The Berkeley-Illinois-Maryland-Association millimeter array
We describe the characteristics of the BIMA millimeter wave array at Hat Creek, CA. The array is an aperture synthesis instrument consisting of nine 6 m diameter antennas which may be deployed in three different configurations, with spacings ranging from 7 m up to 1.3 km. At an observing frequency o...
Päätekijät: | , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Aineistotyyppi: | Journal article |
Julkaistu: |
1996
|
_version_ | 1826295088867704832 |
---|---|
author | Welch, W Thornton, D Plambeck, R Wright, M Lugten, J Urry, L Fleming, M Hoffman, W Hudson, J Lum, W Forster, JR Thatte, N Zhang, X Zivanovic, S Snyder, L Crutcher, R Lo, K Wakker, B Stupar, M Sault, R Miao, Y Rao, R Wan, K Dickel, H Blitz, L |
author_facet | Welch, W Thornton, D Plambeck, R Wright, M Lugten, J Urry, L Fleming, M Hoffman, W Hudson, J Lum, W Forster, JR Thatte, N Zhang, X Zivanovic, S Snyder, L Crutcher, R Lo, K Wakker, B Stupar, M Sault, R Miao, Y Rao, R Wan, K Dickel, H Blitz, L |
author_sort | Welch, W |
collection | OXFORD |
description | We describe the characteristics of the BIMA millimeter wave array at Hat Creek, CA. The array is an aperture synthesis instrument consisting of nine 6 m diameter antennas which may be deployed in three different configurations, with spacings ranging from 7 m up to 1.3 km. At an observing frequency of 100 GHz these configurations yield maps with angular resolutions of 5″, 2″, and 0.″4, over a 2′ field. Larger fields may be mapped by using multiple pointings. For all but the oldest telescopes, the surface accuracy is ≤30 μm rms, and the aperture efficiency is 77% at 100 GHz. Background emission from antenna losses and spillover is very low, about 5 K after subtraction of the cosmic B v(2.1 K). Each antenna contains a single dewar which accommodates up to four separate receivers. SIS mixers are cooled to 3.2 K with novel Gifford-McMahon cycle refrigerators. Both the upper and lower sidebands of the first local oscillator are received and separated, providing two bands extending from 70-900 MHz on each side of the first local oscillator. The correlation spectrometer covers a bandwidth of up to 800 MHz, and provides up to 2048 channels for each antenna pair. There are four independently tunable spectral windows (in each sideband), allowing simultaneous observations of several different spectral lines. The spectral resolution ranges from 6 kHz to 3 MHz. For a single 8-hr track in one configuration, the sensitivity is approximately 1 mJy/beam in the 800 MHz wide continuum. Measurements of atmospheric phase fluctuations as functions of both time and baseline have been made; these indicate that routine imaging at angular resolutions of less than 1″ at 100 GHz is possible only if self-calibration or some other means of phase correction can be applied. Examples of a few recent results are included. We note that 30% of the observing time on the array is granted to visitors. |
first_indexed | 2024-03-07T03:55:43Z |
format | Journal article |
id | oxford-uuid:c2ce5f98-ce84-4aea-b0f2-117d8ca943c7 |
institution | University of Oxford |
last_indexed | 2024-03-07T03:55:43Z |
publishDate | 1996 |
record_format | dspace |
spelling | oxford-uuid:c2ce5f98-ce84-4aea-b0f2-117d8ca943c72022-03-27T06:11:44ZThe Berkeley-Illinois-Maryland-Association millimeter arrayJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:c2ce5f98-ce84-4aea-b0f2-117d8ca943c7Symplectic Elements at Oxford1996Welch, WThornton, DPlambeck, RWright, MLugten, JUrry, LFleming, MHoffman, WHudson, JLum, WForster, JRThatte, NZhang, XZivanovic, SSnyder, LCrutcher, RLo, KWakker, BStupar, MSault, RMiao, YRao, RWan, KDickel, HBlitz, LWe describe the characteristics of the BIMA millimeter wave array at Hat Creek, CA. The array is an aperture synthesis instrument consisting of nine 6 m diameter antennas which may be deployed in three different configurations, with spacings ranging from 7 m up to 1.3 km. At an observing frequency of 100 GHz these configurations yield maps with angular resolutions of 5″, 2″, and 0.″4, over a 2′ field. Larger fields may be mapped by using multiple pointings. For all but the oldest telescopes, the surface accuracy is ≤30 μm rms, and the aperture efficiency is 77% at 100 GHz. Background emission from antenna losses and spillover is very low, about 5 K after subtraction of the cosmic B v(2.1 K). Each antenna contains a single dewar which accommodates up to four separate receivers. SIS mixers are cooled to 3.2 K with novel Gifford-McMahon cycle refrigerators. Both the upper and lower sidebands of the first local oscillator are received and separated, providing two bands extending from 70-900 MHz on each side of the first local oscillator. The correlation spectrometer covers a bandwidth of up to 800 MHz, and provides up to 2048 channels for each antenna pair. There are four independently tunable spectral windows (in each sideband), allowing simultaneous observations of several different spectral lines. The spectral resolution ranges from 6 kHz to 3 MHz. For a single 8-hr track in one configuration, the sensitivity is approximately 1 mJy/beam in the 800 MHz wide continuum. Measurements of atmospheric phase fluctuations as functions of both time and baseline have been made; these indicate that routine imaging at angular resolutions of less than 1″ at 100 GHz is possible only if self-calibration or some other means of phase correction can be applied. Examples of a few recent results are included. We note that 30% of the observing time on the array is granted to visitors. |
spellingShingle | Welch, W Thornton, D Plambeck, R Wright, M Lugten, J Urry, L Fleming, M Hoffman, W Hudson, J Lum, W Forster, JR Thatte, N Zhang, X Zivanovic, S Snyder, L Crutcher, R Lo, K Wakker, B Stupar, M Sault, R Miao, Y Rao, R Wan, K Dickel, H Blitz, L The Berkeley-Illinois-Maryland-Association millimeter array |
title | The Berkeley-Illinois-Maryland-Association millimeter array |
title_full | The Berkeley-Illinois-Maryland-Association millimeter array |
title_fullStr | The Berkeley-Illinois-Maryland-Association millimeter array |
title_full_unstemmed | The Berkeley-Illinois-Maryland-Association millimeter array |
title_short | The Berkeley-Illinois-Maryland-Association millimeter array |
title_sort | berkeley illinois maryland association millimeter array |
work_keys_str_mv | AT welchw theberkeleyillinoismarylandassociationmillimeterarray AT thorntond theberkeleyillinoismarylandassociationmillimeterarray AT plambeckr theberkeleyillinoismarylandassociationmillimeterarray AT wrightm theberkeleyillinoismarylandassociationmillimeterarray AT lugtenj theberkeleyillinoismarylandassociationmillimeterarray AT urryl theberkeleyillinoismarylandassociationmillimeterarray AT flemingm theberkeleyillinoismarylandassociationmillimeterarray AT hoffmanw theberkeleyillinoismarylandassociationmillimeterarray AT hudsonj theberkeleyillinoismarylandassociationmillimeterarray AT lumw theberkeleyillinoismarylandassociationmillimeterarray AT forsterjr theberkeleyillinoismarylandassociationmillimeterarray AT thatten theberkeleyillinoismarylandassociationmillimeterarray AT zhangx theberkeleyillinoismarylandassociationmillimeterarray AT zivanovics theberkeleyillinoismarylandassociationmillimeterarray AT snyderl theberkeleyillinoismarylandassociationmillimeterarray AT crutcherr theberkeleyillinoismarylandassociationmillimeterarray AT lok theberkeleyillinoismarylandassociationmillimeterarray AT wakkerb theberkeleyillinoismarylandassociationmillimeterarray AT stuparm theberkeleyillinoismarylandassociationmillimeterarray AT saultr theberkeleyillinoismarylandassociationmillimeterarray AT miaoy theberkeleyillinoismarylandassociationmillimeterarray AT raor theberkeleyillinoismarylandassociationmillimeterarray AT wank theberkeleyillinoismarylandassociationmillimeterarray AT dickelh theberkeleyillinoismarylandassociationmillimeterarray AT blitzl theberkeleyillinoismarylandassociationmillimeterarray AT welchw berkeleyillinoismarylandassociationmillimeterarray AT thorntond berkeleyillinoismarylandassociationmillimeterarray AT plambeckr berkeleyillinoismarylandassociationmillimeterarray AT wrightm berkeleyillinoismarylandassociationmillimeterarray AT lugtenj berkeleyillinoismarylandassociationmillimeterarray AT urryl berkeleyillinoismarylandassociationmillimeterarray AT flemingm berkeleyillinoismarylandassociationmillimeterarray AT hoffmanw berkeleyillinoismarylandassociationmillimeterarray AT hudsonj berkeleyillinoismarylandassociationmillimeterarray AT lumw berkeleyillinoismarylandassociationmillimeterarray AT forsterjr berkeleyillinoismarylandassociationmillimeterarray AT thatten berkeleyillinoismarylandassociationmillimeterarray AT zhangx berkeleyillinoismarylandassociationmillimeterarray AT zivanovics berkeleyillinoismarylandassociationmillimeterarray AT snyderl berkeleyillinoismarylandassociationmillimeterarray AT crutcherr berkeleyillinoismarylandassociationmillimeterarray AT lok berkeleyillinoismarylandassociationmillimeterarray AT wakkerb berkeleyillinoismarylandassociationmillimeterarray AT stuparm berkeleyillinoismarylandassociationmillimeterarray AT saultr berkeleyillinoismarylandassociationmillimeterarray AT miaoy berkeleyillinoismarylandassociationmillimeterarray AT raor berkeleyillinoismarylandassociationmillimeterarray AT wank berkeleyillinoismarylandassociationmillimeterarray AT dickelh berkeleyillinoismarylandassociationmillimeterarray AT blitzl berkeleyillinoismarylandassociationmillimeterarray |