papers

Publications (25)

astro-ph.HE2022

The Absolute Magnitudes of 1991T-like Supernovae

M. M. Phillips, C. Ashall, Christopher R. Burns +20

1991T-like supernovae are the luminous, slow-declining extreme of the Branch shallow-silicon (SS) subclass of Type Ia supernovae. They are distinguished by extremely weak Ca II H &…

astro-ph.SR2021

The 2019 International Women's Day event: A two-step solar flare with multiple eruptive signatures and low Earth impact

Dumbovic, M., Veronig +15

We present a detailed analysis of an eruptive event that occurred on early 2019 March 8 in active region AR 12734, to which we refer as the International Women's day event. The eve…

astro-ph.EP2020

The CARMENES search for exoplanets around M dwarfs -- LP 714-47b (TOI 442.01): Populating the Neptune desert

S. Dreizler, I., J. +134

We report the discovery of a Neptune-like planet (LP 714-47 b, P = 4.05204 d, m_b = 30.8 +/- 1.5 M_earth , R_b = 4.7 +/- 0.3 R_earth ) located in the 'hot Neptune desert'. Confirma…

astro-ph.GA2019

Cold dust and stellar emissions in dust-rich galaxies observed with ALMA: a challenge for SED-fitting techniques

Buat, V., Ciesla +6

Over the past few years ALMA has detected dust-rich galaxies whose cold dust emission is spatially disconnected from the UV rest-frame emission. This represents a challenge for mod…

astro-ph.GA2019

Optical Spectroscopic Observations of Gamma-Ray Blazar Candidates. VII. Follow-up Campaign in the Southern Hemisphere

Peña-Herazo, H. A., Marchesini +29

Searching for low energy counterparts of gamma-ray sources is one of the major challenges in modern gamma-ray astronomy. In the third Fermi source catalog about 30 % of detected so…

astro-ph.IM2025

HAWC Performance Enhanced by Machine Learning in Gamma-Hadron Separation

R. Alfaro, C. Alvarez, A. Andrés +92

Improving gamma-hadron separation is one of the most effective ways to enhance the performance of ground-based gamma-ray observatories. With over a decade of continuous operation,…

astro-ph.GA2023

Morphology of star-forming clumps in ram-pressure stripped galaxies as seen by HST

Giunchi, E, Poggianti +18

We characterize the morphological properties of a statistically relevant sample of H and UV young star-forming clumps and optical complexes, observed with the \textit{Hubble Sp…

astro-ph.GA2019

Optical spectroscopic observations of gamma-ray blazar candidates VIII: the 2016-2017 follow up campaign carried out at SPM, NOT, KPNO and SOAR telescopes

Marchesini, E. J., Peña-Herazo +24

The third Fermi source catalog lists 3033 gamma-ray sources above significance. More than 30% are classified as either unidentified/unassociated Gamma-ray sources (UGSs), wit…

astro-ph.SR2018

Installation of Solar Chromospheric Telescope at the Indian Astronomical Observatory, Merak

Ravindra B, Prabhu Kesavan, Thulasidharen +13

We report the observations of the solar chromosphere from a newly commissioned solar telescope at the incursion site near Pangong Tso lake in Merak (Leh/Ladakh). This new H te…

nucl-ex2017

Half-lives of neutron-rich Cd

Dunlop, R., Bildstein +69

The -decay half-lives of Cd have been measured with the newly commissioned GRIFFIN -ray spectrometer at the TRIUMF-ISAC facility. The time structures of…

astro-ph.SR2010

Doppler images of the RS CVn binary II Pegasi during the years 1994-2002

Lindborg, M., Korpi +8

We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. The six maps from 1999-2002 are based on previously unpublished observation…

astro-ph.SR2017

Discovery of a Metal-poor, Luminous Post-AGB Star that Failed the Third Dredge-up

D. Kamath, H. Van Winckel, P. R. Wood +4

Post-asymptotic giant branch (post-AGB) stars are known to be chemically diverse. In this paper we present the first observational evidence of a star that has failed the third dred…

astro-ph.GA2023

Global kinematics study of OH masers in W49N

Mendoza-Torres, J. E., Juárez-Gama +3

Star formation is underway in the W49N molecular cloud (MC) at a high level of efficiency, with almost twenty ultra-compact (UC) HII regions observed thus far, indicating a recent…

astro-ph.SR2023

Beyond the disk: EUV coronagraphic observations of the Extreme Ultraviolet Imager on board Solar Orbiter

Auchère, F., Berghmans +58

Most observations of the solar corona beyond 2 Rs consist of broadband visible light imagery from coronagraphs. The associated diagnostics mainly consist of kinematics and derivati…

astro-ph.IM2010

Design, analysis, and testing of a microdot apodizer for the apodized pupil Lyot coronagraph (Research note). III. Application to extremely large telescopes

Martinez, P., Dorrer +7

The apodized-pupil Lyot coronagraph is one of the most advanced starlight cancellation concepts studied intensively in the past few years. Extreme adaptive optics instruments built…

physics.ao-ph2024

Tropical Pacific SST influence on seasonal streamflow variability in Ecuador

Quishpe-Vásquez, C., Gámiz-Fortis +7

This study presents a basin wide assessment about the spatio-temporal variability of streamflows in Ecuador for the period 1979-2015. The influence of the tropical Pacific sea surf…

math.PR2021

Diffusion approximation of controlled branching processes using limit theorems for random step processes

González, M., Martín-Chávez +3

A controlled branching process (CBP) is a modification of the standard Bienaymé-Galton-Watson process in which the number of progenitors in each generation is determined by a rand…

astro-ph.HE2017

EBL constraints with VERITAS gamma-ray observations

Fernandez Alonso, M.

The extragalactic background light (EBL) contains all the radiation emitted by nuclear and accretion processes since the epoch of recombination. Direct measurements of the EBL in t…

astro-ph.GA2010

UWISH2 -- The UKIRT Widefield Infrared Survey for H2

D., Froebrich, C. J. +56

We present the goals and preliminary results of an unbiased, near-infrared, narrow-band imaging survey of the First Galactic Quadrant (10deg<l<65deg ; -1.3deg<b<+1.3deg). This area…

astro-ph.SR2026

Orbital motion and dynamical mass of the complex periodic variable binary system 2MASS J05082729-2101444

S. Curiel, G. N. Ortiz-León, V. J. S. Béjar +22

We used very long baseline interferometry to constrain the orbit of the binary system 2MASS J05082729-2101444. We observed the system with the VLBA in three epochs at a frequency o…

cond-mat.str-el2012

Unusual temperature dependence of the spectral weight near the Fermi level of NdNiO3 thin films

E. F. Schwier, R. Scherwitzl, Z. Vydrova +7

We investigate the behavior of the spectral weight near the Fermi level of NdNiO3 thin films as a function of temperature across the metal-to-insulator transition (MIT) by means of…

physics.optics2019

Performance improvement of refractometric sensors through hybrid plasmonic-Fano resonances

Elshorbagy, M., Cuadrado +6

In this paper, we present a plasmonic refractometric sensor that works under normal incidence; allowing its integration on a fiber tip. The sensor's material and geometry exploit t…

astro-ph.SR2012

Characterizing Low-Mass Binaries From Observation of Long Time-scale Caustic-crossing Gravitational Microlensing Events

I. -G. Shin, C. Han, J. -Y. Choi +119

Despite astrophysical importance of binary star systems, detections are limited to those located in small ranges of separations, distances, and masses and thus it is necessary to u…

astro-ph.GA2019

Which attenuation curves for star-forming galaxies?

Buat, V., Corre +5

Dust attenuation shapes the spectral energy distributions of galaxies and any modelling and fitting procedure of their spectral energy distributions must account for this process.…

physics.flu-dyn2016

Unseeded Large Scale PIV measurements accounting for capillary-gravity waves phase speed

Benetazzo, A., Gamba +3

Large Scale Particle Image Velocimetry (LSPIV) is widely recognized as a reliable method to measure water surface velocity field in open channels and rivers. LSPIV technique is bas…