activity
20132020
most citedConnecting the progenitors, pre-explosion variability, and giant outbursts of luminous blue variables with Gaia16cfr

73 citations · 199 across the 7 of their papers we have counts for

collaborators

12 papers

astro-ph.SR202016 cited

HST astrometry in the Orion Nebula Cluster: census of low-mass runaways

Imants Platais, Massimo Robberto, Andrea Bellini +6

We present a catalog of high-precision proper motions in the Orion Nebula Cluster (ONC), based on Treasury Program observations with the Hubble Space Telescope's (HST) ACS/WFC came…

astro-ph.SR20208 cited

HST survey of the Orion Nebula Cluster in the HO 1.4 m absorption band: III. The population of sub-stellar binary companions

Giovanni M. Strampelli, Jonathan Aguilar, Laurent Pueyo +4

We present new results concerning the sub-stellar binary population in the Orion Nebula Cluster (ONC). Using the Karhunen-Loève Image Projection (KLIP) algorithm, we have reprocess…

astro-ph.SR202022 cited

HST survey of the Orion Nebula Cluster in the HO 1.4 m absorption band: I. A census of substellar and planetary mass objects

Massimo Robberto, Mario Gennaro, Maria Giulia Ubeira Gabellini +15

In order to obtain a complete census of the stellar and sub-stellar population, down to a few M in the Myr old Orion Nebula Cluster, we used the infrared channel of…

astro-ph.SR2020

The not so simple stellar system Omega Cen. II. Evidence in support of a merging scenario

Annalisa Calamida, Alice Zocchi, Giuseppe Bono +7

We present multi-band photometry covering 5°across Cen collected with the Dark Energy Camera, combined to Hubble Space Telescope and Wide Field Imager data fo…

astro-ph.HE201840 cited

Nebular Spectroscopy of Kepler's Brightest Supernova

G. Dimitriadis, C. Rojas-Bravo, C. D. Kilpatrick +9

We present late-time (240-260 days after peak brightness) optical photometry and nebular (+236 and +264 days) spectroscopy of SN 2018oh, the brightest Type Ia supernova (SN I…

astro-ph.HE2018

K2 Observations of SN 2018oh Reveal a Two-Component Rising Light Curve for a Type Ia Supernova

G. Dimitriadis, R. J. Foley, A. Rest +145

We present an exquisite, 30-min cadence Kepler (K2) light curve of the Type Ia supernova (SN Ia) 2018oh (ASASSN-18bt), starting weeks before explosion, covering the moment of explo…