Sensitive far-IR survey spectroscopy: BLISS for SPICA

C. M. Bradford; Matt Kenyon; Warren Holmes; James Bock; Timothy Koch; P. Day; H. Nguyen; M. Werner; R. Cofield; C. Paine; K. Irwin; M. Harwit; G. Stacey; G. Helou; L. Armus; J. D. Smith; S. Chapman; G. Rieke; D. Lester; T. Nakagawa; H. Matsuhara; T. Onaka; H. Shibai; M. Tamura

doi:10.1117/12.790156

Sensitive far-IR survey spectroscopy: BLISS for SPICA

C. M. Bradford
, Matt Kenyon
, Warren Holmes
, James Bock
, Timothy Koch
, P. Day
, H. Nguyen
, M. Werner
, R. Cofield
, C. Paine
, K. Irwin
, M. Harwit
, G. Stacey
, G. Helou
, L. Armus
, J. D. Smith
, S. Chapman
, G. Rieke
, D. Lester
, T. Nakagawa

H. Matsuhara, T. Onaka, H. Shibai, M. Tamura

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

12 Scopus citations

Abstract

We present a concept for BLISS, a sensitive far-IR-submillimeter spectrograph for SPICA. SPICA is a JAXA-led mission featuring a 3.5-meter telescope actively cooled to below 5K, envisioned for launch in 2017. The low-background platform is especially compelling for moderate-resolution survey spectroscopy, for which BLISS is designed. The BLISS / SPICA combination will offer line sensitivities below 10^-20Wm^-2 in modest integrations, enabling rapid survey spectroscopy of galaxies out to redshift 5. The far-IR fine-structure and molecular transitions which BLISS / SPICA will measure are immune to dust extinction, and will unambiguously reveal these galaxies' redshifts, stellar and AGN contents, gas properties, and heavy-element abundances. Taken together, such spectra will reveal the history of galaxies from 1 GY after the Big Bang to the present day. BLISS is comprised of five sub-bands, each with two R ∼ 700 grating spectrometer modules. The modules are configured with polarizing and dichroic splitters to provide complete instantaneous spectral coverage in two sky positions. To approach background-limited performance, BLISS detectors must have sensitivities at or below 5 × 10^-20WHz^-1/2, and the format is 10 arrays of several hundred pixels each. It is anticipated that these requirements can be met on SPICA's timescale with leg-isolated superconducting (TES) bolometers cooled with a 50 mK magnetic refrigerator.

Original language	English (US)
Title of host publication	Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV
DOIs	https://doi.org/10.1117/12.790156
State	Published - 2008
Event	Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV - Marseille, France Duration: Jun 26 2008 → Jun 28 2008

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	7020
ISSN (Print)	0277-786X

Other

Other	Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV
Country/Territory	France
City	Marseille
Period	6/26/08 → 6/28/08

Keywords

BLISS
Bolometers
Far-IR
SPICA
Spectroscopy

ASJC Scopus subject areas

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

Access to Document

10.1117/12.790156

Cite this

Bradford, C. M., Kenyon, M., Holmes, W., Bock, J., Koch, T., Day, P., Nguyen, H., Werner, M., Cofield, R., Paine, C., Irwin, K., Harwit, M., Stacey, G., Helou, G., Armus, L., Smith, J. D., Chapman, S., Rieke, G., Lester, D., ... Tamura, M. (2008). Sensitive far-IR survey spectroscopy: BLISS for SPICA. In Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV Article 70201O (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7020). https://doi.org/10.1117/12.790156

Sensitive far-IR survey spectroscopy: BLISS for SPICA. / Bradford, C. M.; Kenyon, Matt; Holmes, Warren et al.
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV. 2008. 70201O (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7020).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Bradford, CM, Kenyon, M, Holmes, W, Bock, J, Koch, T, Day, P, Nguyen, H, Werner, M, Cofield, R, Paine, C, Irwin, K, Harwit, M, Stacey, G, Helou, G, Armus, L, Smith, JD, Chapman, S, Rieke, G, Lester, D, Nakagawa, T, Matsuhara, H, Onaka, T, Shibai, H & Tamura, M 2008, Sensitive far-IR survey spectroscopy: BLISS for SPICA. in Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV., 70201O, Proceedings of SPIE - The International Society for Optical Engineering, vol. 7020, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV, Marseille, France, 6/26/08. https://doi.org/10.1117/12.790156

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title = "Sensitive far-IR survey spectroscopy: BLISS for SPICA",

abstract = "We present a concept for BLISS, a sensitive far-IR-submillimeter spectrograph for SPICA. SPICA is a JAXA-led mission featuring a 3.5-meter telescope actively cooled to below 5K, envisioned for launch in 2017. The low-background platform is especially compelling for moderate-resolution survey spectroscopy, for which BLISS is designed. The BLISS / SPICA combination will offer line sensitivities below 10-20Wm-2 in modest integrations, enabling rapid survey spectroscopy of galaxies out to redshift 5. The far-IR fine-structure and molecular transitions which BLISS / SPICA will measure are immune to dust extinction, and will unambiguously reveal these galaxies' redshifts, stellar and AGN contents, gas properties, and heavy-element abundances. Taken together, such spectra will reveal the history of galaxies from 1 GY after the Big Bang to the present day. BLISS is comprised of five sub-bands, each with two R ∼ 700 grating spectrometer modules. The modules are configured with polarizing and dichroic splitters to provide complete instantaneous spectral coverage in two sky positions. To approach background-limited performance, BLISS detectors must have sensitivities at or below 5 × 10-20WHz-1/2, and the format is 10 arrays of several hundred pixels each. It is anticipated that these requirements can be met on SPICA's timescale with leg-isolated superconducting (TES) bolometers cooled with a 50 mK magnetic refrigerator.",

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AU - Bradford, C. M.

AU - Kenyon, Matt

AU - Holmes, Warren

AU - Bock, James

AU - Koch, Timothy

AU - Day, P.

AU - Nguyen, H.

AU - Werner, M.

AU - Cofield, R.

AU - Paine, C.

AU - Irwin, K.

AU - Harwit, M.

AU - Stacey, G.

AU - Helou, G.

AU - Armus, L.

AU - Smith, J. D.

AU - Chapman, S.

AU - Rieke, G.

AU - Lester, D.

AU - Nakagawa, T.

AU - Matsuhara, H.

AU - Onaka, T.

AU - Shibai, H.

AU - Tamura, M.

PY - 2008

Y1 - 2008

N2 - We present a concept for BLISS, a sensitive far-IR-submillimeter spectrograph for SPICA. SPICA is a JAXA-led mission featuring a 3.5-meter telescope actively cooled to below 5K, envisioned for launch in 2017. The low-background platform is especially compelling for moderate-resolution survey spectroscopy, for which BLISS is designed. The BLISS / SPICA combination will offer line sensitivities below 10-20Wm-2 in modest integrations, enabling rapid survey spectroscopy of galaxies out to redshift 5. The far-IR fine-structure and molecular transitions which BLISS / SPICA will measure are immune to dust extinction, and will unambiguously reveal these galaxies' redshifts, stellar and AGN contents, gas properties, and heavy-element abundances. Taken together, such spectra will reveal the history of galaxies from 1 GY after the Big Bang to the present day. BLISS is comprised of five sub-bands, each with two R ∼ 700 grating spectrometer modules. The modules are configured with polarizing and dichroic splitters to provide complete instantaneous spectral coverage in two sky positions. To approach background-limited performance, BLISS detectors must have sensitivities at or below 5 × 10-20WHz-1/2, and the format is 10 arrays of several hundred pixels each. It is anticipated that these requirements can be met on SPICA's timescale with leg-isolated superconducting (TES) bolometers cooled with a 50 mK magnetic refrigerator.

AB - We present a concept for BLISS, a sensitive far-IR-submillimeter spectrograph for SPICA. SPICA is a JAXA-led mission featuring a 3.5-meter telescope actively cooled to below 5K, envisioned for launch in 2017. The low-background platform is especially compelling for moderate-resolution survey spectroscopy, for which BLISS is designed. The BLISS / SPICA combination will offer line sensitivities below 10-20Wm-2 in modest integrations, enabling rapid survey spectroscopy of galaxies out to redshift 5. The far-IR fine-structure and molecular transitions which BLISS / SPICA will measure are immune to dust extinction, and will unambiguously reveal these galaxies' redshifts, stellar and AGN contents, gas properties, and heavy-element abundances. Taken together, such spectra will reveal the history of galaxies from 1 GY after the Big Bang to the present day. BLISS is comprised of five sub-bands, each with two R ∼ 700 grating spectrometer modules. The modules are configured with polarizing and dichroic splitters to provide complete instantaneous spectral coverage in two sky positions. To approach background-limited performance, BLISS detectors must have sensitivities at or below 5 × 10-20WHz-1/2, and the format is 10 arrays of several hundred pixels each. It is anticipated that these requirements can be met on SPICA's timescale with leg-isolated superconducting (TES) bolometers cooled with a 50 mK magnetic refrigerator.

KW - BLISS

KW - Bolometers

KW - Far-IR

KW - SPICA

KW - Spectroscopy

UR - https://www.scopus.com/pages/publications/52249096140

UR - https://www.scopus.com/pages/publications/52249096140#tab=citedBy

U2 - 10.1117/12.790156

DO - 10.1117/12.790156

M3 - Conference contribution

AN - SCOPUS:52249096140

SN - 9780819472304

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV

Y2 - 26 June 2008 through 28 June 2008

ER -

Sensitive far-IR survey spectroscopy: BLISS for SPICA

Abstract

Publication series

Other

Keywords

ASJC Scopus subject areas

Access to Document

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