The photodetector array camera and Spectrometer (PACS) on the herschel space observatory

A. Poglitsch; C. Waelkens; N. Geis; H. Feuchtgruber; B. Van Den Bussche; L. Rodriguez; O. Krause; E. Renotte; C. Van Hoof; P. Saraceno; J. Cepa; F. Kerschbaum; P. Agnèse; B. Ali; B. Altieri; P. Andreani; J. L. Augueres; Z. Balog; L. Barl; O. H. Bauer; N. Belbachir; M. Benedettini; N. Billot; O. Boulade; H. Bischof; J. Blommaert; E. Callut; C. Cara; R. Cerulli; D. Cesarsky; A. Contursi; Y. Creten; W. De Meester; V. Doublier; E. Doumayrou; L. Duband; K. Exter; R. Genzel; J. M. Gillis; U. Grözinger; T. Henning; J. Herreros; R. Huygen; M. Inguscio; G. Jakob; C. Jamar; C. Jean; J. De Jong; R. Katterloher; C. Kiss; U. Klaas; D. Lemke; D. Lutz; S. Madden; B. Marquet; J. Martignac; A. Mazy; P. Merken; F. Montfort; L. Morbidelli; T. Müller; M. Nielbock; K. Okumura; R. Orfei; R. Ottensamer; S. Pezzuto; P. Popesso; J. Putzeys; S. Regibo; V. Reveret; P. Royer; M. Sauvage; J. Schreiber; J. Stegmaier; D. Schmitt; J. Schubert; E. Sturm; M. Thiel; G. Tofani; R. Vavrek; M. Wetzstein; E. Wieprecht; E. Wiezorrek

doi:10.1051/0004-6361/201014535

The photodetector array camera and Spectrometer (PACS) on the herschel space observatory

A. Poglitsch
, C. Waelkens
, N. Geis
, H. Feuchtgruber
, B. Van Den Bussche
, L. Rodriguez
, O. Krause
, E. Renotte
, C. Van Hoof
, P. Saraceno
, J. Cepa
, F. Kerschbaum
, P. Agnèse
, B. Ali
, B. Altieri
, P. Andreani
, J. L. Augueres
, Z. Balog
, L. Barl
, O. H. Bauer

N. Belbachir, M. Benedettini, N. Billot, O. Boulade, H. Bischof, J. Blommaert, E. Callut, C. Cara, R. Cerulli, D. Cesarsky, A. Contursi, Y. Creten, W. De Meester, V. Doublier, E. Doumayrou, L. Duband, K. Exter, R. Genzel, J. M. Gillis, U. Grözinger, T. Henning, J. Herreros, R. Huygen, M. Inguscio, G. Jakob, C. Jamar, C. Jean, J. De Jong, R. Katterloher, C. Kiss, U. Klaas, D. Lemke, D. Lutz, S. Madden, B. Marquet, J. Martignac, A. Mazy, P. Merken, F. Montfort, L. Morbidelli, T. Müller, M. Nielbock, K. Okumura, R. Orfei, R. Ottensamer, S. Pezzuto, P. Popesso, J. Putzeys, S. Regibo, V. Reveret, P. Royer, M. Sauvage, J. Schreiber, J. Stegmaier, D. Schmitt, J. Schubert, E. Sturm, M. Thiel, G. Tofani, R. Vavrek, M. Wetzstein, E. Wieprecht, E. Wiezorrek

Communication, Information, Systems and Sensors

MPE
KU Leuven
Orme des Merisiers
MPIA
Université de Liège
IMEC
Istituto di Fisica dello spazio Interplanetario
Instituto de Astrofísica de Canarias
Institut für Astronomie der Universität Wien
Commissariat à l'Énergie Atomique (CEA)
NASA Herschel Science Center
Urbanización Villafranca Del Castillo
European Southern Observatory
Osservatorio Astronomico di Trieste
AIT Austrian Institute of Technology
Technische Universität Graz
LENS - European Laboratory for Non-Linear Spectroscopy
Konkoly Observatory
Osservatorio Astrofisico Di Arcetri

Research output: Contribution to journal › Article › peer-review

2104 Citations (Scopus)

Abstract

The Photodetector Array Camera and Spectrometer (PACS) is one of the three science instruments on ESA's far infrared and submillimetre observatory. It employs two Ge:Ga photoconductor arrays (stressed and unstressed) with 16×25 pixels, each, and two filled silicon bolometer arrays with 16×32 and 32×64 pixels, respectively, to perform integral-field spectroscopy and imaging photometry in the 60-210 μm wavelength regime. In photometry mode, it simultaneously images two bands, 60-85 μm or 85-125 μm and 125-210 μm, over a field of view of ∼1.75'× 3.5', with close to Nyquist beam sampling in each band. In spectroscopy mode, it images a field of 47" × 47", resolved into 5×5 pixels, with an instantaneous spectral coverage of ∼1500 km s^-1 and a spectral resolution of ∼175 km s^-1. We summarise the design of the instrument, describe observing modes, calibration, and data analysis methods, and present our current assessment of the in-orbit performance of the instrument based on the performance verification tests. PACS is fully operational, and the achieved performance is close to or better than the pre-launch predictions.

Original language	English
Article number	L2
Journal	Astronomy and Astrophysics
Volume	518
Issue number	4
DOIs	https://doi.org/10.1051/0004-6361/201014535
Publication status	Published - 2010

Keywords

instrumentation: photometers
instrumentation: spectrographs
space vehicles: instruments

Access to Document

10.1051/0004-6361/201014535

Cite this

Poglitsch, A., Waelkens, C., Geis, N., Feuchtgruber, H., Van Den Bussche, B., Rodriguez, L., Krause, O., Renotte, E., Van Hoof, C., Saraceno, P., Cepa, J., Kerschbaum, F., Agnèse, P., Ali, B., Altieri, B., Andreani, P., Augueres, J. L., Balog, Z., Barl, L., ... Wiezorrek, E. (2010). The photodetector array camera and Spectrometer (PACS) on the herschel space observatory. Astronomy and Astrophysics, 518(4), Article L2. https://doi.org/10.1051/0004-6361/201014535

@article{ba6ae07a494a4082b98c6dac05f39fce,

title = "The photodetector array camera and Spectrometer (PACS) on the herschel space observatory",

abstract = "The Photodetector Array Camera and Spectrometer (PACS) is one of the three science instruments on ESA's far infrared and submillimetre observatory. It employs two Ge:Ga photoconductor arrays (stressed and unstressed) with 16{\texttimes}25 pixels, each, and two filled silicon bolometer arrays with 16{\texttimes}32 and 32{\texttimes}64 pixels, respectively, to perform integral-field spectroscopy and imaging photometry in the 60-210 μm wavelength regime. In photometry mode, it simultaneously images two bands, 60-85 μm or 85-125 μm and 125-210 μm, over a field of view of ∼1.75'{\texttimes} 3.5', with close to Nyquist beam sampling in each band. In spectroscopy mode, it images a field of 47{"} {\texttimes} 47{"}, resolved into 5{\texttimes}5 pixels, with an instantaneous spectral coverage of ∼1500 km s-1 and a spectral resolution of ∼175 km s-1. We summarise the design of the instrument, describe observing modes, calibration, and data analysis methods, and present our current assessment of the in-orbit performance of the instrument based on the performance verification tests. PACS is fully operational, and the achieved performance is close to or better than the pre-launch predictions.",

keywords = "instrumentation: photometers, instrumentation: spectrographs, space vehicles: instruments",

author = "A. Poglitsch and C. Waelkens and N. Geis and H. Feuchtgruber and \{Van Den Bussche\}, B. and L. Rodriguez and O. Krause and E. Renotte and \{Van Hoof\}, C. and P. Saraceno and J. Cepa and F. Kerschbaum and P. Agn{\`e}se and B. Ali and B. Altieri and P. Andreani and Augueres, \{J. L.\} and Z. Balog and L. Barl and Bauer, \{O. H.\} and N. Belbachir and M. Benedettini and N. Billot and O. Boulade and H. Bischof and J. Blommaert and E. Callut and C. Cara and R. Cerulli and D. Cesarsky and A. Contursi and Y. Creten and \{De Meester\}, W. and V. Doublier and E. Doumayrou and L. Duband and K. Exter and R. Genzel and Gillis, \{J. M.\} and U. Gr{\"o}zinger and T. Henning and J. Herreros and R. Huygen and M. Inguscio and G. Jakob and C. Jamar and C. Jean and \{De Jong\}, J. and R. Katterloher and C. Kiss and U. Klaas and D. Lemke and D. Lutz and S. Madden and B. Marquet and J. Martignac and A. Mazy and P. Merken and F. Montfort and L. Morbidelli and T. M{\"u}ller and M. Nielbock and K. Okumura and R. Orfei and R. Ottensamer and S. Pezzuto and P. Popesso and J. Putzeys and S. Regibo and V. Reveret and P. Royer and M. Sauvage and J. Schreiber and J. Stegmaier and D. Schmitt and J. Schubert and E. Sturm and M. Thiel and G. Tofani and R. Vavrek and M. Wetzstein and E. Wieprecht and E. Wiezorrek",

year = "2010",

doi = "10.1051/0004-6361/201014535",

language = "English",

volume = "518",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

number = "4",

}

Poglitsch, A, Waelkens, C, Geis, N, Feuchtgruber, H, Van Den Bussche, B, Rodriguez, L, Krause, O, Renotte, E, Van Hoof, C, Saraceno, P, Cepa, J, Kerschbaum, F, Agnèse, P, Ali, B, Altieri, B, Andreani, P, Augueres, JL, Balog, Z, Barl, L, Bauer, OH, Belbachir, N, Benedettini, M, Billot, N, Boulade, O, Bischof, H, Blommaert, J, Callut, E, Cara, C, Cerulli, R, Cesarsky, D, Contursi, A, Creten, Y, De Meester, W, Doublier, V, Doumayrou, E, Duband, L, Exter, K, Genzel, R, Gillis, JM, Grözinger, U, Henning, T, Herreros, J, Huygen, R, Inguscio, M, Jakob, G, Jamar, C, Jean, C, De Jong, J, Katterloher, R, Kiss, C, Klaas, U, Lemke, D, Lutz, D, Madden, S, Marquet, B, Martignac, J, Mazy, A, Merken, P, Montfort, F, Morbidelli, L, Müller, T, Nielbock, M, Okumura, K, Orfei, R, Ottensamer, R, Pezzuto, S, Popesso, P, Putzeys, J, Regibo, S, Reveret, V, Royer, P, Sauvage, M, Schreiber, J, Stegmaier, J, Schmitt, D, Schubert, J, Sturm, E, Thiel, M, Tofani, G, Vavrek, R, Wetzstein, M, Wieprecht, E & Wiezorrek, E 2010, 'The photodetector array camera and Spectrometer (PACS) on the herschel space observatory', Astronomy and Astrophysics, vol. 518, no. 4, L2. https://doi.org/10.1051/0004-6361/201014535

TY - JOUR

T1 - The photodetector array camera and Spectrometer (PACS) on the herschel space observatory

AU - Poglitsch, A.

AU - Waelkens, C.

AU - Geis, N.

AU - Feuchtgruber, H.

AU - Van Den Bussche, B.

AU - Rodriguez, L.

AU - Krause, O.

AU - Renotte, E.

AU - Van Hoof, C.

AU - Saraceno, P.

AU - Cepa, J.

AU - Kerschbaum, F.

AU - Agnèse, P.

AU - Ali, B.

AU - Altieri, B.

AU - Andreani, P.

AU - Augueres, J. L.

AU - Balog, Z.

AU - Barl, L.

AU - Bauer, O. H.

AU - Belbachir, N.

AU - Benedettini, M.

AU - Billot, N.

AU - Boulade, O.

AU - Bischof, H.

AU - Blommaert, J.

AU - Callut, E.

AU - Cara, C.

AU - Cerulli, R.

AU - Cesarsky, D.

AU - Contursi, A.

AU - Creten, Y.

AU - De Meester, W.

AU - Doublier, V.

AU - Doumayrou, E.

AU - Duband, L.

AU - Exter, K.

AU - Genzel, R.

AU - Gillis, J. M.

AU - Grözinger, U.

AU - Henning, T.

AU - Herreros, J.

AU - Huygen, R.

AU - Inguscio, M.

AU - Jakob, G.

AU - Jamar, C.

AU - Jean, C.

AU - De Jong, J.

AU - Katterloher, R.

AU - Kiss, C.

AU - Klaas, U.

AU - Lemke, D.

AU - Lutz, D.

AU - Madden, S.

AU - Marquet, B.

AU - Martignac, J.

AU - Mazy, A.

AU - Merken, P.

AU - Montfort, F.

AU - Morbidelli, L.

AU - Müller, T.

AU - Nielbock, M.

AU - Okumura, K.

AU - Orfei, R.

AU - Ottensamer, R.

AU - Pezzuto, S.

AU - Popesso, P.

AU - Putzeys, J.

AU - Regibo, S.

AU - Reveret, V.

AU - Royer, P.

AU - Sauvage, M.

AU - Schreiber, J.

AU - Stegmaier, J.

AU - Schmitt, D.

AU - Schubert, J.

AU - Sturm, E.

AU - Thiel, M.

AU - Tofani, G.

AU - Vavrek, R.

AU - Wetzstein, M.

AU - Wieprecht, E.

AU - Wiezorrek, E.

PY - 2010

Y1 - 2010

N2 - The Photodetector Array Camera and Spectrometer (PACS) is one of the three science instruments on ESA's far infrared and submillimetre observatory. It employs two Ge:Ga photoconductor arrays (stressed and unstressed) with 16×25 pixels, each, and two filled silicon bolometer arrays with 16×32 and 32×64 pixels, respectively, to perform integral-field spectroscopy and imaging photometry in the 60-210 μm wavelength regime. In photometry mode, it simultaneously images two bands, 60-85 μm or 85-125 μm and 125-210 μm, over a field of view of ∼1.75'× 3.5', with close to Nyquist beam sampling in each band. In spectroscopy mode, it images a field of 47" × 47", resolved into 5×5 pixels, with an instantaneous spectral coverage of ∼1500 km s-1 and a spectral resolution of ∼175 km s-1. We summarise the design of the instrument, describe observing modes, calibration, and data analysis methods, and present our current assessment of the in-orbit performance of the instrument based on the performance verification tests. PACS is fully operational, and the achieved performance is close to or better than the pre-launch predictions.

AB - The Photodetector Array Camera and Spectrometer (PACS) is one of the three science instruments on ESA's far infrared and submillimetre observatory. It employs two Ge:Ga photoconductor arrays (stressed and unstressed) with 16×25 pixels, each, and two filled silicon bolometer arrays with 16×32 and 32×64 pixels, respectively, to perform integral-field spectroscopy and imaging photometry in the 60-210 μm wavelength regime. In photometry mode, it simultaneously images two bands, 60-85 μm or 85-125 μm and 125-210 μm, over a field of view of ∼1.75'× 3.5', with close to Nyquist beam sampling in each band. In spectroscopy mode, it images a field of 47" × 47", resolved into 5×5 pixels, with an instantaneous spectral coverage of ∼1500 km s-1 and a spectral resolution of ∼175 km s-1. We summarise the design of the instrument, describe observing modes, calibration, and data analysis methods, and present our current assessment of the in-orbit performance of the instrument based on the performance verification tests. PACS is fully operational, and the achieved performance is close to or better than the pre-launch predictions.

KW - instrumentation: photometers

KW - instrumentation: spectrographs

KW - space vehicles: instruments

UR - https://www.scopus.com/pages/publications/77957818536

U2 - 10.1051/0004-6361/201014535

DO - 10.1051/0004-6361/201014535

M3 - Article

AN - SCOPUS:77957818536

SN - 0004-6361

VL - 518

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 4

M1 - L2

ER -

The photodetector array camera and Spectrometer (PACS) on the herschel space observatory

Abstract

Keywords

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