Mostrando 101 - 120 resultados de 655 para a busca 'M.', tempo de busca: 0.15s Refinar Resultados
  1. 101
    por David Hughes, ITZIAR ARETXAGA MENDEZ
    Publicado em 2010
    ... and MIPS images covering the wavelength range 3.6–160 μm from the SINGS project. The availability...
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  2. 102
    por Itziar Aretxaga, David Hughes
    Publicado em 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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  3. 103
    por Carlos del Burgo Díaz
    Publicado em 2013
    ... star. No planet candidate around M-stars has been found, confirming the null detection hypothesis...
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  4. 104
    por OMAR LOPEZ CRUZ
    Publicado em 2010
    ..., measure their flux densities at 870 μm, and search for counterparts at other wavelengths to constrain...
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  5. 105
    por ITZIAR ARETXAGA MENDEZ, David Hughes
    Publicado em 2008
    ... submillimetre galaxies discovered via the SHADES 850μm SCUBA imaging in the Subaru-XMM Deep Field (SXDF...
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  6. 106
    por Itziar Aretxaga, David Hughes
    Publicado em 2011
    ... imaging of the COSMOS field with the AzTEC camera and ASTE 10 m telescope. These data yield one...
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  7. 107
    por David Hughes
    Publicado em 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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    info:eu-repo/semantics/article
  8. 108
    ..., power consumption and area. All the full-adders were designed with a 0.18-μm CMOS technology, and were...
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  9. 109
    por Emmaly Aguilar
    Publicado em 2018
    ... galaxies at high redshifts (z>1), with extreme star formation rates (SFR>500 Mꙩ/year). Recent studies...
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    info:eu-repo/semantics/doctoralThesis
  10. 110
    por David Hughes
    Publicado em 2009
    ... of the bulk of the high-redshift, submm galaxy population responsible for the 850 μm extragalactic background...
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  11. 111
    por ALINE GALINDO TELLEZ
    Publicado em 2017
    ... encapsulado, la caracterización e instalación de los fototubos a 4530 m de altitud. Las simulaciones, usando...
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  12. 112
    por David Hughes
    Publicado em 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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  13. 113
    por Itziar Aretxaga, David Hughes
    Publicado em 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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  14. 114
    por Itziar Aretxaga, David Hughes
    Publicado em 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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  15. 115
    por David Hughes, Itziar Aretxaga
    Publicado em 2011
    ... emission coincides with the stellar position having a flux density of 272 mJy, which is the largest among...
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  16. 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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  17. 117
    por Itziar Aretxaga, David Hughes
    Publicado em 2013
    ... 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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  18. 118
    por NOEMI JASMIN SALAZAR HERMENEGILDO
    Publicado em 2015
    ... spatial and temporal resolution. A modified laser speckle imaging (mLSI) enables computation of blood flow...
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  19. 119
    por David Hughes
    Publicado em 2010
    ...We use new large area far infrared maps ranging from 65-500 μm obtained with the AKARI...
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  20. 120
    por David Hughes
    Publicado em 2008
    ... at cosmological distances. Using a 2m Cassegrain telescope, BLAST images the sky onto a focal plane, which...
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