The Processing and Archiving Unit of the Javalambre Astrophysical - - PowerPoint PPT Presentation

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The Processing and Archiving Unit of the Javalambre Astrophysical - - PowerPoint PPT Presentation

The Processing and Archiving Unit of the Javalambre Astrophysical Observatory. A. Ederoclite CE F CA A. Ederoclite UPAD OAJ Heidelberg, 10 June 2013 1 of 17 J-PAS Expected Beginning: 2015 Expected Duration: 5 7 years A. Ederoclite


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SLIDE 1
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 1 of 17

The Processing and Archiving Unit

  • f the Javalambre Astrophysical

Observatory.

  • A. Ederoclite

CEFCA

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SLIDE 2
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 2 of 17

J-PAS

Expected Beginning: 2015 Expected Duration: 5 – 7 years

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SLIDE 3
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 3 of 17

The Javalambre Astrophysical Observatory (OAJ)

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SLIDE 4
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 4 of 17

The Javalambre Astrophysical Observatory (OAJ)

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SLIDE 5
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 5 of 17

The Javalambre Astrophysical Observatory (OAJ)

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SLIDE 6
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 6 of 17

The JST/T250 ⇒ J-PAS

14 9.2k×9.2k CCDs ⇒ 180.3 MB (2.5 GB per exposure)

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SLIDE 7
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 7 of 17

The JAST/T80 ⇒ J-PLUS

10k×10k CCDs ⇒ 236.5 MB

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SLIDE 8
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 8 of 17

The OAJ/CPD

CPD

OAJ Core Access Switch

Services CPD I/O CPD CPU CPD Disk 100 TB

OAJ Firewall

T80 T250

Tape

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SLIDE 9
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 9 of 17

The Data Transfer

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SLIDE 10
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 10 of 17

The UPAD/T80

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SLIDE 11
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 11 of 17

The UPAD

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SLIDE 12
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 12 of 17

Data Volumes

J-PLUS J-PAS Raw Images ∼40 TB ∼1.2 PB Reduced Images ∼32 TB ∼760 TB Final Catalog * 2 TB 10 TB We want to keep at least DRn and DRn−1 * We expect some 1 × 108 galaxies with 0.3% photo-z (and 3 × 108 with 1% photo-z). For each record, we expect about 60 fields (trick: some fields are arrays which have 56 values).

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SLIDE 13
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 13 of 17

The External Access

“DMZ” ≃ external data access zone

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SLIDE 14
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 14 of 17

Accessing Images

Providing images in a “DSS” way: possibility to define position and size. Provide “data-cubes” and/or tiles (∼ 30 × 30arcmin2). Example of the ALHAMBRA survey (figure from Molino et al. in prep.)

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SLIDE 15
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 15 of 17

Accessing Catalogs

Position X IMAGE, Y IMAGE, ALPHA 2000, DELTA 2000 Fluxes (and errors) MAG APER, MAG ISO, MAG AUTO, Shape KRON RADIUS, PETRO RADIUS, R EFF , FWHM WORLD, A WORLD, B WORLD, THETA J2000 Other CLASS STAR, FLUX MAX, MU MAX,BACKGROUND, THRESHOLD, FLAG Dual mode and Single mode. J-PAS: photo-z J-PLUS: log g, Z, Teff Variable sources (∼ 200 new variable candidates per night).

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SLIDE 16
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 16 of 17

OAJ and the Virtual Observatory

VO-compliancy has been a requirement since the beginning of the project. The database is being designed to be VO-compliant. Basic services already implemented (cone search and TAP access). ADQL queries.

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SLIDE 17
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 16 of 17

OAJ and the Virtual Observatory

VO-compliancy has been a requirement since the beginning of the project. The database is being designed to be VO-compliant. Basic services already implemented (cone search and TAP access). ADQL queries. Next talks:

◮ What is Publishing to the VO? [Markus Demleitner] ⇒

change “brain chip” from “user” to “provider”

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SLIDE 18
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 16 of 17

OAJ and the Virtual Observatory

VO-compliancy has been a requirement since the beginning of the project. The database is being designed to be VO-compliant. Basic services already implemented (cone search and TAP access). ADQL queries. Next talks:

◮ What is Publishing to the VO? [Markus Demleitner] ⇒

change “brain chip” from “user” to “provider”

◮ Why Publish to the VO? [S´

everin Gaudet] ⇒ “The success of a large project like J-PAS can be measured from the amount

  • f people, not involved in the project, who used the data”

(M. Moles)

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SLIDE 19
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 16 of 17

OAJ and the Virtual Observatory

VO-compliancy has been a requirement since the beginning of the project. The database is being designed to be VO-compliant. Basic services already implemented (cone search and TAP access). ADQL queries. Next talks:

◮ What is Publishing to the VO? [Markus Demleitner] ⇒

change “brain chip” from “user” to “provider”

◮ Why Publish to the VO? [S´

everin Gaudet] ⇒ “The success of a large project like J-PAS can be measured from the amount

  • f people, not involved in the project, who used the data”

(M. Moles)

◮ How to Publish to the VO. [Marco Molinaro] ⇒ Right, how?

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SLIDE 20
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 17 of 17

Summary

◮ OAJ ⇒ a new astronomical facility in Europe ◮ J-PAS and J-PLUS: 2 multi-band surveys of ∼8000 sq.deg. ◮ OAJ/CPD already bought and ready to be installed. ◮ UPAD/T80 already bought and ready to be installed. ◮ UPAD/T250 in definition phase. ◮ External Access:

◮ VO compliant ◮ images ◮ catalgs

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SLIDE 21
  • A. Ederoclite – UPAD OAJ

Heidelberg, 10 June 2013 17 of 17

Summary

◮ OAJ ⇒ a new astronomical facility in Europe ◮ J-PAS and J-PLUS: 2 multi-band surveys of ∼8000 sq.deg. ◮ OAJ/CPD already bought and ready to be installed. ◮ UPAD/T80 already bought and ready to be installed. ◮ UPAD/T250 in definition phase. ◮ External Access:

◮ VO compliant ◮ images ◮ catalgs

Danke!