activity
20092023
most citedConstraints on the ultra-high energy cosmic neutrino flux from the fourth flight of ANITA

102 citations · 530 across the 39 of their papers we have counts for

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25 papers · 1 filter

astro-ph.HE2023★ 23 cited

The peak-flux of GRB 221009A measured with GRBAlpha

Jakub Ripa, Hiromitsu Takahashi, Yasushi Fukazawa +42

The brightest gamma-ray burst ever observed, long-duration GRB 221009A, was detected by GRBAlpha nano-satellite without saturation. We present light curves of the prompt emission i…

astro-ph.HE2023★ 14 cited

Localisation of gamma-ray bursts from the combined SpIRIT+HERMES-TP/SP nano-satellite constellation

Matt Thomas, Michele Trenti, Riccardo Campana +24

Multi-messenger observations of the transient sky to detect cosmic explosions and counterparts of gravitational wave mergers critically rely on orbiting wide-FoV telescopes to cove…

astro-ph.HE2021★ 19 cited

Analysis of a Tau Neutrino Origin for the Near-Horizon Air Shower Events Observed by the Fourth Flight of the Antarctic Impulsive Transient Antenna (ANITA)

R. Prechelt, S. A. Wissel, A. Romero-Wolf +65

We study in detail the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to possible point source fluxes detected via -lepton-induced air showers. This inve…

astro-ph.HE2021★ 5 cited

Timing techniques applied to distributed modular high-energy astronomy: the HERMES project

A. Sanna, A. F. Gambino, L. Burderi +15

The HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites -- Technologic and Scientific Pathfinder) is an in-orbit demonstration of the so-called distributed astronomy con…

astro-ph.HE2021★ 24 cited

The HERMES-Technologic and Scientific Pathfinder

F. Fiore, L. Burderi, M. Lavagna +12

HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites Technologic and Scientific Pathfinder) is a constellation of six 3U nano-satellites hosting simple but innovative X-r…

astro-ph.HE2020★ 6 cited

A search for ultrahigh-energy neutrinos associated with astrophysical sources using the third flight of ANITA

C. Deaconu, L. Batten, P. Allison +60

The ANtarctic Impulsive Transient Antenna (ANITA) long-duration balloon experiment is sensitive to interactions of ultra high-energy (E > 10^{18} eV) neutrinos in the Antarctic ice…

astro-ph.HE2020

Gamma-ray bursts: A brief survey of the diversity

Attila Mészáros, Jakub Řípa

The separation of the gamma-ray bursts (GRBs) into short/hard and long/soft subclasses, respectively, is well supported both theoretically and observationally. The long ones are co…

astro-ph.HE2020

The analogy of K-correction in the topic of gamma-ray bursts

Levente Borvák, Attila Mészáros, Jakub Řípa

It is well-known that there are two types of gamma-ray bursts (GRBs): short/hard and long/soft ones, respectively. The long GRBs are coupled to supernovae, but the short ones are a…

astro-ph.HE2019★ 102 cited

Constraints on the ultra-high energy cosmic neutrino flux from the fourth flight of ANITA

P. W. Gorham, P. Allison, O. Banerjee +57

The ANtarctic Impulsive Transient Antenna (ANITA) NASA long-duration balloon payload completed its fourth flight in December 2016, after 28 days of flight time. ANITA is sensitive…

astro-ph.HE2018★ 24 cited

Update on Testing the Isotropy of the Properties of Gamma-Ray Bursts

Jakub Řípa, Arman Shafieloo

Previously we proposed a novel method to inspect the isotropy of the properties of gamma-ray bursts (GRBs) such as their duration, fluences and peak fluxes at various energy bands…

astro-ph.HE2017★ 38 cited

Testing Isotropic Universe Using the Gamma-Ray Burst Data of Fermi / GBM

Jakub Ripa, Arman Shafieloo

The sky distribution of Gamma-Ray Bursts (GRBs) has been intensively studied by various groups for more than two decades. Most of these studies test the isotropy of GRBs based on t…

astro-ph.HE2017

Summary of Parallel Session: "Relativistic and Particle Astrophysics"

Jakub Ripa

The parallel session on "Relativistic and Particle Astrophysics" was held on 14th December 2015. Here a short summary of each presentation of this parallel session is given.

astro-ph.HE2017

Gamma-ray bursts and their relation to astroparticle physics and cosmology

Jakub Ripa

This article gives an overview of gamma-ray bursts (GRBs) and their relation to astroparticle physics and cosmology. GRBs are the most powerful explosions in the universe that occu…

astro-ph.HE2015

Testing and Performance of UFFO Burst Alert & Trigger Telescope

J. Ripa, M. B. Kim, J. Lee +26

The Ultra-Fast Flash Observatory pathfinder (UFFO-p) is a new space mission dedicated to detect Gamma-Ray Bursts (GRBs) and rapidly follow their afterglows in order to provide earl…

astro-ph.HE2012★ 1 cited

Cosmological effects on the observed flux and fluence distributions of gamma-ray bursts

Jakub Ripa, Attila Meszaros, Felix Ryde

Several claims have been put forward that an essential fraction of long-duration BATSE gamma-ray bursts should lie at redshifts larger than 5. This point-of-view follows from the n…

astro-ph.HE2012★ 31 cited

On the Spectral Lags and Peak-Counts of the Gamma-Ray Bursts Detected by the RHESSI Satellite

Jakub Ripa, Attila Meszaros, Peter Veres +1

A sample of 427 gamma-ray bursts from a database (February 2002 - April 2008) of the RHESSI satellite is analyzed statistically. The spectral lags and peak-count rates, which have…

astro-ph.HE2011

Statistical Analysis of the Observable Data of Gamma-Ray Bursts

Jakub Ripa

Gamma-ray bursts are still not fully understood events. However, their exploration could provide a useful tool for a better understanding of the early Universe because they belong…

astro-ph.HE2010★ 1 cited

A comparison of the fluences and photon peak fluxes for the Swift and RHESSI gamma-ray bursts

D. Huja, J. Ripa, A. Meszaros

Fluences and photon peak fluxes of the gamma-ray bursts (GRBs) detected by the Swift and RHESSI satellites are graphically compared.

astro-ph.HE2010★ 1 cited

Rising indications for three gamma-ray burst groups

J. Ripa, D. Huja, A. Meszaros +1

Several papers were written about the gamma-ray burst (GRBs) groups. Our statistical study is based on the durations and hardness ratios of the Swift and RHESSI data.

astro-ph.HE2010★ 1 cited

How the RHESSI gamma-ray burst measurements have been affected by the annealing procedure?

J. Ripa, P. Veres, C. Wigger

The performance of the nine RHESSI germanium detectors has been gradually deteriorating since its launch in 2002 because of radiation damage. To restore its former sensitivity, the…

astro-ph.HE2010

A Search for the Intermediate Subgroup of Gamma-Ray Bursts in the Swift Dataset

D. Huja, J. Ripa

We have searched for the third, 'intermediate', subgroup of gamma-ray bursts among nearly 400 gamma-ray bursts observed by the Swift satellite. The standard chi^2 method and F-test…

astro-ph.HE2010★ 1 cited

Gamma-Ray Burst Classes Found in the RHESSI Data Sample

J. Ripa, C. Wigger, D. Huja +1

A sample of 427 gamma-ray bursts (GRBs), measured by the RHESSI satellite, is studied statistically to determine the number of GRB groups. Previous studies based on the BATSE Catal…

astro-ph.HE2009

Statistical analysis of RHESSI GRB database

J. Ripa, R. Hudec, A. Meszaros +2

The Gamma-ray burst (GRB) database based on the data by the RHESSI satellite provides a unique and homogeneous database for future analyses. Here we present preliminary results on…

astro-ph.HE2009★ 51 cited

A comparison of the gamma-ray bursts detected by BATSE and Swift

D. Huja, A. Meszaros, J. Ripa

The durations of 388 gamma-ray bursts, detected by the Swift satellite, are studied statistically in order to search for their subgroups. Then the results are compared with the res…