activity
20232026
most cited10,000 Resolved Triples from Gaia: Empirical Constraints on Triple Star Populations

20 citations · 52 across the 19 of their papers we have counts for

collaborators

26 papers

astro-ph.HE2026

A concordance model of neutron star kicks

Cheyanne Shariat, Kareem El-Badry, Smadar Naoz

Neutron stars (NSs) receive natal kicks during supernovae that affect their survival in binaries and motion through the Galaxy. The global distribution of these kick velocities acr…

astro-ph.SR2026

Gaia neutron stars: demographics, birth rates, and connections to other neutron star populations

Cheyanne Shariat, Natsuko Yamaguchi, Kareem El-Badry +1

Gaia DR3 revealed a new class of neutron stars (NSs) in au-scale orbits with solar-type companions. How these 'Gaia NSs' form remains unclear, and constraining their intrinsic popu…

astro-ph.SR2026

Beyond what's observed: hierarchical inference of Gaia astrometric compact-object binaries

Natsuko Yamaguchi, Kareem El-Badry, Reed Essick +3

Astrometry from the Gaia mission has revealed a large and homogeneous population of binaries containing compact objects, including more than 3000 white dwarf--main sequence (WDMS)…

astro-ph.EP2026

Worlds Next Door. V. A Candidate Solar System Scale Super-Jupiter in the 61 Cygni Binary System

Aniket Sanghi, Billy Quarles, Andrea S. J. Lin +16

We present new constraints on a candidate third companion in the 61 Cygni binary system-one of the closest neighbors to our solar system (3.5 pc), the first stars to have a measure…

astro-ph.SR2026

A census of massive eclipsing binaries in the Whirlpool Galaxy

Cheyanne Shariat, Kareem El-Badry, Maude Gull +3

We present a census of massive eclipsing binary (EB) candidates in the Whirlpool Galaxy (M51), a face-on spiral galaxy at 7.5 Mpc with . Using 34 epochs of red-optic…

astro-ph.EP2026

Stellar companions sculpt hot Jupiter formation and spin-orbit evolution

Cheyanne Shariat, Kareem El-Badry, Songhu Wang +4

Stellar companions can drive hot-Jupiter (HJ) migration and spin-orbit misalignment, but their role in HJ formation remains uncertain. We construct a homogeneous census of resolved…

astro-ph.SR2026

Population demographics of post-interaction WDMS binaries: From common envelope evolution to stable mass transfer

Natsuko Yamaguchi, Kareem El-Badry, Cheyanne Shariat

Close white dwarf (WD) + main-sequence (MS) binaries are end products of mass transfer (MT) that occurred prior to WD formation, making their population demographics a powerful pro…

astro-ph.GA2026

Probing the IMF in the Early Universe -- Direct measurements in the Boötes I UFD with JWST/NIRCam

Keyi Ding, Mario Gennaro, Roberto J. Avila +20

The dependence of the stellar initial mass function (IMF) on star-formation environment, particularly at low metallicities and high redshifts, remains poorly constrained. Ultra-fai…

cs.DL2026

OverCite: Add citations in LaTeX without leaving the editor

Cheyanne Shariat

Adding citations while drafting in LaTeX often requires leaving the editor, searching for a paper in mind, copying its BibTeX entry into the project bibliography, renaming the cite…

astro-ph.SR2026

Gaia astrometry disfavors a binary origin for long secondary periods

Cheyanne Shariat, Kareem El-Badry, Morgan MacLeod +1

Approximately one-third of luminous pulsating red giant stars exhibit long secondary periods (LSPs): stable photometric variability with periods of several months to years in addit…

astro-ph.SR2026

Thermally inflated accretors in post-mass transfer binaries: Abell 35 and its class revisited

Soumyadeep Bhattacharjee, Kareem El-Badry, Jim Fuller +2

A small but growing class of binaries containing hot () white dwarfs (WDs) and rapidly rotating, apparently subgiant companions -- including the proto…

astro-ph.SR2026

A global view of post-interaction white dwarf-main sequence binaries

Cheyanne Shariat, Kareem El-Badry

Common-envelope evolution (CEE) is among the most uncertain phases in binary evolution. To empirically constrain CEE, we construct a uniformly selected sample of eclipsing post--co…

astro-ph.HE2025

Fast Radio Bursts from White Dwarf Binary Mergers: Isolated and Triple-Induced Channels

Cheyanne Shariat, Claire S. Ye, Smadar Naoz +1

The detection of fast radio bursts (FRBs) in both young and old stellar populations suggests multiple formation pathways, beyond just young magnetars from core-collapse supernovae.…

astro-ph.SR2025★ 2 cited

How precisely can we measure the ages of subgiant and giant stars?

Cheyanne Shariat, Kareem El-Badry, Soumyadeep Bhattacharjee

Precise stellar ages are fundamental to Galactic archaeology. However, obtaining reliable age estimates and uncertainties for field stars has been a long-standing challenge. We tes…

astro-ph.GA2025

Wide binaries in an ultra-faint dwarf galaxy: discovery, population modeling, and a nail in the coffin of primordial black hole dark matter

Cheyanne Shariat, Kareem El-Badry, Mario Gennaro +24

We report the discovery and characterization of a wide binary population in the ultrafaint dwarf galaxy Boötes I using deep JWST/NIRCam imaging. Our sample consists of 52 candidate…

astro-ph.SR2025

Possible Dynamical Pathways to the Misalignment of the VHS 1256-1257 System

Liz Holzknecht, Smadar Naoz, Cheyanne Shariat

Circumbinary planets (CBPs) provide a unique window into planet formation and dynamical evolution in complex gravitational environments. Their orbits are shaped not only by the pro…

astro-ph.HE2025

From Wide Triples to UCXBs: Multimessenger Signatures of Dynamically-formed Black Hole-White Dwarf Systems in the LISA Band

Zeyuan Xuan, Cheyanne Shariat, Smadar Naoz

Ultracompact X-ray binaries (UCXBs) are a subclass of low-mass X-ray binaries characterized by tight orbits and degenerate donors, which pose significant challenges to our understa…

astro-ph.SR2025★ 20 cited

10,000 Resolved Triples from Gaia: Empirical Constraints on Triple Star Populations

Cheyanne Shariat, Kareem El-Badry, Smadar Naoz

We present a catalog of resolved triple star systems within 500 pc of the Sun, constructed using Gaia data. The triples include main-sequence, red giant, and white dw…

astro-ph.SR2025★ 3 cited

Unevolved Li-rich stars at low metallicity: a possible formation pathway through novae

Tadafumi Matsuno, Alex Kemp, Ataru Tanikawa +7

A small fraction of low-mass stars have been found to have anomalously high Li abundances. Although it has been suggested that mixing during the red giant branch phase can lead to…

astro-ph.SR2025★ 10 cited

Cataclysmic Variables in Triples: Formation Models and New Discoveries

Cheyanne Shariat, Kareem El-Badry, Smadar Naoz +2

The formation of cataclysmic variables (CVs) has long been modeled as a product of common envelope evolution (CEE) in isolated binaries. However, a significant fraction of intermed…

astro-ph.SR2024★ 1 cited

Triple Evolution Pathways to Black Hole Low-Mass X-ray Binaries: Insights from V404 Cygni

Cheyanne Shariat, Smadar Naoz, Kareem El-Badry +5

A recent discovery shows that V404 Cygni, a prototypical black hole low-mass X-ray binary (BH-LMXB) is a hierarchical triple: the BH and donor star are orbited by a M$_{\odot…

astro-ph.EP2024

Two Novel Hot Jupiter Formation Pathways: How White Dwarf Kicks Shape the Hot Jupiter Population

Alexander P. Stephan, David V. Martin, Smadar Naoz +2

The origin of Hot Jupiters (HJs) is disputed between a variety of in situ and ex situ formation scenarios. One of the early proposed ex situ scenarios was the Eccentric Kozai-Lidov…

astro-ph.SR2024★ 2 cited

Once a Triple, Not Always a Triple: The Evolution of Hierarchical Triples that Yield Merged Inner Binaries

Cheyanne Shariat, Smadar Naoz, Kareem El-Badry +4

More than half of all main-sequence (MS) stars have one or more companions, and many of those with initial masses <8 M are born in hierarchical triples. These systems featu…

astro-ph.EP2024★ 2 cited

Predicting the Dominant Formation Mechanism of Multi-Planetary Systems

Cheyanne Shariat, Yasuhiro Hasegawa, Bradley M. S. Hansen +2

Most, if not all, sun-like stars host one or more planets, making multi-planetary systems commonplace in our galaxy. We utilize hundreds of multi-planet simulations to explore the…