Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Quenneville, Matthew"'
Autor:
Quenneville, Matthew E., Blakeslee, John P., Ma, Chung-Pei, Greene, Jenny E., Gwyn, Stephen D. J., Ciccone, Stephanie, Nyiri, Blanka
We present wide-field, deep $K$-band photometry of 98 luminous early-type galaxies (ETGs) from the MASSIVE survey based on observations taken with the WIRCam instrument on the Canada-France-Hawaii Telescope. Using these images, we extract accurate to
Externí odkaz:
http://arxiv.org/abs/2210.08043
Autor:
Pilawa, Jacob D., Liepold, Christopher M., Andrade, Silvana C. Delgado, Walsh, Jonelle L., Ma, Chung-Pei, Quenneville, Matthew E., Greene, Jenny E., Blakeslee, John P.
We present a stellar dynamical mass measurement of a newly detected supermassive black hole (SMBH) at the center of the fast-rotating, massive elliptical galaxy NGC 2693 as part of the MASSIVE survey. We combine high signal-to-noise integral field sp
Externí odkaz:
http://arxiv.org/abs/2111.13699
Most stellar-dynamical determinations of the masses of nearby supermassive black holes (SMBHs) have been obtained with the orbit superposition technique under the assumption of axisymmetry. However, few galaxies -- in particular massive early-type ga
Externí odkaz:
http://arxiv.org/abs/2111.06904
Autor:
Gu, Meng, Greene, Jenny, Newman, Andrew B., Kreisch, Christina, Quenneville, Matthew, Ma, Chung-Pei, Blakeslee, John P.
The stellar initial mass function (IMF) is a fundamental property in the measurement of stellar masses and galaxy star formation histories. In this work we focus on the most massive galaxies in the nearby universe $\log(M_{\star}/M_{\odot})>11.2$. We
Externí odkaz:
http://arxiv.org/abs/2110.11985
We present a detailed analysis of the behavior of the triaxial Schwarzschild orbit superposition method near the axisymmetric limit. Orbit superposition modeling is the primary method used to determine dynamical masses of supermassive black holes ($M
Externí odkaz:
http://arxiv.org/abs/2005.00542
Autor:
Liepold, Christopher M., Quenneville, Matthew E., Ma, Chung-Pei, Walsh, Jonelle L., McConnell, Nicholas J., Greene, Jenny E., Blakeslee, John P.
We present a new stellar dynamical mass measurement ($M_\mathrm{BH}$) of the supermassive black hole (SMBH) in NGC 1453, a fast-rotating massive elliptical galaxy in the MASSIVE survey. We measure stellar kinematics in 135 spatial bins in the central
Externí odkaz:
http://arxiv.org/abs/2001.08753
Autor:
Greene, Jenny E, Veale, Melanie, Ma, Chung-Pei, Thomas, Jens, Quenneville, Matthew E., Blakeslee, John P., Walsh, Jonelle L., Goulding, Andrew, Ito, Jennifer
We measure the stellar populations as a function of radius for 90 early-type galaxies (ETGs) in the MASSIVE survey, a volume-limited integral-field spectroscopic (IFS) galaxy survey targeting all northern-sky ETGs with absolute K-band magnitude M_K <
Externí odkaz:
http://arxiv.org/abs/1901.01271
Publikováno v:
Entropy 20(9), 707, 2018
A stochastic system under the influence of a stochastic environment is correlated with both present and future states of the environment. Such a system can be seen as implicitly implementing a predictive model of future environmental states. The non-
Externí odkaz:
http://arxiv.org/abs/1807.00116
Akademický článek
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Autor:
Quenneville, Matthew E, Blakeslee, John P, Ma, Chung-Pei, Greene, Jenny E, Gwyn, Stephen D J, Ciccone, Stephanie, Nyiri, Blanka
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Jan2024, Vol. 527 Issue 1, p249-264, 16p
