Near infrared galaxy counts and evolution from the wide field alhambra survey

MD simulations in this and previous work has allowed us to propose a relation between the nature of the interactions at the interface and the observed properties of nanofluids:

 The expansionary monetary policy measures have had a negative impact on net interest margins both via the reduction in interest rates and –less powerfully- the flattening of the

Jointly estimate this entry game with several outcome equations (fees/rates, credit limits) for bank accounts, credit cards and lines of credit. Use simulation methods to

In our sample, 2890 deals were issued by less reputable underwriters (i.e. a weighted syndication underwriting reputation share below the share of the 7 th largest underwriter

For the elliptical resonator fabricated by the hybrid approach it has been measured the resonance frequency, but still more effort in the fabrication process is needed in order

 The relative strength of these lines coupled with the overall form of the spectra will allow the spectra type to be accurately determined... Some views of EMIR.. E-II:

The fluctuations of the complex amplitude, measured for a given spatial frequency as a function of wavelength (top panel), can be related to the different values of the corresponding

Relationship between the total cluster stellar mass and the photometric blue fraction for the ALHAMBRA cluster and group sample stacked into different redshift bins. The galaxy