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4381
Genotype-environment interactions on growth and inner shell color variation in Hyriopsis cumingii cultured in different iron-level substrates
Published 2025-03-01“…Heritability estimates for growth and inner shell color traits ranged from 0.07 to 0.25 across the experimental population. The anal angle radial rib length (AARRL) displayed stronger genetic and phenotypic correlations with body weight (BW) and shell width (SW) compared to shell height (SH) and total shell height (TSH). …”
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4382
Calibrating the Color–Magnitude Relation of M Giants by Using Open Clusters
Published 2025-01-01“…Using the distances of M giants derived from the CMR, we computed their radial velocity ( V _R ), azimuthal velocity ( V _ϕ ), and vertical velocity ( V _Z ), respectively. …”
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4383
Optimization of Key Parameters for Coal Seam L-CO<sub>2</sub> Phase Transition Blasting Based on Response Surface Methodology
Published 2025-01-01“…L-CO<sub>2</sub> blasting creates a plastic deformation zone and a pulverized zone around the borehole within 500 μs to 800 μs after detonation, with a tensile fracture zone appearing at 2000 μs. By analyzing radial and tangential stresses at different distances from the explosion center, the mechanical mechanisms of fracture formation in different blast zones were revealed. …”
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4384
Preservative-free therapy for glaucoma after corneal refractive surgery
Published 2019-09-01“…</i> </p> <p> <i><b>Keywords</b>: glaucoma, refractive surgery, radial keratotomy, intraocular pressure, tonometry, progressive hyperopia, preservative-free therapy, timolol.…”
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4385
JWST Imaging of Edge-on Protoplanetary Disks. IV. Mid-infrared Dust Scattering in the HH 30 Disk
Published 2025-01-01“…Our multiwavelength images clearly reveal the vertical and radial segregation of micron-sized and submillimeter-sized grains in the disk. …”
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4386
Fotobiomodulación vascular en el tratamiento de niños con transtornos temporomandibulares
Published 2024-12-01“…La técnica no es invasiva, el punto de irradiación es por aplicación transcutánea continua y directa a la arteria radial por medio de pulsera en la que se aplica el haz del láser. …”
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4387
Joint effects of temperature and humidity with PM2.5 on COPD
Published 2025-02-01“…Methods A case–control study was conducted among 1,828 participants from 2017 to 2022 (995 COPD patients and 833 controls). The radial basis function interpolation was utilized to estimate participants' individual mean and differences in PM2.5, temperature, and RH in 1-day, 7-day, and 1-month periods. …”
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4389
An exploratory study of INPP4B, a biomarker of gemcitabine chemoresistance in pancreatic cancer
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4393
An Overview of Patient-reported Outcomes for Men with Prostate Cancer: Results from the PIONEER Consortium
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4396
Pearls on a String: Dark and Bright Galaxies on a Strikingly Straight and Narrow Filament
Published 2025-01-01“…They have redshifts in a very small range of z = 0.0361−0.0370 so that their radial velocities are consistent with galaxy proper motions. …”
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4398
Assessment of myocardial deformation by CMR tissue tracking reveals left ventricular subclinical myocardial dysfunction in patients with gynecologic cancer undergoing chemotherapy
Published 2025-02-01“…Compared to the controls, patients exhibited lower absolute value of global radial strain (GRS) (37.30 ± 8.94% vs. 44.32 ± 8.44%), global circumferential strain (GCS) (-22.12 ± 3.05% vs. -24.08 ± 2.13%) and global longitudinal strain (GLS) (median -15.72% [IQR-17.13 to -13.58%] vs. -17.51 ± 2.00 %) (all p < 0.05). …”
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4399
Reverberation Mapping of Two Variable Active Galactic Nuclei: Probing the Distinct Characteristics of the Inner and Outer Broad-line Regions
Published 2025-01-01“…We measured the time lags of multiple broad emission lines (H α , H β , H γ , He i , and He ii ) and found clear evidence of radial ionization stratification in the BLRs of both AGNs. …”
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4400
WALLABY Pilot Survey: Star Formation Enhancement and Suppression in Gas-rich Galaxy Pairs
Published 2025-01-01“…In contrast, the SFRs of galaxies with M _* > 10 ^9 M _⊙ increase monotonically toward smaller projected distances and radial velocity offsets. When a close companion is present, a pronounced SFR enhancement is found for the most H i -poor high-mass galaxies in our sample. …”
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