Theoretical Evolution of Optical Strong Lines across Cosmic Time
arXiv:1307.0508 · doi:10.1088/0004-637X/774/2/100
Abstract
We use the chemical evolution predictions of cosmological hydrodynamic simulations with our latest theoretical stellar population synthesis, photoionization and shock models to predict the strong line evolution of ensembles of galaxies from z=3 to the present day. In this paper, we focus on the brightest optical emission-line ratios, [NII]/H-alpha and [OIII]/H-beta. We use the optical diagnostic Baldwin-Phillips-Terlevich (BPT) diagram as a tool for investigating the spectral properties of ensembles of active galaxies. We use four redshift windows chosen to exploit new near-infrared multi-object spectrographs. We predict how the BPT diagram will appear in these four redshift windows given different sets of assumptions. We show that the position of star-forming galaxies on the BPT diagram traces the ISM conditions and radiation field in galaxies at a given redshift. Galaxies containing AGN form a mixing sequence with purely star-forming galaxies. This mixing sequence may change dramatically with cosmic time, due to the metallicity sensitivity of the optical emission-lines. Furthermore, the position of the mixing sequence may probe metallicity gradients in galaxies as a function of redshift, depending on the size of the AGN narrow line region. We apply our latest slow shock models for gas shocked by galactic-scale winds. We show that at high redshift, galactic wind shocks are clearly separated from AGN in line ratio space. Instead, shocks from galactic winds mimic high metallicity starburst galaxies. We discuss our models in the context of future large near-infrared spectroscopic surveys.
20 pages, 7 figures, accepted for publication in the Astrophysical Journal
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- Emission-line diagnostics of HII regions using conditional Invertible Neural Networks
- Constraints from dwarf galaxies on black hole seeding and growth models with current and future surveys
- The role of gas kinematics in setting metallicity gradients at high redshift
- ZFIRE: Measuring Electron Density with [OII] as a function of environment at z = 1.62
- SUPER VII. Morphology and kinematics of H emission in AGN host galaxies at Cosmic noon using SINFONI
- Unsupervised Classification of Galaxies. I. ICA feature selection
- The sign of active galactic nucleus quenching in a merger remnant with radio jets
- Euclid preparation. XXX. Performance assessment of the NISP Red-Grism through spectroscopic simulations for the Wide and Deep surveys
- A methodology to select galaxies just after the quenching of star formation
- UNCOVERing the High-redshift AGN Population among Extreme UV Line Emitters
- Investigating the physical properties of galaxies in the Epoch of Reionization with MIRI/JWST spectroscopy
- The resolved chemical abundance properties within the interstellar medium of star-forming galaxies at
- Radiation fields by intermediate-age stellar populations with binaries as ionizing sources of H II regions
- CLASH-VLT: Enhancement of (O/H) in z=0.35 RXJ 2248-4431 cluster galaxies
- Hardness of ionizing radiation fields in MaNGA star-forming galaxies
- EMPRESS. XI. SDSS and JWST Search for Local and z~4-5 Extremely Metal-Poor Galaxies (EMPGs): Clustering and Chemical Properties of Local EMPGs
- Defying jet-gas alignment in two radio galaxies at z~2 with extended light profiles: Similarities to brightest cluster galaxies
- A Flat-Spectrum Radio Transient at 122 Mpc consistent with an Emerging Pulsar Wind Nebula
- Metal-THINGS: The association and optical characterization of SNRs with HI holes in NGC 6946
- Towards a More Complete Optical Census of Active Galactic Nuclei, Via Spatially-Resolved Spectroscopy
- The fundamental metallicity relation from SDSS (z~0) to VIPERS (z~0.7) Data selection or evolution
- The Local Star Formation Rate Surface Density And Metallicity Relation For Star-forming Galaxies
- Quantifying correlations between galaxy emission lines and stellar continua
- Modelling emission lines in star forming galaxies
- Spatially resolved signature of quenching in star-forming galaxies
- Artificial neural network based calibrations for the prediction of galactic [NII] 6584 and H line luminosities
- GA-NIFS: Mapping AGN-driven ionized outflows in the COSMOS field
- A Tale of Two Clusters: An Analysis of Gas-Phase Metallicity and Nebular Gas Conditions in Proto-cluster Galaxies at z~2
- The MOSDEF Survey: Calibrating the relationship between H star-formation rate and radio continuum luminosity at
- Multi-line assessment of narrow-line regions in 3 radio galaxies
- A metal-rich elongated structure in the core of the group NGC4325
- A Spatially-Resolved Survey of Distant Quasar Host Galaxies: II. Photoionization and Kinematics of the ISM
- HII Region Metallicity Constraints Near the Site of the Strongly Lensed Supernova "SN Refsdal" at Redshift 1.49
- The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s
- AGN Triality of Triple Mergers: Multi-wavelength Classifications
- Multiple giant eruptions and X-ray emission in the recoiling AGN/LBV candidate SDSS1133
- NGDEEP: The Star Formation and Ionization Properties of Galaxies at
- The Direct-Method Oxygen Abundance of Typical Dwarf Galaxies at Cosmic High-Noon
- Integral Field Spectroscopy of the circumnuclear region of the Radio Galaxy Pictor A
- MAMBO -- An empirical galaxy and AGN mock catalogue for the exploitation of future surveys
- Spectroscopic confirmation of a dust-obscured, metal-rich dwarf galaxy at z~5
- Reconciling the Results of the z~2 MOSDEF and KBSS-MOSFIRE Surveys
- New Methods of Identifying AGN in the Early Universe using Spectroscopy and Photometry in the JWST Era
- Emission Line Metallicities From The Faint Infrared Grism Survey and VLT/MUSE
- The effect of emission lines on the performance of photometric redshift estimation algorithms
- The MOSDEF Survey: Towards a Complete Census of the z ~ 2.3 Star-forming Galaxy Population
- Spatially Resolved Spectroscopic Study of nearby Seyfert Galaxies: Implications for a Population of "Missed" Seyferts at High-
- Cloudy-Maraston: Integrating nebular continuum and line emission with the Maraston stellar population synthesis models
- Black hole mass of a quiescent galaxy hosting a Type 1 AGN at z=2.09: Implications for black hole - galaxy co-evolution and AGN quenching at high redshift
- The nebular properties of star-forming galaxies at intermediate redshift from the Large Early Galaxy Astrophysics Census
- Disentangling the physical origin of emission line ratio offsets at high redshift with spatially resolved spectroscopy
- Addressing the [O III]/H\b{eta} Offset of Dwarf Galaxies in the RESOLVE Survey
- Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation
- Catastrophic Cooling in Superwinds. II. Exploring the Parameter Space
- Disentangling AGN and Star Formation Activity at High Redshift Using Hubble Space Telescope Grism Spectroscopy
- An Atlas of Star-Forming Galaxy Equivalent Widths
- First IFU observations of two GRB host galaxies at cosmic noon with JWST/NIRSpec
- Effect of cosmic rays and ionizing radiation on observational ultraviolet plasma diagnostics in the circumgalactic medium
- First joint absorption and T-based metallicity measured in a GRB host galaxy at using JWST/NIRSpec
- GLACE survey: galaxy activity in ZwCl0024+1652 cluster from strong optical emission lines
- Testing the role of AGN on the star formation and metal enrichment of "twin galaxies"
- Physical Drivers of Emission Line Diversity of SDSS Seyfert 2s and LINERs After Removal of Contributions by Star Formation
- Capturing dual AGN activity and kiloparsec-scale outflows in IRAS 20210+1121
- A model for the emission line galaxy luminosity function and flux ratios at high-redshifts
- Evaluating star formation rates at z = 5
- Nitrogen abundances in star-forming galaxies 2.2 Gyr after the Big Bang are not elevated
- Resolved molecular gas and star-formation in massive unquenched spirals : I. UGC 8179
- EMU/GAMA: A new approach to characterising radio luminosity functions
- Challenges and Techniques for Simulating Line Emission
- Morpho-kinematics of MACS J0416.1-2403 low mass galaxies
- Implication of a galaxy-scale negative feedback by one of the most powerful multi-phase outflows in a hyper-luminous infrared galaxy at the intermediate redshift