Table 3.
Sources with multiple Faraday depth measurements.
# | Name | 150 MHz This work | 150 MHz Mulcahy et al. (2014) | 610 MHz Farnes et al. (2013) | 1.4 GHz Taylor et al. (2009) | 1 – 2 GHz Mao et al. (2015) | 1.4,1.6 GHz Heald et al. (2009) |
---|---|---|---|---|---|---|---|
1.a | J133920+464115 | +20.4 ± 0.1 | +20.5 ± 0.1 | Outside FOV | +5.5 ± 7.3 | Outside FOV | Outside FOV |
2. | 4C+47.38 | +23.2 ± 0.1 | +23.5 ± 0.1 | Outside FOV | +30.6 ± 1.4 | Outside FOV | Outside FOV |
3. | J132626+473741 | +3.0 ± 0.1 | +3.2 ± 0.1 | ND | NI | Outside FOV | Outside FOV |
4. | J133707+485801 | +9.0 ± 0.1 | +9.2 ± 0.1 | Outside FOV | −8.9 ± 3.2 | Outside FOV | Outside FOV |
6.a | J133613+490037 | +9.2 ± 0.1 | ND | Outside FOV | +11.1 ± 10.6 | Outside FOV | Outside FOV |
7a. | J133045+470318 | −98.0 ± 0.1 | −ND | −15.97 ± 0.03 | ND | +10 ± 2 | Outside FOV |
8. | J133051+475928 | +57.8 ± 0.1 | ND | Edge of FOV | −5.2 ± 17.0 | Outside FOV | Outside FOV |
11. | B3 1323+476 | −57.0 ± 0.1 | ND | −16.97 ± 0.03 | ND | Outside FOV | Outside FOV |
14. | B3 1330+459 | −4.4 ± 0.1 | −5.2 ± 0.1 | Outside FOV | ND | Outside FOV | Outside FOV |
…b | J132930+470612 | +96.2 ± 0.1 | ND | ND | ND | +21 ± 2 | ND |
19. | B3 1324+473 | −56.0 ± 0.1 | ND | −8.11 ± 0.07 | ND | Outside FOV | Outside FOV |
… | B3 1329+459 | ND | −3.8 ± 0.1 | Outside FOV | +35.0 ± 16.3 | Outside FOV | Outside FOV |
… | B3 1326+470 | ND | ND | −6.638 ±0.013 | +10.0 ± 10.3 | Outside FOV | Outside FOV |
… | J132939+465909 | ND | ND | +11.15 ±0.05 | −16.2 ± 16.8 | +16.6 ± 0.3 | +14 ± 1 |
… | J133015+471026 | ND | ND | +33.52 ± 0.03 | ND | +26.0 ± 0.4 | +28 ± 4 |
7b. | J133045+470318 | ND | ND | −3.24 ± 0.04 | ND | +17.2 ± 0.8 | +17 ± 2 |
52a. | J133124+471317 | ND | ND | +11.51 ± 0.03 | NI | +10.7 ± 0.4 | +9 ± 1 |
52b. | J133127+471300 | ND | ND | +7.67 ± 0.04 | ND | +6.0 ±0.5 | +3 ± 1 |
… | B3 1331+472 | ND | ND | +0.93 ± 0.23 | +16.6 ± 17.6 | Outside FOV | Outside FOV |
…b | J132941.5+471734 | ND | ND | ND | ND | +23.5 ± 0.9 | +20 ± 1 |
Notes. ND means that the source is not detected. NI means that it was not included in the Taylor et al. (2009) RM catalog but detected in polarization in the NVSS catalog of Condon et al. (1998) with a polarized flux density (PINVSS) greater than 3 mJy, which is below the 8σ threshold to be included in the Taylor et al. (2009) catalog. The sources are listed by increasing p-value. The top list (above the horizontal dashed line) are the sources detected with a false discovery rate of 5%. Source 5 in Table 2 is not included here because it was not listed in any of the other surveys. The sources listed above the second line (including the top list) have a false discovery rate of 50%. The bottom list (below the horizontal line) contains the sources not detected by us but with a Faraday depth (or RM) measured in at least two other radio polarization studies. 7a and 7b are two components of the same sources but appear in different parts of the table. 52a and 52b are two components of the same source.
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