activity
20042008
most citedLIGO: The Laser Interferometer Gravitational-Wave Observatory

1.2k citations · 1.4k across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph200865 cited

Identifying Decaying Supermassive Black Hole Binaries from their Variable Electromagnetic Emission

Zoltán Haiman, Bence Kocsis, Kristen Menou +2

Supermassive black hole binaries (SMBHBs) with masses in the range 10^4-10^7 M_sun/(1+z), produced in galaxy mergers, are thought to complete their coalescence due to the emission…

astro-ph2008101 cited

Prompt Shocks in the Gas Disk Around a Recoiling Supermassive Black Hole Binary

Zoltan Lippai, Zsolt Frei, Zoltan Haiman

Supermassive black hole binaries (BHBs) produced in galaxy mergers recoil at the time of their coalescence due to the emission of gravitational waves (GWs). We simulate the respons…

gr-qc20071.2k cited

LIGO: The Laser Interferometer Gravitational-Wave Observatory

The LIGO Scientific Collaboration, B. Abbott

The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and study gravitational waves of astrophysical origin. Direct detection of gravitational wa…

astro-ph2005

Finding the Electromagnetic Counterparts of Cosmological Standard Sirens

B. Kocsis, Z. Frei, Z. Haiman +1

The gravitational waves (GW) emitted during the coalescence of supermassive black holes (SMBHs) in the mass range 10^4-10^7 M_sun will be detectable out to high redshifts with LISA…

astro-ph2004

Can Virialization Shocks be Detected Around Galaxy Clusters Through the Sunyaev-Zel'dovich Effect?

Bence Kocsis, Zoltan Haiman, Zsolt Frei

In cosmological structure formation models, massive non-linear objects in the process of formation, such as galaxy clusters, are surrounded by large-scale shocks at or around the e…