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Table 25

Microwave (143GHz) vs. γ-ray flux correlation parameters.

γ-ray Class Fermi-LAT sample Swift-BAT sample ROSAT/RASS sample Radio sample
integration No. of ρ P(%) No. of ρ P(%) No. of ρ P(%) No. of ρ P(%)
period sources sources sources sources
(a)/(b)/(c) (a)/(b)/(c) (a)/(b)/(c) (a)/(b)/(c)
Simult. All 16/5/32 0.22 12.4 8/6/20 0.42 2.49 6/20/25 0.42 1.42 22/2/71 0.35 0.07
FSRQs 10/3/16 0.23 23.4 5/2/12 0.39 9.92 4/3/6 0.65 3.97 15/1/46 0.33 1.19
BL Lacs 5/2/9 0.55 4.76 2/2/2 ...∗ ... 2/11/4 ... ... 4/0/10 0.38 17.6
2 months All 36/5/9 0.29 4.18 11/7/20 0.61 0.07 8/21/18 0.31 6.00 37/3/56 0.40 0.01
FSRQs 19/3/6 0.17 38.7 6/3/15 0.59 0.89 4/4/9 0.51 6.83 23/2/42 0.36 0.39
BL Lacs 11/2/1 0.72 0.92 3/3/2 ... ... 3/11/5 ... ... 10/0/6 0.42 10.2
27 months All 47/3/0 0.47 0.10 22/16/7 0.67 <0.01 12/23/18 0.40 0.99 75/4/16 0.48 <0.01
FSRQs 25/3/0 0.48 1.27 16/3/4 0.54 1.59 8/3/7 0.85 0.15 47/2/19 0.48 0.01
BL Lacs 14/0/0 0.72 0.91 3/4/0 ... ... 2/14/2 ... ... 16/0/0 0.55 3.22

Notes. 

(a)

Number of sources detected both by Planck and Fermi-LAT.

(b)

Number of Planck upper limits.

(c)

Number of Fermi-LAT upper limits.

(*)

The number of detections is too low to allow a reliable estimation of ρ.

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