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• W2301682095 abstract "We report on a search for optical pulsations from PSR J0337+1715 at its observed radio pulse period. PSR J0337+1715 is a millisecond pulsar (2.7 ms spin period) in a triple hierarchical system with two white dwarfs, and has a known optical counterpart with g-band magnitude 18. The observations were done with the ARray Camera for Optical to Near-IR Spectrophotometry at the 200 arcsec Hale telescope at Palomar Observatory. No significant pulsations were found in the range 4000–11 000 Å, and we can limit pulsed emission in g band to be fainter than 25 mag." @default.
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• W2301682095 date "2016-03-20" @default.
• W2301682095 modified "2023-10-01" @default.
• W2301682095 title "Search for optical pulsations in PSR J0337+1715" @default.
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• W2301682095 doi "https://doi.org/10.1093/mnras/stw663" @default.
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