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A new small radio telescope is recently available at the Bosscha Observatory. To properly utilize this telescope some important characteristics must be derived using appropriate methods. This characterization consists of determination of beamwidth, aperture efficiency, and pointing errors. A receive...

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Main Author: UTOMO (NIM 10305017), DYAS
Format: Final Project
Language:Indonesia
Online Access:https://digilib.itb.ac.id/gdl/view/10289
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Institution: Institut Teknologi Bandung
Language: Indonesia
id id-itb.:10289
spelling id-itb.:102892017-09-27T11:42:15Z#TITLE_ALTERNATIVE# UTOMO (NIM 10305017), DYAS Indonesia Final Project INSTITUT TEKNOLOGI BANDUNG https://digilib.itb.ac.id/gdl/view/10289 A new small radio telescope is recently available at the Bosscha Observatory. To properly utilize this telescope some important characteristics must be derived using appropriate methods. This characterization consists of determination of beamwidth, aperture efficiency, and pointing errors. A receiver capable to provide observations at 1420 MHz is then used to determine galactic rotation curve. Therefore, the retrieved galactic rotation curve covers only interior regions of the Galaxy, that is, from the galactic center to the Sun's orbit. Comparison with the published result (Clemens 1985) is discussed. <br /> text
institution Institut Teknologi Bandung
building Institut Teknologi Bandung Library
continent Asia
country Indonesia
Indonesia
content_provider Institut Teknologi Bandung
collection Digital ITB
language Indonesia
description A new small radio telescope is recently available at the Bosscha Observatory. To properly utilize this telescope some important characteristics must be derived using appropriate methods. This characterization consists of determination of beamwidth, aperture efficiency, and pointing errors. A receiver capable to provide observations at 1420 MHz is then used to determine galactic rotation curve. Therefore, the retrieved galactic rotation curve covers only interior regions of the Galaxy, that is, from the galactic center to the Sun's orbit. Comparison with the published result (Clemens 1985) is discussed. <br />
format Final Project
author UTOMO (NIM 10305017), DYAS
spellingShingle UTOMO (NIM 10305017), DYAS
#TITLE_ALTERNATIVE#
author_facet UTOMO (NIM 10305017), DYAS
author_sort UTOMO (NIM 10305017), DYAS
title #TITLE_ALTERNATIVE#
title_short #TITLE_ALTERNATIVE#
title_full #TITLE_ALTERNATIVE#
title_fullStr #TITLE_ALTERNATIVE#
title_full_unstemmed #TITLE_ALTERNATIVE#
title_sort #title_alternative#
url https://digilib.itb.ac.id/gdl/view/10289
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