'Highly Processed Data Products' (HPDP) are the result of further
processing beyond the pipeline and/or using new, refined algorithms.
Several projects have been undertaken by the ISO Data Centre, in
collaboration with the national instrument data centres, for systematic
data reduction of specific instrument modes, that produce homogeneous
sets of HPDP. They include processed IMAGES and SPECTRA, object
CATALOGS, and spectral and image ATLASES.
The list of Highly Processed Data Products currently available is given below.
To query and download these data, access the ISO Data Archive
here
Faint 6.7 micron sources in the high galactic latitude
field SSA13 are extracted by combining 16 CAM01
observations with the total observing time of 23 hours.
This atlas contains 12 micron images of a representative
sample of 75 Bright Spiral Galaxies chosen from the Revised
Shapley-Ames Catalog.
A Catalog with fluxes at 12 microns with different
apertures has been produced.
All CAM LW-CVF have been processed. Zodiacal light
subtraction and stray light from uniform illumination
correction are the main improvements. Final images are
corrected for distortion and in some cases an astrometric
correction is suggested.
CAM CVF spectra are extracted for 42 YSO candidates
identified in an imaging spectroscopy survey of Young
Stellar Objects in four low-mass star formation regions:
RCrA, rho Ophiuchi, Serpens and Chamaeleon I.
These 62 L03 reduced observations include subtraction of
dark currents and straylight; interactive shifting of the
miniscans; correction for FP side order contamination;
improved detector responsivity drift correction; extended
FP throughput calibration.
864 LWS L02 observations have been processed with an
automatic pipeline, including de-glitching and scan
averaging. New flags provide information and warnings
about the spectra.
All LWS L01 observations (1791) have been processed with
an automatic pipeline, including de-glitching,
de-fringing, correction for NIR-leak and SW1
double-peaked features and scan averaging. New flags
provide information and warnings about the spectra.
This catalogue consists of 4 manually reduced LWS
observations of asteroids and background
measurements. Special effort was put into the accurate
dark current substraction, responsivity calibration and
deglitching.
This catalogue consists of 53 manually reduced LWS
observations of asteroids and background
measurements. Special effort was put into the accurate
dark current substraction, responsivity calibration and
deglitching.
An Atlas of combined SWS+LWS spectra of 43 compact HII
regions in the Galaxy, including information on physical
parameters, line fluxes, chemical abundances and an
inventory of the dust and ice features detected.
LWS01 spectra of stars that are bright in the near IR can
show broad spectral features at ~53 and ~103 microns,
due to a near-infrared leak.
A template profile has been removed from the L01
observations known to be affected by this caveat.
This set of Highly Processed Data Products contains 41
science observations which have been reprocessed with an
upgraded version of the legacy pipeline OLP V10.1, fixing
processing problems.
This catalogue contains 124 ISOPHOT observations (184
measurements) of a sample of 63 galaxies later than S0
selected from the Virgo Cluster Catalogue of Bingelli,
Sandage, & Tamman. Galaxies were observed in P32 mode
with the C100/C200 detectors.
This catalogue contains 64 ISOPHOT observations of 64
extragalactic objects. They were observed in sparse map
mode with the C100 detector after revolution 95.
This catalogue contains 237 ISOPHOT observations
(259 measurements) of 179 compact objects. They
were observed in staring mode with the P1 detector
at 3.6 micrometer (and at other wavelengths).
This catalogue contains 32 ISOPHOT observations
of 31 compact objects. They were observed in
staring mode with the P1 detector at 3.6
micrometer (only).
This catalogue contains 77 ISOPHOT observations
(94 measurements) of 54 miscellaneous compact objects.
They were observed in nodding and scan mode with the
C100/C200 detectors.
This catalogue contains 399 ISOPHOT observations (772
measurements) of 353 compact objects. They were observed
in chopped mode with the C200 detectors after revolution 95
(these objects were observed with the C100 array as well).
This catalogue contains 155 ISOPHOT observations (168
measurements) of 11 compact solar-system objects (planets
or asteroids). They were observed in mini-map mode with the
C100/C200 detectors after revolution 95.
This catalogue contains 206 ISOPHOT observations (456
measurements) of 189 compact objects. They were observed
in chopped mode with the C200 detectors (only) after
revolution 95.
This catalogue contains 429 PHT observations (555
measurements). It includes all main-sequence stars
observed in mini-map mode with C100/C200 after revolution
95, and some giant stars from the ISOPHOT standard lists.
A few 1D-scans are also included.
This catalogue contains 48 ISOPHOT observations (49
measurements) of 48 miscellaneous far-infrared sources.
They were observed in mini-map mode with the C100/C200
detectors after revolution 95.
This catalogue contains 52 ISOPHOT observations (53
measurements) of 50 evolved stars or planetary nebulae.
They were observed in mini-map mode with the C100/C200
detectors after revolution 95.
This catalogue contains 579 ISOPHOT observations
(774 measurements) of 325 extragalactic objects.
They were observed in mini-map mode with the
C100/C200 detectors after revolution 95.
406 PHT40 observations have been reprocessed with an
upgraded version of OLPV10.1. A significant reduction in
the noise of the continuum is achieved using a bi-weight
mean deglitching algorithm. The resulting spectra are
smoother and closer to the models.
847 P22 mini-maps have been reprocessed with an upgraded
version of OLPV10.1. The same calib files were used, so
the photometry is expected to be identical. However, the
algorithm to derive the flux densities has now been
implemented in the pipeline code.
This atlas consists of PHT 2.5-12 micron spectra of
all normal galaxies in the IDA with a classified optical
morphology: 87 galaxies ranging from ellipticals to
spirals to dwarf irregulars. These are relatively nearby
galax. without strong interaction.
The full grating scan SWS01 data, reprocessed and
defringed. For the SWS01 speeds 3 and 4, the spectral
resolution is increased over the pipeline processing.
Browse products are derived. A catalogue is provided,
listing noise and average flux per AOTBAND.
An atlas of SWS spectra (2.36-4.1 microns) of ~300 stars
at resolution 1500-2000 aimed at extending the MK
spectral classification to the near infrared. The bulk
of the observations were performed during a dedicated
campaign after helium depletion.
This catalogue contains 66 observations of asteroids and
32 of planetary satellites made with the SWS spectrometer
in the wavelength range between 2.38um to 29.0um (SWS
bands 1A to 3E) in mode AOT06. Of these,65 were
reprocessed with up-to-date techniques
All valid SWS full-scan spectra, systematically processed
from the last stage of the pipeline software. Most of these
can be searched in a catalogue, including a spectral
classification system (Kraemer et al., 2002).
To see also ISO related catalogues in VizieR click
here
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