A SHARP Look at Quenching and Bulge-Disk Growth in Massive Galaxies at Cosmic Noon

Abstract

The physical mechanisms that quench star formation in massive galaxies remain poorly understood. At cosmic noon (1<z<3), when star formation and AGN activity peak, galaxies rapidly evolve from star-forming disks into quiescent, bulge-dominated systems. While quenching correlates with stellar mass and bulge growth, the causal link between bulge assembly, star-formation suppression, and feedback processes remains unclear. Stellar population analysis from spatially resolved spectroscopy of galaxies caught during quenching is crucial to advance on this issue. We show that the SHARP-VESPER Integral-Field Spectrograph (IFS) can efficiently fill this gap by combining ELT-class sensitivity, 31 mas spatial resolution (>3x sharper than JWST) and broad near-IR wavelength coverage with 12-IFU multiplexing. This will enable, for the first time, a simultaneous bulge-disk decomposition of stellar populations and spatially resolved mapping of ionised gas in massive galaxies (log $M_{\ast }/M_{\odot }\ge 11$) at 2.2<z<3.5, targeting systems on the main sequence shortly before quenching or already in the green valley. With typical exposure times of 15 hr, we will obtain S/N>15-20 per spectral resolution element, on the inner bulge, and outer disk extracted spectral continuum, and S/N>5 for nebular lines ([OII], H$\beta$, [OIII], H$\alpha$) on sub-kpc scales. These observations will allow us to reconstruct independent bulge and disk star-formation histories, ages, metallicities, and $\alpha$-enhancements, while mapping spatially resolved star formation, gas kinematics, and feedback-driven outflows. By directly comparing the timing of bulge growth and star-formation suppression across galaxy components, this programme will test whether quenching proceeds inside-out, distinguish fast and slow quenching pathways, and link structural transformation to feedback processes in the most massive galaxies at cosmic noon.

arXiv comment13 pages, 1 figure, published in New Astronomy as part of Special Issue "SHARP Science Book"

References in corpus (93)

• Stellar population synthesis at the resolution of 2003
• Star Formation in Galaxies Along the Hubble Sequence
• The Dust Content and Opacity of Actively Star-Forming Galaxies
• A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
• The Demography of Massive Dark Objects in Galaxy Centres
• Cosmic Star Formation History
• The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
• How Do Galaxies Get Their Gas?
• Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
• Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
• Cold streams in early massive hot haloes as the main mode of galaxy formation
• Galaxy Harassment and the Evolution of Clusters of Galaxies
• The reversal of the star formation-density relation in the distant universe
• Multiwavelength study of massive galaxies at z~2. I. Star formation and galaxy growth
• A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
• 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since $z=3$
• The ages and metallicities of galaxies in the local universe
• The SINS survey: SINFONI Integral Field Spectroscopy of z ~ 2 Star-forming Galaxies
• Virial shocks in galactic haloes?
• Mass assembly in quiescent and star-forming galaxies since z=4 from UltraVISTA
• Formation of Massive Galaxies at High Redshift: Cold Streams, Clumpy Disks and Compact Spheroids
• A Physical Model for the Co-evolution of QSOs and of their Spheroidal Hosts
• Galaxy bimodality versus stellar mass and environment
• Passively Evolving Early-type Galaxies at 1.4<z<2.5 in the Hubble Ultra Deep Field
• The Herschel view of the dominant mode of galaxy growth from z=4 to the present day
• Morphological quenching of star formation: making early-type galaxies red
• Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms
• Confirmation of the remarkable compactness of massive quiescent galaxies at z~2.3: early-type galaxies did not form in a simple monolithic collapse
• Galaxy Structure and Mode of Star Formation in the SFR-Mass Plane from z ~ 2.5 to z ~ 0.1
• De Re Metallica: The cosmic chemical evolution of galaxies
• The SINS survey of z~2 galaxy kinematics: properties of the giant star forming clumps
• A Catalog of Bulge+Disk Decompositions and Updated Photometry for 1.12 Million Galaxies in the Sloan Digital Sky Survey
• From rings to bulges: evidence for rapid secular galaxy evolution at z~2 from integral field spectroscopy in the SINS survey
• Strangulation as the primary mechanism for shutting down star formation in galaxies
• The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7
• A Spectroscopic Catalog of 10 Distant Rich Clusters of Galaxies
• Wet Disc Contraction to Galactic Blue Nuggets and Quenching to Red Nuggets
• SINFONI Integral Field Spectroscopy of z~2 UV-selected Galaxies: Rotation Curves and Dynamical Evolution
• The Secular Evolution of Disk Structural Parameters
• Mass and Environment as Drivers of Galaxy Evolution II: The quenching of satellite galaxies as the origin of environmental effects
• Stellar Population Diagnostics of Elliptical Galaxy Formation
• Early Evolution of Disk Galaxies : Formation of Bulges in Clumpy Young Galactic Disks
• The Confinement of Star-Forming Galaxies into a Main Sequence through Episodes of Gas Compaction, Depletion, and Replenishment
• Multiwavelength study of massive galaxies at z~2. II. Widespread Compton thick AGN and the concurrent growth of black holes and bulges
• Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
• The Main Sequence of star-forming galaxies across cosmic times
• Evidence for Mature Bulges and an Inside-out Quenching Phase 3 Billion Years After the Big Bang
• Mass downsizing and "top-down" assembly of early-type galaxies
• Bulge mass is king: The dominant role of the bulge in determining the fraction of passive galaxies in the Sloan Digital Sky Survey
• Gas Physics, Disk Fragmentation, and Bulge Formation in Young Galaxies
• The SINS/zC-SINF survey of z~2 galaxy kinematics: SINFONI adaptive optics-assisted data and kiloparsec-scale emission line properties
• A substantial population of massive quiescent galaxies at z~4 from ZFOURGE
• MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. II - Star Formation Histories and Galaxy Quenching
• Evidence for Wide-Spread AGN Driven Outflows in the Most Massive z~1-2 Star Forming Galaxies
• The KMOS^3D Survey: Demographics and Properties of Galactic Outflows at z = 0.6 - 2.7
• Post-starburst galaxies: more than just an interesting curiosity
• A Census of Optical and Near-Infrared Selected Star-Forming and Passively Evolving Galaxies at Redshift Z~2
• The SINS/zC-SINF survey of z~2 galaxy kinematics: Evidence for powerful AGN-driven nuclear outflows in massive star-forming galaxies
• Charting the evolution of the ages and metallicities of massive galaxies since z=0.7
• On the estimation of galaxy structural parameters: the Sersic Model
• Fast, Slow, Early, Late: Quenching Massive Galaxies at z~0.8
• The Morphologies of Massive Galaxies at 1<z<3 in the CANDELS-UDS Field: Compact Bulges, and the Rise and Fall of Massive Disks
• Green Valley Galaxies
• On the origin of the galaxy luminosity function
• Dust attenuation, bulge formation and inside-out cessation of star-formation in Star-Forming Main Sequence galaxies at z~2
• Star formation quenching in massive galaxies
• A Consistent Study of Metallicity Evolution at 0.8 < z < 2.6
• Galaxy And Mass Assembly (GAMA): ${\mathcal{M}}_{\star }-R_{\mathrm{e}}$ relations of $z=0$ bulges, discs and spheroids
• The connection between galaxy structure and quenching efficiency
• Black hole growth and starburst activity at z = 0.6-4 in the Chandra Deep Field South. Host galaxies properties of obscured AGN
• Fast and slow paths to quiescence: ages and sizes of 400 quiescent galaxies from the LEGA-C survey
• Relationship between star formation rate and black hole accretion at z=2: The different contributions in quiescent, normal and starburst galaxies
• A catalog of polychromatic bulge-disk decompositions of ~ 17.600 galaxies in CANDELS
• The host galaxies of X-ray selected Active Galactic Nuclei to z=2.5: Structure, star-formation and their relationships from CANDELS and Herschel/PACS
• SDSS-IV MaNGA: Inside-out vs. outside-in quenching in different local environments
• GASP XXIV. The history of abruptly quenched galaxies in clusters
• Rejuvenated galaxies with very old bulges at the origin of the bending of the main sequence and of the "green valley"
• Coincidence between morphology and star-formation activity through cosmic time: the impact of the bulge growth
• Constraining the star formation and the assembly histories of normal and compact early-type galaxies at 1<z<2
• Galaxy And Mass Assembly (GAMA): Understanding the wavelength dependence of galaxy structure with bulge-disc decompositions
• The Effects of Mergers on the Formation of Disc-Bulge Systems in Hierarchical Clustering Scenarios
• Rapid Quenching of Galaxies at Cosmic Noon
• HST grism spectroscopy of z~3 massive quiescent galaxies: Approaching the metamorphosis
• A duality in the origin of bulges and spheroidal galaxies
• High-velocity outflows in massive post-starburst galaxies at z > 1
• A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass and age from $\text{z}=0.6$ to $\text{z}=1.3$
• Star formation and quenching among the most massive galaxies at z~1.7
• VIMOS Public Extragalactic Redshift Survey (VIPERS). The distinct build-up of dense and normal massive passive galaxies
• Stellar populations, stellar masses and the formation of galaxy bulges and discs at $z<3$ in CANDELS
• The MUSE view of ram pressure stripped galaxies in clusters: the GASP sample
• DAWN JWST Archive: Morphology from profile fitting of over 340 000 galaxies in major fields
• Re-assessing the stellar population scaling relations of the galaxies in the Local Universe