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1961
Subthreshold intracortical microstimulation of human somatosensory cortex enhances tactile sensitivity
Published 2025-05-01“…Results: We found that subthreshold ICMS enhanced sensitivity to touch on the skin, as evidenced by a reduction in vibrotactile detection thresholds (median: 1.5 dB), but subthreshold vibration did not systematically impact the detectability of ICMS. …”
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1962
Adaptive immune changes in colorectal cancer: a focus on T and B cell activation genes
Published 2025-06-01“…A panel of 84 genes involved in T and B cell activation was analyzed to assess changes in expression using RT2 QPCR arrays. Additionally, we measured serum levels of the four IgG subclasses (IgG1, IgG2, IgG3, and IgG4) in CRC patients to explore possible alterations in humoral immunity. …”
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1963
Fine mapping genetic variants affecting birth weight in sheep: a GWAS of 3007 individuals using low-coverage whole genome sequencing
Published 2025-08-01“…However, its genetic architecture remains poorly understood due to historical limitations in sample size and reliance on low-density SNP arrays. In this study, we utilized low-coverage whole-genome sequencing (lcWGS) to genotype 3,007 Hu sheep, bypassing the cost and resolution constraints of conventional genotyping arrays while achieving scalable genome-wide variant detection. …”
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1964
The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO). X. Dust Substructures, Disk Geometries, and Dust-disk Radii
Published 2025-01-01“…We perform visibility fitting to the dust continuum Band 6 1.3 mm data of the 30 protoplanetary disks in the Atacama Large Millimeter/submillimeter Array Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO) Large Program. …”
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1965
The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO). III. Dust and Gas Disk Properties in the Lupus Star-forming Region
Published 2025-01-01“…All of our sources are detected in ^12 CO and ^13 CO; seven out of ten are detected in C ^18 O; and three are detected in N _2 H ^+ . …”
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1966
Timing and Spectral Evolution of the Magnetar 1E 1841-045 in Outburst
Published 2025-01-01“…We present timing and spectral analyses of Neutron star Interior Composition Explorer (NICER), Nuclear Spectroscopic Telescope Array (NuSTAR), and IXPE observations of the magnetar 1E 1841−045 covering 82 days following its 2024 August bursting activity as well as radio observations utilizing MeerKAT and Effelsberg. …”
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1967
Autoantibody against UBE2E3 is a common biomarker for atherosclerotic diseases and digestive tract cancer
Published 2025-05-01“…Therefore, identifying novel autoantibody biomarkers associated with atherosclerosis-related conditions is crucial for improving early diagnosis and risk assessment. Methods: We used an array of 9,480 proteins to detect IgG antibodies in the serum of patients with atherosclerosis. …”
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1968
Radio Afterglows from Tidal Disruption Events: An Unbiased Sample from ASKAP RACS
Published 2024-01-01“…Using all-sky multiepoch data from the Australian Square Kilometre Array Pathfinder (ASKAP), taken as a part of the Rapid ASKAP Continuum Survey (RACS), we searched for radio counterparts to a sample of optically discovered TDEs. …”
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1969
Long-wavelength VCSELs with buried tunnel junction: design optimization
Published 2025-01-01“…A modified SC design was also used for 2D VCSEL arrays applied as a short wave infrared illuminator. …”
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1970
A portable biosensor for simultaneous diagnosis of TNF-<i>α</i> and IL-1<i>β</i> in saliva biomarkers using twin electronic devices
Published 2024-12-01“…In this research, we present a sensor platform model that can enable one to detect biomarkers quickly; specifically, this platform can be used to detect TNF-<span class="inline-formula"><i>α</i></span> and IL-1<span class="inline-formula"><i>β</i></span> in saliva. …”
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1971
Serum profiling of the antibody response to HPV in women with or without abnormal cervical cytology undergoing cervical cancer screening
Published 2025-07-01“…This study aimed to profile the humoral immune response to the proteomes of 12 HPV types in women with or without abnormal cervical cytology undergoing cervical cancer screening.MethodsTo detect serum antibodies (Abs) against HPV, we developed custom HPV high-density diffusion-free nucleic acid programmable protein arrays (HD-NAPPA) displaying the proteomes of 2 low-risk (HPV6 and 11) and 10 high-risk (HR) HPV types (HPV16, 18, 31, 33, 35, 39, 45, 51, 52 and 58). …”
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1972
X-Ray and Optical Polarization Aligned with the Radio Jet Ejecta in GX 339–4
Published 2025-01-01“…We also detect a discrete jet knot from radio observations with the Australia Telescope Compact Array taken later in time; this knot would have been ejected from the system around the same time as the hard-to-soft X-ray state transition, and a bright radio flare occurred ∼3 months earlier. …”
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1973
Design and Implementation of a Low-Power Biopotential Amplifier in 28 nm CMOS Technology with a Compact Die-Area of 2500 μm<sup>2</sup> and an Ultra-High Input Impedance
Published 2025-04-01“…Neural signal recording demands compact, low-power, high-performance amplifiers, to enable large-scale, multi-channel electrode arrays. This work presents a bioamplifier optimized for action potential detection, designed using TSMC 28 nm HPC CMOS technology. …”
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1974
The ALMA-CRISTAL Survey: Weak Evidence for Star-formation-driven Outflows in z ∼ 5 Main-sequence Galaxies
Published 2025-01-01“…To this end, we utilize deep, high-resolution [C II ] emission-line data taken as part of the [C II ] resolved interstellar medium (ISM) in star-forming galaxies with the Atacama Large Millimeter/submillimeter Array (CRISTAL) survey. Excluding sources with kinematic evidence for gravitational interactions, we perform a rigorous stacking analysis of the remaining 15 galaxies to search for broad emission features that are too weak to detect in the individual spectra, finding only weak evidence that a broad component is needed to explain the composite spectrum. …”
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1975
Early Planet Formation in Embedded Disks (eDisk). XXI. Limited Role of Streamers in Mass Supply to the Disk in the Class 0 Protostar IRAS 16544-1604
Published 2025-01-01“…By combining data from the James Clerk Maxwell Telescope (JCMT) and Atacama Large Millimeter/submillimeter Array (ALMA), we investigate the physical properties of the streamers and parental dense core in the Class 0 protostar, IRAS 16544–1604. …”
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1976
Monitoring Livestock Health by Modeling Rumination Behavior According to Accelerometer-Based Information
Published 2025-06-01“…Finally, the performance of the final model and sensor was evaluated in the field for a few days.Results and DiscussionAfter calculating the evaluation criteria for different calculation factors, four optimal factors were finally selected from the 50 arrays. Muzzle mode was found to be the best place to install the sensor. …”
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1977
Ultrasensitive bionic photonic-electronic skin with wide red-shift mechanochromic response
Published 2025-08-01“…The PC layer containing in-plane-spaced and interplane-packed nanoparticle arrays was fabricated via a fast, facile, combined method of “Marangoni self-assembly”, “plasma etching”, and “adhesive PDMS transfer”. …”
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1978
ALESS-JWST: Joint (Sub)kiloparsec JWST and ALMA Imaging of z ~ 3 Submillimeter Galaxies Reveals Heavily Obscured Bulge Formation Events
Published 2025-01-01“…\limits^{^{\prime\prime} }$ 16) Atacama Large Millimeter/submillimeter Array 870 μ m imaging. The 2.0–4.4 μ m (observed frame) NIRCam imaging reveals the rest-frame near-infrared stellar emission in these submillimeter-selected galaxies at the same (sub)kiloparsec resolution as the 870 μ m dust continuum. …”
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1979
UNCOVER: Candidate Red Active Galactic Nuclei at 3 < z < 7 with JWST and ALMA
Published 2024-01-01“…Of the 20 sources with deep Atacama Large Millimeter/submillimeter Array (ALMA) 1.2 mm coverage, none are detected individually or in a stack. …”
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1980
GOALS-JWST: The Warm Molecular Outflows of the Merging Starburst Galaxy NGC 3256
Published 2024-01-01“…The gas mass of the warm H _2 outflow component is estimated to be M _warm _,out = (1.4 ± 0.2) × 10 ^6 M _⊙ , as much as 6% of the cold H _2 mass estimated using Atacama Large Millimeter/submillimeter Array CO data. The outflow timescale is about 7 × 10 ^5 yr, resulting in a mass outflow rate ${\dot{M}}_{\mathrm{warm},\mathrm{out}}=2.0\pm 0.8\,{M}_{\odot }\,{\mathrm{yr}}^{-1}$ and kinetic power P _warm,out ∼ 4 × 10 ^41 erg s ^−1 . …”
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