General catalogue of variable stars: Version GCVS 5.1
By N. Samus, E. Kazarovets, O. V. Durlevich, N. Kireeva, E. N. Pastukhova. 2017
310 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Computational Mechanics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/da148f9108cc56a7bf449c563d7c8c949fb62d78
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Citations in the corpus
- The ASAS-SN catalogue of variable stars I: The Serendipitous Survey (2018, methodology): “SRS variables are short period semi-regular variables with P < 30 d, while semiregular SR variables have P > 30 d. Mira variables (VSX type ‘M’) in our sample frequently dip below our detection limits (V & 17), hence their ASASSN amplitudes can be less than the minimum V-band amplitude of A = 2.5 ma”