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Title: 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:
 [1];  [2];  [1];  [1];  [1];  [3];  [1];  [4];  [5];  [6];  [1]
  1. Univ. of California, Santa Barbara, CA (United States)
  2. ASTRON, the Netherlands Institute for Radio Astronomy, Dwingeloo (The Netherlands)
  3. California Institute of Technology, Pasadena, CA (United States)
  4. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  5. NASA Jet Propulsion Lab., Pasadena, CA (United States)
  6. 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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Works referencing / citing this record:

Optical pulsations from a transitional millisecond pulsar
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Pulsating in Unison at Optical and X-Ray Energies: Simultaneous High Time Resolution Observations of the Transitional Millisecond Pulsar PSR J1023+0038
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Optical pulsations from a transitional millisecond pulsar
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Design and Performance of Hafnium Optical and Near-IR Kinetic Inductance Detectors
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Optical and Near-IR Microwave Kinetic Inductance Detectors (MKIDs) in the 2020s
preprint, January 2019