Discovery of merging twin quasars at z = 6.05
arXiv:2405.02465 · doi:10.3847/2041-8213/ad35c7
Abstract
We report the discovery of two quasars at a redshift of = 6.05, in the process of merging. They were serendipitously discovered from the deep multi-band imaging data collected by the Hyper Suprime-Cam (HSC) Subaru Strategic Program survey. The quasars, HSC 121503.42014858.7 (C1) and HSC 121503.55014859.3 (C2), both have luminous (10 erg s) Ly emission with a clear broad component (full width at half maximum 1000 km s). The rest-frame ultraviolet (UV) absolute magnitudes are (C1) and (C2). Our crude estimates of the black hole masses provide in both sources. The two quasars are separated by 12 kpc in projected proper distance, bridged by a structure in the rest-UV light suggesting that they are undergoing a merger. This pair is one of the most distant merging quasars reported to date, providing crucial insight into galaxy and black hole build-up in the hierarchical structure formation scenario. A companion paper will present the gas and dust properties captured by Atacama Large Millimeter/submillimeter Array observations, which provide additional evidence for and detailed measurements of the merger and also demonstrate that the two sources are not gravitationally-lensed images of a single quasar.
Published from ApJL. A companion paper (T. Izumi et al.) presents the associated ALMA observations
References in corpus (11)
- The Gaia mission
- A Catalog of Quasar Properties from SDSS DR7
- Rapidly star-forming galaxies adjacent to quasars at redshifts exceeding 6
- Growth and activity of black holes in galaxy mergers with varying mass ratios
- The REQUIEM Survey I: A Search for Extended Ly-Alpha Nebular Emission Around 31 z>5.7 Quasars
- Quasar Luminosity Function at z = 7
- Dual supermassive black holes at close separation revealed by the Hyper Suprime-Cam Subaru Strategic Program
- A hidden population of high-redshift double quasars unveiled by astrometry
- The Pan-STARRS1 Quasar Survey: III. The Quasar Luminosity Function
- A Survey for High-redshift Gravitationally Lensed Quasars and Close Quasars Pairs. I. the Discoveries of an Intermediately-lensed Quasar and a Kpc-scale Quasar Pair at
- Testing the paradigm: First spectroscopic evidence of a quasar-galaxy Mpc-scale association at cosmic dawn
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- GA-NIFS: High number of dual active galactic nuclei at z~3
- SHELLQs. Bridging the Gap: JWST Unveils Obscured Quasars in the Most Luminous Galaxies at z > 6
- GA-NIFS: The highly overdense system BR1202-0725 at z 4.7. A double AGN with fast outflows plus eight companion galaxies
- JWST's PEARLS: A z=6 quasar in a train-wreck galaxy merger system
- First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
- Multi-wavelength properties of LISA detectable events
- Milliarcsecond astrometric oscillations in active galactic nuclei as a precursor of multi-messenger gravitational wave events
- Fast, dust-poor outflows in the local candidate dual AGN MCG-03-34-64 observed with VLT/ERIS
- Spectroscopic confirmation of dual and offset quasars from the Subaru HSC-SSP program