List of targets for the SEDI project.I 100 is the median, background subtracted intensity at 100 micron. The last two columns mark the fields to be observed at DRAO (HI) and Nanten (CO). |
| Shock processed dust | R.A. (2000) | Dec (2000) | l (deg) | b (deg) | I 100 (MJy/sr) | v (km/s) | nH (H/cm^3) | HI | CO |
| WISM towards HD 93521 | 10 48 00.0 | +37 34 00.0 | 183.2 | 62.1 | 0.4-0.8 | 0, -60 | 0.1 | y | n |
| WISM around SPICA | 13 25 12.0 | -11 09 40.0 | 316.2 | 50.8 | 1-4 | 0 | 0.5 | n | n |
| IVC G210.8+63.1 | 10 51 43.1 | +24 59 03.7 | 210.7 | 63.1 | 0.8-3 | -40 | HI/H2 | y | n |
| IVC Draco | 16 45 00.0 | +60 30 00.0 | 90.4 | 38.8 | 1-4 | -40 | HI/H2 | y | n |
| Cygnus Loop SNR | 20 56 03.8 | +31 51 33.2 | 75.61 | -8.65 | 4-14 | 200 | 1 | y | n |
| From cirrus to GMCs | R.A. (2000) | Dec (2000) | l (deg) | b (deg) | I 100 (MJy/sr) | Av | M (sol. mass) | HI | CO |
| cirrus toward 3C380 | 18 29 30.0 | +48 43 20.0 | 77.2 | 23.5 | 1-4 | 0.1 | - | y | n |
| Ursa Major | 09 39 23.6 | +70 21 26.1 | 141.7 | 39.0 | 4-8 | <1 | - | y | n |
| Polaris flare | 01 43 34.7 | +87 45 14.5 | 123.5 | 24.9 | 5-8 | 0.3-2 | - | y | n |
| DC300-17 | 11 48 14.2 | -79 16 40.7 | 299.9 | -16.8 | 8-18 | 2 | 200 | n | y |
| MBM12 | 02 54 00.0 | +20 17 00.0 | 158.2 | -34.1 | 10-20 | 0.3-5 | 50 | y | y |
| Taurus fil. | 04 19 02.1 | +25 19 13.4 | 171.2 | -17.5 | 10-20 | 1-5 | 500 | y | y |
| L134 | 15 52 37.7 | -04 08 53.7 | 4.5 | 36.3 | 10-20 | 1-8 | 1000 | n | y |
| Serpens GMC | 18 04 39.0 | -04 29 45.5 | 23.5 | 8.3 | 20-40 | 10 | 10E5 | n | y |
| Diffuse H II Regions and PDRs | R.A. (2000) | Dec (2000) | l (deg) | b (deg) | I 100 (MJy/sr) | G0 | nH (H/cm^3) | HI | CO |
| Ced201 | 22 13 20.0 | +70 15 00.0 | 110.3 | 11.4 | 15-30 | 1-100 | 10E4 | y | n |
| California | 03 59 16.0 | +36 23 30.1 | 160.0 | -12.6 | 30-80 | 10-10E4 | 0.5-1000 | y | n |
| Rho-halo | 16 14 53.9 | -18 47 29.4 | 355.6 | 22.6 | 40-90 | 5 | 100-1000 | n | y |
| Index |