Optical and near IR galaxy number counts in the GOYA survey. The ages of Ellipticals

Bibcode
2007RMxAC..29..173P
Prieto, M.; Eliche-Moral, M. C.; Balcells, M.; García-Dabó, C. E.; Cristóbal-Hornillos, D.; Erwin, P.
Bibliographical reference

First Light Science with the GTC (Eds. R. Guzmán, C. Packham, J. M. Rodríguez-Espinosa, & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 29, pp. 173-173 (2007) (http://www.astroscu.unam.mx/~rmaa/)

Advertised on:
6
2007
Number of authors
6
IAC number of authors
0
Citations
0
Refereed citations
0
Description
Based on the GOYA Photometric Survey of the HST Groth-Westphal strip, we present galaxy number counts in B and Ks bands together with a model that simultaneously reproduces the counts and that does not need to add an extra population of blue dwarf galaxies to reproduce the blue excess of the counts at faint magnitudes.
Type
Non-refereed
H II regions

It may interest you

  • Non-refereed
    Design and manufacture of athermalized optomechanical mounts for GRANCAIN, the infrared imaging instrument for GTC's adaptive optics
    GRANCAIN (GRAN CAmara INfrarroja) is a first-light imaging instrument in the infrared J, H and K bands that will be integrated into the adaptive optics focus of the Gran Telescopio de Canarias. The purpose of the instrument is to capture SWIR diffraction-limited images for a field of view of 22x22 arcsec. The instrument boasts a telecentric optical
    González-Carretero, Eduardo D. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13100E..6VG
    Citations
    0
  • Non-refereed
    Optical coating facilities at the Instituto de Astrofísica de Canarias
    The Instrumentation Division of the Instituto de Astrofísica de Canarias (IAC) is involved since several years in upgrading its capacities to design and manufacture optical components. To this end, we have created a new laboratory (Centre for Advanced Optical Systems, CSOA) which will be capable to design, fabricate and qualify large optical
    Insausti, M. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13100E..23I
    Citations
    0
  • Non-refereed
    Measuring Rotation Periods and Stellar Oscillations in Red Giants with TESS Data
    TESS is a powerful engine for studying stellar variability. However, it has been challenging to adopt methods used for other space missions, such as Kepler, to infer rotation periods and solar-like oscillation frequencies in TESS data. The availability of multiple sectors of data for most targets, improved stability, and the release of new
    García, Rafael A. et al.

    Advertised on:

    7
    2024
    Bibcode
    2024tsc3.confE..32G
    Citations
    0