Materials Map

Discover the materials research landscape. Find experts, partners, networks.

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The Materials Map is an open tool for improving networking and interdisciplinary exchange within materials research. It enables cross-database search for cooperation and network partners and discovering of the research landscape.

The dashboard provides detailed information about the selected scientist, e.g. publications. The dashboard can be filtered and shows the relationship to co-authors in different diagrams. In addition, a link is provided to find contact information.

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Materials Map under construction

The Materials Map is still under development. In its current state, it is only based on one single data source and, thus, incomplete and contains duplicates. We are working on incorporating new open data sources like ORCID to improve the quality and the timeliness of our data. We will update Materials Map as soon as possible and kindly ask for your patience.

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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (2/2 displayed)

  • 2020The Terahertz Intensity Mapper (TIM): a Next-Generation Experiment for Galaxy Evolution Studiescitations
  • 2018Design and Characterization of a Balloon-Borne Diffraction-Limited Submillimeter Telescope Platform for BLAST-TNGcitations

Places of action

Chart of shared publication
Angile, Francisco E.
1 / 1 shared
Ashton, Peter C.
1 / 1 shared
Catanzaro, Brian
1 / 1 shared
Devlin, Mark J.
1 / 2 shared
Lourie, Nathan P.
1 / 1 shared
Soler, Juan D.
1 / 1 shared
Romualdez, L. Javier
1 / 1 shared
Williams, Paul A.
1 / 1 shared
Galitzki, Nicholas
1 / 1 shared
Klein, Jeffrey
1 / 1 shared
Gordon, Samuel
1 / 1 shared
Dicker, Simon
1 / 1 shared
Didier, Joy
1 / 1 shared
Lowe, Ian
1 / 1 shared
Dober, Bradley
1 / 1 shared
Novak, Giles
1 / 1 shared
Fissel, Laura M.
1 / 1 shared
Nati, Federico
1 / 2 shared
Chart of publication period
2020
2018

Co-Authors (by relevance)

  • Angile, Francisco E.
  • Ashton, Peter C.
  • Catanzaro, Brian
  • Devlin, Mark J.
  • Lourie, Nathan P.
  • Soler, Juan D.
  • Romualdez, L. Javier
  • Williams, Paul A.
  • Galitzki, Nicholas
  • Klein, Jeffrey
  • Gordon, Samuel
  • Dicker, Simon
  • Didier, Joy
  • Lowe, Ian
  • Dober, Bradley
  • Novak, Giles
  • Fissel, Laura M.
  • Nati, Federico
OrganizationsLocationPeople

document

The Terahertz Intensity Mapper (TIM): a Next-Generation Experiment for Galaxy Evolution Studies

  • Lagache, Guilaine
  • Chang, Tzu-Ching
  • Dore, Oliver
  • Groppi, Christopher
  • Bradford, C. Matt
  • Shirokoff, Erik
  • Bethermin, Matthieu
  • Fu, Jianyang Frank
  • Trumper, Isaac
  • Holder, Gilbert
  • Zmuidzinas, Jonas
  • Keenan, Ryan
  • Vieira, Joaquin
  • Narayanan, Desika
  • Aguirre, James
  • Filippini, Jeffrey
  • Somerville, Rachel
  • Hailey Dunsheath, Steven
  • Marrone, Dan
  • Uzgil, Bade
  • Keating, Garrett
  • Kovetz, Ely
  • Mauskopf, Philip
  • Devlin, Mark
  • Popping, Gergo
Abstract

Understanding the formation and evolution of galaxies over cosmic time is one of the foremost goals of astrophysics and cosmology today. The cosmic star formation rate has undergone a dramatic evolution over the course of the last 14 billion years, and dust obscured star forming galaxies (DSFGs) are a crucial component of this evolution. A variety of important, bright, and unextincted diagnostic lines are present in the far-infrared (FIR) which can provide crucial insight into the physical conditions of galaxy evolution, including the instantaneous star formation rate, the effect of AGN feedback on star formation, the mass function of the stars, metallicities, and the spectrum of their ionizing radiation. FIR spectroscopy is technically difficult but scientifically crucial. Stratospheric balloons offer a platform which can outperform current instrument sensitivities and are the only way to provide large-area, wide bandwidth spatial/spectral mapping at FIR wavelengths. NASA recently selected TIM, the Terahertz Intensity Mapper, with the goal of demonstrating the key technical milestones necessary for FIR spectroscopy. The TIM instrument consists of an integral-field spectrometer from 240-420 microns with 3600 kinetic-inductance detectors (KIDs) coupled to a 2-meter low-emissivity carbon fiber telescope. In this paper, we will summarize plans for the TIM experiment's development, test and deployment for a planned flight from Antarctica....

Topics
  • impedance spectroscopy
  • Carbon
  • experiment
  • forming