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Documentation

Find information, examples, FAQs and extensive descriptions of the data, curated by the survey teams.

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OzDES

Since 2013, OzDES has used the Anglo-Australian Telescope to classify hundreds of transients, monitor active galactic nuclei, and obtain redshifts for tens of thousands of galaxies within the 10 deep fields of the Dark Energy Survey.
April 1, 2020 by C. Lidman
June 19, 2020, 4:59 a.m. C. Lidman

FAQ

Frequently Asked Questions

Q. Which keywords define the wavelength scale?

A. Wavelength is defined using standard FITS keywords, such as CRPIX1, CRVAL1, CDELT1, CTYPE1 and CUNIT1. All spectra have been placed on the heliocentric reference frame.

Q. What is rmag

A. rmag is the r band AB magnitude in a 2" aperture. See the DES data release pages for details?

Q. Are the OzDES spectra flux calibrated?

A. The spectra are not flux calibrated, not even in a relative sense. This is due to fibre positioning errors, chormatic aberrations from the 2dF corrector, and seeing. We are investigating ways to calibrate the spectra using broad band photometry. The flux units are normalised counts per unit wavelength.

Q. Why do some objects with qop=1 or 2 have a redshift.

A. The redshift of these objects comes from the transient and not the host galaxy. For these cases, the redshift flag refers to the confidence in the redshift.

April 1, 2020 by C. Lidman
June 19, 2020, 4:59 a.m. C. Lidman