Aims. With the accumulation of polarization data in gamma-ray burst (GRB) prompt phase, models can be tested. Methods. We predicted time-integrated polarizations 37 GRBs with observation. used their observed spectral parameters to do this. In model, emission mechanism is synchrotron radiation, and magnetic field configuration region was assumed large-scale ordered. Therefore, degrees (PDs) are ...

Artificial intelligence-based hardware devices are deployed in manufacturing units and industries for emission gas monitoring control. The data obtained from the intelligent analyzed at different stages standard emissions carbon This research article proposes a control-centric classification technique (CDCT) analyzing as well controlling pollution-causing units. AI observe intensity, rate, comp...

Using the publicly available eROSITA Final Equatorial Depth Survey (eFEDS) data, we detected stacked X-ray emissions at position of 463 filaments a significance 3.8 sigma based on combination all energy bands. In parallel, found that probability measurement under null hypothesis is ~0.0017. The were identified with galaxies in Sloan Digital Sky survey, ranging from 30 Mpc to 100 length 0.2 < z ...

Abstract The purpose of this work is to characterize the diffuse Galactic polarized synchrotron, which dominant CMB foreground emission at low frequency. We present EE, BB, and EB power spectra estimated from polarization frequency maps 23 30 GHz as observed respectively by WMAP K-band Planck lowest channel, for a set six sky regions covering 30% 94% sky. study synchrotron angular distribution ...