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NOTE: Most of the High Level Science Products are unavailable while unscheduled maintenance is being performed. They will be incrementally restored over the course of this week. We apologize for any inconvenience.

HUT Fully-Calibrated, First-Order Spectra of White Dwarfs G191-B2B and HZ 43

During the Astro-1 mission, an aluminum filter was used to block first-order light, and two white dwarfs (G191-B2B and HZ 43) were observed in second order. The flux from these second-order observations were then subtracted from the first-order spectra of these two objects. This was the only time that such second-order corrections were applied to HUT spectra, because no second-order observations were obtained during Astro-2 due to the SiC coating used on the HUT optics during that mission.

Because these spectra are in a different format compared to the rest of the HUT data products on MAST, we provide them here as a High Level Science Product. The files are simple, two-column text files, where Column 1 is the wavelength in Angstroms, and Column 2 is the flux in units of erg/cm^2/s/Angstrom. These spectra are originally described in Kruk et al. 1997, ApJ, 482, 546, Sections 2.2 and 5 (Figs. 2 and 8), respectively.

Note that the extracted spectra and quick-look plots for the second-order spectra of these two white dwarfs (Data IDs HUT109702 and HUT105203) in the HUT database are in units of counts per second, rather than the nominal erg/cm^2/s/Angstrom. Furthermore, no inverse sensitivity curve is available for these second-order spectra, and the inverse sensitivity curves in their IDF FITS headers should not be used.

Star Name
Link To Spectrum
(.txt file)
G191-B2B Download
HZ 43 Download