Thursday, October 24, 2024

Supernova at Z=2.83 - large angular size, smaller objects on the same image, relatively weak to completely exclude detector saturation - one more confirmation of light scattering

 To confirm the presence of the light scattering for the images of supernovas obtained by JWST the image of supernova was taken from [1]:


In this image supernova which must have the angular size comparable to the angular resolution of the telescope is clearly much larger. The possible experimental errors are excluded:

1.There is at least one 2.7 times sharper object on the image - it means that the telescope trembling during accumulation may be excluded - it would blur both objects equally.

2.Sometimes close supernovas are visible as very large dots (and with projectiles like in [2]) because of the extreme brightness: the detector is saturated and because of cross-talk between pixels on the camera the adjacent to saturated pixel other pixels will be bright like registering light (common problem with both CCD and CMOS cameras). Since the supernova is just a little brighter than the surrounding (and much less bright compare to the brightest stars on the image) this possible experimental error is not possible too.

Only new phenomena, light scattering at very high distances may explain this image of supernova at z=2.83 (z is confirmed by spectroscopy in [1])
    In addition to already published images this one again confirms the author point of view that light from the far galaxies and supernovas is scattered, thus removing need for dark energy and Big Bang (and confirming the tired light hypothesis)

References.

1.2406.05076 (arxiv.org)

https://arxiv.org/pdf/2406.05076

2.Supernova - Wikipedia

3.2311.0060v1.pdf (vixra.org)

https://vixra.org/pdf/2311.0060v1.pdf