Large format heterodyne arrays for observing far-infrared lines with SOFIA

C. Walker, C. Kulesa, J. Kloosterman, D. Lesser, T. Cottam, Christopher Groppi, J. Zmuidzinas, M. Edgar, S. Radford, P. Goldsmith, W. Langer, H. Yorke, J. Kawamura, I. Mehdi, D. Hollenbach, J. Stutzki, H. Huebers, J. R. Gao, C. Martin

Research output: Chapter in Book/Report/Conference proceedingConference contribution

3 Citations (Scopus)

Abstract

In the wavelength regime between 60 and 300 microns there are a number of atomic and molecular emission lines that are key diagnostic probes of the interstellar medium. These include transitions of [CII], [NII], [OI], HD, H 2D+, OH, CO, and H2O, some of which are among the brightest global and local far-infrared lines in the Galaxy. In Giant Molecular Clouds (GMCs), evolved star envelopes, and planetary nebulae, these emission lines can be extended over many arc minutes and possess complicated, often self absorbed, line profiles. High spectral resolution (R> 105) observations of these lines at sub-arcminute angular resolution are crucial to understanding the complicated interplay between the interstellar medium and the stars that form from it. This feedback is central to all theories of galactic evolution. Large format heterodyne array receivers can provide the spectral resolution and spatial coverage to probe these lines over extended regions. The advent of large format (~100 pixel) spectroscopic imaging cameras in the far-infrared (FIR) will fundamentally change the way astronomy is performed in this important wavelength regime. While the possibility of such instruments has been discussed for more than two decades, only recently have advances in mixer and local oscillator technology, device fabrication, micromachining, and digital signal processing made the construction of such instruments tractable. These technologies can be implemented to construct a sensitive, flexible, heterodyne array facility instrument for SOFIA. The instrument concept for StratoSTAR: Stratospheric Submm/THz Array Receiver includes a common user mounting, control system, IF processor, spectrometer, and cryogenic system. The cryogenic system will be designed to accept a frontend insert. The frontend insert and associated local oscillator system/relay optics would be provided by individual user groups and reflect their scientific interests. Rapid technology development in this field makes SOFIA the ideal platform to operate such a modular, continuously evolving instrument.

Original languageEnglish (US)
Title of host publicationProceedings of SPIE - The International Society for Optical Engineering
Volume7741
DOIs
StatePublished - 2010
EventMillimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V - San Diego, CA, United States
Duration: Jun 29 2010Jul 2 2010

Other

OtherMillimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V
CountryUnited States
CitySan Diego, CA
Period6/29/107/2/10

Fingerprint

SOFIA (airborne observatory)
Heterodyne
format
Infrared
Infrared radiation
Line
Spectral resolution
inserts
spectral resolution
Cryogenics
Spectral Resolution
Stars
cryogenics
receivers
oscillators
Star
Receiver
Probe
stars
Wavelength

Keywords

  • array receiver
  • heterodyne
  • SOFIA
  • submillimeter
  • TeraHertz

ASJC Scopus subject areas

  • Applied Mathematics
  • Computer Science Applications
  • Electrical and Electronic Engineering
  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics

Cite this

Walker, C., Kulesa, C., Kloosterman, J., Lesser, D., Cottam, T., Groppi, C., ... Martin, C. (2010). Large format heterodyne arrays for observing far-infrared lines with SOFIA. In Proceedings of SPIE - The International Society for Optical Engineering (Vol. 7741). [77410Z] https://doi.org/10.1117/12.857811

Large format heterodyne arrays for observing far-infrared lines with SOFIA. / Walker, C.; Kulesa, C.; Kloosterman, J.; Lesser, D.; Cottam, T.; Groppi, Christopher; Zmuidzinas, J.; Edgar, M.; Radford, S.; Goldsmith, P.; Langer, W.; Yorke, H.; Kawamura, J.; Mehdi, I.; Hollenbach, D.; Stutzki, J.; Huebers, H.; Gao, J. R.; Martin, C.

Proceedings of SPIE - The International Society for Optical Engineering. Vol. 7741 2010. 77410Z.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Walker, C, Kulesa, C, Kloosterman, J, Lesser, D, Cottam, T, Groppi, C, Zmuidzinas, J, Edgar, M, Radford, S, Goldsmith, P, Langer, W, Yorke, H, Kawamura, J, Mehdi, I, Hollenbach, D, Stutzki, J, Huebers, H, Gao, JR & Martin, C 2010, Large format heterodyne arrays for observing far-infrared lines with SOFIA. in Proceedings of SPIE - The International Society for Optical Engineering. vol. 7741, 77410Z, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V, San Diego, CA, United States, 6/29/10. https://doi.org/10.1117/12.857811
Walker C, Kulesa C, Kloosterman J, Lesser D, Cottam T, Groppi C et al. Large format heterodyne arrays for observing far-infrared lines with SOFIA. In Proceedings of SPIE - The International Society for Optical Engineering. Vol. 7741. 2010. 77410Z https://doi.org/10.1117/12.857811
Walker, C. ; Kulesa, C. ; Kloosterman, J. ; Lesser, D. ; Cottam, T. ; Groppi, Christopher ; Zmuidzinas, J. ; Edgar, M. ; Radford, S. ; Goldsmith, P. ; Langer, W. ; Yorke, H. ; Kawamura, J. ; Mehdi, I. ; Hollenbach, D. ; Stutzki, J. ; Huebers, H. ; Gao, J. R. ; Martin, C. / Large format heterodyne arrays for observing far-infrared lines with SOFIA. Proceedings of SPIE - The International Society for Optical Engineering. Vol. 7741 2010.
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