TRAP: A temporal systematics model for improved direct detection of exoplanets at small angular separations
arXiv:2011.12311 · doi:10.1051/0004-6361/201937308
Abstract
High-contrast imaging surveys for exoplanet detection have shown giant planets at large separations to be rare. It is important to push towards detections at smaller separations, the part of the parameter space containing most planets. The performance of traditional methods for post-processing of pupil-stabilized observations decreases at smaller separations, due to the larger field-rotation required to displace a source on the detector in addition to the intrinsic difficulty of higher stellar contamination. We developed a method of extracting exoplanet signals that improves performance at small angular separations. A data-driven model of the temporal behavior of the systematics for each pixel can be created using reference pixels at a different position, assuming the underlying causes of the systematics are shared across multiple pixels. This is mostly true for the speckle pattern in high-contrast imaging. In our causal regression model, we simultaneously fit the model of a planet signal "transiting" over detector pixels and non-local reference lightcurves describing a basis of shared temporal trends of the speckle pattern to find the best fitting temporal model describing the signal. With our implementation of a spatially non-local, temporal systematics model, called TRAP, we show that it is possible to gain up to a factor of 6 in contrast at close separations () compared to a model based on spatial correlations between images displaced in time. We show that better temporal sampling resulting in significantly better contrasts. At short integration times for Pic data, we increase the SNR of the planet by a factor of 4 compared to the spatial systematics model. Finally, we show that the temporal model can be used on unaligned data which has only been dark and flat corrected, without the need for further pre-processing.
arXiv commentThis paper has 21 pages of which 17 are the main body and 4 pages are appendix. 16 main figures and 4 figures in appendix
References in corpus (48)
- Angular Differential Imaging: a Powerful High-Contrast Imaging Technique
- Detection and Characterization of Exoplanets and Disks using Projections on Karhunen-Loeve Eigenimages
- The Gemini Planet Imager: First Light
- A probable giant planet imaged in the Beta Pictoris disk
- SPHERE: the exoplanet imager for the Very Large Telescope
- Discovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager
- A new algorithm for point spread function subtraction in high-contrast imaging: a demonstration with angular differential imaging
- Astrometric exoplanet detection with Gaia
- Juliet: a versatile modelling tool for transiting and non-transiting exoplanetary systems
- PynPoint: An Image Processing Package for Finding Exoplanets
- Imaging Spectroscopy for Extrasolar Planet Detection
- Hints for a Turnover at the Snow Line in the Giant Planet Occurrence Rate
- The SPHERE infrared survey for exoplanets (SHINE). III. The demographics of young giant exoplanets below 300 au with SPHERE
- Apodized Pupil Lyot Coronagraphs for Arbitrary Telescope Apertures
- VIP: Vortex Image Processing package for high-contrast direct imaging
- Spectral and atmospheric characterization of 51 Eridani b using VLT/SPHERE
- Imaging Polarimetric Observations of a New Circumstellar Disk System
- Performance of the VLT Planet Finder SPHERE II. Data analysis and Results for IFS in laboratory
- The Structure of High Strehl Ratio Point-Spread Functions
- Double-blind test program for astrometric planet detection with Gaia
- HST/NICMOS detection of HR 8799 b in 1998
- The VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs at wide orbits. IV. Gravitational instability rarely forms wide, giant planets
- M-band Imaging of the HR 8799 Planetary System Using an Innovative LOCI-based Background Subtraction Technique
- Direct exoplanet detection and characterization using the ANDROMEDA method: Performance on VLT/NaCo data
- Improving and Assessing Planet Sensitivity of the GPI Exoplanet Survey with a Forward Model Matched Filter
- Azimuthal asymmetries in the debris disk around HD61005
- The Moving Group Targets of the SEEDS High-Contrast Imaging Survey of Exoplanets and Disks: Results and Observations from the First Three Years
- The Orbit and Transit Prospects for Pictoris b constrained with One Milliarcsecond Astrometry
- Confidence Level and Sensitivity Limits in High Contrast Imaging
- Application of a damped Locally Optimized Combination of Images method to the spectral characterization of faint companions using an Integral Field Spectrograph
- Reliable inference of exoplanet light curve parameters using deterministic and stochastic systematics models
- Ring-apodized vortex coronagraphs for obscured telescopes. I. Transmissive ring apodizers
- PynPoint: a modular pipeline architecture for processing and analysis of high-contrast imaging data
- The TRENDS High-Contrast Imaging Survey. I. Three Benchmark M-dwarfs Orbiting Solar-type Stars
- Characterizing the performance of the NIRC2 vortex coronagraph at W.M. Keck Observatory
- New Techniques for High-Contrast Imaging with ADI: the ACORNS-ADI SEEDS Data Reduction Pipeline
- The Young Suns Exoplanet Survey: Detection of a wide orbit planetary mass companion to a solar-type Sco-Cen member
- Post conjunction detection of Pictoris b with VLT/SPHERE
- Origin of the asymmetry of the wind driven halo observed in high contrast images
- The coronagraphic Modal Wavefront Sensor: a hybrid focal-plane sensor for the high-contrast imaging of circumstellar environments
- Deep imaging search for planets forming in the TW Hya protoplanetary disk with the Keck/NIRC2 vortex coronagraph
- Improving Signal to Noise in the Direct Imaging of Exoplanets and Circumstellar Disks
- STIM map: detection map for exoplanets imaging beyond asymptotic Gaussian residual speckle noise
- A Causal, Data-Driven Approach to Modeling the Kepler Data
- The wind-driven halo in high-contrast images I: analysis from the focal plane images of SPHERE
- A High-contrast Imaging Algorithm: Optimized Image Rotation and Subtraction
- Speckle lifetime in XAO coronagraphic images: temporal evolution of SPHERE coronagraphic images
- Wavelet based speckle suppression for exoplanet imaging - Application of a de-noising technique in the time domain
Cited by in corpus (29)
- Spectroscopic time series performance of the Mid-Infrared Instrument on the JWST
- Astrometric Accelerations as Dynamical Beacons: Discovery and Characterization of HIP 21152 B, the First T-Dwarf Companion in the Hyades
- The unpopular Package: a Data-driven Approach to De-trend TESS Full Frame Image Light Curves
- Revisiting the atmosphere of the exoplanet 51 Eridani b with VLT/SPHERE
- MINDS: JWST/NIRCam imaging of the protoplanetary disk PDS 70
- BEAST begins: Sample characteristics and survey performance of the B-star Exoplanet Abundance Study
- Indications for very high metallicity and absence of methane for the eccentric exo-Saturn WASP-117b
- A scaled-up planetary system around a supernova progenitor
- Comparing Apples with Apples: Robust Detection Limits for Exoplanet High-Contrast Imaging in the Presence of non-Gaussian Noise
- Measuring the variability of directly imaged exoplanets using vector Apodizing Phase Plates combined with ground-based differential spectrophotometry
- Half-sibling regression meets exoplanet imaging: PSF modeling and subtraction using a flexible, domain knowledge-driven, causal framework
- Exoplanet Imaging Data Challenge: benchmarking the various image processing methods for exoplanet detection
- Constraints on the nearby exoplanet Ind Ab from deep near/mid-infrared imaging limits
- Impacts of high-contrast image processing on atmospheric retrievals
- Spectral unmixing for exoplanet direct detection in hyperspectral data
- Spectral and angular differential imaging with SPHERE/IFS. Assessing the performance of various PCA-based approaches to PSF subtraction
- Use the 4S (Signal-Safe Speckle Subtraction): Explainable Machine Learning reveals the Giant Exoplanet AF Lep b in High-Contrast Imaging Data from 2011
- Karhunen-Loève Data Imputation in High Contrast Imaging
- Applying a temporal systematics model to vector Apodizing Phase Plate coronagraphic data: TRAP4vAPP
- Improved companion mass limits for Sirius A with thermal infrared coronagraphy using a vector-apodizing phase plate and time-domain starlight-subtraction techniques
- Physically constrained causal noise models for high-contrast imaging of exoplanets
- Speckle Space-Time Covariance in High-Contrast Imaging
- NA-SODINN: a deep learning algorithm for exoplanet image detection based on residual noise regimes
- Auto-RSM: an automated parameter-selection algorithm for the RSM map exoplanet detection algorithm
- High-contrast spectroscopy with the new VLT/ERIS instrument: Molecular maps and radial velocity of the gas giant AF Lep b
- ISPY -- NaCo Imaging Survey for Planets around Young stars. CenteR: the impact of centering and frame selection
- Spectral cube extraction for the VLT/SPHERE IFS: Open-source pipeline with full forward modeling and improved sensitivity
- Spectral analysis of two directly imaged benchmark L dwarf companions at the stellar-substellar boundary
- The Mysterious Lives Of Speckles. I. Residual atmospheric speckle lifetimes in ground-based coronagraphs