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Star formation scaling relations at ~100 pc from PHANGS: Impact of completeness and spatial scale
I. Pessa, E. Schinnerer, F. Belfiore +31
Aims: The complexity of star formation at the physical scale of molecular clouds is not yet fully understood. We investigate the mechanisms regulating the formation of stars in dif…
PHANGS-HST: Star Cluster Spectral Energy Distribution Fitting with CIGALE
Jordan A. Turner, Daniel A. Dale, Janice C. Lee +24
The sensitivity and angular resolution of photometric surveys executed by the Hubble Space Telescope (HST) enable studies of individual star clusters in galaxies out to a few tens…
The PHANGS-HST Survey: Physics at High Angular resolution in Nearby GalaxieS with the Hubble Space Telescope
Janice C. Lee, Bradley C. Whitmore, David A. Thilker +51
The PHANGS program is building the first dataset to enable the multi-phase, multi-scale study of star formation across the nearby spiral galaxy population. This effort is enabled b…
Measuring the mixing scale of the ISM within nearby spiral galaxies
Kathryn Kreckel, I-Ting Ho, Guillermo A. Blanc +28
The spatial distribution of metals reflects, and can be used to constrain, the processes of chemical enrichment and mixing. Using PHANGS-MUSE optical integral field spectroscopy, w…
Kinematic signatures of nuclear discs and bar-driven secular evolution in nearby galaxies of the MUSE TIMER project
Dimitri A. Gadotti, Adrian Bittner, Jesus Falcon-Barroso +13
The central regions of disc galaxies hold clues to the processes that dominate their formation and evolution. The TIMER project has obtained high signal-to-noise and spatial resolu…
Constraining stellar population parameters from narrow band photometric surveys using convolutional neural networks
Choong Ling Liew-Cain, Daisuke Kawata, Patricia Sanchez-Blazquez +2
Upcoming large-area narrow band photometric surveys, such as J-PAS, will enable us to observe a large number of galaxies simultaneously and efficiently. However, it will be challen…