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Visual and Near-infrared Astronomy

Multimessenger Astronomy in Practice, 2021
The first non-electromagnetic messengers from space were discovered in the early 20th century, but it is only now that multimessenger astronomy is coming into its own. The aim of Multimessenger Astronomy in Practice is to aid an astronomer who is new to research in a particular area of multimessenger astronomy.
Gurovich, Sebastian   +2 more
openaire   +3 more sources

LINC-NIRVANA for the large binocular telescope: setting up the world’s largest near infrared binoculars for astronomy

Optical Engineering, 2013
LINC-NIRVANA (LN) is the near-infrared, Fizeau-type imaging interferometer for the large binocular telescope (LBT) on Mt. Graham, Arizona (elevation of 3267 m). The instrument is currently being built by a consortium of German and Italian institutes under the leadership of the Max Planck Institute for Astronomy in Heidelberg, Germany.
Italo Foppiani   +2 more
exaly   +2 more sources

A NICMOS-3 based spectrograph for near infrared astronomy

Experimental Astronomy, 1994
We describe a design for a compact cooled spectrograph which incorporates two cameras and two collimators to achieve high throughput from 0.8 to 2.5μm. The spectrograph utilizes multiple NICMOS 3 arrays, specially mounted to minimize their separation in the spectral dimension.
R. J. Rudy   +3 more
openaire   +1 more source

First experiences with a solid ZnSe grism for near infrared astronomy

Experimental Astronomy, 1994
We present engineering data and initial astronomical observations with the solid ZnSe grisms mounted in the MPIA MAGIC infrared camera.
T. M. Herbst, J. T. Rayner
openaire   +1 more source

Limitations of ground based near and far infrared astronomy

Infrared Physics, 1975
Abstract The possibilities of ground based infrared astronomy are discussed. It is shown that telescopes used up to now are not optimized and that the Diffraction Limited Detectivity conditions (DLD) cannot be reached, in the near infrared, by the larger telescopes. The maximum useful diameters for near i.r. and far i.r.
G. Dall'Oglio   +4 more
openaire   +1 more source

Infrared Spectroscopy of Micro-Organisms near 3.4 μm in Relation to Geology and Astronomy

Astrophysics and Space Science, 1982
Microorganisms sealed in KBr discs have an absorption spectrum over the 2.5-15 μm waveband that shows thermal stability as they are heated in an inert atmosphere to temperatures of about 400 °C. Microfossils tightly sealed within cavities in rocks could be endowed with similar properties of thermal stability.
F. Hoyle   +3 more
openaire   +1 more source

A discussion on infared astronomy - Near infrared night sky background

Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1969
Abstract We have carried out near infrared observations on wide fields of the sky, using both a rocket-borne telescope and ground-based equipment. The rocket observations covered the spectral range of 1 to 8 μm. The ground-based observations were carried out in a narrow spectral region around 1.085 μm.
M. Harwit, K. Fuhrmann, M. Werner
openaire   +1 more source

SPIREX-near infrared astronomy from the South Pole

Experimental Astronomy, 1994
Over the next several years we will deploy a series of spectrometers, imagers, and telescopes at the South Pole as part of a project named SPIREX — for South Pole Infrared Explorer. Our goal is to survey a substantial area of the sky to study the origins of galaxies and stars.
openaire   +1 more source

Near-infrared Organic Photodetector Based on An Aza-BODIPY Dye for Laser Microphone System

Journal of Materials Chemistry C, 2023
Near-infrared (NIR) photodetectors play an irreplaceable role in many fields, such as aerospace, astronomy, meteorology, military, civil and industry.
Xi Chen   +8 more
semanticscholar   +1 more source

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