2023AJ....166...13L


Query : 2023AJ....166...13L

2023AJ....166...13L - Astron. J., 166, 13 (2023/July-0)

Automated SpectroPhotometric Image REDuction (ASPIRED).

LAM M.C., SMITH R.J., ARCAVI I., STEELE I.A., VEITCH-MICHAELIS J. and WYRZYKOWSKI L.

Abstract (from CDS):

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.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Astronomy data reduction - Spectroscopy - Open source software - Publicly available software - Astronomy software - Observational astronomy - Astronomical techniques - Astronomical methods

Simbad objects: 11

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Number of rows : 11
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 Hilt 102 * 01 09 05.0413038576 +62 47 30.268502016 10.88 11.10 10.42     B0III 53 0
2 SN 2016bse SN* 09 20 34.30 +50 41 46.8           SNIIP 134 0
3 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
4 V* V418 Ser CV* 15 14 53.6404088280 +02 09 34.575570360           ~ 22 0
5 BD+33 2642 pA* 15 51 59.8854348048 +32 56 54.329485272 9.806 10.61 10.73 10.884 10.961 O7p 456 0
6 OGLE BLAP-009 dS* 17 58 48.2085416832 -27 16 53.707773360     15.650   15.071 ~ 23 0
7 PSO J180.1536+62.5419 WD* 18 01 53.6701240900 +62 54 14.808287189           DC 5 0
8 CD-44 12736 PM* 18 36 25.9502475648 -44 18 36.907592904   10.83 10.22     G0 222 0
9 ZTF J192014.13+272218.1 EB* 19 20 14.1164858496 +27 22 18.287327784           ~ 4 0
10 V* DO Aql No* 19 31 25.8807151348 -06 25 38.739918640           ~ 66 0
11 Feige 110 HS* 23 19 58.3996844256 -05 09 56.171142864 10.360 11.45 11.50 11.970 12.145 sdO8VIIIHe5 673 1

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