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
| 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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