4 citations · 17 across the 12 of their papers we have counts for
13 papers
Rapid Construction of Joint Pulsar Timing Array Datasets: The Lite Method
Bjorn Larsen, Chiara M. F. Mingarelli, Paul T. Baker +41
The International Pulsar Timing Array (IPTA)'s second data release (IPTA DR2) combines decades of observations of 65 millisecond pulsars from 7 radio telescopes. IPTA datasets shou…
On the simultaneity of Forbush decreases: the simultaneous effects of interplanetary parameters and geomagnetic activity indices
I. O. Eya, E. U. Iyida, O. Okike +9
Forbush decreases (Fd) are transient, short-term reductions in the intensity of galactic cosmic rays that reach the Earth's surface. When this reduction is observed at multiple loc…
The Implication of Enhanced Cosmic Ray Diurnal Anisotropy on the Global Simultaneity of Forbush Decreases: A Statistical Approach
O. Okike, J. A. Alhassan, I. O. Eya
The short-term rapid CR flux depressions, generally referred to as Forbush decreases (FDs), are the most spectacular time-intensity CR variation. The need for analytical transforma…
The ORT and the uGMRT Pulsar Monitoring Program : Pulsar Timing Irregularities & the Gaussian Process Realization
Himanshu Grover, Bhal Chandra Joshi, Jaikhomba Singha +8
The spin-down law of pulsars is generally perturbed by two types of timing irregularities: glitches and timing noise. Glitches are sudden changes in the rotational frequency of pul…
Pulsar glitch activities: the spin parameters approach
Innocent Okwudili Eya, Evaristus Uzochukwu Iyida
Glitch activity refers to the mean increase in pulsar spin frequency per year due to rotational glitches. It is an important tool for studying super-nuclear matter using neutron st…
On the pulsar spin frequency derivatives and the glitch activity
Innocent O. Eya, Jibrin A. Alhassan, Evaristus U. Iyida +2
The number of sudden spin-ups in radio pulsars known as pulsar glitches has increased over the years. Though a consensus has not been reached with regards to the actual cause of th…
Investigating possible unification of Seyfert galaxies and blazars in Fermi-LAT sample
E. U. Iyida, I. O. Eya, F. C. Odo
Statistical analyses are invaluable methods used to understand intrinsic emission processes and the unification of extragalactic radio sources. In this paper, we collected radio, X…
On the Unified View of Extragalactic Sources based on their Broadband Emission Properties
E. U. Iyida, I. O. Eya, F. C. Odo
Our understanding of the unification of jetted AGNs has advanced greatly as the size of extragalactic sources increased. In the present paper, based on the large sample of radio so…
On the challenges of Angular Momentum Transfer Mechanism of Pulsar Glitches
I. O. Eya, C. I. Eze, E. U. Iyida
The angular momentum transfer mechanism of pulsar glitches for over four decades now stands as standalone theory with regards to glitch sizes and inter-glitch time intervals. Howev…
On the bimodal nature of the distributions of pulsar glitch sizes
I. O. Eya, E. U. Iyida, C. I. Eze
Pulsar glitches are sudden spin-ups in pulsar spin frequency (). The glitch size, , is a key parameter in any mechanism puts across towards the understanding of the events…
Microglitches in radio pulsars: the role of strange nuggets
Innocent Okwudili Eya, Evaristus Uzochukwu Iyida, Johnson Ozoemene +2
Strange Nuggets are believed to be among the relics of the early universe. They appear as dark matter due to their low charge-to-mass ratio. Their distribution is believed to be th…
Entrainment factor on individual glitch fractional moment of inertia
Innocent O. Eya, Johnson O. Urama, Augustine E. Chukwude
The superfluid in the inner crust of neutron star is assumed to be the reservoir of momentum released in pulsar glitch. Recently, due to crustal entrainment, it is debatable whethe…
On the distributions of pulsar glitch sizes and the inter-glitch time intervals
Innocent O. Eya, Johnson O. Urama, Augustine E. Chukwude
The glitch size, , inter-glitch time interval, and frequency of glitches in pulsars are key parameters in discussing glitch phenomena. In this paper, the glitch si…