21
...This work presents novel multipliers for Montgomery multiplication defined on binary fields GF(2m...
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22
by Manolis Plionis
Published 2010
... model of Basilakos et al., we manage to break the σ₈–Ω degeneracy. The resulting cosmological...
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23
...A hardware architecture for GF(2m) multiplication and its evaluation in a hardware architecture...
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24
by MAYRA SANTIAGO CORTES
Published 2008
...En esta tesis presento el estudio de la población de cúmulos estelares compactos en M81. Los datos...
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25
.... The wavelength of the light is assumed to be the important communications wavelength of 1.54 μm. A realistic...
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26
by David Hughes
Published 2009
..., and 500μm. We perform jackknife and other tests to confirm the reality of the signal. The measured...
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27
by YALIA DIVAKARA MAYYA
Published 2008
... in the currently active nuclear starburst region, and in the post-starburst disk of M82. Images obtained...
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29
by Esperanza Carrasco Licea
Published 2003
... calidad de imagen, cuando se usa la correctora del campo, del telescopio de 2.1m del Observatorio...
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30
by JOSE ANTONIO ARAIZA DURAN
Published 2016
... of the 2.1-m telescope at the San Pedro Mártir Observatory using the primary mirror's active cell as the wave...
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34
by David Hughes
Published 2010
...We present an 880 μm Submillimeter Array (SMA) detection of the submillimeter galaxy SXDF 850.6...
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35
...We present a comparison of the SCUBA Half Degree Extragalactic Survey (SHADES) at 450 μm, 850 μm...
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36
by JORGE ARMANDO ZAVALA SOLANO
Published 2017
... of SMGs. We also present deep observations at 450 and 850 μm in the Extended Groth Strip (EGS) field taken...
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37
by David Hughes
Published 2010
... catalogue of BLAST 250-μm-selected galaxies, we re-measure the 70–870-μm flux densities at the positions...
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38
by David Hughes
Published 2009
.... By calculating the covariance of these maps with catalogs of 24 μm sources from the Far-Infrared Deep...
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39
... Experiment. We imaged a 270 arcmin² field to a 1σ depth of 0.48 − 0.73mJy/beam, making this one...
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40
by Itziar Aretxaga, David Hughes
Published 2011
... (100, 160 μm), CSO/SHARC II (350μm), and CARMA and PdBI (3 mm). We do not detect CO(5 → 4) line...
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