Optical-radio positional offsets for active galactic nuclei
arXiv:1303.6763 · doi:10.1051/0004-6361/201321279
Abstract
Context. It will soon become possible to directly link the most accurate radio reference frame with the Gaia optical reference frame using many common extragalactic objects. It is important to know the level of coincidence between the radio and optical positions of compact active galactic nuclei (AGN). Aims. Using the best catalogues available at present, we investigate how many AGN with significantly large optical-radio positional offsets exist as well as the possible causes of these offsets. Methods. We performed a case study by finding optical counterparts to the International Celestial Reference Frame (ICRF2) radio sources in the Sloan Digital Sky Survey (SDSS) Data Release 9 (DR9). The ICRF2 catalogue was used as a reference because the radio positions determined by Very Long Baseline Interferometry (VLBI) observations are about two orders of magnitude more accurate than the optical positions. Results. We find 1297 objects in common for ICRF2 and SDSS DR9. Statistical analysis of the optical-radio differences verifies that the SDSS DR9 positions are accurate to ~55 mas in both coordinates, with no systematic offset with respect to ICRF2. We find 51 sources (~4% of the sample) for which the positional offset exceeds 170 mas (~3σ). Astrophysical explanations must exist for most of these outliers. There are 3 known strong gravitational lenses among them. Dual AGN or recoiling supermassive black holes may also be possible. Conclusions. The most accurate Gaia-VLBI reference frame link will require a careful selection of a common set of objects by eliminating the outliers. On the other hand, the significant optical-radio positional non-coincidences may offer a new tool for finding e.g. gravitational lenses or dual AGN candidates. Detailed follow-up radio interferometric and optical spectroscopic observations are encouraged to investigate the outlier sources found in this study.
10 pages, 5 figures. Accepted for publication in Astronomy & Astrophysics
References in corpus (16)
- The Baryon Oscillation Spectroscopic Survey of SDSS-III
- The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey
- The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
- The Sloan Digital Sky Survey quasar catalog: ninth data release
- CGRaBS: An All-Sky Survey of Gamma-Ray Blazar Candidates
- Opacity in compact extragalactic radio sources and its effect on astrophysical and astrometric studies
- The Sixth VLBA Calibrator Survey: VCS6
- Recoiling black holes: electromagnetic signatures, candidates, and astrophysical implications
- VLBI measurement of the secular aberration drift
- Luminosity Function from dedicated SDSS-III and MMT data of quasars in 0.7<z<4.0 selected with a new approach
- Star Formation in Space and Time: The Orion Nebula Cluster
- Correlations of Quasar Optical Spectra with Radio Morphology
- Astrometric suitability of optically-bright ICRF sources for the alignment with the future Gaia celestial reference frame
- Fueling the central engine of radio galaxies. II. The footprints of AGN feedback on the ISM of 3C 236
- Outflowing atomic and molecular gas at towards 1504+377
- Deep Extragalactic VLBI-Optical Survey (DEVOS) II. Efficient VLBI detection of SDSS quasars
Cited by in corpus (31)
- The Last of FIRST: The Final Catalog and Source Identifications
- The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View
- Identification of 1.4 Million AGNs in the Mid-Infrared using WISE Data
- Gaia Data Release 1: The reference frame and the optical properties of ICRF sources
- Deep LOFAR observations of the merging galaxy cluster CIZA J2242.8+5301
- On significance of VLBI/Gaia position offsets
- On the nature of bright compact radio sources at z>4.5
- Astrometric evidence for a population of dislodged AGN
- Fundamental Reference AGN Monitoring Experiment (FRAMEx) I: Jumping Out of the Plane with the VLBA
- ALMA Observations of Quasar Host Galaxies at
- Spatially-Offset AGN Candidates in the CLASS Survey
- A new version of the OCARS catalog of Optical Characteristics of Astrometric Radio Sources
- Radio-Optical Reference Frame Link Using the US Naval Observatory Astrograph and Deep CCD Imaging
- Constraints on galileons from the positions of supermassive black holes
- Gaia reference frame amid quasar variability and proper motion patterns in the data
- Spatially offset black holes in the Horizon-AGN simulation and comparison to observations
- Unprecedented change in the position of four radio sources
- The Search for Binary Supermassive Black Holes Amongst Quasars with Offset Broad Lines Using the Very Long Baseline Array
- Towards the ICRF3: astrometric comparison of the USNO 2016A VLBI solution with ICRF2 and Gaia DR1
- Comparison of multifrequency positions of extragalactic sources from global geodetic VLBI monitoring program and Gaia EDR3
- Constraining VLBI-optical offsets in high redshift galaxies using strong gravitational lensing
- The U.S. Naval Observatory VLBI Spectroscopic Catalog
- Radio-loudness statistics of quasars from Quaia-VLASS
- Galaxies as High-Resolution Telescopes
- Metrics of Astrometric Variability in the International Celestial Reference Frame: I. Statistical analysis and selection of the most variable sources
- Milliarcsecond X-ray astrometry to resolve inner regions of AGN at using gravitational lensing
- High-Resolution Radio Observations of Five Optically Selected Type 2 Quasars
- Identifying massive black hole binaries via light curve variability in optical time-domain surveys
- What is Inside the Double-Double Structure of the Radio Galaxy J0028+0035?
- Radio Properties of Narrow-Line and Broad-Line Seyfert 1 Galaxies
- Role of the companion lensing galaxy in the CLASS gravitational lens B1152+199