Search Results - "Pharo, John"
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1
Finding Peas in the Early Universe with JWST
Published in Astrophysical journal. Letters (01-01-2023)“…Abstract The Early Release Observations (EROs) of JWST beautifully demonstrate the promise of JWST in characterizing the universe at Cosmic Dawn. We analyze…”
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2
Dwarf Galaxies Show Little ISM Evolution from z ∼ 1 to z ∼ 0: A Spectroscopic Study of Metallicity, Star Formation, and Electron Density
Published in The Astrophysical journal (01-12-2023)“…Abstract We present gas-phase metallicity measurements for 583 emission line galaxies at 0.3 < z < 0.85, including 388 dwarf galaxies with log ( M ⋆ / M ⊙ ) <…”
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3
The Neon Gap: Probing Ionization with Dwarf Galaxies at z ∼ 1
Published in Astrophysical journal. Letters (01-03-2023)“…Abstract We present measurements of [Ne iii ] λ 3869 emission in z ∼ 1 low-mass galaxies taken from the Keck/DEIMOS spectroscopic surveys HALO7D and DEEPwinds…”
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4
FIGS-Faint Infrared Grism Survey: Description and Data Reduction
Published in The Astrophysical journal (01-09-2017)“…The Faint Infrared Grism Survey (FIGS) is a deep Hubble Space Telescope (HST) WFC3/IR (Wide Field Camera 3 Infrared) slitless spectroscopic survey of four deep…”
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5
The Lyα Luminosity Function and Cosmic Reionization at z ∼ 7.0: A Tale of Two LAGER Fields
Published in The Astrophysical journal (01-12-2019)“…Abstract We present the largest-ever sample of 79 Ly α emitters (LAEs) at z ∼ 7.0 selected in the COSMOS and CDFS fields of the LAGER project (the Lyman Alpha…”
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6
LAGER Lyα Luminosity Function at z ∼ 7: Implications for Reionization
Published in The Astrophysical journal (01-03-2022)“…Abstract We present a new measurement of the Ly α luminosity function (LF) at redshift z = 6.9, finding moderate evolution from z = 5.7 that is consistent with…”
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7
The Ly Luminosity Function and Cosmic Reionization at z ∼ 7.0: A Tale of Two LAGER Fields
Published in The Astrophysical journal (01-12-2019)“…We present the largest-ever sample of 79 Ly emitters (LAEs) at z ∼ 7.0 selected in the COSMOS and CDFS fields of the LAGER project (the Lyman Alpha Galaxies in…”
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Journal Article -
8
A Lyman-α protocluster at redshift 6.9
Published in Nature astronomy (01-05-2021)“…Protoclusters, the progenitors of the most massive structures in the Universe, have been identified at redshifts of up to 6.6 (refs. 1 – 6 ). Besides…”
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9
New Spectroscopic Confirmations of Lyα Emitters at Z ∼ 7 from the LAGER Survey
Published in The Astrophysical journal (01-08-2022)“…We report spectroscopic confirmations of 15 Lyα galaxies at z ∼ 7, implying a spectroscopic confirmation rate of ∼80% on candidates selected from the Lyα…”
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10
Galaxy Overdensities and Emission Line Galaxies in the Faint Infrared Grism Survey
Published 01-01-2019“…Learning how properties of galaxies such as star formation, galaxy interactions, chemical composition, and others evolve to produce the modern universe has…”
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Dissertation -
11
A Catalog of Emission-line Galaxies from the Faint Infrared Grism Survey: Studying Environmental Influence on Star Formation
Published in The Astrophysical journal (10-01-2020)“…We present a catalog of 208 0.3 < z < 2.1 emission-line galaxies (ELGs) selected from 1D slitless spectroscopy obtained using Hubble's WFC3 G102 grism, as part…”
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12
The Dwarf Galaxy Population at z ∼ 0.7: A Catalog of Emission Lines and Redshifts from Deep Keck Observations
Published in The Astrophysical journal. Supplement series (01-08-2022)“…Abstract We present a catalog of spectroscopically measured redshifts over 0 < z < 2 and emission-line fluxes for 1440 galaxies. The majority (∼65%) of the…”
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13
Hα Emitting Galaxies at z ∼ 0.6 in the Deep And Wide Narrow-band Survey
Published in The Astrophysical journal (10-05-2018)“…Abstract We present new measurements of the H α luminosity function (LF) and star formation rate (SFR) volume density for galaxies at z ∼ 0.62 in the COSMOS…”
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14
Discovery of a z = 7.452 High Equivalent Width Lyα Emitter from the Hubble Space Telescope Faint Infrared Grism Survey
Published in The Astrophysical journal (10-05-2018)“…Abstract We present the results of an unbiased search for Ly α emission from continuum-selected 5.6 < z < 8.7 galaxies. Our data set consists of 160 orbits…”
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15
FIGS: spectral fitting constraints on the star formation history of massive galaxies since the cosmic noon
Published in Monthly notices of the Royal Astronomical Society (11-06-2019)“…We constrain the stellar population properties of a sample of 52 massive galaxies – with stellar mass log (M(s)/M(⊙)) ≳ 10.5 – over the redshift range 0.5 < z…”
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16
Emission-line Metallicities from the Faint Infrared Grism Survey and VLT/MUSE
Published in The Astrophysical journal (01-04-2019)“…We derive direct-measurement gas-phase metallicities of for 14 low-mass emission-line galaxies at 0.3 < z < 0.8 identified in the Faint Infrared Grism Survey…”
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A Comprehensive Study of H Emitters at z ∼ 0.62 in the DAWN Survey: The Need for Deep and Wide Regions
Published in The Astrophysical journal (23-03-2020)“…We present new estimates of the luminosity function (LF) and star formation rate density (SFRD) for an H -selected sample at z ∼ 0.62 from the Deep And Wide…”
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18
A Two-dimensional Spectroscopic Study of Emission-line Galaxies in the Faint Infrared Grism Survey (FIGS). I. Detection Method and Catalog
Published in The Astrophysical journal (20-11-2018)“…We present the results from the application of a two-dimensional emission line detection method, EMission-line two-Dimensional (EM2D), to the near-infrared…”
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Design for the First Narrowband Filter for the Dark Energy Camera: Optimizing the LAGER Survey for z ∼ 7 Galaxies
Published in Publications of the Astronomical Society of the Pacific (01-07-2019)“…We present the design for the first narrowband filter, NB964, for the Dark Energy Camera (DECam), which is operated on the 4-m Blanco Telescope at the Cerro…”
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A Comprehensive Study of Hα Emitters at z ∼ 0.62 in the DAWN Survey: The Need for Deep and Wide Regions
Published in The Astrophysical journal (20-03-2020)“…Abstract We present new estimates of the luminosity function (LF) and star formation rate density (SFRD) for an H α -selected sample at z ∼ 0.62 from the Deep…”
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