Difference between revisions of "The RIMO"
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! There are no detector-level products in the first release, | ! There are no detector-level products in the first release, | ||
| − | so there will be no detector-level parameters in the accompanying RIMO. | + | so there will be no detector-level parameters in the accompanying RIMO … … TBC. |
| + | This section is currently included for completeness | ||
|} | |} | ||
</center> | </center> | ||
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TFORM15 = 'D ' | TFORM15 = 'D ' | ||
TUNIT15 = 'Hz ' | TUNIT15 = 'Hz ' | ||
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== Map-level parameter data == | == Map-level parameter data == | ||
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The effective filter bandpasses are given in different BINTABLE extensions. The extension is named ''BANDPASS_{name}'', where ''name'' specified the detector or the map. In the case of the maps, the bandpasses are a weighted average of the bandpasses of the detectors that are used to build the map. For details see [[ref to 03d HFI_Spectral Band]]. The bandpasses are given as 4-column tables containing | The effective filter bandpasses are given in different BINTABLE extensions. The extension is named ''BANDPASS_{name}'', where ''name'' specified the detector or the map. In the case of the maps, the bandpasses are a weighted average of the bandpasses of the detectors that are used to build the map. For details see [[ref to 03d HFI_Spectral Band]]. The bandpasses are given as 4-column tables containing | ||
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END | END | ||
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== Detector noise spectra == | == Detector noise spectra == | ||
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! There are no detector-level products in the first release, | ! There are no detector-level products in the first release, | ||
| − | so there will be no detector noise spectra in the accompanying RIMO. | + | so there will be no detector noise spectra in the accompanying RIMO … … TBC. |
| + | |||
| + | This section is currently included for completeness | ||
|} | |} | ||
</center> | </center> | ||
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The noise power spectra are the result of the ''detnoise'' pipeline. | The noise power spectra are the result of the ''detnoise'' pipeline. | ||
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END | END | ||
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== Beam Window Functions == | == Beam Window Functions == | ||
Revision as of 10:57, 24 January 2013
Contents
Overview[edit]
The RIMO, or Reduced Instrument Model is a FITS file containing selected instrument characteristics that are needed by users who work with the released data products. It is described in detail in The HFI and LFI RIMO ICD (ref). There will be two RIMOs, one for each instrument, which will follow the same overall structure, but will differ in the details. The type of data in the RIMO can be:
- Parameter
- namely scalars to give properties such as a noise level or a representative beam FWHM
- Table
- to give, e.g., filter transmission profiles or noise power spectra
- Map
- namely 2-D "flat" maps, to give, e.g., the main beam shape
The different types of data are written into different BINTABLE extensions of the FITS file, and these are described below.
Detector-level parameter data[edit]
| There are no detector-level products in the first release,
so there will be no detector-level parameters in the accompanying RIMO … … TBC. This section is currently included for completeness |
|---|
The detector parameter data are given in the form of a table giving the parameter values for each detector. The table columns (whose names are in BOLD ITALICS) are:
- Bolometer name - DETECTOR
- These are the detector names. For HFI these will be of the form 217-3 for SWBs or 100-3b for PSBs, and for LFI they will have the form 27M or 18S. There are 52 HFI detectors and 22 LFI detectors.
- Focal plane geometry parameters - PHI_UV, THETA_UV, and PSI_UV
- These parameters give the geometry of the focal plane, or the positions of the detectors in the focal plane. The angles that give the rotation of the beam pattern from a fiducial orientation (forward beam direction (z-axis) pointing along the telescope line of sight, with y-axis aligned with the nominal scan direction) to their positions in the focal plane. The fiducial position is that given by the Star Tracker. All angles are in radians. These parameters are derived from observations of bright planets; see Detectors pointing & beam for details.
- Polarization parameters - PSI_POL, EPSILON
- These are the direction of maximum polarization, defined with the beam in the fiducial orientation described above, that is, before rotation onto the detector position, and the cross-polarization contamination (or leakage). These values are determined from ground-based measurements.
- Beam parameters - FWHM, ELLIPTICITY, POSANG
- These are the mean FWHM of the scanning beam (in arcmin, the beam ellipticity (no units), and the position angle of the beam major axis. The scanning beam is that recovered from the observation of bright planets; details in Detectors pointing & beam.
- Noise parameters - NET_TOT, NET_WHT, F_KNEE, ALPHA
- Two NETs are given: one determined from the total noise (rms of the noise timeline) and one determined from the white noise level of the noise spectrum. The F_KNEE and ALPHA parameters are the frequency where the 1/f noise component meets the white noise level, and the slope of the former. The NETs are in units of Kcmb or MJy/sr * sqrt(s). These values are determined from the signal timelines as described in TOI processing chapter.
In the HFI RIMO, this table includes entries for the RTS bolometers (143-8 and 545-3), which are approximate or 0.00 when not evaluated.
The basic structure of the BINTABLE extension is as follows:
;----------------------------------------------------------------------------- ; Detector parameters ;----------------------------------------------------------------------------- XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / array data type NAXIS = 2 / number of array dimensions NAXIS1 = 120 / length of dimension 1 NAXIS2 = 52 / length of dimension 2 PCOUNT = 0 / number of group parameters GCOUNT = 1 / number of groups TFIELDS = 15 / number of table fields EXTNAME = 'CHANNEL PARAMETERS' / extension name TTYPE1 = 'DETECTOR' TFORM1 = '8A ' TUNIT1 = 'n/a ' TTYPE2 = 'PHI_UV ' TFORM2 = 'D ' TUNIT2 = 'deg ' TTYPE3 = 'THETA_UV' TFORM3 = 'D ' TUNIT3 = 'deg ' TTYPE4 = 'PSI_UV ' TFORM4 = 'D ' TUNIT4 = 'deg ' TTYPE5 = 'PSI_POL ' TFORM5 = 'D ' TUNIT5 = 'deg ' TTYPE6 = 'EPSILON ' TFORM6 = 'D ' TUNIT6 = 'n/a ' TTYPE7 = 'FWHM ' TFORM7 = 'D ' TUNIT7 = 'arcmin ' TTYPE8 = 'ELLIPTICITY' TFORM8 = 'D ' TUNIT8 = 'n/a ' TTYPE9 = 'POSANG ' TFORM9 = 'D ' TUNIT9 = 'deg ' TTYPE10 = 'NET ' TFORM10 = 'D ' TUNIT10 = 'K*s^1/2 ' TTYPE11 = 'F_KNEE ' TFORM11 = 'D ' TUNIT11 = 'Hz ' TTYPE12 = 'ALPHA ' TFORM12 = 'D ' TUNIT12 = 'n/a ' TTYPE13 = 'F_MIN ' TFORM13 = 'D ' TUNIT13 = 'Hz ' TTYPE14 = 'F_MAX ' TFORM14 = 'D ' TUNIT14 = 'Hz ' TTYPE15 = 'F_SAMP ' TFORM15 = 'D ' TUNIT15 = 'Hz '
Map-level parameter data[edit]
The map-level data table contains the effective beam solid angle (total and out to different multiples of the beamFWHM) and noise information as follows:
- FREQUENCY
- a 3-digit string giving the reference frequency in GHz, i.e., of the form 044 or 217
- Omega_total
- total beam solid angle in armin^2
- Ometa_1fwhm
- beam solid angle out to 1FWHM in arcmin^2
- Omega_2fwhm
- beam solid angle out to 2FWHM in arcmin^2
- FWHM_eff
- FWHM of a Gaussian beam having the same (total) solid angle, in sr. This is the best value for source flux determination
- FWHM_gauss
- FWHM derived from best Gaussian fit to beam maps, in sr. This is the best value for source identification
- NOISE
- This is the typical noise/valid observation sample as derived from an appropriate combination of the NETs of the valid detectors used in the map.
For the Omega columns, the 'DISP' (for dispersion) column gives an estimate of the spatial variation as a function of position on the sky. This is the variation induced by combining the scanning beam determined from the planet observations with the scanning strategy, as described in Detectors pointing & beam.
The BINTABLE extension has the following structure
TABLE TO BE ADDED
Single detector and combined bandpasses[edit]
| There are no detector-level products in the first release,
so there will be no detector-level bandpasses in the accompanying RIMO, but only the combined bandpasses |
|---|
The effective filter bandpasses are given in different BINTABLE extensions. The extension is named BANDPASS_{name}, where name specified the detector or the map. In the case of the maps, the bandpasses are a weighted average of the bandpasses of the detectors that are used to build the map. For details see ref to 03d HFI_Spectral Band. The bandpasses are given as 4-column tables containing
- WAVENUMBER
- the wavenumber in cm-1, conversion to GHz is accomplished by multiplying by [mks].
- TRANSMISSION
- the transmission (normalized to 1 at the max for HFI and to have an integral of 1 for LFI)
- ERROR
- the statistical uncertainty for the Transmission spectra (not provided for LFI).
- FLAG
- a flag indicating if the data point is an independant frequency data point (nominally the case), or an FTS instrument line shape (ILS)-interpolated data point. The frequency data has been over-sampled by a factor of ~10 to assist in CO component separation efforts ref to 03d (HFI Spec Resp) and 03a (HFI CO).
The BINTABLE extension has the following structure
;----------------------------------------------------------------------------- ; Bandpasses (detector or combined) ;----------------------------------------------------------------------------- XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / array data type NAXIS = 2 / number of array dimensions NAXIS1 = 25 / length of dimension 1 NAXIS2 = 12315 / length of dimension 2 PCOUNT = 0 / number of group parameters GCOUNT = 1 / number of groups TFIELDS = 4 / number of table fields EXTNAME = 'BANDPASS_100-2A' / extension name TTYPE1 = 'WAVENUMBER' TFORM1 = 'D ' TUNIT1 = '1/cm ' TTYPE2 = 'TRANSMISSION' TFORM2 = 'D ' TUNIT2 = 'n/a ' TTYPE3 = 'UNCERTAINTY' TFORM3 = 'D ' TUNIT3 = 'n/a ' TTYPE4 = 'FLAG ' TFORM4 = 'L ' TUNIT4 = 'n/a ' COMMENT Spencer v3.02 injection END
Detector noise spectra[edit]
| There are no detector-level products in the first release,
so there will be no detector noise spectra in the accompanying RIMO … … TBC. This section is currently included for completeness |
|---|
The noise power spectra are the result of the detnoise pipeline.
- HFI
- these are the ring noise spectra averaged for rings NN to MM in order to give a representative spectrum. The spectra of all 50 valid bolometers are given in a single table.
- LFI
- TBW
The keyword F_NYQ gives the Nyquist frequency, and can be used together with the number of points in the spectrum to reconstruct the frequency scale. The BINTABLE has the following structure:
XTENSION= 'BINTABLE' /Written by IDL: Wed Aug 8 13:36:33 2012
BITPIX = 8 /
NAXIS = 2 /Binary table
NAXIS1 = 13631488 /Number of bytes per row
NAXIS2 = 1 /Number of rows
PCOUNT = 0 /Random parameter count
GCOUNT = 1 /Group count
TFIELDS = 52 /Number of columns
COMMENT
COMMENT *** End of mandatory fields ***
COMMENT
EXTNAME = 'NOISE_SPECTRA' /Extension name
DBPATH = '/data/dmc/MISS03/DATA/detnoise/' /
TAG = '_MeanSpectrum_deconv_byRing_p17_survey_3_v53' /
N_PTS = 65536 /
F_NYQ = 90.0000 /
UNITS = 'W/rt(Hz)' /
PROCVER = 'v53/DX9 ' / HFI Product version
COMMENT
COMMENT *** Column names ***
COMMENT
TTYPE1 = 'SPECTRUM_100_1A' /
TTYPE2 = 'SPECTRUM_100_1B' /
....
TTYPE52 = 'SPECTRUM_857_4' /
COMMENT
COMMENT *** Column formats ***
COMMENT
TFORM1 = '65536E ' /
TFORM2 = '65536E ' /
....
TFORM52 = '65536E ' /
END
Beam Window Functions[edit]
Beam window functions and associated error descriptions are given into a BINTABLE for each detection unit, where detection unit consists of an auto or a cross product of one or two frequency maps or detset maps used in the likelihood. Here they are:
- the 6 HFI frequency channels, producing 21 extensions
- 26 detsets, producing 351 extensions; the detsets used are, by frequency channel:
- 100_ds1, 100_ds2,
- 143_ds1, 143_ds2, 143_5, 143_6, 143_7,
- 217_ds1, 217_ds2, 217_1, 217_2, 217_3, 217_4,
- 353_ds1, 353_ds2, 353_1, 353_2, 353_7, 353_8,
- 545_1, 545_2, 545_4,
- 857_1, 857_2, 857_3, 857_4
Each extension contains:
- a NOMINAL column (mandatory) with the window function proper,
- a BIAS column (optional),
- a number of EIGEN_n vectors, (5 for Release 1) of error modes.
- a keyword NUMVECT (Integer) specified the number of eigenmode vectors, and
- keywords LMIN and LMAX which give the length of nominal vector
- keywords LMIN_EM and LMAX_EM that give the range of the valid samples of the eigenmode vectors. Here LMAX_EM is always less than or equal to LMAX, and the values between LMAX_EM+1 and LMAX is set to NaN
An example of the FITS header is (Preliminary - to be updated):
;----------------------------------------------------------------------------- ; EXTENSION 11: BEAM_143_DS1X143_5 ;----------------------------------------------------------------------------- XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / array data type NAXIS = 2 / number of array dimensions NAXIS1 = 24 / length of dimension 1 NAXIS2 = 4001 / length of dimension 2 PCOUNT = 0 / number of group parameters GCOUNT = 1 / number of groups TFIELDS = 6 / number of table fields TTYPE1 = 'NOMINAL ' TFORM1 = 'E ' TTYPE2 = 'EIGEN_0 ' TFORM2 = 'E ' TTYPE3 = 'EIGEN_1 ' TFORM3 = 'E ' TTYPE4 = 'EIGEN_2 ' TFORM4 = 'E ' TTYPE5 = 'EIGEN_3 ' TFORM5 = 'E ' TTYPE6 = 'EIGEN_4 ' TFORM6 = 'E ' EXTNAME = 'BEAM_143_DS1X143_5' / extension name NUMVECT = 5 / Number of eigenvectors END
Beam Correlation Matrix[edit]
Two of these matrices are given, one for the frequency channels (21x21) and one for the detsets (351x351). Each is a symmetric matrix with 1-valued diagonal, made of NBEAMS*NBEAMS blocks, each block being NMODES*NMODES in size. Each row- (and column-) block entry relates to the B(l) model whose name is indicated in ROW* keywords below, and the corresponding eigenmodes are stored in a HDU of the same name.
The header is of the form (Preliminary - to be updated)::
;-----------------------------------------------------------------------------
; EXTENSION 381: CORRBEAM_DET
;-----------------------------------------------------------------------------
XTENSION= 'IMAGE ' /
EXTNAME = 'CORRBEAM_DET' /
BITPIX = -32 / IEEE single precision floating point
NAXIS = 2 /
NAXIS1 = 1755 /
NAXIS2 = 1755 /
DATE = '2012-11-23' / Creation date (CCYY-MM-DD) of FITS header
…
NDETS = 26 / number of detector assemblies
NBEAMS = 351 / number of beams = NDETS*(NDETS+1)/2
NMODES = 5 / number of eigen modes for each beam B(l)
DATAMIN = -0.979880 / minimum value (should be >=-1)
DATAMAX = 1.00000 / maximum value (should be 1)
ROW1 = 'BEAM_100-DS1x100-DS1' / block #1 on row (or column)
ROW2 = 'BEAM_100-DS1x100-DS2' / block #2 on row (or column)
ROW3 = 'BEAM_100-DS1x143-DS1' / block #3 on row (or column)
...
ROW350 = 'BEAM_857-3x857-4' / block #350 on row (or column)
ROW351 = 'BEAM_857-4x857-4' / block #351 on row (or column)
END
reduced IMO
Flexible Image Transfer Specification
(Planck) High Frequency Instrument
(Planck) Low Frequency Instrument
Interface Control Document
Full-Width-at-Half-Maximum
To be confirmed
Noise Equivalent Temperature
random telegraphic signal
Instrument Line Shape
