Welcome to SHERLOCK PIPEline’s documentation!
The SHERLOCK (Searching for Hints of Exoplanets fRom Lightcurves Of spaCe-based seeKers) PIPEline is a user-friendly pipeline, which
minimizes the interaction of the user to the minimum when using data coming from Kepler or TESS missions. SHERLOCK makes use of previous well-known and well-tested codes which allow the exoplanets community to explore the public data from space-based missions without need of a deep knowledge of how the data are built and stored.
In most of cases the user only needs to provide with a KIC-ID, EPIC-ID, TIC-ID or coordinates of the host star where wants to search for exoplanets.
Contents:
- Installation
- SHERLOCK PIPEline
- SHERLOCK PIPEline: Programmatic API
- Fit Module
- Vet Module
- Stability Module
- Plan Module
- Tutorials
- Step 1: Understanding the Properties Configuration
- Step 2: Running SHERLOCK with the Properties File
- Step 3: Selected signals bayesian fit
- Step 4: Candidates vetting
- Step 5: TIC 305048087 candidates system stability
- Step 6: TIC 305048087 candidates follow-up program plan
- Summary
- Searching for TOI-178 candidates
- TOI 270 exploration
- Searching for planetary candidates around fast rotators
- TOI 175: Search & Vetting
- TOI 1798: Search & Vetting
- Who we are