MARZ: Manual and Automatic Redshifting Software
arXiv:1603.09438 · doi:10.1016/j.ascom.2016.03.001
Abstract
The Australian Dark Energy Survey (OzDES) is a 100-night spectroscopic survey underway on the Anglo-Australian Telescope using the fibre-fed 2-degree-field (2dF) spectrograph. We have developed a new redshifting application Marz with greater usability, flexibility, and the capacity to analyse a wider range of object types than the Runz software package previously used for redshifting spectra from 2dF. Marz is an open-source, client-based, Javascript web-application which provides an intuitive interface and powerful automatic matching capabilities on spectra generated from the AAOmega spectrograph to produce high quality spectroscopic redshift measurements. The software can be run interactively or via the command line, and is easily adaptable to other instruments and pipelines if conforming to the current FITS file standard is not possible. Behind the scenes, a modified version of the Autoz cross-correlation algorithm is used to match input spectra against a variety of stellar and galaxy templates, and automatic matching performance for OzDES spectra has increased from 54% (Runz) to 91% (Marz). Spectra not matched correctly by the automatic algorithm can be easily redshifted manually by cycling automatic results, manual template comparison, or marking spectral features.
arXiv comment15 pages, 12 figures
References in corpus (16)
- The 2dF Galaxy Redshift Survey: Spectra and redshifts
- The Sixth Data Release of the Sloan Digital Sky Survey
- The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III
- The Multi-Object, Fiber-Fed Spectrographs for SDSS and the Baryon Oscillation Spectroscopic Survey
- The DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts
- Spectral Classification and Redshift Measurement for the SDSS-III Baryon Oscillation Spectroscopic Survey
- The 6dF Galaxy Survey: Samples, Observational Techniques and the First Data Release
- The WiggleZ Dark Energy Survey: Survey Design and First Data Release
- RVSAO 2.0: Digital Redshifts and Radial Velocities
- The Anglo-Australian Observatory's 2dF Facility
- The Gemini Deep Deep Survey: I. Introduction to the Survey, Catalogs and Composite Spectra
- Galaxy And Mass Assembly (GAMA): Spectroscopic analysis
- Galaxy And Mass Assembly (GAMA): autoz spectral redshift measurements, confidence and errors
- EZ: A Tool for Automatic Redshift Measurement
- OzDES multi-fibre spectroscopy for the Dark Energy Survey: first-year operation and results
- Automatic Redshift Determination by use of Principal Component Analysis --- I: Fundamentals
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