) that can take images at 3. 6, 4.5, 5.8, 8.0, 24, 70, and 160 µm, spectra over 5-38 µm, and spectral energy distribution over 52-100 µm. The Spitzer archive contains targeted imaging observations for more than 100 PNe. Spitzer legacy surveys, particularly the GLIMPSE survey of the Galactic plane, contain additional serendipitous imaging observations of PNe. Spitzer imaging and spectroscopic observations of PNe allow us to … Show more

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“…The terahertz (THz) wave band (frequency range from 0.1 to 10 THz) contains the spectral fingerprint information of many celestial bodies and biological targets [ 1 , 2 ]. Therefore, THz detecting technology is regarded as a potential technical means for astronomical observation, medical diagnosis, nondestructive flaw detection, and so on.…”
Section: Introductionmentioning
confidence: 99%
“…The terahertz (THz) wave band (frequency range from 0.1 to 10 THz) contains the spectral fingerprint information of many celestial bodies and biological targets [ 1 , 2 ]. Therefore, THz detecting technology is regarded as a potential technical means for astronomical observation, medical diagnosis, nondestructive flaw detection, and so on.…”
Section: Introductionmentioning
confidence: 99%