AIPS HELP file for IN2NAME in 31DEC22
As of Wed Jul 6 6:12:51 2022
HELP SECTION
IN2NAME
Type: Adverb (String*12)
Use: Data files are stored in AIPS under logical names which have 3
parts: a 12-character "name" field, a 6-character "class" field,
and a numeric "sequence number" field. IN2NAME is used to specify
the "name" field for the 2nd of the input data files used by a
verb or task. This adverb is handled by AIPS tasks and verbs
under special "wildcard" rules. These rules determine which test
strings (e.g. image names in the catalog) match the user-specified
string. Except for '*', '?', and trailing blanks (when an * is
present), all characters specified in IN2NAME must exactly match
the corresponding characters in the test string. A '?' in IN2NAME
matches any single character in the test string. An '*' in
IN2NAME matches 0 or more characters in the test string. Thus,
IN2NAME = '*' matches any test string. IN2NAME = 'A?B*D' matches
'ASBD', 'A BXYZD D', and 'A3B45678901D', but does not match 'ABCD'
or 'ASBCDE'.
Null value: ' '
Taken as '*' unless the Help file for the specific task or verb
states otherwise.
Verbs:
CLR2NAME......Clears adverbs specifying the second input image.
GET2NAME......Fills 2nd input image name parameters by catalog slot
number.
IM2HEAD.......Displays the image 2 header contents to terminal, message
file.
IMDIST........Determines spherical distance between two pixels.
Q2HEADER......Verb to summarize the image 2 header: positions at
center.
Procedures:
DOFARS........Procedure to aid in Faraday rotation synthesis using the
FARS task. The 2nd image is of U polarization.
IMFRING.......Large image delay fitting with IM2CC and OOFRING. The
2nd catalog file is the large image to be broken into
facets.
IMSCAL........Large image self-cal with IM2CC and OOCAL. The 2nd
catalog file is the large image to be broken into facets.
OOCAL.........Determines antenna complex gain with frequency-dependent
models. The 2nd image is the source model.
OOFRING.......Fringe fit data to determine calibration with spectral
index options. The 2nd image is the source model.
PEELR.........Calibrates interfering sources in multi-facet images.
The 2nd image is the Clean map model.
TVDIST........Determines spherical distance between two pixels on TV
screen. The 2nd image contains the 2nd pixel.
VLBABPSS......Computes spectral bandpass correction table. the 2nd
image is the Clean model.
VLBAMPHC......Applies VLBARUN calibration to additional phase stopping
centers. The 2nd data set contains the VLBARUN
calibration and flag tables.
Tasks:
ACFIT.........Determine antenna gains from autocorrelations. The 2nd
data set contains the template.
AFARS.........Is used after FARS to determine Position and Value of the
maximum. The 2nd image is the imaginary part or phase.
APCLN.........Deconvolves images with CLEAN algorithm. The 2nd image
is the dirty beam,
APGS..........Deconvolves image with Gerchberg-Saxton algorithm.
The 2nd image is the dirty beam,
APVC..........Deconvolves images with van Cittert algorithm.
The 2nd image is the dirty beam,
BDAPL.........Applies a BD table to another data set. The 2nd data
set is the one with the BD table.
BDEPO.........Computes depolarization due to rotation measure
gradients. The 2nd image is of the y-axis RN gradient.
BLANK.........Blanks out selected, e.g. non-signal, portions of an
image. The 2nd image contains the clip levels.
BLCAL.........Compute closure offset corrections. The 2nd image is
the Clean model image.
BLCHN.........Compute closure offset corrections on a
channel-by-channel basis. The 2nd image is the Clean
model image.
BLING.........Find residual rate and delay on individual baselines.
The 2nd image is the Clean model image.
BLSUM.........Sums images over irregular sub-images, displays spectra.
The 2nd image is the blotch image.
BPASS.........Computes spectral bandpass correction table.
The 2nd image is the Clean model image.
BSCLN.........Hogbom Clean on beam-switched difference image. The
2nd image is of the minus switch position.
BSCOR.........Combines two beam-switched images. The
2nd image is of the minus switch position.
CALIB.........Determines antenna calibration: complex gain.
The 2nd image is the Clean model image.
CAPLT.........Plots closure amplitude and model from CC file.
The 2nd image is the Clean model image.
CCRES.........Removes or restores a CC file to a map with a gaussian
beam. The 2nd image is the image with the Clean
components.
CLPLT.........Plots closure phase and model from CC file.
The 2nd image is the Clean model image.
CMPLX.........Combines complex images by a variety of mathematical
methods.
COMB..........Combines two images by a variety of mathematical methods.
CONVL.........Convolves an image with a gaussian or another image.
The 2nd image is the convolving image.
CPASS.........Computes polynomial spectral bandpass correction table.
The 2nd image is the Clean model image.
CXCLN.........Complex Hogbom CLEAN. The 2nd image is of the dirty beam.
DBCON.........Concatenates two UV data sets.
DCONV.........Deconvolves a gaussian from an image. The 2nd image is
of weights.
DGAUS.........Correct UV model for convolution by Clean beam
DIFUV.........Outputs the difference of two matching input uv data
sets.
EDITR.........Interactive baseline-oriented visibility editor using the
TV. The 2nd data set is displayed for comparison
purposes only and is optional.
EVAUV.........Subtracts & divides a model into UV data, does statistics
on results. The 2nd image is the Clean model image.
FARS..........Faraday rotation synthesis based on the brightness vs
wavelength. The 2nd image is of U polarization.
FFT...........Takes Fourier Transform of an image or images. The 2nd
image is the imaginary part.
FIXAL.........Least squares fit aliasing function and remove. The
2nd data set contains calibration information.
FRCAL.........Faraday rotation self calibration task. The 2nd image
is the Clean model image.
FRING.........Fringe fit data to determine antenna calibration, delay,
rate. The 2nd image is the Clean model image.
GAL...........Determine parameters from a velocity field. The 2nd
image is of weights.
GREYS.........Plots images as contours over multi-level grey. The
2nd image is used for contouring.
HGEOM.........Interpolates image to different gridding and/or geometry.
The 2nd image is the template for regridding the 1st.
HUINT.........Make RGB image from images of intensity & hue, like
TVHUEINT. The 2nd image is of hue.
IMAGR.........Wide-field and/or wide-frequency Cleaning / imaging task.
The 2nd data set is the work file.
IMERG.........Merges images of different spatial resolutions. The
2nd image is the low resolution one.
IMLHS.........Converts images to luminosity/hue TV display. The 2nd
image is of hue.
IMVIM.........Plots one image's values against another's. The 2nd
image values control the Y values.
KNTR..........Make a contour/grey plot file from an image w multiple
panels. The 2nd image may be used for contours, grey
scale, or as a polarization cutoff (I pol).
KRING.........Fringe fit data to determine antenna calibration, delay,
rate. The 2nd image is the Clean model image.
LPCAL.........Determines instrumental polarization for UV data. The
2nd image is the Clean model image.
MARSP.........Check Mars polarization angles
MATCH.........Changes antenna, source, FQ numbers to match a data set.
The 2nd data set defines the source, FQ, and antenna
numbers to be put in the 1st data set.
MEDI..........Combines four images by a variety of mathematical
methods.
MOD3D.........Computes a 3D CC model from a set of facets. The 2nd
image is the multi-facet Clean model.
MODIM.........Adds images of model objects to image cubes in IQU
polarization. The 2nd image is of Q polarization.
MODSP.........Adds images of model objects to image cubes in I/V
polarization. The 2nd image is of V polarization.
MOMFT.........Calculates images of moments of a sub-image. The 2nd
image is the dirty beam.
OFUDG.........Modifies UV data with user's algorithm no cal adverbs:
paraform task.
OHGEO.........Geometric interpolation with correction for 3-D effects.
The 2nd image is the template for regridding the 1st.
OOSUB.........Subtracts/divides a model from/into a uv data base.
The 2nd image is the Clean model.
PANEL.........Convert HOLOG output to panel adjustment table. The
2nd image is the mask image.
PASTE.........Pastes a selected subimage of one image into another.
The 2nd image is pasted into the first.
PCAL..........Determines instrumental polarization for UV data.
The 2nd image is the Clean model.
PCNTR.........Generate plot file with contours plus polarization
vectors. The 2nd image is of polarization intensity.
PDPLT.........Plots selected contents of PD tables.
PLAYR.........Task to load one or two images and play with them on the
TV.
PPAPP.........Applies Right minus Left phase difference to a 2nd data
set. The 2nd data set contains the PP file to apply.
QUFIX.........Determines Right minus Left phase difference, corrects
cal files. The 2nd image is a well-calibrated spectral
and polarization cube.
QUXTR.........Extracts text files from Q,U cubes for input to TARS.
The 2nd image is of U polarization.
RFARS.........Correct Q/U cubes for Faraday rotation synthesis results.
The 2nd image is of U polarization.
RLCAL.........Determines instrumental right-left phase versus time (a
self-cal). The 2nd image is a Clean model.
RM............Task to calculate rotation measure and magnetic field.
The 2nd image is of noise.
RM2PL.........Plots spectrum of a pixel with RMFIT fit.
The 2nd image is of U polarization.
RMFIT.........Fits 1-dimensional polarization spectrum to Q/U cube.
The 2nd image is of U polarization.
RSTOR.........Restores a Clean component file to a map with a Gaussian
beam. The 2nd image has the Clean components to be
restored to the 1st image.
SAD...........Finds and fits Gaussians to portions of an image.
The 2nd image is of the noise (rms).
SDCLN.........Deconvolves image by Clark and then "SDI" cleaning
methods. The 2nd image is of the dirty beam.
SDMOD.........Modifies single-dish UV data with model sources. The
2nd image is of the model.
SPCOR.........Task to correct an image for a primary beam and spectral
index. The 2nd image is of spectral index.
SPFIX.........Makes cube from input to and output from SPIXR spectral
index. The 2nd images are the outputs from SPIXR.
STEER.........Task which deconvolves the David Steer way. The 2nd
imager is of the dirty beam.
TADIF.........Prints differences between two table-format extension
files.
TBDIF.........Compare entries in two tables.
TRUEP.........Determines true antenna polarization from special data
sets. The 2nd data set is of visibilities with a feed
having been rotated.
TVHUI.........Make TV image from images of intensity, hue, saturation.
The 2nd image is of hue.
TVIEW.........Display image cube in all 3 transpositions with rotation
& reference. The 2nd image is the "reference"
TVRGB.........Make TV image from images of true color (RGB) images.
The 2nd image is of green.
TVSAD.........Finds and fits Gaussians to portions of an image with
interaction. The 2nd image is of noise (rms).
TVSPC.........Display images and spectra from a cube. The 2nd image
is of the transposed cube.
UTESS.........Deconvolves images by maximizing emptiness. The 2nd
image is of the dirty beam.
UVADC.........Fourier transforms and corrects a model and adds to uv
data. The 2nd image is of the Clean model.
UVADD.........Combines two matching uv data sets.
UVCON.........Generate sample UV coverage given a user defined array
layout. The 2nd image is of the model.
UVDI1.........Subtract UV data (averaged up to one time) from the other
UV data. The 2nd data set is averaged over all times
and then subtracted from the first.
UVDIF.........Prints differences between two UV data sets.
UVFRE.........Makes one data set have the spectral structure of
another. The 2nd data set defines the desired spectral
structure.
UVGLU.........Glues UV data frequency blocks back together.
UVMTH.........Averages one data set and applies it to another. The
2nd data set has the averaged 1st data set applied to
it.
UVSUB.........Subtracts/divides a model from/into a uv data base.
The 2nd image is the Clean model.
VBGLU.........Glues together data from multiple passes thru the VLBA
corr.
VLABP.........VLA antenna beam polarization correction for snapshot
images. The 2nd image is of the antenna fractional
polarization.
VPLOT.........Plots uv data and model from CC file. The 2nd image is
of a Clean model.
VTESS.........Deconvolves sets of images by the Maximum Entropy Method.
The 2nd image is of the dirty beam.
WARP..........Model warps in Galaxies.
WTSUM.........Task to do a a sum of images weighted by other images.
The 2nd image is the single image to be added. If
IN2NAME is blank the INSEQ to IN2SEQ are added.
XG2PL.........Plots spectrum of a pixel with XGAUS/AGAUS and
ZEMAN/ZAMAN fits. The 2nd image is of V polarization.
ZAMAN.........Fits 1-dimensional Zeeman model to absorption-line data.
The 2nd image is of I polarization.
ZEMAN.........Fits 1-dimensional Zeeman model to data.
The 2nd image is of I polarization.
EXPLAIN SECTION