| Date |
Speaker 1 |
Speaker 2 |
| Jul 28 |
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| Jul 21 |
Ken Nagamine (Osaka University): TBA |
Ralf Konietzka (CfA): TBA |
| Jul 14 |
Pranav Satheesh (Florida): TBA |
|
| Jul 7 |
Azadeh Maleknejad (Swansea University): TBA |
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| Jun 30 |
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| Jun 23 |
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| Jun 16 |
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| Jun 9 |
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| Jun 2 |
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| May 26 |
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| May 19 |
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| May 12 |
LOFAR EoR workshop |
LOFAR EoR workshop |
| May 5 |
|
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| Apr 28 (A006) |
Chris Lovell (Cambridge): Efficiently emulating distribution functions in gigaparsec volumes for varying cosmological parameters |
|
| Apr 21 |
Talia O'Shea (U Wisconsin Madison): Differentiating direct and preventative AGN jet feedback via jet deceleration |
|
| Apr 14 |
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| Apr 7 |
Kai Wu (Heidelberg): Multi-scale Stellar Dynamics in Dense Clusters: From Planetary Debris to Black Hole Seeds |
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| Mar 31 |
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| Mar 24 |
Why do we do astrophysics in the era of AI? (Part I) |
Why do we do astrophysics in the era of AI? (Part II) |
| Mar 17 (A006) |
Sophie Vogt (USM): Understanding nDGP gravity with galaxy clusters - constraints from SPTx(DES+HST) with Planck CMB |
Phil Hopkins (Caltech): TBA |
| Mar 10 |
FACHBEIRAT |
FACHBEIRAT |
| Mar 3 |
Linda Blot (IPMU): Detecting dark energy perturbations in the large-scale structure of the Universe |
Adriaan Duivenvoorden (MPA): Robust CMB B-mode analysis with simulation-based inference |
| Feb 24 |
Daniel Gruen (USM): DES-y6 3x2pt results (Part I) |
Daniel Gruen (USM): DES-y6 3x2pt results (Part II) |
| Feb 17 |
Ken Osato (Chiba University): Multi-wavelength Full-sky Cosmological Simulations for Stage-IV Surveys |
Agustina Colazo (Cordoba): Probing galaxy-halo alignments across cosmic time with IllustrisTNG |
| Feb 10 |
IMPRS Symposium |
IMPRS Symposium |
| Feb 3 |
Erin Hayes (Cambridge): Time-Delay Cosmography in the Era of LSST: Estimating Precise Time Delays for Gravitationally Lensed Supernovae with Gaussian Processes |
|
| Jan 27 |
Mahlet Shiferaw (Stanford): How do Uncertainties in Galaxy Formation Physics Impact Field-Level Galaxy Bias? |
|
| Jan 22 (Thursday) |
Evan Saraivanov (Stony Brook): 2-loop EFT Power Spectrum and Application to Roman Cosmic Shear |
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