activity
20132024
most citedPESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects

361 citations · 1.1k across the 25 of their papers we have counts for

collaborators

26 papers

astro-ph.HE2024★ 1 cited

A Novel Optimal Transport-Based Approach for Interpolating Spectral Time Series: Paving the Way for Photometric Classification of Supernovae

M. Ramirez, G. Pignata, Francisco Förster +7

This paper introduces a novel method for creating spectral time series, which can be used for generating synthetic light curves for photometric classification but also for applicat…

astro-ph.HE2024

CSS161010: a luminous, fast blue optical transient with broad blueshifted hydrogen lines

Claudia P. Gutiérrez, Seppo Mattila, Peter Lundqvist +38

We present ultraviolet, optical and near-infrared photometric and optical spectroscopic observations of the luminous, fast blue optical transient (LFBOT), CSS161010:045834-081803 (…

astro-ph.CO2024

Modelling the impact of host galaxy dust on type Ia supernova distance measurements

B. Popovic, P. Wiseman, M. Sullivan +65

Type Ia Supernovae (SNe Ia) are a critical tool in measuring the accelerating expansion of the universe. Recent efforts to improve these standard candles have focused on incorporat…

astro-ph.IM2024★ 5 cited

Narrow absorption lines from intervening material in supernovae I. Measurements and temporal evolution

Santiago González-Gaitán, Claudia P. Gutiérrez, Joseph P. Anderson +6

Narrow absorption features in nearby supernova (SN) spectra are a powerful diagnostic of the slow-moving material in the line of sight: they are extensively used to infer dust exti…

astro-ph.GA2022★ 15 cited

A Sample of Dust Attenuation Laws for DES Supernova Host Galaxies

J. Duarte, S. González-Gaitán, A. Mourao +58

Type Ia supernovae (SNe Ia) are useful distance indicators in cosmology, provided their luminosity is standardized by applying empirical corrections based on light-curve properties…

astro-ph.HE2022★ 15 cited

Carnegie Supernova Project-II: Near-infrared spectral diversity and template of Type Ia Supernovae

Jing Lu, Eric Y. Hsiao, Mark M. Phillips +30

We present the largest and most homogeneous collection of near-infrared (NIR) spectra of Type Ia supernovae (SNe Ia): 339 spectra of 98 individual SNe obtained as part of the Carne…

astro-ph.SR2022★ 38 cited

Type II supernovae from the Carnegie Supernova Project-I. III. Understanding SN II diversity through correlations between physical and observed properties

L. Martinez, J. P. Anderson, M. C. Bersten +17

SNe II show great photometric and spectroscopic diversity which is attributed to the varied physical characteristics of their progenitor and explosion properties. In this study, th…

astro-ph.GA2021★ 11 cited

Aperture-corrected spectroscopic type Ia supernova host galaxy properties

Lluís Galbany, Mat Smith, Salvador Duarte Puertas +7

We use type Ia supernovae (SNe Ia) data obtained by the Sloan Digital Sky Survey-II Supernova Survey (SDSS-II/SNe) in combination with the publicly available SDSS DR16 fiber spectr…

astro-ph.SR2021★ 37 cited

Type II supernovae from the Carnegie Supernova Project-I. I. Bolometric light curves of 74 SNe II using uBgVriYJH photometry

L. Martinez, M. C. Bersten, J. P. Anderson +18

The present study is the first of a series of three papers where we characterise the type II supernovae (SNe~II) from the Carnegie Supernova Project-I to understand their diversity…

astro-ph.SR2021★ 71 cited

Type II supernovae from the Carnegie Supernova Project-I. II. Physical parameter distributions from hydrodynamical modelling

L. Martinez, M. C. Bersten, J. P. Anderson +18

Linking supernovae to their progenitors is a powerful method for furthering our understanding of the physical origin of their observed differences, while at the same time testing s…

astro-ph.HE2020★ 19 cited

Optical and Near-Infrared Observations of the Nearby Type Ia Supernova 2017cbv

Lingzhi Wang, Carlos Contreras, Maokai Hu +28

Supernova (SN) 2017cbv in NGC 5643 is one of a handful of type Ia supernovae (SNe~Ia) reported to have excess blue emission at early times. This paper presents extensive $BVRIYJHK_…

astro-ph.HE2020★ 24 cited

SN 2017ivv: two years of evolution of a transitional Type II supernova

C. P. Gutiérrez, A. Pastorello, A. Jerkstrand +39

We present the photometric and spectroscopic evolution of the Type II supernova (SN II) SN 2017ivv (also known as ASASSN-17qp). Located in an extremely faint galaxy (M ma…

astro-ph.SR2020★ 26 cited

Progenitor properties of type II supernovae: fitting to hydrodynamical models using Markov chain Monte Carlo methods

L. Martinez, M. C. Bersten, J. P. Anderson +3

The progenitor and explosion properties of type II supernovae (SNe II) are fundamental to understand the evolution of massive stars. Special interest has been given to the range of…

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.IM2019★ 24 cited

Tips and Tricks in linear imaging polarimetry of extended sources with FORS2 at the VLT

S. González-Gaitán, A. M. Mourão, F. Patat +5

Context: Polarimetry is a very powerful tool to uncover various properties of astronomical objects that remain otherwise hidden in standard imaging or spectroscopic observations. H…

astro-ph.SR2019★ 49 cited

On the Ca-strong 1991bg-like type Ia supernova 2016hnk: evidence for a Chandrasekhar-mass explosion

Lluís Galbany, Chris Ashall, Peter Hoeflich +46

We present a comprehensive dataset of optical and near-infrared photometry and spectroscopy of type~Ia supernova (SN) 2016hnk, combined with integral field spectroscopy (IFS) of it…

astro-ph.GA2018★ 9 cited

Elemental gas-phase abundances of intermediate redshift type Ia supernova star-forming host galaxies

M. E. Moreno-Raya, L. Galbany, A. R. López-Sánchez +4

The maximum luminosity of type Ia supernovae (SNe Ia) depends on the oxygen abundance of the regions of the host galaxies where they explode. This metallicity dependence reduces th…

astro-ph.HE2017★ 17 cited

Continuum Foreground Polarization and Na~I Absorption in Type Ia SNe

P. Zelaya, A. Clocchiatti, D. Baade +9

We present a study of the continuum polarization over the 400--600 nm range of 19 Type Ia SNe obtained with FORS at the VLT. We separate them in those that show Na I D lines at the…

astro-ph.HE2016★ 15 cited

Supernova 2010ev: A reddened high velocity gradient type Ia supernova

Claudia P. Gutiérrez, Santiago González-Gaitán, Gastón Folatelli +10

Aims. We present and study the spectroscopic and photometric evolution of the type Ia supernova (SN Ia) 2010ev. Methods. We obtain and analyze multi-band optical light curves and o…

astro-ph.HE2015★ 51 cited

A Hubble diagram from Type II Supernovae based solely on photometry: the Photometric-Colour Method

T. de Jaeger, S. González-Gaitán, J. P. Anderson +20

We present a Hubble diagram of type II supernovae using corrected magnitudes derived only from photometry, with no input of spectral information. We use a data set from the Carnegi…

astro-ph.HE2015

Searching for light echoes due to CSM in SN Ia spectra

Sebastián Marino, Santiago González-Gaitán, Francisco Förster +3

We present an analytical model for light echoes (LEs) coming from circumstellar material (CSM) around Type Ia Supernovae (SNe Ia). Using this model we find two spectral signatures…

astro-ph.SR2014★ 361 cited

PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects

S. J. Smartt, S. Valenti, M. Fraser +99

The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. We describe the data reduction str…

astro-ph.HE2014★ 33 cited

Defining Photometric Peculiar Type Ia Supernovae

S. Gonzalez-Gaitan, E. Y. Hsiao, G. Pignata +9

We present a new photometric identification technique for SN 1991bg-like type Ia supernovae (SNe Ia), i.e. objects with light-curve characteristics such as later primary maxima and…

astro-ph.HE2014★ 85 cited

Analysis of blue-shifted emission peaks in type II supernovae

J. P. Anderson, L. Dessart, C. P. Gutierrez +10

In classical P-Cygni profiles, theory predicts emission to peak at zero rest velocity. However, supernova spectra exhibit emission that is generally blue shifted. While this charac…