| People | Locations | Statistics |
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| Naji, M. |
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| Motta, Antonella |
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| Aletan, Dirar |
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| Mohamed, Tarek |
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| Ertürk, Emre |
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| Taccardi, Nicola |
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| Kononenko, Denys |
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| Petrov, R. H. | Madrid |
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| Alshaaer, Mazen | Brussels |
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| Bih, L. |
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| Casati, R. |
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| Muller, Hermance |
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| Kočí, Jan | Prague |
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| Šuljagić, Marija |
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| Kalteremidou, Kalliopi-Artemi | Brussels |
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| Azam, Siraj |
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| Ospanova, Alyiya |
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| Blanpain, Bart |
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| Ali, M. A. |
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| Popa, V. |
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| Rančić, M. |
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| Ollier, Nadège |
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| Azevedo, Nuno Monteiro |
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| Landes, Michael |
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| Rignanese, Gian-Marco |
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Wang, Xin
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (21/21 displayed)
- 2024Interpenetrated and Bridged Nanocylinders from Self-Assembled Star Block Copolymerscitations
- 2024CEERS: 7.7 μm PAH Star Formation Rate Calibration with JWST MIRIcitations
- 2024From quinary Co–Cu–Mo–Pd–Re materials libraries to gas diffusion electrodes for Alkaline hydrogen evolutioncitations
- 2023Nanocellulose and PEDOT:PSS composites and their applicationscitations
- 2023Battery metals recycling by flash Joule heatingcitations
- 2023CEERS: 7.7 {mu}m PAH Star Formation Rate Calibration with JWST MIRI
- 2023CEERS: 7.7 ${mu}$m PAH Star Formation Rate Calibration with JWST MIRI
- 2022Nanocellulose and PEDOT:PSS composites and their applications
- 2022Durable, Lightweight, Washable and Comfortable Cooling Textiles from Nanodiamond/Polydopamine/Wool Nanocompositescitations
- 2022Analysis of Sensitivity of Distance between Embedded Ultrasonic Sensors and Signal Processing on Damage Detectability in Concrete Structurescitations
- 2021Modeling Optimal Laboratory Testing Strategies for Bacterial Meningitis Surveillance in Africa
- 2021The installation of embedded ultrasonic transducers inside a bridge to monitor temperature and load influence using coda wave interferometry techniquecitations
- 2020The Tajik Basin: A composite record of sedimentary basin evolution in response to tectonics in the Pamircitations
- 2019Anisotropic conductivity of Cellulose-PEDOT:PSS composite materials studied with a generic 3D four-point probe toolcitations
- 2019Unveiling the mechanisms of solid-state dewetting in Solid Oxide Cells with novel 2D electrodescitations
- 2018Processing ultrasonic data by coda wave interferometry to monitor load tests of concrete beams
- 2017Hybrid surface patterns mimicking the design of the adhesive toe pad of tree frog
- 2017Fast, wide‐field and distortion‐free telescope with curved detectors for surveys at ultralow surface brightnesscitations
- 2017Hybrid Surface Patterns Mimicking the Design of the Adhesive Toe Pad of Tree Frogcitations
- 2017Hybrid Surface Patterns Mimicking the Design of the Adhesive Toe Pad of Tree Frogcitations
- 2008Pulsed laser micromachining of yttria-stabilized zirconia dental ceramic for manufacturingcitations
Places of action
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document
CEERS: 7.7 {mu}m PAH Star Formation Rate Calibration with JWST MIRI
Abstract
We test the relationship between UV-derived star formation rates (SFRs) and the 7.7 m polycyclic aromatic hydrocarbon (PAH) luminosities from the integrated emission of galaxies at z ~ 0 - 2. We utilize multi-band photometry covering 0.2 - 160 m from HST, CFHT, JWST, Spitzer, and Herschel for galaxies in the Cosmic Evolution Early Release Science (CEERS) Survey. We perform spectral energy distribution (SED) modeling of these data to measure dust-corrected far-UV (FUV) luminosities, $L_{FUV}$, and UV-derived SFRs. We then fit SED models to the JWST/MIRI 7.7 - 21 m CEERS data to derive rest-frame 7.7 m luminosities, $L_{770}$, using the average flux density in the rest-frame MIRI F770W bandpass. We observe a correlation between $L_{770}$ and $L_{FUV}$, where log $L_{770}$ is proportional to (1.27+/-0.04) log $L_{FUV}$. $L_{770}$ diverges from this relation for galaxies at lower metallicities, lower dust obscuration, and for galaxies dominated by evolved stellar populations. We derive a "single-wavelength" SFR calibration for $L_{770}$ which has a scatter from model estimated SFRs (${_{SFR}}$) of 0.24 dex. We derive a "multi-wavelength" calibration for the linear combination of the observed FUV luminosity (uncorrected for dust) and the rest-frame 7.7 m luminosity, which has a scatter of ${_{SFR}}$ = 0.21 dex. The relatively small decrease insuggests this is near the systematic accuracy of the total SFRs using either calibration. These results demonstrate that the rest-frame 7.7 m emission constrained by JWST/MIRI is a tracer of the SFR for distant galaxies to this accuracy, provided the galaxies are dominated by star-formation with moderate-to-high levels of attenuation and metallicity....