Browsing by Author "Guerrero, Andrea"

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    Age as Risk Factor for Death from Pandemic (H1N1) 2009, Chile
    (CENTERS DISEASE CONTROL, 2011) Dabanch, Jeannette; Perret, Cecilia; Najera, Manuel; Gonzalez, Claudia; Guerrero, Andrea; Olea, Andrea; Fasce, Rodrigo; Morales, Cecilia; Vega, Jeanette; Advisory Comm Chilean Minist Hlth
    Pandemic (H1N1) 2009 affected Chile during the winter of 2009. The hospitalization rate was 0.56% overall and 3.47% for persons >= 60 years of age at risk for severe disease and death independent of concurrent conditions. Age >= 60 years was the major risk factor for death from pandemic (H1N1) 2009.
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    ALMA Lensing Cluster Survey: average dust, gas, and star-formation properties of cluster and field galaxies from stacking analysis
    (2023) Guerrero, Andrea; Nagar, Neil; Kohno, Kotaro; Fujimoto, Seiji; Kokorev, Vasily; Brammer, Gabriel; Jolly, Jean-Baptiste; Knudsen, Kirsten; Sun, Fengwu; Bauer, Franz E.; Caminha, Gabriel B.; Caputi, Karina; Neumann, Gerald; Orellana-Gonzalez, Gustavo; Cerulo, Pierluigi; Gonzalez-Lopez, Jorge; Laporte, Nicolas; Koekemoer, Anton M.; Ao, Yiping; Espada, Daniel; Arancibia, Alejandra M. Munoz
    We develop new tools for continuum and spectral stacking of Atacama Large Millimeter/submillimeter Array (ALMA) data, and apply these to the ALMA Lensing Cluster Survey. We derive average dust masses, gas masses, and star-formation rates (SFRs) from the stacked observed 260-GHz continuum of 3402 individually undetected star-forming galaxies, of which 1450 are cluster galaxies and 1952 field galaxies, over three redshift and stellar mass bins (over z = 0-1.6 and log M-*[M-circle dot] = 8-11.7), and derive the average molecular gas content by stacking the emission line spectra in a SFR-selected subsample. The average SFRs and specific SFRs of both cluster and field galaxies are lower than those expected for main-sequence (MS) star-forming galaxies, and only galaxies with stellar mass of log M-*[M-circle dot] = 9.35-10.6 show dust and gas fractions comparable with those in the MS. The ALMA-traced average 'highly obscured' SFRs are typically lower than the SFRs observed from optical to near-infrared spectral analysis. Cluster and field galaxies show similar trends in their contents of dust and gas, even when field galaxies were brighter in the stacked maps. From spectral stacking we find a potential CO (J = 4 -> 3) line emission (signal-to-noise ratio being similar to 4) when stacking cluster and field galaxies with the highest SFRs.
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    Seroprevalence study of infection with influenza A (H1N1)pdm09 virus in San Felipe Town, Chile
    (2013) Olea, Andrea; Fasce, Rodrigo; Aguilera, Ximena; Oliva, Otavio; Muñoz, Sergio; García, Maritza; Pedroni, Elena; Nájera, Manuel; Cerda, Jaime; Abarca Villaseca, Katia; Guerrero, Andrea; Bustos, Patricia; Mora, Judith; Vega, Jeanette; Mccarron, Meg; Widdowson, Marc-Alain; Castillo, E. R.