Is the "cosmological constant tension" the prime reason that we believe the expansion of the universe is accelerating? Background: For a few years now there is significant difference in the calculation of the cosmological constant between standard candles methods and CMB methods. CMB measurement comes from a very young universe (~400k years) and the resulting cosmological constant as calculated by the Planck collaboration is smaller than what is observed today. 
Question: Is this so-called "tension" the main reason for talking about accelerated expansion? 
I've found a relevant article by Hossenfelder. I understand that according to the article, the answer to this question is "yes; but we've also seen some other minor indications in support of accelerated expansion". 
Note: The question is not about whether any of the measurements are plagued by uncertainties or how trustworthy they are in general. 
 A: No. Evidence for the accelerating expansion of the universe comes from multiple angles: supernovae data, Baryon acoustic oscillations, the mass functions of galaxy clusters, etc. That the universe's expansion is accelerating is not in doubt; the question is by how much. 
A: There is a potential tension between low redshift probes of mass clustering and Planck data (CMB measurements). This ongoing speculation might be evidence of new physics or even modifications of general relativity. However, the author of the article you cited seems to have a confusion between the cosmological constant (no tension discussed in the literature) and the Hubble constant (that has $3\sigma$ differences), which becomes clear when you read the comments where a noted CMB researcher expresses his views. There is even no real evidence that the cosmological constant is not constant.
So it is really exciting if some tensions in CMB data grows into significant differences. But one should not confuse the cosmological constant with the Hubble constant which are completely different stuffs.
A: Cosmologists believe the universe is expanding at an accelerating rate because the measured value of the cosmological is positive.
The "tension" is that the two different methods give different values of the Hubble parameter (from which the cosmological constant can be calculated). There is a low probability ($4.4 \sigma$ according to Wikipedia) that these results are due to chance, which leads some people to believe that the cosmological constant is not in fact constant and may vary in space and time. This would be an indicator of new physical effects beyond our current theories. However, all measured values (and data from other sources) still suggest an accelerated expansion.
