scholarly journals Infrared Spectral Energy Distributions ofz∼ 0.7 Star‐forming Galaxies

2007 ◽  
Vol 670 (1) ◽  
pp. 301-312 ◽  
Author(s):  
Xian Zhong Zheng ◽  
Herve Dole ◽  
Eric F. Bell ◽  
Emeric Le Floc’h ◽  
George H. Rieke ◽  
...  
Keyword(s):  
Spectral Energy ◽  
Spectral Energy Distributions ◽  
Energy Distributions ◽  
Star Forming ◽  
Infrared Spectral

scholarly journals The Far‐Infrared Spectral Energy Distributions of X‐Ray–selected Active Galaxies

2003 ◽  
Vol 590 (1) ◽  
pp. 128-148 ◽  
Author(s):  
Joanna K. Kuraszkiewicz ◽  
Belinda J. Wilkes ◽  
Eric ◽  
J. Hooper ◽  
Kim K. McLeod ◽  
...  
Keyword(s):  
Far Infrared ◽  
Active Galaxies ◽  
Spectral Energy ◽  
Spectral Energy Distributions ◽  
Energy Distributions ◽  
X Ray ◽  
Infrared Spectral

scholarly journals WELL-SAMPLED FAR-INFRARED SPECTRAL ENERGY DISTRIBUTIONS OFz∼ 2 GALAXIES: EVIDENCE FOR SCALED UP COOL GALAXIES

2010 ◽  
Vol 725 (1) ◽  
pp. 742-749 ◽  
Author(s):  
Adam Muzzin ◽  
Pieter van Dokkum ◽  
Mariska Kriek ◽  
Ivo Labbé ◽  
Iara Cury ◽  
...  
Keyword(s):  
Far Infrared ◽  
Spectral Energy ◽  
Spectral Energy Distributions ◽  
Energy Distributions ◽  
Infrared Spectral

scholarly journals Which attenuation curves for star-forming galaxies?

2019 ◽  
Vol 15 (S341) ◽  
pp. 70-73
Author(s):  
Véronique Buat ◽  
David Corre ◽  
Médéric Boquien ◽  
Katarzyna Małek
Keyword(s):  
Radiative Transfer ◽  
Spectral Energy ◽  
Spectral Energy Distributions ◽  
Energy Distributions ◽  
Star Forming ◽  
Radiative Transfer Models ◽  
Attenuation Law ◽  
Dust Attenuation ◽  
Attenuation Laws ◽  
Transfer Models

AbstractDust attenuation shapes the spectral energy distributions of galaxies and any modelling and fitting procedure of their spectral energy distributions must account for this process. We present results of two recent works dedicated at measuring the dust attenuation curves in star forming galaxies at redshift from 0.5 to 3, by fitting continuum (photometric) and line (spectroscopic) measurements simultaneously with CIGALE using variable attenuation laws based on flexible recipes. Both studies conclude to a large variety of effective attenuation laws with an attenuation law flattening when the obscuration increases. An extra attenuation is found for nebular lines. The comparison with radiative transfer models implies a flattening of the attenuation law up to near infrared wavelengths, which is well reproduced with a power-laws recipe inspired by the Charlot and Fall recipe. Here we propose a global modification of the Calzetti attenuation law to better reproduce the results of radiative transfer models.

scholarly journals WHAT SHAPES THE FAR-INFRARED SPECTRAL ENERGY DISTRIBUTIONS OF GALAXIES?

2016 ◽  
Vol 818 (1) ◽  
pp. 62 ◽  
Author(s):  
Mohammadtaher Safarzadeh ◽  
Christopher C. Hayward ◽  
Henry C. Ferguson ◽  
Rachel S. Somerville
Keyword(s):  
Far Infrared ◽  
Spectral Energy ◽  
Spectral Energy Distributions ◽  
Energy Distributions ◽  
Infrared Spectral

scholarly journals Ultraviolet through Infrared Spectral Energy Distributions from 1000 SDSS Galaxies: Dust Attenuation

2007 ◽  
Vol 173 (2) ◽  
pp. 392-403 ◽  
Author(s):  
Benjamin D. Johnson ◽  
David Schiminovich ◽  
Mark Seibert ◽  
Marie Treyer ◽  
D. Christopher Martin ◽  
...  
Keyword(s):  
Spectral Energy ◽  
Spectral Energy Distributions ◽  
Energy Distributions ◽  
Infrared Spectral ◽  
Dust Attenuation

scholarly journals The Ages of Elliptical Galaxies from Infrared Spectral Energy Distributions

2006 ◽  
Vol 647 (1) ◽  
pp. 265-275 ◽  
Author(s):  
Joel N. Bregman ◽  
Pasquale Temi ◽  
Jesse D. Bregman
Keyword(s):  
Elliptical Galaxies ◽  
Spectral Energy ◽  
Spectral Energy Distributions ◽  
Energy Distributions ◽  
Infrared Spectral
Sign in / Sign up

Export Citation Format

Share Document