Black-Body Stars
Abstract
We report the discovery of stars that show spectra very close to the black-body radiation. We found 17 such stars out of 798,593 stars in the Sloan Digital Sky Survey (SDSS) spectroscopic data archives. We discuss the value of these stars for the calibration of photometry, whatever is the physical nature of these stars. This gives us a chance to examine the accuracy of the zero point of SDSS photometry across various passbands: we conclude that the zero point of SDSS photometric system is internally consistent across its five passbands to the level below 0.01 mag. We may also examine the consistency of the zero-points between UV photometry of Galaxy Evolution Explorer and SDSS, and IR photometry of Wide-field Infrared Survey Explorer against SDSS. These stars can be used as not only photometric but spetrophotometric standard stars. We suggest that these stars showing the featureless black-body like spectrum of the effective temperature of K are consistent with DB white dwarfs with the temperature too low to develop helium absorption features.
Cite
@article{arxiv.1711.01122,
title = {Black-Body Stars},
author = {Nao Suzuki and Masataka Fukugita},
journal= {arXiv preprint arXiv:1711.01122},
year = {2018}
}
Comments
AJ submitted