Redshifts and luminosity distances of blazars producing the sample of brightest gamma-ray flares. I adopt standard ΛCDM cosmology with H0 = 71 km s−1 Mpc−1, Ωm = 0.27 and ΩΛ = 0.73.
| Blazar . | z . | dL [Gpc] . |
|---|---|---|
| 3C 454.3 | 0.859 | 5.49 |
| PKS 1510−089 | 0.360 | 1.92 |
| PKS 1222+216 | 0.432 | 2.37 |
| 3C 273 | 0.158 | 0.75 |
| PKS 0402−362 | 1.423 | 10.31 |
| Blazar . | z . | dL [Gpc] . |
|---|---|---|
| 3C 454.3 | 0.859 | 5.49 |
| PKS 1510−089 | 0.360 | 1.92 |
| PKS 1222+216 | 0.432 | 2.37 |
| 3C 273 | 0.158 | 0.75 |
| PKS 0402−362 | 1.423 | 10.31 |
Redshifts and luminosity distances of blazars producing the sample of brightest gamma-ray flares. I adopt standard ΛCDM cosmology with H0 = 71 km s−1 Mpc−1, Ωm = 0.27 and ΩΛ = 0.73.
| Blazar . | z . | dL [Gpc] . |
|---|---|---|
| 3C 454.3 | 0.859 | 5.49 |
| PKS 1510−089 | 0.360 | 1.92 |
| PKS 1222+216 | 0.432 | 2.37 |
| 3C 273 | 0.158 | 0.75 |
| PKS 0402−362 | 1.423 | 10.31 |
| Blazar . | z . | dL [Gpc] . |
|---|---|---|
| 3C 454.3 | 0.859 | 5.49 |
| PKS 1510−089 | 0.360 | 1.92 |
| PKS 1222+216 | 0.432 | 2.37 |
| 3C 273 | 0.158 | 0.75 |
| PKS 0402−362 | 1.423 | 10.31 |
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