Showing 41 - 60 results of 655 for search 'M.', query time: 0.10s Refine Results
  1. 41
    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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  2. 42
    ...We present a comparison of the SCUBA Half Degree Extragalactic Survey (SHADES) at 450 μm, 850 μm...
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  3. 43
    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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  4. 44
    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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    info:eu-repo/semantics/doctoralThesis
  5. 45
    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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  6. 46
    ... Experiment. We imaged a 270 arcmin² field to a 1σ depth of 0.48 − 0.73mJy/beam, making this one...
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  7. 47
    ... from 0.4 to 1.7 mJy, and derive the strongest constraints to date on the 1.1 mm source counts at flux...
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  8. 48
    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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  9. 49
    by Itziar Aretxaga, David Hughes
    Published 2011
    ...We report on the detection of an extremely bright (∼37 mJy at 1100 μm and ∼91 mJy at 880 μm...
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  10. 50
    ... sample of 48 H II regions in M81, observed by us with the 10.4-m GTC telescope, and of other 68 H II...
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    info:eu-repo/semantics/doctoralThesis
  11. 51
    by Carlos del Burgo Díaz
    Published 2013
    ... grains to km sized asteroidal bodies, and their infrared emission peaks at wavelengths 60–100 μm. Recent...
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  12. 52
    by David Hughes
    Published 2010
    ...We present results from Submillimeter Array (SMA) 860 μm subarcsecond astrometry...
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  13. 53
    by OMAR LOPEZ CRUZ
    Published 2007
    ... > -21, with a weaker dependence on radius than the red LFs. The dispersion of M* was determined...
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  14. 54
    ...² region with near uniform coverage to a depth of 0.96–1.16mJy beamˉ¹. Our robust catalogue contains 28...
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  15. 55
    ... y cuenta con un volumen de medición de 4.5m x 6m horizontal por 4.2m vertical. El instrumento...
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    info:eu-repo/semantics/report
  16. 56
    ... the sensor and the readout circuit. Offset error is reduced from 123 to 20 mV and gain error is reduced from...
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  17. 57
    by Itziar Aretxaga, David Hughes
    Published 2011
    ...) have flux densities >100 mJy at 500 μm, but are not visible in existing optical imaging. We fit light...
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  18. 58
    ...We present the 250, 350, and 500 μm detection of bright submillimeter emission in the direction...
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  19. 59
    ... at 100μm in the rest frame⁹. At 1 ≤ z ≤ 4, the peak is redshifted to wavelengths between 200 and 500 μm...
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  20. 60
    by IVANIO PUERARI
    Published 2009
    ... of wavenumbers with a gradual steepening from 3.6 or 4.5μm to 8.0 μm, in the order of an increasing contribution...
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    info:eu-repo/semantics/article