This site will be out of service for maintenance tomorrow, May 15 from 7:00 to 9:30 am

Deep Optical and Near Infrared Observations in ELAIS Areas

Bibcode
2001ESASP.460..421G
González-Solares, E. A.; Pérez-Fournon, I.; McMahon, R.; Sabbey, C.; Almaini, O.; Manners, J.; Willott, C.; Cabrera-Guerra, F.; Ciliegi, P.; Lawrence, A.; Mann, B.; Oliver, S. J.; Rowan-Robinson, M.; Serjeant, S.; Verma, A.
Bibliographical reference

The Promise of the Herschel Space Observatory. Eds. G.L. Pilbratt, J. Cernicharo, A.M. Heras, T. Prusti, & R. Harris. ESA-SP 460, p. 421

Advertised on:
7
2001
Number of authors
15
IAC number of authors
3
Citations
1
Refereed citations
1
Description
We present deep optical and near infrared imaging over half square degree of sky in the centres of the ELAIS regions N1 and N2 and coincident with deep XMM/Chandra observations. The data have been obtained with the Wide Field Camera (WFC) and the Cambridge InfraRed Survey Instrument (CIRSI) both at the Isaac Newton Telescope (Observatorio del Roque de los Muchachos, Canary Islands). Limiting magnitudes achieved are g'=26.7, r'=26.2, i'=25.0 and H=20.2 (3 sigma). These data have been used to identify the faint optical counterparts of the Infrared Space Observatory (ISO), radio and X-ray sources in these areas.
Type
Non-refereed
Galaxies
Surveys

It may interest you

  • Non-refereed
    Constraining the core-rotation rate along the red-giant evolution
    The evolution of the core rotation rate of red giant stars is a key parameter in understanding the stellar behavior in the late phases of stellar evolution. Thanks to the mixed-dipole modes, we can constrain the core rotation and internal rotational gradient as a star advances through the red-giant phase. This master thesis presents a pipeline
    Muntean, N. et al.

    Advertised on:

    3
    2024
    Bibcode
    2024aecc.conf...34M
    Citations
    0
  • Non-refereed
    Identification of Superclusters and their Properties in the Sloan Digital Sky Survey
    Superclusters are the largest massive structures in the cosmic web on tens to hundreds of megaparsecs (Mpc) scales. They are the largest assembly of galaxy clusters in the Universe. Apart from a few detailed studies of such structures, their evolutionary mechanism is still an open question. In order to address and answer the relevant questions, a
    Sankhyayan, Shishir et al.

    Advertised on:

    1
    2024
    Bibcode
    2024asi..confP..81S
    Citations
    0
  • Non-refereed
    Rapid multiwavelength variability reveals jet emission in the black hole binary V404 Cygni in quiescence
    Spitzer Space Telescope observations of several quiescent black hole low mass X-ray binaries (LMXBs) have shown mid-infrared excesses above the emission of a companion star. The excess has been proposed to originate from either a relativistic jet or circumbinary disk. If the mid-IR originates in a jet, then it probes the region closest to the black
    Borowski, Eric et al.

    Advertised on:

    5
    2024
    Bibcode
    2024HEAD...2130105B
    Citations
    0