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19561
UV-bright Star-forming Clumps and Their Host Galaxies in UVCANDELS at 0.5 ≤ z ≤ 1
Published 2023-01-01“…Using the Hubble Space Telescope/Wide Field Camera 3 F275W images from the Ultraviolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey, we detect and analyze giant star-forming clumps in galaxies at 0.5 ≤ z ≤ 1, connecting two epochs when clumps are common (at cosmic high noon, z ∼ 2) and rare (in the local Universe). …”
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19562
A Spatially Resolved Analysis of Star Formation Burstiness by Comparing UV and Hα in Galaxies at z ∼ 1 with UVCANDELS
Published 2023-01-01“…The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) program provides Hubble Space Telescope (HST)/UVIS F275W imaging for four CANDELS fields. …”
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19563
Identification of 1RXS J165424.6-433758 as a Polar Cataclysmic Variable
Published 2023-01-01“…We present the results of our X-ray, ultraviolet, and optical follow-up campaigns of 1RXS J165424.6-433758, an X-ray source detected with the Swift Deep Galactic Plane Survey. …”
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19564
Evaluating the contamination level of total petroleum hydrocarbons (TPHs) and heavy metals in coastal sediments of Tiab Mangroves (Hormozgan Province)
Published 2019-03-01“…TPHs and heavy metal concentrations (Pb, Zn, Cr, Ni, V) in sediment samples were quantified using Ultraviolet Fluorescence Spectroscopy (UFS) and Inductively Coupled Plasma-Optical Emission Spectrometry (ICP-OES), respectively. …”
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19565
SN 2022joj: A Peculiar Type Ia Supernova Possibly Driven by an Asymmetric Helium-shell Double Detonation
Published 2023-01-01“…Despite the blue optical-band colors, SN 2022joj exhibits extremely red ultraviolet minus optical colors at maximum luminosity ( u − v ≃ 0.6 mag and uvw 1 − v ≃ 2.5 mag), suggesting a suppression of flux at ∼2500–4000 Å. …”
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19566
Asteroseismology and Spectropolarimetry of the Exoplanet Host Star λ Serpentis
Published 2023-01-01“…We reanalyze the complete time series of chromospheric activity measurements from the Mount Wilson Observatory, and we present new X-ray and ultraviolet observations from the Chandra and Hubble space telescopes. …”
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19567
The micro-LED roadmap: status quo and prospects
Published 2023-01-01“…The innovation in epitaxy, such as the tunnel junction, the direct epitaxy and nitride-based quantum wells for red and ultraviolet, can provide critical solutions to the micro-LED performance in various aspects. …”
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19568
PHANGS–JWST First Results: A Combined HST and JWST Analysis of the Nuclear Star Cluster in NGC 628
Published 2023-01-01“…We combine archival Hubble Space Telescope and new James Webb Space Telescope imaging data covering the ultraviolet to mid-infrared regime to morphologically analyze the nuclear star cluster (NSC) of NGC 628, a grand-design spiral galaxy. …”
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19569
Evaluation of the daytime tropospheric loss of 2-methylbutanal
Published 2022-03-01“…In this work, we report the rate coefficients for the gas-phase reaction of 2 MB with OH (<span class="inline-formula"><i>k</i><sub>OH</sub></span>) and Cl (<span class="inline-formula"><i>k</i><sub>Cl</sub></span>), together with the photolysis rate coefficient (<span class="inline-formula"><i>J</i></span>), in the ultraviolet solar actinic region in Valencia (Spain) at different times of the day. …”
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19570
EUNADICS-AV early warning system dedicated to supporting aviation in the case of a crisis from natural airborne hazards and radionuclide clouds
Published 2021-11-01“…Satellite products from hyperspectral ultraviolet–visible (UV–vis) and infrared (IR) sensors (e.g. …”
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19571
InGaN/GaN light-emitting diodes : from modeling to their hybrid applications with novel nanomaterials
Published 2017“…In last two decades, InGaN/GaN light-emitting diodes have been one of the main focus of research thanks to their low power consumption, high efficiency, long lifetime, high color purity and color quality, narrow luminescence, possibility to tune the emission wavelength from near ultraviolet to green by increasing the In content, and several other promising properties. …”
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Thesis -
19572
Studies on nucleocytoplasmic relationships during differentiation in vertebrates (1961)
Published 1961“…(iii) the unfertilised recipient eggs are "enucleated" by a short exposure of their animal hemisphere to ultraviolet irradiation. There are many reasons for believing that this irradiation treatment has no effect on the egg cytoplasm. …”
Thesis -
19573
Growth performance morphomeristic and genetic characterization of crossbreeding between gift and UPM red tilapia
Published 2018“…The extracted DNAs were viewed in a gel electrophoresis under ultraviolet light using Gel doc XR system Pc and Mac from USA for the qualitative validation. …”
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Thesis -
19574
Wastewater treatment
Published 2013-10-01“…To improve the taste of distilled water, <em>aeration</em> should be performed. The sun’s ultraviolet rays destroy biological pollutants. Mechanical, biological and chemical methods are used for water purification.…”
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19575
An approach to sulfate geoengineering with surface emissions of carbonyl sulfide
Published 2022-05-01“…According to the model results, the resulting ultraviolet B (UVB) perturbation at the surface accounts for <span class="inline-formula">−</span>4.3 % as a global and annual average (versus <span class="inline-formula">−</span>2.4 % in the SG-SO2 case), with a springtime Antarctic decrease of <span class="inline-formula">−</span>2.7 % (versus a <span class="inline-formula">+</span>5.8 % increase in the SG-SO2 experiment). …”
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19576
Treatment of drug residues (emerging contaminants) in hospital effluent by the combination of biological and physiochemical treatment process: a review
Published 2021-07-01“…Based on test results, two out of different treatment effectively reducing conventional parameters and pharmaceuticals from secondary and tertiary treatments except regeneration of microbes were observed in the tertiary level by these two treatments were studies followed by ozonation and ultraviolet-ray treatment.…”
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19577
Quasar Luminosity Function at z = 7
Published 2023-01-01“…The sample of 22 quasars from the Subaru High- z Exploration of Low-Luminosity Quasars (SHELLQs) project, combined with 13 brighter quasars in the literature, covers an unprecedentedly wide range of rest-frame ultraviolet magnitudes over −28 < M _1450 < −23. We found that the binned LF flattens significantly toward the faint end populated by the SHELLQs quasars. …”
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19578
JWST’s PEARLS: A JWST/NIRCam View of ALMA Sources
Published 2023-01-01“…The counterparts’ spectral energy distributions cover from rest-frame ultraviolet to near-IR and provide photometric redshifts (1 < z < 4.5) and stellar masses ( M _* > 10 ^10.5 M _⊙ ), which are similar to submillimeter galaxies (SMGs) studied previously. …”
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19579
Two-Dimensional Octuple-Atomic-Layer M<sub>2</sub>Si<sub>2</sub>N<sub>4</sub> (M = Al, Ga and In) with Long Carrier Lifetime
Published 2023-02-01“…Moreover, Al<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>2</mn></msub></semantics></math></inline-formula>Si<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>2</mn></msub></semantics></math></inline-formula>N<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>4</mn></msub></semantics></math></inline-formula> and In<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>2</mn></msub></semantics></math></inline-formula>Si<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>2</mn></msub></semantics></math></inline-formula>N<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>4</mn></msub></semantics></math></inline-formula> have good absorption ability in the visible light region, while Ga<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>2</mn></msub></semantics></math></inline-formula>Si<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>2</mn></msub></semantics></math></inline-formula>N<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>4</mn></msub></semantics></math></inline-formula> is an ultraviolet-light-absorbing material. Furthermore, the carrier lifetimes of Ga<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>2</mn></msub></semantics></math></inline-formula>Si<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>2</mn></msub></semantics></math></inline-formula>N<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>4</mn></msub></semantics></math></inline-formula> and In<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>2</mn></msub></semantics></math></inline-formula>Si<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>2</mn></msub></semantics></math></inline-formula>N<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mrow></mrow><mn>4</mn></msub></semantics></math></inline-formula> are as large as 157.89 and 103.99 ns, respectively. …”
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19580
Marine organic matter in the remote environment of the Cape Verde islands – an introduction and overview to the MarParCloud campaign
Published 2020-06-01“…Lipids, sugar-like compounds, UV-absorbing (UV: ultraviolet) humic-like substances and low-molecular-weight neutral components were important organic compounds in the seawater, and highly surface-active lipids were enriched within the SML. …”
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