A An alphabetical summary of Surf commands

ADD_DBM: Generate simulated dual beam images (page 112)

BOLREBIN: Generate a separate regridded image for each bolometer. (page 113)

CALCSKY: Calculate sky variation independent of source structure (page 117)

CHANGE_DATA: Change data (or variance) values in a dataset. (page 119)

CHANGE_FLAT: Change the stored flatfield information. (page 121)

CHANGE_NACENTRE: Shift Nasmyth centre of array (page 122)

CHANGE_POINTING: Change Az and El pointing offsets for map data. (page 123)

CHANGE_QUALITY: Change data quality. (page 124)

DESPIKE: Despike JIGGLE/MAP data (page 126)

DESPIKE2: Despike SCAN/MAP data (page 129)

DSPBOL: Interactive despiking and data inspection (Requires Kappa) (page 131)

EXTINCTION: Corrects demodulated data for atmospheric extinction (page 133)

EXTRACT_DATA: Write bolometer positions and data to text a file (page 134)

EXTRACT_FLAT: Write flatfield information to text file (page 136)

FLATFIELD: Multiply the data array by the flatfield volumes. (page 137)

INTREBIN: Generate a separate regridded image for each integration. (page 138)

MAPSUM: Generate a summary of map observations (page 142)

OBSSUM: Summarize all observations (page 144)

PHOTSUM: Generate a summary of photometry observations (page 146)

PLTBOL: Interactive data inspection (Requires Kappa) (page 148)

POINTSUM: Generate a summary of pointing observations (page 149)

QDRAW: Plot photometry data (requires Kappa). (page 151)

REBIN: Rebin all data onto a rectangular grid (page 152)

REDUCE_NOISE: Process raw noise data files (page 156)

REDUCE_SWITCH: Convert raw demodulated data to standard format and process individual switches. (page 157)

REMDBM: Remove dual beam signature from SCAN/MAP images (requires Kappa). (page 158)

REMIP: Remove instrumental polarisation from polarimetry data (page 159)

REMSKY: Remove sky contribution from each jiggle (page 161)

RESTORE: Remove dual-beam response from SCAN/MAP data. (page 164)

RLINPLOT: Interactive data inspection via mlinplot (Requires Kappa) (page 165)

SCAN_RLB: Remove linear baselines from SCAN/MAP data (page 166)

SCUBA2MEM: Calculates bolometer positions with chops (page 168)

SCUCAT: Concatenates photometry results into a single NDF. (page 170)

SCUCLIP: Perform sigma clipping of each bolometer (page 172)

SCUCLKERR: Determine potential inconsistency in the SCUBA time headers (page 173)

SCUHELP: Interactive help system (page 174)

SCULOG: Provide detailed descriptions of all observation data. (page 176)

SCUMAKEWT: Generate fourier weights of chop function (page 178)

SCUNOISE: Display SCUBA noise data (page 179)

SCUOVER: Overlay bolometer array on image (page 180)

SCUPA: Show position angle of array (Requires Kappa) (page 182)

SCUPHOT: Reduces photometry data to a single point per integration (page 183)

SCUPLOT: Interactive despiking and data inspection (Requires Kappa) (page 185)

SCUQUICK: Semi-automated data reduction pipeline. (page 187)

SCUSETENV: Set SCUBA environment variables (JAC only) (page 190)

SCUSHIFT: Shift bolometers on A-to-D card (page 191)

SDIP: Script to reduce and display skydip data (requires Kappa). (page 192)

SETBOLWT: Calculate and set bolometer weights (requires Kappa) (page 193)

SIGCLIP: Remove spikes from photometry data (requires Kappa). (page 194)

SKYDIP: Calculate sky opacity from skydip data (page 195)

SKYSUM: Generate a summary of skydip observations (page 197)