; DOACOR ;--------------------------------------------------------------- ;! specifies whether autocorrelation data are included ;# ADVERB UV CALIBRATION ;----------------------------------------------------------------------- ;; Copyright (C) 2001, 2020 ;; Associated Universities, Inc. Washington DC, USA. ;; ;; This program is free software; you can redistribute it and/or ;; modify it under the terms of the GNU General Public License as ;; published by the Free Software Foundation; either version 2 of ;; the License, or (at your option) any later version. ;; ;; This program is distributed in the hope that it will be useful, ;; but WITHOUT ANY WARRANTY; without even the implied warranty of ;; MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the ;; GNU General Public License for more details. ;; ;; You should have received a copy of the GNU General Public ;; License along with this program; if not, write to the Free ;; Software Foundation, Inc., 675 Massachusetts Ave, Cambridge, ;; MA 02139, USA. ;; ;; Correspondence concerning AIPS should be addressed as follows: ;; Internet email: aipsmail@nrao.edu. ;; Postal address: AIPS Project Office ;; National Radio Astronomy Observatory ;; 520 Edgemont Road ;; Charlottesville, VA 22903-2475 USA ;----------------------------------------------------------------------- DOACOR LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC ---------------------------------------------------------------- DOACOR Type: Adverb (Logical, > 0 => true) Use: True (> 0) means to include autocorrelation data in some operation. False (<= 0) means to omit autocorrelation data. Null value: false (-1). Tasks: ALVPR.........Prints statistics on the Allan Variance of a UV data set. AVSPC.........Averages uv-data in the frequency domain. BPWGT.........Calibrates data and scales weights by bandpass correction. DIFRL.........Divides the RR data by LL data. FGCNT.........Counts samples comparing two flag tables. FILLM.........Reads VLA on-line/archive format uv data tapes (post Jan 88). FLOPM.........Reverses the spectral order of UV data, can fix VLA error. FRPLT.........Task to plot fringe rate spectra. FUDGE.........Modifies UV data with user's algorithm: paraform task. LISTR.........Prints contents of UV data sets and assoc. calibration tables. NOIFS.........Makes all IFs into single spectrum. PHSRF.........Perform phase-referencing within a spectral line database. REWAY.........Computes weights based in rms in spectra. SPMOD.........Modify UV database by adding a model with spectral lines. SUFIX.........Modifies source numbers on uv data. SWAPR.........Modifies UV data by swapping real and imaginary parts. UVAVG.........Average or merge a sorted (BT, TB) uv database. UVBAS.........Averages several channels and subtracts from uv data. UVFRE.........Makes one data set have the spectral structure of another. UVLIN.........Fits and removes continuum visibility spectrum, also can flag. UVLSD.........Least squares fit to channels and divides the uv data. UVLSF.........Least squares fit to channels and subtracts from uv data. UVMOD.........Modify UV database by adding a model incl spectral index. UVMTH.........Averages one data set and applies it to another. UVPLT.........Plots data from a UV data base in multiple ways. UVPRT.........Prints data from a UV data base with calibration. UVRFI.........Mitigate RFI by Fourier transform or fitting the circle. XYMOD.........Compute linear polarization point source model, applies to data. ----------------------------------------------------------------