A SPECTRAL LINE SURVEY FROM 159.7 TO 164.7 GHZ TOWARD ORION-KL: THE DATA |
LEE CHANG WON
(Korea Astronomy Observatory)
CHO SE-HYUNG (Korea Astronomy Observatory) |
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DOI ScienceOn |
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Microwave Spectra of Molecules of Astrophysical Interest. XXIV. Methanol (CH₃OH and <TEX>$^{13}CH_3$</TEX>OH)
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DOI ScienceOn |
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A Spectral Line Survey from 138.3 to 150.7 GHZ toward Orion-KL
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DOI ScienceOn |
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A molecular line survey of Sagittarius B2 and Orion-KL from 70 to 115 GHz. Ⅱ - analysis of the data
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DOI |
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Submillimeter, Millimeter, and Microwave Spectral Line Catalog
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DOI ScienceOn |
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The spectrum of Orion-KL at 2 millimeters (150-160 GHz)
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DOI |
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Surface Measurement of the TRAO 14 Meter Antenna with a Shearing Interferometry
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DOI ScienceOn |
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The Development of a Dual Channel SIS Receiver of TRAO Telescop
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DOI ScienceOn |
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Recommended Rest Frequencies for Observed Interstellar Molecular Microwave Transitions?1991 Revision
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DOI |
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A Quasioptical system of the Dual Channel SIS Receiver for TRAO Telescope
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DOI ScienceOn |
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The rotational emission-line spectrum of Orion A between 247 and 263 GHz
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DOI |
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