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SDSS-IV MaNGA: identification of active galactic nuclei in optical integral field unit surveys

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SDSS-IV MaNGA : identification of active galactic nuclei in optical integral field unit surveys. / Wylezalek, Dominika; Zakamska, Nadia L.; Greene, Jenny E.; Riffel, Rogemar A.; Drory, Niv; Andrews, Brett H.; Merloni, Andrea; Thomas, Daniel.

In: Monthly Notices of the Royal Astronomical Society, Vol. 474, No. 2, 02.2018, p. 1499–1514.

Research output: Contribution to journalArticle

Harvard

Wylezalek, D, Zakamska, NL, Greene, JE, Riffel, RA, Drory, N, Andrews, BH, Merloni, A & Thomas, D 2018, 'SDSS-IV MaNGA: identification of active galactic nuclei in optical integral field unit surveys', Monthly Notices of the Royal Astronomical Society, vol. 474, no. 2, pp. 1499–1514. https://doi.org/10.1093/mnras/stx2784

APA

Wylezalek, D., Zakamska, N. L., Greene, J. E., Riffel, R. A., Drory, N., Andrews, B. H., ... Thomas, D. (2018). SDSS-IV MaNGA: identification of active galactic nuclei in optical integral field unit surveys. Monthly Notices of the Royal Astronomical Society, 474(2), 1499–1514. https://doi.org/10.1093/mnras/stx2784

Vancouver

Wylezalek D, Zakamska NL, Greene JE, Riffel RA, Drory N, Andrews BH et al. SDSS-IV MaNGA: identification of active galactic nuclei in optical integral field unit surveys. Monthly Notices of the Royal Astronomical Society. 2018 Feb;474(2):1499–1514. https://doi.org/10.1093/mnras/stx2784

Author

Wylezalek, Dominika ; Zakamska, Nadia L. ; Greene, Jenny E. ; Riffel, Rogemar A. ; Drory, Niv ; Andrews, Brett H. ; Merloni, Andrea ; Thomas, Daniel. / SDSS-IV MaNGA : identification of active galactic nuclei in optical integral field unit surveys. In: Monthly Notices of the Royal Astronomical Society. 2018 ; Vol. 474, No. 2. pp. 1499–1514.

Bibtex

@article{da292e9714574f34a8066b1dd47bb3e8,
title = "SDSS-IV MaNGA: identification of active galactic nuclei in optical integral field unit surveys",
abstract = "In this paper, we investigate 2727 galaxies observed by MaNGA as of June 2016 to develop spatially resolved techniques for identifying signatures of active galactic nuclei (AGN). We identify 303 AGN candidates. The additional spatial dimension imposes challenges in identifying AGN due to contamination from diffuse ionized gas, extra-planar gas and photoionization by hot stars. We show that the combination of spatially-resolved line diagnostic diagrams and additional cuts on H$\alpha$ surface brighness and H$\alpha$ equivalent width can distinguish between AGN-like signatures and high-metallicity galaxies with LINER-like spectra. Low mass galaxies with high specific star formation rates are particularly difficult to diagnose and routinely show diagnostic line ratios outside of the standard star-formation locus. We develop a new diagnostic -- the distance from the standard diagnostic line in the line-ratios space -- to evaluate the significance of the deviation from the star-formation locus. We find 173 galaxies that would not have been selected as AGN candidates based on single-fibre spectral measurements but exhibit photoionization signatures suggestive of AGN activity in the MaNGA resolved observations, underscoring the power of large integral field unit (IFU) surveys. A complete census of these new AGN candidates is necessary to understand their nature and probe the complex co-evolution of supermassive black holes and their hosts.",
keywords = "astro-ph.GA, astro-ph.CO",
author = "Dominika Wylezalek and Zakamska, {Nadia L.} and Greene, {Jenny E.} and Riffel, {Rogemar A.} and Niv Drory and Andrews, {Brett H.} and Andrea Merloni and Daniel Thomas",
note = "18 pages, 11 figures, accepted to MNRAS",
year = "2018",
month = "2",
doi = "10.1093/mnras/stx2784",
language = "English",
volume = "474",
pages = "1499–1514",
journal = "MNRAS",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "2",

}

RIS

TY - JOUR

T1 - SDSS-IV MaNGA

T2 - identification of active galactic nuclei in optical integral field unit surveys

AU - Wylezalek, Dominika

AU - Zakamska, Nadia L.

AU - Greene, Jenny E.

AU - Riffel, Rogemar A.

AU - Drory, Niv

AU - Andrews, Brett H.

AU - Merloni, Andrea

AU - Thomas, Daniel

N1 - 18 pages, 11 figures, accepted to MNRAS

PY - 2018/2

Y1 - 2018/2

N2 - In this paper, we investigate 2727 galaxies observed by MaNGA as of June 2016 to develop spatially resolved techniques for identifying signatures of active galactic nuclei (AGN). We identify 303 AGN candidates. The additional spatial dimension imposes challenges in identifying AGN due to contamination from diffuse ionized gas, extra-planar gas and photoionization by hot stars. We show that the combination of spatially-resolved line diagnostic diagrams and additional cuts on H$\alpha$ surface brighness and H$\alpha$ equivalent width can distinguish between AGN-like signatures and high-metallicity galaxies with LINER-like spectra. Low mass galaxies with high specific star formation rates are particularly difficult to diagnose and routinely show diagnostic line ratios outside of the standard star-formation locus. We develop a new diagnostic -- the distance from the standard diagnostic line in the line-ratios space -- to evaluate the significance of the deviation from the star-formation locus. We find 173 galaxies that would not have been selected as AGN candidates based on single-fibre spectral measurements but exhibit photoionization signatures suggestive of AGN activity in the MaNGA resolved observations, underscoring the power of large integral field unit (IFU) surveys. A complete census of these new AGN candidates is necessary to understand their nature and probe the complex co-evolution of supermassive black holes and their hosts.

AB - In this paper, we investigate 2727 galaxies observed by MaNGA as of June 2016 to develop spatially resolved techniques for identifying signatures of active galactic nuclei (AGN). We identify 303 AGN candidates. The additional spatial dimension imposes challenges in identifying AGN due to contamination from diffuse ionized gas, extra-planar gas and photoionization by hot stars. We show that the combination of spatially-resolved line diagnostic diagrams and additional cuts on H$\alpha$ surface brighness and H$\alpha$ equivalent width can distinguish between AGN-like signatures and high-metallicity galaxies with LINER-like spectra. Low mass galaxies with high specific star formation rates are particularly difficult to diagnose and routinely show diagnostic line ratios outside of the standard star-formation locus. We develop a new diagnostic -- the distance from the standard diagnostic line in the line-ratios space -- to evaluate the significance of the deviation from the star-formation locus. We find 173 galaxies that would not have been selected as AGN candidates based on single-fibre spectral measurements but exhibit photoionization signatures suggestive of AGN activity in the MaNGA resolved observations, underscoring the power of large integral field unit (IFU) surveys. A complete census of these new AGN candidates is necessary to understand their nature and probe the complex co-evolution of supermassive black holes and their hosts.

KW - astro-ph.GA

KW - astro-ph.CO

U2 - 10.1093/mnras/stx2784

DO - 10.1093/mnras/stx2784

M3 - Article

VL - 474

SP - 1499

EP - 1514

JO - MNRAS

JF - MNRAS

SN - 0035-8711

IS - 2

ER -

ID: 8557414