Search for optical pulsations in PSR J0337+1715
Abstract
In this study, 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 (ARCONS) at the 200" Hale telescope at Palomar Observatory. No significant pulsations were found in the range 4000-11000 angstroms, and we can limit pulsed emission in g-band to be fainter than 25 mag.
- Authors:
-
- Univ. of California, Santa Barbara, CA (United States)
- ASTRON, the Netherlands Institute for Radio Astronomy, Dwingeloo (The Netherlands)
- California Institute of Technology, Pasadena, CA (United States)
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- NASA Jet Propulsion Lab., Pasadena, CA (United States)
- Univ. of Wisconsin, Milwaukee, WI (United States)
- Publication Date:
- Research Org.:
- Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1249203
- Report Number(s):
- arXiv:1603.05270; FERMILAB-PUB-16-116-AE
Journal ID: ISSN 0035-8711; 1429627
- Grant/Contract Number:
- AC02-07CH11359
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 459; Journal Issue: 1; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; stars: neutron; pulsars: general; pulsars: individual: PSR J0337+1715
Citation Formats
Strader, M. J., Archibald, A. M., Meeker, S. R., Szypryt, P., Walter, A. B., van Eyken, J. C., Ulbricht, G., Stoughton, C., Bumble, B., Kaplan, D. L., and Mazin, B. A. Search for optical pulsations in PSR J0337+1715. United States: N. p., 2016.
Web. doi:10.1093/mnras/stw663.
Strader, M. J., Archibald, A. M., Meeker, S. R., Szypryt, P., Walter, A. B., van Eyken, J. C., Ulbricht, G., Stoughton, C., Bumble, B., Kaplan, D. L., & Mazin, B. A. Search for optical pulsations in PSR J0337+1715. United States. https://doi.org/10.1093/mnras/stw663
Strader, M. J., Archibald, A. M., Meeker, S. R., Szypryt, P., Walter, A. B., van Eyken, J. C., Ulbricht, G., Stoughton, C., Bumble, B., Kaplan, D. L., and Mazin, B. A. Sun .
"Search for optical pulsations in PSR J0337+1715". United States. https://doi.org/10.1093/mnras/stw663. https://www.osti.gov/servlets/purl/1249203.
@article{osti_1249203,
title = {Search for optical pulsations in PSR J0337+1715},
author = {Strader, M. J. and Archibald, A. M. and Meeker, S. R. and Szypryt, P. and Walter, A. B. and van Eyken, J. C. and Ulbricht, G. and Stoughton, C. and Bumble, B. and Kaplan, D. L. and Mazin, B. A.},
abstractNote = {In this study, 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 (ARCONS) at the 200" Hale telescope at Palomar Observatory. No significant pulsations were found in the range 4000-11000 angstroms, and we can limit pulsed emission in g-band to be fainter than 25 mag.},
doi = {10.1093/mnras/stw663},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 459,
place = {United States},
year = {Sun Mar 20 00:00:00 EDT 2016},
month = {Sun Mar 20 00:00:00 EDT 2016}
}
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