The discussion centers on the limits of redshift in detecting distant cosmic objects. Participants agree there are practical limits to detection, particularly due to the universe's opacity before the surface of last scattering, which occurred about 400,000 years after the Big Bang. The Cosmic Microwave Background (CMB) represents a practical limit for electromagnetic radiation redshift, with a redshift of approximately z~1000. While visible light observations are constrained, shorter wavelengths like x-rays and gamma rays may still be detectable, although methods to observe beyond the CMB, such as using neutrinos or gravitational waves, pose significant challenges. Ultimately, the universe's expansion complicates the ability to observe light from distant objects, as regions beyond the observable universe are receding faster than the speed of light.