Sentence examples for deeper surveys from inspiring English sources

In deeper surveys one will probe more easily faint HI structures, typically located in the vicinity of galaxies, such as tails, filaments, and extraplanar gas.

AKARI has also provided deeper surveys centered on the North and South Ecliptic Poles (e.g., Wada et al., 2008; Matsuura et al., 2011; Takagi et al., 2012).

The modified cSBT method for high-throughput, high-resolution HLA typing should accelerate studies involving large cohort genotyping, and allow a deeper survey of worldwide HLA polymorphism in historically understudied regions [ 32].

Because M. lucifugus is a good candidate for investigating possible HT, a deeper survey of Helitrons was performed, a previously uncharacterized family (HeligloriaB_Ml) was identified, and was used as a starting point for a series of Blast searches.

Finally, the properties of the X-ray sources populating the deep surveys will be described and compared with the predictions of the most recent synthesis models.

Optical and near-infrared (NIR) deep surveys have been very powerful for detecting very faint sources in the high-redshift (z) universe.

With reasonable assumptions, however, we can make predictions for the source populations that we should detect in the AXAF and XMM deep surveys.

In the near- and mid-infrared regions, wide and deep surveys of pre-selected sky areas will be made with large low-noise arrays.

From the deep surveys performed with the ROSAT and ASCA X-ray observatories, we have now built up a plausible picture of the constitution of the X-ray background and the way in which AGNs (and starburst nuclei surrounding AG Ns account for it.

Deep surveys at mid-infrared through submillimeter wavelengths indicate that a substantial fraction of the total luminosity output from galaxies at high redshift (z>1) emerges at wavelengths 30 300 μm.

Deep surveys at 850μm from Mauna Kea using the SCUBA camera on the JCMT appear to have discovered a substantial population of ultraluminous infrared galaxies (ULIGs: Lir > 1012L⊙) at high redshift (z ∼ 1 4).