Intermediate-redshift galaxies show systematically higher dust attenuation at fixed star formation rate surface density than local galaxies, with the excess strongest for galaxies below the star-forming main sequence.
Title resolution pending
9 Pith papers cite this work. Polarity classification is still indexing.
9
Pith papers citing it
representative citing papers
Fast-rotating green valley galaxies maintain higher metallicities than slow-rotating ones because slow rotators experience stronger outflows and more mergers that deplete their chemical content.
Empirical aperture corrections for SDSS absorption indices, derived via CALIFA simulations, reach 15% of dynamical range at low redshift and reduce overestimates of old galaxy fractions by up to 10%.
Void galaxies show modestly higher star formation rates in early spirals and outer disks, lower extinction, and higher gas-fraction proxies than matched galaxies in filaments and walls, suggesting slower quenching in underdense environments.
Neural network derives LAMOST instrumental profiles from arc lamps and reduces RV dispersion by ~3 km/s.
X-ray AGN fraction increases with central star formation rate density in local galaxies, supporting coeval black hole and galaxy growth with only modest time-averaged AGN feedback effects.
Green valley galaxies live preferentially in the outskirts of galaxy clusters as satellites, consistent with environmental quenching processes.
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.
Observational proposal to obtain rest-frame optical stellar kinematics at z~2 with E-ELT to study bulge-disk continuum and co-evolution of mass, kinematics, and star formation.
citing papers explorer
-
The MAGPI Survey: Evidence for Non-Universal Resolved Dust Attenuation Relations Beyond the Local Universe
Intermediate-redshift galaxies show systematically higher dust attenuation at fixed star formation rate surface density than local galaxies, with the excess strongest for galaxies below the star-forming main sequence.
-
Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
Fast-rotating green valley galaxies maintain higher metallicities than slow-rotating ones because slow rotators experience stronger outflows and more mergers that deplete their chemical content.
-
Correcting the fiber-aperture bias affecting galaxy stellar populations in the Sloan Digital Sky Survey. Aperture corrections to absorption indices based on CALIFA integral field observations
Empirical aperture corrections for SDSS absorption indices, derived via CALIFA simulations, reach 15% of dynamical range at low redshift and reduce overestimates of old galaxy fractions by up to 10%.
-
The CAVITY project. The spatially resolved SFR of galaxies in voids
Void galaxies show modestly higher star formation rates in early spirals and outer disks, lower extinction, and higher gas-fraction proxies than matched galaxies in filaments and walls, suggesting slower quenching in underdense environments.
-
Characterizing the Instrumental Profile of LAMOST
Neural network derives LAMOST instrumental profiles from arc lamps and reduces RV dispersion by ~3 km/s.
-
Investigating central star formation in local AGN host galaxies: is there tension between coeval growth and AGN feedback?
X-ray AGN fraction increases with central star formation rate density in local galaxies, supporting coeval black hole and galaxy growth with only modest time-averaged AGN feedback effects.
-
Cluster-green galaxy correlations: where do these galaxies live?
Green valley galaxies live preferentially in the outskirts of galaxy clusters as satellites, consistent with environmental quenching processes.
-
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.
-
Morpho-kinematic of galaxies at cosmic noon
Observational proposal to obtain rest-frame optical stellar kinematics at z~2 with E-ELT to study bulge-disk continuum and co-evolution of mass, kinematics, and star formation.