81
by RICARDO RETES ROMERO
Published 2017
... is obtained in the mass range from 0.1 M⊙ to 30 M⊙. The resulting MF have a log normal form for low masses...
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82
by Itziar Aretxaga, David Hughes
Published 2012
... arcsec and a depth of ≃ 1mJy. We have used the deep optical-to-radio multi-wavelength data in the SHADES...
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83
... and MIPS images covering the wavelength range 3.6–160 μm from the SINGS project. The availability...
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84
by Itziar Aretxaga, David Hughes
Published 2011
... imaging of the COSMOS field with the AzTEC camera and ASTE 10 m telescope. These data yield one...
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85
by OMAR LOPEZ CRUZ
Published 2010
..., measure their flux densities at 870 μm, and search for counterparts at other wavelengths to constrain...
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86
... submillimetre galaxies discovered via the SHADES 850μm SCUBA imaging in the Subaru-XMM Deep Field (SXDF...
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87
by Emmaly Aguilar
Published 2018
... galaxies at high redshifts (z>1), with extreme star formation rates (SFR>500 Mꙩ/year). Recent studies...
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88
..., power consumption and area. All the full-adders were designed with a 0.18-μm CMOS technology, and were...
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89
by David Hughes
Published 2010
... Telescope (BLAST) on a 9 deg² field near the South Ecliptic Pole at 250, 350, and 500 μm. The median 1σ...
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90
by ALINE GALINDO TELLEZ
Published 2017
... encapsulado, la caracterización e instalación de los fototubos a 4530 m de altitud. Las simulaciones, usando...
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91
by Itziar Aretxaga, David Hughes
Published 2011
... 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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92
by Itziar Aretxaga, David Hughes
Published 2011
... level of 0.32–0.71 mJy. This is one of the deepest and widest maps thus far at millimetre...
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93
by David Hughes, Itziar Aretxaga
Published 2011
... emission coincides with the stellar position having a flux density of 272 mJy, which is the largest among...
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94
by David Hughes
Published 2010
... SMGs that are candidates for harboring powerful AGNs on the basis of IRAC color selection (S₈ μm/S₄.₅ μ...
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95
by Esperanza Carrasco Licea
Published 2011
... in the first 2 km above the 1.5 m and the 2.1 m telescopes decrease by 15.8% and 13.6%, respectively...
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96
by David Hughes
Published 2009
... of the bulk of the high-redshift, submm galaxy population responsible for the 850 μm extragalactic background...
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97
...) with a thickness of 8 ± 2nm. This structure gets an Isc of 43 ± 2mA and a Voc of 0.44 ± 0.02 V...
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98
...-magnitude reduction is used to demonstrate that an M -bit MASH architecture dithered by a simple M -bit...
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99
by David Hughes
Published 2010
...We use new large area far infrared maps ranging from 65-500 μm obtained with the AKARI...
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100
by David Hughes
Published 2008
... at cosmological distances. Using a 2m Cassegrain telescope, BLAST images the sky onto a focal plane, which...
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