141
by VALERIA RODRIGUEZ FAJARDO
Published 2010
... used as 3.55 μm-diameter polystyrene beads. In the setup for Raman spectroscopy we use a 532 nm diode...
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142
by JESUS ABRAHAM REYES DE LIBRADO
Published 2013
...1. A multi-wavelength photometric catalog of about 38 000 sources from 2 μm to 1.1 mm in a 1 square...
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143
by David Hughes
Published 2010
... for these in the Herschel-ATLAS (H-ATLAS) science demonstration phase (SDP) survey catalog. We cross-matched 500 μm sources...
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144
... de a-Si:H. Por debajo de 3 mW las micropartículas son atrapadas en el centro del haz, entre 3 y 11 m...
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145
... in CMOS technologies, applied to di_erent 2-D sensor arrays: a 3x3 cells array fabricated in 0.35m AMI...
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146
by Manolis Plionis
Published 2012
... of Mₕ ≃ 2.7 (±0.6) × 10¹² h⁻¹MꙨ, while the corresponding value for optical galaxies is Mₕ≃ 6.3 (±2.1...
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147
by David Hughes
Published 2009
..., and 500 μm from the 2006 flight of the Balloon-borne Large Aperture Submillimeter Telescope. The map has...
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148
by David Hughes
Published 2009
... μm background is generated at z≲ 1 and the 500 μm background generated at z ≳ 1. A significant...
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149
by EVGUENI LEKHT EVGUENIEVICH
Published 2008
... in the giant molecular cloud Cygnus OB7 are presented. The observations were carried out on the 22-m radio...
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150
by NICOLAY SILANTIEV ALEKSEEVICH
Published 2008
... and the values of magnetic energy fluctuations. The spectra of polarization in the optical (λ = 0–1 μm), infrared...
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151
by MARIELA MARTINEZ PAREDES
Published 2016
...) hemos realizado observaciones en el Gran Telescopio CANARIAS de 10.4 m (GTC) de 20 QSO cercanos (z < 0.1...
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152
...) designed to the 10.4m GTC (Gran Telescopio de Canarias) telescope in La Palma, Spain. MEGARA (Multi...
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153
by Itziar Aretxaga
Published 2011
... ± 0.001, and measure molecular gas masses of (1–3) ×10¹°Mꙩ, corrected for lens amplification and assuming...
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154
by Carlos del Burgo Díaz
Published 2012
..., which began observations at the 3.8-m United Kingdom Infrared Telescope. Light curves comprising almost...
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155
by WILLIAM FRANK WALL
Published 2010
... 1.25–250 THz (240–1.25 μm) spectral ranges in order to reconstruct the global SEDs of the Magellanic...
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156
by ITZIAR ARETXAGA MENDEZ
Published 2008
... 10.4m telescope at the Observatorio del Roque de los Muchachos on La Palma. One of the science drivers...
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157
...ASTE is a 10-m submillimeter telescope operating in Atacama desert in northern Chile since 2002...
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158
... lens with a photoinduced focal length dependent on the Gaussian beam radius ωᵐ (where m is an integer...
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159
by LUZ KARINE SANDOVAL GRANADOS
Published 2011
... room (3.9m x 7m), four base stations were transmitting continuously in different channels and a mobile...
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160
...Using the 100-m Green Bank Telescope, we have conducted a cm-wavelength search for CO J=1-0 line...
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