activity
19962025
most citedThe DESI Experiment Part I: Science,Targeting, and Survey Design

1.3k citations · 5.5k across the 105 of their papers we have counts for

collaborators

108 papers

astro-ph.GA2025

JWST Observations of the Double Nucleus in NGC 4486B: Possible Evidence for a Recent Binary SMBH Merger and Recoil

Behzad Tahmasebzadeh, Monica Valluri, Shashank Dattathri +19

A recent study of the compact elliptical galaxy NGC 4486B using JWST-NIRSpec IFU kinematics confirmed a supermassive black hole (SMBH) of mass (~8% of…

astro-ph.GA2025

A Stellar Dynamical Mass for the Central Black Hole in MCG06-30-15

Nabanita Das, Misty C. Bentz, Eugene Vasiliev +4

We present the stellar dynamical mass of the central black hole in the nearby Seyfert galaxy MCG06-30-15 using the Schwarzschild orbit-superposition method implemented in the op…

astro-ph.GA2025

A JWST View of the Overmassive Black Hole in NGC 4486B

Behzad Tahmasebzadeh, Matthew A. Taylor, Monica Valluri +19

We present a new stellar dynamical measurement of the supermassive black hole (SMBH) in the compact elliptical galaxy NGC 4486B, based on integral field spectroscopy with JWST/NIRS…

astro-ph.GA2025

A Supermassive Black Hole in a Diminutive Ultra-compact Dwarf Galaxy Discovered with JWST/NIRSpec+IFU

Matthew A. Taylor, Behzad Tahmasebzadeh, Solveig Thompson +18

The integral-field unit mode of the Near-Infrared Spectrograph (NIRSpec+IFU) mounted on the James Webb Space Telescope has now enabled kinematic studies of smaller and less massive…

astro-ph.GA2024★ 1 cited

Orbital Support and Evolution of CX/OX Structures in Boxy/Peanut Bars

Behzad Tahmasebzadeh, Shashank Dattathri, Monica Valluri +7

Barred galaxies exhibit boxy/peanut or X-shapes (BP/X) protruding from their disks in edge-on views. Two types of BP/X morphologies exist depending on whether the X-wings meet at t…

astro-ph.GA2024

The Lower Limit of Dynamical Black Hole Masses Detectable in Virgo Compact Stellar Systems Using the JWST/NIRSpec IFU

Behzad Tahmasebzadeh, Andrew Lapeer, Eugene Vasiliev +3

Due to observational challenges, the mass function of black holes (BH) at lower masses is poorly constrained in the local universe. Understanding the occupation fraction of BHs in…