Search for High-redshift Blazars with Fermi/LAT

Kreter M, Gokus A, Krauss F, Kadler M, Ojha R, Buson S, Wilms J, Bottcher M (2020)


Publication Type: Journal article

Publication year: 2020

Journal

Book Volume: 903

Article Number: 128

Journal Issue: 2

DOI: 10.3847/1538-4357/abb8da

Abstract

High-z blazars (z 2.5) are the most powerful class of persistent γ-ray sources in the universe. These objects possess the highest jet powers and luminosities and have black hole masses often in excess of 109 solar masses. In addition, high-z blazars are important cosmological probes and serve as test objects for blazar evolution models. Due to their large distance, their high-energy emission typically peaks below the GeV range, which makes them difficult to study with Fermi/Large Area Telescope (LAT). Therefore, only the very brightest objects are detectable and, to date, only a small number of high-z blazars have been detected with Fermi/LAT. In this work, we studied the monthly binned long-term γ-ray emission of a sample of 176 radio and optically detected blazars that have not been reported as known γ-ray sources in the 3FGL catalog. To account for false-positive detections, we calculated monthly Fermi/LAT light curves for a large sample of blank sky positions and derived the number of random fluctuations that we expect at various test statistic (TS) levels. For a given blazar, a detection of TS > 9 in at least one month is expected ∼15% of the time. Although this rate is too high to secure detection of an individual source, half of our sample shows such single-month γ-ray activity, indicating a population of high-energy blazars at distances of up to z = 5.2. Multiple TS > 9 monthly detections are unlikely to happen by chance, and we have detected several individual new sources in this way, including the most distant γ-ray blazar, BZQ J1430+4204 (z = 4.72). Finally, two new γ-ray blazars at redshifts of z = 3.63 and z = 3.11 are unambiguously detected via very significant (TS > 25) flares in individual monthly time bins.

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How to cite

APA:

Kreter, M., Gokus, A., Krauss, F., Kadler, M., Ojha, R., Buson, S.,... Bottcher, M. (2020). Search for High-redshift Blazars with Fermi/LAT. Astrophysical Journal, 903(2). https://dx.doi.org/10.3847/1538-4357/abb8da

MLA:

Kreter, M., et al. "Search for High-redshift Blazars with Fermi/LAT." Astrophysical Journal 903.2 (2020).

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