activity
19962019
most citedBVRI Light Curves for 22 Type Ia Supernovae

758 citations · 3k across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.HE2019★ 25 cited

Luminous Type II supernovae for their low expansion velocities

Ó. Rodríguez, G. Pignata, J. P. Anderson +27

We present optical and near-IR data of three Type II supernovae (SNe II), SN 2008bm, SN 2009aj, and SN 2009au. These SNe display the following common characteristics: signs of earl…

astro-ph2008★ 32 cited

The CHilean Automatic Supernova sEarch (CHASE)

G. Pignata, J. Maza, M. Hamuy +16

The CHASE project started in 2007 with the aim of providing young southern supernovae (SNe) to the Carnegie Supernova Project (CSP) and Millennium Center for Supernova Studies (MCS…

astro-ph2008★ 96 cited

Optical and IR observations of SN 2002dj: some possible common properties of fast expanding SNe Ia

G. Pignata, S. Benetti, P. A. Mazzali +17

As part of the European Supernova Collaboration we obtained extensive photometry and spectroscopy of the type Ia SN 2002dj covering epochs from 11 days before to nearly two years a…

astro-ph2008★ 53 cited

Galaxy Clusters in the Line of Sight to Background Quasars: I. Survey Design and Incidence of MgII Absorbers at Cluster Redshifts

S. Lopez, L. F. Barrientos, P. Lira +7

We describe the first optical survey of absorption systems associated with galaxy clusters at z= 0.3-0.9. We have cross-correlated SDSS DR3 quasars with high-redshift cluster/group…

astro-ph2006★ 47 cited

Tomography of the intergalactic medium with Ly-alpha forests in close QSO pairs

V. D'Odorico, M. Viel, F. Saitta +6

We study the three-dimensional distribution of non virialised matter at z~2 using high resolution spectra of QSO pairs and simulated spectra drawn from cosmological hydrodynamical…

astro-ph2006★ 189 cited

The Physical Nature of Lyman Alpha Emitting Galaxies at z=3.1

Eric Gawiser, Pieter G. van Dokkum, Caryl Gronwall +20

We selected 40 candidate Lyman Alpha Emitting galaxies (LAEs) at z ~=3.1 with observed frame equivalent widths >150A and inferred emission line fluxes >2.5x10^-17 ergs/cm^2/s from…