Designing Large-Scale Imaging Surveys for a Retrospective Relative Photometric Calibration

Details Designing Large-Scale Imaging Surveys for a Retrospective Relative Photometric Calibration Designing Large-Scale Imaging Surveys for a Retrospective Relative Photometric Calibration

2012-03-28

arxiv.org/abs/1203.6255v1

Astronomy and Astrophysics

Astrophysics

Instrumentation and Methods for Astrophysics

Scientific paper

We study the self-calibration - the determination of a complex system response from science data alone - for precise photometric catalogs from wide-field imaging surveys. We create an artificial sky of sources and synthetically observe it under four basic survey strategies, creating an end-to-end simulation of an imaging survey for each. These catalog-level simulations include realistic measurement uncertainties and a complex focal-plane dependence of the instrument response. In the self-calibration step, we simultaneously fit for all the star fluxes and the parameters of a position-dependent flat-field. For realism, we deliberately fit with a wrong noise model and a flat-field functional basis that does not include the model that generated the synthetic data. We demonstrate that with a favorable survey strategy, a complex (but smooth) instrument response can be precisely self-calibrated. We show that returning the same sources to very different focal plane positions is the key property of any survey strategy designed for accurate retrospective calibration. The results of this work suggest the following advice for those considering the design of large-scale imaging surveys: Do not use a regular tiling of the sky; instead return the same sources to very different focal plane positions.

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