ﻻ يوجد ملخص باللغة العربية
Hybrid Morphology Radio Sources (HyMoRS) are a very rare and newly discovered subclass of radio galaxies that have mixed FR morphology i.e., these galaxies have FR-I structure on one side of the core and FR-II structure on the other side of the core. We systematically searched for HyMoRS using VLA Faint Images of the Radio Sky at Twenty-cm (FIRST) survey at 1400 MHz and identified forty-five confirmed HyMoRS and five candidates HyMoRS. Our finding significantly increased the known sample size of HyMoRS. HyMoRS may play an essential role in understanding the interaction of jets with the interstellar medium and a very debated topic of the FR dichotomy. We identified optical/IR counterparts for thirty-nine sources in our catalogue. In our sample of sources, five sources had Quasar-like behavior. We had estimated the spectral index and radio luminosity of HyMoR sources in our catalogue, when possible. We found that the source J1336+2329 ($log L=26.93$ W Hz$^{-1}$sr$^{-1}$) was the most luminous and the source J1204+3801, a Quasar, was the farthest HyMoRS (with redshift $z$=1.28) in our sample. With the help of a large sample size of the newly discovered sources, various statistical properties were studied.
Ultra-steep spectrum (USS) radio sources are good tracers of powerful radio galaxies at $z > 2$. Identification of even a single bright radio galaxy at $z > 6$ can be used to detect redshifted 21cm absorption due to neutral hydrogen in the intervenin
We present Clusterrank, a new algorithm for identifying dispersed astrophysical pulses. Such pulses are commonly detected from Galactic pulsars and rotating radio transients (RRATs), which are neutron stars with sporadic radio emission. More recently
We report the first discovery of a fast radio burst (FRB), FRB 20200125A, by the Green Bank Northern Celestial Cap (GBNCC) Pulsar Survey conducted with the Green Bank Telescope at 350 MHz. FRB 20200125A was detected at a Galactic latitude of 58.43 de
Hybrid morphology radio sources (HyMoRS) are a rare group of radio galaxies in which differing Fanaroff & Riley morphologies (FR I/II) are observed for each of the two lobes. While they potentially provide insights into the formation of lobe structur
The radio spectral index is a powerful probe for classifying cosmic radio sources and understanding the origin of the radio emission. Combining data at 147 MHz and 1.4 GHz from the TIFR GMRT Sky Survey (TGSS) and the NRAO VLA Sky Survey (NVSS), we pr