BASS. XXXIV. A Catalog of the Nuclear Millimeter-wave Continuum Emission Properties of AGNs Constrained on Scales ≤ 100–200 pc

Taiki Kawamuro; Claudio Ricci; Richard F. Mushotzky; Masatoshi Imanishi; Franz E. Bauer; Federica Ricci; Michael J. Koss; George C. Privon; Benny Trakhtenbrot; Takuma Izumi; Kohei Ichikawa; Alejandra F. Rojas; Krista Lynne Smith; Taro Shimizu; Kyuseok Oh; Jakob S. den Brok; Shunsuke Baba; Mislav Baloković; Chin Shin Chang; Darshan Kakkad; Ryan W. Pfeifle; Matthew J. Temple; Yoshihiro Ueda; Fiona Harrison; Meredith C. Powell; Daniel Stern; Meg Urry; David B. Sanders

doi:https://doi.org/10.3847/1538-4365/acf467

BASS. XXXIV. A Catalog of the Nuclear Millimeter-wave Continuum Emission Properties of AGNs Constrained on Scales ≤ 100–200 pc

Taiki Kawamuro, Claudio Ricci, Richard F. Mushotzky, Masatoshi Imanishi, Franz E. Bauer, Federica Ricci, Michael J. Koss, George C. Privon, Benny Trakhtenbrot, Takuma Izumi, Kohei Ichikawa, Alejandra F. Rojas, Krista Lynne Smith, Taro Shimizu, Kyuseok Oh, Jakob S. den Brok, Shunsuke Baba, Mislav Baloković, Chin Shin Chang, Darshan KakkadRyan W. Pfeifle, Matthew J. Temple, Yoshihiro Ueda, Fiona Harrison, Meredith C. Powell, Daniel Stern, Meg Urry, David B. Sanders

School of Physics and Astronomy

Tel Aviv University

Research output: Contribution to journal › Article › peer-review

Abstract

We present a catalog of the millimeter-wave (mm-wave) continuum properties of 98 nearby (z < 0.05) active galactic nuclei (AGNs) selected from the 70 month Swift/BAT hard-X-ray catalog that have precisely determined X-ray spectral properties and subarcsecond-resolution Atacama Large Millimeter/submillimeter Array Band 6 (211–275 GHz) observations as of 2021 April. Due to the hard-X-ray (>10 keV) selection, the sample is nearly unbiased for obscured systems at least up to Compton-thick-level obscuration, and provides the largest number of AGNs with high-physical-resolution mm-wave data (<100–200 pc). Our catalog reports emission peak coordinates, spectral indices, and peak fluxes and luminosities at 1.3 mm (230 GHz). Additionally, high-resolution mm-wave images are provided. Using the images and creating radial surface brightness profiles of mm-wave emission, we identify emission extending from the central sources and isolated blob-like emission. Flags indicating the presence of these emission features are tabulated. Among 90 AGNs with significant detections of nuclear emission, 37 AGNs (≈41%) appear to have both or one of extended or blob-like components. We, in particular, investigate AGNs that show well-resolved mm-wave components and find that these seem to have a variety of origins (i.e., a jet, radio lobes, a secondary AGN, stellar clusters, a narrow-line region, galaxy disk, active star formation regions, or AGN-driven outflows), and some components have currently unclear origins.

Original language	English
Article number	acf467
Journal	Astrophysical Journal, Supplement Series
Volume	269
Issue number	1
DOIs	https://doi.org/10.3847/1538-4365/acf467
State	Published - 1 Nov 2023

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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https://doi.org/10.3847/1538-4365/acf467

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Kawamuro, T., Ricci, C., Mushotzky, R. F., Imanishi, M., Bauer, F. E., Ricci, F., Koss, M. J., Privon, G. C., Trakhtenbrot, B., Izumi, T., Ichikawa, K., Rojas, A. F., Smith, K. L., Shimizu, T., Oh, K., den Brok, J. S., Baba, S., Baloković, M., Chang, C. S., ... Sanders, D. B. (2023). BASS. XXXIV. A Catalog of the Nuclear Millimeter-wave Continuum Emission Properties of AGNs Constrained on Scales ≤ 100–200 pc. Astrophysical Journal, Supplement Series, 269(1), Article acf467. https://doi.org/10.3847/1538-4365/acf467

@article{70d419b1762b44ad866f4db5af5b7566,

title = "BASS. XXXIV. A Catalog of the Nuclear Millimeter-wave Continuum Emission Properties of AGNs Constrained on Scales ≤ 100–200 pc",

abstract = "We present a catalog of the millimeter-wave (mm-wave) continuum properties of 98 nearby (z < 0.05) active galactic nuclei (AGNs) selected from the 70 month Swift/BAT hard-X-ray catalog that have precisely determined X-ray spectral properties and subarcsecond-resolution Atacama Large Millimeter/submillimeter Array Band 6 (211–275 GHz) observations as of 2021 April. Due to the hard-X-ray (>10 keV) selection, the sample is nearly unbiased for obscured systems at least up to Compton-thick-level obscuration, and provides the largest number of AGNs with high-physical-resolution mm-wave data (<100–200 pc). Our catalog reports emission peak coordinates, spectral indices, and peak fluxes and luminosities at 1.3 mm (230 GHz). Additionally, high-resolution mm-wave images are provided. Using the images and creating radial surface brightness profiles of mm-wave emission, we identify emission extending from the central sources and isolated blob-like emission. Flags indicating the presence of these emission features are tabulated. Among 90 AGNs with significant detections of nuclear emission, 37 AGNs (≈41%) appear to have both or one of extended or blob-like components. We, in particular, investigate AGNs that show well-resolved mm-wave components and find that these seem to have a variety of origins (i.e., a jet, radio lobes, a secondary AGN, stellar clusters, a narrow-line region, galaxy disk, active star formation regions, or AGN-driven outflows), and some components have currently unclear origins.",

author = "Taiki Kawamuro and Claudio Ricci and Mushotzky, {Richard F.} and Masatoshi Imanishi and Bauer, {Franz E.} and Federica Ricci and Koss, {Michael J.} and Privon, {George C.} and Benny Trakhtenbrot and Takuma Izumi and Kohei Ichikawa and Rojas, {Alejandra F.} and Smith, {Krista Lynne} and Taro Shimizu and Kyuseok Oh and {den Brok}, {Jakob S.} and Shunsuke Baba and Mislav Balokovi{\'c} and Chang, {Chin Shin} and Darshan Kakkad and Pfeifle, {Ryan W.} and Temple, {Matthew J.} and Yoshihiro Ueda and Fiona Harrison and Powell, {Meredith C.} and Daniel Stern and Meg Urry and Sanders, {David B.}",

year = "2023",

month = nov,

day = "1",

doi = "https://doi.org/10.3847/1538-4365/acf467",

language = "الإنجليزيّة",

volume = "269",

journal = "Astrophysical Journal, Supplement Series",

issn = "0067-0049",

publisher = "IOP Publishing Ltd.",

number = "1",

}

Kawamuro, T, Ricci, C, Mushotzky, RF, Imanishi, M, Bauer, FE, Ricci, F, Koss, MJ, Privon, GC, Trakhtenbrot, B, Izumi, T, Ichikawa, K, Rojas, AF, Smith, KL, Shimizu, T, Oh, K, den Brok, JS, Baba, S, Baloković, M, Chang, CS, Kakkad, D, Pfeifle, RW, Temple, MJ, Ueda, Y, Harrison, F, Powell, MC, Stern, D, Urry, M & Sanders, DB 2023, 'BASS. XXXIV. A Catalog of the Nuclear Millimeter-wave Continuum Emission Properties of AGNs Constrained on Scales ≤ 100–200 pc', Astrophysical Journal, Supplement Series, vol. 269, no. 1, acf467. https://doi.org/10.3847/1538-4365/acf467

TY - JOUR

T1 - BASS. XXXIV. A Catalog of the Nuclear Millimeter-wave Continuum Emission Properties of AGNs Constrained on Scales ≤ 100–200 pc

AU - Kawamuro, Taiki

AU - Ricci, Claudio

AU - Mushotzky, Richard F.

AU - Imanishi, Masatoshi

AU - Bauer, Franz E.

AU - Ricci, Federica

AU - Koss, Michael J.

AU - Privon, George C.

AU - Trakhtenbrot, Benny

AU - Izumi, Takuma

AU - Ichikawa, Kohei

AU - Rojas, Alejandra F.

AU - Smith, Krista Lynne

AU - Shimizu, Taro

AU - Oh, Kyuseok

AU - den Brok, Jakob S.

AU - Baba, Shunsuke

AU - Baloković, Mislav

AU - Chang, Chin Shin

AU - Kakkad, Darshan

AU - Pfeifle, Ryan W.

AU - Temple, Matthew J.

AU - Ueda, Yoshihiro

AU - Harrison, Fiona

AU - Powell, Meredith C.

AU - Stern, Daniel

AU - Urry, Meg

AU - Sanders, David B.

PY - 2023/11/1

Y1 - 2023/11/1

N2 - We present a catalog of the millimeter-wave (mm-wave) continuum properties of 98 nearby (z < 0.05) active galactic nuclei (AGNs) selected from the 70 month Swift/BAT hard-X-ray catalog that have precisely determined X-ray spectral properties and subarcsecond-resolution Atacama Large Millimeter/submillimeter Array Band 6 (211–275 GHz) observations as of 2021 April. Due to the hard-X-ray (>10 keV) selection, the sample is nearly unbiased for obscured systems at least up to Compton-thick-level obscuration, and provides the largest number of AGNs with high-physical-resolution mm-wave data (<100–200 pc). Our catalog reports emission peak coordinates, spectral indices, and peak fluxes and luminosities at 1.3 mm (230 GHz). Additionally, high-resolution mm-wave images are provided. Using the images and creating radial surface brightness profiles of mm-wave emission, we identify emission extending from the central sources and isolated blob-like emission. Flags indicating the presence of these emission features are tabulated. Among 90 AGNs with significant detections of nuclear emission, 37 AGNs (≈41%) appear to have both or one of extended or blob-like components. We, in particular, investigate AGNs that show well-resolved mm-wave components and find that these seem to have a variety of origins (i.e., a jet, radio lobes, a secondary AGN, stellar clusters, a narrow-line region, galaxy disk, active star formation regions, or AGN-driven outflows), and some components have currently unclear origins.

AB - We present a catalog of the millimeter-wave (mm-wave) continuum properties of 98 nearby (z < 0.05) active galactic nuclei (AGNs) selected from the 70 month Swift/BAT hard-X-ray catalog that have precisely determined X-ray spectral properties and subarcsecond-resolution Atacama Large Millimeter/submillimeter Array Band 6 (211–275 GHz) observations as of 2021 April. Due to the hard-X-ray (>10 keV) selection, the sample is nearly unbiased for obscured systems at least up to Compton-thick-level obscuration, and provides the largest number of AGNs with high-physical-resolution mm-wave data (<100–200 pc). Our catalog reports emission peak coordinates, spectral indices, and peak fluxes and luminosities at 1.3 mm (230 GHz). Additionally, high-resolution mm-wave images are provided. Using the images and creating radial surface brightness profiles of mm-wave emission, we identify emission extending from the central sources and isolated blob-like emission. Flags indicating the presence of these emission features are tabulated. Among 90 AGNs with significant detections of nuclear emission, 37 AGNs (≈41%) appear to have both or one of extended or blob-like components. We, in particular, investigate AGNs that show well-resolved mm-wave components and find that these seem to have a variety of origins (i.e., a jet, radio lobes, a secondary AGN, stellar clusters, a narrow-line region, galaxy disk, active star formation regions, or AGN-driven outflows), and some components have currently unclear origins.

UR - http://www.scopus.com/inward/record.url?scp=85180449785&partnerID=8YFLogxK

U2 - https://doi.org/10.3847/1538-4365/acf467

DO - https://doi.org/10.3847/1538-4365/acf467

M3 - مقالة

SN - 0067-0049

VL - 269

JO - Astrophysical Journal, Supplement Series

JF - Astrophysical Journal, Supplement Series

IS - 1

M1 - acf467

ER -

BASS. XXXIV. A Catalog of the Nuclear Millimeter-wave Continuum Emission Properties of AGNs Constrained on Scales ≤ 100–200 pc

Abstract

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