building a simple image server from available tools steven gibson (arecibo observatory, puerto rico)...

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Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov Observatory, Czech Republic )

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Page 1: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

Building a Simple Image Server

from Available Tools

Steven Gibson (Arecibo Observatory, Puerto Rico)

NVO Summer School, Aspen, 2006

Petr Škoda (Ondřejov Observatory, Czech Republic )

Page 2: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

Motivation

● Want to learn the basics of SIAP, which was not covered in detail in the lectures.

● Have been tasked by employers with making ongoing surveys part of the NVO.

● Have existing data that want to share!● Start with a small, simple set of data . . .

Page 3: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov
Page 4: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

Perseus HISAComplex:

Distance ~ 2000 pcAngular Size ~ 3 deg2

Physical Size ~ 100 pc2

H I Self-Absorption (HISA) Cold H I visible asintricate shadows against warmer H I emission in the Galactic disk.

HISA comes in bothlarge, organizedcomplexes and small, random ``fluff’’.

Page 5: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

Northern Coalsack Cyg OB7 HISA

Distance ~ 800 pcAngular size ~ (3 deg)2

Physical size ~ (40 pc)2

A Big HISA Cloud

Page 6: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

IC 2944(Thackeray's Globules)

Distance ~ 1800 pcAngular size ~ < 40”Physical size ~ < 0.3 pc

Local HISA Filament

Distance ~ 100 - 500 pcAngular size ~ 1' x 5'Physical size ~ 0.03-0.1 x 0.13-0.25 pc

A Small HISA Cloud

Page 7: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

Why Study Cold H I ?

● Abundant ISM phase (30% by mass)● Quiescent gas (needed for star formation)● Relation to molecular hydrogen (condensation?)● Intricate small-scale structure (turbulence?)● Probe of Galactic structure (spiral arms)

Page 8: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

HISA Census Motivation● How is HISA distributed in the Galaxy?

What does this distribution tell us about the mechanism(s) producing the HISA?

What does it tell us about Galactic structure? How does the HISA relate to the rest of the ISM?

● Large area - unbiased survey of cold H I clouds (not merely known dark/molecular clouds)

● High angular resolution - many HISA features are missed at low resolution

Page 9: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

(map: Taylor & Cordes 1993 electron density)

International Galactic Plane Survey

SouthernSurvey(SGPS;ATCA)

VLASurvey(VGPS)

CanadianSurvey(CGPS;DRAO)

McClure-Griffithset al. (2005)

Stil et al. (2006)

Taylor et al. (2003)

Page 10: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

SIAP-like Server Examples

● 36 CGPS HISA 2-D tile images● Modified Cone-search from Brian’s exercise

Comma-separated variable (CSV) table of image metadata read into MySQL database

This read in turn by java routines● Search for atlas tiles covering desired position, output links

to FITS tiles and canned GIF images● Create cutout images covering desired area using C code

called by CSH scripts called by java/HTML● Access both searches with same HTML web form

Page 11: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

See Example.

Page 12: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

SIAP Server, Part II

● Saada package available from France● Installation difficult, but lots of features available● Read PostgreSQL data into package● Requires j2ee● Can display images overlapping cone search● Can read into Aladdin and do object queries● As with previous example, some confusion

between RA+DEC and GLON+GLAT coordinate systems, due to current limitations of software

Page 13: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

See Example.

Page 14: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

Conclusions

● SIAP server works on both systems● Saada is useful for keeping local data and

browsing● Relations flexible but problem to adopt for

custom work (like cutout service)● Version 1.3 has SIAP, Conesearch● Next one will have SSAP, ? End of Sep 2006● Steve's solution compact, robust – example of

custom processing in VO environment● Thanks for Summer School templates (Cone.jsp)

Page 15: Building a Simple Image Server from Available Tools Steven Gibson (Arecibo Observatory, Puerto Rico) NVO Summer School, Aspen, 2006 Petr Škoda (Ondřejov

This work was supported by grant GAČR 205/06/0584 and by the U.S. National Science Foundationthrough Arecibo Observatory.