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The Palomar Digital Sky Survey (DPOSS)

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arxiv astro-ph/9809187 v1 pith:DESCEJXC submitted 1998-09-15 astro-ph

classification astro-ph
keywords surveydatascientificdescribedigitaldposslimitsome
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abstract

We describe DPOSS, a new digital survey of the northern sky, based on the POSS-II photographic sky atlas. The survey covers the entire sky north of delta = -3 deg in 3 bands, calibrated to the Gunn $gri$ system, reaching to equivalent limiting magnitude of B_lim ~ 22 mag. As a result of the state-of-the-art digitisation of the plates, detailed processing of the scans, and a very extensive CCD calibration program, the data quality exceedes that of the previous photographically-based efforts. The end product of the survey will be the Palomar-Norris Sky Catalog, anticipated to contain > 50 million galaxies and > 2 billion stars, down to the survey classification limit, ~ 1 mag above the flux detection limit. Numerous scientific projects utilising these data have been started, and we describe briefly some of them; they illustrate the scientific potential of the data, and serve as the scientific verification tests of the survey. Finally, we discuss some general issues posed by the advent of multi-terabyte data sets in astronomy.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 8 citations worldwide. Full citation record

  1. The ASAS-SN Low Surface Brightness Survey I: Proof-of-Concept and Potential Applications

    astro-ph.IM 2025-06 conditional novelty 6.0 of 10

    Stacked ASAS-SN images reach a median 3-sigma surface brightness limit of 26.1 mag per square arcsecond off the Galactic plane and recover 82 percent of known ultra-diffuse galaxies in the DES footprint.

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