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Nick P. Konidaris

Researcher at California Institute of Technology

Publications -  15
Citations -  1028

Nick P. Konidaris is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Redshift & Galaxy. The author has an hindex of 9, co-authored 15 publications receiving 960 citations.

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Line Emitting Galaxies Beyond a Redshift of 7: An Improved Method for Estimating the Evolving Neutrality of the Intergalactic Medium

TL;DR: In this article, an improved method was proposed based on the measured slopes of the rest-frame ultraviolet continua of galaxies to interpret the growing body of near-infrared spectra of z > 7 galaxies.
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ANALYSIS OF THE EARLY-TIME OPTICAL SPECTRA OF SN 2011fe IN M101

TL;DR: In this article, the authors studied the early evolution of a "normal" SN Ia, its compositional structure, and its elusive progenitor system using high signal-to-noise spectra.
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The SED Machine: a robotic spectrograph for fast transient classification

TL;DR: The Spectral Energy Distribution Machine (SEDM) as mentioned in this paper was designed and operated on the Palomar 60-inch telescope (P60) for spectral classification and high observing efficiency.
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Contamination of broadband photometry by nebular emission in high-redshift galaxies: Investigations with Keck's Mosfire near-infrared spectrograph

TL;DR: In this article, the spectral energy distribution (SED) fitting technique was used to estimate the rest-frame equivalent widths (EWs) of [O III] emission of a sample of 28 3.0 < z < 3.8 Lyman break galaxies using the MOSFIRE near-infrared spectrograph at the Keck I telescope.
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MOSFIRE ABSORPTION LINE SPECTROSCOPY OF z > 2 QUIESCENT GALAXIES: PROBING A PERIOD OF RAPID SIZE GROWTH

TL;DR: In this paper, the authors used the MOSFIRE near-infrared multi-slit spectrograph on the Keck 1 Telescope to obtain high signal-to-noise ratio absorption line spectra for six massive galaxies with redshift 2 < z < 2.