AstroSem - The Astro-Seminar

Organiser: Emilio Romano-Diaz

Information for the SS2025

Welcome to the four-credit-point Seminar on Astronomy and Astrophysics (astro830) in the Master of Astrophysics program at the Argelander-Institute for Astronomy.

In this course, students will present a talk based on a recently published research paper selected by professors and research staff at the AIfA.  Students must discuss the research topic, the paper content, and their presentation with their respective supervisors before their presentation.

Time: Mondays, 14.00-15:15 when two talks or 13:45-15:30 when three talks,
Place: Lecture Hall 0.012, AIfA.

The AstroSem introductory session will be on Monday 14.04.25 at 14.00, where the papers will be briefly introduced (list below). Students shall have a close look at them in the following days and express their interest in two papers via email to the respective supervisors by Friday, April 18th. The papers will assigned after that date.

The talks will be scheduled for a date after the registration deadline of 28.04.2025. The first presentations will take place on 05.05.2025
The latest date available for scheduling a talk this semester is 14..07.2025. 

Students (and advisors) are strongly recommended to read the guidelines.  Do also read the guides to good seminar talks linked below!

Please register on basis for this seminar course: the registration and de-registration deadlines 20.04.2025. Late registrations will not be possible! 

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Studium / Lectures © COLOURBOX

Papers:

Supersivor:

Not available:

Student:

Date:

Cloud-cloud collisions in the Antennae galaxies: Does high-speed collision suppress star formation?

Zein Bazzi

26/05, 02/06

Jendrik Sievers

19/05

Evolution of Primordial Magnetic Fields during Large-scale Structure Formation

Prof. Jennifer Schober    

Vasco Silver

26/05

The hot gas mass fraction in halos.
From Milky Way-like groups to massive clusters

Prof. Andrina Nicola

Yinghua Huang

26/05

Fire and Ice in the Whirlpool: Spatially Resolved Scaling Relations between X-Ray-emitting Hot Gas and Cold Molecular Gas in M51

Dr. Mallory Thorpe

19/05, 26/05, 23/06, 7/07, 14/07

Patrick Lenz

2/06

Morphology and Kinematics of the Gas in M51: How Interaction with NGC 5195 Has Molded the Structure of Its Arms

Ina Galic

Amarilli Rutigliano

2/06

Nonstop Variability of Sgr A* Using JWST at 2.1 and 4.8 μm Wavelengths: Evidence for Distinct Populations of Faint and Bright Variable Emission

Dr. Gunther Witzel

Yanhanle Zhao

16/06

Dynamical Dark Energy in light of the DESI DR2 Baryonic Acoustic Oscillations Measurements

Prof. Cristiano Porciani

Rishabh Ranjan

16/06

Three-Dimensional Stacking as a Line Intensity Mapping Statistic

Christos Karoumpis

Do stars still form in molecular gas within CO-dark dwarf galaxies?

Dr. Emilio Romano-Diaz
Quantifying Baryonic Feedback on the Warm–Hot Circumgalactic Medium in CAMELS Simulations Dr. Reza Ayromlou
The diverse star formation histories of early massive, quenched galaxies in modern galaxy formation simulations Dr. Reza Ayromlou

Witnessing the onset of reionization through Lyman-α emission at redshift 13

Ankur Dev 2/06, 9/06, 16/06

The critical role of dark matter halos in driving star formation

Dr. Dario Colombo

The Moving Lens Effect: Simulations, Forecasts and Foreground Mitigation

Dr. Kaustuv Basu 5/05, 16/05, 23/06

Impact of Weak Lensing Mass Mapping Algorithms on Cosmology Inference

Dr. Lucas Porth

Principal Components for Model-Agnostic Modified Gravity with 3x2pt

Dr. Matteo Cataneo 28/04, 12/05, 26/05, 9/06, 23/06, 7/07, 21/07

What Drives Cluster Cool-Core Transformations? A Population Level Analysis of TNG-Cluster

Prof. Thomas Reiprich


Contact:

Avatar Romano-Diaz

Emilio Romano-Diaz

Avatar Bertoldi

Frank Bertoldi

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