A NEW POPULATION of Compton-THICK AGNs IDENTIFIED USING the SPECTRAL CURVATURE above 10 keV

Michael J. Koss, R. Assef, M. Baloković, D. Stern, P. Gandhi, I. Lamperti, D. M. Alexander, D. R. Ballantyne, F. E. Bauer, S. Berney, William Nielsen Brandt, A. Comastri, N. Gehrels, F. A. Harrison, G. Lansbury, C. Markwardt, C. Ricci, E. Rivers, K. Schawinski, B. Trakhtenbrot & 2 others E. Treister, C. Megan Urry

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Abstract

We present a new metric that uses the spectral curvature (SC) above 10 keV to identify Compton-thick active galactic nuclei (AGNs) in low-quality Swift/Burst Alert Telescope (BAT) X-ray data. Using NuSTAR, we observe nine high SC-selected AGNs. We find that high-sensitivity spectra show that the majority are Compton-thick (78% or 7/9) and the remaining two are nearly Compton-thick (N H ≃ (5-8) × 1023 cm-2). We find that the SCBAT and SCNuSTAR measurements are consistent, suggesting that this technique can be applied to future telescopes. We tested the SC method on well-known Compton-thick AGNs and found that it is much more effective than broadband ratios (e.g., 100% using SC versus 20% using 8-24 keV/3-8 keV). Our results suggest that using the >10 keV emission may be the only way to identify this population since only two sources show Compton-thick levels of excess in the Balmer decrement corrected [O iii] to observed X-ray emission ratio (F[O III]/Fobs2-10 keV > 1) and WISE colors do not identify most of them as AGNs. Based on this small sample, we find that a higher fraction of these AGNs are in the final merger stage (<10 kpc) than typical BAT AGNs. Additionally, these nine obscured AGNs have, on average, ≈4× higher accretion rates than other BAT-detected AGNs (〈λEDD〉) = 0.068 ± 0.023 compared to 〈λEDD〉 = 0.016 ± 0.004) . The robustness of SC at identifying Compton-thick AGNs implies that a higher fraction of nearby AGNs may be Compton-thick (≈22%) and the sum of black hole growth in Compton-thick AGNs (Eddington ratio times population percentage) is nearly as large as mildly obscured and unobscured AGNs.

Original languageEnglish (US)
Article number85
JournalAstrophysical Journal
Volume825
Issue number2
DOIs
StatePublished - Jul 10 2016

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active galactic nuclei
curvature
telescopes
bursts
merger
accretion
Wide-field Infrared Survey Explorer
x rays
broadband
color

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Koss, M. J., Assef, R., Baloković, M., Stern, D., Gandhi, P., Lamperti, I., ... Urry, C. M. (2016). A NEW POPULATION of Compton-THICK AGNs IDENTIFIED USING the SPECTRAL CURVATURE above 10 keV. Astrophysical Journal, 825(2), [85]. https://doi.org/10.3847/0004-637X/825/2/85
Koss, Michael J. ; Assef, R. ; Baloković, M. ; Stern, D. ; Gandhi, P. ; Lamperti, I. ; Alexander, D. M. ; Ballantyne, D. R. ; Bauer, F. E. ; Berney, S. ; Brandt, William Nielsen ; Comastri, A. ; Gehrels, N. ; Harrison, F. A. ; Lansbury, G. ; Markwardt, C. ; Ricci, C. ; Rivers, E. ; Schawinski, K. ; Trakhtenbrot, B. ; Treister, E. ; Urry, C. Megan. / A NEW POPULATION of Compton-THICK AGNs IDENTIFIED USING the SPECTRAL CURVATURE above 10 keV. In: Astrophysical Journal. 2016 ; Vol. 825, No. 2.
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abstract = "We present a new metric that uses the spectral curvature (SC) above 10 keV to identify Compton-thick active galactic nuclei (AGNs) in low-quality Swift/Burst Alert Telescope (BAT) X-ray data. Using NuSTAR, we observe nine high SC-selected AGNs. We find that high-sensitivity spectra show that the majority are Compton-thick (78{\%} or 7/9) and the remaining two are nearly Compton-thick (N H ≃ (5-8) × 1023 cm-2). We find that the SCBAT and SCNuSTAR measurements are consistent, suggesting that this technique can be applied to future telescopes. We tested the SC method on well-known Compton-thick AGNs and found that it is much more effective than broadband ratios (e.g., 100{\%} using SC versus 20{\%} using 8-24 keV/3-8 keV). Our results suggest that using the >10 keV emission may be the only way to identify this population since only two sources show Compton-thick levels of excess in the Balmer decrement corrected [O iii] to observed X-ray emission ratio (F[O III]/Fobs2-10 keV > 1) and WISE colors do not identify most of them as AGNs. Based on this small sample, we find that a higher fraction of these AGNs are in the final merger stage (<10 kpc) than typical BAT AGNs. Additionally, these nine obscured AGNs have, on average, ≈4× higher accretion rates than other BAT-detected AGNs (〈λEDD〉) = 0.068 ± 0.023 compared to 〈λEDD〉 = 0.016 ± 0.004) . The robustness of SC at identifying Compton-thick AGNs implies that a higher fraction of nearby AGNs may be Compton-thick (≈22{\%}) and the sum of black hole growth in Compton-thick AGNs (Eddington ratio times population percentage) is nearly as large as mildly obscured and unobscured AGNs.",
author = "Koss, {Michael J.} and R. Assef and M. Baloković and D. Stern and P. Gandhi and I. Lamperti and Alexander, {D. M.} and Ballantyne, {D. R.} and Bauer, {F. E.} and S. Berney and Brandt, {William Nielsen} and A. Comastri and N. Gehrels and Harrison, {F. A.} and G. Lansbury and C. Markwardt and C. Ricci and E. Rivers and K. Schawinski and B. Trakhtenbrot and E. Treister and Urry, {C. Megan}",
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Koss, MJ, Assef, R, Baloković, M, Stern, D, Gandhi, P, Lamperti, I, Alexander, DM, Ballantyne, DR, Bauer, FE, Berney, S, Brandt, WN, Comastri, A, Gehrels, N, Harrison, FA, Lansbury, G, Markwardt, C, Ricci, C, Rivers, E, Schawinski, K, Trakhtenbrot, B, Treister, E & Urry, CM 2016, 'A NEW POPULATION of Compton-THICK AGNs IDENTIFIED USING the SPECTRAL CURVATURE above 10 keV', Astrophysical Journal, vol. 825, no. 2, 85. https://doi.org/10.3847/0004-637X/825/2/85

A NEW POPULATION of Compton-THICK AGNs IDENTIFIED USING the SPECTRAL CURVATURE above 10 keV. / Koss, Michael J.; Assef, R.; Baloković, M.; Stern, D.; Gandhi, P.; Lamperti, I.; Alexander, D. M.; Ballantyne, D. R.; Bauer, F. E.; Berney, S.; Brandt, William Nielsen; Comastri, A.; Gehrels, N.; Harrison, F. A.; Lansbury, G.; Markwardt, C.; Ricci, C.; Rivers, E.; Schawinski, K.; Trakhtenbrot, B.; Treister, E.; Urry, C. Megan.

In: Astrophysical Journal, Vol. 825, No. 2, 85, 10.07.2016.

Research output: Contribution to journalArticle

TY - JOUR

T1 - A NEW POPULATION of Compton-THICK AGNs IDENTIFIED USING the SPECTRAL CURVATURE above 10 keV

AU - Koss, Michael J.

AU - Assef, R.

AU - Baloković, M.

AU - Stern, D.

AU - Gandhi, P.

AU - Lamperti, I.

AU - Alexander, D. M.

AU - Ballantyne, D. R.

AU - Bauer, F. E.

AU - Berney, S.

AU - Brandt, William Nielsen

AU - Comastri, A.

AU - Gehrels, N.

AU - Harrison, F. A.

AU - Lansbury, G.

AU - Markwardt, C.

AU - Ricci, C.

AU - Rivers, E.

AU - Schawinski, K.

AU - Trakhtenbrot, B.

AU - Treister, E.

AU - Urry, C. Megan

PY - 2016/7/10

Y1 - 2016/7/10

N2 - We present a new metric that uses the spectral curvature (SC) above 10 keV to identify Compton-thick active galactic nuclei (AGNs) in low-quality Swift/Burst Alert Telescope (BAT) X-ray data. Using NuSTAR, we observe nine high SC-selected AGNs. We find that high-sensitivity spectra show that the majority are Compton-thick (78% or 7/9) and the remaining two are nearly Compton-thick (N H ≃ (5-8) × 1023 cm-2). We find that the SCBAT and SCNuSTAR measurements are consistent, suggesting that this technique can be applied to future telescopes. We tested the SC method on well-known Compton-thick AGNs and found that it is much more effective than broadband ratios (e.g., 100% using SC versus 20% using 8-24 keV/3-8 keV). Our results suggest that using the >10 keV emission may be the only way to identify this population since only two sources show Compton-thick levels of excess in the Balmer decrement corrected [O iii] to observed X-ray emission ratio (F[O III]/Fobs2-10 keV > 1) and WISE colors do not identify most of them as AGNs. Based on this small sample, we find that a higher fraction of these AGNs are in the final merger stage (<10 kpc) than typical BAT AGNs. Additionally, these nine obscured AGNs have, on average, ≈4× higher accretion rates than other BAT-detected AGNs (〈λEDD〉) = 0.068 ± 0.023 compared to 〈λEDD〉 = 0.016 ± 0.004) . The robustness of SC at identifying Compton-thick AGNs implies that a higher fraction of nearby AGNs may be Compton-thick (≈22%) and the sum of black hole growth in Compton-thick AGNs (Eddington ratio times population percentage) is nearly as large as mildly obscured and unobscured AGNs.

AB - We present a new metric that uses the spectral curvature (SC) above 10 keV to identify Compton-thick active galactic nuclei (AGNs) in low-quality Swift/Burst Alert Telescope (BAT) X-ray data. Using NuSTAR, we observe nine high SC-selected AGNs. We find that high-sensitivity spectra show that the majority are Compton-thick (78% or 7/9) and the remaining two are nearly Compton-thick (N H ≃ (5-8) × 1023 cm-2). We find that the SCBAT and SCNuSTAR measurements are consistent, suggesting that this technique can be applied to future telescopes. We tested the SC method on well-known Compton-thick AGNs and found that it is much more effective than broadband ratios (e.g., 100% using SC versus 20% using 8-24 keV/3-8 keV). Our results suggest that using the >10 keV emission may be the only way to identify this population since only two sources show Compton-thick levels of excess in the Balmer decrement corrected [O iii] to observed X-ray emission ratio (F[O III]/Fobs2-10 keV > 1) and WISE colors do not identify most of them as AGNs. Based on this small sample, we find that a higher fraction of these AGNs are in the final merger stage (<10 kpc) than typical BAT AGNs. Additionally, these nine obscured AGNs have, on average, ≈4× higher accretion rates than other BAT-detected AGNs (〈λEDD〉) = 0.068 ± 0.023 compared to 〈λEDD〉 = 0.016 ± 0.004) . The robustness of SC at identifying Compton-thick AGNs implies that a higher fraction of nearby AGNs may be Compton-thick (≈22%) and the sum of black hole growth in Compton-thick AGNs (Eddington ratio times population percentage) is nearly as large as mildly obscured and unobscured AGNs.

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