NAME¶visir_util_img_std_cat - Convert ASCII-file(s) to a FITS standard star catalog
SYNOPSIS¶esorex visir_util_img_std_cat [OPTIONS] FILE.sof
DESCRIPTION¶This recipe generates a FITS standard star catalog for imaging from one or more ASCII-files.
Each line in the text file must have 45 fields separated by white-space.
The first field is the star name, e.g. ´HD108903´ which will be stored in a table column labeled ´STARS´.
The 3 next fields are the RA (hh mm ss) which will be stored in degrees in a table column labeled ´RA´ - all three are non-negative and hh and mm are integer.
The 3 next fields are the DEC (dd mm ss) which will be stored in degrees in a table column labeled ´DEC´ - all three are non-negative, dd and mm are integer, while dd has either a ´+´ or a ´-´ prepended (including -00).
The next field is the spectral type which will be stored in a table column labeled ´SP_TYPE´.
The 31 next fields are the JY values for the 31 supported image filters.
The 6 next fields are the JY values for the 6 supported spectral filters.
All JY values must be positive.
For each filter the JY value is stored in a table column labeled with the filter name.
The 37 filter names are hard-coded in the recipe.
Lines beginning with a hash (#) are treated as comments.
The ASCII-input should be tagged IMG_LINES_ASCII, but all input files will currently be processed regardless.
OPTIONS¶Note that it is possible to create a configuration file containing these options, along with suitable default values. Please refer to the details provided by the 'esorex --help' command.
SEE ALSO¶The full documentation for the visir pipeline can be downloaded as a PDF file using the following URL:
An overview over the existing ESO pipelines can be found on the web page https://www.eso.org/sci/software/pipelines/.
Basic documentation about the EsoRex program can be found at the esorex (1) man page.
It is possible to call the pipelines from python using the python-cpl package. See https://packages.python.org/python-cpl/index.html for further information.
The other recipes of the visir pipeline are visir_img_dark(7), visir_img_ff(7), visir_img_reduce(7), visir_img_trans(7), visir_old_img_combine(7), visir_old_img_phot(7), visir_old_spc_obs(7), visir_old_spc_obs_ech(7), visir_old_spc_phot(7), visir_old_spc_phot_ech(7), visir_old_spc_wcal(7), visir_old_spc_wcal_ech(7), visir_old_util_destripe(7), visir_spc_reduce(7), visir_util_apply_calib(7), visir_util_clip(7), visir_util_convert_weight(7), visir_util_detect_shift(7), visir_util_join(7), visir_util_qc(7), visir_util_repack(7), visir_util_run_swarp(7), visir_util_spc_std_cat(7), visir_util_spc_txt2fits(7), visir_util_undistort(7)
AUTHOR¶Lars Lundin <firstname.lastname@example.org>
BUG REPORTS¶Please report any problems to email@example.com. Alternatively, you may send a report to the ESO User Support Department <firstname.lastname@example.org>.
LICENSE¶This file is part of the VISIR Instrument Pipeline Copyright (C) 2004, 2005 European Southern Observatory
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., 51 Franklin St, Fifth Floor, Boston, MA 02111-1307 USA