Table 1
List of new γ-ray detections and associations for the Radio-Planck sources, following a case–case description in Sect. 4.
| Source | Redshift | log( ) |
log(ν f ) |
log( ) |
log(νf ) |
N0 (10−13) | Γ | TS |
|---|---|---|---|---|---|---|---|---|
| 5BZQJ 0359+5057a | 1.512 | 12.1 | –10.7 | 21.3 | –10.4 | 36.6 ± 1.5 | 2.72 ± 0.04 | 786.0 |
| 5BZQJ 1955+5131a | 1.210 | 12.6 | –11.7 | 20.8 | –11.1 | 7.0 ± 0.7 | 2.56 ± 0.10 | 119.7 |
| 5BZUJ 0909+4253a | 0.670 | 12.9 | –11.5 | 20.9 | –11.7 | 3.5 ± 0.5 | 2.62 ± 0.15 | 74.4 |
| 5BZQJ 1153+8058a | 1.250 | 12.6 | –12.0 | 21.1 | –11.9 | 2.1 ± 0.4 | 2.53 ± 0.19 | 33.7 |
| 5BZQJ 0646+4451a | 3.396 | 11.6 | –11.8 | 20.8? | –11.7 | 3.8 ± 0.7 | 3.39 ± 0.24 | 85.6 |
| 5BZQJ 0125–0005a | 1.077 | 12.8 | –11.6 | 20.3 | –11.6 | 2.2 ± 0.5 | 2.90 ± 0.31 | 22.5 |
| 5BZQJ 0555+3948b | 2.365 | 12.0 | –11.8 | 20.8 | –10.9 | 10.2 ± 1.0 | 3.12 ± 0.11 | 195.5 |
| 5BZUJ 0433+0521b | 0.033 | 13.8 | –10.2 | 19.8 | –10.2 | 14.4 ± 1.0 | 2.97 ± 0.08 | 370.4 |
| 5BZQJ 0228+6721b | 0.523 | 12.8 | –11.2 | 21.1 | –11.4 | 8.0 ± 1.0 | 2.65 ± 0.12 | 79.4 |
| 5BZQJ 2218–0335c | 0.901 | 12.3 | –11.3 | 21.0? | –11.7 | 2.7 ± 0.6 | 2.80 ± 0.27 | 19.9 |
| 5BZBJ 0006–0623c | 0.347 | 13.0 | –11.1 | 20.3 | –11.9 | 1.4 ± 0.4 | 2.13 ± 0.20 | 17.5 |
| 5BZQJ 1038+0512c | 0.450 | 12.0 | –11.8 | 20.8? | –12.1 | 1.6 ± 0.6 | 2.79 ± 0.38 | 10.1 |
| 5BZQJ 0010+1058d | 0.089 | 14.5 | –10.7 | 20.5 | –10.8 | 4.1 ± 1.9 | 3.22 ± 0.53 | 26.0* |
| 5BZUJ 0241–0815d | 0.005 | 13.9? | –10.3 | 20.9? | –10.6 | 6.3 ± 0.2 | 1.64 ± 0.01 | 12.0* |
| 5BZQJ 2136+0041d | 1.941 | 10.8 | –11.7 | 21.2 | –11.2 | 19.9 ± 2.0 | 2.46 ± 0.10 | 7.5* |
| 5BZQJ 1642+6856e | 0.751 | 12.5 | –11.6 | 20.1? | –12.3 | 9.1 ± 4.0 | 2.31 ± 0.28 | 8.3 |
Notes. Columns Source and Redshift list the blazar name and distance as from Massaro et al. (2015). We note that Table A.1 brings an extra name reference as from NVSS Radio Catalog (Condon et al. 1998) given that each blazar has a well-defined radio counterpart. Columns 
and log(
) refer to the peak frequency from Syn and IC components measured in Hz. Columns log(
) and log(
) correspond to the Syn and IC peak-power measured in erg cm−2 s−1. Column N0 list the pre-factor as of Eq. (1) in units of ph cm−2 s−1 MeV−1 when assuming E0 = 1000 MeV. Column Γ list the photon spectral index as of Eq. (1). Column TS list the test statistic values associated with the γ-ray signature for each source when integrating over 7.5 yr of Fermi-LAT PASS8 observations. All model parameters were derived using the Fermi Science Tools assuming a power-law spectrum within the 0.3–500 GeV energy band. (a)New detections at TS > 20 level; (b)new association from better positioning of 3FGL sources, (c)faint detections with TS between 10–20; (d)sources only detectable during short flare episodes (for those cases, TS values refer to the bright state integrated over one month); and (e)sources that could be confused with a second γ-ray emitter.
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