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Author Chen, P. S.
Title Infrared properties of barium stars Type Journal Article
Year 2001 Publication Astron. Astrophys. Abbreviated Journal A&A
Volume 372 Issue 1 Pages 245-248
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ISSN 0004-6361 ISBN Medium
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Notes Approved no
Call Number RPLAB @ s @ Serial (up) 415
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Author Omar, A.; Anantharamaiah, K. R.; Rupen, M.; Rigby, J.
Title VLA detection of OH absorption from the elliptical galaxy NGC 1052 Type Journal Article
Year 2002 Publication Astron. Astrophys. Abbreviated Journal A&A
Volume 381 Issue 1 Pages L29-L32
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ISSN 0004-6361 ISBN Medium
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Notes Approved no
Call Number RPLAB @ s @ Serial (up) 435
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Author Käufl, H. U.; Rothermal, H.; Drapatz, S.
Title Investigation of the Martian atmosphere by 10 micron heterodyne spectroscopy Type Journal Article
Year 1984 Publication Astron. Astrophys. Abbreviated Journal A&A
Volume 136 Issue Pages 319-325
Keywords astronomical spectroscopy, atmospheric composition, infrared astronomy, mars atmosphere, spectral line width, carbon dioxide concentration, nonequilibrium thermodynamics, optical heterodyning, planetary radiation, mars, atmosphere, spectroscopy, atmosphere, carbon dioxide, altitude, kinetics, rotation, thermal properties, temperature, emissions, intensity, models, data, spectra
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Call Number Serial (up) 449
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Author Rothermel, H.; Käufl, H. U.; Schrey, U.; Drapatz, S.
Title Thermal structure of the Martian mesosphere Type Journal Article
Year 1988 Publication Astron. Astrophys. Abbreviated Journal A&A
Volume 196 Issue Pages 296-300
Keywords atmospheric temperature, carbon dioxide, infrared spectroscopy, mars atmosphere, mesosphere, emission spectra, line spectra, spatial resolution, mars, atmosphere, mesosphere, structure, thermal properties, spectra, spectroscopy, earth-based observations, temperature, patterns, infrared, polar regions, wavelengths, equipment, procedure, carbon dioxide, emissions
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Call Number Rothermel1988 Serial (up) 450
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Author Johnson, M. A.; Betz, A. L.; McLaren, R. A.; Townes, C. H.; Sutton, E. C.
Title Nonthermal 10 micron CO2 emission lines in the atmospheres of Mars and Venus Type Journal Article
Year 1976 Publication Astron. Astrophys. Abbreviated Journal A&A
Volume 208 Issue Pages 145
Keywords carbon dioxide, emission spectra, infrared spectra, mars atmosphere, nonthermal radiation, optical heterodyning, planetary radiation, venus atmosphere, absorption spectra, energy transfer, line spectra, molecular absorption, molecular collisions, near infrared radiation, solar flux
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Call Number ref1976ApJ...208L.145J Serial (up) 451
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Author Kaeufl, H. U.; Rothermel, H.; Drapatz, S.
Title Indication for H2O in the upper atmosphere of Mars Type Journal Article
Year 1984 Publication Astron. Astrophys. Abbreviated Journal A&A
Volume 141 Issue Pages 430-432
Keywords atmospheric moisture, mars atmosphere, upper atmosphere, water vapor, carbon dioxide, emission spectra, nonequilibrium thermodynamics, polar regions
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Notes Approved no
Call Number Serial (up) 452
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Author Rothermel, H.; Käufl, H. U.; Yu, Y.
Title A heterodyne spectrometer for astronomical measurements at 10 micrometers Type Journal Article
Year 1983 Publication Astron. Astrophys. Abbreviated Journal A&A
Volume 126 Issue Pages 387-392
Keywords astronomical spectroscopy, infrared astronomy, infrared spectrometers, optical heterodyning, infrared telescopes, laser spectrometers, mars (planet), venus (planet)
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Call Number Serial (up) 453
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Author Hansen, Lene; Jørgensen, H.E.; Nørgaard-Nielsen, Hans Ulrik; Pedersen, Kenneth; Goudfrooij, P.; Linden-Vornle, M.J.D.
Title ISO far-infrared observations of rich galaxy clusters III. Abell 2029, Abell 2052, Abell 2142 Type Journal Article
Year 2000 Publication Astron. Astrophys. Abbreviated Journal A&A
Volume 362 Issue 1 Pages 133-137
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Abstract A sample of five rich galaxy clusters has been mapped by ISO at 60 μm, 100 μm, 135 μm, and 200 μm using the PHT-C camera. In previous papers Abell 2670 and Sersic 159-03 were discussed. Here we present the results for Abell 2029, Abell 2052, and Abell 2142. The conclusion of the survey is that the relatively small fields (approximate to 60 square are minutes) are structured with filaments or superpositions of point sources. In some cases point sources (approximate to 0.1 Jy) can be identified with cluster galaxies. An attempt to demonstrate infrared emission from dust in the cooling flows (due to star formation) was inconclusive.
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Call Number RPLAB @ s @ Serial (up) 456
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Author Soifer, B. T.; Pipher, J. L.
Title Instrumentation for infrared astronomy Type Journal Article
Year 1978 Publication Annual Rev. Astron. Astrophys. Abbreviated Journal
Volume 16 Issue 1 Pages 335-369
Keywords infrared applications
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ISSN 0066-4146 ISBN Medium
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Notes Approved no
Call Number Serial (up) 492
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Author Poglitsch, A.; Waelkens, C.; Geis, N.; Feuchtgruber, H.; Vandenbussche, 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.; Bauer, O. H.; 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, J.-M.; 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.
Title The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory Type Journal Article
Year 2010 Publication Astron. Astrophys. Abbreviated Journal A&A
Volume 518 Issue Pages 12
Keywords PACS
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.
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Call Number RPLAB @ gujma @ Serial (up) 694
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