at specific temperatures, ranging from 5000 K and 65,000 K, and up to 10 MK during solar flares. IRIS is a sub-full-disk instrument, imaging portions of the solar disk and limb.

The timing and pointing of IRIS observation studies that were run during the start and end times of a given GOES event were obtained using the routine. This searches the Heliophysics Coverage Registry for the [^12] corresponding to the time of the flare, as shown by the horizontal purple line in the upper-left panel for Figure \[sff\_plot\]. Similar to the previously mentioned instruments with limited fields of view, the pointing information obtained from the was cross-referenced with the flare location to determine if IRIS was pointed at the required location (purple box overlaid on the EUV image in Figure \[sff\_plot\]).

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  ------------------- ------------ ---------- --------- ------------ ----------------
  Instrument/                                                          Success Rate
  Database              C-class     M-class    X-class     Total      Over 6.5 Years
  NOAA/GOES               7360        685        45         8090           100%
  SSW Latest Events       6339        581        33         6953           86%
  RHESSI                  3673        370        23         4066           58%
  SDO/EVE MEGS-A          3825        343        19         4187           100%
  SDO/EVE MEGS-B          787          97         8         892            12%
  *Hinode*/EIS            496          54         6         556             8%
  *Hinode*/SOT            1167        177        15         1359           20%
  *Hinode*/XRT            3739        357        26         