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Dark Matter Halos of Luminous Active Galactic Nuclei from Galaxy–Galaxy Lensing with the HSC Subaru Strategic Program
Published 2024-01-01“…We assess the dark matter halo masses of luminous active galactic nuclei (AGNs) over the redshift range 0.2–1.2 using galaxy–galaxy lensing based on imaging data from the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP). …”
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Effectiveness and Safety of Preoperative Halo Gravity Traction-Assisted Posterior Spinal Fusion Surgery for Severe and Rigid Scoliosis: A Comparative Matched-Cohort Study
Published 2024-01-01“…There was no significant difference in the etiologies of scoliosis between two groups (15/7/3/2 vs. 25/16/4/2, P=0.85). The main curve in HGT and non-HGT groups were corrected from an average of 113.69°–51.25° and 111.94°–63.79° (P<0.01). …”
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Overview: quasi-Lagrangian observations of Arctic air mass transformations – introduction and initial results of the HALO–(𝒜 𝒞)<sup>3</sup> aircraft campaign
Published 2024-08-01“…To collect data that help to constrain the models, the HALO–(<span class="inline-formula">𝒜𝒞</span>)<span class="inline-formula"><sup>3</sup></span> aircraft campaign was conducted over the Norwegian and Greenland seas, the Fram Strait, and the central Arctic Ocean in March and April 2022. …”
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Metallicity and α-abundance for 48 Million Stars in Low-extinction Regions in the Milky Way
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The Multiple Extended Tidal Tails of NGC 288
Published 2025-01-01“…On the other hand, NGC 288 is believed to have been brought into the Galactic halo during the Gaia–Enceladus–Sausage accretion event, and the tangential velocity dispersions of our stream candidates are indeed mostly consistent with having been stripped in a parent galaxy that had a large, cored dark matter halo. …”
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Embedding class-I traversable wormhole in f(T,T) gravity via Karmarkar condition
Published 2025-03-01“…., f(T,T) gravity showcasing the influence of prominent dark matter (DM) halos in such a structure by including energy densities of Universal Rotation Curve (URC), Navarro-Frenk-White (NFW), and Scalar Field Dark Matter (SFDM) DM profiles within the solution. …”
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The features of the first impression effect in political perception
Published 2017-12-01Get full text
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GD-1 Stellar Stream and Cocoon in the DESI Early Data Release
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The Rapid Formation of the Metal-poor Milky Way
Published 2025-01-01“…These results reinforce the emerging picture that both the disk and halo of the Milky Way experienced a rapid assembly.…”
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Finding Lensed Radio Sources with the Very Large Array Sky Survey
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A 22 Billion M⊙ Black Hole in Holmberg 15A with Keck KCWI Spectroscopy and Triaxial Orbit Modeling
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A New Deep Vision-Based Identifier As An Intelligent Herbicide Spraying Agent For Potato Farm Application
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The SUPERCOLD-CGM Survey. II. [C i](1–0) Emission and the Physical Conditions of Cold Gas in Enormous Lyα Nebulae at z ∼ 2
Published 2024-01-01“…The 3 σ mass limits of molecular CGM for the remaining QSO fields are (0.2–1.4) × 10 ^10 M _☉ . This translates into a baryon fraction of <0.4%–3% in the molecular CGM relative to the total baryonic halo mass. …”
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Risk factors for photic phenomena in two different multifocal diffractive intraocular lenses
Published 2025-01-01“…There was no difference in glare between the two groups. The halo was larger and thicker, and the starburst was larger and stronger in the Synergy group (P < 0.01). …”
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Visual Outcomes and Patient Satisfaction of Two Continuous Range of Vision Intraocular Lenses
Published 2025-01-01“…J Morgan Micheletti,1 Brad Hall,2 Hayden G Smiley,3 William J Langston4 1Berkeley Eye Center, Houston, TX, USA; 2Sengi, Penniac, NB, Canada; 3Baylor Scott and White Medical Center, Temple, TX, USA; 4Long School of Medicine, San Antonio, TX, USACorrespondence: J Morgan Micheletti, Berkeley Eye Center, Houston, TX, USA, Tel +1-713-526-1600, Email morgan.micheletti@gmail.comPurpose: To determine if visual outcomes with PanOptix are non-inferior to visual outcomes with Synergy.Methods: This was an ambispective, single center, comparative, bilateral, observational study. …”
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