Search Results - "Jordan, C J"
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Spectroscopy and dynamics of the hydrated electron at the water/air interface
Published in Nature communications (02-01-2024)“…The hydrated electron, e – (aq) , has attracted much attention as a central species in radiation chemistry. However, much less is known about e – (aq) at the…”
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Star Formation and AGN Activity 500 Myr after the Big Bang: Insights from JWST
Published in Astrophysical journal. Letters (01-12-2023)“…We consider the effect of including an active galactic nuclei (AGN) component when fitting spectral energy distributions of 109 spectroscopically confirmed z ≈…”
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The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0
Published in The Astrophysical journal (01-02-2024)“…A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z…”
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Author Correction: Spectroscopy and dynamics of the hydrated electron at the water/air interface
Published in Nature communications (15-01-2024)Get full text
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JWST's PEARLS: Bright 1.5–2.0 μm Dropouts in the Spitzer/IRAC Dark Field
Published in Astrophysical journal. Letters (01-01-2023)“…Using the first epoch of four-band NIRCam observations obtained by the James Webb Space Telescope (JWST) Prime Extragalactic Areas for Reionization and Lensing…”
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JWST View of Four Infant Galaxies at z = 8.31–8.49 in the MACS J0416.1−2403 Field and Implications for Reionization
Published in The Astrophysical journal (01-11-2024)“…New JWST/NIRCam wide-field slitless spectroscopy provides redshifts for four z > 8 galaxies located behind the lensing cluster MACS J0416.1−2403. Two of them,…”
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PEARLS: Discovery of Point-source Features within Galaxies in the North Ecliptic Pole Time Domain Field
Published in The Astrophysical journal (01-10-2024)“…The first public 0.9–4.4 μ m NIRCam images of the North Ecliptic Pole Time Domain Field uncovered galaxies displaying point-source features in their cores as…”
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PEARLS: JWST Counterparts of Microjansky Radio Sources in the Time Domain Field
Published in The Astrophysical journal (01-12-2023)“…The Time Domain Field (TDF) near the North Ecliptic Pole in JWST’s continuous-viewing zone will become a premier “blank field” for extragalactic science…”
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Allophycocyanin A is a carbon dioxide receptor in the cyanobacterial phycobilisome
Published in Nature communications (08-09-2022)“…Light harvesting is fundamental for production of ATP and reducing equivalents for CO 2 fixation during photosynthesis. However, electronic energy transfer…”
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Inhomogeneous Galactic chemical evolution: modelling ultra-faint dwarf galaxies of the Large Magellanic Cloud
Published in Monthly notices of the Royal Astronomical Society (11-05-2023)“…ABSTRACT Ultra-faint dwarf galaxies (UFDs) are among the oldest and most metal-poor galaxies in the cosmos, observed to contain no gas and a high dark matter…”
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A Combined Spectrophotometer and Fluorometer to Demonstrate the Principles of Absorption Spectroscopy
Published in Journal of chemical education (14-12-2021)“…A dual-function student-crafted instrument is described as part of a laboratory activity aimed to teach both the principles and practical aspects of absorption…”
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Airway injury associated with cervical bite wounds in dogs and cats: 56 cases
Published in Veterinary and comparative orthopaedics and traumatology (01-01-2013)“…To investigate the frequency of airway injury and damage to other vital structures associated with cervical bite wounds in dogs and cats and the implications…”
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Unveiling the main sequence of galaxies at z ≥ 5 with the JWST : predictions from simulations
Published in Monthly notices of the Royal Astronomical Society (01-01-2023)“…We use two independent galaxy-formation simulations, flares, a cosmological hydrodynamical simulation, and shark, a semi-analytic model, to explore how well…”
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EPOCHS. II. The Ultraviolet Luminosity Function from 7.5 < z < 13.5 Using 180 arcmin2 of Deep, Blank Fields from the PEARLS Survey and Public JWST Data
Published in The Astrophysical journal (01-04-2024)“…We present an analysis of the ultraviolet luminosity function (UV LF) and star formation rate density of distant galaxies (7.5 < z < 13.5) in the “blank”…”
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Hidden Giants in JWST's PEARLS: An Ultramassive z = 4.26 Submillimeter Galaxy that Is Invisible to HST
Published in The Astrophysical journal (01-11-2023)“…We present a multiwavelength analysis using the Submillimeter Array (SMA), James Clerk Maxwell Telescope, NOEMA, JWST, the Hubble Space Telescope (HST), and…”
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GAMA/DEVILS: cosmic star formation and AGN activity over 12.5 billion years
Published in Monthly notices of the Royal Astronomical Society (04-07-2023)“…ABSTRACT We use the Galaxy and Mass Assembly (GAMA) and the Deep Extragalactic Visible Legacy Survey (DEVILS) observational data sets to calculate the cosmic…”
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EPOCHS VII: discovery of high-redshift (6.5 < z < 12) AGN candidates in JWST ERO and PEARLS data
Published in Monthly notices of the Royal Astronomical Society (09-08-2023)“…ABSTRACT We present an analysis of a sample of robust high-redshift galaxies selected from the ‘blank’ fields of the Prime Extragalactic Areas for Reionization…”
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Forecasting the magnitude of potential landslides based on InSAR techniques
Published in Remote sensing of environment (01-05-2020)“…A new method, combining empirical modeling with time series Interferometric Synthetic Aperture Radar (InSAR) data, is proposed to provide an assessment of…”
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EPOCHS IX. When cosmic dawn breaks: evidence for evolved stellar populations in 7 < z < 12 galaxies from PEARLS GTO and public NIRCam imaging
Published in Monthly notices of the Royal Astronomical Society (01-02-2024)“…ABSTRACT The presence of evolved stars in high-redshift galaxies can place valuable indirect constraints on the onset of star formation in the Universe. Thus,…”
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Birds of a Feather: Resolving Stellar Mass Assembly with JWST/NIRCam in a Pair of Kindred z ∼ 2 Dusty Star-forming Galaxies Lensed by the PLCK G165.7+67.0 Cluster
Published in The Astrophysical journal (01-09-2024)“…We present a new parametric lens model for the G165.7+67.0 galaxy cluster, which was discovered with Planck through its bright submillimeter flux, originating…”
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