Table A.3
Image properties of the TeV-detected AGN in our observations.
Source | Morphology(a) | Epoch | bmaj(b) | bmin(c) | PA(d) | Stot(e) | σ(f) | Ibase(g) | Score(h) | Θcore(i) | Tb(j) | S0.1−100GeV(k) | STeV(l) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
[yyyy-mm-dd] | [mas] | [mas] | [º] | [mJy] | [mJy/beam] | [mJy/beam] | [mJy] | [mas] | [K] | [ph/cm2/s] | CU | ||
0011–191 | C | 2020-11-20 | 17.6 | 3.9 | 1 | 16.4 | 0.1 | 0.3 | 16.6 ± 1.7 | 8.8 ±0.8 | (5.5 ± 1.1) × 107 | (2.71 ± 0.33) × 10−10 | 0.006 |
0031–196 | C | 2020-11-20 | 22.2 | 2.8 | −1 | 19.1 | 0.2 | 0.4 | 19.1 ± 1.9 | 14.2 ± 0.6 | (3.6 ± 0.5) × 107 | (2.69 ± 0.08) × 10−9 | 0.009 |
0236–314 | SS | 2020-02-18 | 11.4 | 3.2 | 2 | 24.9 | 0.1 | 0.3 | 14.9 ± 1.5 | 3.3 ± 0.6 | (4.0 ± 1.6) × 108 | (9.13 ± 0.48) × 10−10 | - |
0301–243 | SS | 2020-11-20 | 14.4 | 2.9 | 2 | 170.5 | 0.5 | 1.1 | 91.9 ±9.2 | 1.4 ±0.6 | (1.4 ± 1.2) × 1010 | (4.79 ± 0.11) × 10−9 | 0.014 |
0347–121 | SS | 2020-02-18 | 23.3 | 3.1 | 2 | 10.4 | 0.1 | 0.2 | 10.0 ± 1.0 | 10.0 ±0.6 | (2.8 ± 0.4) × 107 | (3.69 ± 0.37) × 10−10 | 0.02 |
0426–380 | SS | 2020-02-18 | 9.1 | 3.0 | 4 | 761.1 | 1.6 | 5.3 | 599.1 ± 59.9 | 1.5 ±0.6 | (1.4 ± 1.1) × 1011 | (2.14 ± 0.02) × 10−8 | - |
0447–439 | SS | 2020-02-18 | 9.3 | 3.1 | 3 | 89.9 | 0.3 | 0.8 | 58.2 ±5.8 | 1.9 ±0.6 | (4.3 ± 2.9) × 109 | (1.25 ± 0.02) × 10−8 | 0.03 |
0548–322 | C | 2020-11-20 | 10.6 | 3.0 | 1 | 27.2 | 0.3 | 0.7 | 13.9 ± 1.4 | 1.0 ±0.55 | (1.1 ±0.7) × 109 | (3.13 ± 0.34) × 10−10 | 0.013 |
0625–354 | SS | 2020-02-18 | 9.0 | 3.0 | 1 | 352.0 | 2.5 | 5.3 | 218.0 ±21.8 | 1.8 ±0.6 | (1.7 ± 1.2) × 1010 | 1.26 ± 0.06) × 10−9 | 0.04 |
0903–573 | SS | 2020-11-20 | 7.6 | 3.4 | 16 | 346.8 | 0.8 | 1.8 | 196.8 ± 19.7 | 2.4 ± 0.7 | (1.4 ± 0.8) × 1010 | (9.09 ± 0.15) × 10−9 | - |
1008–310 | C | 2021-12-04 | 21.2 | 2.7 | 3 | 28.7 | 2.0 | 0.3 | 19.0 ± 1.9 | 2.3 ± 0.5 | (9.0 ± 4.0) × 108 | (6.08 ± 0.54) × 10−10 | 0.008 |
1101–232 | C | 2021-12-04 | 17.6 | 2.3 | 1 | 38.3 | 0.3 | 0.9 | 30.3 ± 3.0 | 2.2 ± 0.5 | (1.7 ± 0.7) × 109 | (4.29 ± 0.44) × 10−10 | 0.02 |
1253–053 | SS | 2020-02-18 | 20.6 | 2.5 | 3 | 8133.5 | 7.9 | 45.1 | 5220.1 ± 522.0 | 1.1 ±0.5 | (1.6 ± 1.4) × 1012 | (4.09 ± 0.03) × 10−8 | - |
1312–423 | C | 2020-02-18 | 18.0 | 2.8 | −6 | 11.9 | 0.1 | 0.2 | 8.3 ± 0.8 | 2.0 ± 0.6 | (5.1 ± 2.8) × 108 | (3.85 ± 0.47) × 10−10 | 0.005 |
1322–428 | DS | 2021-12-04 | 7.1 | 2.7 | 5 | 3630.6 | 2.5 | 8.6 | 519.8 ±52.0 | 2.3 ± 0.5 | (2.3 ± 1.1) × 1010 | (3.59 ± 0.09) × 10−9 | 0.08 |
1440–389 | SS | 2020-11-20 | 10.3 | 2.6 | 4 | 133.5 | 0.2 | 0.6 | 104.7 ± 10.5 | 1.7 ±0.5 | (9.0 ± 5.0) × 109 | (4.08 ± 0.11) × 10−9 | 0.054 |
1510–089 | SS | 2020-02-18 | 13.4 | 5.9 | 16 | 2445.4 | 7.9 | 30.5 | 1842.5 ± 184.3 | 3.6 ± 1.2 | (4.5 ± 2.9) × 1010 | (3.38 ± 0.03) × 10−8 | 0.03 |
1514–241 | DS | 2020-11-20 | 11.0 | 3.1 | 2 | 2571.3 | 0.9 | 2.9 | 993.7 ± 99.4 | 2.2 ± 0.6 | (5.0 ± 2.9) × 1010 | (6.67 ± 0.13) × 10−9 | 0.04 |
1515–273 | SS | 2020-11-20 | 15.4 | 7.5 | 0 | 120.6 | 0.3 | 0.7 | 81.0 ± 8.1 | 3.7 ± 1.5 | (1.5 ± 1.2) × 109 | (1.71 ± 0.07) × 10−9 | - |
1600–489 | DS | 2020-11-20 | 8.7 | 4.2 | −2 | 1282.9 | 1.1 | 3.8 | 581.4 ±58.1 | 5.4 ±0.8 | (5.7 ± 1.9) × 109 | (5.62 ± 0.20) × 10−9 | - |
2005–489 | SS | 2020-02-18 | 7.4 | 2.6 | 3 | 751.7 | 2.1 | 5.4 | 235.1 ± 23.5 | 1.4 ±0.5 | (2.9 ± 2.1)×1010 | (2.90 ± 0.09) × 10−9 | 0.03 |
2155–304 | SS | 2020-02-18 | 12.3 | 2.6 | −1 | 320.3 | 0.6 | 2.0 | 186.0 ± 18.6 | 3.0 ±0.5 | (5.5 ± 2.0) × 109 | (2.00 ± 0.02) × 10−8 | 0.15 |
2322–409 | SS | 2020-11-20 | 10.0 | 3.5 | 0 | 55.8 | 0.2 | 0.6 | 43.5 ± 4.4 | 2.3 ± 0.7 | (2.3 ± 1.4) × 109 | (1.07 ± 0.06) × 10−9 | 0.011 |
2356–309 | SS | 2021-12-04 | 16.6 | 3.2 | 1 | 24.1 | 0.1 | 0.3 | 14.0 ± 1.4 | 2.6 ± 0.6 | (5.8 ± 2.9) × 108 | (4.50 ± 0.39) × 10−10 | 0.02 |
Notes. (a)Source morphology: C - core only; SS - single-sided; DS - double-sided jet morphology. (b)Beam major axis. (c)Beam minor axis. (d)Beam position angle. (e)Total flux density. (ƒ)Rms noise of the image. (g)Lowest contour. (h)Flux density of the core. (i)FWHM of the core. (j)Brightness temperature. (k)Photon flux from (Abdollahi et al. 2022). (l)Very high energy flux in Crab units.
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