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Showing 1 - 20 results of 72 for search 'Accept (band)', query time: 0.23s Refine Results
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    .... There are "band gaps", frequency ranges over which no eigenmodes exist. A model ice shelf that is 50 km in lateral...
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  4. 4
    by Maercker, M., Burton, M. G.
    Published 2005
    ...L-band data of 30 Doradus at 3.5 micron taken with SPIREX (South Pole Infrared Explorer...
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  5. 5
    by Pipino, A., Pierpaoli, E.
    Published 2010
    ...We use the high quality pressure profiles of 239 galaxy clusters made available by the ACCEPT...
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  6. 6
    by Masetti, N.
    Published 1999
    ... detected the counterpart of this GRB in the near-infrared H band and optical V band. The power-law decline...
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    Report
  7. 7
    by Steinbring, Eric
    Published 2016
    ..., falling below 32 Jy/square-arcsec in N band, and to sub-Jansky levels by M and shortwards; reaching only...
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  8. 8
    by Yang, Bin, Hsieh, Henry
    Published 2011
    ...-resolution spectra of Scheila in the HK-band (1.4 - 2.5$μ$m) and low-resolution spectra in the KL-band (2.0...
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  9. 9
  10. 10
    ... measurements made at 91.5 and 103.5 GHz in Band 3. For both comparisons, flux density measurements were...
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    Article in Journal/Newspaper
  11. 11
    ... $T_\mathrm{d}$ and low dust abundance. For ALMA Band 6, there is no tendency of high-$T_\mathrm{d}$ LBGs...
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    Article in Journal/Newspaper
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    ... with those deduced from the two-year COBE-DMR data, although the Ka-band data prefer a normalization $\sim 1σ...
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  15. 15
    by Hamilton, J. -Ch., Ganga, K. M.
    Published 2001
    .../DIRBE data and the Haslam 408 MHz data. We find a marginal correlation between the dust and the Q-band...
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  16. 16
    ... constructed tipping radiometers to measure the broad band atmospheric transparency in the window around 350 $μ...
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  17. 17
    by Sollerman, Jesper
    Published 2003
    ... in the IR. Using also archival HST data for the knot, we have measured its broad band spectrum to rise...
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  18. 18
    ...We present observations of Galactic H alpha emission along two declination bands where the South...
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  19. 19
    ... coming from a spectral band centered around the Mg I b-triplet and with spectra from FGK stars are very...
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  20. 20
    .... This can be achieved by optimizing the frequency band in order to obtain a higher level of signal-to-noise...
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