# Appendix C: TMG, TMC, and TMT Files¶

Note

This is currently not yet available for JWST.

stsynphot computes the combined throughput for an observing mode (obsmode) with the following steps:

1. The comma-separated obsmode is broken into individual keywords, each becoming a component of the obsmode.

2. The individual components or keywords are used to search the graph table, which has 6 columns, starting at the row with the lowest INNODE value. All rows with this INNODE are examined. The row whose keyword matches one of the keywords in the obsmode is selected. If no such row is found, the row with the keyword “default” is selected. If there is no such row and there is only one entry with the current INNODE, then this row is selected. Otherwise, an exception is raised.

3. Once the row is selected, the component name that is not “clear” is saved for its throughput lookup in a later step. “Clear” components are discarded because their throughput will not modify the combined throughput.

4. The OUTNODE of the selected row becomes the new INNODE, and the process of searching the graph continues until the OUTNODE is not found in the graph table. For example, see Figure 1.

5. Once all of the component names are found in the instrument graph table, the component lookup table (i.e., the TMC table), which has 4 columns, is searched for the actual names of the throughput tables, matching by the COMPNAME column. For example, see Figure 2.

6. Once the throughput values are read from the component throughput tables, they are resampled onto the specified wavelength set (if necessary) and multiplied together to form the combined throughput.

The thermback() method actually traverses the graph table twice; Once in the usual fashion, using the COMPNAME column; And once to obtain the optical train necessary for thermal calculations for IR detectors, using the THCOMPNAME column. These trains differ because of the existence of opaque but emissive components in the optical path, such as the spider that supports the HST secondary mirror.

The graph table is used to obtain the train of thermally emissive components in the same way it is used for optical components, except that:

• obsmode keywords are compared to the thermal component name (THCOMPNAME) instead of the usual COMPNAME.

• Once all of the component names are found in the graph table, the thermal component lookup table (i.e., the TMT table) is searched for the actual filenames of the emissivity tables. This file has the same format as the TMC file.

Further details and examples can be found in Diaz (2012).

This figure shows the path followed in the graph table (TMG) to gather the components that make the “acs,wfc2,f435w” observing mode. In this example, the keywords are mapped to the components “hst_ota”, “acs_wfc_im123”, “acs_f435w_wfc”, “acs_wfc_ebe_win12f”, and “acs_wfc_ccd1”.

This figure shows the component table (TMC) with the filenames of the components mentioned in Figure 1.

## Graph Table (TMG)¶

The instrument graph table has 6 columns, as follow:

Column Name

Description

Data Format

COMPNAME

Component name

String of 20 characters

KEYWORD

obsmode keyword

String of 12 characters

INNODE

Input node

Integer

OUTNODE

Output node

Integer

THCOMPNAME

Thermal component name

String of 20 characters

COMMENT 1

Comment (not used)

String of 68 characters

1(1,2)

The comment column is not used by stsynphot. It exists solely for documentation.

The COMPNAME column contains the name of the component. Each component must have a unique name, as it is used as primary key for Component Table (TMC, TMT) lookup. The THCOMPNAME column is similar to COMPNAME but for Thermal Emissivity Table.

The KEYWORD column is used to match the component keywords in the obsmode string (also see Appendix B: OBSMODE Keywords). The same component could be represented by multiple keywords; In that case, it will have multiple row entries, all of which are identical except for the keywords, in the graph table. The keyword values are not case-sensitive. The entry for a parameterized keyword should contain the keyword followed by a “#” at the end; For example, MJD# and aper# in Figure 3.

The INNODE and OUTNODE columns specify the light path through the HST. They are used in the process of searching the graph, as explained above. Node numbers in those columns should increase as one goes down the light path in the instrument.

Column         1               2           3          4               5
Label  _____COMPNAME_____ __KEYWORD___ __INNODE__ _OUTNODE__ _____THCOMPNAME_____
1791   clear              default      8224       8225       clear
1792   stis_os21          default      8225       8230       clear
1793   stis_ng21_mjd      MJD#         8230       8233       clear
1794   stis_ng21          default      8230       8233       clear
. . . .
2887   clear              default      10100      10101      clear
2888   acs_wfc_aper       aper#        10100      10101      clear
2889   acs_wfc_im123      default      10101      10130      clear
. . . .
3481   clear              g141         12750      12752      clear
3482   wfc3_ir_g102_bkg   bkg          12701      12800      wfc3_ir_g102_bkg
3483   wfc3_ir_g102_src   default      12701      12800      wfc3_ir_g102_src
3484   wfc3_ir_g102_bkg   bkg          12751      12800      wfc3_ir_g102_bkg

Figure 3: Example contents of a graph (TMG) table.

## Component Table (TMC, TMT)¶

TMC and TMT files are the master component and thermal component lookup tables, respectively. Both of them have the same 4 columns, as follow:

Column Name

Description

Data Format

TIME 2

Insertion time

String of 26 characters

COMPNAME

Component name

String of 18 characters

FILENAME

Throughput file name and column

String of 50 characters

COMMENT 1

Comment (not used)

String of 68 characters

2

The insertion time column is used by stsynphot. It contains the time that the component file was delivered. It is included for documentation and to simplify traceability of the data files. The time format is yyyymmdd:HHMMSS.

The COMPNAME column is used in TMC and TMT files to link from the Graph Table (TMG) using the latter’s COMPNAME and THCOMPNAME columns, respectively.

The FILENAME column provides the filename of the throughput table, which includes abbreviated path names, as defined in stsynphot.config.conf.irafshortcutfile. The table must be in binary FITS format. The entry for a parameterized component should contain its filename followed by square brackets containing the parameterized keyword; For example, cracscomp$acs_cor_aper_002_syn.fits[aper#] in Figure 4. For thermal component, the throughput file should contain thermal emissivity information (see Figure 5). The filenames are not stored directly in the graph table because the files themselves change more frequently than instrument light paths. Therefore, by doing this, we can avoid modifying the more complicated graph table every time a new version of a component throughput is delivered to CRDS. Column 1 2 3 Label _______TIME_________ ___COMPNAME____ ___________________FILENAME__________________ ____________________________COMMENT_____________________________ 7 oct 30 2013 15:44:42 acs_blocking3 cracscomp$acs_blocking3_001_syn.fits          throughput curve (all zeroes) for blocking3 filter
8    oct 30 2013 15:44:42  acs_blocking4   cracscomp$acs_blocking4_001_syn.fits throughput curve (all zeroes) for blocking3 filter 9 apr 03 2003 18:14:16 acs_cor_aper cracscomp$acs_cor_aper_002_syn.fits[aper#]    acs coronagraph encircled energy table
1   aug 14 2009 18:13:04  acs_f115lp       cracscomp$acs_f115lp_005_syn.fits updated files. setting throughput zero at end of curves 11 aug 14 2009 18:13:04 acs_f115lp_sbc cracscomp$acs_f115lp_sbc_004_syn.fits         updated files. setting throughput zero at end of curves
. . . . .
2313 oct 01 2013 19:55:56  stis_ng22       crstiscomp$stis_ng22_016_syn.fits default date 57113 & end date 57480. turned mjd extrapolation on 2314 oct 01 2013 19:55:56 stis_ng22_mjd crstiscomp$stis_ng22_mjd_016_syn.fits[mjd#]   default date 57113 & end date 57480. turned mjd extrapolation on
2315 oct 01 2013 19:55:56  stis_ng22b      crstiscomp$stis_ng22b_010_syn.fits default date 57113 & end date 57480. turned mjd extrapolation on 2316 oct 01 2013 19:55:56 stis_ng22b_mjd crstiscomp$stis_ng22b_mjd_010_syn.fits[mjd#]  default date 57113 & end date 57480. turned mjd extrapolation on
2317 oct 01 2013 19:55:56  stis_ng23       crstiscomp$stis_ng23_011_syn.fits default date 57113 & end date 57480. turned mjd extrapolation on 2318 oct 01 2013 19:55:56 stis_ng23_mjd crstiscomp$stis_ng23_mjd_011_syn.fits[mjd#]   default date 57113 & end date 57480. turned mjd extrapolation on
2319 oct 01 2013 19:55:56  stis_ng24       crstiscomp$stis_ng24_011_syn.fits default date 57113 & end date 57480. turned mjd extrapolation on 2320 oct 01 2013 19:55:56 stis_ng24_mjd crstiscomp$stis_ng24_mjd_011_syn.fits[mjd#]   default date 57113 & end date 57480. turned mjd extrapolation on
2321 oct 01 2013 19:55:56  stis_ng31       crstiscomp$stis_ng31_011_syn.fits default date 57113 & end date 57480. turned mjd extrapolation on  Figure 4: Example contents of a TMC table, taken from z4k1425fm_tmc.fits. Column 1 2 3 4 Label __________TIME____________ ___COMPNAME____ __________________FILENAME_________________ __________________COMMENT___________________ 116 aug 15 2006 8:00:00:000am wfc3_ir_fold crwfc3comp$wfc3_ir_fold_001_th.fits         Reflectivity of IR fold mirror
117  aug 15 2006 8:00:00:000am  wfc3_ir_mir1    crwfc3comp$wfc3_ir_mir1_001_th.fits Reflectivity of IR mirror 1 118 aug 15 2006 8:00:00:000am wfc3_ir_mir2 crwfc3comp$wfc3_ir_mir2_001_th.fits         Reflectivity of IR mirror 2
119  aug 15 2006 8:00:00:000am  wfc3_ir_rcp     crwfc3comp$wfc3_ir_rcp_001_th.fits Transmission of refractive corrector plate 120 aug 15 2006 8:00:00:000am wfc3_ir_wmring crwfc3comp$wfc3_ir_wmring_001_th.fits       WFC3 warm ring

Figure 5: Example contents of a TMT table, taken from tae17277m_tmt.fits.

## Throughput Table¶

The throughput table contains the component throughput as a function of wavelength (see FITS Table Format). It may also contain an optional column of estimated errors or uncertainties associated with the throughput values; The error column must have the following naming convention:

Wavelength Column Name

Throughput Column Name

Error Column Name

WAVELENGTH

THROUGHPUT

ERROR

<other> (Example: DN1)

<other>_ERR (Example: DN1_ERR)

<other>#<value> (Example: APER#0.1)

<other>_ERR#<value> (Example: APER_ERR#0.1)

Wavelength values must be in monotonically ascending or descending order. Wavelength unit must be specified for the column (see Wavelength Units for acceptable units). Throughput and error columns do not need units, but you may specify them as “transmission”, “qe”, “dn”, or “photon” (or any of their unique abbreviations) for documentation. Values in all columns must be 64-bit floating-point numbers. Figure 6 shows an example of a simple throughput table.

A component throughput may also be parameterized, meaning that the throughput is a function of some other variable besides wavelength. In this case, the table has multiple throughput columns, each named keyword#value. Examples of such tables are shown in Figure 7, Figure 8, and Figure 9. For more details, see Parameterized Keyword.

Column     1           2            3
Label  WAVELENGTH _THROUGHPUT_ ___ERROR____
1      1838.9     0.           INDEF
2      1839.0     1.           INDEF
3      1929.0     1.           INDEF
4      1929.1     0.           INDEF

Figure 6: Example contents of a simple throughput table.

Column     1            2             3             4             5             6
Label  WAVELENGTH FR647M#5366.0 FR647M#5586.8 FR647M#5807.6 FR647M#6028.4 FR647M#6249.2 ...
1      3500.0     0.            0.            0.            0.            0.            ...
2      3500.2     1.00000E-6    1.00000E-6    1.00000E-6    1.00000E-6    1.00000E-6    ...
3      4829.0     1.96935E-4    8.76876E-5    7.62487E-5    7.39577E-5    7.32903E-5    ...
4      4834.0     2.09608E-4    9.15258E-5    7.94214E-5    7.70256E-5    7.63329E-5    ...

Figure 7: Example contents of a throughput table parameterized for the ACS FR647M ramp filter.

Column       1               2               3               4               5               6
Label __WAVELENGTH___ __THROUGHPUT___ _____ERROR_____ __MJD#50586.0__ __MJD#50959.0__ __MJD#51287.0__
1     1099.           0.              0.              0.              0.              0.
2     1100.           0.9446287       0.              1.              1.011037        1.020443
3     1150.           0.9446287       0.              1.              1.011037        1.020443

Figure 8: Example contents of a throughput table parameterized for MJD to characterize time-dependent change in STIS sensitivity.

Column     1          2          3          4          5          6
Label  WAVELENGTH _APER#0.__ _APER#0.1_ _APER#0.2_ _APER#0.3_ _APER#0.4_
1      3500.      0.28       0.67       0.84       0.88       0.89           ...
2      4000.      0.22       0.68       0.85       0.88       0.9            ...
3      5000.      0.21       0.7        0.86       0.9        0.92           ...
4      6000.      0.22       0.69       0.85       0.9        0.92           ...

Figure 9: Example contents of a throughput table parameterized for encircled energy in ACS/WFC detector.

## Thermal Emissivity Table¶

The thermal emissivity table contains the component emissivity as a function of wavelength. This is only relevant for IR instruments with non-negligible thermal background. It is similar to throughput table, except that it has the following columns:

• WAVELENGTH

• EMISSIVITY

• ERROR (optional)

Unlike the throughput table, the keyword# parameterization syntax is overridden for use with the thermal emissivity tables. Instead, this syntax is used to specify a component temperature, overriding the default temperature present in the DEFT header keyword (see below).

In addition, it must also contain the following keywords in its table (Extension 1) header:

• BEAMFILL, which specifies the fraction of the optical beam filled by this component. This value is usually 1, but it depends on the precise optical layout of the instrument.

• DEFT, which specifies the default temperature (in Kelvin) of the component. This is the temperature that will be used in thermal calculations unless it is overridden in the obsmode.

• THTYPE, which specifies the type of thermal component that is described by this file:

• “opaque” component is the type that partially obstructs the beam. It emits radiation, but does not pass it.

• “thru” component is the type that has both throughput and emissivity. This is the case for most optical elements.

• “numeric” component is the type that does not correspond to a physical device in the instrument, but is represented as such for convenience. For instance, the detector quantum efficiency.

• “clear” component is the type that does not contribute to either throughput or emissivity. It is commonly used as a placeholder in the graph table to organize the flow.

• THCOMPNAME and THMODE are the associated pair of values used when traversing the graph table. THMODE contains the obsmode keyword which points to the associated THCOMPNAME.

The example below displays the header keywords mentioned above:

>>> import os
>>> from astropy.io import fits
>>> filename = os.path.join(
...     os.environ['PYSYN_CDBS'], 'comp', 'nicmos',
...     'nic2_f110w_002_th.fits')
>>> with fits.open(filename) as pf:
...
BEAMFILL=                   1. / Fraction of beam filled by this component
DEFT    =                 77.1 / Default temperature in kelvins
THTYPE  = 'THRU    '           / Thermal type (opaque/thru/numeric/clear)
THCMPNAM= 'nic2_f110w'         / Name of thermal component
THMODE  = 'f110w   '           / Keyword in obsmode to specify temperature
...


## Parameterized Keyword¶

Parameterized keywords are used to access throughput tables for which the throughput is a function of some other variables in addition to wavelength. The syntax for a parameterized keyword is keyword#value, where value is a numeric (integer or float) value for the keyword to take. The hash sign # indicates to stsynphot that a parameterized keyword is being used.

A parameterized throughput table contains several throughput columns, each for a specified value of the parameterized component. When an arbitrary value is given, stsynphot will linearly interpolate the throughput values between the two closest keyword values; This is done using interpolate_spectral_element(). If the table’s primary (Extension 0) header contains PARAMS=WAVELENGTH, wavelength shift will be done before the interpolation.

Extrapolation is only allowed if the table’s primary header contains an EXTRAP keyword and it is set to True. Otherwise, the default THROUGHPUT column will be used (if available) or an exception will be raised.

The parameterized keywords are also defined in both the TMG and TMC files. For TMG, the KEYWORD value will be followed by a “#”; For example, in Figure 3, “MJD#” indicates that the parameterization is time dependent, while “aper#” indicates there is a variation in the encircled energy with aperture size. For TMC, the FILENAME value will be followed by a “[keyword#]”; For example, in Figure 4, the “cracscomp\$acs_cor_aper_002_syn.fits” file is parameterized by aperture size.

The ACS ramp filter is an example of a parameterized component. The throughput of the ramp filter varies as a function of position (wavelength) on the filter. Therefore, its throughput table contains several throughput columns, each evaluated at a different central wavelength. Figure 7 shows part of the throughput table for ACS FR647M ramp filter, where the first throughput column is for 5366 Angstrom, the second for 5586.8 Angstrom, and so forth. In this case, a request for 5400 Angstrom will result in interpolation between the first two columns.

Another example is the STIS time-dependent change in sensitivity, as illustrated in Figure 8. In this case, when “mjd#value” is given as part of an obsmode, the parameterized column(s) will be used and interpolated, as needed. If “mjd#value” is not given, then the default THROUGHPUT column is used.

Similarly, parameterization of encircled energy via aperture size is shown in Figure 9 for ACS/WFC detector. In this case, the throughput table is only used when “aper#value” is given in the obsmode, therefore, a default THROUGHPUT column is unnecessary.

All available parameterized keywords are listed in Appendix B: OBSMODE Keywords as keyword# or keyword#value.