https://kailaronayne.carrd.co 2026-03-16 daily 1.0 https://kailaronayne.carrd.co/assets/images/image01.jpg https://kailaronayne.carrd.co/assets/images/image05.jpg https://kailaronayne.carrd.co/assets/images/gallery01/cb87627c.jpg Untitled https://kailaronayne.carrd.co/assets/images/gallery01/0a33962e.jpg Untitled https://kailaronayne.carrd.co/assets/images/gallery01/122adfe7.jpg Untitled https://kailaronayne.carrd.co/assets/images/gallery01/6f9e2db8.jpg Untitled https://kailaronayne.carrd.co/assets/images/gallery01/bf2591f0.jpg Claude Monet - The Japanese Footbridge at Giverny https://kailaronayne.carrd.co/assets/images/gallery02/c901aefc.jpg Vincent (Beagle) https://kailaronayne.carrd.co/assets/images/gallery02/c798add1.jpg Vincent (Beagle) https://kailaronayne.carrd.co/assets/images/gallery02/944f6cdc.jpg Achilles (Pit Mix) https://kailaronayne.carrd.co/assets/images/gallery02/48a4b883.jpg Achilles (Pit Mix) https://kailaronayne.carrd.co/assets/images/gallery03/a8da11fd.jpg We find that the 7.7 micron luminosity (L770) is linearly correlated to the dust-corrected FUV luminosity and thus the total star formation with a scatter of σ = 0.289 dex. https://kailaronayne.carrd.co/assets/images/gallery04/03dece70.jpg We analyze 8 spectroscopically confirmed LRDs with JWST/NIRCam, NIRSpec, and MIRI. SEDs modeled with CIGALE, PROSPECTOR, and dense-gas templates show that only dense-gas and some AGN scenarios are consistent with far-IR and radio limits.