Multi-messenger astrophysics

Multi-messenger astrophysics

Discussions around tools and discoveries in the novel domain of multi-messenger and time domain astrophysics. We'll highlight recent publications, discuss tools to faciliate observations and generally talk about the cool science behind the most violent explosions in the universe.

Tämä podcast on lisätty Podme-palveluun avoimen RSS-syötteen kautta eikä se ole Podmen omaa tuotantoa. Siksi podcastin jaksot saattavat sisältää mainontaa.

Jaksot(101)

Beyond the GW Horizon: Hunting for Kilonovae with KNTraP

Beyond the GW Horizon: Hunting for Kilonovae with KNTraP

Kilonovae (KNe) are bright, rapidly fading astronomical events believed to be caused by the radioactive decay of heavy elements produced during the merger of neutron stars or a neutron star and a blac...

3 Joulu 202420min

Unveiling the Milky Way's Hidden Glow: Diffuse Gamma Rays measured by LHAASO

Unveiling the Milky Way's Hidden Glow: Diffuse Gamma Rays measured by LHAASO

In this episode, we explore the fascinating world of diffuse gamma rays emanating from the Galactic plane. A new study using the Large High Altitude Air Shower Observatory's Water Cherenkov Detector A...

28 Marras 202414min

Cosmic Coincidence? Exploring the Gamma-Ray Flare Potentially Associated with FRB 20240114A

Cosmic Coincidence? Exploring the Gamma-Ray Flare Potentially Associated with FRB 20240114A

Publication: arXiv:2411.06996 Acknowledements: Podcast prepared with Google/NotebookLM. Illustration credits: Y. Xing et al. (arXiv:2411.06996)

15 Marras 202410min

Unlocking the Muon Puzzle with IACTs

Unlocking the Muon Puzzle with IACTs

IACTs (Imaging Atmospheric Cherenkov Telescopes) are typically used for gamma-ray astronomy. Muons are produced in hadronic showers and IACTs can detect these muons, which are normally considered back...

12 Marras 20249min

Cosmic Magnetism: How the Milky Way Bends the Path of UHECRs

Cosmic Magnetism: How the Milky Way Bends the Path of UHECRs

Ultra-high-energy cosmic rays (UHECRs) are the most energetic particles ever detected, with energies exceeding 10^18 eV. Their origin remains a mystery, as their paths are deflected by magnetic fields...

7 Marras 202411min

Swift's Continuous Commanding: Enabling New Discoveries in the Gravitational Wave Era

Swift's Continuous Commanding: Enabling New Discoveries in the Gravitational Wave Era

Swift's New Capability: Continuous Commanding A new capability of the Neil Gehrels Swift Observatory, called "continuous commanding", allows Swift to respond to targets of opportunity within 10 secon...

4 Marras 202410min

Ultra-High-Energy Photons: Unlocking the Secrets of Gravitational Wave Sources

Ultra-High-Energy Photons: Unlocking the Secrets of Gravitational Wave Sources

The Pierre Auger Observatory, situated in Argentina, is designed to detect UHE cosmic rays. The observatory is also sensitive to UHE photons and has been used to search for photons from various source...

31 Loka 20249min

The Mystery of the 21-Minute Pulsar

The Mystery of the 21-Minute Pulsar

Astronomers discovered a new long-period (21-minute) radio transient called GPM J1839–10, with the Murchison Widefield Array (MWA). Follow-up observations were done using other telescopes, including t...

28 Loka 202412min

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