GLACE survey: galaxy activity in ZwCl0024+1652 cluster from strong optical emission lines

Abstract

Although ZwCl0024+1652 galaxy cluster at $z\sim 0.4$ has been thoroughly analysed, it lacks a comprehensive study of star formation and nuclear activity of its members. With GaLAxy Cluster Evolution (GLACE) survey, a total of 174 H$\alpha$ emission-line galaxies (ELGs) were detected, most of them having [NII}]. We reduced and analysed a set of [OIII] and H$\beta$ tunable filter (TF) observations within GLACE survey. Using H$\alpha$ priors, we identified [OIII] and H$\beta$ in 35 ($\sim$20%) and 59 ($\sim$34%) sources, respectively, with 21 of them having both emission lines, and 20 having in addition [NII]. Applying BPT-NII diagnostic diagram, we classified these ELGs into 40% star-forming (SF), 55% composites, and 5% LINERs. Star formation rate (SFR) measured through extinction corrected H$\alpha$ fluxes increases with stellar mass (${\mathrm{M}}_{\ast }$), attaining its peak at ${\mathrm{M}}_{\ast }\sim 10^{9.8}{\mathrm{M}}_{\odot }$. We observed that the cluster centre to $\sim$1.3Mpc is devoid of SF galaxies and AGN. Our results suggest that the star formation efficiency declines as the local density increases in the cluster medium. Moreover, the SF and AGN fractions drop sharply towards high-density environments. We observed a strong decline in SF fraction in high ${\mathrm{M}}_{\ast }$, confirming that star formation is highly suppressed in high-mass cluster galaxies. Finally, we determined that SFR correlates with ${\mathrm{M}}_{\ast }$ while specific SFR (sSFR) anti-correlates with ${\mathrm{M}}_{\ast }$, both for cluster and field. This work shows the importance and strength of TF observations when studying ELGs in clusters at higher redshifts. We provide with this paper a catalogue of ELGs with H$\beta$ and/or [OIII] lines in ZwCl0024+1652 cluster.

arXiv commentAccepted for publication in MNRAS main journal, 22 pages, 21 figures

References in corpus (141)

• Stellar population synthesis at the resolution of 2003
• Galactic Stellar and Substellar Initial Mass Function
• Star Formation in Galaxies Along the Hubble Sequence
• The Host Galaxies of AGN
• The physical properties of star forming galaxies in the low redshift universe
• Theoretical Modeling of Starburst Galaxies
• The Host Galaxies and Classification of Active Galactic Nuclei
• Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
• Gaia Data Release 2: The astrometric solution
• 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
• Hierarchical Galaxy Formation
• Galaxy Harassment and the Evolution of Clusters of Galaxies
• Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey
• K-corrections and filter transformations in the ultraviolet, optical, and near infrared
• A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
• The Environmental Dependence of the Relations between Stellar Mass, Structure, Star Formation and Nuclear Activity in Galaxies
• Galaxy bimodality versus stellar mass and environment
• Galaxy Star-Formation as a Function of Environment in the Early Data Release of the Sloan Digital Sky Survey
• Observational evidence for AGN feedback in early-type galaxies
• The Origin of Star Formation Gradients in Rich Galaxy Clusters
• Properties of Galaxy Groups in the SDSS: I.-- The Dependence of Colour, Star Formation, and Morphology on Halo Mass
• Old Stellar Populations. VI. Absorption-Line Spectra of Galaxy Nuclei and Globular Clusters
• A comprehensive classification of galaxies in the SDSS: How to tell true from fake AGN?
• Gaia Data Release 1: Astrometry - one billion positions, two million proper motions and parallaxes
• The Importance of Satellite Quenching for the Build-Up of the Red Sequence of Present Day Galaxies
• Theoretical Evolution of Optical Strong Lines across Cosmic Time
• Mass and Environment as Drivers of Galaxy Evolution II: The quenching of satellite galaxies as the origin of environmental effects
• The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z~6.7 selected with 17.5<=i_{AB}<=24.7
• A wide field Hubble Space Telescope study of the cluster CL0024+16 at z=0.4. I: morphological distributions to 5 Mpc radius
• GASP I: Gas stripping phenomena in galaxies with MUSE
• The Gemini Cluster Astrophysics Spectroscopic Survey (GCLASS): The Role of Environment and Self-Regulation in Galaxy Evolution at z ~ 1
• The DEEP2 Galaxy Redshift Survey: The Role of Galaxy Environment in the Cosmic Star-Formation History
• The Environment of AGNs in the Sloan Digital Sky Survey
• BUDHIES II: A phase-space view of HI gas stripping and star-formation quenching in cluster galaxies
• Star Formation in Cluster Galaxies at 0.2<z<0.55
• The Galaxy Content of SDSS Clusters and Groups
• A Wide Field Hubble Space Telescope Study of the Cluster Cl0024+1654 at z=0.4 II: The Cluster Mass Distribution
• Reversal of Fortune: Confirmation of an Increasing Star Formation-Density Relation in a Cluster at z=1.62
• The Era of Star Formation in Galaxy Clusters
• Star formation and AGN activity in SDSS cluster galaxies
• A Wide-field Survey of Two Z~0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s
• Effects of Local Environment and Stellar Mass on Galaxy Quenching out to z~3
• On the evolution and environmental dependence of the star formation rate versus stellar mass relation since z~2
• Discovery of a Ringlike Dark Matter Structure in the Core of the Galaxy Cluster Cl 0024+17
• The Cluster and Field Galaxy AGN Fraction at z = 1 to 1.5: Evidence for a Reversal of the Local Anticorrelation Between Environment and AGN Fraction
• The relation between star formation, morphology and local density in high redshift clusters and groups
• Comparing the relation between star formation and galaxy mass in different environments
• Reconstructing the History of Star Formation in Rich Cluster Cores
• The Colour-Magnitude Relation as a Constraint on the Formation of Rich Cluster Galaxies
• AGNs and galaxy interactions
• LoCuSS: The steady decline and slow quenching of star formation in cluster galaxies over the last four billion years
• A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images. I Method description
• Substructure and dynamical state of 2092 rich clusters of galaxies derived from photometric data
• The Las Campanas/AAT Rich Cluster Survey II: The Environmental Dependance of Galaxy Colours in Clusters at z~0.1
• The IMACS Cluster Building Survey: II. Spectral Evolution of Galaxies in the Epoch of Cluster Assembly
• A Panoramic Halpha Imaging Survey of the z=0.4 cluster Cl0024.0+1652 with Subaru
• A Panoramic Mid-infrared Survey of Two Distant Clusters
• The survival of dark matter halos in the cluster Cl0024+16
• Cosmic Web of Galaxies in the COSMOS Field: Public Catalog and Different Quenching for Centrals and Satellites
• LoCuSS: The mid-infrared Butcher-Oemler effect
• The evolution of dust-obscured star formation activity in galaxy clusters relative to the field over the last 9 billion years
• Star Formation and AGN Activity in Galaxy Clusters from $z=1-2$: a Multi-wavelength Analysis Featuring $Herschel$/PACS
• The Trouble with Hubble Types in the Virgo Cluster
• zCOSMOS 20k: Satellite galaxies are the main drivers of environmental effects in the galaxy population at least to z~0.7
• The Star Formation Rate-Density Relation at 0.6<z<0.9 and the Role of Star Forming Galaxies
• Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. I. The evolution of the mass-metallicity relation up to z~0.9
• Panoramic H-alpha and mid-infrared mapping of star formation in a z=0.8 cluster
• Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5
• A wide-field spectroscopic survey of the cluster of galaxies Cl0024+1654. II. A high-speed collision?
• Evidence for strong evolution in galaxy environmental quenching efficiency between z = 1.6 and z = 0.9
• Overdensities of Y-dropout Galaxies from the Brightest-of-Reionizing Galaxies Survey: A Candidate Protocluster at Redshift z~8
• The drivers of AGN activity in galaxy clusters: AGN fraction as a function of mass and environment
• Morphology of galaxies in the WINGS clusters
• A Wide-field Hubble Space Telescope Survey of the Cluster Cl 0024+16 at z=0.4. III: Spectroscopic Signatures of Environmental Evolution in Early Type Galaxies
• The evolution of the quenching of star formation in cluster galaxies since z $\sim$ 1
• The rise and fall of star-formation in $\mathbf{z}\sim 0.2$ merging galaxy clusters
• First Measurement of a Rapid Increase in the AGN Fraction in High-Redshift Clusters of Galaxies
• An Unexpectedly High AGN Fraction in Red Cluster Galaxies
• MC${}^2$: Boosted AGN and star-formation activity in CIZA J2242.8+5301, a massive post-merger cluster at z=0.19
• Caustic and Weak Lensing Estimators of Galaxy Cluster Masses
• The GOGREEN survey: The environmental dependence of the star-forming galaxy main sequence at $1.0<z<1.5$
• Mapping dusty star formation in and around a cluster at z=0.81 by wide-field imaging with AKARI
• Morphological Fractions of Galaxies in WINGS Clusters: revisiting the Morphology-Density Paradigm
• From blue star-forming to red passive: galaxies in transition in different environments
• Disentangling Morphology, Star Formation, Stellar Mass, and Environment in Galaxy Evolution
• AGN-Host Galaxy Connection: Morphology and Colours of X-ray Selected AGN at z < 2
• A wide-field spectroscopic survey of the cluster of galaxies Cl0024+1654: I. The catalogue
• Red Star Forming Galaxies and Their Environment at z=0.4 Revealed by Panoramic H-alpha Imaging
• Activity in galactic nuclei of cluster and field galaxies in the local universe
• Retired galaxies: not to be forgotten in the quest of the star formation -- AGN connection
• Detection and Measurement from Narrowband Tunable Filter Scans
• The nature of dusty starburst galaxies in a rich cluster at z=0.4: the progenitors of lenticulars?
• The complete census of optically selected AGNs in the Coma Supercluster: the dependence of AGN activity on the local environment
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The decline of cosmic star formation: quenching, mass, and environment connections
• The role of thermal evaporation in galaxy formation
• Triggering Active Galactic Nuclei in galaxy clusters
• The nature of H-alpha star-forming galaxies at z~0.4 in and around Cl 0939+4713: the environment matters
• Cluster and field elliptical galaxies at z~1.3. The marginal role of the environment and the relevance of the galaxy central regions
• A WISE View of Star Formation in Local Galaxy Clusters
• KYDISC: Galaxy Morphology, Quenching, and Mergers in the Cluster Environment
• Conditional Quenching: A detailed look at the SFR-Density Relation at z ~ 0.9 from ORELSE
• The VIMOS VLT Deep Survey: the group catalogue
• The ALHAMBRA survey: reliable morphological catalogue of 22,051 early- and late-type galaxies
• CLASH-VLT: Strangulation of cluster galaxies in MACSJ0416.1-2403 as seen from their chemical enrichment
• Ram pressure stripping of disk galaxies in galaxy clusters
• Wide-Field Chandra X-Ray Observations of AGN in Abell 85 & Abell 754
• Formation of S0s in extreme environments I: clues from kinematics and stellar populations
• Galaxy evolution in merging clusters: The passive core of the "Train Wreck" cluster of galaxies, A520
• High density of active galactic nuclei in the outskirts of distant galaxy clusters
• Evolution of star formation rate-density relation over cosmic time in a simulated universe: the observed reversal reproduced
• Herschel deep far-infrared counts through the Abell 2218 cluster-lens
• Lower AGN Abundance in Galaxy Clusters at z < 0.5
• An ISOCAM survey through gravitationally lensing galaxy clusters. III. New results from mid-infrared observations of th e cluster Abell 2219
• HST/WFC3 grism observations of $z\sim 1$ clusters: evidence for evolution in the mass-size relation of quiescent galaxies from poststarburst galaxies
• VIS3COS: I. survey overview and the role of environment and stellar mass on star formation
• The time delay between star formation quenching and morphological transformation of galaxies in clusters: a phase-space view of EDisCS
• The impact from survey depth and resolution on the morphological classification of galaxies
• Determining the Halo Mass Scale where Galaxies Lose Their Gas
• Emission Line Galaxies and Active Galactic Nuclei in WINGS clusters
• The OTELO survey. I. Description, data reduction, and multi-wavelength catalogue
• Disc colours in field and cluster spiral galaxies at 0.5 < z < 0.8
• The mass and environmental dependence on the secular processes of AGN in terms of morphology, colour, and specific star-formation rate
• The Role of Host Galaxy for the Environmental Dependence of Active Nuclei in Local Galaxies
• Morphology with Light Profile Fitting of Confirmed Cluster Galaxies at z=0.84
• Differences in the structural properties and star-formation rates of field and cluster galaxies at z~1
• General Formulation for the Calibration and Characterization of Narrow-gap Etalons: the OSIRIS/GTC Tunable Filters Case
• Multi-wavelength landscape of the young galaxy cluster RXJ1257.2+4738 at z=0.866: I. The infrared view
• The CIDA-UCM-Yale Shallow Survey for Emission Line Galaxies
• Effect of richness on AGN and star formation activities in SDSS galaxy groups
• The XXL Survey: XXXVII. The role of the environment in shaping the stellar population properties of galaxies at 0.1<z<0.5
• K-CLASH: spatially-resolving star-forming galaxies in field and cluster environments at $z\approx 0.2$-$0.6$
• Host galaxy properties and environment of obscured and unobscured X-ray selected Active Galactic Nuclei in the COSMOS survey
• Star-formation rates of cluster galaxies: nature vs nurture
• GLACE survey: OSIRIS/GTC Tuneable Filter H$\alpha$ imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. Part I -- Survey presentation, TF data reduction techniques and catalogue
• Group pre-processing versus cluster ram-pressure stripping: the case of ESO156-G029
• The OTELO survey. III. Demography, morphology, IR luminosity and environment of AGN hosts
• The OTELO survey. II. The faint-end of the H$\alpha$ luminosity function at z $\sim$ 0.40
• A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z $\sim$ 0.4
• OTELO survey: optimal emission-line flux determination with OSIRIS/GTC
• Multi-wavelength landscape of the young galaxy cluster RXJ1257.2+4738 at z=0.866. II. Morphological properties
• Galaxy kinematics across different environments in the RXJ1347-1145 cluster complex

Cited by in corpus (1)

• GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652 II. The mass--metallicity relationship and the effect of the environment