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Background and Environment Affect Phenotype02:27

Background and Environment Affect Phenotype

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Although the genetic makeup of an organism plays a major role in determining the phenotype, there are also several environmental factors, such as temperature, oxygen availability, presence of mutagens, that can alter an organism’s phenotype.
An example of how genetic background affects phenotype can be seen in horses. The Extension gene in horses is responsible for their coat color. A wild-type gene (EE) produces black pigment in the coat, while a mutant gene (ee) produces red pigment. A...
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Difference from Background: Limit of Detection01:05

Difference from Background: Limit of Detection

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The limit of detection (LOD) is the smallest amount of analyte that can be distinguished from the background noise. The LOD value corresponds to the concentration at which the analyte signal is three times larger than the standard deviation of the blank signal. Below this value, the analyte signal cannot be differentiated from the background noise. It is calculated by dividing the calibration slope by 3 times the standard deviation of the blank signals.
The LOD indicates the presence or absence...
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The Electromagnetic Spectrum02:37

The Electromagnetic Spectrum

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The electromagnetic spectrum consists of all the types of electromagnetic radiation arranged according to their frequency and wavelength. Each of the various colors of visible light has specific frequencies and wavelengths associated with them, and you can see that visible light makes up only a small portion of the electromagnetic spectrum. Because the technologies developed to work in various parts of the electromagnetic spectrum are different, for reasons of convenience and historical...
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The Wave Nature of Light02:12

The Wave Nature of Light

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The nature of light has been a subject of inquiry since antiquity. In the seventeenth century, Isaac Newton performed experiments with lenses and prisms and was able to demonstrate that white light consists of the individual colors of the rainbow combined together. Newton explained his optics findings in terms of a "corpuscular" view of light, in which light was composed of streams of extremely tiny particles traveling at high speeds according to Newton's laws of motion.
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Cross-Sectional Research01:50

Cross-Sectional Research

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In cross-sectional research, a researcher compares multiple segments of the population at the same time. If they were interested in people's dietary habits, the researcher might directly compare different groups of people by age. Instead of following a group of people for 20 years to see how their dietary habits changed from decade to decade, the researcher would study a group of 20-year-old individuals and compare them to a group of 30-year-old individuals and a group of 40-year-old...
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Groupthink01:34

Groupthink

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When in group settings, we are often influenced by the thoughts, feelings, and behaviors around us. Groupthink is another phenomenon of conformity where modification of the opinions of members in a group aligns with what they believe is the group consensus (Janis, 1972). In such situations, the group often takes action that individuals would not perform outside the group setting because groups make more extreme decisions than individuals do. Moreover, groupthink can hinder opposing trains of...
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Video Experimental Relacionado

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Time-Resolved Fluorescence Anisotropy from Single Molecules for Characterizing Local Flexibility in Biomolecules
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Anisotropía del fondo cósmico de microondas

Nick Kaiser, Joseph Silk

    Nature
    |March 9, 2018
    PubMed
    Resumen
    Este resumen es generado por máquina.

    Los científicos están cerca de medir las anisotropías de la radiación de fondo cósmica de microondas, lo que podría confirmar las teorías sobre la estructura del universo o requerir revisiones a los modelos de formación de galaxias.

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    Área de la Ciencia:

    • Cosmología
    • La astrofísica
    • La radiación cósmica de fondo de microondas

    Sus antecedentes:

    • Los modelos cosmológicos actuales predicen amplitudes específicas de las anisotropías del fondo cósmico de microondas (CMB).
    • Estas anisotropías están vinculadas a las fluctuaciones de densidad a gran escala y nuestro movimiento relativo a las galaxias.

    Objetivo del estudio:

    • Investigar las predicciones de las hipótesis actuales con respecto al origen de la estructura en el Universo.
    • Para refinar las mediciones de las anisotropías del CMB, en particular la anisotropía del dipolo.

    Principales métodos:

    • Análisis de los datos de la radiación de fondo cósmica de microondas.
    • Comparación de datos observacionales con predicciones teóricas para la formación de estructuras a gran escala.

    Principales resultados:

    • Los esfuerzos observacionales y teóricos se están acercando a la medición precisa de las anisotropías CMB.
    • Los resultados validarán los modelos existentes o indicarán la necesidad de revisiones sustanciales.

    Conclusiones:

    • La medición precisa de las anisotropías CMB es una prueba crítica para los modelos cosmológicos.
    • Las futuras observaciones aclararán nuestra comprensión del origen del universo y la formación de estructuras a gran escala.