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researcher

K. E. Saavik Ford

25 papers hereh-index 368 citations3 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author3
  • middle author15
  • last author4

Across the 22 of 25 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE11
  • astro-ph.GA5
  • astro-ph.CO3
  • astro-ph.IM3
  • astro-ph1
  • astro-ph.EP1
same name
  • K. E. Saavik Ford — 6 papers
  • K. E. Saavik Ford — 1 paper
  • K. E. Saavik Ford — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20012026
most citedOn stellar-mass black hole mergers in AGN disks detectable with LIGO

296 citations · 977 across the 24 of their papers we have counts for

collaborators
Showing 2022Show all

3 papers · 1 filter

astro-ph.IM2022★ 23 cited

The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope -- IV. Aperture Masking Interferometry

Anand Sivaramakrishnan, Peter Tuthill, James P. Lloyd +36

The James Webb Space Telescope's Near Infrared Imager and Slitless Spectrograph (JWST-NIRISS) flies a 7-hole non-redundant mask (NRM), the first such interferometer in space, opera…

astro-ph.HE2022★ 93 cited

A light in the dark: searching for electromagnetic counterparts to black hole-black hole mergers in LIGO/Virgo O3 with the Zwicky Transient Facility

Matthew J. Graham, Barry McKernan, K. E. Saavik Ford +11

The accretion disks of active galactic nuclei (AGN) are promising locations for the merger of compact objects detected by gravitational wave (GW) observatories. Embedded within a b…

astro-ph.GA2022★ 32 cited

Aligning Retrograde Nuclear Cluster Orbits with an Active Galactic Nucleus Accretion Disc

Syeda S. Nasim, Gaia Fabj, Freddy Caban +6

Stars and stellar remnants orbiting a supermassive black hole (SMBH) can interact with an active galactic nucleus (AGN) disc. Over time, prograde orbiters (inclination $i<90^{\circ…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.