Journal article · Preprint article
A New Compton-thick AGN in Our Cosmic Backyard: Unveiling the Buried Nucleus in NGC 1448 with NuSTAR
Durham University1
Astrophysics and Atmospheric Physics, National Space Institute, Technical University of Denmark2
Virginia Polytechnic Institute and State University3
Princeton University4
Columbia University5
Swiss Federal Institute of Technology Zurich6
NASA Goddard Space Flight Center7
Harvard University8
University of Southampton9
European Southern Observatory10
Georgia Institute of Technology11
Pontificia Universidad Católica de Chile12
University of California at Berkeley13
Pennsylvania State University14
California Institute of Technology15
National Space Institute, Technical University of Denmark16
...and 6 moreNGC 1448 is one of the nearest luminous galaxies (L 8-1000μm >109 L o) to ours (z = 0.00390), and yet the active galactic nucleus (AGN) it hosts was only recently discovered, in 2009. In this paper, we present an analysis of the nuclear source across three wavebands: mid-infrared (MIR) continuum, optical, and X-rays.
We observed the source with the Nuclear Spectroscopic Telescope Array (NuSTAR), and combined these data with archival Chandra data to perform broadband X-ray spectral fitting (≈0.5-40 keV) of the AGN for the first time. Our X-ray spectral analysis reveals that the AGN is buried under a Compton-thick (CT) column of obscuring gas along our line of sight, with a column density of N H(los) ≥2.5 ×1024 cm-2.
The best-fitting torus models measured an intrinsic 2-10 keV luminosity of L (3.5-7.6) ×1040 erg s-1, making NGC 1448 one of the lowest luminosity CTAGNs known. In addition to the NuSTAR observation, we also performed optical spectroscopy for the nucleus in this edge-on galaxy using the European Southern Observatory New Technology Telescope.
We re-classify the optical nuclear spectrum as a Seyfert on the basis of the Baldwin-Philips-Terlevich diagnostic diagrams, thus identifying the AGN at optical wavelengths for the first time. We also present high spatial resolution MIR observations of NGC 1448 with Gemini/T-ReCS, in which a compact nucleus is clearly detected.
The absorption-corrected 2-10 keV luminosity measured from our X-ray spectral analysis agrees with that predicted from the optical [O iii]λ5007 Å emission line and the MIR 12 μm continuum, further supporting the CT nature of the AGN.
Language: | English |
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Publisher: | American Astronomical Society |
Year: | 2017 |
Pages: | 165 |
ISSN: | 15384357 , 0004637x , 15384365 and 00670049 |
Types: | Journal article and Preprint article |
DOI: | 10.3847/1538-4357/836/2/165 |
ORCIDs: | Christensen, Finn Erland , 0000-0003-0387-1429 , 0000-0002-5896-6313 , 0000-0003-3105-2615 , 0000-0002-5328-9827 , 0000-0003-0220-2063 , 0000-0001-8128-6976 , 0000-0002-8686-8737 , 0000-0002-0167-2453 , 0000-0001-6854-7545 , 0000-0003-2992-8024 , 0000-0002-7998-9581 , 0000-0002-5907-3330 , 0000-0001-5231-2645 , 0000-0002-0001-3587 and 0000-0003-2686-9241 |