Caution!! Although I am happy to share my research notes below with all visitors to my webpages, these pages are mainly designed for my own use and subject to change without warning. I do not guarantee the correctness of all contents as well. |
ARO HHT telescope (see more details at ARO HHT telescope's homepage) Table of contents: 1. basic information
Basic information of the HHT telescope Name: Heinrich Hertz Submillimeter Telescope The temperature given in HHT observation data file is T*_A, the observed source antenna temperature corrected for atmospheric attenuation, radiative loss and rearward scattering and spillover. The main beam temperature can be calculated as T_mb = T*_A / eta_fss / eta*_m = T*_A / eta_m Here eta*_m is corrected main beam efficiency, Beam sizes and telescope efficiencies [back to top] I got the measurements of beam size and efficienies of HHT from Dr. Bill Peters, the ARO stuff member. The measurements are roughly valid for observations using 1.3mm receiver during 2004-2005, but should be also valid for other years not far from this time range. For observations with the Martin-Puplett installed (the image side band reducer used for single side band observations), the special main beam efficiency is eta_m = 0.65 (+-0.1) for
polarization channel A (Note: The measured values of eta_m do not show significant variation with frequency or elevation within the measurement errors.) For observations without the Martin-Puplett installed (e.g., the observations with the ALMA band 6 mixer), the efficency is somewhat higher, say, eta_m = 75-80%. -------------------- FWHM main beam size can be calculated for different frequencies by the empirical formula: BWHM = 1.2 * Lambda / D
(for using the 1.3 mm receiver) where 1.2 and 1.25 are measured coefficients, Lambda is the observed wavelength in unit of meter and D is the physical diameter of HHT collector -- 10 m. The difference in the coefficients 1.2 and 1.25 is due to the slight difference in the illumination patterns for the two receivers. Examples of the main beam size: BWHM = 34 arcsec at 220 GHz (1.3mm receiver) Flux density can be derived from the main beam temperature as [back to top] S_nu = BWHM(")2 / lambda(cm)2 * T_mb * 5.097 X 10-4 [Jy] Here BWHM is angular full beam width at half maximum of the Gaussian main beam in arcsec, lambda is observed wavelength in cm. HHT BWHM and special main beam efficiency used by literature: [back to top] Data File Formats [back to top]
# List of some Extended Green Objects:
# Spectral line pointing Catalogue # Positions Obtained from Simbad unless otherwise noted, # * adjusted for PM 00:23:14.26 +55:47:33.9 J2000 TCas -7.0 LSR RAD # 1.0 01:06:25.96 +12:35:53.5 J2000 WXPsc 8.5 LSR RAD # 1.4 01:26:58.07 -32:32:34.0 J2000 RScl -18.4 LSR RAD # 1.5 2.2 01:33:51.21 +62:26:53.5 J2000 GL230 -54.0 LSR RAD # 0.9 02:19:20.80 -02:58:40.7 J2000 Mira 46.5 LSR RAD # 6.8 *J2005[back to top] |
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