UCR

Department of Physics & Astronomy



Gabriela Canalizo


Gabriela Canalizo

Gabriela Canalizo

Associate Professor

Office:
Pierce 2100B

Telephone: 951-827-5310
Email: gabriela.canalizo@ucr.edu
Fax: 951-827-6229

Personal Home Page

Current Research:

The main focus of my research is the study of Active Galactic Nuclei (AGN) in the near and distant universe.   AGN are centers of galaxies containing supermassive black holes (BH) that are actively accreting matter at relatively high rates.   Much of the gravitational energy of the infalling material is transformed into radiative energy across the electromagnetic spectrum, making AGN some of the most powerful and luminous objects in the universe.   There are many outstanding fundamental questions regarding the origins and astrophysics of AGN, such as determining the most common triggering mechanisms, the duty cycle, and the mass of the central BH.   I investigate these topics through the detailed study of the environments and host galaxies of AGN, as well as establishing relationships between observable parameters in the host galaxies and fundamental parameters in their active nuclei.

Research Interests:

  • Astrophysics
  • Observational Extragalactic Astrophysics
  • Active Galactic Nuclei
  • Quasar host galaxies and their environments
  • Ultraluminous Infrared Galaxies (ULIGs)
  • Galaxy interactions and mergers
  • Modeling stellar populations
  • Old galaxies at high redshift
  • Adaptive Optics

Education:

Ph.D. 2000, University of Hawaii

Selected Publications:

1. Stellar Velocity Dispersion in Dissipative Galaxy Mergers with Star Formation," Stickley, N.R., Canalizo, G. 2013, ApJ, in press.

2. Intermediate-age Stellar Populations in Classical Quasi-stellar Object Host Galaxies," Canalizo, G., Stockton, A. 2013, ApJ, 772, 132.

3. The Lick AGN Monitoring Project 2011: Fe II Reverberation from the Outer Broad-line Region," Barth, A.J., Pancoast, A., Bennert, V.N., Brewer, B.J., Canalizo, G., et al., 2013, ApJ, 769, 128.

4. Probing the MBH- Relation in the Non-local Universe Using Red QSOs," Canalizo, G., Wold, M., Hiner, K.D., Lazarova, M., Lacy, M., Aylor, K. 2012, ApJ, 760, 38.

5. Black-hole-Bulge Relationship of Post-starburst Quasars at z ~0.3," Hiner, K.D., Canalizo, G., Wold, M., Brotherton, M.S., Cales, S.L. 2012, ApJ, 756, 162.

6. The Nature of LoBAL QSOs. I. SEDs and Mid-infrared Spectral Properties," Lazarova, M.S., Canalizo, G., Lacy, M., Sajina, A. 2012, ApJ, 755, 29.

7. An Infrared Comparison of Type-1 and Type-2 Quasars", Hiner, K.D., Canalizo, G., Lacy, M., Sajina, A., Armus, L., Ridgway, S., Storrie-Lombardi, L. 2009, ApJ, 706, 508.

8. Evidence for Merger Remnants in Early-Type Host Galaxies of Low-Redshift QSOs", Bennert, N., Canalizo, G., Jungwiert, B., Stockton, A., Schweizer, F., Lacy, M., Peng, C. 2008, ApJ, 677, 846.

9. Spectacular Shells in the Host Galaxy of the QSO MC2 1635+119", Canalizo, G., Bennert, N., Jungwiert, B., Stockton, A., Schweizer, F., Lacy, M., Peng, C. 2007, ApJ, 669, 801.

10. Quasi-Stellar Objects, Ultraluminous IR Galaxies, and Mergers", Canalizo, G. & Stockton, A. 2001, ApJ, 555, 719



More Information

General Campus Information

University of California, Riverside
900 University Ave.
Riverside, CA 92521
Tel: (951) 827-1012

Career OpportunitiesUCR Libraries
Campus StatusDirections to UCR

Department Information

Physics & Astronomy
Physics Building

Main Office Tel: (951) 827-5331
Main Office Fax: (951) 827-4529
Maynard, Bonnie; Chair's Assistant, Academic Personnel
E-mail: bonnie.maynard@ucr.edu

Footer