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Published November 20, 2017 | Published
Journal Article Open

Search for Optical Pulsation in M82 X-2

Abstract

We report on a search for optical pulsation from M82 X-2 over a range of periods. M82 X-2 is an X-ray pulsar with a 1.37s average spin period and a 2.5 day sinusoidal modulation. The observations were done with the ARray Camera for Optical to Near-IR Spectrophotometry at the 200 inch Hale telescope at the Palomar Observatory. We performed H test and χ^2 statistical analysis. No significant optical pulsations were found in the wavelength range of 3000–11000 Å with a pulsation period between 1.36262 and 1.37462 s. We found an upper limit on pulsed emission in the 4000–8000 Å wavelength range to be fainter than ~20.5 mag_(AB) , corresponding to ~23 μJy.

Additional Information

© 2017 The American Astronomical Society. Received 2017 July 25; revised 2017 October 10; accepted 2017 October 13; published 2017 November 17. This material is based upon work supported by the National Science Foundation under grant No. AST-1411613. Observations were made using the Palomar 200 inch Hale Telescope of the Caltech Optical Observatories. We are pleased to acknowledge the Palomar Observatory staff for their enthusiastic and excellent support.

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