SED Machine Spectra for HO Puppis and V722 Tauri
نویسندگان
چکیده
We present low-resolution spectra collected with the Spectral Energy Distribution Machine (SEDM) for an IW And-type dwarf nova, HO Puppis, and a Be star, V722 Tauri. The SEDM is integrated field unit spectrograph mounted on 60 inch telescope at Palomar Observatory, spectral resolution of R ∼ 100 in optical wavelength range. Hα emission line was clearly detected bright star Tauri ∼12.5 mag, but barely ∼13.7 mag Puppis. Our observations could be used as guidance observing similar objects SEDM, well other spectrographs, future.
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ژورنال
عنوان ژورنال: Research notes of the AAS
سال: 2021
ISSN: ['2515-5172']
DOI: https://doi.org/10.3847/2515-5172/abf503