Statistical Summary
The following graphics illustrate that all of the expected science and calibration areas are well represented in the SODRM 2012.
SODRM Program Statistics
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Category # of Programs Total Time [Days] Percentage of Total Time Solar System 8 51.3 7.9% Exoplanets 14 104.4 16.1% Galactic 19 132.3 20.4% Nearby Galaxies 13 111.3 17.2% Distant Galaxies & Cosmology 16 204.5 31.5% Instrument Calibration 40 31.9 4.9% Observation Calibration 2 13.0 2.0% Total 112 648.7 100.0% -
Category Total Time [Days] Percentage of Total Time NIRCam 225.3 34.7% NIRSpec 194.4 30.0% NIRISS 51.9 8.0% MIRI 177.1 27.3% Total 648.7 100.0% -
Category Total Time [Days] Percentage of Total Time NIRCam Imaging 200.1 20.8% NIRCam Coronagraphy 25.2 3.9% NIRSpec Multi-Object Spectroscopy 102.2 15.8% NIRSpec Integral Field Slit Spectroscopy 43.5 6.7% NIRSpec Fixed Slit Spectroscopy 48.7 7.5% NIRISS Slitless Wide Field Spectroscopy 10.2 1.6% NIRISS Slitless Single Object Spectroscopy 17.3 2.7% NIRISS Aperture Mask Interferometry 22.7 3.5% NIRISS Imaging 1.7 0.3% MIRI Imaging 94.6 14.6% MIRI Coronagraphy 28.7 4.4% MIRI Low Resolution Spectroscopy 18.8 2.9% MIRI Medium Resolution Spectroscopy 35.0 5.4% Subtotal By Observation Type
Category Total Time [Days] Percentage of Total Time Total Imaging 296.4 45.7% Total Coronagraphy 76.6 11.8% Total Spectroscopy 275.7 42.5% Total 648.7 100.0% -
The distribution of non-moving sources from all the SODRM programs is shown in galactic coordinates. The size of the symbol is proportional to the total exposure time per observing template on that target. The symbols are coded by science/calibration area with dark green for Exoplanets, light green for Galactic, red for Nearby Galaxies, purple for Distant Galaxies & Cosmology, and light blue for Instrument/Observatory Calibration. Solar System targets are moving targets and not shown. The large purple circles show the locations of the JWST deep field programs.
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