output
20042026
most citedSatellite-to-ground quantum key distribution

1.8k citations

499 papers

astro-ph.IM2026

Quantifying the temperature-dependent yields of N and NH formation in vacuum-ultraviolet-irradiated NH ice

P. Samarth, G. Fedoseev, S. Ioppolo +3

Gas--grain astrochemical models predict that a substantial fraction of elemental nitrogen in dense cores and protoplanetary disks is locked in molecular nitrogen (N), in the ga…

astro-ph.GA2026★ 2 cited

In situ characterization of volatile and refractory hydrocarbons produced by UV photolysis of interstellar CH ice

P. Samarth, G. Fedoseev, M. Bulak +5

Acetylene (CH) is commonly observed in star-forming regions, young stellar objects, and the Solar System. Laboratory and theoretical studies have linked this simplest alkyn…

astro-ph.GA2026

ALMA Reveals an Explosive Outflow Candidate in IRAS 16119--5048

Yongquan Luo, Jianjun Zhou, Tie Liu +24

We present a multiwavelength study of the massive star formation region IRAS 16119-5048 (I16119) using ALMA ATOMS Band 3 and QUARKS Band 6 observations, complemented by archival AT…

astro-ph.SR2026

SN 2021pfs: A Type Ia Supernova Likely Affected by Progenitor Metallicity, as Revealed by Comparison with Its Twin Counterpart

Abdusamatjan Iskandar, Xiaofeng Wang, Ali Esamdin +16

We present extensive photometric and spectroscopic observations of the normal type Ia supernovae (SNe Ia) 2021pfs, which occurred in the Seyfert 2 galaxy NGC 5427 at a redshift 0.0…

astro-ph.SR2026★ 6 cited

TESS Observations of Seven Newly Identified High-amplitude Scuti Stars

Chenglong Lv, Ali Esamdin, Amir Hasanzadeh +3

We report seven newly identified high-amplitude Scuti (HADS) stars. Among them, two stars (TIC 30977864 and TIC 387379145) exhibit pure radial pulsation without the excitation…

astro-ph.SR2026★ 4 cited

Statistical analysis of asteroseismic indices and stellar parameters of TESS-observed Scuti stars

C. Lv, A. Esamdin, A. Hasanzadeh +4

We analyze the statistical properties and asteroseismic indices of delta Scuti stars observed during TESS Cycle 4. Using 2 minute cadence photometry and Fourier analysis, we identi…