line |
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time |
code |
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=head1 NAME |
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Astro::FITS::HdrTrans::NIRI - Gemini NIRI translations |
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6
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=head1 SYNOPSIS |
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8
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use Astro::FITS::HdrTrans::NIRI; |
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10
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%gen = Astro::FITS::HdrTrans::NIRI->translate_from_FITS( %hdr ); |
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12
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=head1 DESCRIPTION |
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14
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This class provides a generic set of translations that are specific to |
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NIRI on the Gemini Observatory. |
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17
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=cut |
18
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19
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use 5.006; |
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10
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10
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4744113
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use warnings; |
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43
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21
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use strict; |
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10
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274
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10
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10
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use Carp; |
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16
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10
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185
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23
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10
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10
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39
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10
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21
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10
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653
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# Inherit from GEMINI |
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use base qw/ Astro::FITS::HdrTrans::GEMINI /; |
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10
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10
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59
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10
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23
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10
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1311
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27
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use vars qw/ $VERSION /; |
28
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10
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10
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52
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10
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18
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10
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5461
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29
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$VERSION = "1.65"; |
30
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31
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# for a constant mapping, there is no FITS header, just a generic |
32
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# header that is constant |
33
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my %CONST_MAP = ( |
34
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GAIN => 12.3, # hardwire for now |
35
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OBSERVATION_MODE => 'imaging', |
36
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SPEED_GAIN => "NA", |
37
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STANDARD => 0, # hardwire for now as all objects not a standard. |
38
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WAVEPLATE_ANGLE => 0, # hardwire for now |
39
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); |
40
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41
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# NULL mappings used to override base class implementations |
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my @NULL_MAP = qw/ /; |
43
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44
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# unit mapping implies that the value propogates directly |
45
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# to the output with only a keyword name change |
46
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47
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my %UNIT_MAP = ( |
48
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DETECTOR_READ_TYPE => "MODE", |
49
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); |
50
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51
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52
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# Create the translation methods |
53
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__PACKAGE__->_generate_lookup_methods( \%CONST_MAP, \%UNIT_MAP, \@NULL_MAP ); |
54
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55
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=head1 METHODS |
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57
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=over 4 |
58
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59
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=item B<this_instrument> |
60
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61
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The name of the instrument required to match (case insensitively) |
62
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against the INSTRUME/INSTRUMENT keyword to allow this class to |
63
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translate the specified headers. Called by the default |
64
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C<can_translate> method. |
65
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66
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$inst = $class->this_instrument(); |
67
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68
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Returns "NIRI". |
69
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70
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=cut |
71
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72
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return qr/^NIRI/; |
73
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} |
74
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20
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20
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1
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78
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75
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=back |
76
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77
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=head1 COMPLEX CONVERSIONS |
78
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79
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=over 4 |
80
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81
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=cut |
82
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83
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my $self = shift; |
84
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my $FITS_headers = shift; |
85
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my $et = $FITS_headers->{EXPTIME}; |
86
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0
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0
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0
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my $co = $FITS_headers->{COADDS}; |
87
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0
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return $et *= $co; |
88
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0
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} |
89
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0
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90
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0
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my $self = shift; |
91
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my $FITS_headers = shift; |
92
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my $obsnum = 0; |
93
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if ( exists ( $FITS_headers->{FRMNAME} ) ) { |
94
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0
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0
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0
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my $fname = $FITS_headers->{FRMNAME}; |
95
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0
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$obsnum = substr( $fname, index( $fname, ":" ) - 4, 4 ); |
96
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0
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} |
97
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0
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0
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return $obsnum; |
98
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0
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} |
99
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0
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100
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=item B<to_ROTATION> |
101
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0
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102
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Converts a linear transformation CD matrix into a single rotation angle. |
103
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This angle is measured counter-clockwise from the positive x-axis. |
104
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It uses the SLALIB routine slaDcmpf obtain the rotation angle without |
105
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assuming perpendicular axes. |
106
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107
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This routine also copes with errors in the matrix that can generate angles |
108
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+/-90 degrees instead of near 0 that they should be. |
109
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110
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=cut |
111
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112
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my $self = shift; |
113
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my $FITS_headers = shift; |
114
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my $rotation = 0.0; |
115
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if ( exists( $FITS_headers->{CD1_1} ) ) { |
116
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117
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0
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0
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1
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# Access the CD matrix. |
118
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0
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my $cd11 = $FITS_headers->{"CD1_1"}; |
119
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0
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my $cd12 = $FITS_headers->{"CD1_2"}; |
120
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0
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0
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my $cd21 = $FITS_headers->{"CD2_1"}; |
121
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my $cd22 = $FITS_headers->{"CD2_2"}; |
122
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123
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0
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# Determine the orientation using PAL routine. This has the |
124
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0
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# advantage of not assuming perpendicular axes (i.e. allows for |
125
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0
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# shear). |
126
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0
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my ( $xz, $yz, $xs, $ys, $perp ); |
127
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my @coeffs = ( 0.0, $cd11, $cd21, 0.0, $cd12, $cd22 ); |
128
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eval { |
129
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require Astro::PAL; |
130
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( $xz, $yz, $xs, $ys, $perp, $rotation ) = Astro::PAL::palDcmpf( \@coeffs ); |
131
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0
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|
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}; |
132
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0
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if (!defined $perp) { |
133
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0
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croak "NIRI translations require Astro::PAL"; |
134
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0
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} |
135
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0
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136
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|
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# Convert from radians to degrees. |
137
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0
|
0
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my $rtod = 45 / atan2( 1, 1 ); |
138
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0
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$rotation *= $rtod; |
139
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140
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# The actual WCS matrix has errors and sometimes the angle which |
141
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# should be near 0 degrees, can be out by 90 degrees. So for this |
142
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0
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# case we hardwire the main rotation and merely apply the small |
143
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0
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# deviation from the cardinal orientations. |
144
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if ( abs( abs( $rotation ) - 90 ) < 2 ) { |
145
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my $delta_rho = 0.0; |
146
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147
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$delta_rho = $rotation - ( 90 * int( $rotation / 90 ) ); |
148
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$delta_rho -= 90 if ( $delta_rho > 45 ); |
149
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0
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0
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$delta_rho += 90 if ( $delta_rho < -45 ); |
150
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0
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151
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# Setting to near 180 is a fudge because the CD matrix appears is wrong |
152
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0
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# occasionally by 90 degrees, judging by the telescope offsets, CTYPEn, and |
153
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0
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0
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# the support astronomer. |
154
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0
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0
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$rotation = 180.0 + $delta_rho; |
155
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} |
156
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157
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} |
158
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return $rotation; |
159
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0
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} |
160
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161
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# Shift the bounds to GRID co-ordinates. |
162
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my $self = shift; |
163
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0
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my $FITS_headers = shift; |
164
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my $bound = 1; |
165
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if ( exists( $FITS_headers->{LOWCOL} ) ) { |
166
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$bound = $self->nint( $FITS_headers->{LOWCOL} + 1 ); |
167
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} |
168
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0
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0
|
0
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return $bound; |
169
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0
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} |
170
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0
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|
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|
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|
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171
|
0
|
0
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my $self = shift; |
172
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0
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my $FITS_headers = shift; |
173
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my $bound = 1; |
174
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0
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if ( exists( $FITS_headers->{LOWROW} ) ) { |
175
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$bound = $self->nint( $FITS_headers->{LOWROW} + 1 ); |
176
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} |
177
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return $bound; |
178
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0
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0
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0
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|
} |
179
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0
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|
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|
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180
|
0
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|
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my $self = shift; |
181
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0
|
0
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|
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my $FITS_headers = shift; |
182
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0
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my $bound = 1024; |
183
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if ( exists( $FITS_headers->{HICOL} ) ) { |
184
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0
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$bound = $self->nint( $FITS_headers->{HICOL} + 1 ); |
185
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} |
186
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return $bound; |
187
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|
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|
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} |
188
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0
|
|
|
0
|
0
|
|
|
189
|
0
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|
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|
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|
my $self = shift; |
190
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0
|
|
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|
my $FITS_headers = shift; |
191
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0
|
0
|
|
|
|
|
my $bound = 1024; |
192
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0
|
|
|
|
|
|
if ( exists( $FITS_headers->{HIROW} ) ) { |
193
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|
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|
$bound = $self->nint( $FITS_headers->{HIROW} + 1 ); |
194
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0
|
|
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|
|
|
} |
195
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|
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|
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|
return $bound; |
196
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|
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|
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|
} |
197
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|
198
|
0
|
|
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0
|
0
|
|
|
199
|
0
|
|
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|
=back |
200
|
0
|
|
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|
|
|
|
201
|
0
|
0
|
|
|
|
|
=head1 SEE ALSO |
202
|
0
|
|
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203
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|
C<Astro::FITS::HdrTrans>, C<Astro::FITS::HdrTrans::UKIRT>. |
204
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0
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205
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=head1 AUTHOR |
206
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207
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|
Malcolm J. Currie E<lt>mjc@star.rl.ac.ukE<gt> |
208
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Paul Hirst E<lt>p.hirst@jach.hawaii.eduE<gt>, |
209
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|
Tim Jenness E<lt>t.jenness@jach.hawaii.eduE<gt>. |
210
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211
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=head1 COPYRIGHT |
212
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213
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Copyright (C) 2008 Science and Technology Facilities Council |
214
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Copyright (C) 1998-2005 Particle Physics and Astronomy Research Council. |
215
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All Rights Reserved. |
216
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217
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This program is free software; you can redistribute it and/or modify it under |
218
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the terms of the GNU General Public License as published by the Free Software |
219
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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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222
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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 |
224
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PARTICULAR PURPOSE. See the GNU General Public License for more details. |
225
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226
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You should have received a copy of the GNU General Public License along with |
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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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=cut |
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232
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1; |