activity
20132021
most citedThe HETDEX Instrumentation: Hobby-Eberly Telescope Wide Field Upgrade and VIRUS

151 citations · 215 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM2021★ 151 cited

The HETDEX Instrumentation: Hobby-Eberly Telescope Wide Field Upgrade and VIRUS

Gary J. Hill, Hanshin Lee, Phillip J. MacQueen +46

The Hobby-Eberly Telescope (HET) Dark Energy Experiment (HETDEX) is undertaking a blind wide-field low-resolution spectroscopic survey of 540 square degrees of sky to identify and…

astro-ph.HE2020★ 6 cited

Medium-band observation of the neutrino emitting blazar, TXS 0506+056

Sungyong Hwang, Myungshin Im, Yoon Chan Taak +15

TXS 0506+056 is a blazar that has been recently identified as the counterpart of the neutrino event IceCube-170922A. Understanding blazar type of TXS 0506+056 is important to const…

astro-ph.IM2018★ 1 cited

Systems engineering applied to ELT instrumentation: The GMACS case

D. M. Faes, A. Souza, C. Froning +14

An important tool for the development of the next generation of extremely large telescopes (ELTs) is a robust Systems Engineering (SE) methodology. GMACS is a first-generation mult…

astro-ph.IM2014★ 35 cited

Characterization of the Reflectivity of Various Black Materials

Jennifer L. Marshall, Patrick Williams, Jean-Philippe Rheault +3

We present total and specular reflectance measurements of various materials that are commonly (and uncommonly) used to provide baffling and/or to minimize the effect of stray light…

astro-ph.IM2014★ 15 cited

Mass production of volume phase holographic gratings for the VIRUS spectrograph array

Taylor S. Chonis, Amy Frantz, Gary J. Hill +7

The Visible Integral-field Replicable Unit Spectrograph (VIRUS) is a baseline array of 150 copies of a simple, fiber-fed integral field spectrograph that will be deployed on the Ho…

astro-ph.IM2013★ 1 cited

aTmcam: A Simple Atmospheric Transmission Monitoring Camera For Sub 1% Photometric Precision

Ting Li, D. L. DePoy, R. Kessler +8

Traditional color and airmass corrections can typically achieve ~0.02 mag precision in photometric observing conditions. A major limiting factor is the variability in atmospheric t…