First results from the lick AGN monitoring project: The mass of the black hole in ARP 151

Misty C. Bentz; Jonelle L. Walsh; Aaron J. Barth; Nairn Baliber; Nicola Bennert; Gabriela Canalizo; Alexei V. Filippenko; Mohan Ganeshalingam; Elinor L. Gates; Jenny E. Greene; Marton G. Hidas; Kyle D. Hiner; Nicholas Lee; Weidong Li; Matthew A. Malkan; Takeo Minezaki; Frank J.D. Serduke; Joshua H. Shiode; Jeffrey M. Silverman; Thea N. Steele; Daniel Stern; Rachel A. Street; Carol E. Thornton; Tommaso Treu; Xiaofeng Wang; Jong Hak Woo; Yuzuru Yoshiill

doi:10.1086/595719

First results from the lick AGN monitoring project: The mass of the black hole in ARP 151

Misty C. Bentz
, Jonelle L. Walsh
, Aaron J. Barth
, Nairn Baliber
, Nicola Bennert
, Gabriela Canalizo
, Alexei V. Filippenko
, Mohan Ganeshalingam
, Elinor L. Gates
, Jenny E. Greene
, Marton G. Hidas
, Kyle D. Hiner
, Nicholas Lee
, Weidong Li
, Matthew A. Malkan
, Takeo Minezaki
, Frank J.D. Serduke
, Joshua H. Shiode
, Jeffrey M. Silverman
, Thea N. Steele

Daniel Stern, Rachel A. Street, Carol E. Thornton, Tommaso Treu, Xiaofeng Wang, Jong Hak Woo, Yuzuru Yoshiill

Astrophysical Sciences

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

76 Scopus citations

Abstract

We have recently completed a 64 night spectroscopic monitoring campaign at the Lick Observatory 3 m Shane telescope with the aim of measuring the masses of the black holes in 13 nearby (z<0.05) Seyfert 1 galaxies with expected masses in the range-10⁶-10⁷ M⊙. We present here the first results from this project-the mass of the central black hole in Arp 151. Strong variability throughout the campaign led to an exceptionally clean Hβ lag measurement in this object of 4.25^+0.68_-0.66 days in the observed frame. Coupled with the width of the Hβ emission line in the variable spectrum, we determine a black hole mass of (7.1 ± 1.2) × 10⁶ M⊙, assuming the Onken et al. normalization for reverberation-based virial masses. We also find velocity-resolved lag information within the Hβ emission line which clearly shows infalling gas in the Hβ-emitting region. Further detailed analysis may lead to a full model of the geometry and kinematics of broad line region gas around the central black hole in Arp 151.

Original language	English (US)
Pages (from-to)	L21-L24
Journal	Astrophysical Journal
Volume	689
Issue number	1 PART 2
DOIs	https://doi.org/10.1086/595719
State	Published - 2008

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Galaxies: Individual (Arp 151)
Galaxies: Nuclei
Galaxies: Seyfert
Galaxies: active

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10.1086/595719

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Bentz, M. C., Walsh, J. L., Barth, A. J., Baliber, N., Bennert, N., Canalizo, G., Filippenko, A. V., Ganeshalingam, M., Gates, E. L., Greene, J. E., Hidas, M. G., Hiner, K. D., Lee, N., Li, W., Malkan, M. A., Minezaki, T., Serduke, F. J. D., Shiode, J. H., Silverman, J. M., ... Yoshiill, Y. (2008). First results from the lick AGN monitoring project: The mass of the black hole in ARP 151. Astrophysical Journal, 689(1 PART 2), L21-L24. https://doi.org/10.1086/595719

@article{f4623f4f29614d9eaa5aa5b8507384c1,

title = "First results from the lick AGN monitoring project: The mass of the black hole in ARP 151",

abstract = "We have recently completed a 64 night spectroscopic monitoring campaign at the Lick Observatory 3 m Shane telescope with the aim of measuring the masses of the black holes in 13 nearby (z<0.05) Seyfert 1 galaxies with expected masses in the range-106-107 M⊙. We present here the first results from this project-the mass of the central black hole in Arp 151. Strong variability throughout the campaign led to an exceptionally clean Hβ lag measurement in this object of 4.25+0.68-0.66 days in the observed frame. Coupled with the width of the Hβ emission line in the variable spectrum, we determine a black hole mass of (7.1 ± 1.2) × 106 M⊙, assuming the Onken et al. normalization for reverberation-based virial masses. We also find velocity-resolved lag information within the Hβ emission line which clearly shows infalling gas in the Hβ-emitting region. Further detailed analysis may lead to a full model of the geometry and kinematics of broad line region gas around the central black hole in Arp 151.",

keywords = "Galaxies: Individual (Arp 151), Galaxies: Nuclei, Galaxies: Seyfert, Galaxies: active",

author = "Bentz, \{Misty C.\} and Walsh, \{Jonelle L.\} and Barth, \{Aaron J.\} and Nairn Baliber and Nicola Bennert and Gabriela Canalizo and Filippenko, \{Alexei V.\} and Mohan Ganeshalingam and Gates, \{Elinor L.\} and Greene, \{Jenny E.\} and Hidas, \{Marton G.\} and Hiner, \{Kyle D.\} and Nicholas Lee and Weidong Li and Malkan, \{Matthew A.\} and Takeo Minezaki and Serduke, \{Frank J.D.\} and Shiode, \{Joshua H.\} and Silverman, \{Jeffrey M.\} and Steele, \{Thea N.\} and Daniel Stern and Street, \{Rachel A.\} and Thornton, \{Carol E.\} and Tommaso Treu and Xiaofeng Wang and Woo, \{Jong Hak\} and Yuzuru Yoshiill",

year = "2008",

doi = "10.1086/595719",

language = "English (US)",

volume = "689",

pages = "L21--L24",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1 PART 2",

}

Bentz, MC, Walsh, JL, Barth, AJ, Baliber, N, Bennert, N, Canalizo, G, Filippenko, AV, Ganeshalingam, M, Gates, EL, Greene, JE, Hidas, MG, Hiner, KD, Lee, N, Li, W, Malkan, MA, Minezaki, T, Serduke, FJD, Shiode, JH, Silverman, JM, Steele, TN, Stern, D, Street, RA, Thornton, CE, Treu, T, Wang, X, Woo, JH & Yoshiill, Y 2008, 'First results from the lick AGN monitoring project: The mass of the black hole in ARP 151', Astrophysical Journal, vol. 689, no. 1 PART 2, pp. L21-L24. https://doi.org/10.1086/595719

TY - JOUR

T1 - First results from the lick AGN monitoring project

T2 - The mass of the black hole in ARP 151

AU - Bentz, Misty C.

AU - Walsh, Jonelle L.

AU - Barth, Aaron J.

AU - Baliber, Nairn

AU - Bennert, Nicola

AU - Canalizo, Gabriela

AU - Filippenko, Alexei V.

AU - Ganeshalingam, Mohan

AU - Gates, Elinor L.

AU - Greene, Jenny E.

AU - Hidas, Marton G.

AU - Hiner, Kyle D.

AU - Lee, Nicholas

AU - Li, Weidong

AU - Malkan, Matthew A.

AU - Minezaki, Takeo

AU - Serduke, Frank J.D.

AU - Shiode, Joshua H.

AU - Silverman, Jeffrey M.

AU - Steele, Thea N.

AU - Stern, Daniel

AU - Street, Rachel A.

AU - Thornton, Carol E.

AU - Treu, Tommaso

AU - Wang, Xiaofeng

AU - Woo, Jong Hak

AU - Yoshiill, Yuzuru

PY - 2008

Y1 - 2008

N2 - We have recently completed a 64 night spectroscopic monitoring campaign at the Lick Observatory 3 m Shane telescope with the aim of measuring the masses of the black holes in 13 nearby (z<0.05) Seyfert 1 galaxies with expected masses in the range-106-107 M⊙. We present here the first results from this project-the mass of the central black hole in Arp 151. Strong variability throughout the campaign led to an exceptionally clean Hβ lag measurement in this object of 4.25+0.68-0.66 days in the observed frame. Coupled with the width of the Hβ emission line in the variable spectrum, we determine a black hole mass of (7.1 ± 1.2) × 106 M⊙, assuming the Onken et al. normalization for reverberation-based virial masses. We also find velocity-resolved lag information within the Hβ emission line which clearly shows infalling gas in the Hβ-emitting region. Further detailed analysis may lead to a full model of the geometry and kinematics of broad line region gas around the central black hole in Arp 151.

AB - We have recently completed a 64 night spectroscopic monitoring campaign at the Lick Observatory 3 m Shane telescope with the aim of measuring the masses of the black holes in 13 nearby (z<0.05) Seyfert 1 galaxies with expected masses in the range-106-107 M⊙. We present here the first results from this project-the mass of the central black hole in Arp 151. Strong variability throughout the campaign led to an exceptionally clean Hβ lag measurement in this object of 4.25+0.68-0.66 days in the observed frame. Coupled with the width of the Hβ emission line in the variable spectrum, we determine a black hole mass of (7.1 ± 1.2) × 106 M⊙, assuming the Onken et al. normalization for reverberation-based virial masses. We also find velocity-resolved lag information within the Hβ emission line which clearly shows infalling gas in the Hβ-emitting region. Further detailed analysis may lead to a full model of the geometry and kinematics of broad line region gas around the central black hole in Arp 151.

KW - Galaxies: Individual (Arp 151)

KW - Galaxies: Nuclei

KW - Galaxies: Seyfert

KW - Galaxies: active

UR - https://www.scopus.com/pages/publications/66649111645

UR - https://www.scopus.com/pages/publications/66649111645#tab=citedBy

U2 - 10.1086/595719

DO - 10.1086/595719

M3 - Article

AN - SCOPUS:66649111645

SN - 0004-637X

VL - 689

SP - L21-L24

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 PART 2

ER -

First results from the lick AGN monitoring project: The mass of the black hole in ARP 151

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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