DOOp, an automated wrapper for DAOSPEC

作者：Cantat Gaudin Tristan^*; Donati Paolo; Pancino Elena; Bragaglia Angela; Vallenari Antonella; Friel Eileen D; Sordo Rosanna; Jacobson Heather R; Magrini Laura

来源：Astronomy & Astrophysics, 2014, 562: A10.

DOI：10.1051/0004-6361/201322533

• techniques: spectroscopic

Context. Large spectroscopic surveys such as the Gaia-ESO Survey produce huge quantities of data. Automatic tools are necessary to efficiently handle this material. The measurement of equivalent widths in stellar spectra is traditionally done by hand or with semiautomatic procedures that are time-consuming and not very robust with respect to the repeatability of the results.
Aims. The program DAOSPEC is a tool that provides consistent measurements of equivalent widths in stellar spectra while requiring a minimum of user intervention. However, it is not optimised to deal with large batches of spectra, as some parameters still need to be modified and checked by the user. Exploiting the versatility and portability of BASH, we have built a pipeline called DOOp (DAOSPEC Option Optimiser) automating the procedure of equivalent widths measurement with DAOSPEC.
Methods. DOOp is organised in different modules that run one after the other to perform specific tasks, taking care of the optimisation of the parameters needed to provide the final equivalent widths, and providing log tiles to ensure better control over the procedure.
Results. In this paper, making use of synthetic and observed spectra, we compare the performance of DOOp with other methods, including DAOSPEC used manually. The measurements made by DOOp are identical to the ones produced by DAOSPEC when used manually, while requiring less user intervention, which is especially convenient when dealing with a large quantity of spectra. Like DAOSPEC, DOOp shows its best performance on high-resolution spectra (R > 20 000) and high signal-to-noise ratio (S/N > 30), with uncertainties ranging from 6 m angstrom to 2 m angstrom. Th e only subjective parameter that remains is the choice of the normalisation, as the user still has to make a choice on the order of the polynomial used for the continuum fitting. As a test, we use the equivalent widths measured by DOOp to re-derive the stellar parameters of four well-studied stars.

• 出版日期2014-2
• 单位MIT