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PODCAST

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.

science astronomy

All Episodes

00:13:19

A Star’s Death by a Thousand Cuts: The Runaway...

Multi-messenger astrophysics ·

2025/11/03

In this episode, we dive into the fascinating and violent world of galactic centers with the discovery of **AT2023uqm**, a new nuclear transient offering unprecedented insights into stellar consumption by supermassive black holes (SMBHs).AT2023uqm is only the second confirmed case of a star undergoing **repeated partial tidal disruption events (rpTDEs)**, where a star on a bound, eccentric orbit repeatedly loses its outer layers as it approaches the SMBH.**What makes AT2023uqm unique?**Unlike its

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00:12:33

NGC1068 and Its Kin: New Evidence for Neutrino...

Multi-messenger astrophysics ·

2025/10/20

Join us as we discuss the latest results from the IceCube Neutrino Observatory, utilizing 13.1 years of data, that further link high-energy neutrinos to powerful cosmic sources.### Episode Highlights* **The Extragalactic Neutrino Puzzle:** The IceCube Neutrino Observatory consistently detects a diffuse flux of high-energy cosmic neutrinos, the majority of which are extragalactic in origin. These neutrinos are expected to be produced in hadronic interactions, which also generate gamma rays.*

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00:18:50

LHAASO’s Giant Peanut: A Challenge to Extreme...

Multi-messenger astrophysics ·

2025/10/13

Join us as we discuss the groundbreaking discovery by the LHAASO Collaboration of a vast and unique ultra-high-energy (UHE) $\gamma$-ray source. This mysterious object, nicknamed the **"Peanut"** for its distinctive asymmetric shape, spans approximately $0.45^\circ \times 4.6^\circ$ and is located far off the Galactic plane, at a high Galactic latitude ($b \approx -17.5^\circ$), a region where UHE $\gamma$-ray sources are typically sparse.**Key Takeaways:*** **Extreme Energies Detected:**

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00:19:37

Cosmic Ray Neighbors: How Nearby Transients Solve the...

Multi-messenger astrophysics ·

2025/10/09

The origin of ultra-high-energy cosmic rays (UHECRs) has long been one of the central open questions in astroparticle physics. We dive into fascinating new research suggesting that the answer lies not in distant, powerful sources, but in **rare, stellar transients (like neutron star mergers) occurring right here in our neighboring galaxies**.**Key Takeaways:*** **Nearby Dominance:** The UHECR flux above 25 EeV is shown to be largely **dominated by just ten nearby galaxies located within 8 Mpc** of

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00:17:32

Cosmic Outlier: X-ray Clues to the Mystery of GRB...

Multi-messenger astrophysics ·

2025/10/01

**GRB 250702B** is an **exceptional transient** that has puzzled astronomers, as it does not neatly fit into the expected populations of **ultra-long Gamma-Ray Bursts (GRBs)** or **relativistic Tidal Disruption Events (TDEs)**.The event produced luminous gamma-ray radiation lasting **over 25 ks** (thousands of seconds), classifying it as an ultra-long GRB. However, unlike any previously known GRB, the Einstein Probe discovered a soft X-ray "precursor" activity up to **24 hours before the

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00:15:35

Constraining Gamma-Ray Burst Parameters with the...

Multi-messenger astrophysics ·

2025/09/22

This week, we dive into the cosmic puzzle posed by ultra-high-energy (UHE) neutrinos. The conversation centers on the **KM3-230213A event**, detected by the KM3NeT/ARCA detector, which is the **highest-energy neutrino observed to date**, estimated at $220^{+570}_{-110}$ PeV. This detection marks the first observation of a presumed astrophysical neutrino in the UHE regime.We explore the longstanding candidates for these UHE neutrinos: **Gamma-Ray Bursts (GRBs)**. GRBs are the most energetic transient

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00:14:19

Unmasking Cosmic Explosions with the Einstein Probe

Multi-messenger astrophysics ·

2025/09/15

his episode dives into the groundbreaking discoveries of the Einstein Probe, a new soft X-ray mission revolutionizing our understanding of high-energy transients in the universe.The Einstein Probe (EP), launched on January 9, 2024, has opened a new era of transient discovery in the previously largely unexplored soft X-ray band. It detects numerous fast X-ray transients, many of which surprisingly show no gamma-ray emission, making their connection to more common gamma-ray bursts (GRBs) a key

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00:16:56

Unprecedented Radio Views: Decoding GRB 231117A's...

Multi-messenger astrophysics ·

2025/08/27

Join us as we explore the groundbreaking observations of **GRB231117A**, a short gamma-ray burst (SGRB) located at a redshift of z = 0.257. This event, detected by the Neil Gehrels Swift Observatory, was quickly followed up by the Australia Telescope Compact Array (ATCA) just 1.3 hours post-burst, providing **unprecedented early radio detection**.**In this episode, we discuss:*** **Early Radio Afterglow:** How ATCA's rapid response revealed a dynamic early radio afterglow with **flaring,

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00:16:57

Beyond the Burst: How Host Galaxies Shape Fast Radio...

Multi-messenger astrophysics ·

2025/08/13

Join us as we explore the latest research into Fast Radio Bursts (FRBs), mysterious, intense pulses of radio emission lasting only milliseconds. These cosmic phenomena are not just fleeting signals; they are powerful probes of the ionized gas across the universe and valuable tools for cosmological studies. In this episode, we delve into an investigation of FRB properties and their host galaxies, aiming to understand how the environment surrounding an FRB influences its observed characteristics.What

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00:21:49

A Glimpse into the Early Universe with FRB 20240304B

Multi-messenger astrophysics ·

2025/08/07

Join us as we explore the groundbreaking discovery of FRB 20240304B, the most distant Fast Radio Burst (FRB) ever detected, offering unprecedented insights into the early universe.In this episode, we discuss:• What are Fast Radio Bursts (FRBs)? These enigmatic, millisecond-duration radio signals provide unique information about the plasma permeating our universe, revealing details about magnetic fields and gas distributions.• The Record-Breaking Discovery: FRB 20240304B was detected by the MeerKAT

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00:16:38

Einstein Telescope + WST: Spectroscopy's Role in the...

Multi-messenger astrophysics ·

2025/07/10

In this episode, we dive into the exciting future of **multi-messenger astronomy**, specifically focusing on the detection and characterization of binary neutron star (BNS) mergers.* **The Dawn of Multi-Messenger Astrophysics:** Our understanding of cosmic events was revolutionized by the extraordinary joint detection of gravitational waves (GWs) and light from a BNS merger on August 17, 2017 (GW170817). This single event confirmed theoretical hypotheses about short gamma-ray bursts (SGRBs)

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00:16:00

The Muon Puzzle: IceCube's Quest for Cosmic Ray Clues

Multi-messenger astrophysics ·

2025/07/01

Dive into the fascinating world of cosmic rays with the latest research from the IceCube Neutrino Observatory! This episode explores new measurements of high-energy muons in extensive air showers, shedding light on the mysterious mass composition of cosmic rays and the challenges of simulating their interactions in Earth's atmosphere.**What we discuss:*** **Measuring High-Energy Muons:** Learn about the first measurement of the **mean number of muons with energies above 500 GeV** in

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00:23:46

X-Ray Clues to Cosmic Rays: The Discovery of a...

Multi-messenger astrophysics ·

2025/06/24

Join us as we dive into the latest astronomical discovery! Scientists have identified a **new candidate pulsar wind nebula (PWN)**, named XMMU 034124.2+525720, which may be directly linked to **1LHAASO J0343+5254u**, a powerful "PeVatron" in our galaxy.**What are PeVatrons?** They are the most energetic astrophysical objects in our galaxy, producing cosmic rays (CRs) with energies exceeding 1 PeV (10^15 eV), far surpassing what terrestrial accelerators can achieve. Understanding them is

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00:15:46

Cosmic Clash: LHAASO's Proton-Gamma Ray Mystery

Multi-messenger astrophysics ·

2025/06/17

In this episode, we dive into a fascinating new study that performs the **first direct consistency check** between two crucial measurements from the Large High Altitude Air Shower Observatory (LHAASO): the **cosmic-ray (CR) proton spectrum at the "knee"** and the **Galactic diffuse gamma-ray emission**.The "knee" in the cosmic ray spectrum (around a few PeV) is thought to mark the maximum energy reached by Galactic CR accelerators. Diffuse gamma-ray emission, primarily from CR

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00:29:55

Magnetars, Supernovae, and FRBs: A Delayed Connection?

Multi-messenger astrophysics ·

2025/06/12

In this episode, we dive into the mysterious world of Fast Radio Bursts (FRBs) and the ongoing quest to understand their origins. We discuss a systematic search for **past supernovae (SNe) and other historical optical transients** at the positions of FRB sources, exploring a leading theory that links FRBs to **magnetars**.The study **found no statistically significant associations** within the 5σ FRB localization uncertainties between the observed CHIME-KKO or literature FRBs and optical transients,

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00:21:02

Beyond Fermi: LST-1 Detects Geminga Pulsar Down to 20...

Multi-messenger astrophysics ·

2025/06/03

In this episode, we discuss a significant new detection of the Geminga pulsar, a middle-aged, radio-quiet gamma-ray pulsar. The **Large-Sized Telescope (LST-1)**, the first of the Cherenkov Telescope Array Observatory (CTAO) Northern Array, has detected Geminga at energies down to 20 GeV.Key takeaways from the study:* The LST-1 detected the Geminga pulsar using 60 hours of data.* The **second emission peak (P2)** of Geminga was detected with a high significance of **12.2σ** in the energy range

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00:11:01

The 44-Minute Pulsar ASKAP J1832−0911 seen in radio...

Multi-messenger astrophysics ·

2025/05/29

Astronomers have made a significant discovery, detecting X-ray emission from a rare type of cosmic object known as a **Long-Period Radio Transient (LPT)** for the very first time.The object, designated **ASKAP J1832−0911**, is extraordinarily bright in radio, reaching flux densities of 10–20 Jy.Crucially, it exhibits **coincident radio and X-ray emission**, both pulsing with a regular period of **44.2 minutes** (2,656.2412 seconds in radio, 2,634 seconds in X-rays). This combination of properties –

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00:16:33

Challenging the Models: New Fermi-LAT Insights into...

Multi-messenger astrophysics ·

2025/05/14

A recent study utilized **15 years of observations** from the **Fermi Large Area Telescope (LAT)** to analyze the gamma-ray emission from the Sun in its quiet state, meaning when it's not flaring. This is the first study to separately analyze the flux variation of the two distinct components of this quiet-state gamma-ray emission over solar cycles.According to theoretical understanding, the Sun's steady-state gamma-ray emission arises from interactions with Galactic cosmic rays (CRs). There

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00:08:01

PeV Power from Stellar Explosions: The Role of Dense...

Multi-messenger astrophysics ·

2025/05/03

The research investigates **how supernovae exploding into dense circumstellar environments, specifically those with dense shells of material, can potentially accelerate particles to energies of a few PeV**, thus acting as "PeVatrons" and contributing to the "knee" feature in the cosmic ray spectrum.Supernova remnants (SNRs) have long been considered prime candidates for the sources of Galactic Cosmic Rays (CRs) up to energies of a few PeV. However, despite decades of gamma-ray

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00:22:32

The HAWC Observatory peering into the Extreme...

Multi-messenger astrophysics ·

2025/03/31

The research presents **new observations of the gamma-ray binary system LS 5039 using the High Altitude Water Cherenkov (HAWC) observatory**, revealing significant insights into the nature of this high-energy source.One of the most striking findings is that **HAWC detected gamma rays from LS 5039 extending up to 200 TeV with no apparent spectral cutoff**. This is a crucial extension of previous observations by the High Energy Stereoscopic System (H.E.S.S.), which had observed the system up to TeV

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