Table A.4
SMGPS SNR candidates (extract).
| Name | GLong | GLat | Radius | Reliability a |
|---|---|---|---|---|
| deg. | deg. | arcmin. | ||
| G257.408−00.162 | 257.408 | −0.162 | 35.6 | I |
| G259.683−01.235 | 259.683 | −1.235 | 7.7 | I |
| G275.256−00.979 | 275.256 | −0.979 | 17.2 | I |
| G275.986−01.077 | 275.986 | −1.077 | 4.8 | I |
| G276.229+00.419 | 276.229 | 0.419 | 1.5 | II |
| G277.162+00.396 | 277.162 | 0.396 | 4.8 | II |
| G278.924−01.195 | 278.924 | −1.195 | 24.1 | II |
| G280.151+00.206 | 280.151 | 0.206 | 12.8 | I |
| G281.188−00.053 | 281.188 | −0.053 | 29.1 | I |
| G282.674−00.737 … | 282.674 | −0.737 | 10.4 | I |
Notes. (a)’Sources with I are the most reliable and have clear SMGPS emission that is not confused with that of other SNRs or H II regions, with a morphology that is similar to that of known SNRs; II sources are less reliable and are either in confused regions with other SNRs or H II regions or have a morphology that is slightly ambiguous; III sources are the least reliable and are badly confused with other SNRs or H II regions, have spatially coincident radio and MIR emission that may indicate that at least some of the radio emission is thermal, or are incomplete shells. The full table is available at the CDS.
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