2006
DOI: 10.1090/s0025-5718-06-01913-2
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On mixed and componentwise condition numbers for Moore–Penrose inverse and linear least squares problems

Abstract: Abstract. Classical condition numbers are normwise: they measure the size of both input perturbations and output errors using some norms. To take into account the relative of each data component, and, in particular, a possible data sparseness, componentwise condition numbers have been increasingly considered. These are mostly of two kinds: mixed and componentwise. In this paper, we give explicit expressions, computable from the data, for the mixed and componentwise condition numbers for the computation of the … Show more

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Cited by 84 publications
(51 citation statements)
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“…In the following part, we show that these mixed and componentwise condition numbers for the STLS problem respectively approach some existing mixed and componentwise condition numbers for the LS problem, i.e., μ M ST LS → μ LS and ν M ST LS → ν LS , when λ → 0. Under the condition that A is of full column rank, Cucker et al [2] derived the following mixed and componentwise condition numbers for the LS problem (2.4):…”
Section: Definition 41mentioning
confidence: 99%
“…In the following part, we show that these mixed and componentwise condition numbers for the STLS problem respectively approach some existing mixed and componentwise condition numbers for the LS problem, i.e., μ M ST LS → μ LS and ν M ST LS → ν LS , when λ → 0. Under the condition that A is of full column rank, Cucker et al [2] derived the following mixed and componentwise condition numbers for the LS problem (2.4):…”
Section: Definition 41mentioning
confidence: 99%
“…Note that the norm on the solution space G has not been chosen yet. Following the terminology given in [13] and also used in [9], K(y) is referred to as componentwise (resp. mixed) condition number when · G is componentwise (resp.…”
Section: Application To Condition Numbersmentioning
confidence: 99%
“…When L is the identity matrix, the expression given in (3.3) is the same as the one established in [9] (using the norm · = · ∞ x ∞ on the solution space). Note that bounds of K ∞ (I, A, b) are also given in [7, p. 34] and in [21, p. 384].…”
Section: Use Of the Infinity Norm On The Solution Spacementioning
confidence: 99%
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