AstroSem - The Astro-Seminar

Module astro830

Organiser: Emilio Romano-Diaz

Information for the WS2024

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 14.10.24 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, October 18th. The papers will assigned after that date.

The talks will be scheduled for a date after the registration deadline of 31.10.2024. The first presentations will take place on November 11th.
The latest date available for scheduling a talk this semester is 27.01.2025. 

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 October 31st and November 7th. Late registrations will not be possible! 

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Studium / Lectures © COLOURBOX

Papers:

Supersivor:

Not available:

Student:

Date:

Growth of Light-Seed Black Holes in Gas-Rich Galaxies at High Redshift

Prof. Cristiano Porciani

Pantho Chakraborty

11/11/2024

 Runaway OB Stars in the Small Magellanic Cloud. III. Updated Kinematics and Insights into Dynamical versus Supernova Ejections

Dr. Abel Schootemeijer

24/02/2025

Erik Stehr

18/11/2024

SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model

Christos Karoumpis

Stefanos Lialios

18/11/2024

Evolutionary growth of molecular clouds as traced by their infrared bright fraction Dr. Dario Colombo Vikalp Sharma 18/11/2024
Two waves of massive stars running away from the young cluster R136 Dr. Abel Schootemeijer 24/02/2025 Lorenzo Breuer 25/11/2024

First Step Towards Matter Power Spectrum Reconstruction with Stage-III Weak Gravitational Lensing Surveys

Dr. Lucas Porth

11-18/11/24

2-9-16-23/12/24

6-13-27/01/25

Lena Schürmann 25/11/2024

Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum

Dr. Lucas Porth

11-18/11/24

2-9-16-23/12/24

6-13-27/01/25

Elyas Farah 25/11/2024
Polarized signatures of adiabatically expanding hotspots in Sgr A*’s accretion flow Dr. Gunther Witzel Zhengxu Hou 02/12/2024

The MAGPI survey: evolution of radial trends in star formation activity across cosmic time

Dr. Mallory Thorp

11/11/2024

18/11/2024

Philipp Siebold 02/12/2024

The warm-hot intergalactic medium (WHIM) in inter-cluster filaments - A forecast for HUBS observations based on eRASS1 superclusters

Prof. Thomas Reiprich

18/11/2024

20/01/2025

Sravan Krishnan Perinthatta Eettisseri 02/12/2024
COMAP Early Science. VIII. A Joint Stacking Analysis with eBOSS Quasars Christos Karoumpis Dinesh Maheswari Vaittinadane 09/12/2024
Turbulent Pressure Heats Gas and Suppresses Star Formation in Galactic Bar Molecular Clouds Prof. Frank Bigiel

25/11/2024

02,16/12/2024

20/01/2025

Varun Sohanda 09/12/2024
Prevention is better than cure? Feedback from high specific energy winds in cosmological simulations with Arkenstone Dr. Nastasha Wijers Felicitas Freche 09/12/2024
The hot circumgalactic medium in the eROSITA All-Sky Survey I. X-ray surface brightness profiles Prof. Thomas Reiprich

18/11/2024

20/01/2025

Amanda Sabovic 16/12/2024
REBELS-25: Discovery of a dynamically cold disc galaxy at z = 7.31 Dr. Emilio Romano-Diaz 11-18-25/11/2024 Rita Reis 16/12/2024

Relight the Candle: What happens to High Redshift Massive Quenched Galaxies

Dr. M. Reza Ayromlou

02/12/2024

23/12/2024

Eirini Rodiou 16/12/2024

Evidence for large baryonic feedback at low and intermediate redshifts from kinematic Sunyaev-Zel'dovich observations with ACT and DESI photometric galaxies

Prof. Andrina Nicola

Diana Lopez Navarro 13/01/2025

DESI Peculiar Velocity Survey -- Fundamental Plane

Dr. Alexander Eggemeier

20/01/2025

Antonio Buzza 13/01/2025

Clusters, clouds, and correlations: relating young clusters to giant molecular clouds in M33 and M31

Dr. Hao He

18-25/11/2024

20-27/01/2024

Cosme Aquino Ovelar 13/01/2025

JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H0

Dr. Florian Pacaud

Anna Vervelaki 20/01/2025

Psi-GAN: A power-spectrum-informed generative adversarial network for the emulation of large-scale structure maps across cosmologies and redshifts

Dr. Robert Reischke

Sviatoslav Khukhlaev 20/01/2025

High-Precision Galaxy Clustering Predictions from Small-Volume Hydrodynamical Simulations via Control Variates

Dr. Alexander Eggemeier

20/01/2024

Marek Majoch 27/01/2025

The MillenniumTNG Project: semi-analytic galaxy formation models on the past lightcone

Dr. M. Reza Ayromlou​

02/12/2024

23/12/2024

Aleyna Döven 27/01/2025

Foreground removal and angular power spectrum estimation of 21 cm signal using harmonic space ILC method

Dr. Kaustuv Moni Basu

The Moving Lens Effect: Simulations, Forecasts and Foreground Mitigation

Dr. Kaustuv Moni Basu

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

Dr. Emilio Romano-Diaz

11-18-25/11/2024

Rapid Methods for Modeling Overdensities of Massive Neutrinos and Other Non-Cold Relics Prof. Cristiano Porciani
Stage IV baryonic feedback correction for non-Gaussianity inference Dr. Robert Reischke
CHEX-MATE: A non-parametric deep learning technique to deproject and deconvolve galaxy cluster X-ray temperature profiles Dr. Florian Pacaud

Contact:

Avatar Romano-Diaz

Emilio Romano-Diaz

Avatar Bertoldi

Frank Bertoldi

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