Enhancing the H2O Megamaser Detection Rate Using Optical and Mid-infrared Photometry

C. Y. Kuo, A. Constantin, J. A. Braatz, H. H. Chung, C. A. Witherspoon, D. Pesce, C. M.V. Impellizzeri, F. Gao, Lei Hao, J. H. Woo, Ingyin Zaw

Research output: Contribution to journalArticle

Abstract

Water megamasers from circumnuclear disks in galaxy centers provide the most accurate measurements of supermassive black hole masses and uniquely probe the subparsec accretion processes. At the same time, these systems offer independent crucial constraints of the Hubble constant in the nearby universe, and thus, the arguably best single constraint on the nature of dark energy. The chances of finding these golden standards are, however, abysmally low, at ≲3% overall for any level of water maser emission detected at 22 GHz and ≲1% for those exhibiting disk-like configuration. We provide here a thorough summary of the current state of detection of water megamaser disks along with a novel investigation of the likelihood of increasing their detection rates based on a multivariate parameter analysis of the optical and mid-infrared (mid-IR) photometric properties of the largest database of galaxies surveyed for 22 GHz emission. We find that galaxies with water megamaser emission tend to be associated with strong emission in all Wide-field Infrared Survey Explorer mid-IR wavelengths, with the strongest enhancement in the W4 band, at 22 μm, as well as with previously proposed and newly found indicators of active galactic nucleus strength in the mid-IR, such as red W1 -W2 and W1 -W4 colors, and the integrated mid-IR luminosity of the host galaxy. These trends offer a potential boost of the megamaser detection rates to 6%-15%, or a factor of 2-8 relative to the current rates, depending on the chosen sample selection criteria, while fostering real chances for discovering 20 new megamaser disks.

Original languageEnglish (US)
Article number169
JournalAstrophysical Journal
Volume860
Issue number2
DOIs
StatePublished - Jun 20 2018

Fingerprint

infrared photometry
galaxies
water
Wide-field Infrared Survey Explorer
water masers
Hubble constant
acceleration (physics)
dark energy
active galactic nuclei
universe
accretion
luminosity
probe
wavelength
trends
color
rate
detection
augmentation
probes

Keywords

  • galaxies: active
  • galaxies: nuclei
  • infrared: galaxies
  • masers
  • surveys

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Kuo, C. Y., Constantin, A., Braatz, J. A., Chung, H. H., Witherspoon, C. A., Pesce, D., ... Zaw, I. (2018). Enhancing the H2O Megamaser Detection Rate Using Optical and Mid-infrared Photometry. Astrophysical Journal, 860(2), [169]. https://doi.org/10.3847/1538-4357/aac498

Enhancing the H2O Megamaser Detection Rate Using Optical and Mid-infrared Photometry. / Kuo, C. Y.; Constantin, A.; Braatz, J. A.; Chung, H. H.; Witherspoon, C. A.; Pesce, D.; Impellizzeri, C. M.V.; Gao, F.; Hao, Lei; Woo, J. H.; Zaw, Ingyin.

In: Astrophysical Journal, Vol. 860, No. 2, 169, 20.06.2018.

Research output: Contribution to journalArticle

Kuo, CY, Constantin, A, Braatz, JA, Chung, HH, Witherspoon, CA, Pesce, D, Impellizzeri, CMV, Gao, F, Hao, L, Woo, JH & Zaw, I 2018, 'Enhancing the H2O Megamaser Detection Rate Using Optical and Mid-infrared Photometry', Astrophysical Journal, vol. 860, no. 2, 169. https://doi.org/10.3847/1538-4357/aac498
Kuo CY, Constantin A, Braatz JA, Chung HH, Witherspoon CA, Pesce D et al. Enhancing the H2O Megamaser Detection Rate Using Optical and Mid-infrared Photometry. Astrophysical Journal. 2018 Jun 20;860(2). 169. https://doi.org/10.3847/1538-4357/aac498
Kuo, C. Y. ; Constantin, A. ; Braatz, J. A. ; Chung, H. H. ; Witherspoon, C. A. ; Pesce, D. ; Impellizzeri, C. M.V. ; Gao, F. ; Hao, Lei ; Woo, J. H. ; Zaw, Ingyin. / Enhancing the H2O Megamaser Detection Rate Using Optical and Mid-infrared Photometry. In: Astrophysical Journal. 2018 ; Vol. 860, No. 2.
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