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3781
Static Properties of 980 nm Vertical Cavity Surface Emitting Lasers With Different Monolithic High Refractive Index Contrast Grating Mirror Designs
Published 2025-01-01“…By supporting a broader range of resonance wavelengths and enabling post-growth wavelength tuning, MHCG-based DBR VCSELs offer significant potential for applications in 2D VCSEL arrays, data transmission, sensing, and imaging.…”
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3782
SO Emission in the Dynamically Perturbed Protoplanetary Disks around CQ Tau and MWC 758
Published 2025-01-01“…We report the serendipitous detection of the SO J _N = 6 _5 –5 _4 (219.949 GHz) rotational transition in archival Atacama Large Millimeter/submillimeter Array observations of the spiral hosting protoplanetary disks around CQ Tau (with ≈4.9 σ significance) and MWC 758 (with ≈3.4 σ significance). …”
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3783
Seismic Mitigation Performance and Damage of Prefabricated Base Isolation Structure Based on the Shaking Table Test
Published 2025-01-01“…ObjectiveImproving the seismic performance of prefabricated reinforced concrete frame structure system has always been a research focus. At present, strengthening the design of beam-column assembly joints and adopting seismic isolation techniques are two different ways to achieve this goal. …”
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3784
Associations of plasma SMOC1 and soluble IL6RA levels with the progression from mild cognitive impairment to dementia
Published 2024-12-01“…Employing a hierarchical clustering approach, we thoroughly evaluated the intercompartmental correlations of 63 distinct inflammation mediators, quantified in paired CSF and plasma samples, using advanced SOMAscan technology. Of the array of mediators investigated, only six mediators (CRP, IL1RAP, ILRL1, IL6RA, PDGFRB, and YKL-40) exhibited robust correlations between the central and peripheral compartments (proximity scores <400). …”
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3785
MINDS: Detection of an Inner Gas Disk Caused by Evaporating Bodies around HD 172555
Published 2025-01-01“…All lines are broadened by Keplerian rotation, pinpointing the gas location. The HD 172555 system serves as a unique laboratory to study the composition of planetesimals, asteroids, and comets beyond the solar system. …”
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3786
Introduction
Published 2019-07-01“…Among decision-making procedures that emerged in the context of spatial planning in the Netherlands was an array of practices commonly referred to as regional design. …”
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3787
Editorial
Published 2025-03-01“…The authors of these articles represent a wide array of countries, each bringing unique insights into science education. …”
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3788
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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3789
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3790
GOALS-JWST: The Warm Molecular Outflows of the Merging Starburst Galaxy NGC 3256
Published 2024-01-01“…We present James Webb Space Telescope (JWST) integral-field spectrograph observations of NGC 3256, a local infrared-luminous late-stage merging system with two nuclei roughly 1 kpc apart, both of which have evidence of cold molecular outflows. …”
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3791
RIOJA. Complex Dusty Starbursts in a Major Merger B14-65666 at z = 7.15
Published 2025-01-01“…Atacama Large Millimeter/submillimeter Array archival data show that the bluer galaxy W is brighter in dust continua than the redder galaxy E, while the tails are bright in [O iii ] 88 μ m. …”
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3792
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3793
UNCOVER: A NIRSpec Census of Lensed Galaxies at z = 8.50–13.08 Probing a High-AGN Fraction and Ionized Bubbles in the Shadow
Published 2024-01-01“…We identify at least two unambiguous and several possible active galactic nucleus (AGN) systems based on X-ray, broad H β , high ionization lines, and excess in the UV LF. …”
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3794
Constraints on the X-Ray and Very-high-energy Gamma-Ray Flux from Supernova Remnant W44
Published 2025-01-01“…We estimate the VHE flux upper limit of ∼1.2 × 10 ^−12 erg s ^−1 cm ^−2 in the 0.5–5.0 TeV range from W44 using data from the Very Energetic Radiation Imaging Telescope Array System. Our nondetection of W44 at VHE wavelengths is in agreement with observations from other imaging atmospheric Cherenkov telescopes and is perhaps consistent with the evolutionary stage of the SNR.…”
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3795
Magnetic Fields in Massive Star-forming Regions (MagMaR). V. The Magnetic Field at the Onset of High-mass Star Formation
Published 2025-01-01“…Using Atacama Large Millimeter/submillimeter Array (ALMA) 250 GHz polarization observations (0 $\mathop{.}…”
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3796
The Circular Kitchen
Published 2024-09-01“…Additionally, they argue that achieving circular design requires a systems approach, encompassing the entire design system from macro to micro levels. …”
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3797
ALMA Lensing Cluster Survey: Physical Characterization of Near-infrared-dark Intrinsically Faint ALMA Sources at z = 2–4
Published 2025-01-01“…We present results from Atacama Large Millimeter/submillimeter Array (ALMA) spectral line-scan observations at 3 mm and 2 mm bands of three near-infrared-dark (NIR-dark) galaxies behind two massive lensing clusters MACS J0417.5-1154 and RXC J0032.1+1808. …”
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3798
COSMOS-Web: The Role of Galaxy Interactions and Disk Instabilities in Producing Starbursts at z < 4
Published 2025-01-01“…For this, we use a sample of 387 galaxies with robust total star formation rate measurements from Herschel, gas masses from the Atacama Large Millimeter/submillimeter Array, stellar masses and redshifts from multiband photometry, and JWST/NIRCam rest-frame optical imaging. …”
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3799
Millimeter Light Curves of Sagittarius A* Observed during the 2017 Event Horizon Telescope Campaign
Published 2022-01-01“…At the same time, interferometric array data from the Atacama Large Millimeter/submillimeter Array and the Submillimeter Array were collected, providing Sgr A* light curves simultaneous with the EHT observations. …”
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3800
First M87 Event Horizon Telescope Results. III. Data Processing and Calibration
Published 2019-01-01“…They are validated through a series of quality assurance tests that show consistency across pipelines and set limits on baseline systematic errors of 2% in amplitude and 1° in phase. …”
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