19 results
Part II - SFR Measurements
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- Star-Formation Rates of Galaxies
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Part I - Background
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List of Figures
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List of Tables
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Preface
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Contents
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Index
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Frontmatter
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Star-Formation Rates of Galaxies
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List of Contributors
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Properties of LBGs with [OIII] detection at z > 3: The importance of including nebular emission data in SED fitting
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- Proceedings of the International Astronomical Union / Volume 15 / Issue S341 / November 2019
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- 10 June 2020, pp. 201-205
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- November 2019
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DEIMOS and MOSFIRE spectroscopy of star-forming galaxies in the AKARI NEP-Deep field
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- Proceedings of the International Astronomical Union / Volume 15 / Issue S341 / November 2019
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- 10 June 2020, pp. 279-280
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- November 2019
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HELP project - a dreamed-of multiwavelength dataset for SED fitting: The influence of used models for the main physical properties of galaxies
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- Proceedings of the International Astronomical Union / Volume 15 / Issue S341 / November 2019
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- 10 June 2020, pp. 39-43
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- November 2019
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Which attenuation curves for star-forming galaxies?
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- Proceedings of the International Astronomical Union / Volume 15 / Issue S341 / November 2019
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- 10 June 2020, pp. 70-73
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- November 2019
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Mass–metallicity relation for AKARI-FMOS infrared luminous galaxies at z ~ 0.9
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- Proceedings of the International Astronomical Union / Volume 11 / Issue S315 / August 2015
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- 12 September 2016, E60
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- August 2015
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Gas and attenuation in galaxies
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- Proceedings of the International Astronomical Union / Volume 8 / Issue S292 / August 2012
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- 21 March 2013, p. 283
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- August 2012
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Fitting the full SED of galaxies to put constraints on dust attenuation and star formation determinations
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- Proceedings of the International Astronomical Union / Volume 7 / Issue S284 / September 2011
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- 17 August 2012, pp. 297-300
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- September 2011
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AKARI/IRC broadband mid-infrared data as an indicator of the Star Formation Rate
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- Proceedings of the International Astronomical Union / Volume 7 / Issue S284 / September 2011
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- 17 August 2012, pp. 357-359
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- September 2011
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HerMES: Lyman Break Galaxies Individually Detected at 0.7 ≤ z ≤ 2.0 in GOODS-N with Herschel/SPIRE
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- Proceedings of the International Astronomical Union / Volume 6 / Issue S277 / December 2010
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- 05 December 2011, pp. 313-316
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- December 2010
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