The Galactic latitude dependence of centimeter-wavelength flicker

1987 ◽  
Vol 93 ◽  
pp. 589 ◽  
Author(s):  
D. S. Heeschen ◽  
B. J. Rickett
2021 ◽  
Vol 923 (1) ◽  
pp. 2 ◽  
Author(s):  
A. Josephy ◽  
P. Chawla ◽  
A. P. Curtin ◽  
V. M. Kaspi ◽  
M. Bhardwaj ◽  
...  

Abstract We investigate whether the sky rate of fast radio bursts (FRBs) depends on Galactic latitude using the first catalog of FRBs detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Project. We first select CHIME/FRB events above a specified sensitivity threshold in consideration of the radiometer equation, and then we compare these detections with the expected cumulative time-weighted exposure using Anderson–Darling and Kolmogorov–Smirnov tests. These tests are consistent with the null hypothesis that FRBs are distributed without Galactic latitude dependence (p-values distributed from 0.05 to 0.99, depending on completeness threshold). Additionally, we compare rates in intermediate latitudes (∣b∣ < 15°) with high latitudes using a Bayesian framework, treating the question as a biased coin-flipping experiment–again for a range of completeness thresholds. In these tests the isotropic model is significantly favored (Bayes factors ranging from 3.3 to 14.2). Our results are consistent with FRBs originating from an isotropic population of extragalactic sources.


2020 ◽  
Vol 889 (1) ◽  
pp. 56 ◽  
Author(s):  
María Gabriela Navarro ◽  
Dante Minniti ◽  
Joyce Pullen ◽  
Rodrigo Contreras Ramos

1977 ◽  
Vol 212 ◽  
pp. 707 ◽  
Author(s):  
R. C. Henry ◽  
J. R. Swandic ◽  
S. D. Shulman ◽  
G. Fritz

1970 ◽  
Vol 37 ◽  
pp. 280-288
Author(s):  
B. A. Cooke ◽  
R. E. Griffiths ◽  
K. A. Pounds

It is widely believed that the diffuse X-ray background, observed on several occasions over the energy range from 0.25 keV to above 1 MeV has an extragalactic origin. Evidence for this comes from the generally reported isotropy above several keV [1, 2, 3] and the observed galactic latitude dependence at 0.25 keV, believed to result from the interstellar attenuation of these low energy photons in passage through the Galaxy [4, 5].


2016 ◽  
Vol 821 (1) ◽  
pp. L11 ◽  
Author(s):  
K. Sano ◽  
S. Matsuura ◽  
K. Tsumura ◽  
T. Arai ◽  
M. Shirahata ◽  
...  

1972 ◽  
Vol 177 ◽  
pp. 365 ◽  
Author(s):  
D. J. Yentis ◽  
R. Novick ◽  
P. vanden Bout

Sign in / Sign up

Export Citation Format

Share Document