Galaxy star formation in different environments

Four different scenarios are considered: skilled and random forgeries with 5 and 20 training signatures. The original features are divided into four different groups according to

The study of the calibration vectors indicate that the square-root of the vari- ance is less than 20% of the mean Balmer artifact deviations and the study of quasar spectra

• Stellar kinematic signatures of intermediate mass black holes in nuclear stellar clusters (with T.. Compare star formation history deduced from fit to absorption line spectra

As a first step in our study, we characterized the mid-IR high-ionization emission lines produced by AGN and star-formation for a large sample of local galaxies, includ- ing

By measuring the two-point correlation function of galaxy populations that differ in redshift, color, luminosity, star-formation history and bias, and using high-resolution

With the aim to check the impact and usefulness of these mobile learning environments in education (focusing on helping students with time management by recommending them

It would also be possible to weight the different types of plagiarism because, in real teaching environments, the detection of single source plagiarism is usually less challenging

We present simulation results in miscellaneous TCP environments (different target rates, different round trip times, different packet sizes and share of resources with