Results 1 to 10 of about 81,818 (284)
A model for suppressing stray light in astronomical images based on deep learning [PDF]
Wide-Field Small Aperture Telescopes (WFSAT) are widely used for surveilling space objects. Due to their wide-field of view (FOV) characteristics, these telescopes can cover a large areas of the sky at once, improving observation efficiency.
Mo Chen +9 more
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A purely reflective large wide-field telescope [PDF]
Two versions of a fast, purely reflective Paul-Baker type telescope are discussed, each with an 8.4-m aperture, 3 deg diameter flat field and f/1.25 focal ratio. The first version is based on a common, even asphere type of surface with zero conic constant.
V. Yu. Terebizh
openalex +4 more sources
The Wide Field X–ray Telescope [PDF]
P. Tozzi
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ULTRASAT: A Wide-field Time-domain UV Space Telescope [PDF]
Abstract The Ultraviolet Transient Astronomy Satellite (ULTRASAT) is scheduled to be launched to geostationary orbit in 2027. It will carry a telescope with an unprecedentedly large field of view (204 deg2) and near-ultraviolet (NUV; 230–290 nm) sensitivity (22.5 mag, 5σ, at 900 s).
Yossi Shvartzvald +43 more
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Wide-field conversions for reflecting telescopes [PDF]
R. V. Willstrop
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A wide-field reflecting telescope.
F. Henroteau
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A Simple Wide-Field Cassegrain Telescope [PDF]
C. F. W. Harmer, C. G. Wynne
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Astrometric Calibration and Performance of the Dark Energy Spectroscopic Instrument Focal Plane
The Dark Energy Spectroscopic Instrument, consisting of 5020 robotic fiber positioners and associated systems on the Mayall telescope at Kitt Peak, Arizona, is carrying out a survey to measure the spectra of 40 million galaxies and quasars and produce ...
S. Kent +48 more
doaj +1 more source
Towards a BRICS Optical Transient Network (BRICS-OTN) [PDF]
This paper is based on a proposal submitted for a BRICS astronomy flagship program, which was presented at the 2019 meeting of the BRICS Astronomy Working Group, held in Rio de Janeiro from 29 September to 2 October 2019.
DAVID A.H. BUCKLEY +10 more
doaj +1 more source
Predicting the Yields of z > 6.5 Quasar Surveys in the Era of Roman and Rubin
About 70 luminous quasars discovered at z > 6.5 are strongly biased toward the bright end, thus not providing a comprehensive view of quasar abundance beyond the cosmic dawn. We present the predicted results of the Roman/Rubin high-redshift quasar survey,
Wei Leong Tee +5 more
doaj +1 more source

