Search Results - "E, F. Olivares"
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ASASSN-15lh: A highly super-luminous supernova
Published in Science (American Association for the Advancement of Science) (15-01-2016)“…We report the discovery of ASASSN-15lh (SN 2015L), which we interpret as the most luminous supernova yet found. At redshift z = 0.2326, ASASSN-15lh reached an…”
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Investigating the properties of stripped-envelope supernovae; what are the implications for their progenitors?
Published in Monthly notices of the Royal Astronomical Society (2019)“…ABSTRACT We present observations and analysis of 18 stripped-envelope supernovae observed during 2013–2018. This sample consists of five H/He-rich SNe, six…”
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Type II supernovae in low-luminosity host galaxies
Published in Monthly notices of the Royal Astronomical Society (21-09-2018)“…We present an analysis of a new sample of type II core-collapse supernovae (SNe II) occurring within low-luminosity galaxies, comparing these with a sample of…”
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Signatures of an eruptive phase before the explosion of the peculiar core-collapse SN 2013gc
Published in Monthly notices of the Royal Astronomical Society (01-01-2019)Get full text
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SN 2011hs: a fast and faint Type IIb supernova from a supergiant progenitor
Published in Monthly notices of the Royal Astronomical Society (01-04-2014)“…Observations spanning a large wavelength range, from X-ray to radio, of the Type IIb supernova (SN) 2011hs are presented, covering its evolution during the…”
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Unraveling the link between Type II supernova luminosity and host galaxy velocity dispersion
Published in Astronomische Nachrichten (01-07-2024)“…Abstract Type II supernovae (SNe II) have emerged as valuable cosmological probes, serving as alternative and independent tools to Type Ia supernova (SN Ia)…”
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The delay of shock breakout due to circumstellar material evident in most type II supernovae
Published in Nature astronomy (01-10-2018)“…Type II supernovae (SNe II) originate from the explosion of hydrogen-rich supergiant massive stars. Their first electromagnetic signature is the shock breakout…”
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A HUBBLE DIAGRAM FROM TYPE II SUPERNOVAE BASED SOLELY ON PHOTOMETRY: THE PHOTOMETRIC COLOR METHOD
Published in The Astrophysical journal (20-12-2015)“…We present a Hubble diagram of SNe II using corrected magnitudes derived only from photometry, with no input of spectral information. We use a data set from…”
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PS15cey and PS17cke: prospective candidates from the Pan-STARRS Search for kilonovae
Published in Monthly notices of the Royal Astronomical Society (01-01-2021)“…ABSTRACT Time domain astronomy was revolutionized with the discovery of the first kilonova, AT2017gfo, in August 2017, which was associated with the…”
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LSQ14efd: observations of the cooling of a shock break-out event in a type Ic Supernova
Published in Monthly notices of the Royal Astronomical Society (01-10-2017)“…We present the photometric and spectroscopic evolution of the type Ic supernova LSQ14efd, discovered by the La Silla QUEST survey and followed by PESSTO…”
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GRB 171010A/SN 2017htp: a GRB-SN at z = 0.33
Published in Monthly notices of the Royal Astronomical Society (21-12-2019)“…ABSTRACT The number of supernovae known to be connected with long-duration gamma-ray bursts (GRBs) is increasing and the link between these events is no longer…”
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A Very Metal-poor Damped Lyman-α System Revealed Through the Most Energetic GRB 090926A
Published in The Astrophysical journal (01-09-2010)Get full text
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Astronomy. ASASSN-15lh: A highly super-luminous supernova
Published in Science (American Association for the Advancement of Science) (15-01-2016)“…We report the discovery of ASASSN-15lh (SN 2015L), which we interpret as the most luminous supernova yet found. At redshift z = 0.2326, ASASSN-15lh reached an…”
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A PHOTOMETRIC REDSHIFT OF z ∼ 9.4 FOR GRB 090429B
Published in The Astrophysical journal (20-07-2011)“…Gamma-ray bursts (GRBs) serve as powerful probes of the early universe, with their luminous afterglows revealing the locations and physical properties of…”
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Pan-STARRS and PESSTO search for an optical counterpart to the LIGO gravitational-wave source GW150914
Published in Monthly notices of the Royal Astronomical Society (11-11-2016)“…We searched for an optical counterpart to the first gravitational-wave source discovered by LIGO (GW150914), using a combination of the Pan-STARRS1 wide-field…”
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Supersolar metal abundances in two galaxies at z 3.57 revealed by the GRB090323 afterglow spectrum
Published in Monthly notices of the Royal Astronomical Society (01-02-2012)“…ABSTRACT We report on the surprisingly high metallicity measured in two absorption systems at high redshift, detected in the Very Large Telescope spectrum of…”
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Designing an Optimal Kilonova Search Using DECam for Gravitational-wave Events
Published in The Astrophysical journal (01-01-2024)“…Abstract We address the problem of optimally identifying all kilonovae detected via gravitational-wave emission in the upcoming LIGO/Virgo/KAGRA observing run,…”
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Supersolar metal abundances in two galaxies at z similar to 3.57 revealed by the GRB090323 afterglow spectrum
Published in Monthly notices of the Royal Astronomical Society (11-02-2012)“…We report on the surprisingly high metallicity measured in two absorption systems at high redshift, detected in the Very Large Telescope spectrum of the…”
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ILLUMINATING THE DARKEST GAMMA-RAY BURSTS WITH RADIO OBSERVATIONS
Published in The Astrophysical journal (20-04-2013)“…We present X-ray, optical, near-infrared (IR), and radio observations of gamma-ray bursts (GRBs) 110709B and 111215 A, as well as optical and near-IR…”
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Author Correction: The delay of shock breakout due to circumstellar material evident in most type II supernovae
Published in Nature astronomy (2019)“…In the version of this Article originally published, the authors Pablo Huijse and Pablo Huentelemu were mistakenly affiliated with the University of…”
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