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1   package nom.tam.fits.header;
2   
3   /*
4    * #%L
5    * nom.tam FITS library
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7    * Copyright (C) 1996 - 2024 nom-tam-fits
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32   */
33  
34  /**
35   * <p>
36   * This data dictionary contains FITS keywords that have been widely used within the astronomical community. It is
37   * recommended that these keywords only be used as defined here. These are the Keywords that describe the instrument
38   * that took the data.
39   * </p>
40   * <p>
41   * See <a href=
42   * "http://heasarc.gsfc.nasa.gov/docs/fcg/common_dict.html">http://heasarc.gsfc.nasa.gov/docs/fcg/common_dict.html</a>
43   * </p>
44   *
45   * @author Richard van Nieuwenhoven
46   */
47  public enum InstrumentDescription implements IFitsHeader {
48      /**
49       * The value field shall contain a character string which gives the name of the instrumental aperture though which
50       * the observation was made. This keyword is typically used in instruments which have a selection of apertures which
51       * restrict the field of view of the detector.
52       */
53      APERTURE(SOURCE.UNKNOWN, HDU.ANY, VALUE.STRING, "name of field of view aperture"),
54      /**
55       * The value field shall contain a character string which identifies the configuration or mode of the pre-processing
56       * software that operated on the raw instrumental data to generate the data that is recorded in the FITS file.
57       * Example: some X-ray satellite data may be recorded in 'BRIGHT', 'FAINT', or 'FAST' data mode.
58       */
59      DATAMODE(SOURCE.HEASARC, HDU.ANY, VALUE.STRING, "pre-processor data mode"),
60      /**
61       * The value field shall contain a character string giving the name of the detector within the instrument that was
62       * used to make the observation. Example: 'CCD1'
63       */
64      DETNAM(SOURCE.HEASARC, HDU.ANY, VALUE.STRING, "name of the detector used to make the observation"),
65      /**
66       * The value field shall contain a character string which gives the name of the filter that was used during the
67       * observation to select or modify the radiation that was transmitted to the detector. More than 1 filter may be
68       * listed by using the FILTERn indexed keyword. The value 'none' or 'NONE' indicates that no filter was used.
69       */
70      FILTER(SOURCE.HEASARC, HDU.ANY, VALUE.STRING, "name of filter used during the observation"),
71      /**
72       * The value field of this indexed keyword shall contain a character string which gives the name of one of multiple
73       * filters that were used during the observation to select or modify the radiation that was transmitted to the
74       * detector. The value 'none' or 'NONE' indicates that no filter was used.
75       */
76      FILTERn(SOURCE.HEASARC, HDU.ANY, VALUE.STRING, "name of filters used during the observation"),
77      /**
78       * The value field shall contain a character string which gives the name of the defraction grating that was used
79       * during the observation. More than 1 grating may be listed by using the GRATINGn indexed keyword. The value 'none'
80       * or 'NONE' indicates that no grating was used.
81       */
82      GRATING(SOURCE.HEASARC, HDU.ANY, VALUE.STRING, "name of the grating used during the observation."),
83      /**
84       * The value field of this indexed keyword shall contain a character string which gives the name of one of multiple
85       * defraction gratings that were used during the observation. The value 'none' or 'NONE' indicates that no grating
86       * was used.
87       */
88      GRATINGn(SOURCE.HEASARC, HDU.ANY, VALUE.STRING, "name of gratings used during the observation."),
89      /**
90       * The value field shall contain a character string which gives the observing mode of the observation. This is used
91       * in cases where the instrument or detector can be configured to operate in different modes which significantly
92       * affect the resulting data. Examples: 'SLEW', 'RASTER', or 'POINTING'
93       */
94      OBS_MODE(SOURCE.HEASARC, HDU.ANY, VALUE.STRING, "instrumental mode of the observation"),
95      /**
96       * The value field shall contain an integer giving the data value at which the detector becomes saturated. This
97       * keyword value may differ from the maximum value implied by the BITPIX in that more bits may be allocated in the
98       * FITS pixel values than the detector can accommodate.
99       */
100     SATURATE(SOURCE.STScI, HDU.ANY, VALUE.INTEGER, "data value at which saturation occurs");
101 
102     private final FitsKey key;
103 
104     InstrumentDescription(IFitsHeader.SOURCE status, HDU hdu, VALUE valueType, String comment) {
105         key = new FitsKey(name(), status, hdu, valueType, comment);
106     }
107 
108     @Override
109     public final FitsKey impl() {
110         return key;
111     }
112 }