| Astro-FITS-HdrTrans documentation | Contained in the Astro-FITS-HdrTrans distribution. |
Astro::FITS::HdrTrans::GEMINI - Base class for translation of Gemini instruments
use Astro::FITS::HdrTrans::GEMINI;
This class provides a generic set of translations that are common to instrumentation from the Gemini Observatory. It should not be used directly for translation of instrument FITS headers.
These methods are more complicated than a simple mapping. We have to provide both from- and to-FITS conversions All these routines are methods and the to_ routines all take a reference to a hash and return the translated value (a many-to-one mapping) The from_ methods take a reference to a generic hash and return a translated hash (sometimes these are many-to-many)
$Id: ESO.pm 14385 2007-08-27 22:01:06Z timj $
Astro::FITS::HdrTrans, Astro::FITS::HdrTrans::Base.
Paul Hirst <p.hirst@jach.hawaii.edu> Malcolm J. Currie <mjc@star.rl.ac.uk> Tim Jenness <t.jenness@jach.hawaii.edu>
Copyright (C) 2007-2008 Science and Technology Facilities Council. Copyright (C) 2006-2007 Particle Physics and Astronomy Research Council. All Rights Reserved.
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.
| Astro-FITS-HdrTrans documentation | Contained in the Astro-FITS-HdrTrans distribution. |
package Astro::FITS::HdrTrans::GEMINI;
use 5.006; use warnings; use strict; use Carp; # Inherit from the Base translation class and not HdrTrans itself # (which is just a class-less wrapper). use base qw/ Astro::FITS::HdrTrans::FITS /; use Scalar::Util qw/ looks_like_number /; use Astro::FITS::HdrTrans::FITS; use vars qw/ $VERSION /; $VERSION = "1.50"; # in each class we have three sets of data. # - constant mappings # - unit mappings # - complex mappings # for a constant mapping, there is no FITS header, just a generic # header that is constant my %CONST_MAP = ( ); # unit mapping implies that the value propogates directly # to the output with only a keyword name change my %UNIT_MAP = ( AIRMASS_END => "AMEND", AIRMASS_START => "AMSTART", DEC_BASE => "CRVAL2", EXPOSURE_TIME => "EXPTIME", EQUINOX => "EQUINOX", INSTRUMENT => "INSTRUME", NUMBER_OF_EXPOSURES => "NSUBEXP", NUMBER_OF_EXPOSURES => "COADDS", OBJECT => "OBJECT", X_REFERENCE_PIXEL => "CRPIX1", Y_REFERENCE_PIXEL => "CRPIX2" ); # Create the translation methods __PACKAGE__->_generate_lookup_methods( \%CONST_MAP, \%UNIT_MAP );
# Note use list context as there are multiple CD matrices in # the header. We want scalar context. sub to_DEC_SCALE { my $self = shift; my $FITS_headers = shift; my $cd11 = $FITS_headers->{"CD1_1"}; my $cd12 = $FITS_headers->{"CD1_2"}; my $cd21 = $FITS_headers->{"CD2_1"}; my $cd22 = $FITS_headers->{"CD2_2"}; my $sgn; if ( ( $cd11 * $cd22 - $cd12 * $cd21 ) < 0 ) { $sgn = -1; } else { $sgn = 1; } abs( sqrt( $cd11**2 + $cd21**2 ) ); } sub to_DEC_TELESCOPE_OFFSET { my $self = shift; my $FITS_headers = shift; # It's simple when there's a header. my $offset = $FITS_headers->{ "DECOFFSE" }; # Otherwise for older data have to derive an offset from the source # position and the frame position. This does assume that the # reference pixel is unchanged in the group. The other headers # are measured in degrees, but the offsets are in arceseconds. if ( !defined( $offset ) ) { my $decbase = $FITS_headers->{ "CRVAL2" } ; my $dec = $FITS_headers->{ "DEC" }; if ( defined( $decbase ) && defined( $dec ) ) { $offset = 3600.0 * ( $dec - $decbase ); } else { $offset = 0.0; } } return $offset; } sub from_DEC_TELESCOPE_OFFSET { my $self = shift; my $generic_headers = shift; "DECOFFSE", $generic_headers->{ "DEC_TELESCOPE_OFFSET" }; } sub to_FILTER { my $self = shift; my $FITS_headers = shift; my $filter = ""; my $filter1 = $FITS_headers->{ "FILTER1" }; my $filter2 = $FITS_headers->{ "FILTER2" }; my $filter3 = $FITS_headers->{ "FILTER3" }; if ( $filter1 =~ "open" ) { $filter = $filter2; } if ( $filter2 =~ "open" ) { $filter = $filter1; } if ( ( $filter1 =~ "blank" ) || ( $filter2 =~ "blank" ) || ( $filter3 =~ "blank" ) ) { $filter = "blank"; } return $filter; } sub to_OBSERVATION_TYPE { my $self = shift; my $FITS_headers = shift; my $type = $FITS_headers->{ "OBSTYPE" }; if ( $type eq "SCI" || $type eq "OBJECT-OBS" ) { $type = "OBJECT"; } return $type; } sub to_RA_BASE { my $self = shift; my $FITS_headers = shift; my $ra = 0.0; if ( exists ( $FITS_headers->{CRVAL1} ) ) { $ra = $FITS_headers->{CRVAL1}; } $ra = defined( $ra ) ? $ra: 0.0; return $ra; } sub to_RA_SCALE { my $self = shift; my $FITS_headers = shift; my $cd12 = $FITS_headers->{"CD1_2"}; my $cd22 = $FITS_headers->{"CD2_2"}; sqrt( $cd12**2 + $cd22**2 ); } sub to_RA_TELESCOPE_OFFSET { my $self = shift; my $FITS_headers = shift; # It's simple when there's a header. my $offset = $FITS_headers->{ "RAOFFSET" }; # Otherwise for older data have to derive an offset from the source # position and the frame position. This does assume that the # reference pixel is unchanged in the group. The other headers # are measured in degrees, but the offsets are in arceseconds. if ( !defined( $offset ) ) { my $rabase = $FITS_headers->{ "CRVAL1" }; my $ra = $FITS_headers->{ "RA" }; my $dec = $FITS_headers->{ "DEC" }; if ( defined( $rabase ) && defined( $ra ) && defined( $dec ) ) { $offset = 3600* ( $ra - $rabase ) * cosdeg( $dec ); } else { $offset = 0.0; } } return $offset; } sub from_RA_TELESCOPE_OFFSET { my $self = shift; my $generic_headers = shift; "RAOFFSE", $generic_headers->{ "RA_TELESCOPE_OFFSET" }; } # ROTATION, DEC_SCALE and RA_SCALE transformations courtesy Micah Johnson, from # the cdelrot.pl script supplied for use with XIMAGE. Extended here to the # FITS-WCS Paper II Section 6.2 prescription, averaging the rotation. sub to_ROTATION { my $self = shift; my $FITS_headers = shift; my $cd11 = $FITS_headers->{"CD1_1"}; my $cd12 = $FITS_headers->{"CD1_2"}; my $cd21 = $FITS_headers->{"CD2_1"}; my $cd22 = $FITS_headers->{"CD2_2"}; # Obtain the plate scales CDELT1 and CDELT2 equivalents as if we hasd a PCi_i matrix. my $sgn; if ( ( $cd11 * $cd22 - $cd12 * $cd21 ) < 0 ) { $sgn = -1; } else { $sgn = 1; } my $cdelt1 = $sgn * sqrt( $cd11**2 + $cd21**2 ); my $cdelt2 = $sgn * sqrt( $cd22**2 + $cd12**2 ); # Determine the sense of the scales. my $sgn2; if ( $cd12 < 0 ) { $sgn2 = -1; } else { $sgn2 = 1; } my $sgn3; if ( $cd21 < 0 ) { $sgn3 = -1; } else { $sgn3 = 1; } my $rtod = 45 / atan2( 1, 1 ); # Average the estimates of the rotation. my $rotation = $rtod * 0.5 * ( atan2( $sgn2 * $cd21 / $rtod, $sgn2 * $cd11 / $rtod ) + atan2( $sgn3 * $cd12 / $rtod, -$sgn3 * $cd22 / $rtod ) ); return $rotation; } sub to_UTSTART { my $self = shift; my $FITS_headers = shift; my $return; if (exists $FITS_headers->{'DATE-OBS'}) { my $iso; if ( $FITS_headers->{'DATE-OBS'} =~ /T/ ) { # standard format $iso = $FITS_headers->{'DATE-OBS'}; } elsif ( exists $FITS_headers->{UTSTART} ) { $iso = $FITS_headers->{'DATE-OBS'}. "T" . $FITS_headers->{UTSTART}; } elsif ( exists $FITS_headers->{UT} ) { $iso = $FITS_headers->{'DATE-OBS'}. "T" . $FITS_headers->{UT}; } $return = $self->_parse_iso_date( $iso ) if $iso; } return $return; } sub to_UTEND { my $self = shift; my $FITS_headers = shift; my $return; if ( exists $FITS_headers->{'DATE-END'} ) { $return = $self->_parse_iso_date( $FITS_headers->{'DATE-END'} ); } elsif (exists $FITS_headers->{'DATE-OBS'}) { my $iso; my $ut; if ( $FITS_headers->{'DATE-OBS'} =~ /T/ ) { $ut = $FITS_headers->{'DATE-OBS'}; $ut =~ s/T.*$//; } else { $ut = $FITS_headers->{'DATE-OBS'}; } if (exists $FITS_headers->{UTEND}) { $iso = $ut. "T" . $FITS_headers->{UTEND}; } $return = $self->_parse_iso_date( $iso ) if $iso; } return $return; } sub to_UTDATE { my $self = shift; my $FITS_headers = shift; return $self->get_UT_date( $FITS_headers ); } sub from_UTEND { my $self = shift; my $generic_headers = shift; my $utend = $generic_headers->{UTEND}->strptime( '%T' ); return ( "UTEND"=> $utend ); } sub from_UTSTART { my $self = shift; my $generic_headers = shift; my $utstart = $generic_headers->{UTSTART}->strptime('%T'); return ( "UTSTART"=> $utstart ); } sub from_UTDATE { my $self = shift; my $generic_headers = shift; my $ymd = $generic_headers->{UTDATE}; my $dobs = substr( $ymd, 0, 4 ) . "-" . substr( $ymd, 4, 2 ) ."-" . substr( $ymd, 6, 2 ); return ( "DATE-OBS"=>$dobs ); } # Supplementary methods for the translations # ------------------------------------------ # Returns the UT date in YYYYMMDD format. sub get_UT_date { my $self = shift; my $FITS_headers = shift; # This is UT start and time. my $dateobs = $FITS_headers->{"DATE-OBS"}; # Extract out the data in yyyymmdd format. return substr( $dateobs, 0, 4 ) . substr( $dateobs, 5, 2 ) . substr( $dateobs, 8, 2 ); }
1;