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package Astro::FITS::HdrTrans::SCUBA2; |
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=head1 NAME |
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Astro::FITS::HdrTrans::SCUBA2 - JCMT SCUBA-2 translations |
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=head1 DESCRIPTION |
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Converts information contained in SCUBA-2 FITS headers to and from |
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generic headers. See L<Astro::FITS::HdrTrans> for a list of generic |
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headers. |
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=cut |
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use 5.006; |
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use warnings; |
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use strict; |
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use Carp; |
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use base qw/ Astro::FITS::HdrTrans::JCMT /; |
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use vars qw/ $VERSION /; |
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$VERSION = "1.63"; |
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# For a constant mapping, there is no FITS header, just a generic |
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# header that is constant. |
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my %CONST_MAP = ( |
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BACKEND => 'SCUBA-2', |
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DATA_UNITS => 'pW', |
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); |
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# NULL mappings used to override base class implementations |
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my @NULL_MAP = (); |
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# Unit mapping implies that the value propogates directly |
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# to the output with only a keyword name change. |
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my %UNIT_MAP = ( |
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FILTER => "FILTER", |
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INSTRUMENT => "INSTRUME", |
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DR_GROUP => "DRGROUP", |
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OBSERVATION_TYPE => "OBS_TYPE", |
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UTDATE => "UTDATE", |
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TELESCOPE => "TELESCOP", |
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AMBIENT_TEMPERATURE => 'ATSTART', |
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); |
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# Values that are derived from the last subheader entry |
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my %ENDOBS_MAP = ( |
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AIRMASS_END => 'AMEND', |
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AZIMUTH_END => 'AZEND', |
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ELEVATION_END => 'ELEND', |
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); |
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# Create the translation methods |
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__PACKAGE__->_generate_lookup_methods( \%CONST_MAP, \%UNIT_MAP, \@NULL_MAP, \%ENDOBS_MAP ); |
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=head1 METHODS |
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=over 4 |
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=item B<this_instrument> |
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The name of the instrument required to match (case insensitively) |
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against the INSTRUME/INSTRUMENT keyword to allow this class to |
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translate the specified headers. Called by the default |
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C<can_translate> method. |
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$inst = $class->this_instrument(); |
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Returns "SCUBA-2". |
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=cut |
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sub this_instrument { |
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return "SCUBA-2"; |
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} |
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=back |
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=head1 COMPLEX CONVERSIONS |
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These methods are more complicated than a simple mapping. We have to |
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provide both from- and to-FITS conversions All these routines are |
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methods and the to_ routines all take a reference to a hash and return |
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the translated value (a many-to-one mapping) The from_ methods take a |
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reference to a generic hash and return a translated hash (sometimes |
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these are many-to-many) |
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=over 4 |
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=item B<to_OBSERVATION_MODE> |
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If Observation type is SCIENCE, return the sample mode, else |
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return the sample mode and observation type. For example, "STARE", |
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"SCAN", "SCAN_POINTING". |
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Do not currently take into account polarimeter or FTS. |
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=cut |
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sub to_OBSERVATION_MODE { |
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my $self = shift; |
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my $FITS_headers = shift; |
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my $return; |
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if ( exists( $FITS_headers->{'SAM_MODE'} ) && |
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exists( $FITS_headers->{'OBS_TYPE'} ) ) { |
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my $sam_mode = $FITS_headers->{'SAM_MODE'}; |
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$sam_mode =~ s/\s//g; |
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my $obs_type = $FITS_headers->{'OBS_TYPE'}; |
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$obs_type =~ s/\s//g; |
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$return = $sam_mode; |
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if ($obs_type !~ /science/i) { |
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if ($obs_type =~ /(setup)/i) { |
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$return = lc($1); |
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} else { |
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$return .= "_$obs_type"; |
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} |
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} |
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} |
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return $return; |
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} |
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=item B<to_SUBSYSTEM_IDKEY> |
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=cut |
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sub to_SUBSYSTEM_IDKEY { |
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my $self = shift; |
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my $FITS_headers = shift; |
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# Try the general headers first |
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my $general = $self->SUPER::to_SUBSYSTEM_IDKEY( $FITS_headers ); |
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return ( defined $general ? $general : "FILTER" ); |
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} |
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=item B<to_DR_RECIPE> |
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Fix up recipes that were incorrect in the early years of the |
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observing tool. |
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Converts SASSy survey data to use the SASSy recipe. |
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=cut |
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sub to_DR_RECIPE { |
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my $class = shift; |
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my $FITS_headers = shift; |
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my $dr = $FITS_headers->{RECIPE}; |
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my $survey = $FITS_headers->{SURVEY}; |
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if (defined $survey && $survey =~ /sassy/i) { |
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if ($dr !~ /sassy/i) { |
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$dr = "REDUCE_SASSY"; |
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} |
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} |
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return $dr; |
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} |
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=item B<to_POLARIMETER> |
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Determine if POL-2 is in the beam, based on the INBEAM header. |
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=cut |
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sub to_POLARIMETER { |
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my $class = shift; |
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my $FITS_headers = shift; |
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my $inbeam = $FITS_headers->{'INBEAM'}; |
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return 0 unless defined $inbeam; |
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return ($inbeam =~ /\bpol/i) ? 1 : 0; |
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} |
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=item B<from_POLARIMETER> |
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Attempt to recreate the INBEAM header. Since this also |
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depends on FTS-2, use the _reconstruct_INBEAM method. |
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=cut |
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sub from_POLARIMETER { |
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my $class = shift; |
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my $generic_headers = shift; |
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return $class->_reconstruct_INBEAM($generic_headers); |
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} |
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=item B<to_FOURIER_TRANSFORM_SPECTROMETER> |
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Determine if FTS-2 is in the beam, based on the INBEAM header. |
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=cut |
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sub to_FOURIER_TRANSFORM_SPECTROMETER { |
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my $class = shift; |
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my $FITS_headers = shift; |
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my $inbeam = $FITS_headers->{'INBEAM'}; |
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return 0 unless defined $inbeam; |
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return ($inbeam =~ /\bfts/i) ? 1 : 0; |
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} |
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=item B<from_FOURIER_TRANSFORM_SPECTROMETER> |
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213
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Attempt to recreate the INBEAM header. Since this also |
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depends on POL-2, use the _reconstruct_INBEAM method. |
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216
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=cut |
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218
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sub from_FOURIER_TRANSFORM_SPECTROMETER { |
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1
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1
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1
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my $class = shift; |
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2
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my $generic_headers = shift; |
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return $class->_reconstruct_INBEAM($generic_headers); |
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} |
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=item B<_reconstruct_INBEAM> |
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Since the INBEAM header becomes multiple generic headers, we need to look at |
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them all to reconstruct it. In order to work within the confines of the |
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Astro::FITS::HdrTrans::Base::translate_to_FITS method, we need to work |
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on a per-generic header basis. This internal method can then be used for |
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the "from_" method for each of these. It will end up returning the same |
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INBEAM header each time -- the versions generated from different generic |
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headers will overwrite eachother in the Base translate_to_FITS method |
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but that shouldn't be a problem. |
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Note that the INBEAM header may not be reconstructed exactly. For example |
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it will just include the short form "pol" even if it would originally have |
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included specific POL-2 components instead. |
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=cut |
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sub _reconstruct_INBEAM { |
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2
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my $class = shift; |
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3
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my $generic_headers = shift; |
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my @components; |
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push @components, 'fts2' if $generic_headers->{'FOURIER_TRANSFORM_SPECTROMETER'}; |
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push @components, 'pol' if $generic_headers->{'POLARIMETER'}; |
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5
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my $inbeam = undef; |
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$inbeam = join(' ', @components) if scalar @components; |
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return (INBEAM => $inbeam); |
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} |
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=back |
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262
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=head1 SEE ALSO |
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C<Astro::FITS::HdrTrans>, C<Astro::FITS::HdrTrans::Base> |
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=head1 AUTHOR |
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Tim Jenness E<lt>t.jenness@jach.hawaii.eduE<gt> |
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=head1 COPYRIGHT |
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Copyright (C) 2007-2009,2011,2013 Science & Technology Facilities Council. |
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Copyright (C) 2003-2005 Particle Physics and Astronomy Research Council. |
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All Rights Reserved. |
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This program is free software; you can redistribute it and/or modify it under |
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the terms of the GNU General Public License as published by the Free Software |
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Foundation; either Version 2 of the License, or (at your option) any later |
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version. |
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This program is distributed in the hope that it will be useful,but WITHOUT ANY |
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WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A |
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PARTICULAR PURPOSE. See the GNU General Public License for more details. |
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You should have received a copy of the GNU General Public License along with |
286
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this program; if not, write to the Free Software Foundation, Inc., 59 Temple |
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Place, Suite 330, Boston, MA 02111-1307, USA. |
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289
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=cut |
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291
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1; |