Table 4.
Observing conditions adopted for the artificial photometric images of the remnants.
| Band | μlim [mag arcsec−2] | (S/N)lim | FWHM [arcsec] | References |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) |
| B | 26.0 | 5 | 0.7 | 1 |
| V | 26.0 | 5 | 0.5 | 2 |
| R | 27.5 | 5 | 0.7 | 3, 4 |
| I | 26.0 | 5 | 0.7 | 1 |
| K | 22.0 | 3 | 0.7 | 5 |
Notes. Column 1: photometric band. Column 2: assumed limiting surface brightness in mag arcsec−2 (Vega system). Column 3: signal-to-noise (S/N) ratio corresponding to the limiting surface brightness. Column 4: full width at half maximum of the assumed PSF in arcsec. Column 5: reference observational studies.
References. (1) SDSS, Abazajian et al. (2009); (2) KB12; (3) Erwin et al. (2008); (4) Gutiérrez et al. (2011); (5) NIRS0S, L11.
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