http://cso.caltech.edu/wiki/ 2026-09-16T00:35:39+00:00 http://cso.caltech.edu/wiki/ http://cso.caltech.edu/wiki/lib/tpl/cso/images/favicon.ico text/html 2015-06-27T07:11:58+00:00 http://cso.caltech.edu/wiki/cso/instruments/music/data_qa?rev=1435389118&do=diff data QA Several tools are available for quality assurance checks on the data you collect. In order to use these tools, you must first enter your sources in the MUSIC data reduction parameters files, which are located on kilauea in the folder ~/bolocam_svn/pipeline/automation/params/. There are two files, a cleaning parameters file and a mapping parameters file. Your sources must be entered in these files using the same name as entered in the uip source catalog, although all letters must be lowe… text/html 2015-01-16T01:15:36+00:00 http://cso.caltech.edu/wiki/cso/instruments/music/macros?rev=1421370936&do=diff Scripts Scripts are used for MUSIC observations. These scripts interact with the MUSIC data acquisition system (DAQ) and control the scan pattern of the telescope. Standard scripts are located at kilauea:~bolocam/macros/. The standard file extension is text/html 2015-05-21T20:48:37+00:00 http://cso.caltech.edu/wiki/cso/instruments/music/music?rev=1432241317&do=diff MUSIC In its present configuration, the MUltiwavelength Sub/millimeter Inductance Camera (MUSIC) has an 12×6 arcmin field of view, three simultaneous colors, and 175 operational detectors. Sensitivity Band Wavel. Freq. Bandw. Beam Lissajous text/html 2015-02-17T20:49:18+00:00 http://cso.caltech.edu/wiki/cso/instruments/music/observing?rev=1424206158&do=diff Observing To Start an Observation * Select a target. * For a cataloged, non-planet target, uip> observe obj_name * For a planet, uip> planet name * Wait for the telescope to start tracking. * The CSO Antenna Monitor will display text/html 2015-02-17T20:52:08+00:00 http://cso.caltech.edu/wiki/cso/instruments/music/setup?rev=1424206328&do=diff Startup This is a brief synopsis of the setup for Music at the CSO. It continues from the general Introduction to Observing. In case of difficulties, consult the staff. Fridge temperature Check the cryostat temperature. The UC Stage (bottom row, second from the right) should be 0.225 K text/html 2014-10-31T22:17:13+00:00 http://cso.caltech.edu/wiki/cso/instruments/music/shutdown?rev=1414793833&do=diff Shutdown Hand Off to Another Observer If you are remote observing and someone else is taking over: * Contact the next observers to verify they are ready to observe. * Save the observing log. * Exit from ooffice if necessary. * Verify the new observers have control of the telescope and the transition went smoothly. text/html 2014-12-16T00:58:22+00:00 http://cso.caltech.edu/wiki/cso/instruments/music/strategy?rev=1418691502&do=diff General observing strategy In order to obtain data with accurate flux and pointing calibration, the following general strategy should be followed: * An IQ sweep of the resonators should be performed once per hour while tracking a source and whenever a new source is acquired.