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41по David Hughes“...We present an 880 μm Submillimeter Array (SMA) detection of the submillimeter galaxy SXDF 850.6...”
Опубликовано 2010
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42“...We present a comparison of the SCUBA Half Degree Extragalactic Survey (SHADES) at 450 μm, 850 μm...”
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43по David Hughes“... catalogue of BLAST 250-μm-selected galaxies, we re-measure the 70–870-μm flux densities at the positions...”
Опубликовано 2010
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44по JORGE ARMANDO ZAVALA SOLANO“... of SMGs. We also present deep observations at 450 and 850 μm in the Extended Groth Strip (EGS) field taken...”
Опубликовано 2017
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45по David Hughes“.... By calculating the covariance of these maps with catalogs of 24 μm sources from the Far-Infrared Deep...”
Опубликовано 2009
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46по 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...”
Опубликовано 2010
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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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48“... (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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49“...We report on the detection of an extremely bright (∼37 mJy at 1100 μm and ∼91 mJy at 880 μm...”
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50по 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...”
Опубликовано 2018
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51по Carlos del Burgo Díaz“... grains to km sized asteroidal bodies, and their infrared emission peaks at wavelengths 60–100 μm. Recent...”
Опубликовано 2013
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52по David Hughes“...We present results from Submillimeter Array (SMA) 860 μm subarcsecond astrometry...”
Опубликовано 2010
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53по OMAR LOPEZ CRUZ“... > -21, with a weaker dependence on radius than the red LFs. The dispersion of M* was determined...”
Опубликовано 2007
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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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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 -
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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57“...) have flux densities >100 mJy at 500 μm, but are not visible in existing optical imaging. We fit light...”
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58“...We present the 250, 350, and 500 μm detection of bright submillimeter emission in the direction...”
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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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60по 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...”
Опубликовано 2009
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