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Published: (2025)
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SHELLQs-JWST: Revealing the Spectra of Extended Emission in 12 z > 6 Quasar Host Galaxies using the JWST NIRSpec Fixed Slit
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SHELLQs-JWST Unveils the Host Galaxies of 12 Quasars at z>6
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Published: (2025)
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SHELLQs. Bridging the Gap: JWST Unveils Obscured Quasars in the Most Luminous Galaxies at z > 6
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Published: (2025)
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Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$
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Tip of the iceberg: overmassive black holes at 4<z<7 found by JWST are not inconsistent with the local $\mathcal{M}_{\rm BH}$-$\mathcal{M}_\star$ relation
by: Li, Junyao, et al.
Published: (2024)
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by: Matsuoka, Yoshiki, et al.
Published: (2024)
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Subaru High-$z$ Exploration of Low-Luminosity Quasars (SHELLQs). XXV. Large-scale environments of low-luminosity quasars at $z\sim6$ traced by Ly$α$ emitters
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Published: (2026)
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The nature of low-luminosity AGNs discovered by JWST based on clustering analysis: progenitors of low-$z$ quasars?
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Published: (2024)
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Spectroscopic confirmation of dual and offset quasars from the Subaru HSC-SSP program
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Published: (2026)
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Merging gas-rich galaxies that harbor low-luminosity twin quasars at z = 6.05: a promising progenitor of the most luminous quasars
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UNIONS Optical Identifications for VLASS Radio Sources in the Euclid Sky (UNVEIL) I. A Catalog of ~146,000 Radio Galaxies up to z~5
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A z ~ 0.4 Galaxy Reflecting the high-redshift Little Red Dots: An Extended Starburst with an Overmassive Black Hole
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Published: (2025)
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Diagnosing the massive-seed pathway to high-redshift black holes: statistics of the evolving black hole to host galaxy mass ratio
by: Scoggins, Matthew T., et al.
Published: (2023)
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No Galaxy-Scale [CII] Fast Outflow in the z=6.72 Red Quasar HSC J1205$-$0000
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Environments around quasars at $z\sim$3 revealed by wide-field imaging with Subaru HSC and CFHT
by: Suzuki, Yuta, et al.
Published: (2024)
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Blackbody Quasar and Radio Source (BBQSORS): A Candidate of Transitional Little Red Dots with a $T\sim10^4\ K$ Blackbody Spectrum
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Published: (2026)
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HST Confirms Sub-5 kpc Dual Quasar Pairs at Cosmic Noon
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Subaru High-$z$ Exploration of Low-Luminosity Quasars (SHELLQs). XXIII. The powering mechanisms of the Ly$α$ haloes around high-$z$ quasars probed by slit spectroscopy
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Published: (2025)
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Reconstruction of Cosmic Black Hole Growth and Mass Distribution from Quasar Luminosity Functions at $z>4$: Implications for Faint and Low-mass Populations in JWST
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Published: (2023)
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Black hole mass of a quiescent galaxy hosting a Type 1 AGN at z=2.09: Implications for black hole - galaxy co-evolution and AGN quenching at high redshift
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Ongoing and fossil large-scale outflows detected in a high-redshift radio galaxy: [C II] observations of TN J0924$-$2201 at $z=5.174$
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Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) XXII. Chandra observations of narrow-line quasar candidates at z>6
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Merger fraction in galaxy groups and clusters at z < 0.2: A non-parametric morphological study with Subaru Hyper Suprime-Cam
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BEES: Quasar lifetime measurements from extended rest-optical emission line nebulae at $z\sim6$
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Published: (2025)
by: Ďurovčíková, Dominika, et al.
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Maris polarization in the ($p,pd$) reaction
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The Equational Theory of Relational Kleene Algebra with Graph Loop is PSPACE-Complete
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Similar Items
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SHELLQs-JWST perspective on the intrinsic mass relation between supermassive black holes and their host galaxies at z > 6
by: Silverman, John, et al.
Published: (2025) -
SHELLQs-JWST: Revealing the Spectra of Extended Emission in 12 z > 6 Quasar Host Galaxies using the JWST NIRSpec Fixed Slit
by: Phillips, Camryn L., et al.
Published: (2025) -
SHELLQs-JWST Unveils the Host Galaxies of 12 Quasars at z>6
by: Ding, Xuheng, et al.
Published: (2025) -
SHELLQs. Bridging the Gap: JWST Unveils Obscured Quasars in the Most Luminous Galaxies at z > 6
by: Matsuoka, Yoshiki, et al.
Published: (2025) -
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$
by: Matsuoka, Yoshiki, et al.
Published: (2025)