This site will be out of service for maintenance on Monday, May 6 from 7:30 to 8:00.

Final analysis of ELAIS 15-{mu}m (Vaccari+, 2005)

Bibcode
2005yCat..73580397V
Vaccari, M.; Lari, C.; Angeretti, L.; Fadda, D.; Gruppioni, C.; Pozzi, F.; Prouton, O.; Aussel, H.; Babbedge, T.; Ciliegi, P.; Franceschini, A.; Gonzalez-Solares, E.; La Franca, F.; Oliver, S.; Perez-Fournon, I.; Rowan-Robinson, M.; Serjeant, S.; Vaisanen, P.
Bibliographical reference

VizieR On-line Data Catalog: J/MNRAS/358/397. Originally published in: 2005MNRAS.358..397V

Advertised on:
11
2005
Number of authors
18
IAC number of authors
0
Citations
0
Refereed citations
0
Description
We present the final analysis of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) 15-{mu}m observations, carried out with the ISO Camera (ISOCAM) instrument on board the ISO. The data-reduction method, known as the Lari Method, is based on a mathematical model of the behaviour of the detector and was specifically designed for the detection of faint sources in ISOCAM/ISO Photopolarimeter (ISOPHOT) data. The method is fully interactive and leads to very reliable and complete source lists. The resulting catalogue includes 1923 sources detected with signal-to-noise ratio of >5 in the 0.5-100mJy flux range and over an area of 10.85deg2 split into four fields, making it the largest non-serendipitous extragalactic source catalogue obtained to date from the ISO data. (1 data file).
Type
Non-refereed
Surveys
Galaxies

It may interest you

  • Non-refereed
    The NIKA2 Sunyaev-Zeldovich Large Program. Sample and upcoming product public release
    The NIKA2 camera operating at the IRAM 30-m telescope excels in high-angular resolution mapping of the thermal Sunyaev-Zel'dovich effect towards galaxy clusters at intermediate and high-redshift. As part of the NIKA2 guaranteed-time, the SZ Large Program (LPSZ) aims at tSZ-mapping a representative sample of SZ-selected galaxy clusters in the
    Perotto, L. et al.

    Advertised on:

    6
    2024
    Bibcode
    2024EPJWC.29300040P
    Citations
    0
  • Non-refereed
    3D scaling laws and projection effects in The300-NIKA2 Sunyaev-Zeldovich Large Program Twin Samples
    The abundance of galaxy clusters with mass and redshift is a wellknown cosmological probe. The cluster mass is a key parameter for studies that aim to constrain cosmological parameters using galaxy clusters, making it critical to understand and properly account for the errors in its estimates. Subsequently, it becomes important to correctly
    Paliwal, A. et al.

    Advertised on:

    6
    2024
    Bibcode
    2024EPJWC.29300037P
    Citations
    0
  • Non-refereed
    CONCERTO: Instrument and status
    CONCERTO (CarbON CII line in post-rEionization and ReionizaTiOn) is a low-resolution Fourier transform spectrometer dedicated to the study of star-forming galaxies and clusters of galaxies in the transparent millimeter windows from the ground. It is characterized by a wide instantaneous 18.6 arcmin field of view, operates at 130-310 GHz, and was
    Fasano, Alessandro et al.

    Advertised on:

    6
    2024
    Bibcode
    2024EPJWC.29300018F
    Citations
    0