PPT-Mass Measurements of Black Holes in X-Ray Transients: is there a Mass Gap?

Will M Farr Northwestern University CIERA See Kreidberg Bailyn WMF Kalogera arXiv12051805 The Mass Gap Strange because mainsequence mass distribution rising at low M . Peter Hall, Tim Colegate, J-P Macquart, Nathan Clarke, Steven Tingay, Cathryn Trott and Randall Wayth. ICRAR / Curtin Institute of Radio Astronomy. Overview. Fast transients in radio astronomy. < 5 s duration for the purpose of this talk. Formation and cosmic evolution of massive black holes. Andrea Merloni. MPE, Garching. Syllabus. Monday:. Observational evidence of Supermassive Black Holes. AGN surveys. Tuesday: . The evolution of SMBH mass function and spin distributions. ELCT222- Lecture Notes. University of S. Carolina. Spring 2012. Outline. RC transients charging. RC transients discharge. RC transients . Thevenin. P-SPICE. RL transients charging. RL transients discharge. The . sole responsibility for the content of this publication lies with the authors. It does not necessarily reflect the opinion of the European Union. Neither the EASME nor the European Commission are responsible for any use that may be made of the information contained therein. ELCT222- Lecture Notes. University of S. Carolina. Spring 2012. Outline. RC transients charging. RC transients discharge. RC transients . Thevenin. P-SPICE. RL transients charging. RL transients discharge. Fiducialisation. Sylvain GRIFFET, 21/03/2011. Measurements performed in February and early March 2011. 1. /13. EDMS n°. 1134701. Plan. Measurements of DB supporting systems. Sylvain GRIFFET, 21/03/2011. Black Holes. Philip Kahn – 02/20/2009. Tri-Valley . Stargazers. Know Thy Enemy. Black holes are:. Infinitesimally small. Asymptotically dense. ρ ∝ M/. L. P. 3. . Black holes do:. Heavily distort . The exciting parts of the universe. Sydney Institute for Astronomy (. SIfA. )/ CAASTRO – The University of Sydney. Dr. Paul Hancock. (and occasionally the Sydney Observatory). Transients are Extreme. M87. Hercules A radio jets. Active Galactic Nuclei (AGNs) and Supermassive Black Holes. The identification by Maarten Schmidt (1963, . Nature. , 197, 1040) of the radio source 3C 273 as a . “. star. Centaurus. X-3 Over its Binary Orbit”. -. Sachindra. Naik, . Biswajit. Paul, and . Zulfikar. Ali. Introduction:. Interest: Extended dips in the light curve. Cen-X: Eclipsing HMXRB pulsar. Orbital period ~2.1 days, pulse period ~4.8 s. The Magnetic Origin of Black Hole Accretion Disk Winds Chris Shrader* (NASA Goddard Space Flight Center ) Collaborators: D. Kazanas (GSFC), K. Fukumura (JMU), F. Tombesi (UMD), Ehud Behar ( Simeon Bird . (JHU). I. Cholis, J. Munoz, Y. Ali-Haimoud, M. Kamionkowski, E. Kovetz, A. Raccanelli, A. Riess. PRL 116 201301. arXiv: 1603.00464. LIGO detected Gravitational Waves. LIGO Detection. Two merging 30 solar mass BHs. Jeff McClintock. Harvard-Smithsonian Center for Astrophysics. Black Holes’ New Horizons. Oaxaca, May 2016 . Introduction. Spin via continuum-fitting. Applications of spin data. X-ray “reflection” spectroscopy. catalog. Eric Thrane (Monash University). October 24, 2019. The 2. nd. . Pietro. . Baracchi. Conference. Welcome to the era of routine detections!. Thirty-three . new events since the beginning of the third observing run on April 1..