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The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151. / Yuan, W.; Fausnaugh, M. M.; Hoffmann, S. L.; Macri, L. M.; Peterson, B. M.; Riess, A. G.; Bentz, M. C.; Brown, J. S.; Dalla Bonta, E.; Davies, R.; De Rosa, G.; Ferrarese, L.; Grier, C. J.; Hicks, E. K. S.; Onken, C. A.; Pogge, R. W.; Storchi-Bergmann, T.; Vestergaard, M.
In:
Astrophysical Journal, Vol. 902, No. 1, 26, 10.2020.
Research output: Contribution to journal › Journal article › Research › peer-review
Harvard
Yuan, W, Fausnaugh, MM, Hoffmann, SL, Macri, LM, Peterson, BM, Riess, AG, Bentz, MC, Brown, JS, Dalla Bonta, E, Davies, R, De Rosa, G, Ferrarese, L, Grier, CJ, Hicks, EKS, Onken, CA, Pogge, RW, Storchi-Bergmann, T
& Vestergaard, M 2020, '
The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151',
Astrophysical Journal, vol. 902, no. 1, 26.
https://doi.org/10.3847/1538-4357/abb377APA
Yuan, W., Fausnaugh, M. M., Hoffmann, S. L., Macri, L. M., Peterson, B. M., Riess, A. G., Bentz, M. C., Brown, J. S., Dalla Bonta, E., Davies, R., De Rosa, G., Ferrarese, L., Grier, C. J., Hicks, E. K. S., Onken, C. A., Pogge, R. W., Storchi-Bergmann, T.
, & Vestergaard, M. (2020).
The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151.
Astrophysical Journal,
902(1), [26].
https://doi.org/10.3847/1538-4357/abb377Vancouver
Yuan W, Fausnaugh MM, Hoffmann SL, Macri LM, Peterson BM, Riess AG et al.
The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151.
Astrophysical Journal. 2020 Oct;902(1). 26.
https://doi.org/10.3847/1538-4357/abb377Author
Yuan, W. ; Fausnaugh, M. M. ; Hoffmann, S. L. ; Macri, L. M. ; Peterson, B. M. ; Riess, A. G. ; Bentz, M. C. ; Brown, J. S. ; Dalla Bonta, E. ; Davies, R. ; De Rosa, G. ; Ferrarese, L. ; Grier, C. J. ; Hicks, E. K. S. ; Onken, C. A. ; Pogge, R. W. ; Storchi-Bergmann, T. ; Vestergaard, M. / The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151. In: Astrophysical Journal. 2020 ; Vol. 902, No. 1.
Bibtex
@article{74c359bcb3d44d45a36cbc3d67d1252f,
title = "The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151",
abstract = "We derive a distance of 15.8 0.4 Mpc to the archetypal Seyfert 1 galaxy NGC 4151 based on the near-infrared Cepheid period-luminosity relation and new Hubble Space Telescope multiband imaging. This distance determination, based on measurements of 35 long-period (P> 25 days) Cepheids, will support the absolute calibration of the supermassive black hole mass in this system, as well as studies of the dynamics of the feedback or feeding of its active galactic nucleus.",
keywords = "Cepheid variable stars, Distance measure, Cepheid distance, AGN host galaxies, Hubble Space Telescope, HST photometry, Time series analysis, Near infrared astronomy, Optical observatories, Distance indicators, Galaxy distances, SUPERMASSIVE BLACK-HOLES, ACTIVE GALACTIC NUCLEI, NARROW-LINE REGION, GRAVITATIONAL LENSING EXPERIMENT., REVERBERATION MAPPING DATA, OGLE-III CATALOG, GEMINI NIFS, KINEMATICS, MASS, MAGNITUDES",
author = "W. Yuan and Fausnaugh, {M. M.} and Hoffmann, {S. L.} and Macri, {L. M.} and Peterson, {B. M.} and Riess, {A. G.} and Bentz, {M. C.} and Brown, {J. S.} and {Dalla Bonta}, E. and R. Davies and {De Rosa}, G. and L. Ferrarese and Grier, {C. J.} and Hicks, {E. K. S.} and Onken, {C. A.} and Pogge, {R. W.} and T. Storchi-Bergmann and M. Vestergaard",
year = "2020",
month = oct,
doi = "10.3847/1538-4357/abb377",
language = "English",
volume = "902",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "1",
}
RIS
TY - JOUR
T1 - The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151
AU - Yuan, W.
AU - Fausnaugh, M. M.
AU - Hoffmann, S. L.
AU - Macri, L. M.
AU - Peterson, B. M.
AU - Riess, A. G.
AU - Bentz, M. C.
AU - Brown, J. S.
AU - Dalla Bonta, E.
AU - Davies, R.
AU - De Rosa, G.
AU - Ferrarese, L.
AU - Grier, C. J.
AU - Hicks, E. K. S.
AU - Onken, C. A.
AU - Pogge, R. W.
AU - Storchi-Bergmann, T.
AU - Vestergaard, M.
PY - 2020/10
Y1 - 2020/10
N2 - We derive a distance of 15.8 0.4 Mpc to the archetypal Seyfert 1 galaxy NGC 4151 based on the near-infrared Cepheid period-luminosity relation and new Hubble Space Telescope multiband imaging. This distance determination, based on measurements of 35 long-period (P> 25 days) Cepheids, will support the absolute calibration of the supermassive black hole mass in this system, as well as studies of the dynamics of the feedback or feeding of its active galactic nucleus.
AB - We derive a distance of 15.8 0.4 Mpc to the archetypal Seyfert 1 galaxy NGC 4151 based on the near-infrared Cepheid period-luminosity relation and new Hubble Space Telescope multiband imaging. This distance determination, based on measurements of 35 long-period (P> 25 days) Cepheids, will support the absolute calibration of the supermassive black hole mass in this system, as well as studies of the dynamics of the feedback or feeding of its active galactic nucleus.
KW - Cepheid variable stars
KW - Distance measure
KW - Cepheid distance
KW - AGN host galaxies
KW - Hubble Space Telescope
KW - HST photometry
KW - Time series analysis
KW - Near infrared astronomy
KW - Optical observatories
KW - Distance indicators
KW - Galaxy distances
KW - SUPERMASSIVE BLACK-HOLES
KW - ACTIVE GALACTIC NUCLEI
KW - NARROW-LINE REGION
KW - GRAVITATIONAL LENSING EXPERIMENT.
KW - REVERBERATION MAPPING DATA
KW - OGLE-III CATALOG
KW - GEMINI NIFS
KW - KINEMATICS
KW - MASS
KW - MAGNITUDES
U2 - 10.3847/1538-4357/abb377
DO - 10.3847/1538-4357/abb377
M3 - Journal article
VL - 902
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 1
M1 - 26
ER -
