Published July 12, 2024 | Version 1.0
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ULTRACAM observations of PSR J1622-0315

  • 1. School of Physics, University Collge Cork, Cork, Ireland
  • 2. Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, United Kingdom
  • 3. Department of Physics, Norwegian University of Science and Technology, NO-7491 Trondheim, Norway
  • 4. Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, UK
  • 5. Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
  • 6. Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
  • 7. Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
  • 8. Leibniz Universität Hannover, D-30167 Hannover, Germany

Description

Optical observations of PSR J1622-0315 taken by the high-speed triple-beam CCD camera ULTRACAM on the New Technology Telescope. As presented in Sen et al. 2024 (ApJ, in press). The first letter  in each file name represents the observing filter for that specific file. The raw data for creating the light curves can be requested by contacting Rene Breton or Vik Dhillon.

The columns in each file are:
1) MJD time
2) orbital phase (in rotations, with phase = 0 corresponding to pulsar's ascending node),
3) flux density (in erg cm^-2 s^-1 Hz^-1)
4) flux density uncertainty (in erg cm^-2 s^-1 Hz^-1)

Files

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md5:9e174c4d0be49721b82e0083153c134b
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md5:b2b2cd2d1e0bd65629dbfa63c89d0e59
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Additional details

Related works

Is published in
Publication: arXiv:2407.10800 (arXiv)

Funding

European Commission
Spiders - Fundamental Physics Using Black Widow, Redback and Transitional Pulsar Binaries 715051
European Commission
LOVE-NEST - Looking for Super-Massive Neutron Stars 101002352
UK Research and Innovation
A consolidated grant for Sheffield Astrophysics 2021-2024 ST/V000853/1