Volume 540, April 2012
|Number of page(s)||15|
|Section||Interstellar and circumstellar matter|
|Published online||13 April 2012|
The extinction law from photometric data: linear regression methods⋆
1 European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany
2 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
3 Centro de Astrofisica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
4 University of Milan, Department of Physics, via Celoria 16, 20133 Milan, Italy
5 University of Vienna, Türkenschanzstrasse 17, 1180 Vienna, Austria
Received: 28 October 2011
Accepted: 14 February 2012
Context. The properties of dust grains, in particular their size distribution, are expected to differ from the interstellar medium to the high-density regions within molecular clouds. Since the extinction at near-infrared wavelengths is caused by dust, the extinction law in cores should depart from that found in low-density environments if the dust grains have different properties.
Aims. We explore methods to measure the near-infrared extinction law produced by dense material in molecular cloud cores from photometric data.
Methods. Using controlled sets of synthetic and semi-synthetic data, we test several methods for linear regression applied to the specific problem of deriving the extinction law from photometric data. We cover the parameter space appropriate to this type of observations.
Results. We find that many of the common linear-regression methods produce biased results when applied to the extinction law from photometric colors. We propose and validate a new method, LinES, as the most reliable for this effect. We explore the use of this method to detect whether or not the extinction law of a given reddened population has a break at some value of extinction.
Key words: methods: data analysis / ISM: clouds / dust, extinction / stars: formation
© ESO, 2012
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