Award Abstract # 1028162
CDI-Type II: Understanding the Universe through Scalable Navigation of a Galaxy of Annotations

NSF Org: OIA
OIA-Office of Integrative Activities
Recipient: UNIVERSITY OF PITTSBURGH - OF THE COMMONWEALTH SYSTEM OF HIGHER EDUCATION
Initial Amendment Date: September 14, 2010
Latest Amendment Date: September 14, 2010
Award Number: 1028162
Award Instrument: Standard Grant
Program Manager: Stephen Meacham
smeacham@nsf.gov
 (703)292-7599
OIA
 OIA-Office of Integrative Activities
O/D
 Office Of The Director
Start Date: September 15, 2010
End Date: August 31, 2016 (Estimated)
Total Intended Award Amount: $1,599,841.00
Total Awarded Amount to Date: $1,599,841.00
Funds Obligated to Date: FY 2010 = $1,599,841.00
History of Investigator:
  • Alexandros Labrinidis (Principal Investigator)
    labrinid@cs.pitt.edu
  • Panos Chrysanthis (Co-Principal Investigator)
  • Jeffrey Newman (Co-Principal Investigator)
  • William Wood-Vasey (Co-Principal Investigator)
  • Georgeta-Elisab Marai (Co-Principal Investigator)
Recipient Sponsored Research Office: University of Pittsburgh
4200 FIFTH AVENUE
PITTSBURGH
PA  US  15260-0001
(412)624-7400
Sponsor Congressional District: 12
Primary Place of Performance: University of Pittsburgh
4200 FIFTH AVENUE
PITTSBURGH
PA  US  15260-0001
Primary Place of Performance
Congressional District:
12
Unique Entity Identifier (UEI): MKAGLD59JRL1
Parent UEI:
NSF Program(s): CDI TYPE II
Primary Program Source: 01001011DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s): 7721
Program Element Code(s): 775100
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.083

ABSTRACT

The growing onslaught of astronomical data available presents a great challenge. Astronomy lacks an easy-to-use and scalable way to collect and distribute expert information about objects from datasets of tens of thousands to billions of individual events and objects. Over the next decade, the amount of information available to the typical astronomer will grow by two orders of magnitude both in raw data size and in the number of objects.

This project pursues three research directions, each of which has the potential to transform how astronomers interface with large datasets: (1) a scalable annotation framework to enable linking of observations to specific experiments, models, or other observations; (2) a continuous workflow enactment system that would support automated reasoning in the presence of uncertainty; and (3) a computational framework for interactively analyzing astronomical datasets, allowing the construction and testing of hypotheses.

Project plans include the design and development of a prototype system (AstroShelf) and its evaluation using two timely science programs: (a) Using multi-wavelength data from the DEEP3 and AEGIS surveys, develop methods to incorporate images and catalogs from disparate datasets, allowing us to study how the demographics of galaxies have changed over the last 8 billion years. (b) Using properties of time-variable events found by the Pan-STARRS survey, develop techniques for rapid classification of transient phenomena, dissemination of their properties, and incorporation of feedback from follow-up observations. AstroShelf will include a publicly accessible, flexible annotation system for public datasets, which will also lend itself to outreach efforts involving annotations by the general public.

This project's significant impact is the ability to share information and expert opinions quickly and widely, about each new observation or event, fundamentally changing our ability to learn about the Universe; such functionality can also be applied in support of other scientific domains.

Results of this research will be made publicly available at www.astroshelf.pitt.edu.

PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

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(Showing: 1 - 10 of 11)
Andreas Konstantinidis, George Nikolaides, Georgios Chatzimilioudis, Giannis Evagorou, Demetrios Zeinalipour-Yazti, Panos K. Chrysanthis "Radiomap Prefetching for Indoor Navigation in Intermittently Connected Wi-Fi Networks" 16th IEEE International Conference on Mobile Data Management (MDM) , 2015 10.1109/MDM.2015.45
Angen Zheng, Alexandros Labrinidis, Panos K. Chrysanthis "Planar: Parallel Lightweight Architecture-Aware Adaptive Graph Repartitioning" 2016 IEEE 32nd International Conference on Data Engineering (ICDE) , 2016 10.1109/ICDE.2016.7498234
Angen Zheng, Alexandros Labrinidis, Patrick Pisciuneri, Panos K. Chrysanthis, Peyman Givi "PARAGON: Parallel Architecture-Aware Graph Partition Refinement Algorithm" 19th International Conference on Extending Database Technology (EDBT) , 2016 10.5441/002/edbt.2016.34
Anja Weyant, W. Michael Wood-Vasey, Lori Allen, Peter M. Garnavich, Saurabh W. Jha, Richard Joyce, and Thomas Matheson "weetSpot: Near-infrared Observations of 13 Type Ia Supernovae from a New NOAO Survey Probing the Nearby Smooth Hubble Flow" The Astrophysical Journal , v.784 , 2014 10.1088/0004-637X/784/2/105
Cory Thoma, Adam J. Lee, Alexandros Labrinidis "PolyStream: Cryptographically Enforced Access Controls for Outsourced Data Stream Processing" 21st ACM Symposium on Access Control Models and Technologies (SACMAT) , 2016 10.1145/2914642.2914660
Humaira Ehsan, Mohamed A. Sharaf, Panos K. Chrysanthis "MuVE: Efficient Multi-Objective View Recommendation for Visual Data Exploration" 32nd IEEE International Conference on Data Engineering (ICDE) , 2016 10.1109/ICDE.2016.7498285
H. V. Jagadish, Johannes Gehrke, Alexandros Labrinidis, Yannis Papakonstantinou, Jignesh M. Patel, Raghu Ramakrishnan, Cyrus Shahabi "Big Data and Its Technical Challenges" Communications of the ACM , v.57 , 2014 , p.86 10.1145/2611567
Stavros Papastavrou, Panos K. Chrysanthis, George Samaras "Performance vs. freshness in web database applications" World-Wide Web , v.17 , 2013 , p.969 10.1007/s11280-013-0262-0
Thao N. Pham, Panos K. Chrysanthis, Alexandros Labrinidis "Avoiding class warfare: Managing Continuous Queries with Differentiated Classes of Service" The VLDB Journal , v.25 , 2016 10.1007/s00778-015-0411-4
T. Luciani, B. Cherinka, D. Oliphant, S. Myers, W.M. Wood-Vasey, A. Labrinidis, G.E. Marai "Large-Scale Overlays and Trends: Visually Mining, Panning and Zooming the Observable Universe" IEEE Transactions on Visualization and Computer Graphics , v.7 , 2014
T. Luciani, J. Wenskovitch, K. Chen, D. Koes, T. Travers, G.E. Marai "FixingTIM: Interactive Exploration of Sequence and Structural Data to Identify Functional Mutations in Protein Families" BMC Proceedings , v.8 , 2014
(Showing: 1 - 10 of 11)

PROJECT OUTCOMES REPORT

Disclaimer

This Project Outcomes Report for the General Public is displayed verbatim as submitted by the Principal Investigator (PI) for this award. Any opinions, findings, and conclusions or recommendations expressed in this Report are those of the PI and do not necessarily reflect the views of the National Science Foundation; NSF has not approved or endorsed its content.

This project brought together astronomers and computer scientists (experts in data management and in data visualization) with the goal of creating a tool that would allow astronomers to easily explore, search, and annotate large-scale astronomical survey data. The project considered scalability both from a systems point-of-view (i.e., how to make the system work fast, despite the large volumes of data) and from a human point-of-view (i.e., how to make it easy for humans to discern interesting information/patterns from large data sets).

The developed tool, AstroShelf, is an easy to use dashboard, that has the following novel features: 

  • ability to visually overlay different data sources (e.g., SDSS and LSST) on top of each other, with knobs to adjust the transparency,
  • ability to aggregate multiple data points as trend images, in order to facilitate pattern discovery,
  • ability to show stamp-sized previews of the results, organized in a compressed way, and
  • ability to interact with AstroShelf through a web-based user interface, but also programmatically, allowing mixed use (e.g., adding a few annotations using the web site and then accessing these through a program). 

The developed technologies also include:

  • support for multiple types of query personalization, and 
  • a new type of workflows, called continuous workflows, perfectly suited for complex alerting queries

As a proof of concept for using Astroshelf as a platform for the sharing of databases of astronomical objects of interest, we have used the public Astroshelf tools to share a catalog of Milky Way Analogs: galaxies that, based upon their mass and star formation histories, should closely resemble our own Milky Way Galaxy.  Ideas from AstroShelf have informed efforts on visualization and analysis frameworks for two major astronomical surveys: the 4th generation of the Sloan Digital Sky Survey, and the Large Synoptic Survey Telescope.

The project has had a significant impact on the training of the next generation of astronomers and computer scientists. It has involved 20 graduate students (7 of which where female) in different stages of their studies as well as four undergraduate students (one of whom pursued graduate studies).

The deliverables of the project include a web site (http://astro.cs.pitt.edu), a full code release on github (https://github.com/admtlab/astroshelfv3/) and two instructional YouTube videos that summarize/demonstrate the AstroShelf project from a regular user point of view (http://bit.ly/astroshelf1) and from a programmer user point of view (http://bit.ly/astroshelf2).


Last Modified: 04/04/2017
Modified by: Alexandros Labrinidis

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