Seeking help understanding definition of Riemann sum So, my textbook gives the definition of a Riemann sum in the screenshot below. I understand most of the definition, but I'm lost on \(c_i\) and what the i'th sub-interval is. Previously I was finding the definite integral by: \[\lim_{n \to \infty} \sum_{i=1}^n f(m_i)\cdot \Delta x\] or \[\lim_{n \to \infty} \sum_{i=1}^n f(M_i) \cdot \Delta x\] where \(f(m_i\)) are the minimum endpoints and \(f(M_i\)) are the maximum endpoints. But now my textbook is showing me examples where it's best to use \(f(c_i\)) instead of the endpoint
(continued) instead of the endpoints. If anybody can offer an explanation (perhaps a visual example) I'd greatly appreciate it. I'd also quite like any resources on this, as I couldn't find anything about \((c_i)\). I looked on google and khanacademy but didn't find anything. P.S. Sorry for the long post(s), I just don't know what info is relevant or not. Thanks in advance!
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