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CREATING A MULTI-WAVELENGTH
GALACTIC PLANE ATLAS WITH
AMAZON WEB SERVICES
G. Bruce Berriman, John Good
IPAC, California Institute of Technology
Ewa Deelman, Gideon Juve, Mats Rynge
ISI, University of Southern California
Jamie Kinney, Ann Merrihew
Amazon Web Services
How Can Astronomers Use The Cloud?
• How well can we …
• Manage virtual machines and operate a virtual
cluster for processing data.
• Abstract the technical details of processing
from astronomers.
• Optimize processing and manage costs.
• Exploit cloud storage in operations.
• Create turnkey tools for astronomers to exploit
cloud platforms.
A Multi-wavelength Image Atlas of the
Galactic Plane
• Use open source tools to create a new data product
on the Amazon Elastic Compute Cloud (EC2).
• 16 wavelengths from 1μm to 24 μm.
• Coverage l = 0° - 360°; b = ±20°.
• Processed at 1 arcsec spatial sampling, Cartesian
projection, Galactic coordinates.
The Montage Image Mosaic Engine
• ANSI-C Toolkit for creating and managing
image mosaics in FITS format.
• Portable and scalable – runs on all Unix
platforms.
• BSD 3-clause license.
• Widely adopted by astronomy and IT
communities.
5Montage Workflow
Reprojection Background Rectification Co-addition OutputInput
BgModel
Project
Project
Project
Diff
Diff
Fitplane
Fitplane
Background
Background
Background
Add
Image1
Image2
Image3
http://montage.ipac.caltech.edu
Three-color Spitzer mosaic of the LMC created from
300,000 frames. Seven degrees on a side.
Blue - 3.6 μm; green- 8 μm red - 24 μm
The Pegasus Workflow Management
System
• Pegasus is a workflow planner
• Mature and used in many fields.
• Takes abstract descriptions of workflows
and sets up and runs a processing plan
for an environment whose configuration
is incorporated into workflow manager.
• Layered on HTCondor (scheduler) and
DAGMan (submits jobs to HTCondor in
the correct order).
• EC2 environment is already known to
Pegasus.
• Abstract Workflows
• Directed Acyclical Graphs
• Identifies the computational flow and
dependencies. http://pegasus.isi.edu
Galactic Plane
Workflow
16 hierarchical workflows
Each one with 1,001 sub-
workflows
Over 10M input files
45 TB output dataset
System Architecture Design
Be careful about your choices.
• Amazon offers a wide range of instance types and costs
of running applications can vary widely.
• hi1.4xlarge (the one we used)
• Memory optimized, with 2 x SSD ephemeral drives.
• 318,000 core hours.
• Spot instance price: US $5,950.
• cc2.8xlarge (benchmarked)
• Compute cluster optimized, with 4 ephemeral drives (2
used.)
• 274,000 core hours.
• Spot instance price: US $2,200.
• Best practice: do a cost benefit analysis or
benchmarking.
Multi-Color Mosaics
Top to bottom: 2MASS, GLIMPSE, MSX, WISE
Three color mosaics near NGC 6537
Three color-infrared images of the
Galactic Plane, extracted from the 16-
wavelength Galactic Plane Atlas.
Top left: 2MASS 1.2 μm, 1.6 μm, 2.2
μm
Top right: GLIMPSE 4.5 μm, 5.8 μm
and 8 μm
Bottom left: 2MASS 1.2 μm,
GLIMPSE 8.0 μm, MSX 21.3μm
WISE Mosaics
Top to bottom: 3.4 mm, 4.6 mm, 12 mm, 22 mm.
http://vaoweb2.ipac.caltech.edu/cgi-bin/GalPlane/nph-gpInit
What Have We Learned?
• Amazon EC2 is a powerful platform for
astronomical computing.
• Open Source tools are invaluable for taking
advantage of it.
• Optimizing operations requires human
intervention.
• Be mindful of pay-as-you-go: need to do cost
benefit analyses, benchmarking for optimization.
• High latency in recovering images from S3
storage.
Next Generation Montage: Data Cubes
The structure of a molecular disk wind
in HD 163296, measured by ALMA (PI: M. Rawlings).
Re-projection by Montage of a data cube of the star that
covers multiple velocities relative to the center of the CO J=3-
2 line. Shown are images at four velocities.
Next Generation Montage: Sky
Partitioning Schemes
Transform HEALPix images,
standard in cosmic background
missions, for multi-wavelength
image analysis and visualization.
353 GHz all-sky map measured
by Planck.
Re-project images to TOAST and
visualize in World Wide
Telescope

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Creating A Multi-wavelength Galactic Plane Atlas With Amazon Web Services

  • 1. CREATING A MULTI-WAVELENGTH GALACTIC PLANE ATLAS WITH AMAZON WEB SERVICES G. Bruce Berriman, John Good IPAC, California Institute of Technology Ewa Deelman, Gideon Juve, Mats Rynge ISI, University of Southern California Jamie Kinney, Ann Merrihew Amazon Web Services
  • 2.
  • 3. How Can Astronomers Use The Cloud? • How well can we … • Manage virtual machines and operate a virtual cluster for processing data. • Abstract the technical details of processing from astronomers. • Optimize processing and manage costs. • Exploit cloud storage in operations. • Create turnkey tools for astronomers to exploit cloud platforms.
  • 4. A Multi-wavelength Image Atlas of the Galactic Plane • Use open source tools to create a new data product on the Amazon Elastic Compute Cloud (EC2). • 16 wavelengths from 1μm to 24 μm. • Coverage l = 0° - 360°; b = ±20°. • Processed at 1 arcsec spatial sampling, Cartesian projection, Galactic coordinates.
  • 5. The Montage Image Mosaic Engine • ANSI-C Toolkit for creating and managing image mosaics in FITS format. • Portable and scalable – runs on all Unix platforms. • BSD 3-clause license. • Widely adopted by astronomy and IT communities. 5Montage Workflow Reprojection Background Rectification Co-addition OutputInput BgModel Project Project Project Diff Diff Fitplane Fitplane Background Background Background Add Image1 Image2 Image3 http://montage.ipac.caltech.edu Three-color Spitzer mosaic of the LMC created from 300,000 frames. Seven degrees on a side. Blue - 3.6 μm; green- 8 μm red - 24 μm
  • 6. The Pegasus Workflow Management System • Pegasus is a workflow planner • Mature and used in many fields. • Takes abstract descriptions of workflows and sets up and runs a processing plan for an environment whose configuration is incorporated into workflow manager. • Layered on HTCondor (scheduler) and DAGMan (submits jobs to HTCondor in the correct order). • EC2 environment is already known to Pegasus. • Abstract Workflows • Directed Acyclical Graphs • Identifies the computational flow and dependencies. http://pegasus.isi.edu
  • 7. Galactic Plane Workflow 16 hierarchical workflows Each one with 1,001 sub- workflows Over 10M input files 45 TB output dataset
  • 9. Be careful about your choices. • Amazon offers a wide range of instance types and costs of running applications can vary widely. • hi1.4xlarge (the one we used) • Memory optimized, with 2 x SSD ephemeral drives. • 318,000 core hours. • Spot instance price: US $5,950. • cc2.8xlarge (benchmarked) • Compute cluster optimized, with 4 ephemeral drives (2 used.) • 274,000 core hours. • Spot instance price: US $2,200. • Best practice: do a cost benefit analysis or benchmarking.
  • 10. Multi-Color Mosaics Top to bottom: 2MASS, GLIMPSE, MSX, WISE
  • 11. Three color mosaics near NGC 6537 Three color-infrared images of the Galactic Plane, extracted from the 16- wavelength Galactic Plane Atlas. Top left: 2MASS 1.2 μm, 1.6 μm, 2.2 μm Top right: GLIMPSE 4.5 μm, 5.8 μm and 8 μm Bottom left: 2MASS 1.2 μm, GLIMPSE 8.0 μm, MSX 21.3μm
  • 12. WISE Mosaics Top to bottom: 3.4 mm, 4.6 mm, 12 mm, 22 mm.
  • 14. What Have We Learned? • Amazon EC2 is a powerful platform for astronomical computing. • Open Source tools are invaluable for taking advantage of it. • Optimizing operations requires human intervention. • Be mindful of pay-as-you-go: need to do cost benefit analyses, benchmarking for optimization. • High latency in recovering images from S3 storage.
  • 15. Next Generation Montage: Data Cubes The structure of a molecular disk wind in HD 163296, measured by ALMA (PI: M. Rawlings). Re-projection by Montage of a data cube of the star that covers multiple velocities relative to the center of the CO J=3- 2 line. Shown are images at four velocities.
  • 16.
  • 17. Next Generation Montage: Sky Partitioning Schemes Transform HEALPix images, standard in cosmic background missions, for multi-wavelength image analysis and visualization. 353 GHz all-sky map measured by Planck. Re-project images to TOAST and visualize in World Wide Telescope

Hinweis der Redaktion

  1. http://vaoweb2.ipac.caltech.edu/cgi-bin/GalPlane/nph-gpInit