collaborators

6 papers

astro-ph.CO2026

Probing inflationary features with galaxy ultraviolet luminosity function observables

Sandeep Kumar Acharya

We use the galaxy ultraviolet luminosity function measurements at to constrain modification to standard inflationary power spectrum. These observables are sensitive to the…

astro-ph.HE2026

The role of the galaxy stellar mass function in determining the cosmological distribution of astrophysical transients with applications to fast radio bursts and merging binary black holes

Sandeep Kumar Acharya

The cosmological distribution and formation rate of compact astrophysical objects such as fast radio bursts (FRBs) are typically assumed to be proportional to a linear combination…

astro-ph.CO2025

Utilizing localized fast radio bursts to constrain their progenitors and the expansion history of the Universe

Sandeep Kumar Acharya, Paz Beniamini

Fast radio bursts (FRBs) are increasingly being used for cosmological applications such as measuring the Hubble constant and baryon abundance. The increasing number of localized FR…

astro-ph.HE2025

Persistent radio sources associated with fast radio bursts: Implications from magnetar progenitors

Sk. Minhajur Rahaman, Sandeep Kumar Acharya, Paz Beniamini +1

The rare association of three persistent radio sources (confirmed PRS1 and PRS2, candidate PRS3) with repeating fast radio bursts (FRB 20121102A, 20190520B, 20201124A) offers a uni…

astro-ph.CO2025

Redshift dependence of FRB host dispersion measures across cosmic epochs

Sandeep Kumar Acharya, Paz Beniamini

We constrain the redshift dependence of (rest frame) host galaxy dispersion measures of localized Fast Radio Bursts (FRBs) by assuming it to vary as a simple power law ($\propto (1…

astro-ph.HE2025

Features and prospects for kilonova remnant detection with current and future surveys

Sandeep Kumar Acharya, Paz Beniamini, Kenta Hotokezaka

We study the observable spectral and temporal properties of kilonova remnants (KNRs) analytically, and point out quantitative differences with respect to supernova remnants. We pro…