A Six-year Image-subtraction Light Curve of SN 2010jl
Abstract
SN 2010jl was a luminous Type IIn supernova (SN), detected in radio, optical, X-ray and hard X-rays. Here we report on its six-year R- and g-band light curves obtained using the Palomar Transient Factory. The light curve was generated using a pipeline based on the proper image-subtraction method and we discuss the algorithm performances. As noted before, the R-band light curve, up to about 300 days after maximum light is well described by a power-law decline with a power-law index of α ≈ -0.5. Between day 300 and day 2300 after maximum light, it is consistent with a power-law decline, with a power-law index of about α ≈ -3.4. Here, the longevity of the light curve suggests that the massive circumstellar material around the progenitor was ejected on timescales of at least tens of years prior to the progenitor explosion.
- Authors:
-
- Weizmann Inst. of Science, Rehovot (Israel)
- Inst. for Advanced Study, Princeton, NJ (United States)
- Stockholm Univ., Stockholm (Sweden)
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1564026
- Grant/Contract Number:
- AC02-05CH11231
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Publications of the Astronomical Society of the Pacific
- Additional Journal Information:
- Journal Volume: 131; Journal Issue: 999; Journal ID: ISSN 0004-6280
- Publisher:
- Astronomical Society of the Pacific (ASP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Ofek, E. O., Zackay, B., Gal-Yam, A., Sollerman, J., Fransson, C., Fremling, C., Kulkarni, S. R., Nugent, P. E., Yaron, O., Kasliwal, M. M., Masci, F., and Laher, R. A Six-year Image-subtraction Light Curve of SN 2010jl. United States: N. p., 2019.
Web. doi:10.1088/1538-3873/ab0a19.
Ofek, E. O., Zackay, B., Gal-Yam, A., Sollerman, J., Fransson, C., Fremling, C., Kulkarni, S. R., Nugent, P. E., Yaron, O., Kasliwal, M. M., Masci, F., & Laher, R. A Six-year Image-subtraction Light Curve of SN 2010jl. United States. https://doi.org/10.1088/1538-3873/ab0a19
Ofek, E. O., Zackay, B., Gal-Yam, A., Sollerman, J., Fransson, C., Fremling, C., Kulkarni, S. R., Nugent, P. E., Yaron, O., Kasliwal, M. M., Masci, F., and Laher, R. Fri .
"A Six-year Image-subtraction Light Curve of SN 2010jl". United States. https://doi.org/10.1088/1538-3873/ab0a19. https://www.osti.gov/servlets/purl/1564026.
@article{osti_1564026,
title = {A Six-year Image-subtraction Light Curve of SN 2010jl},
author = {Ofek, E. O. and Zackay, B. and Gal-Yam, A. and Sollerman, J. and Fransson, C. and Fremling, C. and Kulkarni, S. R. and Nugent, P. E. and Yaron, O. and Kasliwal, M. M. and Masci, F. and Laher, R.},
abstractNote = {SN 2010jl was a luminous Type IIn supernova (SN), detected in radio, optical, X-ray and hard X-rays. Here we report on its six-year R- and g-band light curves obtained using the Palomar Transient Factory. The light curve was generated using a pipeline based on the proper image-subtraction method and we discuss the algorithm performances. As noted before, the R-band light curve, up to about 300 days after maximum light is well described by a power-law decline with a power-law index of α ≈ -0.5. Between day 300 and day 2300 after maximum light, it is consistent with a power-law decline, with a power-law index of about α ≈ -3.4. Here, the longevity of the light curve suggests that the massive circumstellar material around the progenitor was ejected on timescales of at least tens of years prior to the progenitor explosion.},
doi = {10.1088/1538-3873/ab0a19},
journal = {Publications of the Astronomical Society of the Pacific},
number = 999,
volume = 131,
place = {United States},
year = {Fri Apr 12 00:00:00 EDT 2019},
month = {Fri Apr 12 00:00:00 EDT 2019}
}
Web of Science
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