Astro::Fluxes - Class for handling a collection of astronomical flux quantities.
use Astro::Fluxes;
$fluxes = new Astro::Fluxes( $flux1, $flux2, $color1 );
my $flux = $fluxes->flux( waveband => $waveband );
Class for handling a collection of astronomical flux quantities.
- new
- Create a new instance of an
"Astro::Fluxes" object.
$fluxes = new Astro::Fluxes( $flux1, $flux2, $color1 );
Any number of "Astro::Flux"
or "Astro::FluxColor" objects can be
passed as arguments.
- flux
- Returns the flux for a requested waveband.
my $flux = $fluxes->flux( waveband => 'J' );
Arguments are passed as key-value pairs. The sole mandatory
named argument is 'waveband'; its value can either be an
"Astro::WaveBand" object or a string
that can be used to create a new
"Astro::WaveBand" via its Filter
parameter.
Optional arguments are:
derived - Whether or not to return fluxes that have been derived
from colors. Defaults to false, so that derived fluxes will not
be returned.
datetime - whether we should return a flux from a specified object,
should be passed as a C<DateTime> object.
type - which type of flux to return. If this is not given this method
will default to 'mag'. If you supply a type that is not
'mag' or 'magnitudes' and are attempting to return a derived flux,
this method will return undef.
This method returns an
"Astro::Flux" object.
- color
- Returns the color for two requested wavebands.
my $color =
$fluxes->color( upper => new
Astro::WaveBand( Filter => 'H' ),
lower => new Astro::WaveBand( Filter => 'J' ) );
my $color =
$fluxes->color( upper => new
Astro::WaveBand( Filter => 'H' ),
lower => new Astro::WaveBand( Filter => 'J' ), datetime =>
new DateTime );
Arguments are passed as key-value pairs. The two mandatory
named arguments are 'upper' and 'lower', denoting the upper (longer
wavelength) and lower (shorter wavelength) wavebands for the color. The
value for either can be either an
"Astro::WaveBand" object or a string
that can be used to create a new
"Astro::WaveBand" object via its
Filter parameter.
The above example will return the first H-K color in the
Fluxes object. The optional datetime arguement allows you to return a
colour at a specific datetime stamp.
- pushfluxes
- Push "Astro::Flux" and
"Astro::FluxColor" object into the
"Astro::Fluxes" object,
$fluxes->pushfluxes( $flux1, $flux2, $color1 );
Any number of "Astro::Flux"
or "Astro::FluxColor" objects can be
passed as arguments.
- allfluxes
- Returns an array of all the
"Astro::Flux" objects contained in the
"Astro::Fluxes" object,
@fluxes_not_dervied = $fluxes->allfluxes();
@fluxes_including_dervied = $fluxes->allfluxes( 'derived' );
by default this will not return the derived fluxes, however
the method takes an optional arguement of 'derived', in which case it
will do.
- fluxesbywaveband
- Returns an hash of all the "Astro::Flux"
objects contained in the "Astro::Fluxes"
object,
@fluxes = $fluxes->fluxesbywaveband( waveband => 'J' );
- original_colors
- Returns an array of the original (not derived) colors contained in the
object
@colors = $fluxes->original_colors( );
- original_wavebands
- Returns an array of the original (not derived) filters contained in the
object
@wavebands = $fluxes->original_wavebands( );
@filters = $fluxes->original_wavebands( 'filters' );
optional arguement 'filters' returns an actual filter list
rather than a list of
"Astro::WaveBand" objects.
- merge
- Merges another "Astro::Fluxes" object
with this object
$fluxes1->merge( $fluxes2 );
- datestamp
- Applies a datestamp to all "Astro::Flux"
object with this object
$fluxes->datestamp( new DateTime );
$Id: Fluxes.pm,v 1.19 2005/11/15 23:50:32 bradc Exp $
Brad Cavanagh <b.cavanagh@jach.hawaii.edu>, Alasdair Allan
<aa@astro.ex.ac.uk>
Copyright (C) 2004 - 2005 Particle Physics and Astronomy Research Council. All
Rights Reserved.
This program is free software; you can redistribute it and/or
modify it under the same terms as Perl itself.