; ORDER ;--------------------------------------------------------------- ;! Adverb used usually to specify the order of polynomial fit ;# ADVERB GENERAL SPECTRAL ;----------------------------------------------------------------------- ;; Copyright (C) 1999, 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 ;----------------------------------------------------------------------- ORDER LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC ---------------------------------------------------------------- ORDER Type: Adverb (Real) Use: ORDER usually is used to express the order of a polynomial in fitting a spectral baseline. Null value: 0 Means fit a zero-order polynomial (DC). Tasks: AGAUS.......Fits 1-dimensional Gaussians to absorption-line spectra BSCOR.......Combines two beam-switched images. ORDER controls the removal of a baseline from each row of each image. BSGRD.......Task to image beam-switched single-dish data. ORDER controls the removal of a baseline from each row of each image. ELFIT.......Plots/fits selected contents of SN, TY, SY, PC or CL files. ORDER is the polynomial order fit to the data in antenna zenith angle, elevation, hour angle, etc. FLGIT.......Flags data based on the rms of the spectrum IMLIN.......Fits and removes continuum emission from image cube SDLSF.......Removes continuum from single-dish line data, flags bad samples, writes also a continuum data set. SLFIT.......Task to fit gaussians to slice data. SOUSP.......Fits source spectral index from SU table or adverbs. ORDER selects spectral index plus optionally various degrees of spectral curvature. UVLIN.......Fits and removes continuum visibility spectrum, also can flag. UVLSD.......Least squares fit to channels and divides the uv data. UVLSF.......Removes continuum from UV data, flags bad samples, writes also a continuum data set. UVMLN.......Edits data based on the rms of the spectrum. XBASL.......Fits and subtracts nth-order baselines from cube (x axis) XGAUS.......Fits 1-dimensional Gaussians to images: restartable. XTRAN.......Create an image with transformed coordinates. ORDER is the number of parameters to be fit (3 or 6). "Verbs": BDF2AIPS....Read EVLA ASDM/BDF data into AIPS. ORDER is a logical to prevent/allow reordering of IFs. ----------------------------------------------------------------