SEDBYS: A python-based SED Builder for Young Stars

Abstract

Spectral energy distributions (SEDs) are useful primary and complementary tools in the analysis of observations of young stars. However, the process of collating, inspecting, and flux-converting archival photometry and spectroscopy to build spectral energy distributions for young stars can be time-consuming. Here, I present SEDBYS (Spectral Energy Distribution Builder for Young Stars), a python-based repository of command-line tools built to (i) query online photometric and spectroscopic catalogs and a distributed database of archival photometry, (ii) use a look-up table of zero points to flux-convert the acquired data, (iii) enable visual inspection of the SED and (iv) handle book-keeping to collate references in bibTeX format. The code is distributed via git and is equipped with additional tools to enable users to add existing or forthcoming catalogs to the list of sources queried, ensuring the longevity of SEDBYS as a tool for the star formation community.

Accepted for publication in Software X (Received 29 October 2020, Accepted 11 March 2021, Available online 3 April 2021.)

References in corpus (22)

• astroquery: An Astronomical Web-Querying Package in Python
• A Spitzer Survey of Young Stellar Clusters within One Kiloparsec of the Sun: Cluster Core Extraction and Basic Structural Analysis
• VOSA: Virtual Observatory SED Analyzer. An application to the Collinder 69 open cluster
• A Steeper than Linear Disk Mass-Stellar Mass Scaling Relation
• The SCUBA Legacy Catalogue: Continuum Objects Detected by SCUBA
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• A Millimeter Continuum Size-Luminosity Relationship for Protoplanetary Disks
• The Disk Population of the Chamaeleon I Star-Forming Region
• Structure of Herbig AeBe disks at the milliarcsecond scale A statistical survey in the H band using PIONIER-VLTI
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• A modular set of synthetic spectral energy distributions for young stellar objects
• Circumstellar disks around Herbig Be stars
• Proplyds and Massive Disks in the Orion Nebula Cluster Imaged with CARMA and SMA
• Silica in Protoplanetary Disks
• ALMA survey of Class II protoplanetary disks in Corona Australis: a young region with low disk masses
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• An evolved disk surrounding the massive main sequence star MWC 297?
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Cited by in corpus (5)

• The Mass Accretion Rate and Stellar Properties in Class I Protostars
• Imaging the inner astronomical unit of Herbig Be star HD 190073
• The Ages of Optically Bright Sub-Clusters in the Serpens Star-Forming Region
• Spectral energy distribution of late stage stars
• Scattering and sublimation: a multi-scale view of $\mu$m-sized dust in the inclined disc of HD 145718