.TH HAWKI_SCIENCE_POSTPROCESS "7" "2.4.11" "hawki_science_postprocess" "hawki recipes" .SH NAME hawki_science_postprocess \- HAWKI post processing recipe .SH SYNOPSIS esorex .B hawki_science_postprocess [OPTIONS] FILE.sof .SH DESCRIPTION hawki_science_postprocess \-\- HAWKI science post processing recipe. .PP Postprocess a stacked pawprint for HAWKI data. Form a filled tile and photometrically and astrometrically calibrate the tiled image Optionally nebulise the stacked images before source detection The program accepts the following files in the SOF: Tag Description BASIC_CALIBRATED_SCI A set of processed images from a jitter sequence BASIC_VAR_MAP A variance map for each sequence image MASTER_CONF A master confidence map for the jitter sequence PHOTCAL_TAB A photometric calibration table MASTER_2MASS_CATALOGUE_ASTROM A master 2MASS index for astrometry or MASTER_PPMXL_CATALOGUE_ASTROM A master PPMXL index for astrometry or MASTER_LOCAL_CATALOGUE_ASTROM A master local astrometric FITS file MASTER_2MASS_CATALOGUE_PHOTOM A master 2MASS index for photometry or MASTER_PPMXL_CATALOGUE_PHOTOM A master PPMXL index photometry or MASTER_LOCAL_CATALOGUE_PHOTOM A master local photometric FITS file MATCHSTD_PHOTOM A master photometric matched stds catalogue (optional) SCHLEGEL_MAP_NORTH Northern Schlegel Map SCHLEGEL_MAP_SOUTH Southern Schlegel Map All of the above are required unless specified otherwise. The astrometricand photometric files are not required if these can be obtained fromthe CDS using the \-\-cdssearch options .SH OPTIONS .TP \fB\-\-nebulise\fR \fI\fR Nebulise the stacks before object detection? (bool; default: False). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.nebulise\fR [default = \fIFalse\fR]. .TP \fB\-\-minphotom\fR \fI\fR Minimum number of stars for photometry solution (int; default: 20). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.minphotom\fR [default = \fI20\fR]. .TP \fB\-\-prettynames\fR \fI\fR Use pretty product names? (bool; default: False). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.prettynames\fR [default = \fIFalse\fR]. .TP \fB\-\-cdssearch_astrom\fR \fI\fR CDS astrometric catalogue (str; default: \'none\'). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.cdssearch_astrom\fR [default = \fInone\fR]. .TP \fB\-\-cdssearch_photom\fR \fI\fR CDS photometric catalogue (str; default: \'none\'). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.cdssearch_photom\fR [default = \fInone\fR]. .TP \fB\-\-stk_fast\fR \fI\fR Use fast stacking? (str; default: \'auto\'). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.stk_fast\fR [default = \fIauto\fR]. .TP \fB\-\-stk_nfst\fR \fI\fR Nframes before we switch to slow stack algorithm (int; default: 30). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.stk_nfst\fR [default = \fI30\fR]. .TP \fB\-\-savemstd\fR \fI\fR Save matched standard catalogues? (bool; default: False). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.savemstd\fR [default = \fIFalse\fR]. .TP \fB\-\-neb_medfilt\fR \fI\fR Median filter size for nebuliser (int; default: 101). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.neb_medfilt\fR [default = \fI101\fR]. .TP \fB\-\-neb_linfilt\fR \fI\fR Linear filter size for nebuliser (int; default: 33). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.neb_linfilt\fR [default = \fI33\fR]. .TP \fB\-\-cat_ipix\fR \fI\fR Minimum pixel area for each detected object (int; default: 4). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.cat_ipix\fR [default = \fI4\fR]. .TP \fB\-\-cat_thresh\fR \fI\fR Detection threshold in sigma above sky (float; default: 2.5). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.cat_thresh\fR [default = \fI2.5\fR]. .TP \fB\-\-cat_icrowd\fR \fI\fR Use deblending? (bool; default: True). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.cat_icrowd\fR [default = \fITrue\fR]. .TP \fB\-\-cat_rcore\fR \fI\fR Value of Rcore in pixels (float; default: 10.0). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.cat_rcore\fR [default = \fI10.0\fR]. .TP \fB\-\-cat_nbsize\fR \fI\fR Background smoothing box size (int; default: 64). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.cat_nbsize\fR [default = \fI64\fR]. .TP \fB\-\-cacheloc\fR \fI\fR Location for standard star cache (str; default: \'.\'). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.cacheloc\fR [default = \fI.\fR]. .TP \fB\-\-magerrcut\fR \fI\fR Cut in magnitude error (float; default: 100.0). The full name of this option for the EsoRex configuration file is \fBhawki.hawki_science_postprocess.magerrcut\fR [default = \fI100.0\fR]. .PP 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. .SH SEE ALSO The full documentation for the hawki pipeline can be downloaded as a PDF file using the following URL: .IP .B ftp://ftp.eso.org/pub/dfs/pipelines/hawki/hawki\-pipeline\-manual\-2.4.11.pdf .PP An overview over the existing ESO pipelines can be found on the web page \fBhttps://www.eso.org/sci/software/pipelines/\fR. .PP Basic documentation about the EsoRex program can be found at the esorex (1) man page. .PP It is possible to call the pipelines from python using the python\-cpl package. See \fBhttps://packages.python.org/python\-cpl/index.html\fR for further information. .PP The other recipes of the hawki pipeline are .IR hawki_cal_dark (7), .IR hawki_cal_distortion (7), .IR hawki_cal_flat (7), .IR hawki_cal_zpoint (7), .IR hawki_dark_combine (7), .IR hawki_detector_noise (7), .IR hawki_linearity_analyse (7), .IR hawki_sci_jitter (7), .IR hawki_science_process (7), .IR hawki_standard_process (7), .IR hawki_step_apply_dist (7), .IR hawki_step_basic_calib (7), .IR hawki_step_combine (7), .IR hawki_step_compute_bkg (7), .IR hawki_step_detect_obj (7), .IR hawki_step_photom_2mass (7), .IR hawki_step_refine_offsets (7), .IR hawki_step_stats (7), .IR hawki_step_stitch (7), .IR hawki_step_subtract_bkg (7), .IR hawki_tec_filtchk (7), .IR hawki_twilight_flat_combine (7), .IR hawki_util_gendist (7), .IR hawki_util_stdstars (7) .SH VERSION hawki_science_postprocess 2.4.11 .SH AUTHOR Jim Lewis .SH BUG REPORTS Please report any problems to jrl@ast.cam.ac.uk. Alternatively, you may send a report to the ESO User Support Department . .SH LICENSE This file is part of the HAWKI Instrument Pipeline Copyright (C) 2015 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., 59 Temple Place, Suite 330, Boston, MA 02111\-1307 USA