L. Rodríguez-Muñoz

Advancing Rapid Response to Earthquakes with Tiered Physics-Based Ground-Shaking Simulations: The UrgentShake System

Elisa Zuccolo, Giorgio Bolzon, Fabio Pitari, L. Rodríguez-Muñoz et autres

Abstract The rapid response system currently in operation in northeastern Italy is based on the U.S. Geological Survey ShakeMap tool, which integrates ground-motion observations with selected ground-motion models (GMMs), similar to the systems used worldwide. To overcome the well-known limitations of conventional …

it (code pays fourni par la source)

High performance computing to support land, climate, and user‐oriented services: The HIGHLANDER Data Portal

Michele Bottazzi, L. Rodríguez-Muñoz, Beatrice Chiavarini, Cinzia Caroli et autres

Abstract The Italian territory is located at the heart of one of the global hot spots of climate change, where the implementation of climate‐smart land management practices is imperative to guarantee the present and future maintenance of ecosystem functions as well as …

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Emission Line Galaxies in the SHARDS Hubble Frontier Fields. II. Limits on Lyman-continuum Escape Fractions of Lensed Emission Line Galaxies at Redshifts 2 < z < 3.5

Alex Griffiths, Christopher J. Conselice, Leonardo Ferreira, Daniel Ceverino et autres

Abstract We present an investigation of escape fractions of UV photons from a unique sample of lensed low-mass emission line–selected galaxies at z < 3.5 found in the SHARDS Hubble Frontier Fields medium-band survey. We have used this deep imaging survey to …

gb, es, mx, us, it, cl (code pays fourni par la source)

Emission Line Galaxies in the SHARDS Hubble Frontier Fields II: Limits on Lyman-Continuum Escape Fractions of Lensed Emission Line Galaxies at Redshifts 2 < z < 3.5

Alex Griffiths, Christopher J. Conselice, Leonardo Ferreira, Daniel Ceverino et autres

We present an investigation on escape fractions of UV photons from a unique sample of lensed low-mass emission line selected galaxies at z < 3.5 found in the SHARDS Hubble Frontier Fields medium-band survey. We have used this deep imaging survey to …

Erratum: “Identification of Single Spectral Lines in Large Spectroscopic Surveys Using UMLAUT: an Unsupervised Machine-learning Algorithm Based on Unbiased Topology” (2021, ApJS, 257, 67)

Ivano Baronchelli, Claudia Scarlata, L. Rodríguez-Muñoz, Matteo Bonato et autres

Due to an error at the publisher two symbol errors were introduced. 1. In Section 3.1, in list item 1 “Data samples that are similar in a sufficiently large amount of independent dimensions (N=) tend to be similar also when considering an …

it, us, Afrique du Sud, cl, ch, fr, au, cn, gb (code pays fourni par la source)

Ultraviolet to far infrared self-consistent analysis of the stellar populations of massive starburst galaxies at intermediate redshifts

Néstor Espino-Briones, Pablo G. Pérez‐González, J. Zamorano, L. Rodríguez-Muñoz

ABSTRACT We study in detail the properties of the stellar populations of 111 massive [log (M⋆/M⊙) ≥ 10] dusty [far-infrared (FIR)-selected] starburst (SFR/SFRMS > 2) galaxies at 0.7 < z < 1.2. For that purpose, we use self-consistent methods that analyse the …

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Differential attenuation in star-forming galaxies at 0.3 ≲ z ≲ 1.5 in the SHARDS/CANDELS field

L. Rodríguez-Muñoz, G. Rodighiero, Pablo G. Pérez‐González, M. Talia et autres

ABSTRACT We use a sample of 706 galaxies, selected as [O ii]λ3727 ([O ii]) emitters in the Survey for High-z Absorption Red and Dead Sources (SHARDS) on the CANDELS/GOODS-N field, to study the differential attenuation of the nebular emission with respect to …

it, es, gb, fr, cl, nl, us (code pays fourni par la source)

Differential attenuation in star-forming galaxies at 0.3 $\lesssim$ $z$ $\lesssim$ 1.5 in the SHARDS/CANDELS field

L. Rodríguez-Muñoz, G. Rodighiero, Pablo G. Pérez‐González, M. Talia et autres

We use a sample of 706 galaxies, selected as [OII]$λ$3727 ([OII]) emitters in the Survey for High-$z$ Absorption Red and Dead Sources (SHARDS) on the CANDELS/GOODS-N field, to study the differential attenuation of the nebular emission with respect to the stellar continuum. …

Identification of Single Spectral Lines in Large Spectroscopic Surveys Using UMLAUT: an Unsupervised Machine-learning Algorithm Based on Unbiased Topology

Ivano Baronchelli, Claudia Scarlata, L. Rodríguez-Muñoz, Matteo Bonato et autres

Abstract The identification of an emission line is unambiguous when multiple spectral features are clearly visible in the same spectrum. However, in many cases, only one line is detected, making it difficult to correctly determine the redshift. We developed a freely available …

it, us, Afrique du Sud, cl, ch, au, cn, gb (code pays fourni par la source)

Identification of Single Spectral Lines through Supervised Machine Learning in a Large HST Survey (WISP): A Pilot Study for Euclid and WFIRST

Ivano Baronchelli, Claudia Scarlata, L. Rodríguez-Muñoz, Matteo Bonato et autres

Abstract Future surveys focusing on understanding the nature of dark energy (e.g., Euclid and WFIRST) will cover large fractions of the extragalactic sky in near-IR slitless spectroscopy. These surveys will detect a large number of galaxies that will have only one emission …

it, us, fr, de, cn, gb (code pays fourni par la source)

A panchromatic spatially resolved analysis of nearby galaxies – II. The main sequence – gas relation at sub-kpc scale in grand-design spirals

L. Morselli, G. Rodighiero, A Enia, E. Corbelli et autres

ABSTRACT In this work, we analyse the connection between gas availability and the position of a region with respect to the spatially resolved main-sequence (MS) relation. Following the procedure presented in Enia et al. (2020), for a sample of five face-on, grand …

it, us, gb, de (code pays fourni par la source)

The ALPINE−ALMA [C ii ] Survey: on the nature of an extremely obscured serendipitous galaxy

Michael Romano, P. Cassata, L. Morselli, B. C. Lemaux et autres

ABSTRACT We report the serendipitous discovery of a dust-obscured galaxy observed as part of the Atacama Large Millimeter Array (ALMA) Large Program to INvestigate [C ii] at Early times (ALPINE). While this galaxy is detected both in line and continuum emissions in …

it, us, fr, dk, ch, jp, cl, gb, de, nl (code pays fourni par la source)