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The integration of the data from Telescope Fabra The integration of the data from Telescope ROA Montsec to the Virtual Observatory Fabra ROA Montsec to the Virtual Observatory Data centre overview Type of data to be published in Octavi


  1. The integration of the data from Telescope Fabra The integration of the data from Telescope ROA Montsec to the Virtual Observatory Fabra ROA Montsec to the Virtual Observatory Data centre overview Type of data to be published in Octavi Fors 1 , 2 , Guillem Pérez 3 the VO & rest of TFRM team 1 , 2 , 4 Why to publish data in the VO? Experience 1 Departament d’Astronomia i Meteorologia, Universitat de Barcelona Problems faced and help received 2 Observatori Fabra from VO experts Conclusions 3 Escola Tècnica Superior d’Enginyeria Informàtica, Universitat Autònoma de Barcelona 4 Real Observatorio de la Armada EuroVO CoSADIE, Heidelberg 10-11 Jun 2013

  2. Index The integration of the data from Telescope Fabra ROA Montsec to the Virtual Observatory Data centre overview Data centre overview Type of data to be published in the VO Type of data to be published in the VO Why to publish Why to publish data in the VO? data in the VO? Experience Experience Problems faced and help received from VO experts Conclusions Problems faced and help received from VO experts Conclusions

  3. Index The integration of the data from Telescope Fabra ROA Montsec to the Virtual Observatory Data centre overview Data centre overview Type of data to be published in the VO Type of data to be published in the VO Why to publish Why to publish data in the VO? data in the VO? Experience Experience Problems faced and help received from VO experts Conclusions Problems faced and help received from VO experts Conclusions

  4. Index The integration of the data from Telescope Fabra ROA Montsec to the Virtual Observatory Data centre overview Data centre overview Type of data to be published in the VO Type of data to be published in the VO Why to publish Why to publish data in the VO? data in the VO? Experience Experience Problems faced and help received from VO experts Conclusions Problems faced and help received from VO experts Conclusions

  5. Index The integration of the data from Telescope Fabra ROA Montsec to the Virtual Observatory Data centre overview Data centre overview Type of data to be published in the VO Type of data to be published in the VO Why to publish Why to publish data in the VO? data in the VO? Experience Experience Problems faced and help received from VO experts Conclusions Problems faced and help received from VO experts Conclusions

  6. Index The integration of the data from Telescope Fabra ROA Montsec to the Virtual Observatory Data centre overview Data centre overview Type of data to be published in the VO Type of data to be published in the VO Why to publish Why to publish data in the VO? data in the VO? Experience Experience Problems faced and help received from VO experts Conclusions Problems faced and help received from VO experts Conclusions

  7. Index The integration of the data from Telescope Fabra ROA Montsec to the Virtual Observatory Data centre overview Data centre overview Type of data to be published in the VO Type of data to be published in the VO Why to publish Why to publish data in the VO? data in the VO? Experience Experience Problems faced and help received from VO experts Conclusions Problems faced and help received from VO experts Conclusions

  8. Location The integration of the data from Telescope Fabra Montsec Astronomical Observatory at Pre-Pyrenees range ROA Montsec to the Virtual φ = 42 . ◦ 0516 N, λ = 0 . ◦ 7293 E, h = 1570 m HMSL Observatory Data centre overview Type of data to be published in the VO Why to publish data in the VO? Experience Problems faced and help received from VO experts Conclusions

  9. Location The integration of the data from Telescope Fabra ROA Montsec to Telescope Fabra ROA Montsec (TFRM) the Virtual Observatory Data centre overview Type of data to be published in the VO Why to publish data in the VO? Experience Problems faced and help received from VO experts Conclusions http://www.am.ub.edu/bnc Fors, O. et al. 2013 PASP, 125, 927 (in press, arXiv:1211.5581)

  10. TFRM description The integration of the data from Telescope Fabra ROA Montsec to the Virtual Observatory Data centre ◮ Optic design: refigured Baker-Nunn Camera. overview ◮ Focal ratio: f/0.96. Type of data to be published in the VO ◮ 0.5m three-element corrector cell and 0.78m primary Why to publish spherical mirror. data in the VO? ◮ FoV: 4 . Experience ◦ 4x4 . ◦ 4. Problems faced ◮ Pixel scale: 3 . 9 ′′ . and help received from VO experts ◮ Spider vanes and focus system with ± 10 µ m or better Conclusions focus repeatability.

  11. TFRM description The integration of the data from Telescope Fabra ROA Montsec to Layout of the corrected Baker-Nunn Camera design. the Virtual Observatory Data centre overview Type of data to be published in the VO Why to publish data in the VO? Experience Problems faced and help received from VO experts Conclusions

  12. TFRM description The integration of the data from Telescope Fabra ROA Montsec to the Virtual Observatory Design and manufacture of spider vanes and CCD focus Data centre system. overview Type of data to be published in the VO Why to publish data in the VO? Experience Problems faced and help received from VO experts Conclusions

  13. TFRM description The integration of the data from Telescope Fabra Huge 4 . ◦ 4x4 . ◦ 4 FoV with outstanding image quality through all the CCD. ROA Montsec to the Virtual Observatory Data centre overview Type of data to be published in the VO Why to publish data in the VO? Experience Problems faced and help received from VO experts Conclusions

  14. TFRM description: observational programs The integration of the data from Telescope Fabra ROA Montsec to the Virtual Observatory Data centre overview Type of data to ◮ TFRM-PSES: TFRM-Preselected Super-Earths Survey. be published in the VO ◮ Optical asset for Space Situational Awareness/Space Why to publish data in the VO? Surveillance and Tracking (SSA/SST) of GEO ring Experience space debris (in collaboration to ESA and ISON). Problems faced ◮ NEOs survey. and help received from VO experts Conclusions

  15. TFRM description: observational programs The integration of the data from Telescope Fabra ROA Montsec to the Virtual Observatory Data centre overview Type of data to ◮ TFRM-PSES: TFRM-Preselected Super-Earths Survey. be published in the VO ◮ Optical asset for Space Situational Awareness/Space Why to publish data in the VO? Surveillance and Tracking (SSA/SST) of GEO ring Experience space debris (in collaboration to ESA and ISON). Problems faced ◮ NEOs survey. and help received from VO experts Conclusions

  16. TFRM description: observational programs The integration of the data from Telescope Fabra ROA Montsec to the Virtual Observatory Data centre overview Type of data to ◮ TFRM-PSES: TFRM-Preselected Super-Earths Survey. be published in the VO ◮ Optical asset for Space Situational Awareness/Space Why to publish data in the VO? Surveillance and Tracking (SSA/SST) of GEO ring Experience space debris (in collaboration to ESA and ISON). Problems faced ◮ NEOs survey. and help received from VO experts Conclusions

  17. TFRM description: robotic operations & The integration of the data from Telescope Fabra insfrastructure ROA Montsec to the Virtual Observatory Data centre overview ◮ TFRM remote and robotic control software based on Type of data to INDI protocol. be published in the VO ◮ robotic observations are formalized in XML files. Why to publish data in the VO? ◮ symmetric 100 Mbps fiber cable Internet connection. Experience ◮ data archive stored at site in a NAS RAID system. Problems faced and help received ◮ 140,000 useful science images per year (4.5 from VO experts Tb/year) . Conclusions ◮ plus calibration images, robotic operations exceed 6.5Tb/year .

  18. TFRM description: robotic operations & The integration of the data from Telescope Fabra insfrastructure ROA Montsec to the Virtual Observatory Data centre overview ◮ TFRM remote and robotic control software based on Type of data to INDI protocol. be published in the VO ◮ robotic observations are formalized in XML files. Why to publish data in the VO? ◮ symmetric 100 Mbps fiber cable Internet connection. Experience ◮ data archive stored at site in a NAS RAID system. Problems faced and help received ◮ 140,000 useful science images per year (4.5 from VO experts Tb/year) . Conclusions ◮ plus calibration images, robotic operations exceed 6.5Tb/year .

  19. TFRM description: robotic operations & The integration of the data from Telescope Fabra insfrastructure ROA Montsec to the Virtual Observatory Data centre overview ◮ TFRM remote and robotic control software based on Type of data to INDI protocol. be published in the VO ◮ robotic observations are formalized in XML files. Why to publish data in the VO? ◮ symmetric 100 Mbps fiber cable Internet connection. Experience ◮ data archive stored at site in a NAS RAID system. Problems faced and help received ◮ 140,000 useful science images per year (4.5 from VO experts Tb/year) . Conclusions ◮ plus calibration images, robotic operations exceed 6.5Tb/year .

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