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.
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DLSDara NormanList of Jupiter trojans (Greek camp) (1–100000)List of Jupiter trojans (Greek camp) (200001–300000)List of Jupiter trojans (Greek camp) (300001–400000)List of acronyms: DList of minor planet discoverersList of minor planets: 104001–105000List of minor planets: 107001–108000List of minor planets: 114001–115000List of minor planets: 143001–144000List of minor planets: 144001–145000List of minor planets: 147001–148000List of minor planets: 148001–149000List of minor planets: 154001–155000List of minor planets: 156001–157000List of minor planets: 159001–160000List of minor planets: 160001–161000List of minor planets: 189001–190000List of minor planets: 193001–194000List of minor planets: 196001–197000List of minor planets: 205001–206000List of minor planets: 208001–209000List of minor planets: 216001–217000List of minor planets: 220001–221000List of minor planets: 223001–224000List of minor planets: 226001–227000List of minor planets: 231001–232000List of minor planets: 242001–243000List of minor planets: 244001–245000List of minor planets: 245001–246000List of minor planets: 252001–253000List of minor planets: 257001–258000List of minor planets: 264001–265000List of minor planets: 267001–268000List of minor planets: 270001–271000List of minor planets: 275001–276000List of minor planets: 283001–284000List of minor planets: 285001–286000List of minor planets: 287001–288000
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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.
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Le Deep Lens Survey (en abrégé ...... effectuée entre 2000 et 2006.
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O Deep Lens Survey (DLS, abrev ...... s são liberados em tempo real.
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The Deep Lens Survey (DLS, sho ...... tes are released in real time.
@en
Глубинный линзированный обзор ...... отдельных участков для работы.
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1.000.136.224
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Le Deep Lens Survey (en abrégé ...... galement détectés et signalés.
@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.
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Deep Lens Survey
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Deep Lens Survey
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Deep Lens Survey
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Deep Lens Survey
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Глубинный линзированный обзор
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