z=1-3 ULIRGs from the Spitzer SWIRE survey (Berta+, 2007)

Bibcode
2007yCat..34670565B
Berta, S.; Lonsdale, C. J.; Siana, B.; Farrah, D.; Smith, H. E.; Polletta, M. C.; Franceschini, A.; Fritz, J.; Perez-Fournon, I.; Rowan-Robinson, M.; Shupe, D.; Surace, J.
Bibliographical reference

VizieR On-line Data Catalog: J/A+A/467/565. Originally published in: 2007A&A...467..565B

Advertised on:
10
2007
Number of authors
12
IAC number of authors
0
Citations
0
Refereed citations
0
Description
We present Keck/LRIS optical spectroscopy of 35 z>=1.4 luminous IR galaxies in the Spitzer Wide-area Infra-Red Extragalactic survey (SWIRE) northern fields (Lockman Hole, ELAIS-N1, ELAIS-N2). The primary targets belong to the "IR-peak" class of galaxies, having the 1.6{mu}m (restframe) stellar feature detected in the IRAC Spitzer channels. The spectral energy distributions of the main targets are thoroughly analyzed, by means of spectro-photometric synthesis and multi-component fits (stars + starburst dust + AGN torus). Observations were carried out in multi-object mode with the Low Resolution Imaging Spectrometer (LRIS) at the Cassegrain focus of the Keck-I telescope, during the nights of May 27th and 28th, 2006. (6 data files).
Type
Non-refereed

It may interest you

  • Non-refereed
    New Robotic Telescope system progress towards critical design review
    The 4m class New Robotic Telescope (NRT) is an optical facility designed to revolutionize the rapid follow-up and classification of variable and transient objects. The project is at the stage where key systems are progressing through their detailed design phases, which presents a major engineering challenge for all project partners to manage design
    Copley, David et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..3WC
    Citations
    0
  • Non-refereed
    Phase diversity application on the EST MCAO testbench
    Phase Diversity (PD) is a technique widely used to measure and compensate for Non-Common Path Aberrations (NCPA) in optical systems. Beyond its traditional applications, PD has found further uses in solar astrophysics, where it enhances image quality by processing multiple images to correct residual aberrations. In this work, we introduce a
    Rodriguez-Linares, Nicolas et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13097E..5OR
    Citations
    0
  • Non-refereed
    First light of the upgraded Gregor Infrared Spectrograph
    For more than ten years, the Gregor Infrared Spectrograph (GRIS) has been the infrared spectropolarimeter on the Gregor telescope since its inauguration in 2012. The instrument mainly performs polarimetric observations of the wavelength regions at 1083 and 1565nm, which have high scientific potential. There, observers can find spectral lines that
    Quintero Noda, C. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..42Q
    Citations
    0