activity
20182022
most citedSN 2013aa and SN 2017cbv: Two Sibling Type Ia Supernovae in the spiral galaxy NGC 5643

37 citations · 70 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202213 cited

APEX at the QSO MUSEUM: molecular gas reservoirs associated with 3 quasars and their link to the extended Ly emission

N. Muñoz-Elgueta, F. Arrigoni Battaia, G. Kauffmann +5

Cool gas (T10~K) traced by hydrogen Ly emission is now routinely detected around quasars, but little is known about their molecular gas reservoirs. Here, we…

astro-ph.HE202120 cited

SN2017jgh - A high-cadence complete shock cooling lightcurve of a SN IIb with the Kepler telescope

P. Armstrong, B. E. Tucker, A. Rest +69

SN 2017jgh is a type IIb supernova discovered by Pan-STARRS during the C16/C17 campaigns of the Kepler/K2 mission. Here we present the Kepler/K2 and ground based observations of SN…

astro-ph.SR202037 cited

SN 2013aa and SN 2017cbv: Two Sibling Type Ia Supernovae in the spiral galaxy NGC 5643

Christopher R Burns, Chris Ashall, Carlos Contreras +26

We present photometric and spectroscopic observations of SN 2013aa and SN 2017cbv, two nearly identical type Ia supernovae (SNe Ia) in the host galaxy NGC 5643. The optical photome…

astro-ph.GA2019

Assessing the photometric redshift precision of the S-PLUS survey: the Stripe-82 as a test-case

A. Molino, M. V. Costa-Duarte, L. Sampedro +42

In this paper we present a thorough discussion about the photometric redshift (photo-z) performance of the Southern Photometric Local Universe Survey (S-PLUS). This survey combines…

astro-ph.GA2019

The Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies and redshifts with 12 optical filters

C. Mendes de Oliveira, T. Ribeiro, W. Schoenell +142

The Southern Photometric Local Universe Survey (S-PLUS) is imaging ~9300 deg^2 of the celestial sphere in twelve optical bands using a dedicated 0.8 m robotic telescope, the T80-So…

astro-ph.GA2018

Kinematics and physical properties of the nearby galaxy NGC 4656 and its TDG candidate

N. Muñoz-Elgueta, S. Torres-Flores, P. Amram +4

Interacting galaxies provide us with an excellent laboratory for studying a number of physical phenomena associated with these processes. In this paper, we present a spectroscopic…