VLBA14B-343

The Megamaser Cosmology Project

Abstract

To constrain models of dark energy, a precise measurement of the Hubble constant provides the best complement to observations of the Cosmic Microwave Background. The Megamaser Cosmology Project (MCP) aims to determine Ho to 3% by measuring geometric distances to water vapor megamasers in the Hubble flow. Based on published observations of UGC 3789 and NGC 6264, the MCP measures Ho = 68.6 +/- 5.6 km/s/Mpc, an 8% result. Including 4 additional preliminary measurements, we determine Ho = 69.0 +/- 3.8 km/s/Mpc (5.5%). We are improving this result by measuring distances to additional galaxies. As a second important science result, the MCP determines the most precise (< 10%) masses of supermassive black holes in external galaxies by measuring the Keplerian rotation curves of masers within a parsec of the black hole. We have determined masses for 17 SMBHs so far, and these measurements are key to understanding the co-evolution of supermassive black holes and their host galaxies. In this proposal we request GBT, HSA, and VLA time to measure the distance to ESO 558-G009, continue our successful survey for additional megamasers in AGNs, and map two newly-discovered maser disks.

Investigators

Name Institution
Wei Zhao Shanghai Astronomical Observatory, CAS; Independent
Jan Wagner Max-Planck-Institut für Radioastronomie
Mark Reid Center for Astrophysics | Harvard & Smithsonian
Dominic Pesce Virginia, University of; Smithsonian Astrophysical Observatory
Fred K. Y. Lo National Radio Astronomy Observatory
Eugenia Litzinger Würzburg, Universität
Cheng-Yu Kuo Virginia, University of; National Sun Yat-sen University
Violette Impellizzeri National Radio Astronomy Observatory; Leiden, University of; Joint ALMA Observatory
Chris Henkel Max-Planck-Institut für Radioastronomie
Lei Hao Shanghai Astronomical Observatory, CAS
Jenny Greene Princeton University
Feng Gao Max-Planck-Institut für Radioastronomie
Anca Constantin James Madison University
Jim Condon Independent
Jim Braatz * National Radio Astronomy Observatory
GBT Operator Green Bank Observatory
vlbaops vlbaops National Radio Astronomy Observatory
vlbiobs vlbiobs National Radio Astronomy Observatory

* indicates the PI