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101“... and MIPS images covering the wavelength range 3.6–160 μm from the SINGS project. The availability...”
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102“... arcsec and a depth of ≃ 1mJy. We have used the deep optical-to-radio multi-wavelength data in the SHADES...”
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103Autor Carlos del Burgo Díaz“... star. No planet candidate around M-stars has been found, confirming the null detection hypothesis...”
Vydáno 2013
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104Autor OMAR LOPEZ CRUZ“..., measure their flux densities at 870 μm, and search for counterparts at other wavelengths to constrain...”
Vydáno 2010
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105“... submillimetre galaxies discovered via the SHADES 850μm SCUBA imaging in the Subaru-XMM Deep Field (SXDF...”
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106“... imaging of the COSMOS field with the AzTEC camera and ASTE 10 m telescope. These data yield one...”
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107Autor David Hughes“... Telescope (BLAST) on a 9 deg² field near the South Ecliptic Pole at 250, 350, and 500 μm. The median 1σ...”
Vydáno 2010
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108“..., power consumption and area. All the full-adders were designed with a 0.18-μm CMOS technology, and were...”
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109Autor Emmaly Aguilar“... galaxies at high redshifts (z>1), with extreme star formation rates (SFR>500 Mꙩ/year). Recent studies...”
Vydáno 2018
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110Autor David Hughes“... of the bulk of the high-redshift, submm galaxy population responsible for the 850 μm extragalactic background...”
Vydáno 2009
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111Autor ALINE GALINDO TELLEZ“... encapsulado, la caracterización e instalación de los fototubos a 4530 m de altitud. Las simulaciones, usando...”
Vydáno 2017
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112Autor David Hughes“... SMGs that are candidates for harboring powerful AGNs on the basis of IRAC color selection (S₈ μm/S₄.₅ μ...”
Vydáno 2010
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113“... Survey field carried out to a 1σ ≈ 1.26 mJy beam⁻¹ depth with the AzTEC camera mounted on the 10-m...”
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114“... level of 0.32–0.71 mJy. This is one of the deepest and widest maps thus far at millimetre...”
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115“... emission coincides with the stellar position having a flux density of 272 mJy, which is the largest among...”
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116“... is frequency modulated. An AGC circuit in a 0.35μm and biased with VDD=3V is presented in this paper...”
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117“... Magellanic Cloud (SMC). This SMG is detected as a 43.3 ± 8.4 mJy point source (MM J01071−7302, hereafter MMJ...”
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118Autor NOEMI JASMIN SALAZAR HERMENEGILDO“... spatial and temporal resolution. A modified laser speckle imaging (mLSI) enables computation of blood flow...”
Vydáno 2015
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119Autor David Hughes“...We use new large area far infrared maps ranging from 65-500 μm obtained with the AKARI...”
Vydáno 2010
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120Autor David Hughes“... at cosmological distances. Using a 2m Cassegrain telescope, BLAST images the sky onto a focal plane, which...”
Vydáno 2008
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