AGN and Starburst Classification from Spitzer Mid-Infrared Spectra for High Redshift SWIRE Sources
arXiv:astro-ph/0608609 · doi:10.1086/508647
Abstract
Spectra have been obtained with the Infrared Spectrograph (IRS) on the Spitzer Space Telescope for 20 sources in the Lockman Hole field of the SWIRE survey. The sample is divided between sources with indicators of an obscured AGN, based primarily on X-ray detections of optically-faint sources, and sources with indicators of a starburst, based on optical and near-infrared spectral energy distributions (SEDs) which show a luminosity peak from stellar photospheric emission. Ten of the 11 AGN sources have IRS spectra which show silicate absorption or are power laws; only one AGN source shows PAH emission features. All 9 of the sources showing starburst SEDs in the near-infrared show PAH emission features in the IRS spectra. Redshifts are determined from the IRS spectra for all 9 starbursts (1.0 < z < 1.9) and 8 of the 11 AGN (0.6 < z < 2.5). Classification as AGN because of an X-ray detection, the classification as AGN or starburst derived from the photometric SED, and the IRS spectroscopic classification as AGN (silicate absorption) or starburst (PAH emission) are all consistent in 18 of 20 sources. The surface density for starbursts which are most luminous in the mid-infrared is less than that for the most luminous AGN within the redshift interval 1.7 < z < 1.9. This result implies that mid-infrared source counts at high redshift are dominated by AGN for f(24micron) > 1.0 mJy.
arXiv comment34 pages, 11 figures, ApJ accepted (Dec 2006)
References in corpus (33)
- The Infrared Array Camera (IRAC) for the Spitzer Space Telescope
- The Infrared Spectrograph on the Spitzer Space Telescope
- Infrared Emission from Interstellar Dust. II. The Diffuse Interstellar Medium
- Rotating Nuclear Rings and Extreme Starbursts in Ultraluminous Galaxies
- What Powers Ultra-luminous IRAS Galaxies?
- SWIRE: The SIRTF Wide-area InfraRed Extragalactic Survey
- The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: I. Limits and Detections
- The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background
- The SMART Data Analysis Package for the Infrared Spectrograph on the Spitzer Space Telescope
- A large mid-infrared spectroscopic and near-IR imaging survey of ULIRGs: their nature and evolution
- The 24 Micron Source Counts in Deep Spitzer Surveys
- The nature and evolution of Ultraluminous Infrared Galaxies: A mid-infrared spectroscopic survey
- PAHs contribution to the infrared output energy of the Universe at z~2
- Starburst and AGN activity in ultraluminous infrared galaxies
- Spectroscopic Redshifts to z > 2 for Optically Obscured Sources Discovered with the Spitzer Space Telescope
- Mid-Infrared Spectra of Classical AGN Observed with the Spitzer Space Telescope
- Chandra and Spitzer unveil heavily obscured quasars in the SWIRE/Chandra Survey
- The Chandra Deep Field North Survey. VI. The Nature of the Optically Faint X-ray Source Population
- First Insights into the SWIRE Galaxy Populations
- Spitzer Detection of PAH and Silicate Dust Features in the Mid-Infrared Spectra of z~2 Ultraluminous Infrared Galaxies
- The Reddest Quasars
- The Nature of Faint 24 micron Sources Seen in Spitzer Observations of ELAIS-N1
- The AGN Contribution to the Mid-IR Emission of Luminous Infrared Galaxies
- The 1<z<5 Infrared Luminosity Function of Type I Quasars
- Mid-infrared spectroscopy of two luminous submillimeter galaxies at z~2.8
- The detection and photometric redshift determination of distant galaxies using SIRTF's Infrared Array Camera
- X-raying the Ultraluminous Infrared Starburst Galaxy and Broad Absorption Line QSO, Markarian 231, with Chandra
- Spitzer-IRS Spectroscopy of the Prototypical Starburst Galaxy NGC7714
- Spitzer IRS Spectra of Optically Faint Infrared Sources with Weak Spectral Features
- Redshifts from Spitzer Spectra for Optically Faint, Radio Selected Infrared Sources
- Spatially-resolved spectrophotometric analysis and modelling of the Superantennae
- IRS spectra of two ultraluminous infrared galaxies at z=1.3
- Variation in the Scattering Shroud Surrounding Markarian 231
Cited by in corpus (74)
- Spectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey
- AGN Dusty Tori: II. Observational Implications of Clumpiness
- Identifying Luminous AGN in Deep Surveys: Revised IRAC Selection Criteria
- Photometric redshift and classification for the XMM-COSMOS sources
- Swift BAT Survey of AGN
- The First Hyper-Luminous Infrared Galaxy Discovered by WISE
- The distribution of silicate strength in Spitzer spectra of AGNs and ULIRGs
- Submillimeter Follow-up of WISE-Selected Hyperluminous Galaxies
- A Physical Model for z~2 Dust Obscured Galaxies
- The nature of star formation in distant ultraluminous infrared galaxies selected in a remarkably narrow redshift range
- Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z~2 II: Diagnostics
- Blind detections of CO J = 1--0 in 11 H-ATLAS galaxies at z = 2.1--3.5 with the GBT/Zpectrometer
- Reliable Identification of Compton-thick Quasars at z~2: Spitzer Mid-IR spectroscopy of HDF-oMD49
- Obscuration in extremely luminous quasars
- A large population of mid-infrared selected, obscured active galaxies in the Bootes field
- The metallicity gradient of M 33: chemical abundances of HII regions
- Spitzer/IRS 5-35 um Low-Resolution Spectroscopy of the 12 um Seyfert Sample
- The WISE properties of complete samples of radio-loud AGN
- Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z~2 III: Far-IR to Radio Properties and Optical Spectral Diagnostics
- A Multiwavelength Study of a Sample of 70 micron Selected Galaxies in the COSMOS Field I: Spectral Energy Distributions and Luminosities
- Molecules in galaxies
- The planetary nebula population of M33 and its metallicity gradient: A look into the galaxy's distant past
- The Origin of Line Emission in Massive z~2.3 Galaxies: Evidence for Cosmic Downsizing of AGN Host Galaxies
- The Spitzer Infrared Nearby Galaxies Survey: A High-Resolution Spectroscopy Anthology
- Mid-infrared spectroscopy of infrared-luminous galaxies at z~0.5-3
- An atlas of mid-infrared spectra of star-forming and active galaxies
- Far-Infrared Properties of Spitzer-selected Luminous Starbursts
- Measuring PAH Emission in Ultradeep Spitzer IRS Spectroscopy of High Redshift IR Luminous Galaxies
- IRS Spectroscopy and Multi-wavelength Study of Luminous Star-forming Galaxies at z~1.9
- Mid-infrared spectroscopy of candidate AGN-dominated submillimeter galaxies
- Searching for mid-IR obscured AGN in the CDF-N
- Infrared Luminosities and Dust Properties of z ~ 2 Dust-Obscured Galaxies
- HST Morphologies of z~2 Dust Obscured Galaxies I: Power-law Sources
- Mid- to far infrared properties of star-forming galaxies and active galactic nuclei
- A Millimetre Survey of Starburst Dominated Ultraluminous Infrared Galaxies at z~2
- Spitzer Spectra of a 10 mJy Galaxy Sample and the Star Formation Rate in the Local Universe
- The Most Luminous Starbursts in the Universe
- Infrared Spectra and Spectral Energy Distributions for Dusty Starbursts and AGN
- Clarifying the nature of the brightest submillimetre sources: interferometric imaging of LH850.02
- MAMBO 1.2mm observations of luminous starbursts at z~2 in the SWIRE fields
- Anomalous Silicate Dust Emission in the Type 1 LINER Nucleus of M81
- Star Formation Rates for Starburst Galaxies from Ultraviolet, Infrared, and Radio Luminosities
- The Star-Formation Histories of z~2 DOGs and SMGs
- HST Morphologies of z ~ 2 Dust-Obscured Galaxies II: Bump Sources
- The HELLAS2XMM survey. XIII. Multi-component analysis of the spectral energy distribution of obscured AGN
- Mid-infrared spectroscopy of Spitzer-selected ultra-luminous starbursts at z~2
- Unveiling the Nature of Submillimeter Galaxy SXDF850.6
- Multi-Wavelength Study of a Complete IRAC 3.6micron-Selected Galaxy Sample: a Fair Census of Red and Blue Populations at Redshifts 0.4-1
- Obscured and powerful AGN and starburst activities at z~3.5
- Variations in the 6.2 m emission profile in starburst-dominated galaxies: a signature of polycyclic aromatic nitrogen heterocycles (PANHs)?
- An extinction free AGN selection by 18-band SED fitting in mid-infrared in the AKARI NEP deep field
- The XMM-Newton survey of the ELAIS-S1 field II: optical identifications and multiwavelength catalogue of X-ray sources
- Multi-wavelength properties of Spitzer-selected starbursts at z~2
- The ESO-Spitzer Imaging extragalactic Survey (ESIS) II: VIMOS I,z wide field imaging of ELAIS-S1 and selection of distant massive galaxies
- Spitzer Mid-Infrared Spectroscopy of Distant X-ray Luminous AGN
- Spitzer IRS Spectra of Optically Faint IRAS Sources
- Spitzer Mid-Infrared Spectroscopy of 70um-Selected Distant Luminous Infrared Galaxies
- Discovery of Compton-thick quasars in the Sloan Digital Sky Survey
- The Environment on few Mpc scales of Infrared Luminous Galaxies at Redshifts z~1
- Spitzer 24 um Excesses for Bright Galactic Stars in Bootes and First Look Survey Fields
- SSGSS: The Spitzer-SDSS-GALEX Spectroscopic Survey
- Automated measurement of redshift from mid-infrared low resolution spectroscopy
- Mid-Infrared Spectroscopy of Optically Faint Extragalactic 70 micron Sources
- A multi-wavelength survey of AGN in the XMM-LSS field: I. Quasar selection via the KX technique
- Evolution of the Most Luminous Dusty Galaxies
- The radio properties of optically obscured Spitzer sources
- Physical Properties, Star Formation, and Active Galactic Nucleus Activity in Balmer Break Galaxies at 0 < z < 1
- The role of SPICA-like missions and the Origins Space Telescope in the quest for heavily obscured AGN and synergies with Athena
- Selection and Mid-infrared Spectroscopy of Ultraluminous Star-Forming Galaxies at z~2
- Comparing Ultraviolet and Infrared-Selected Starburst Galaxies in Dust Obscuration and Luminosity
- Black hole growth and stellar assembly at high-z
- AGN counts at 15um. XMM observations of the ELAIS-S1-5 sample
- MAMBO Observations at 240GHz of optically obscured Spitzer sources: source clumps and radio activity at high redshift
- Dusty Quasars at High Redshifts