activity
20032023
most cited3D kinematics of white dwarfs from the SPY project II

138 citations · 368 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2023★ 14 cited

Membership analysis and 3D kinematics of the star-forming complex around Trumpler 37 using Gaia-DR3

Swagat R. Das, Saumya Gupta, Prem Prakash +2

Identifying and characterizing young populations of star-forming regions is crucial to unravel their properties. In this regard, Gaia-DR3 data and machine learning tools are very u…

astro-ph.HE2020★ 30 cited

VHE gamma-ray detection of FSRQ QSO B1420+326 and modeling of its enhanced broadband state in 2020

V. A. Acciari, S. Ansoldi, L. A. Antonelli +230

Context. QSO B1420+326 is a blazar classified as a Flat Spectrum Radio Quasar (FSRQ). In the beginning of 2020 it underwent an enhanced flux state. An extensive multiwavelength cam…

astro-ph.GA2020

ALMA detection of the dusty object silhouetted against the S0 galaxy NGC 3269 in the Antlia cluster

L. K. Haikala, R. Salinas, T. Richtler +3

An intriguing silhouette of a small dust patch can be seen against the disk of the S0 galaxy NGC 3269 in the Antlia cluster in optical images. The images do not provide any clue as…

astro-ph.EP2020★ 15 cited

Asteroids' Size Distribution and Colors from HiTS

J. Peña, C. Fuentes, F. Förster +8

We report the observations of solar system objects during the 2015 campaign of the High cadence Transient Survey (HiTS). We found 5740 bodies (mostly Main Belt asteroids), 1203 of…

astro-ph.SR2019★ 19 cited

New type II Cepheids from VVV data towards the Galactic center

V. F. Braga, R. Contreras Ramos, D. Minniti +5

The Galactic center (GC) is the densest region of the Milky Way. Variability surveys towards the GC potentially provide the largest number of variable stars per square degree withi…

astro-ph.SR2018★ 31 cited

New Near-Infrared light-curve templates for RR Lyrae variables

V. F. Braga, P. B. Stetson, G. Bono +34

We provide homogeneous optical (UBVRI) and near-infrared (JHK) time series photometry for 254 cluster (omega Cen, M4) and field RR Lyrae (RRL) variables. We ended up with more than…