output
20092026
most citedJADES. The diverse population of infant Black Holes at 4<z<11: merging, tiny, poor, but mighty

361 citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

collaborating institutions
Showing 2025 · astro-ph.SRShow all

8 papers · 2 filters

astro-ph.SR2025★ 1 cited

Observational Properties of Cephei Stars: 88 new samples discovered Based on TESS and Gaia Data

Xiang-dong Shi, Sheng-bang Qian, Li-ying Zhu +5

We present a systematic investigation of Cephei (BCEP) stars by integrating photometric data from the Transiting Exoplanet Survey Satellite (TESS) with astrometric parameters f…

astro-ph.SR2025★ 5 cited

Evidence for the Keplerian orbit of a close companion around a giant star

Mats Esseldeurs, Leen Decin, Joris De Ridder +31

Close companions influence stellar evolution through tidal interactions, mass transfer, and mass loss effects. While such companions are detected around young stellar objects, main…

astro-ph.SR2025★ 6 cited

SN 2022xlp: The second-known well-observed, intermediate-luminosity Iax supernova

D. Bánhidi, B. Barna, T. Szalai +17

We present a detailed analysis of type Iax supernova SN 2022xlp. With a V-band absolute magnitude light curve peaking at mag, this object is regarded…

astro-ph.SR2025★ 2 cited

Chemical abundances and doppler imaging of the Ap Si/He-wk star HD 100357

Athul Dileep, Santosh Joshi, Sofya Alexeeva +11

We present the results of time-resolved photometry, abundance analysis and Doppler imaging of an Ap star, HD 100357. The {\it TESS} photometry revealed rotational modulation with a…

astro-ph.SR2025★ 7 cited

ATOMIUM: Continuum emission and evidence of dust enhancement from binary motion

T. Danilovich, N. Samaratunge, Y. Mori +35

Low- and intermediate-mass stars on the asymptotic giant branch (AGB) account for a significant portion of the dust and chemical enrichment in their host galaxy. Here we present AL…

astro-ph.SR2025

Investigating Pulsating Variables and Eclipsing Binaries in NGC 2126 using Ground and Space-based Photometry, Astrometry, Spectroscopy and Modeling

Athul Dileep, Santosh Joshi, Sneh Lata +12

Pulsating variables are prevalent in the classical δ Scuti instability strip of intermediate-age open star clusters. The cluster membership of these stars facilitates a comparative…

astro-ph.SR2025

Characterisation of H spectra from EXO 051910+3737.7 X-rays binaries

Pornisara Nuchvanichakul, Puji Irawati, Pakakaew Rittipruk +4

We investigate the spectral characteristics of the Be/X-ray binary system, EXO 051910+3737.7, in which Be/X-ray systems are the largest sub-class of high-mass X-ray binaries. Spect…

astro-ph.SR2025★ 5 cited

GOTO065054+593624: a 8.5 mag amplitude dwarf nova identified in real time via Kilonova Seekers

T. L. Killestein, G. Ramsay, M. Kennedy +62

Dwarf novae are astrophysical laboratories for probing the nature of accretion, binary mass transfer, and binary evolution -- yet their diverse observational characteristics contin…