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- BRIGHT_POINT_SOURCE_NCOLOUR
- Reduces a multi-colour bright-point-source photometry observation.
- BRIGHT_POINT_SOURCE_NCOLOUR_APHOT
- Reduces a multi-colour bright-point-source photometry observation
and performs aperture photometry.
- BRIGHT_POINT_SOURCE_CATALOGUE
- Reduces a bright-point-source photometry observation, producing
a catalogue of all sources in the field.
- BRIGHT_POINT_SOURCE_TELE
- Reduces a bright-point-source photometry observation, using
telescope offsets for registration.
- BRIGHT_POINT_SOURCE_TELE_APHOT
- Reduces a bright-point-source photometry observation, using
telescope offsets for registration, and performs aperture photometry.
- DIFFERENCE_STATS
- Calculates statistics for Michelle darks in a pairwise manner.
- JITTER_SELF_FLAT_CATALOGUE
- Reduces a ``standard jitter'' photometry observation using
object masking, and produces a catalogue of all sources
in the field.
- JITTER_SELF_FLAT_NCOLOUR_APHOT
- Reduces a multi-colour ``standard jitter'' photometry observation
using object masking, and performs aperture photometry.
- LAMP_FLAT
- Creates and files imaging flat fields derived from a calibration
lamp for ISAAC and NACO.
- POL_QU_FIRST_NOD_CHOP
- Reduces a Michelle chopped and nodded polarimetry observation, where
waveplate angle iterates in pairs at each jitter position. Its purpose
is to form the Q,U Stokes parameters as quickly as possible,
hence offer more-accurate polarimetry than integrating at four waveplate
angles before nodding.
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Up: Release Notes V4.1
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ORAC-DR -- imaging data reduction
Starlink User Note 232
Malcolm J. Currie
Brad Cavanagh
Joint Astronomy Centre, Hilo, Hawaii
2004 June
E-mail:ussc@star.rl.ac.uk
Copyright © 2004 Particle Physics and Astronomy Research Council