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41Yazar: David Hughes“...We present an 880 μm Submillimeter Array (SMA) detection of the submillimeter galaxy SXDF 850.6...”
Baskı/Yayın Bilgisi 2010
Tam Metin Erişim
info:eu-repo/semantics/article -
42“...We present a comparison of the SCUBA Half Degree Extragalactic Survey (SHADES) at 450 μm, 850 μm...”
Tam Metin Erişim
info:eu-repo/semantics/article -
43Yazar: David Hughes“... catalogue of BLAST 250-μm-selected galaxies, we re-measure the 70–870-μm flux densities at the positions...”
Baskı/Yayın Bilgisi 2010
Tam Metin Erişim
info:eu-repo/semantics/article -
44Yazar: JORGE ARMANDO ZAVALA SOLANO“... of SMGs. We also present deep observations at 450 and 850 μm in the Extended Groth Strip (EGS) field taken...”
Baskı/Yayın Bilgisi 2017
Tam Metin Erişim
info:eu-repo/semantics/doctoralThesis -
45Yazar: David Hughes“.... By calculating the covariance of these maps with catalogs of 24 μm sources from the Far-Infrared Deep...”
Baskı/Yayın Bilgisi 2009
Tam Metin Erişim
info:eu-repo/semantics/article -
46Yazar: EMMALY AGUILAR PEREZ, ITZIAR ARETXAGA MENDEZ, DANIEL FERRUSCA RODRIGUEZ, David Hughes“... Experiment. We imaged a 270 arcmin² field to a 1σ depth of 0.48 − 0.73mJy/beam, making this one...”
Baskı/Yayın Bilgisi 2010
Tam Metin Erişim
info:eu-repo/semantics/article -
47“... from 0.4 to 1.7 mJy, and derive the strongest constraints to date on the 1.1 mm source counts at flux...”
Tam Metin Erişim
info:eu-repo/semantics/article -
48“... (100, 160 μm), CSO/SHARC II (350μm), and CARMA and PdBI (3 mm). We do not detect CO(5 → 4) line...”
Tam Metin Erişim
info:eu-repo/semantics/article -
49“...We report on the detection of an extremely bright (∼37 mJy at 1100 μm and ∼91 mJy at 880 μm...”
Tam Metin Erişim
info:eu-repo/semantics/article -
50Yazar: Karla Ziboney Arellano Córdova“... sample of 48 H II regions in M81, observed by us with the 10.4-m GTC telescope, and of other 68 H II...”
Baskı/Yayın Bilgisi 2018
Tam Metin Erişim
info:eu-repo/semantics/doctoralThesis -
51Yazar: Carlos del Burgo Díaz“... grains to km sized asteroidal bodies, and their infrared emission peaks at wavelengths 60–100 μm. Recent...”
Baskı/Yayın Bilgisi 2013
Tam Metin Erişim
info:eu-repo/semantics/article -
52Yazar: David Hughes“...We present results from Submillimeter Array (SMA) 860 μm subarcsecond astrometry...”
Baskı/Yayın Bilgisi 2010
Tam Metin Erişim
info:eu-repo/semantics/article -
53Yazar: OMAR LOPEZ CRUZ“... > -21, with a weaker dependence on radius than the red LFs. The dispersion of M* was determined...”
Baskı/Yayın Bilgisi 2007
Tam Metin Erişim
info:eu-repo/semantics/article -
54“...² region with near uniform coverage to a depth of 0.96–1.16mJy beamˉ¹. Our robust catalogue contains 28...”
Tam Metin Erişim
info:eu-repo/semantics/article -
55“... y cuenta con un volumen de medición de 4.5m x 6m horizontal por 4.2m vertical. El instrumento...”
Tam Metin Erişim
info:eu-repo/semantics/report -
56Yazar: Luis Antonio Carrillo-Martínez, MARIA TERESA SANZ PASCUAL, Joel Molina Reyes“... the sensor and the readout circuit. Offset error is reduced from 123 to 20 mV and gain error is reduced from...”
Baskı/Yayın Bilgisi 2013
Tam Metin Erişim
info:eu-repo/semantics/article -
57“...) have flux densities >100 mJy at 500 μm, but are not visible in existing optical imaging. We fit light...”
Tam Metin Erişim
info:eu-repo/semantics/article -
58Yazar: ITZIAR ARETXAGA MENDEZ, David Hughes, ALFREDO AGUSTIN MONTAÑA BARBANO“...We present the 250, 350, and 500 μm detection of bright submillimeter emission in the direction...”
Baskı/Yayın Bilgisi 2009
Tam Metin Erişim
info:eu-repo/semantics/article -
59“... at 100μm in the rest frame⁹. At 1 ≤ z ≤ 4, the peak is redshifted to wavelengths between 200 and 500 μm...”
Tam Metin Erişim
info:eu-repo/semantics/article -
60Yazar: IVANIO PUERARI“... of wavenumbers with a gradual steepening from 3.6 or 4.5μm to 8.0 μm, in the order of an increasing contribution...”
Baskı/Yayın Bilgisi 2009
Tam Metin Erişim
info:eu-repo/semantics/article