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Found 13 papers, 1 papers with code
Network strategies to study Epstein-Barr virus associated carcinomas and potential etiological mechanisms for oncogenesis
Based on the DisGeNET (v7. 0) data set, we constructed a disease-gene network bipartite graph to identify genes that are involved in various carcinomas namely, gastric cancer (GC), nasopharyngeal cancer (NPC), Hodgkin's lymphoma (HL) and Burkitt's lymphoma (BL).
Network-based community detection of comorbidities and their association with SARS-CoV-2 virus during COVID-19 pathogenesis
Given this scenario, we identified biological processes and pathways which are most likely affected by COVID-19.
Constraining Galaxy Haloes from the Dispersion and Scattering of Fast Radio Bursts and Pulsars
We compare our analysis of the Milky Way halo with other galaxy haloes by placing limits on the scattering contributions from haloes intersecting the lines-of-sight to FRB 181112 and FRB 191108.
Astrophysics of Galaxies High Energy Astrophysical Phenomena
The NANOGrav 11-Year Data Set: Limits on Gravitational Wave Memory
At a strain of $2. 5\times10^{-14}$, corresponding to the median upper limit as a function of source sky position, we set a limit on the rate of GW memory events at $<0. 4$ yr$^{-1}$.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
A sample of low energy bursts from FRB 121102
The bursts are generally detected in less than a third of the 580-MHz observing bandwidth, demonstrating that narrow-band FRB signals may be more common than previously thought.
High Energy Astrophysical Phenomena
A Radio Source Coincident with the Superluminous Supernova PTF10hgi: Evidence for a Central Engine and an Analogue of the Repeating FRB121102?
We present the detection of an unresolved radio source coincident with the position of the Type I superluminous supernova (SLSN) PTF10hgi ($z=0. 098$) about 7. 5 years post-explosion, with a flux density of $F_\nu(6\,\,{\rm GHz)}\approx 47. 3\ \mu Jy$ and a luminosity of $L_\nu(6\,\,{\rm GHz})\approx 1. 1\times 10^{28}$ erg s$^{-1}$ Hz$^{-1}$.
High Energy Astrophysical Phenomena
The NANOGrav 11-year Data Set: Pulse Profile Variability
The strongest evidence for long-timescale pulse profile changes is seen in PSRs B1937+21 and J1643-1224.
High Energy Astrophysical Phenomena
The NANOGrav 11-year Data Set: Solar Wind Sounding Through Pulsar Timing
We filter out long time scale DM fluctuations attributable to structure in the interstellar medium and carry out a simultaneous analysis of all pulsars in our sample that can differentiate the correlated signature of the wind from signals unique to individual lines of sight.
Solar and Stellar Astrophysics
Testing Convolutional Neural Networks for finding strong gravitational lenses in KiDS
We have tested the ConvNet lens-finders on a sample of 21789 Luminous Red Galaxies (LRGs) selected from KiDS and we have analyzed and compared the results with our previous ConvNet lens-finder on the same sample.
Astrophysics of Galaxies Instrumentation and Methods for Astrophysics
A Second Chromatic Timing Event of Interstellar Origin toward PSR J1713+0747
The frequency dependence of radio pulse arrival times provides a probe of structures in the intervening media.
High Energy Astrophysical Phenomena
Optimal Frequency Ranges for Sub-Microsecond Precision Pulsar Timing
We also find that arrival-time precision can be improved by increases in total bandwidth.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics
Automated Diagnosis of Epilepsy Employing Multifractal Detrended Fluctuation Analysis Based Features
In fractal geometry, Multifractal Detrended Fluctuation Analysis MFDFA is a popular technique to examine the self-similarity of a nonlinear, chaotic and noisy time series.
Finding Strong Gravitational Lenses in the Kilo Degree Survey with Convolutional Neural Networks
The volume of data that will be produced by new-generation surveys requires automatic classification methods to select and analyze sources.
Astrophysics of Galaxies
