activity
19972013
most citedOptical and Radio Properties of Extragalactic Sources Observed by the FIRST and SDSS Surveys

517 citations · 1.1k across the 13 of their papers we have counts for

collaborators

13 papers

nlin.CD2013

Efficient hierarchical analysis of the stability of a network through dimensional reduction of its influence topology

Ali Kinkhabwala

The connection between network topology and stability remains unclear. General approaches that clarify this relationship and allow for more efficient stability analysis would be de…

math.ST2013★ 2 cited

Maximum Fidelity

Ali Kinkhabwala

The most fundamental problem in statistics is the inference of an unknown probability distribution from a finite number of samples. For a specific observed data set, answers to the…

astro-ph2003★ 1 cited

Atomic Calculations and Spectral Models of X-ray Absorption and Emission Features From Astrophysical Photoionized Plasmas

A. Kinkhabwala, E. Behar, M. Sako +3

We present a detailed model of the discrete X-ray spectroscopic features expected from steady-state, low-density photoionized plasmas. We apply the Flexible Atomic Code (FAC) to ca…

astro-ph2002

Soft X-ray Spectra of Seyfert 2 Galaxies

Masao Sako, Ali Kinkhabwala, Steven M. Kahn +6

High resolution spectroscopic observations of Seyfert galaxies with Chandra and XMM-Newton allows us to study the detailed ionization and thermal structures of the X-ray absorbing/…

astro-ph2002★ 330 cited

XMM-Newton Reflection Grating Spectrometer Observations of Discrete Soft-X-ray Emission Features from NGC 1068

A. Kinkhabwala, M. Sako, E. Behar +6

We present the first high-resolution, soft-X-ray spectrum of the prototypical Seyfert 2 galaxy, NGC 1068. This spectrum was obtained with the XMM-Newton Reflection Grating Spectrom…

astro-ph2002★ 3 cited

Soft X-ray Spectroscopy of NGC 1068 with XMM-Newton RGS and Chandra LETGS

A. Kinkhabwala, M. Sako, E. Behar +7

We present high-resolution soft-X-ray spectra of the prototypical Seyfert 2 galaxy, NGC 1068, taken with XMM-Newton RGS and Chandra LETGS. Its rich emission-line spectrum is domina…