Progress on background-limited membrane-isolated TES bolometers for far-IR/submillimeter spectroscopy

Submillimeter Spectroscopy of To-Phonon Mode Softening in PbTe

1976 International Conference on Submillimeter Waves and Their Applications ◽

10.1109/icswa.1976.9350051 ◽

1976 ◽

Author(s):

G. Bauer ◽

H. Burkhard ◽

A. Lopez-Otero

Keyword(s):

Phonon Mode ◽

Mode Softening ◽

Submillimeter Spectroscopy

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Submillimeter Spectroscopy in the Liquid and Solid State with a Tunable Optically Pumped Laser

1976 International Conference on Submillimeter Waves and Their Applications ◽

10.1109/icswa.1976.9350040 ◽

1976 ◽

Author(s):

B. L. Bean ◽

S. Perkowitz

Keyword(s):

Solid State ◽

Optically Pumped ◽

Optically Pumped Laser ◽

Submillimeter Spectroscopy

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On the road to the large deployable reflector (LDR): The utility of balloon-borne platforms for far-infrared and submillimeter spectroscopy

International Journal of Infrared and Millimeter Waves ◽

10.1007/bf01010660 ◽

1988 ◽

Vol 9 (9) ◽

pp. 781-812 ◽

Cited By ~ 3

Author(s):

Gary J. Melnick

Keyword(s):

Far Infrared ◽

The Road ◽

Submillimeter Spectroscopy ◽

On The Road ◽

Deployable Reflector

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Electrical and Thermal Characterization of Membrane-Isolated, Antenna-Coupled, TES Bolometers for the SPIDER Experiment

Journal of Low Temperature Physics ◽

10.1007/s10909-007-9623-3 ◽

2008 ◽

Vol 151 (1-2) ◽

pp. 138-143 ◽

Cited By ~ 5

Author(s):

J. A. Bonetti ◽

P. Day ◽

M. Kenyon ◽

A. Turner ◽

H. G. LeDuc ◽

...

Keyword(s):

Thermal Characterization ◽

Tes Bolometers

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New Techniques and Applications for High Resolution Tunable Submillimeter Spectroscopy

Laser Spectroscopy V - Springer Series in Optical Sciences ◽

10.1007/978-3-540-38804-3_11 ◽

1981 ◽

pp. 76-80 ◽

Cited By ~ 1

Author(s):

H. R. Fetterman ◽

W. A. M. Blumberg

Keyword(s):

High Resolution ◽

New Techniques ◽

Submillimeter Spectroscopy

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A frequency domain multiplexing system to readout the TES bolometers on the LSPE/SWIPE experiment

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment ◽

10.1016/j.nima.2018.10.116 ◽

2019 ◽

Vol 936 ◽

pp. 169-171 ◽

Cited By ~ 1

Author(s):

D. Vaccaro ◽

A.M. Baldini ◽

F. Cei ◽

L. Galli ◽

M. Grassi ◽

...

Keyword(s):

Frequency Domain ◽

Frequency Domain Multiplexing ◽

Tes Bolometers

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Submillimeter spectroscopy of tilted Nd1.85Ce0.15CuO4−δ films: Observation of a mixed ac-plane excitation

Applied Physics Letters ◽

10.1063/1.126999 ◽

2000 ◽

Vol 77 (3) ◽

pp. 429-431 ◽

Cited By ~ 5

Author(s):

A. Pimenov ◽

A. V. Pronin ◽

A. Loidl ◽

A. P. Kampf ◽

S. I. Krasnosvobodtsev ◽

...

Keyword(s):

Submillimeter Spectroscopy

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Millimeter and Submillimeter Spectroscopy in Support of Upper Atmospheric Research

Spectroscopy from Space ◽

10.1007/978-94-010-0832-7_4 ◽

2001 ◽

pp. 59-71 ◽

Cited By ~ 1

Author(s):

Edward A. Cohen

Keyword(s):

Atmospheric Research ◽

Submillimeter Spectroscopy

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Submillimeter spectroscopy of the electron excitationsin rare-earth orthoferrites

18th International Conference on Infrared and Millimeter Waves ◽

10.1117/12.2298749 ◽

2017 ◽

Author(s):

G. V. Kozlov

Keyword(s):

Rare Earth ◽

Submillimeter Spectroscopy

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Molecular Outflows

International Astronomical Union Colloquium ◽

10.1017/s0252921100023794 ◽

1989 ◽

Vol 120 ◽

pp. 231-243

Author(s):

Ronald L. Snell

Keyword(s):

Carbon Monoxide ◽

Sound Speed ◽

Molecular Clouds ◽

Molecular Form ◽

Line Profiles ◽

Internal Dynamics ◽

Molecular Outflows ◽

Submillimeter Spectroscopy ◽

Line Widths ◽

Co Emission

The development of millimeter and submillimeter spectroscopy has allowed astronomers to probe the cold, dense component of the interstellar medium. This medium, primarily composed of gas in molecular form, is gravitationally bound into relatively distinct clouds that are sites of star formation within our Galaxy. The most ubiquitous tracers of these molecular clouds are the rotational transitions of carbon monoxide. Observations of CO emission have been commonly used to estimate the size, temperature, mass, and density of molecular clouds; in addition, the spectral line profiles can be used to study the internal dynamics of these clouds. Although the sound speed within molecular clouds is only about 0.2 km s−1, observed CO line widths are more typically 1 to 5 km s−1. Thus, the internal dynamics of molecular clouds are characterized by supersonic gas motions whose nature is poorly understood.

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