Page History
Upcoming JC
Title:
Revisiting the Hβ Size-Luminosity Relation Using a Uniform Reverberation-Mapping AnalysisTBC
Speaker
Speaker: Daryl
Summary: TBC
Past JC
Title:
Rising from the ashes: evidence of old stellar populations and rejuvenation events in the very early Universe.A 3D view on the local gravitational instability of cold gas discs in star-forming galaxies at 0 ≲ z ≲ 5
Speaker: Stavros
Title: A Cosmic Miracle: A Remarkably Luminous Galaxy at zspec=14.44 Confirmed with JWST
Speaker: Jean-Baptiste
Title: Bar ages derived for the first time in nearby galaxies: Insights on secular evolution from the TIMER sample
Speaker: Letizia
Title: Galaxy Zoo CEERS: Bar fractions up to z~4.0
Speaker: Capucine
Title: The dawn of disks: unveiling the turbulent ionised gas kinematics of the galaxy population at z∼4−6 with JWST/NIRCam grism spectroscopy
Speaker: Claudia
Title: Seoul National University AGN Monitoring Project. V. Velocity-resolved Hβ Reverberation Mapping and Evidence of Kinematics Evolution
Speaker: Daryl
Title: JWST's little red dots: an emerging population of young, low-mass AGN cocooned in dense ionized gas
Speaker: Jianhang
Title: Euclid Quick Data Release (Q1) - Data release overview
Speaker: Yixian
Title: Optical+NIR analysis of a newly found Einstein ring at z∼1 from the Kilo-Degree Survey: Dark matter fraction, total and dark matter density slope and IMF
Speaker: Juan
Title: Dominant Role of Coplanar Inflows in Driving Disk Evolution Revealed by Gas-phase Metallicity Gradients
Speaker: Lilian
Title: Estimating Black Hole Masses in Obscured AGN from X-ray and Optical Emission Line Luminosities
Speaker: Giulia
Title: Feedback and dynamical masses in high-z galaxies: the advent of high-resolution NIRSpec spectroscopy
Speaker: Eleonora
Title: Less Wound and More Asymmetric: JWST Confirms the Evolution of Spiral Structure in Galaxies at z≲3
Speaker: Jean-Baptiste
Title: Clumps as multiscale structures in Cosmic Noon galaxies
Speaker: Capucine
Title: Comparison of bar formation mechanisms I: does a tidally-induced bar rotate slower than an internally-induced bar?
Speaker: Stavros
Title: Another piece to the puzzle: radio detection of a JWST discovered AGN candidate
Speaker: Daryl
2024
Speaker: Jianhang
Summary: TBC
Title: MIDIS. Near-infrared rest-frame morphology of massive galaxies at 3<z<5.5 in the Hubble eXtreme Deep Field
Speaker: Lilian
Summary: TBC
Title: The Structure of Massive Star-Forming Galaxies from JWST and ALMA: Dusty, High Redshift Disk Galaxies
Speaker: Shangguan
Summary: TBC
Title: JWST meets Chandra: a large population of Compton thick, feedback-free, and X-ray weak AGN, with a sprinkle of SNe
Speaker: Taro
Summary: TBC
Title: Molecular gas kinematics in local early-type galaxies with ALMA
Speaker: Yixian
Summary: TBC
Title: Calibrating non-parametric morphological indicators from JWST images for galaxies over 0.5<z<3
Speaker: Capucine
Summary: TBC
Title: EPOCHS Paper V. The dependence of galaxy formation on galaxy structure at 𝑧 < 7 from JWST observations
Speaker: Claudia
Summary: TBC
Title: FRESCO: The Paschen-α Star Forming Sequence at Cosmic Noon
Speaker: Juan
Summary: See here.
Title:
The rise and fall of bars in disc galaxies from z=1 to z=0. The role of the environment
Detecting a disk bending wave in a barred-spiral galaxy at redshift 4.4
Speaker: Stavros
Summary:
Title: Quantitative analysis of the molecular gas morphology in nearby disk galaxies.
Speaker: Jean-Baptiste
Summary: TBC
Title: GA-NIFS: NIRSpec reveals evidence for non-circular motions and AGN feedback in GN20
Speaker: Giulia
Summary: See here.
Title: Primordial Rotating Disk Composed of ≥15 Dense Star-Forming Clumps at Cosmic Dawn
Speaker: Jianhang
Summary: TBC
Title: The evolution of the SFR and ΣSFR of galaxies in cosmic morning (4<z<10)
Speaker: Lilian
Summary: See here.
Title: Chugunov+2024: Galaxies decomposition with spiral arms - I: 29 galaxies from S4G
Speaker: Yixian
Summary:
1. The authors proposed a new 2D model with 20 parameters to describe a spiral arm.
2. Using their model, they found that spiral arms contribute to 10-25% of the galaxy’s total luminosity. When averaged azimuthally, spiral arms produce a bump at r_gal ~ 1-2 scale length (see the figure).
Title: The evolution of galaxy morphology from redshift z=6 to 3: Mock JWST observations of galaxies in the ASTRID simulation
Speaker: Capucine
Summary: TBC
Title: The MBH−M∗ relation up to z∼2 through decomposition of COSMOS-Web NIRCam images
Speaker: Daryl
Summary: TBC
Title: JWST Reveals a Surprisingly High Fraction of Galaxies Being Spiral-like at $0.5\leq z\leq4$
Speaker: Claudia
Summary: See here2023
Meeting location: MPE IR meeting room and mpeir Zoom (passcode: 123)
Date and time: Every Monday at 13h45
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Q&A:
Q: Where should I look for or suggest papers?
A: MPE IR Benty-fields or in the MPE IR Group Slack channel #galev-interesting-papers
Q: What if I do not have access to MPE IR Benty-fields page or the Slack channel?
A: Send an email to Lilian (lilian[at]mpe.mpg.de)
This page is maintained by Lai Yee Lilian Lee and Claudia Pulsoni . Last updated on 20 July 20246 Jun 2025.
