Splinter Meeting JungeAG

junge AG / young AG

Time: Tuesday September 10, 14:00-16:30 CEST (UTC+2)

Room: S25

Convenor(s): Sabina Bahic [1], Steven Hämmerich [2], Markus Hundertmark [3]
[1] AIP, Potsdam, [2] Dr. Karl Remeis Sternwarte Bamberg & ECAP (FAU), [3] ZfA Uni Heidelberg

The Junge AG splinter meeting provides a forum for young astronomers. Established 2020 we would like to consider all students and early postdocs as members of the Junge AG, regardless of their actual age. Young members in this sense who would like to talk about their thesis or ongoing projects and have not found a suitable slot or prefer to talk to a different audience are invited to present. Submitted talks should be between 10 and 15 minutes long. The winner of the Jugend forscht award will also be invited to present.

Program

Tuesday September 10, 14:00-16:30 junge AG / young AG (S25)

14:05  Anna Gebhardt:
Spectrophotometric investigations of hot subdwarf stars in the Plato field with Gaia DR3

14:18  Harvey Stemmler:
A spectral analysis of hot stars in a search for OB-binaries

14:31  Sebastian Weich:
Investigation of the Interstellar Medium by Using the Light of Hot Subdwarf Stars

14:44  Lennard Kufleitner:
Spectroscopic analysis of hot subluminous stars from the Hamburg Quasar Survey: New atmospheric- and stellar parameters

14:57  Lukas Stock:
How to use inexpensive echelle spectrographs at your own observatory

15:10  Mauritz Wicker:
Unveiling Hidden Milky Way Objects through Gaia Microlensing Events and the Besançon Galaxy Model

15:23  Nick Horstmann:
The Large Magellanic Cloud in S-Band: Literature Review, Full Sky Simulations, and New SKAMPI Observations

15:36  Mattia Pacicco:
MHD simulations of the Local Bubble

15:49  Kamalpreet Kaur:
Exploring Radio Point Sources in the Galactic Center using S Band of MeerKAT

16:02  Pranav Limaye:
Long-term Statistical Study of an Active Repeating Fast Radio Burst using the Effelsberg 100-m Radio Telescope

16:15  Xueying Zheng:
eROSITA narrowband maps at the energies of soft X-ray emission lines

16:28  Polina Smirnova:
Machine learning analysis of supernova remnant simulations

Related contributions

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