activity
20142026
most citedSix Months of Multi-Wavelength Follow-up of the Tidal Disruption Candidate ASASSN-14li and Implied TDE Rates from ASAS-SN

324 citations · 470 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2026

Unresolved triples in the open cluster NGC 2437 (M 46) confirmed by the KMOS VVVX-GalCen Spectroscopic Survey

D. Minniti, T. Palma, C. O. Obasi +31

Recent optical and near-IR photometric databases like Gaia data release 3 (DR3) and the VISTA Variables in the Vía Láctea eXtended (VVVX) ESO public survey allow the exploration of…

astro-ph.SR2026

Unresolved triple systems in the aged open cluster Trumpler 19: Discovery, confirmation, and implications

D. Minniti, R. K. Saito, V. D. Ivanov +31

It is difficult to identify unresolved triple and higher-order systems beyond the solar vicinity. Star clusters yield controlled environments with known physical parameters, provid…

astro-ph.SR2026

Infrared-excess sources in VVV: candidate debris discs, SED characterization, and variability analysis

P. Esteves, R. K. Saito, C. Chavero +9

Debris disks around main-sequence stars provide important insights into planetary formation and evolution; however, identifying these systems in the Galactic plane, where high inte…

astro-ph.HE2026

A newly born spider system at the core of a radio shell: Evidence for a low-energy supernova

S. Lazarević, R. Brose, L. M. Oskinova +24

In a search for low surface brightness radio nebulae using the ASKAP-EMU survey, we discovered a faint radio shell, G289.6+5.8, and its central point radio source at the position o…

astro-ph.SR2025★ 8 cited

The Outbursting YSOs Catalogue (OYCAT)

C. Contreras Peña, J. -E. Lee, G. Herczeg +39

YSOs can display unpredictable and high-amplitude rises in brightness that can last from a few months to possibly over 100 years. These types of outbursts are explained by large ch…

astro-ph.SR2025

Eruptive YSOs in Cygnus-X: a mid-infrared variability study with NEOWISE and SPICY

C. Morris, Z. Guo, P. W. Lucas +3

The mass accretion process controls pre-main-sequence evolution, although its intrinsic instability has yet to be fully understood, especially towards the protostellar stage. In th…

astro-ph.SR2024★ 15 cited

Mode identification and ensemble asteroseismology of 119 Cep stars detected by Gaia light curves and monitored by TESS

D. J. Fritzewski, M. Vanrespaille, C. Aerts +3

The Gaia mission detected many new candidate Cephei ( Cep) pulsators, whose variability classification has since been confirmed from Transiting Exoplanet Survey Satellite (T…

astro-ph.GA2024★ 38 cited

The VISTA Variables in the Vía Láctea eXtended (VVVX) ESO public survey: Completion of the observations and legacy

R. K. Saito, M. Hempel, J. Alonso-García +143

The ESO public survey VISTA Variables in the Vía Láctea (VVV) surveyed the inner Galactic bulge and the adjacent southern Galactic disk from . Upon its conclusion, the c…

astro-ph.SR2024★ 14 cited

The most variable VVV sources: eruptive protostars, dipping giants in the Nuclear Disc and others

P. W. Lucas, L. C. Smith, Z. Guo +16

We have performed a comprehensive search of a VISTA Variables in the Via Lactea (VVV) database of 9.5 yr light curves for variable sources with mag, aiming to provide…

astro-ph.SR2022★ 1 cited

UGPS J194310+183851: an Unusual Optical and X-ray Faint Cataclysmic Variable?

C. Morris, T. J. Maccarone, P. W. Lucas +7

The growing number of multi-epoch optical and infrared sky surveys are uncovering unprecedented numbers of new variable stars, of an increasing number of types. The short interval…

astro-ph.HE2015★ 324 cited

Six Months of Multi-Wavelength Follow-up of the Tidal Disruption Candidate ASASSN-14li and Implied TDE Rates from ASAS-SN

T. W. -S. Holoien, C. S. Kochanek, J. L. Prieto +21

We present ground-based and Swift photometric and spectroscopic observations of the candidate tidal disruption event (TDE) ASASSN-14li, found at the center of PGC 043234 ($d\simeq9…

astro-ph.SR2014★ 70 cited

KIC 3858884: a hybrid δ Sct pulsator in a highly eccentric eclipsing binary

C. Maceroni, H. Lehmann, R. da Silva +10

The analysis of eclipsing binaries containing non-radial pulsators allows: i) to combine two different and independent sources of information on the internal structure and evolutio…