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Possible Science Cases with the HSC Medium band filters
Possible Science Cases with the HSC Medium band filters
Lyman Break Galaxy (LBG) / Lyman Alpha Emitter (LAE)
Weak Lensing
CMB Lensing
Intrinsic Alignment
Galaxy clustering with photometric redshift
Strong lensing
Mock simulations
Training set construction
Calibration methodology for Rubin, Roman and Euclid
SED reconstruction
Chromatic PSF calibration field for Euclid
AGN variability
Machine Learning for AGN classification
Type I - Type II AGNs
Low luminosity AGNs
Dual AGNs
Quasars
High-z galaxies (JWST, JADES, SPHEREx)
Galaxy-halo connection
Galaxy quenching
Galaxy physical properties
ML for galaxy classification
Simulations
Cluster cosmology
Proto clusters
Splashback radius
Galaxy evolution in dense environments
Strong lensing
Galaxy distribution around clusters
Large Scale Structure and Cosmic Web
Baryonic effects
Stellar Population Studies
Stellar Atmosphere Characterization
Exoplanet Characterization
Circumstellar Disks and Planet Formation
Debris Disks
Variable Stars and Transients
Stellar Populations and Ages
Galactic Structure and Morphology
Low-z galaxies
Dwarf galaxies
Satellite galaxies
Co-evolution of large galaxies and their neighbours
We very much welcome any other science cases which will be available using the HSC medium band filters.
More detailed Info about the Proposal
More detailed Info about the Proposal
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