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We present the results of light curve fits to two DBV white dwarfs, PG 1351+489 and GD 358. For both fits, we include recent improvements in calculations relating the bolometric and observed flux variations. We provide a preliminary map of convection across the DB instability strip, and we show how this allows us to choose between two possible spectroscopic fits to PG 1351+489.

What We Can Learn from the Light Curves of GD 358 and PG 1351+489