An Empirical Ultraviolet Template for Iron Emission in Quasars as Derived from I Zw 1
arXiv:astro-ph/0104320 · doi:10.1086/320357
Abstract
We present an empirical template spectrum suitable for fitting/subtracting and studying the FeII and FeIII line emission in the restframe UV spectra of active galatic nuclei (AGNs), the first empirical UV iron template to cover the full 1250 - 3090 A range. Iron emission is often a severe contaminant in optical--UV spectra of AGNs. Its presence complicates and limits the accuracy of measurements of both strong and weak emission lines and the continuum emission, affecting studies of line and continuum interrelations, the ionization structure, and elemental abundances in AGNs. Despite the wealth of work on modeling the AGN FeII emission and the need to account for it in observed AGN spectra, there is no UV template electronically available to aid this process. The iron template we present is based on HST spectra of the Narrow Line Seyfert 1, IZw1. Its intrinsic narrow lines (~900 km/s) and rich iron spectrum make the template particularly suitable for use with most AGN spectra. The iron emission spectrum and the line identifications and measurements are presented and compared with the work of Laor et al. We illustrate the application of the derived FeII and FeIII templates by fitting and subtracting the iron emission from UV spectra of four high-z quasars and of the nearby quasar, 3C273. We briefly discuss the small discrepancies between this observed iron emission and the UV template, and compare the template with previously published ones. We discuss the advantages and limitations of the templates and of the template fitting method. We conclude that the templates work sufficiently well to be a valuable and important tool for eliminating and studying the iron emission in AGNs, at least until accurate theoretical iron emission models are developed. (Abridged)
73 pages including 7 figures, 6 tables. To appear in ApJS. Preprint is also available at http://www.astronomy.ohio-state.edu/~vester/IronEmission/
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- Discovery of the Most-Distant Double-Peaked Emitter at z=1.369
- Estimating black hole masses: Accretion disk fitting versus reverberation mapping and single epoch
- Hubble Space Telescope Ultraviolet Spectroscopy of Fourteen Low-Redshift Quasars
- Emission Line Variability during a Nonthermal Outburst in the Gamma-Ray Bright Quasar 1156+295
- Wavelength Dependences of the Optical/UV and X-ray Luminosity Correlations of Quasars
- Statistical analysis of AlIII 1860 and CIII] 1909 emission lines as virial black hole mass estimators in quasars
- Discovery of a Low-Redshift Hot Dust-Obscured Galaxy
- Radio-Loud and Radio-Quiet BAL Quasars: A Detailed Ultraviolet Comparison
- Ultraviolet emission lines of Si II in quasars --- investigating the "Si II disaster"
- Discovery of the most luminous quasar of the last 9 Gyr
- An X-ray fading, UV brightening QSO at
- The quasar SDSS J142507.32+323137.4 : dual AGNs?
- UV Fe II emission model of HE 0413-4031 and its relation to broad-line time delays
- JADES -- The small blue bump in GN-z11: insights into the nuclear region of a galaxy at z=10.6
- Optical IFU Observations of GOALS Sample with KOOLS-IFU on Seimei Telescope: Initial results of 9 U/LIRGs at 0.04
- The U.S. Naval Observatory VLBI Spectroscopic Catalog
- A QSO plus host system lensed into a 6" Einstein ring by a low redshift galaxy
- Gemini Near Infrared Spectrograph - Distant Quasar Survey: Prescriptions for Calibrating UV-Based Estimates of Supermassive Black Hole Masses in High-Redshift Quasars
- Testing Einstein's Equivalence Principle and its Cosmological Evolution from Quasar Gravitational Redshifts
- Far-Ultraviolet Spectroscopy Of Active Galactic Nuclei With AstroSat/UVIT
- The MURALES survey. VII. Optical spectral properties of the nuclei of 3C radio sources at 0.3<z<0.82
- Composite spectra of quasars with different UV spectral index
- The low-mass end of the Mbh/Mhost relation in quasars
- Characterising SMSS J2157--3602, the most luminous known quasar, with accretion disc models
- A new apparent quasar pair: Q2225-403A,B
- A γ-ray emitting NLS1 galaxy SDSS J095909.51+460014.3 identified by multiwavelength contemporaneous brightening
- The Active Galactic Nuclei in the Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX) II. Luminosity Function
- A Closer Look at Two of the Most Luminous Quasars in the Universe
- Comprehensive view on a radio-loud QSO: from the radio to the optical/NIR to the X-ray band
- Unveiling the quasar main sequence: illuminating the complexity of active galactic nuclei and their evolution
- SALT long-slit spectroscopy of HE 0435-4312: fast displacement in the Mg II emission line
- When Spectral Modeling Meets Convolutional Networks: A Method for Discovering Reionization-era Lensed Quasars in Multi-band Imaging Data
- Detection of Iron Emission in the z = 5.74 QSO SDSSp J104433.04-012502.2
- Revealing the structure of the lensed quasar Q 0957+561: III. SMBH mass via gravitational redshift
- Spectroscopic follow-up of double quasar candidates
- AGN mass estimates in large spectroscopic surveys: the effect of host galaxy light
- Monster radio jet (>66 kpc) observed in quasar at z5
- Exploring the links between quasar winds and radio emission along the Main Sequence at high redshift
- Deep CFHT Y-band Imaging of VVDS-F22 Field: II. Quasar Selection and Quasar Luminosity Function
- X-ray and Multiwavelength Insights into the Inner Structure of High-Luminosity Disc-Like Emitters
- Unveiling the monster heart: unbeamed properties of blazar 4C 71.07
- Optical Spectroscopy of Dual Quasar Candidates from the Subaru HSC-SSP program
- Fading Light, Fierce Winds: JWST Snapshot of a Sub-Eddington Quasar at Cosmic Dawn
- Elucidating the Correlation of the Quasar \ion{Fe}{2}/\ion{Mg}{2} Ratio with Redshift
- The detections of inflowing gas from narrow absorption lines at the parsec scale
- Probing the He II re-Ionization ERa via Absorbing C IV Historical Yield (HIERACHY) I: A Strong Outflow from a z~4.7 Quasar
- Gaia-assisted discovery of a detached low-ionisation BAL quasar with very large ejection velocities
- A Catalog of Post-starburst Quasars from Sloan Digital Sky Survey Data Release 7
- Quasars' Optical Polarization and Balmer Edge Feature Revealed by Ultra-Violet, and Polarized Visible to Near Infrared Emissions
- Evidence of Increased UV FeII Emission in Quasars in Candidate Overdense Regions
- SDSS spectroscopy for blazars in the LAT bright AGN sample
- Uncertainty Quantification of the Virial Black Hole Mass with Conformal Prediction
- Discovery of six high-redshift quasars with the Lijiang 2.4m telescope and the Multiple Mirror Telescope
- Serendipitous discovery of a projected pair of QSOs separated by 4.5 arcsec on the sky
- Discovering bright quasars at intermediate redshifts based on the optical/near-IR colors
- Ultraviolet Fe II Emission in Fainter Quasars: Luminosity Dependences, and the Influence of Environments
- Narrow [O III] emission lines as a potential proxy for the evolutionary stage of quasars
- Accelerating lensed quasar discovery and modeling with physics-informed variational autoencoders
- Multi-phase investigation of outflows in the circumgalactic and interstellar media of luminous quasars at z~5
- Robust AGN and host-galaxy decomposition in optical spectral fitting
- The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: Quasar Properties from Data Release 10 to 12
- Extreme Galaxy-scale Outflows Are Frequent among Luminous Early Quasars
- A broad-line quasar with unexplained extreme velocity offsets: post-shock outflow?
- Ultradense Gases beyond Dusty Torus in a Partially Obscured Quasar
- The broad band SEDs of four 'hypervariable' AGN
- The CaFe Project: Optical FeII and Near-Infrared Ca II triplet emission in active galaxies. II. The driver(s) of the Ca II and Fe II and its potential use as a chemical clock
- A simple non-parametric method for resolving merged doublet lines: Insights into complex kinematics and outflows
- Mg II line properties in lobe-dominated quasars
- QUEST (Quasar Unsupervised Encoder and Synthesis Tool): A machine learning framework to generate quasar spectra
- Far-UV Fe Emission as Proxy of Eddington Ratios
- The Sloan Digital Sky Survey Reverberation Mapping Project: UV-Optical Accretion Disk Measurements with Hubble Space Telescope
- A New Member of the Fast and Furious Family: A Relativistic and Time-Variable UV Outflow in a Luminous Quasar
- Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds
- Cold Quasar Investigation: Comparing Star Formation Rates to Black Hole Growth
- An equal mass ratio supermassive binary black holes in Q J0158-4325 with periodic microlensing signature?
- Models of Optical Emission Lines To Investigate Narrow-Line Seyfert 1 Galaxies in Spectroscopic Databases
- Evidence for the connection between star formation rate and evolutionary phases of quasars
- Strong correlation between FeII/MgII ratio and Eddington ratio of type 1 Active galactic nuclei
- ELFO: A Python Package for Emission Line Fitting Optimization in Integral Field Spectroscopy Data
- Spectroscopic confirmation of dual and offset quasars from the Subaru HSC-SSP program
- Indicators of Black Hole Mass and Eddington Accretion Ratio from QSO X-ray and UV Spectra
- The Relationship Between Emission Line and Continuum Luminosity and the Baldwin Effect in Blazars. I. The Case of the Mg II λ2798 Å Emission Line
- The miniJPAS survey quasar selection I: Mock catalogues for classification
- Testing [O II] as a Star Formation Rate Tracer in Quasar Host Galaxies
- Quiescent Host Galaxies of Extended Quasars Revealed by Spectrophotometric Decomposition