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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Michele Cappellari

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Galaxy formation and evolution
  • Extremely Large Telescope
michele.cappellari@physics.ox.ac.uk
Telephone: 01865 (2)73647
Denys Wilkinson Building, room 755
  • About
  • Publications

Recovering stellar population parameters via different population models and stellar libraries

(2019)

Authors:

Junqiang Ge, Shude Mao, Youjun Lu, Michele Cappellari, Renbin Yan
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The fifteenth data release of the Sloan Digital Sky Surveys: First release of MaNGA-derived quantities, data visualization tools, and Stellar Library

Astrophysical Journal Supplement Institute of Physics 240:23 (2019)

Authors:

DS Aguado, R Ahumada, A Almeida, Michele Cappellari, R Davies, Chris Lintott

Abstract:

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years of operation (2014 July–2017 July). This is the third data release for SDSS-IV, and the 15th from SDSS (Data Release Fifteen; DR15). New data come from MaNGA—we release 4824 data cubes, as well as the first stellar spectra in the MaNGA Stellar Library (MaStar), the first set of survey-supported analysis products (e.g., stellar and gas kinematics, emission-line and other maps) from the MaNGA Data Analysis Pipeline, and a new data visualization and access tool we call "Marvin." The next data release, DR16, will include new data from both APOGEE-2 and eBOSS; those surveys release no new data here, but we document updates and corrections to their data processing pipelines. The release is cumulative; it also includes the most recent reductions and calibrations of all data taken by SDSS since first light. In this paper, we describe the location and format of the data and tools and cite technical references describing how it was obtained and processed. The SDSS website (www.sdss.org) has also been updated, providing links to data downloads, tutorials, and examples of data use. Although SDSS-IV will continue to collect astronomical data until 2020, and will be followed by SDSS-V (2020–2025), we end this paper by describing plans to ensure the sustainability of the SDSS data archive for many years beyond the collection of data.
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Improved Dynamical Constraints on the Masses of the Central Black Holes in Nearby Low-mass Early-type Galactic Nuclei And the First Black Hole Determination for NGC 205

(2019)

Authors:

Dieu D Nguyen, Anil C Seth, Nadine Neumayer, Satoru Iguchi, Michele Cappellari, Jay Strader, Laura Chomiuk, Evangelia Tremou, Fabio Pacucci, Kouichiro Nakanishi, Arash Bahramian, Phuong M Nguyen, Mark den Brok, Christopher Ahn, Karina T Voggel, Nikolay Kacharov, Takafumi Tsukui, Cuc K Ly, Antoine Dumont, Renuka Pechetti
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Rejuvenated galaxies with very old bulges at the origin of the bending of the main sequence and of the "green valley"

(2019)

Authors:

Chiara Mancini, Emanuele Daddi, Stéphanie Juneau, Alvio Renzini, Giulia Rodighiero, Michele Cappellari, Lucía Rodríguez-Muñoz, Daizhong Liu, Maurilio Pannella, Ivano Baronchelli, Alberto Franceschini, Pietro Bergamini, Chiara D'Eugenio, Annagrazia Puglisi
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The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Overview

(2019)

Authors:

Kyle B Westfall, Michele Cappellari, Matthew A Bershady, Kevin Bundy, Francesco Belfiore, Xihan Ji, David R Law, Adam Schaefer, Shravan Shetty, Christy A Tremonti, Renbin Yan, Brett H Andrews, Joel R Brownstein, Brian Cherinka, Lodovico Coccato, Niv Drory, Claudia Maraston, Taniya Parikh, José R Sánchez-Gallego, Daniel Thomas, Anne-Marie Weijmans, Jorge Barrera-Ballesteros, Cheng Du, Daniel Goddard, Niu Li, Karen Masters, Héctor Javier Ibarra Medel, Sebastián F Sánchez, Meng Yang, Zheng Zheng, Shuang Zhou
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