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Trigonometrical Parallaxes of LB 3303 and LB 3459
1971Radcliffe spectra [1] of this star in 1961 confirmed Luyten’s suspicion on the basis of colour and proper motion that this object is a bright white dwarf. The profile of Hγ was found to be closely similar to that of o2 Eri B. Hill and Hill [2] have published photometry yielding V=11.40.
J. Churms, A. D. Thackeray
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DLP: Achieve Customizable Location Privacy With Deceptive Dummy Techniques in LBS Applications
IEEE Internet of Things Journal, 2022Jiezhen Tang, Hui Zhu, Rongxing Lu
exaly
LBS Meets Blockchain: An Efficient Method With Security Preserving Trust in SAGIN
IEEE Internet of Things Journal, 2022Bohan Li, Han Gao, Ken Cai
exaly