Home > Data Vault > Surveys

Surveys Using NRAO Telescopes

Welcome to the Data Vault. Here you will find information about how to access raw and calibrated data, images, previously proposed observations, and published findings from observations made with NRAO telescopes.

VLA

Overall view of the VLA, looking South.

    A project designed to produce the radio equivalent of the Palomar Observatory Sky Survey over 10,000 square degrees of the North Galactic Cap. FIRST was observed with the VLA at L band in the B array configuration and contains 28,292 images.
  • CLASS - Cosmic Lens All-Sky Survey
    A high-resolution VLA radio image survey of over 10,000 flat-spectrum radio sources in order to create the largest and best studied statistical sample of radio-loud gravitationally lensed systems. Observations conducted using the VLA at X band in the A array configuration. The archive contains 14,674 images.
  • MITVLA - MITVLA Gravitational Lens Snapshot Survey
    The 19 year MITVLA gravitational lens survey contains over 5,000 images, and was observed with the VLA in the A array configuration at C and X bands. The are MITVLA 4,318 images in the archive.
  • GBT HI Galaxy Survey
  • 2cmVLBA - NRAO VLBA 2cm Survey
    An imaging survey of compact radio sources at 15 GHZ. The VLBA provides images having milliarcsecond resolution. The survey achieves a dynamic range of typically exceeding 1000:1, with a typical noise limit (rms) of 0.35 milli-Jansky. The survey covers the entire sky, was observed at 2cm wavelength and contains 1,710 images.
  • VCS - NRAO VLBA Calibrator Source Survey
    A catalog containing milliarcsecond-accurate positions (and images) of 1,659 extragalactic radio sources distributed over the northern sky is presented-the Very Long Baseline Array Calibrator Survey (VCS). The positions have been derived from astrometric analysis of dual-frequency 2.3 and 8.4 GHz VLBA snapshot observations.
  • VLSS - The VLA Low-frequency Sky Survey
    The VLA Low-Frequency Sky Survey (VLSS) is a 74 MHz (4-meter wavelength) continuum survey covering the entire sky north of -30° declination. Utilizing the Very Large Array (VLA), the survey provides images with a resolution of 80" and with an average rms noise of 0.1 Jy/beam. Complete details are in "The VLA Low-Frequency Sky Survey" (Astron. J., vol. 134, p. 1245).
Staff | Contact Us | Careers | Help | Policies | Diversity Policy | Site Map