VIP: Vortex Image Processing package for high-contrast direct imaging
arXiv:1705.06184 · doi:10.3847/1538-3881/aa73d7
Abstract
We present the Vortex Image Processing (VIP) library, a python package dedicated to astronomical high-contrast imaging. Our package relies on the extensive python stack of scientific libraries and aims to provide a flexible framework for high-contrast data and image processing. In this paper, we describe the capabilities of VIP related to processing image sequences acquired using the angular differential imaging (ADI) observing technique. VIP implements functionalities for building high-contrast data processing pipelines, encompass- ing pre- and post-processing algorithms, potential sources position and flux estimation, and sensitivity curves generation. Among the reference point-spread function subtraction techniques for ADI post-processing, VIP includes several flavors of principal component analysis (PCA) based algorithms, such as annular PCA and incremental PCA algorithm capable of processing big datacubes (of several gigabytes) on a computer with limited memory. Also, we present a novel ADI algorithm based on non-negative matrix factorization (NMF), which comes from the same family of low-rank matrix approximations as PCA and provides fairly similar results. We showcase the ADI capabilities of the VIP library using a deep sequence on HR8799 taken with the LBTI/LMIRCam and its recently commissioned L-band vortex coronagraph. Using VIP we investigated the presence of additional companions around HR8799 and did not find any significant additional point source beyond the four known planets. VIP is available at http://github.com/vortex-exoplanet/VIP and is accompanied with Jupyter notebook tutorials illustrating the main functionalities of the library.
References in corpus (12)
- The NumPy array: a structure for efficient numerical computation
- scikit-image: Image processing in Python
- Direct Imaging of Multiple Planets Orbiting the Star HR 8799
- New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit
- Fundamental limitations of high contrast imaging set by small sample statistics
- Instrumentation for the detection and characterization of exoplanets
- Reconnaissance of the HR 8799 Exosolar System II: Astrometry and Orbital Motion
- VLT/SPHERE robust astrometry of the HR8799 planets at milliarcsecond-level accuracy Orbital architecture analysis with PyAstrOFit
- The LEECH Exoplanet Imaging Survey. Further constraints on the planet architecture of the HR 8799 system
- L'-band AGPM vector vortex coronagraph's first light on LBTI/LMIRCam
- Sequential Covariance Calculation for Exoplanet Image Processing
- High contrast imaging at the LBT: the LEECH exoplanet imaging survey
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- A New Standard for Assessing the Performance of High Contrast Imaging Systems
- The Effect of Binarity on Circumstellar Disk Evolution
- Discovery of a White Dwarf Companion to HD 159062