VAR-PZ uses DRW-modeled variability to create photo-z priors that reduce catastrophic outliers in AGN redshift estimates from 32% to below 7% when combined with SED fitting, validated on SDSS data and LSST simulations.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
verdicts
UNVERDICTED 3representative citing papers
IllustrisTNG simulations link filament density to galaxy morphology trends across redshifts and predict that Roman's planned HLWAS survey needs greater depth to accurately map the z=1 cosmic web.
The FOBOS proposal describes a high-multiplex fiber spectrograph for Keck II offering 1.7 times the survey speed of PFS and greater sampling density for deep spectroscopic follow-up of panoramic imaging surveys.
citing papers explorer
-
VAR-PZ: Constraining the Photometric Redshifts of Quasars using Variability
VAR-PZ uses DRW-modeled variability to create photo-z priors that reduce catastrophic outliers in AGN redshift estimates from 32% to below 7% when combined with SED fitting, validated on SDSS data and LSST simulations.
-
Impact of Cosmic Filaments on Galaxy Morphological Evolution and Predictions of Early Cosmic Web Structure for Roman
IllustrisTNG simulations link filament density to galaxy morphology trends across redshifts and predict that Roman's planned HLWAS survey needs greater depth to accurately map the z=1 cosmic web.
-
FOBOS: A Next-Generation Spectroscopic Facility at the W. M. Keck Observatory
The FOBOS proposal describes a high-multiplex fiber spectrograph for Keck II offering 1.7 times the survey speed of PFS and greater sampling density for deep spectroscopic follow-up of panoramic imaging surveys.