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X-shooter survey of disk accretion in Upper Scorpius - I. Very high accretion rates at age \>\; 5 Myr
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Band structures of GaAs, InAs, and InP: A 34 k⋅p model: Journal of Applied Physics: Vol 104, No 2
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X-shooter survey of disk accretion in Upper Scorpius - I. Very high accretion rates at age \>\; 5 Myr
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Band structures of GaAs, InAs, and InP: A 34 k⋅p model: Journal of Applied Physics: Vol 104, No 2
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X-shooter survey of disk accretion in Upper Scorpius - I. Very high accretion rates at age \>\; 5 Myr
![PDF] Interferometric and noise signatures of Majorana fermion edge states in transport experiments. | Semantic Scholar](https://d3i71xaburhd42.cloudfront.net/490a1a18594517025c10c111a95e6651d14cccaf/4-TableI-1.png "PDF] Interferometric and noise signatures of Majorana fermion edge states in transport experiments. | Semantic Scholar")
PDF] Interferometric and noise signatures of Majorana fermion edge states in transport experiments. | Semantic Scholar
X-shooter survey of disk accretion in Upper Scorpius - I. Very high accretion rates at age \>\; 5 Myr
Band structures of GaAs, InAs, and InP: A 34 k⋅p model: Journal of Applied Physics: Vol 104, No 2
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X-shooter survey of disk accretion in Upper Scorpius - I. Very high accretion rates at age \>\; 5 Myr
![PDF] Interferometric and noise signatures of Majorana fermion edge states in transport experiments. | Semantic Scholar](https://d3i71xaburhd42.cloudfront.net/490a1a18594517025c10c111a95e6651d14cccaf/3-Figure2-1.png "PDF] Interferometric and noise signatures of Majorana fermion edge states in transport experiments. | Semantic Scholar")
PDF] Interferometric and noise signatures of Majorana fermion edge states in transport experiments. | Semantic Scholar
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X-shooter survey of disk accretion in Upper Scorpius - I. Very high accretion rates at age \>\; 5 Myr
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IMPRS Solar System School News Archive | Max Planck Institute for Solar System Research
PDF) Modelling of electronic states in InAs/GaAs quantum dots with GaAsSb strain reducing overlayer
IMPRS Solar System School News Archive | Max Planck Institute for Solar System Research
