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CALSPEC-Calibrated IUE White Dwarfs ("IUE-FLUXCAL")Bohlin & Bianchi 2018, AJ, accepted
Introduction
Fig. 7 from Bohlin & Bianchi (2018) showing discrepant regions of the star GRW+70 5824. Inserts show ratio of IUE to CALSPEC/STIS in 20 Å (SWP) and 40 Å (LWP) bins, respectively.
IUE-FLUXCAL is a collection spectral energy distributions (SEDs) for six white dwarfs in the HST CALSPEC database that are also observed by IUE. Composite IUE SEDs of each white dwarf are constructed by co-adding available low-resolution NEWSIPS spectra. The published paper compares the IUE to CALSPEC in 20 Å bins for SWP and 40 Å bins for LWP or LWR. A global average of these binned ratios across all six white dwarfs define corrections to the IUE NEWSIPS flux scale. This HLSP provides the co-added IUE SEDs of the six white dwarfs, as well as the table of IUE-to-CALSPEC flux ratios required to calibrate IUE data onto the HST standard scale.
Description of Data ProductsEach of the six white dwarfs have SEDs available in both TXT and FITS format. The available columns in the SED files are:
In addition to the SEDs, two tables are provided that have the IUE-to-CALSPEC flux ratios in different wavelength bins. IUE NEWSIPS spectra should be multiplied by the average corrections in these tables to place them on the HST/CALSPEC scale. The two text tables contain the correction ratios for SWP and LWP/LWR, respectively, and can be interpolated to define the IUE correction at intermediate wavelengths.
Data Access
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