Deep Lens Survey
The Deep Lens Survey (DLS, short for "Deep Gravitational Lensing Survey") is an ultra-deep multi-band optical survey of seven 4 square degree fields. Mosaic CCD imagers at the National Optical Astronomy Observatory's Blanco (Cerro Tololo) and Mayall telescopes (Kitt Peak) are being used. The deep fields took five years to complete (2001–2006), in four bands: B, V, R, and z', to 29/29/29/28 mag per square arcsecond surface brightness. Optical transient events (including moving objects such as minor planets and comets) and supernova candidates are released in real time.
Deep Lens Survey
The Deep Lens Survey (DLS, short for "Deep Gravitational Lensing Survey") is an ultra-deep multi-band optical survey of seven 4 square degree fields. Mosaic CCD imagers at the National Optical Astronomy Observatory's Blanco (Cerro Tololo) and Mayall telescopes (Kitt Peak) are being used. The deep fields took five years to complete (2001–2006), in four bands: B, V, R, and z', to 29/29/29/28 mag per square arcsecond surface brightness. Optical transient events (including moving objects such as minor planets and comets) and supernova candidates are released in real time.
has abstract
Le Deep Lens Survey (en abrégé ...... s magnitudes 29, 29, 29 et 28.
@fr
O Deep Lens Survey (DLS, abrev ...... s são liberados em tempo real.
@pt
The Deep Lens Survey (DLS, sho ...... tes are released in real time.
@en
Глубинный линзированный обзор ...... отдельных участков для работы.
@ru
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Le Deep Lens Survey (en abrégé ...... s magnitudes 29, 29, 29 et 28.
@fr
O Deep Lens Survey (DLS, abrev ...... s são liberados em tempo real.
@pt
The Deep Lens Survey (DLS, sho ...... tes are released in real time.
@en
Глубинный линзированный обзор ...... рировались в реальном времени.
@ru
label
Deep Lens Survey
@en
Deep Lens Survey
@fr
Deep Lens Survey
@pt
Глубинный линзированный обзор
@ru