Measured D values for 8 examined optical fields and their IRIS counterparts. In addition, we include the results for Herschel Field#5 and two IRAS testing fields, Chameleon and Taurus. Second column lists an area of the image, columns (3) and (5) list the fractal dimensions and intercepts for the optical (or Herschel) data; (5) and (6) lists the results for the optical data rebinned to 90 arcsec and reconvolved with the IRIS PSF; columns (7) and (8) list the results for the IRIS counterpart with the optical or Herschel mask applied where possible, columns (9) and (10) – for the same data without a mask. Column (11) is the difference between (5) and (7). All presented values of D indicate a median for the MC realizations, the upper and lower error boundaries are 1σ from the corresponding percentiles.
| Field . | A, deg2 . | D . | K . | D90 . | K90 . | DIRIS . | KIRIS . | |$D_\mathrm{IRIS}^\mathrm{orig}$| . | |$K_\mathrm{IRIS}^\mathrm{orig}$| . | D90−DIRIS . |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . |
| #1 | 2.0 | |$1.88^{+0.02}_{-0.01}$| | 1.03 | |$1.41^{+0.12}_{-0.12}$| | 1.83 | |$1.49^{+0.16}_{-0.08}$| | 1.61 | |$1.34^{+0.04}_{-0.05}$| | 2.02 | −0.09 |
| #2 | 0.8 | |$1.66^{+0.06}_{-0.06}$| | 1.41 | |$1.54^{+0.08}_{-0.04}$| | 1.49 | |$1.65^{+0.09}_{-0.06}$| | 1.32 | |$1.50^{+0.12}_{-0.10}$| | 1.61 | −0.10 |
| #3 | 1.8 | |$1.70^{+0.04}_{-0.05}$| | 1.33 | |$1.54^{+0.07}_{-0.09}$| | 1.53 | |$1.59^{+0.18}_{-0.09}$| | 1.43 | |$1.52^{+0.07}_{-0.06}$| | 1.53 | −0.06 |
| #4 | 2.0 | |$1.66^{+0.06}_{-0.06}$| | 1.41 | |$1.52^{+0.09}_{-0.09}$| | 1.53 | |$1.57^{+0.08}_{-0.08}$| | 1.44 | |$1.40^{+0.10}_{-0.07}$| | 1.76 | −0.05 |
| #5 | 3.0 | |$1.66^{+0.05}_{-0.06}$| | 1.40 | |$1.57^{+0.05}_{-0.04}$| | 1.43 | |$1.43^{+0.05}_{-0.05}$| | 1.76 | |$1.41^{+0.05}_{-0.05}$| | 1.75 | 0.14 |
| #16 | 1.0 | |$1.64^{+0.04}_{-0.05}$| | 1.42 | |$1.55^{+0.14}_{-0.07}$| | 1.46 | |$1.40^{+0.04}_{-0.02}$| | 1.69 | |$1.33^{+0.02}_{-0.02}$| | 2.01 | 0.15 |
| #join1 | 9.2 | |$1.69^{+0.06}_{-0.05}$| | 1.31 | |$1.63^{+0.05}_{-0.04}$| | 1.34 | |$1.45^{+0.10}_{-0.08}$| | 1.68 | |$1.35^{+0.06}_{-0.05}$| | 1.92 | 0.18 |
| #join2 | 6.8 | |$1.67^{+0.05}_{-0.04}$| | 1.35 | |$1.61^{+0.04}_{-0.03}$| | 1.38 | |$1.32^{+0.09}_{-0.09}$| | 2.11 | |$1.22^{+0.10}_{-0.05}$| | 2.35 | 0.29 |
| Avg | – | |$1.69^{+0.05}_{-0.05}$| | 1.33 | |$1.54^{+0.08}_{-0.09}$| | 1.50 | |$1.48^{+0.10}_{-0.07}$| | 1.63 | |$1.38^{+0.07}_{-0.06}$| | 1.86 | – |
| Herschel #5 | 3.0 | |$1.65^{+0.07}_{-0.04}$| | 1.37 | |$1.40^{+0.08}_{-0.05}$| | 1.87 | |$1.43^{+0.05}_{-0.05}$| | 1.76 | |$1.41^{+0.05}_{-0.05}$| | 1.75 | −0.03 |
| Chameleon | – | – | – | – | – | – | – | |$1.36^{+0.02}_{-0.02}$| | 1.91 | – |
| Taurus | – | – | – | – | – | – | – | |$1.33^{+0.03}_{-0.03}$| | 1.98 | – |
| Field . | A, deg2 . | D . | K . | D90 . | K90 . | DIRIS . | KIRIS . | |$D_\mathrm{IRIS}^\mathrm{orig}$| . | |$K_\mathrm{IRIS}^\mathrm{orig}$| . | D90−DIRIS . |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . |
| #1 | 2.0 | |$1.88^{+0.02}_{-0.01}$| | 1.03 | |$1.41^{+0.12}_{-0.12}$| | 1.83 | |$1.49^{+0.16}_{-0.08}$| | 1.61 | |$1.34^{+0.04}_{-0.05}$| | 2.02 | −0.09 |
| #2 | 0.8 | |$1.66^{+0.06}_{-0.06}$| | 1.41 | |$1.54^{+0.08}_{-0.04}$| | 1.49 | |$1.65^{+0.09}_{-0.06}$| | 1.32 | |$1.50^{+0.12}_{-0.10}$| | 1.61 | −0.10 |
| #3 | 1.8 | |$1.70^{+0.04}_{-0.05}$| | 1.33 | |$1.54^{+0.07}_{-0.09}$| | 1.53 | |$1.59^{+0.18}_{-0.09}$| | 1.43 | |$1.52^{+0.07}_{-0.06}$| | 1.53 | −0.06 |
| #4 | 2.0 | |$1.66^{+0.06}_{-0.06}$| | 1.41 | |$1.52^{+0.09}_{-0.09}$| | 1.53 | |$1.57^{+0.08}_{-0.08}$| | 1.44 | |$1.40^{+0.10}_{-0.07}$| | 1.76 | −0.05 |
| #5 | 3.0 | |$1.66^{+0.05}_{-0.06}$| | 1.40 | |$1.57^{+0.05}_{-0.04}$| | 1.43 | |$1.43^{+0.05}_{-0.05}$| | 1.76 | |$1.41^{+0.05}_{-0.05}$| | 1.75 | 0.14 |
| #16 | 1.0 | |$1.64^{+0.04}_{-0.05}$| | 1.42 | |$1.55^{+0.14}_{-0.07}$| | 1.46 | |$1.40^{+0.04}_{-0.02}$| | 1.69 | |$1.33^{+0.02}_{-0.02}$| | 2.01 | 0.15 |
| #join1 | 9.2 | |$1.69^{+0.06}_{-0.05}$| | 1.31 | |$1.63^{+0.05}_{-0.04}$| | 1.34 | |$1.45^{+0.10}_{-0.08}$| | 1.68 | |$1.35^{+0.06}_{-0.05}$| | 1.92 | 0.18 |
| #join2 | 6.8 | |$1.67^{+0.05}_{-0.04}$| | 1.35 | |$1.61^{+0.04}_{-0.03}$| | 1.38 | |$1.32^{+0.09}_{-0.09}$| | 2.11 | |$1.22^{+0.10}_{-0.05}$| | 2.35 | 0.29 |
| Avg | – | |$1.69^{+0.05}_{-0.05}$| | 1.33 | |$1.54^{+0.08}_{-0.09}$| | 1.50 | |$1.48^{+0.10}_{-0.07}$| | 1.63 | |$1.38^{+0.07}_{-0.06}$| | 1.86 | – |
| Herschel #5 | 3.0 | |$1.65^{+0.07}_{-0.04}$| | 1.37 | |$1.40^{+0.08}_{-0.05}$| | 1.87 | |$1.43^{+0.05}_{-0.05}$| | 1.76 | |$1.41^{+0.05}_{-0.05}$| | 1.75 | −0.03 |
| Chameleon | – | – | – | – | – | – | – | |$1.36^{+0.02}_{-0.02}$| | 1.91 | – |
| Taurus | – | – | – | – | – | – | – | |$1.33^{+0.03}_{-0.03}$| | 1.98 | – |
Measured D values for 8 examined optical fields and their IRIS counterparts. In addition, we include the results for Herschel Field#5 and two IRAS testing fields, Chameleon and Taurus. Second column lists an area of the image, columns (3) and (5) list the fractal dimensions and intercepts for the optical (or Herschel) data; (5) and (6) lists the results for the optical data rebinned to 90 arcsec and reconvolved with the IRIS PSF; columns (7) and (8) list the results for the IRIS counterpart with the optical or Herschel mask applied where possible, columns (9) and (10) – for the same data without a mask. Column (11) is the difference between (5) and (7). All presented values of D indicate a median for the MC realizations, the upper and lower error boundaries are 1σ from the corresponding percentiles.
| Field . | A, deg2 . | D . | K . | D90 . | K90 . | DIRIS . | KIRIS . | |$D_\mathrm{IRIS}^\mathrm{orig}$| . | |$K_\mathrm{IRIS}^\mathrm{orig}$| . | D90−DIRIS . |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . |
| #1 | 2.0 | |$1.88^{+0.02}_{-0.01}$| | 1.03 | |$1.41^{+0.12}_{-0.12}$| | 1.83 | |$1.49^{+0.16}_{-0.08}$| | 1.61 | |$1.34^{+0.04}_{-0.05}$| | 2.02 | −0.09 |
| #2 | 0.8 | |$1.66^{+0.06}_{-0.06}$| | 1.41 | |$1.54^{+0.08}_{-0.04}$| | 1.49 | |$1.65^{+0.09}_{-0.06}$| | 1.32 | |$1.50^{+0.12}_{-0.10}$| | 1.61 | −0.10 |
| #3 | 1.8 | |$1.70^{+0.04}_{-0.05}$| | 1.33 | |$1.54^{+0.07}_{-0.09}$| | 1.53 | |$1.59^{+0.18}_{-0.09}$| | 1.43 | |$1.52^{+0.07}_{-0.06}$| | 1.53 | −0.06 |
| #4 | 2.0 | |$1.66^{+0.06}_{-0.06}$| | 1.41 | |$1.52^{+0.09}_{-0.09}$| | 1.53 | |$1.57^{+0.08}_{-0.08}$| | 1.44 | |$1.40^{+0.10}_{-0.07}$| | 1.76 | −0.05 |
| #5 | 3.0 | |$1.66^{+0.05}_{-0.06}$| | 1.40 | |$1.57^{+0.05}_{-0.04}$| | 1.43 | |$1.43^{+0.05}_{-0.05}$| | 1.76 | |$1.41^{+0.05}_{-0.05}$| | 1.75 | 0.14 |
| #16 | 1.0 | |$1.64^{+0.04}_{-0.05}$| | 1.42 | |$1.55^{+0.14}_{-0.07}$| | 1.46 | |$1.40^{+0.04}_{-0.02}$| | 1.69 | |$1.33^{+0.02}_{-0.02}$| | 2.01 | 0.15 |
| #join1 | 9.2 | |$1.69^{+0.06}_{-0.05}$| | 1.31 | |$1.63^{+0.05}_{-0.04}$| | 1.34 | |$1.45^{+0.10}_{-0.08}$| | 1.68 | |$1.35^{+0.06}_{-0.05}$| | 1.92 | 0.18 |
| #join2 | 6.8 | |$1.67^{+0.05}_{-0.04}$| | 1.35 | |$1.61^{+0.04}_{-0.03}$| | 1.38 | |$1.32^{+0.09}_{-0.09}$| | 2.11 | |$1.22^{+0.10}_{-0.05}$| | 2.35 | 0.29 |
| Avg | – | |$1.69^{+0.05}_{-0.05}$| | 1.33 | |$1.54^{+0.08}_{-0.09}$| | 1.50 | |$1.48^{+0.10}_{-0.07}$| | 1.63 | |$1.38^{+0.07}_{-0.06}$| | 1.86 | – |
| Herschel #5 | 3.0 | |$1.65^{+0.07}_{-0.04}$| | 1.37 | |$1.40^{+0.08}_{-0.05}$| | 1.87 | |$1.43^{+0.05}_{-0.05}$| | 1.76 | |$1.41^{+0.05}_{-0.05}$| | 1.75 | −0.03 |
| Chameleon | – | – | – | – | – | – | – | |$1.36^{+0.02}_{-0.02}$| | 1.91 | – |
| Taurus | – | – | – | – | – | – | – | |$1.33^{+0.03}_{-0.03}$| | 1.98 | – |
| Field . | A, deg2 . | D . | K . | D90 . | K90 . | DIRIS . | KIRIS . | |$D_\mathrm{IRIS}^\mathrm{orig}$| . | |$K_\mathrm{IRIS}^\mathrm{orig}$| . | D90−DIRIS . |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . |
| #1 | 2.0 | |$1.88^{+0.02}_{-0.01}$| | 1.03 | |$1.41^{+0.12}_{-0.12}$| | 1.83 | |$1.49^{+0.16}_{-0.08}$| | 1.61 | |$1.34^{+0.04}_{-0.05}$| | 2.02 | −0.09 |
| #2 | 0.8 | |$1.66^{+0.06}_{-0.06}$| | 1.41 | |$1.54^{+0.08}_{-0.04}$| | 1.49 | |$1.65^{+0.09}_{-0.06}$| | 1.32 | |$1.50^{+0.12}_{-0.10}$| | 1.61 | −0.10 |
| #3 | 1.8 | |$1.70^{+0.04}_{-0.05}$| | 1.33 | |$1.54^{+0.07}_{-0.09}$| | 1.53 | |$1.59^{+0.18}_{-0.09}$| | 1.43 | |$1.52^{+0.07}_{-0.06}$| | 1.53 | −0.06 |
| #4 | 2.0 | |$1.66^{+0.06}_{-0.06}$| | 1.41 | |$1.52^{+0.09}_{-0.09}$| | 1.53 | |$1.57^{+0.08}_{-0.08}$| | 1.44 | |$1.40^{+0.10}_{-0.07}$| | 1.76 | −0.05 |
| #5 | 3.0 | |$1.66^{+0.05}_{-0.06}$| | 1.40 | |$1.57^{+0.05}_{-0.04}$| | 1.43 | |$1.43^{+0.05}_{-0.05}$| | 1.76 | |$1.41^{+0.05}_{-0.05}$| | 1.75 | 0.14 |
| #16 | 1.0 | |$1.64^{+0.04}_{-0.05}$| | 1.42 | |$1.55^{+0.14}_{-0.07}$| | 1.46 | |$1.40^{+0.04}_{-0.02}$| | 1.69 | |$1.33^{+0.02}_{-0.02}$| | 2.01 | 0.15 |
| #join1 | 9.2 | |$1.69^{+0.06}_{-0.05}$| | 1.31 | |$1.63^{+0.05}_{-0.04}$| | 1.34 | |$1.45^{+0.10}_{-0.08}$| | 1.68 | |$1.35^{+0.06}_{-0.05}$| | 1.92 | 0.18 |
| #join2 | 6.8 | |$1.67^{+0.05}_{-0.04}$| | 1.35 | |$1.61^{+0.04}_{-0.03}$| | 1.38 | |$1.32^{+0.09}_{-0.09}$| | 2.11 | |$1.22^{+0.10}_{-0.05}$| | 2.35 | 0.29 |
| Avg | – | |$1.69^{+0.05}_{-0.05}$| | 1.33 | |$1.54^{+0.08}_{-0.09}$| | 1.50 | |$1.48^{+0.10}_{-0.07}$| | 1.63 | |$1.38^{+0.07}_{-0.06}$| | 1.86 | – |
| Herschel #5 | 3.0 | |$1.65^{+0.07}_{-0.04}$| | 1.37 | |$1.40^{+0.08}_{-0.05}$| | 1.87 | |$1.43^{+0.05}_{-0.05}$| | 1.76 | |$1.41^{+0.05}_{-0.05}$| | 1.75 | −0.03 |
| Chameleon | – | – | – | – | – | – | – | |$1.36^{+0.02}_{-0.02}$| | 1.91 | – |
| Taurus | – | – | – | – | – | – | – | |$1.33^{+0.03}_{-0.03}$| | 1.98 | – |
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