## IMPORTANT NOTE: ## When you use this page as a template for creating your project's groups page: ## * please remove all lines starting with two hashes (##) ## * except the acl line, please keep that, but remove one hash, so it reads #acl ... ## * fix the acl line so it has the correct page instead of the sample Project/AdminGroup ## * the "ME" will be automatically replaces with your name when you save the page ##acl Project/AdminGroup:read,write,delete,revert ##master-page:Unknown-Page ##master-date:Unknown-Date #format wiki #language en Title: Nway--An accurate algorithm to pair sources simultaneously between N catalogs Contact person: Mara Salvato (mara@mpe.mpg.de) Interested/contributing people: Johannes Buchner, Tamas Budavari, Tom Dwelly, Andrea Merloni,Marcella Brusa +Interested people Description: The increasing number of surveys available at any wavelength is allowing the construction of Spectral Energy Distribution (SED) for any kind of astrophysical object. However, a)different surveys/instruments have different positional accuracy and resolution and often are not registered to the same reference system and b) surveys's depth that do not match each other and depending on its redshift and SED, a given source might or might not be detected in a survey. All this makes the pairing of sources among catalogs not trivial.}{ We propose a new algorithm that combine the best of Bayesian and frequentist methods. We extend on the work presented in \citet {Budavari:2008qy}, where we weight the probability that 2 or more sources are associated by one or more priors. We tested the algorithm computing the association between X-ray detected AGN (XMM- and Chandra-COSMOS) and optical and near-infrared sources, simultaneously. When comparing with literature where Maximum Likelihood ratio methods have been used, we find an agreement up to 95\%. For the remaining 5\% of the case we can not access whether either the new code or the literature is providing the correct associations. We finally used the code to compute the optical and mid-infrared counterparts to the Rosat all-sky faint sources. In this paper we release the code and the new catalog of counterparts. Data used: ROSAT, XMM- and Chandra COSMOS, SDSS, WISE, COSMOS photmetry Project conclusion / Publication date: We aim for submission by Dec 2014 / Jan 2015.