@kevinschawinski
ETH black hole group
Grüp Bœgg Negar Politecnic da Zürig
Artificial Intelligence meets Data Driven Astrophysics
Kevin Schawinski
Institute for Particle Physics and Astrophysics ETH Zurich
Artificial Intelligence meets Data Driven Astrophysics Kevin - - PowerPoint PPT Presentation
Artificial Intelligence meets Data Driven Astrophysics Kevin Schawinski Institute for Particle Physics and Astrophysics ETH Zurich ETH black hole group @kevinschawinski Grp Bgg Negar Politecnic da Zrig how can machine learning/
@kevinschawinski
ETH black hole group
Grüp Bœgg Negar Politecnic da Zürig
Kevin Schawinski
Institute for Particle Physics and Astrophysics ETH Zurich
early 2020s, 20 TB/night
mid 2020s, 160 TB/second
λ - wavelength at which you observe D - diameter of your telescope aperture
Original Image Degraded Image Artificial Degrading
Data Prep. Training of GAN
Recovered Image Generator Original Image Discriminator (Original Image, Degraded Image) or (Recovered Image, Degraded Image)
Schawinski+17
degraded GAN recovered deconvolved PSF=2.5”, 10σ
Schawinski+17
low-resolution radio data NVSS survey high resolution ground truth FIRST survey GAN prediction
Semester project Nina Glaser Glaser et al. in prep.
Training Architecture Discriminator Generator Preprocessing Recovered Original Original + AGN
PSFGAN, Stark+ in press
Dominik Stark
PSFGAN, Stark+ in press
GAN performance vesus SOTA parametric fitting tool GALFIT
Less sensitive to PSF changes
PSFGAN, Stark+ in press
PSFGAN, Stark+ submitted
Less sensitive to training set
Dennis Turp
Encoder-decoder structure with a domain adversarial aspect
Fader network, Lample+17
Encoder-decoder structure with a domain adversarial aspect
Hypothesis generation
where we are where we want to get to
where we are where we want to get to
changing SSFR in latent space changing bulge-to-disk in latent space
go to space.ml to try out our projects!