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181av Manolis Plionis“... of Mₕ ≃ 2.7 (±0.6) × 10¹² h⁻¹MꙨ, while the corresponding value for optical galaxies is Mₕ≃ 6.3 (±2.1...”
Publicerad 2012
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182av SUSANA ALEJANDRA TORRES HURTADO“... de a-Si:H. Por debajo de 3 mW las micropartículas son atrapadas en el centro del haz, entre 3 y 11 m...”
Publicerad 2016
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183av Héctor Christian Bandala Hernández“... in CMOS technologies, applied to di_erent 2-D sensor arrays: a 3x3 cells array fabricated in 0.35m AMI...”
Publicerad 2018
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184“...Using the 100-m Green Bank Telescope, we have conducted a cm-wavelength search for CO J=1-0 line...”
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185av LUZ KARINE SANDOVAL GRANADOS“... room (3.9m x 7m), four base stations were transmitting continuously in different channels and a mobile...”
Publicerad 2011
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186av MIRIAM ESTEFANIA CISNEROS GONZALEZ“...) designed to the 10.4m GTC (Gran Telescopio de Canarias) telescope in La Palma, Spain. MEGARA (Multi...”
Publicerad 2016
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187av WILLIAM FRANK WALL“... 1.25–250 THz (240–1.25 μm) spectral ranges in order to reconstruct the global SEDs of the Magellanic...”
Publicerad 2010
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188av Itziar Aretxaga“... ± 0.001, and measure molecular gas masses of (1–3) ×10¹°Mꙩ, corrected for lens amplification and assuming...”
Publicerad 2011
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189av CARLOS GERARDO TREVIÑO PALACIOS, OSCAR BALDOVINO PANTALEON, RUBEN RAMOS GARCIA, MARCELO DAVID ITURBE CASTILLO“... lens with a photoinduced focal length dependent on the Gaussian beam radius ωᵐ (where m is an integer...”
Publicerad 2008
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190av ITZIAR ARETXAGA MENDEZ“... 10.4m telescope at the Observatorio del Roque de los Muchachos on La Palma. One of the science drivers...”
Publicerad 2008
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191“...ASTE is a 10-m submillimeter telescope operating in Atacama desert in northern Chile since 2002...”
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192av MARIELA MARTINEZ PAREDES“...) hemos realizado observaciones en el Gran Telescopio CANARIAS de 10.4 m (GTC) de 20 QSO cercanos (z < 0.1...”
Publicerad 2016
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193av Carlos del Burgo Díaz“..., which began observations at the 3.8-m United Kingdom Infrared Telescope. Light curves comprising almost...”
Publicerad 2012
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194av PAULINA MARIANA MAYA HERNANDEZ“... integrados de amplificador lockin con tecnología CMOS de 0.18m y voltaje de alimentación única de 1.8V...”
Publicerad 2012
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195av ALFREDO AGUSTIN MONTAÑA BARBANO“... high-resolution simulations of the SZE produced by massive galaxy clusters (M > 1014 M_) at different...”
Publicerad 2012
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196av Francisco Javier López Tiro“... levels up to 1000μm. The proposed model improves the visualization of superficial blood vessels (up...”
Publicerad 2019
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197av Manolis Plionis“...We use group-sized haloes, with masses in the range 1013 < M < 2 × 1014 h−1Mʘ, identified with a...”
Publicerad 2007
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198av ITZIAR ARETXAGA MENDEZ, David Hughes, ENRIQUE GAZTAÑAGA BALBAS, Douglas Scott, Duncan Farrah, Matt Jarvis, Laura Silva“...-mm-FIR colours of 120 robustly detected 850μm sources in the Lockman Hole East (LH) and Subaru XMM...”
Publicerad 2007
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199“... performed in a vacuum chamber with pressure P=10 mTorr. In general the S(f) measured on our devices...”
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200“... 4.9x10⁶ and 4.3x10⁷Mꙩ and between 1.8 and 8.7x10⁶Mꙩ for the individual star clusters. Stellar and gas...”
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