Two files give the data for the low-resolution spectra (LRS) which, as described in Chapter IX, consist of two bands (8-13 um and 11-22 µm). The first file on the tape consists of a single 80-character ASCII record giving the date and version of the LRS data. The next file lists only the wavelengths corresponding to each sample of the spectra (Table X.E.1a). The last file contains the spectra and associated header information (Table X.E.1b). The spectra are in order of increasing right ascension. Both files have 80-character ASCII logical records and 256 logical records per physical record. An atlas of the spectra will be published as an Astronomy and Astrophysics Supplement.
E.1 Catalog Header File
Distance from Slit. ANGLE(100)
As described in detail in Chapter IX, each sample in the spectrum corresponds to a certain in-scan distance of the source from the centerline of the spectrometer entrance aperture. ANGLE lists these angular distances.
Wavelength Calibration.: LAMBDA1, LAMBDA2
There is a non-linear relation between the displacement of the source from the centerline of the spectrometer and the sampled wavelength. The wavelengths corresponding to each sample (or ANGLE) are given in (LAMBDA1 and LAMBDA2 for the two wavelength bands. The beginning and end of each spectrum contain measurements that lie outside of the wavelength coverage of the instrument but which can be used for electronic baseline determination. The wavelength values corresponding to these values of sample number (or ANGLE) are set to 0.
E.2 Spectra Records
The items starting at bytes 0 through 25 are identical to the items with the same names in the point source catalog (see Section X.B.1). This is also the case for the items starting at bytes 71, 73, 75 and 960.
Number of Spectra: NSPECTRA, NACCEPT
NSPECTRA is the number of spectra of this source observed; NACCEPT are the numbers of 8-13 µm and the 11-22 µm spectrum halves ultimately averaged to make the entry in the catalog.
Characterization of the Spectrum.: LRSCHAR
A description of the method of characterization is given in Section IX.D. Table X.E.2 lists the spectral classes used to characterize the spectrum.
Quality of the Spectrum Halves:. SPQUAL
Depending on the signal-to-noise ratio of the 8-13 µm and 11-22 µm halves of the spectra, the number of accepted spectra halves and the difference in level of the baselines on either side of the spectrum halves, a quality digit is assigned to each half of the spectrum; 1 indicates good quality, 2 moderate quality, and 3 barely acceptable.
X-38
Scale factor For All Spectrum Flux Densities: SCALE
Multiplying the integers BASELINE, NOISE, and SPECTRUM by the factor SCALE converts the values into units of W m-2 µm-1.
Baseline of Spectrum Halves: BASELINE
These four values give the average value of samples 1 through 20 (short wavelength end) and 81 through 100 (long wavelength end) of both the 8-13 µm and the 11-22 µm halves of the spectrum.
RMS Noise: NOISE
Using the twenty samples on the long wavelength end used for BASELINE, the rms noise per spectrum half is determined.
Signal-to-Noise Ratio: SNR
The average value of the samples in the wavelength ranges 8-13 µm and 11-22 µm, respectively, are divided by the NOISE values determined.
Baseline Asymmetry: ASYMM
This value indicates by what fraction of the average signal the baselines on the short and long wavelength sides of the spectrum halves differ. A large baseline asymmetry indicates that a confusing source may have contaminated the spectrum. The baseline asymmetry is usually large near the Galactic plane.
LRS/Survey Flux Ratio:. SRATIO
The ratio of the integrated flux (after convolution of the spectrum flux densities with the 12 µm band pass of the survey instrument) in the spectrum and the 12 µm survey flux is given in this item. Normally this value should be close to unity (Section IX.C). As the 11-22 µm part of the LRS spectrum hardly overlaps with the 25 µm survey band, a ratio of LRS/survey for this band is not significant.
The Spectrum: SPECTRUM
The integer values of the spectrum must be multiplied by SCALE for conversion to m-2 µm-1. The wavelengths corresponding to the 100 samples given for the 8-13 µm and the 11-22 µm halves of the spectrum are given in the catalog header file. Values for non-significant wavelengths are set to zero. For baseline interpolation, either the sample numbers or the ANGLE (distance in arcmin from the spectrometer center line) can be used.
X-39
Table X.E.1a Header Information for Catalog of Spectra
Start
Byte Name Description Units Format
0 ANGLE Angle from center of arc min 100F8.4
slit (one number per
sample)
800 LAMBDA1 Wavelength in 8-13 µm µm 100F8.4
corresponding to each
sample
1600 LAMBDA2 Wavelength in 11-22 µm µm 100F8.4
corresponding to each
sample
X-40
Table X.E.1b. Format of Spectra in Catalog
Start
Byte Name Description Units Format
0 NAME Source name --- 11A1
11 HOURS RA 1950 hrs I2
13 MINUTE RA 1950 min I2
15 SECOND RA 1950 deci-sec I3
18 DSIGN Declination sign ± A1
19 DECDEG DEC 1950 arc deg I2
21 DECMIN DEC 1950 arc min I2
23 DECSEC DEC 1950 arc sec I2
25 FLUX Averaged non-color Jy 4E9.3
corrected flux
densities (1 value per
band)
61 NSPECTRA No. of observed spectra --- I2
63 NACCEPT No. of accepted spectrum --- 2I2
halves
67 LRSCHAR Characterization of --- 2I1
spectrum
69 SPQUAL Quality of 8-13 µm and --- 2I1
11-22 µm parts of
spectra
71 VAR Percent of variability --- I2
likelihood (from catalog)
73 NID No. of associations --- I2
(<25)
75 IDTYPE Type of association --- I1
76 SPARE 4 spare bytes --- 4A1
(---------------new record--------------)
80 BASELINE Average of outer 20 scaled by SCALE 4I4
samples of spectra.
Short and long wavelength
end for each spectrum half
96 NOISE RMS noise per sample scaled by SCALE 2I4
(one value per spectrum half)
104 SNR Signal-to-noise ratio --- 2E10.3
(average signal in
spectrum part divided
by noise, one value per
spectrum half)
X-41
Table X.E.1b Format of Spectra in Catalog (Continued)
Start
Byte Name Description Units Format
124 ASYMM Relative baseline --- 2E10.3
asymmetry (difference ---
of left and right
baselines divided by
average signal. one value
per band)
144 SRATIO Ratio of integrated LRS --- F5.2
flux to 12 µm survey
flux
149 SCALE Scale factor for all W m-2 µm-1 E11.5
flux densities
(---------------new record---------------)
160 SPECTRUM 100 samples for each scaled by SCALE 200I4
of the two bands
(8-13 µm, 11-22 µm),
scaled by SCALE
(---------------new record--------------)
960 ID#1 Association field from --- 40A1
main catalog (see
Section X.B.1)
1000 ID#2 additional records
as required.