etd etd exoplanet transit database
play

ETD ETD Exoplanet Transit Database in past, present and future - PowerPoint PPT Presentation

ETD ETD Exoplanet Transit Database in past, present and future Lubos Brat Variable Star and Exoplanet Section of Czech Astronomical Society ETD in past 2004 first exoplanet transit observation in Czech republic 2006 TRESCA


  1. ETD ETD – Exoplanet Transit Database in past, present and future Lubos Brat Variable Star and Exoplanet Section of Czech Astronomical Society

  2. ETD in past • 2004 – first exoplanet transit observation in Czech republic • 2006 – TRESCA project started • 2008 – ETD founded, inspired by O-C Gateway • August – during simultanous observation of HD189733b transit, two ideas were born (TRESCA on-line form and ETD concept) • September – on-line TRESCA application form created by Pejcha and Brát • December – ETD was created (Brát, Poddaný) • 2009 – ETD become famous and the only and complex source of informations for transit observers all around the world

  3. Global success of f ETD

  4. ETD in present ETD statistics 2001 - 2019 • Data statistics 10000 • 11 years 9000 • 1500 authors • 9000 transits 8000 • 225 exoplanets and 1400 candidates 7000 Transit totals in ETD • Citation statistics 6000 ETD totals • 2010 - New Astronomy, Volume 15, Issue 3, p. 297-301, Poddaný, Brát, Pejcha, 5000 72 citations so far 4000 • Data workflow TRESCA transits 3000 • Transits are collected in TRESCA project * verified by human * included in ETD 2000 • Transits are gathered from papers and displayed in ETD with proper reference 1000 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 YEAR 2000 +

  5. ETD technological background • Technical solution (2008, PHP, MySQL, Apache web server, FreeBSD os) • Internal databases (table of transits, table of transiting exoplanets – both confirmed and candidates) • Transit light curve processing • C++ application called from web, input: parameters from database and data • Error bars are rescaled to real poison scatter • 𝑛 𝑢 𝑗 = 𝐵 − 2.5 log 𝐺 𝑨 𝑢 𝑗 , 𝑢 𝑝 , 𝐸, 𝑐 , 𝑞, 𝑑 1 + 𝐶 𝑢 𝑗 − 𝑢 𝑛𝑓𝑏𝑜 + 𝐷 𝑢 𝑗 − 𝑢 𝑛𝑓𝑏𝑜 2 • Where F(z,p,c) is computed artificial light curve using Mandel & Agol (2002) occultsmall routing • Levenberg-Marquardt non-linear least squares fit from Price et al. (1992)

  6. ETD technological background • Automatical data-quality rating • 1 (best) – 5 (worst), depends on transit depth 𝜀 , data sampling 𝜍 and mean 𝜀 absolute deviation S,  = 𝑇 𝜍 • Modeling of host star – exoplanet geometry

  7. ETD in (near) future • ETD v 2.0 – technical solution (ASP.NET Core, C#, REST API) • New design • TTV plots in list of exoplanets • Interactive plots and grids • DateTimes both in UTC and LOCAL TIME • Storing user settings (coordinates, time zone, grids filters and sorts) • UI better works with a large number of exoplanets • Interesting exoplanets TIPs

  8. ETD in (near) future • Client independent approach • REST API could be used by any web application, Windows / Linux / MacOS desktop application, Android & iOS mobile app • ETD REST API functions • GET exoplanets, GET transits for some exoplanet, GET transit, GET data • POST new transit, POST new transiting exoplanet • GET predictions • GET model fit of transit observation • Public interface for developers (Swagger) • Expected release: 2020 • Far future: AI searching for TTV and wrong data points in TTV plots

  9. ETD call for cooperation 1. Become ETD editor • Adding new transits from literature and other sources 2. Become ETD donator • Send a voluntary financial contribution to support ETD further development 3. Become ETD developer • Join the .NET development team and work on new features and bug fixes 4. Give ETD your feedback • Tell us your needs / expectations / complains and help us improve ETD

  10. We are just in the beginning … Thank you for your attention!

Recommend


More recommend