Bright galaxies in 5 medium redshift clusters. I. (Ascaso+, 2008)

Bibcode
2010yCat..34870453A
Ascaso, B.; Moles, M.; Aguerri, J. A. L.; Sanchez-Janssen, R.; Varela, J.
Bibliographical reference

VizieR On-line Data Catalog: J/A+A/487/453. Originally published in: 2008A&A...487..453A

Advertised on:
9
2010
Number of authors
5
IAC number of authors
0
Citations
0
Refereed citations
0
Description
Two of us (M.M. and J.A.L.A.) imaged five galaxy clusters with the 2.5m Nordic Optical Telescope (NOT) located at the Roque de Los Muchachos Observatory (La Palma). The observations were taken with the Stand Camera, with a field of view of 3'x3', a plate scale of 0.176"/pix, a gain of 1.69e-/ADU and a readout noise of 6.36e-. All images were taken under photometric sky conditions and very good seeing (between 0.5" and 0.8"). The clusters were observed through two broad-band filters: Gunn-r' (r) and Bessel B (B). (1 data file).
Type
Non-refereed
Galaxies
Photometry

It may interest you

  • Non-refereed
    ANDES, the high-resolution spectrograph for the ELT: design of the adaptive optics system
    ANDES,the high resolution spectrograph for the ELT, will work both in seeing limited mode and with Adaptive Optics (AO) correction. ANDES-SCAO is a single conjugated AO system working with natural guide stars, feeding the IFU coupled to the YJH spectrograph. The main science goal of the ANDES AO mode is the characterization of the exo-planet
    Pinna, Enrico et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13097E..4WP
    Citations
    0
  • Non-refereed
    HARMONI at ELT: verification tests of opto-mechanical mounts for HARMONI preoptics in cryogenic environment
    HARMONI is the high angular optical and near-IR integral field spectrograph (IFS) for the ELT. The instrument covers a large spectral range from 470 to 2450nm with resolving powers from 3300 to 18000 and spatial sampling from 60 to 4mas. A workhorse instrument designed to operate in two Adaptive Optics modes - Single-Conjugate Adaptive Optics (SCAO
    Hernández-González, Alberto et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13100E..52H
    Citations
    0