Global Far-Ultraviolet (912-1800 Å) Properties of Star-forming Galaxies

By C. Leitherer, I. Li, D. Calzetti, T. Heckman. 2002

138 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/a5b18a97df1fefec517bc9403c3538900c5618d7

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In Astronomy and Astrophysics

Citations in the corpus

BULGE AND CLUMP EVOLUTION IN HUBBLE ULTRA DEEP FIELD CLUMP CLUSTERS, CHAINS AND SPIRAL GALAXIES (2008, methodology): “Dust absorption was included as a third parameter of the fit using the wavelength dependence in Calzetti et al. (2000) with the short-wavelength modification in Leitherer et al. (2002), and using discrete multiples of MA times the redshift dependence for galaxy intrinsic AV in Rowan-Robinson (2003).”
Stellar Populations in 10 Clump-Cluster Galaxies of the Hubble Ultra Deep Field (2005, methodology): “Dust absorption was included using the wavelength dependence in Calzetti et al. (2000) with the short-wavelength modification in Leitherer et al. (2002) and the redshift dependence for galaxy intrinsic AV extinction in Rowan-Robinson (2003).”
Analysis of galaxy spectral energy distributions from far-UV to far-IR with CIGALE: studying a SINGS test sample (2009, methodology): “…1200 Å, for which the Calzetti law is not defined, we linearly extrapolate by using the value and slope at 1200 Å. Thisapproach, which resembles the method of Bolzonella et al. (2000), avoids extreme slopes at low wavelengths that are not supported by observations (Leitherer et al. 2002).”
OBSERVATIONS OF STARBURST GALAXIES WITH FAR-ULTRAVIOLET SPECTROGRAPHIC EXPLORER: GALACTIC FEEDBACK IN THE LOCAL UNIVERSE (2009, background): “Hopkins Ultraviolet Telescope (HUT) observations of star-forming galaxies analyzed by Leitherer et al. (2002) probed the 912 Å–1800 Å regime but with very low spectral resolution.”
CIGALE: a python Code Investigating GALaxy Emission (2018, unknown): “It is based on the Calzetti et al. (2000) starburst attenuation curve, extended with the Leitherer et al. (2002) curve between the Lyman break and 150 nm.”
Dust Attenuation Curves in the Local Universe: Demographics and New Laws for Star-forming Galaxies and High-redshift Analogs (2018, methodology): “5 For the far-UV region (912-1500 Å), the Calzetti curve (defined at λ > 1200 Å) is substituted with the curve from Leitherer et al. (2002).”
GOODS-Herschel: dust attenuation properties of UV selected high redshift galaxies (2012, background): “We start at 1300 Å to avoid the flattening of the UV continuum at shorter wavelengths, down to 1200 Å (Leitherer et al., 2002; Buat et al., 2002). β is calculated in two ways, with and without data corresponding to the wavelength of the UV bump, and both estimates are found to be very similar.”
EXTREME FEEDBACK AND THE EPOCH OF REIONIZATION: CLUES IN THE LOCAL UNIVERSE (2011, background): “For a normal starburst or SMC dust attenuation law (Calzetti 2001; Leitherer et al, 2002) these SEDs imply roughly two magnitudes of dust extinction along the line-of- sight to the DCO in the far-UV.”
x-cigale: fitting AGN/galaxy SEDs from X-ray to infrared (2020, methodology): “For the galactic dust attenuation, we adopt the dustatt calzleit module in X-CIGALE (Calzetti et al. 2000; Leitherer et al. 2002).”
Observations of Thick Disks in the Hubble Space Telescope Ultra Deep Field (2006, background): “…using the star formation rate as a weighting factor, diminished by absorption from Hα lines (Madau 1995) and dust (RowanRobinson 2003; Calzetti et al. 2000; Leitherer et al. 2002), and then integrated over the ACS filter functions to get the intensity in each filter per unit solar mass of stars.”
New insights into the stellar content and physical conditions of star-forming galaxies at z = 2-3 from spectral modelling (2008, background): “1; such models would be able to reproduce the observations of He II λ1640 in individual star-forming galaxies at low (e.g. González Delgado et al. 1999; Leitherer et al. 2002; Chandar, Leitherer & Tremonti 2004), as well as high (e.g. Lowenthal et al. 1997; Kobulnicky & Koo 2000), redshifts.”