Automated SpectroPhotometric Image REDuction (ASPIRED)
arXiv:2111.02127 · doi:10.3847/1538-3881/acd75c
Abstract
We provide a suite of public open-source spectral data-reduction software to rapidly obtain scientific products from all forms of long-slit-like spectroscopic observations. Automated SpectroPhotometric REDuction (ASPIRED) is a Python-based spectral data-reduction toolkit. It is designed to be a general toolkit with high flexibility for users to refine and optimize their data-reduction routines for the individual characteristics of their instruments. The default configuration is suitable for low-resolution long-slit spectrometers and provides a quick-look quality output. However, for repeatable science-ready reduced spectral data, some moderate one-time effort is necessary to modify the configuration. Fine-tuning and additional (pre)processing may be required to extend the reduction to systems with more complex setups. It is important to emphasize that although only a few parameters need updating, ensuring their correctness and suitability for generalization to the instrument can take time due to factors such as instrument stability. We compare some example spectra reduced with ASPIRED to published data processed with iraf-based and STARLINK-based pipelines, and find no loss in the quality of the final product. The Python-based, iraf-free ASPIRED can significantly ease the effort of an astronomer in constructing their own data-reduction workflow, enabling simpler solutions to data-reduction automation. This availability of near-real-time science-ready data will allow adaptive observing strategies, particularly important in, but not limited to, time-domain astronomy.
23 pages, 10 figures, 1 table, 1 appendix
References in corpus (12)
- Array Programming with NumPy
- Molecfit: A general tool for telluric absorption correction. I. Method and application to ESO instruments
- Molecfit: A general tool for telluric absorption correction II. Quantitative evaluation on ESO-VLT X-Shooter spectra
- The Rapid Reddening and Featureless Optical Spectra of the optical counterpart of GW170817, AT 2017gfo, During the First Four Days
- Energetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star
- Flux calibration of medium-resolution spectra from 300 nm to 2500 nm: Model reference spectra and telluric correction
- SpectRes: A Fast Spectral Resampling Tool in Python
- Skycorr: A general tool for spectroscopic sky subtraction
- Spectroscopic and Photometric Periods of Six Ultracompact Accreting Binaries
- Eclipsing White Dwarf Binaries in Gaia and the Zwicky Transient Facility
- Identifying Blue Large Amplitude Pulsators from Gaia DR2 & ZTF DR3
- Two New Nova Shells associated with V4362 Sagittarii and DO Aquilae
Cited by in corpus (6)
- AT 2021loi: A Bowen Fluorescence Flare with a Rebrightening Episode, Occurring in a Previously-Known AGN
- Cyclotron emitting magnetic white dwarfs in post common envelope binaries discovered with the Zwicky Transient Facility
- An upper limit on the frequency of short-period black hole companions to Sun-like stars
- A low mass, binary-stripped envelope for the Type IIb SN 2024abfo
- An update on the development of ASPIRED
- SPAN: A cross-platform Python GUI software for optical and near-infrared spectral analysis