The Novel Method for Identifying Fast Optical Transients The Application of Multi-Exposure Plates - PowerPoint PPT Presentation

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The Novel Method for Identifying Fast Optical Transients The Application of Multi-Exposure Plates

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  1. The Novel Method for Identifying Fast Optical Transients The Application of Multi-Exposure Plates for OT/GRBs analyses René Hudec1 and Lukáš Hudec2 1 ASTRONOMICAL INSTITUTE, CZ-251 65 ONDREJOV, CZECH REPUBLIC 2 Department of Informatics, FACULTY OF MATHEMATICS AND PHYSICS, CHARLES UNIVERSITY, PRAGUE, CZECH REPUBLIC

  2. Archival sky patrol plates There are more than 3 millions archival plates in the world, lim mag up to 23, > 5 x 5 deg in most cases .... Ondrejov has 110 000 plates Suitable for dense long-term photometry (up to 100 years, up to 2000 points, up to 23 mag) Suitable to detect rare events - years od CONTINUOUS monitoring easily possible However, the access to the data is still difficult, but: Recently, efforts to digitize the plates Use of scanners, powerful computers and innovative software allows the effective data evaluation for the first time

  3. Optical Transients of Astrophysical Origin • OTs and OAs of Gamma Ray Bursts - including Orphans (seen only in optical) • flares on blazars and AGNs - up to 10 mag amplitudes revealed by extended plate analyses • stellar OTs such as stellar flares, CVs flares etc. • OTs of unclear origin (observational reports)

  4. Optical Transients - very large amplitude AGN flares Example of results from extended analyses on archival sky patrol plates > 10 mag amplitude optical flare from a faint AGN, HCO plate Flares on faint AGNs - up to more than 10 mag amplitudes revealed by extended plateanalyses (up to 3 years of continuous monitoringtime analysed)

  5. Optical Transient Analyses - OT in Triangulum, Sonneberg Astrograph Plate, 6 mag above plate limitthe searches for analogous OTs are difficult since the plates contains typically 10 000 - 100 000 star images

  6. Sonneberg Observatory Plate Archive: 270 000 plates 1928 - 2002, largest European plate collection

  7. History: evaluation of archival plates by eye estimation Eye estimation can however still yields valuable results: Experienced person can provide measurements with precision analogous to plate photometers and CCD scanning The method is quick and suitable for evaluation of one selected object on many plates where digitization is less effective

  8. New: The digitisation of the astronomical plates, the novel software and the use of powerful computers allow the automated data mining and scientific evaluation of the plates for the first time Interface between astronomy and informatics

  9. We report on the novel method how to identify brief optical transients (OTs) on sky archival plates. This method does not require identification of all objects and their comparison with the catalogue, but rely solely on the information included in the particular plate itself.

  10. If we look for optical prompt emission (including orphans) from GRBs, we need to look for short-living transient phenomena lasting minutes. However, on long-exposed deep images and plates, it is very difficult to look for brief transients since the OT image is hidden by typically tens to hundreds of thousands stellar images with similar appearance. The methods of comparing plates and/or comparison with catalogues is still not very effective and reliable.

  11. Here we propose novel method using multiply exposed astronomical plates and based solely on the information in the plate itself. Such plates are available in various sky plate archives, e,g. at the Royal Observatory Brussels. These plates contains several (typically 2 to 10) identical star field images on the same plate. This means, each star inside the FOV of the telescope, is represented several times. Such plates have been obtained by mutiple exposures on the same plate with tiny shifts between the exposures

  12. It is very difficult to find transient objects on these plates by classical methods. However, using digitisation, and dedicated novel software programs, it is relatively easy, effective and reliable to identify the OT candidates. Program by informatics student L. Hudec: Program input: scanned multiple exposure plates from the Royal Observatory Brussels - ESO Schmidt (and analogous plates)

  13. Typical ROB ESO multiple exposure plate, scanned binned, 1 from 4 pixels read out

  14. Example of OT found: duration less than 30 min real object - 2 images

  15. fast OT and moving object (asteroid)

  16. Example of fast OT found - duration less than 5 minutes

  17. The first results of the application of the novel software program on multiply exposed plates are very promising. At moment, the program identifies objects showing deviations regarding to normal star constant images. Then the human inspection is required to discard the obvious defects. This is easy and fast. Typically 1 OT candidate remains after the procedure for 1 plate. The examples shown are for binned plates (1 from 4 pixels read out) to accelerate the computing process. The final program will use non-binned data.

  18. Excellent example how the valuable information obtained in archival astronomical plates can be accessed and scientifically used • Such analyses are possible only based on plate digitisation, novel software and powerful computers • Analogous procedures can be applied also for trailed star images, spectral plates with objective prisma, etc. - searches for objects with strange spectra, spectral emission lines, rapid light changes etc. • Collaboration with informatics students

  19. All Sky Photographic Monitoring - central part of a scanned plate Directed by the Ondrejov Observatory Still in operation 12 stations lim mag 12 9 x 12 cm photographic plates High quality photographic scanner available

  20. Real time optical data for GRBs - Digitized Ondrejov All Sky Plate The area of the GRB000926 on the plates of the EN network. Simultaneous optical image, lim magnitude 8. The position of the GRB is indicated by a circle. The image contains airplane trails/lights. Important coinstraints on the prompt optical emission of GRBs

  21. Scanned Sonneberg Sky Patrol Plate - small part. The full plate has 30 x 30 degrees, lim mag 14.5, V and B plates are taken simultaneously.Time coverage is 74 years.

  22. Sonneberg Photographic Sky Patrol Digitized Plate - 1/4 shown here i.e. 15 x 15 deg the full plate has 30 x 30 deg Lim mag 14.5 Scanned with the HISS scanner 12 microns resolution

  23. All Sky CCD Camera, Sonneberg Observatory, 7K x 4K CCD and f/3.5 FE lens. Lim mag 10 in 1 min integration time.

  24. Astronomical plates - our contribution • Development of software for automated evaluation of Sonneberg Sky Patrol Plates • Software to detect and to classify variable objects on Schmidt plates (Tautenburg) • Search for faint variable and flaring objects on digitized UKSTU plates (lim mag 23) • Participation on the European Plate Centre Project in Brussel

  25. Our contribution … continue • automated evaluation of digitised plates: spectral, trailed, multiple images,....

  26. Digitized Schmidt plate, TLS Tautenburg, lim mag 20, field M92. Newly detected variable objects with light amplitude > 2 mag are indicated

  27. UKSTU Plates • faint limits, 19 - 23 • FOV 40 sq. degrees • various colors/filters • spectral plates down to mag 18 • 18 000 plates over 30 years • Unfortunately end of operation in 2001

  28. Our projects at the UKSTU • Analyses on digitized UKSTU plates, focusing on densely populated time periods and in different filtres • Independent searches for optical afterglows of GRBs • Statistics and classification of faint variable stars • No realiable statistics of variable stars is available yet below mag 18! • Long-term evolution of selected faint sources such as XTE J2123-058, XTE J1550-564, RXJ 1313.2-3259 etc.

  29. Another possible analogous informatics works: • comparison of scanned plates - identical fields • the same for all-sky images • automated generating of ligh curves of all objects on the plates - for typically 1000 plates, the same field, different times • spectral plates - objective prisma • trailed plates - stars as long trails - flares, dips • a lot of work for informatics students....