Master index
| Master index |
Index for comms |
 BestOpacity | |
| CalcTheoOp | calculated theoretical zenith opacity based on weather station data |
| NoiseDiodeOp | NoiseDiodeOp gives the zenith opacity by calibrating the skydip amplitude |
| SkyDipMethod2v2 | calculate Zenith Opacity from SkyDips using new filtered data |
| analyzeSpectrograms | This script reads in data between start and finish. It plots and returns |
| beammap | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
| fit_various | d = read_arc('27-jan-2010:00:12:00','27-jan-2010:00:20:00'); %cygA |
| integrateDown | Ystd = integrateDown(Y,intLength) |
| longTermOp | records long term opacity data alongside weather info |
| moon_scan | Moon Scan |
| noiseCalc | variables |
| parseBurst | |
| plotOvroSurf | %%%%%%%%%%%%%%%5 |
| raster | quick function to make a raster of a source when using the "beam_map.sch" |
| readOps | |
| read_spa | Get data |
| reduceData_simple | reduce the nice new data (from 6 channels not switch data) without |
| reduce_on_off | |
| scanForNDEvents | This script searches the data archive for noise diode events between |
| scanForNDEvents_DD | This script searches the data archive for noise diode events between |
| script4matthew | d = read_arc('10-dec-2009:23:48:46', '11-dec-2009:00:05:20'); |
| sidelobes_bb | first let's cut out the noise source data |
| sidelobes_cw_ms | tried to cut out the non-relevant data first, but that causes the |
| sidelobes_cw_sm | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
| skydip | Noise diode and sky dips |
| skydip_investigation | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
| source_raster | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
| source_raster_cal | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
| source_raster_remLeak_v2 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
| stare_track | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |