TA-DA: a Tool for Astrophysical Data Analysis
arXiv:1210.1850 · doi:10.1088/0004-6256/144/6/176
Abstract
We present TA-DA, a new software aimed at greatly simplify and improve the analysis of stellar photometric data in comparison with theoretical models, and allow the derivation of stellar parameters from multi-band photometry. Its flexibility allows one to address a number of such problems: from the interpolation of stellar models, or sets of stellar physical parameters in general, to the computation of synthetic photometry in arbitrary filters or units; from the analysis of observed color-magnitude diagrams, to a Bayesian derivation of stellar parameters (and extinction) based on multi-band data. TA-DA is available as a pre-compiled IDL widget-based application; its graphical user interface makes it considerably user-friendly. In this paper we describe the software and its functionalities.
AJ accepted. The software is available at http://www.rssd.esa.int/staff/ndario/TADA/ . Comments are welcome for future additions/updates to TA-DA
References in corpus (6)
- The ACS Nearby Galaxy Survey Treasury IX. Constraining asymptotic giant branch evolution with old metal-poor galaxies
- Empirical isochrones and relative ages for young stars, and the radiative-convective gap
- A Multi-Color Optical Survey of the Orion Nebula Cluster. Part I: the Catalog
- The Complete Initial Mass Function Down to the Sub-Solar Regime in the Large Magellanic Cloud with Hubble Space Telescope ACS Observations
- Pre-main-sequence isochrones -- I. The Pleiades benchmark
- Empirical Near Infrared colors for low-mass stars and brown dwarfs in the Orion Nebula Cluster
Cited by in corpus (15)
- The Mass Dependence Between Protoplanetary Disks and their Stellar Hosts
- IN-SYNC I: Homogeneous Stellar Parameters from High Resolution APOGEE Spectra for Thousands of Pre-main Sequence Star
- An extensive VLT/X-Shooter library of photospheric templates of pre-main sequence stars
- The Panchromatic Hubble Andromeda Treasury XV. The BEAST: Bayesian Extinction and Stellar Tool
- The very low-mass stellar content of the young supermassive Galactic star cluster Westerlund 1
- Photometric determination of the mass accretion rate of pre-main sequence stars. IV. Recent star formation in NGC 602
- Photometric determination of the mass accretion rates of pre-main sequence stars. V. Recent star formation in the 30 Dor nebula
- Single stars in the Hyades open cluster. Fiducial sequence for testing stellar and atmospheric models
- Precise High-Cadence Time Series of Five Variable Young Stars in Auriga with MOST
- Strong Biases in Estimating the Time Dependence of Mass Accretion Rates in Young Stars
- Benchmarking MESA isochrones against the Hyades single star sequence
- HST survey of the Orion Nebula Cluster in the HO 1.4 m absorption band: II. The substellar IMF down to planetary masses
- Constraining the escape fraction of ionizing photons from HII regions within NGC 300: A concept paper
- The stellar content of the infalling molecular clump G286.21+0.17
- Sequential Star Formation in the Young SMC Region NGC 602: Insights from ALMA