Search Results - (Author, Cooperation:R. Maiolino)
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1Latest Papers from Table of Contents or Articles in PressStaff View
Publication Date: 2015-05-15Publisher: Nature Publishing Group (NPG)Print ISSN: 0028-0836Electronic ISSN: 1476-4687Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsPublished by: -
2Latest Papers from Table of Contents or Articles in PressF. Walter ; R. Decarli ; C. Carilli ; F. Bertoldi ; P. Cox ; E. Da Cunha ; E. Daddi ; M. Dickinson ; D. Downes ; D. Elbaz ; R. Ellis ; J. Hodge ; R. Neri ; D. A. Riechers ; A. Weiss ; E. Bell ; H. Dannerbauer ; M. Krips ; M. Krumholz ; L. Lentati ; R. Maiolino ; K. Menten ; H. W. Rix ; B. Robertson ; H. Spinrad ; D. P. Stark ; D. Stern
Nature Publishing Group (NPG)
Published 2012Staff ViewPublication Date: 2012-06-16Publisher: Nature Publishing Group (NPG)Print ISSN: 0028-0836Electronic ISSN: 1476-4687Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsPublished by: -
3Articles: DFG German National LicensesSchneider, R. ; Oliva, E. ; Bianchi, S. ; Ferrara, A. ; Mannucci, F. ; Pedani, M. ; Roca Sogorb, M. ; Maiolino, R.
[s.l.] : Macmillian Magazines Ltd.
Published 2004Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Interstellar dust plays a crucial role in the evolution of the Universe by assisting the formation of molecules, by triggering the formation of the first low-mass stars, and by absorbing stellar ultraviolet–optical light and subsequently re-emitting it at infrared/millimetre wavelengths. ...Type of Medium: Electronic ResourceURL: -
4Articles: DFG German National LicensesStaff View
ISSN: 1572-9508Keywords: Imaging camera ; IR Photometry ; NICMOS 3Source: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract ARNICA (ARcetri Near Infrared CAmera) is the imaging camera for the near infrared bands between 1.0 and 2.5 μm that Arcetri Observatory has designed and built as a common use instrument for the TIRGO telescope (1.5 m diameter, f/20) located at Gornergrat (Switzerland). The scale is 1″ per pixel, with sky coverage of more than 4′×4′ on the NICMOS 3 (256×256 pixels, 40 μm side) detector array. The optical path is compact enough to be enclosed in a25.4 cm diameter dewar; the working temperature of detector and optics is 76 K. We give an estimate of performance, in terms of sensitivity with an assigned observing time, along with some preliminary considerations on photometric accuracy.Type of Medium: Electronic ResourceURL: