scholarly journals Publisher’s Note: “Robust diffraction-limited near-infrared-to-near-ultraviolet wide-field imaging from stratospheric balloon-borne Platforms—Super-pressure Balloon-borne Imaging Telescope performance” [Rev. Sci. Instrum. 91, 034501 (2020)]

2021 ◽  
Vol 92 (1) ◽  
pp. 019901
Author(s):  
L. Javier Romualdez ◽  
Steven J. Benton ◽  
Anthony M. Brown ◽  
Paul Clark ◽  
Christopher J. Damaren ◽  
...  
Keyword(s):  
Near Infrared ◽  
Wide Field ◽  
Near Ultraviolet ◽  
Imaging Telescope ◽  
Stratospheric Balloon ◽  
Field Imaging ◽  
Wide Field Imaging

scholarly journals Lite: The Large Imaging Telescope

1994 ◽  
Vol 161 ◽  
pp. 73-76
Author(s):  
L. Vigroux
Keyword(s):  
Wide Field ◽  
Large Telescope ◽  
Very Large Telescope ◽  
Imaging Telescope ◽  
Field Imaging ◽  
Wide Field Imaging

It was realised very early in the development of the ESO 16 metre equivalent Very Large Telescope (VLT) that wide-field imaging is too complicated and costly to implement on the VLT itself and should be done with a smaller telescope.

scholarly journals Wide-Field-Imaging 3-Mirror-Systems by High Light Gathering Power and a Wide-Field Optical System for the ‘Large Imaging Telescope’ (Lite)

1994 ◽  
Vol 161 ◽  
pp. 101-107
Author(s):  
U. Laux
Keyword(s):  
Optical System ◽  
High Light ◽  
Field Of View ◽  
Wide Field ◽  
Light Gathering Power ◽  
Imaging Telescope ◽  
Light Gathering ◽  
Field Imaging ◽  
Wide Field Imaging

The desire of astronomers for wide field telescope systems which surpass the RCC (1:8 max. 1.5 degree) in light gathering power and field of view are relative concrete today. For this type of telescope, detectors planned ARE CCDs in multichip arrangement.

scholarly journals Wide-Field Imaging of Nearby Galaxies in Near-Infrared Bands

1994 ◽  
Vol 161 ◽  
pp. 599-600
Author(s):  
T. Ichikawa ◽  
K. Tarusawa ◽  
K. Yanagisawa ◽  
N. Itoh ◽  
M. Ueno
Keyword(s):  
Near Infrared ◽  
Wide Field ◽  
Large Format ◽  
Nearby Galaxies ◽  
Field Imaging ◽  
Wide Field Imaging

We present the results of wide-field imaging of nearby galaxies observed in the near-infrared using a large format array. The total magnitudes and mass-to-luminosity ratios of NGC 253, M 82, NGC 891, and some cluster members are discussed.

Wide-Field Imaging of Nearby Galaxies in Near-Infrared Bands

1994 ◽  
pp. 599-600
Author(s):  
T. Ichikawa ◽  
K. Tarusawa ◽  
K. Yanagisawa ◽  
N. Itoh ◽  
M. Ueno
Keyword(s):  
Near Infrared ◽  
Wide Field ◽  
Nearby Galaxies ◽  
Field Imaging ◽  
Wide Field Imaging

scholarly journals Near-Infrared Imaging by a Schmidt Telescope

1994 ◽  
Vol 161 ◽  
pp. 89-90
Author(s):  
K. Yanagisawa ◽  
N. Itoh ◽  
T. Ichikawa ◽  
K. Tarusawa ◽  
M. Ueno
Keyword(s):  
Thermal Radiation ◽  
Near Infrared ◽  
Infrared Imaging ◽  
Image Resolution ◽  
Wide Field ◽  
Schmidt Telescope ◽  
Large Format ◽  
Array Camera ◽  
Field Imaging ◽  
Wide Field Imaging

We have carried out wide field imaging observations in the near-infrared (J, H and K′ band) with a large format array camera attached to the prime focus of the 105 cm Schmidt telescope at Kiso Observatory. The image resolution, limiting magnitudes and the effect of thermal radiation are discussed.

scholarly journals The UV Content of Virgo Cluster Galaxies

1995 ◽  
Vol 164 ◽  
pp. 450-451
Author(s):  
Noah Brosch
Keyword(s):  
Preliminary Analysis ◽  
Virgo Cluster ◽  
Wide Field ◽  
Space Astronomy ◽  
Cluster Galaxies ◽  
Cluster Region ◽  
Imaging Telescope ◽  
Field Imaging ◽  
Wide Field Imaging

I present a preliminary analysis of three UV images of the Virgo cluster region, obtained by the FAUST experiment (Bowyer et al. 1993) in April 1992. FAUST is a wide-field imaging telescope covering an 8° area with effective resolution of 3′.5. The experiment was constructed by the Berkeley Space Astronomy Group together with the Laboratoire d'Astrophysique Spatiale of the CNES. It operated on board the Shuttle during the mission ATLAS-1.

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