Magellan Spectroscopy of AGN Candidates in the COSMOS Field
arXiv:astro-ph/0606016 · doi:10.1086/516578
Abstract
We present spectroscopic redshifts for the first 466 X-ray and radio-selected AGN targets in the 2 deg^2 COSMOS field. Spectra were obtained with the IMACS instrument on the Magellan (Baade) telescope, using the nod-and-shuffle technique. We identify a variety of Type 1 and Type 2 AGN, as well as red galaxies with no emission lines. Our redshift yield is 72% down to i_AB=24, although the yield is >90% for i_AB<22. We expect the completeness to increase as the survey continues. When our survey is complete and additional redshifts from the zCOSMOS project are included, we anticipate ~1100 AGN with redshifts over the entire COSMOS field. Our redshift survey is consistent with an obscured AGN population that peaks at z~0.7, although further work is necessary to disentangle the selection effects.
19 pages, 14 figures. Accepted to ApJS special COSMOS issue. The full electronic version of Table 2 can be found at http://shaihulud.as.arizona.edu/~jtrump/tab2.txt
References in corpus (8)
- The Cosmic Evolution Survey (COSMOS) -- Overview
- zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field
- The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
- The VLA-COSMOS Survey: II. Source Catalog of the Large Project
- The XMM-Newton wide-field survey in the COSMOS field: III. optical identification and multiwavelength properties of a large sample of X-ray selected sources
- The effects of environment on morphological evolution between 0<z<1.2 in the COSMOS Survey
- The XMM-Newton wide-field survey in the COSMOS field. IV: X-ray spectral properties of Active Galactic Nuclei
- The Serendipitous Extragalactic X-Ray Source Identification (SEXSI) Program. III. Optical Spectroscopy
Cited by in corpus (41)
- The Chandra COSMOS Survey, I: Overview and Point Source Catalog
- The bulk of the black hole growth since z~1 occurs in a secular universe: No major merger-AGN connection
- Photometric redshift and classification for the XMM-COSMOS sources
- The VLA-COSMOS Survey: II. Source Catalog of the Large Project
- The XMM-Newton wide-field survey in the COSMOS field: VI. Statistical properties of clusters of galaxies
- UV/Optical Detections of Candidate Tidal Disruption Events by GALEX and CFHTLS
- The XMM-Newton wide-field survey in the COSMOS field: III. optical identification and multiwavelength properties of a large sample of X-ray selected sources
- A new method to separate star forming from AGN galaxies at intermediate redshift: The submillijansky radio population in the VLA-COSMOS survey
- First catalog of strong lens candidates in the COSMOS field
- Measuring the Fraction of Obscured Quasars by the Infrared Luminosity of Unobscured Quasars
- The Chandra COSMOS-Legacy survey: Source X-ray spectral properties
- The VLA-COSMOS Survey: III. Further Catalog Analysis and the Radio Source Counts
- The XMM-Newton wide-field survey in the COSMOS field. IV: X-ray spectral properties of Active Galactic Nuclei
- The spatial clustering of X-ray selected AGN in the XMM-COSMOS field
- High redshift quasars in the COSMOS survey: the space density of z>3 X-ray selected QSOs
- Observational Constraints on the Dependence of Radio-Quiet Quasar X-ray Emission on Black Hole Mass and Accretion Rate
- An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution
- Physical properties of z>4 submillimeter galaxies in the COSMOS field
- The GALEX Time Domain Survey I. Selection and Classification of Over a Thousand UV Variable Sources
- The faint radio sky: VLBA observations of the COSMOS field
- A wide angle tail radio galaxy in the COSMOS field: evidence for cluster formation
- The XMM-Newton wide-field survey in the COSMOS field: V. Angular Clustering of the X-ray Point Sources
- Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z=2.16 in the Cosmos field
- Properties of the molecular gas in a starbursting QSO at z=1.83 in the COSMOS field
- The Chandra COSMOS Legacy survey: the z>3 sample
- Cluster candidates around low power radio-galaxies at z~1-2 in COSMOS
- The VLA-COSMOS Survey: V. 324 MHz continuum observations
- The evolution of galaxy star formation activity in massive halos
- The Chandra COSMOS Legacy Survey: Clustering of X-ray selected AGN at 2.9<z<5.5 using photometric redshift Probability Distribution Functions
- The evolution of star formation activity in galaxy groups
- Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3.5
- X-ray properties of radio-selected star forming galaxies in the Chandra-COSMOS survey
- Morphological Evolution of the Hosts of Far-Infrared/Submillimeter Galaxies
- MAGIC: Muse gAlaxy Groups In Cosmos -- A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr
- DESI Complete Calibration of the Color-Redshift Relation (DC3R2): Results from early DESI data
- Obscured AGN enhancement in galaxy pairs at cosmic noon: evidence from a probabilistic treatment of photometric redshifts
- A slitless spectroscopic survey for quasars near quasars
- A new method to search for high redshift clusters using photometric redshifts
- Optical Selection of Faint AGN in the COSMOS Field
- Exploring the X-ray-radio connection for AGN via measurements of the multi-dimensional luminosity function
- Where's Swimmy?: Mining unique color features buried in galaxies by deep anomaly detection using Subaru Hyper Suprime-Cam data