Discovery of a GeV blazar shining through the galactic plane
Abstract
The Fermi Large Area Telescope (LAT) discovered a new gamma-ray source near the Galactic plane, Fermi J0109+6134, when it flared brightly in 2010 February. The low Galactic latitude (b = –1$$ο\atop{.}$$2) indicated that the source could be located within the Galaxy, which motivated rapid multi-wavelength follow-up including radio, optical, and X-ray observations. Here, we report the results of analyzing all 19 months of LAT data for the source, and of X-ray observations with both Swift and the Chandra X-ray Observatory. We determined the source redshift, z = 0.783, using a Keck Low-Resolution Imaging Spectrometer observation. Finally, we compiled a broadband spectral energy distribution (SED) from both historical and new observations contemporaneous with the 2010 February flare. The redshift, SED, optical line width, X-ray absorption, and multi-band variability indicate that this new GeV source is a blazar seen through the Galactic plane. Because several of the optical emission lines have equivalent width >5 Å, this blazar belongs in the flat-spectrum radio quasar category.
- Authors:
- more »
- Publication Date:
- Research Org.:
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- Contributing Org.:
- The Fermi LAT Collaboration
- OSTI Identifier:
- 1357541
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal. Letters
- Additional Journal Information:
- Journal Volume: 718; Journal Issue: 2; Journal ID: ISSN 2041-8205
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; galaxies active
Citation Formats
Vandenbroucke, J., Buehler, R., Ajello, M., Bechtol, K., Bellini, A., Bolte, M., Cheung, C. C., Civano, F., Donato, D., Fuhrmann, L., Funk, S., Healey, S. E., Hill, A. B., Knigge, C., Madejski, G. M., Romani, R. W., Santander-García, M., Shaw, M. S., Steeghs, D., Torres, M. A. P., Van Etten, A., and Williams, K. A. Discovery of a GeV blazar shining through the galactic plane. United States: N. p., 2010.
Web. doi:10.1088/2041-8205/718/2/L166.
Vandenbroucke, J., Buehler, R., Ajello, M., Bechtol, K., Bellini, A., Bolte, M., Cheung, C. C., Civano, F., Donato, D., Fuhrmann, L., Funk, S., Healey, S. E., Hill, A. B., Knigge, C., Madejski, G. M., Romani, R. W., Santander-García, M., Shaw, M. S., Steeghs, D., Torres, M. A. P., Van Etten, A., & Williams, K. A. Discovery of a GeV blazar shining through the galactic plane. United States. https://doi.org/10.1088/2041-8205/718/2/L166
Vandenbroucke, J., Buehler, R., Ajello, M., Bechtol, K., Bellini, A., Bolte, M., Cheung, C. C., Civano, F., Donato, D., Fuhrmann, L., Funk, S., Healey, S. E., Hill, A. B., Knigge, C., Madejski, G. M., Romani, R. W., Santander-García, M., Shaw, M. S., Steeghs, D., Torres, M. A. P., Van Etten, A., and Williams, K. A. Wed .
"Discovery of a GeV blazar shining through the galactic plane". United States. https://doi.org/10.1088/2041-8205/718/2/L166. https://www.osti.gov/servlets/purl/1357541.
@article{osti_1357541,
title = {Discovery of a GeV blazar shining through the galactic plane},
author = {Vandenbroucke, J. and Buehler, R. and Ajello, M. and Bechtol, K. and Bellini, A. and Bolte, M. and Cheung, C. C. and Civano, F. and Donato, D. and Fuhrmann, L. and Funk, S. and Healey, S. E. and Hill, A. B. and Knigge, C. and Madejski, G. M. and Romani, R. W. and Santander-García, M. and Shaw, M. S. and Steeghs, D. and Torres, M. A. P. and Van Etten, A. and Williams, K. A.},
abstractNote = {The Fermi Large Area Telescope (LAT) discovered a new gamma-ray source near the Galactic plane, Fermi J0109+6134, when it flared brightly in 2010 February. The low Galactic latitude (b = –1$ο\atop{.}$2) indicated that the source could be located within the Galaxy, which motivated rapid multi-wavelength follow-up including radio, optical, and X-ray observations. Here, we report the results of analyzing all 19 months of LAT data for the source, and of X-ray observations with both Swift and the Chandra X-ray Observatory. We determined the source redshift, z = 0.783, using a Keck Low-Resolution Imaging Spectrometer observation. Finally, we compiled a broadband spectral energy distribution (SED) from both historical and new observations contemporaneous with the 2010 February flare. The redshift, SED, optical line width, X-ray absorption, and multi-band variability indicate that this new GeV source is a blazar seen through the Galactic plane. Because several of the optical emission lines have equivalent width >5 Å, this blazar belongs in the flat-spectrum radio quasar category.},
doi = {10.1088/2041-8205/718/2/L166},
journal = {The Astrophysical Journal. Letters},
number = 2,
volume = 718,
place = {United States},
year = {Wed Jul 14 00:00:00 EDT 2010},
month = {Wed Jul 14 00:00:00 EDT 2010}
}
Web of Science
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