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/sci/ - Science & Math

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>> No.14703351 [View]
File: 897 KB, 4096x2304, specz16point6.jpg [View same] [iqdb] [saucenao] [google]
14703351

>>14703056
It's how filters are labelled on JWST. F is for filter. 200 means it's centred on 2 microns in wavelength. W means it's a wide broadband filter.
The fact that is disappears at short wavelengths is a possible indication that it's a dropout caused by the Lyman break. For the most distant galaxies these wavelengths correspond to light emitted in the far ultraviolet. Below a specific wavelength (Lyman alpha 121.6 nm) the hydrogen between galaxies strongly absorbs the light. This causes a dramatic break in the spectrum, which can be used to select these galaxies from imaging data.

>> No.14703349 [DELETED]  [View]
File: 897 KB, 4096x2304, specz16point6.jpg [View same] [iqdb] [saucenao] [google]
14703349

>>14703056
It's how filters are labelled on JWST. F is for filter. 200 means it's centred on 2 microns in wavelength. W means it's a wide broadband filter.
The fact that is dispersers at short wavelengths is a possible indication that it's a dropout showing caused by the Lyman break. For the most distant galaxies these wavelengths correspond to light emitted in the far ultraviolet. Below a specific wavelength (Lyman alpha 121.6 nm) the hydrogen between galaxies strongly absorbs the light. This causes a dramatic break in the spectrum, which can be used to select these galaxies from imaging data.

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