activity
20082020
most citedThe All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0

1.2k citations · 1.5k across the 7 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2020

Multi-phase feedback processes in the Sy2 galaxy NGC 5643

I. García-Bernete, A. Alonso-Herrero, S. García-Burillo +11

We study the multi-phase feedback processes in the central ~3 kpc of the barred Sy 2 galaxy NGC 5643. We use observations of the cold molecular gas (ALMA CO(2-1)) and ionized gas (…

astro-ph.GA2020

Mapping the Galactic disk with the LAMOST and Red clump sample: V: On the origin of the "young" [/Fe]-enhanced stars

Weixiang Sun, Yang Huang, Haifeng Wang +8

Using a sample of nearly 140,000 primary red clump stars selected from the LAMOST and surveys, we have identified a large sample of "young" [/Fe]-enhanced stars with stel…

astro-ph.EP202021 cited

Is the gap in the DS Tau disc hiding a planet?

Benedetta Veronesi, Enrico Ragusa, Giuseppe Lodato +6

Recent mm-wavelength surveys performed with the Atacama Large Millimeter Array (ALMA) have revealed protoplanetary discs characterized by rings and gaps. A possible explanation for…

astro-ph.GA202034 cited

Probing the circumnuclear absorbing medium of the buried AGN in NGC 1068 through NuSTAR observations

A. Zaino, S. Bianchi, A. Marinucci +9

We present the results of the latest NuSTAR monitoring campaign of the Compton-thick Seyfert 2 galaxy NGC 1068, composed of four 50 ks observations performed between July 201…

astro-ph.GA201956 cited

Torus model properties of an ultra-hard X-ray selected sample of Seyfert galaxies

I. García-Bernete, C. Ramos Almeida, A. Alonso-Herrero +15

We characterize for the first time the torus properties of an ultra-hard X-ray (14-195 keV) volume-limited (DL<40 Mpc) sample of 24 Seyfert (Sy) galaxies (BCS40 sample). The sample…

astro-ph.GA2018

Structure and kinematics of Type II Cepheids in the Galactic bulge based on near-infrared VVV data

V. F. Braga, A. Bhardwaj, R. Contreras Ramos +5

Type II Cepheids (T2Cs) are radially pulsating variables that trace old stellar populations and provide distance estimates through their period-luminosity (PL) relation. We trace t…