2020
DOI: 10.48550/arxiv.2009.00617
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CLEAR: Paschen-$β$ Star Formation Rates and Dust Attenuation of Low Redshift Galaxies

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Cited by 6 publications
(9 citation statements)
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“…Previous work on the metallicities, ages, and formation histories of massive galaxies at 1 < z < 2 has been published in Estrada-Carpenter et al (2019, and the gas-phase metallicity gradients of star-forming galaxies is investigated in Simons et al (2020). Also, Cleri et al (2020) studied Paschen-β as a star-formation rate indicator in low redshift galaxies, using the CLEAR dataset.…”
Section: Clear Hst/grism Surveymentioning
confidence: 99%
“…Previous work on the metallicities, ages, and formation histories of massive galaxies at 1 < z < 2 has been published in Estrada-Carpenter et al (2019, and the gas-phase metallicity gradients of star-forming galaxies is investigated in Simons et al (2020). Also, Cleri et al (2020) studied Paschen-β as a star-formation rate indicator in low redshift galaxies, using the CLEAR dataset.…”
Section: Clear Hst/grism Surveymentioning
confidence: 99%
“…Morelli et al (2020) probed that the index behaviour in the cool IRTF stars is driven by temperature, with no trends with surface gravity and metallicity. Cleri et al (2020) showed that the Paβ index could adopted as a tracer of the star formation rate in galaxies, showing a similar (and somewhat even better) behaviour with respect to the Hα and Hβ indicators. This supports our findings (Fig.…”
Section: Trends With the Metal Indicesmentioning
confidence: 76%
“…Observational constraints on the degree to which stars and dust are spatially coupled are difficult to obtain but recent work by Leslie et al (2018) and van der Giessen et al (2022) using the Tuffs et al (2004) model show that galaxies in both SDSS and COSMOS exhibit significant 'clumpiness' fractions, such that young stars are heavily attenuated and the overall attenuation curves are shaped by this non-uniformity in dust geometry. Paβ and Hα emission line ratios, which can be used to infer dust attenuation, have been shown to lie outside the expected relation when measured in resolved galaxies with prominent dust lanes, as demonstrated in Cleri et al (2020), indicating the need to accommodate the star-dust geometry in dust attenuation measurements.…”
Section: Understanding Variations In Dust Attenuation Curvesmentioning
confidence: 96%
“…Correlations have been found between attenuation curve shape and galaxy physical properties like stellar mass and star formation activity (e.g. Noll et al 2007Noll et al , 2009aSalim et al 2016;Battisti et al 2016Battisti et al , 2017aCorre et al 2018;Salim et al 2018;Reddy et al 2018;Cleri et al 2020;Bogdanoska & Burgarella 2020), galaxy spectral type (e.g. Kriek & Conroy 2013), morphology and observed inclination angle (e.g.…”
Section: Introductionmentioning
confidence: 99%