wp3000 : padova icc contribution 2007-2010 mattia vaccari (mv) gabriele mainetti (gm) & giulia...

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WP3000 : Padova ICC Contribution 2007-2010 Mattia Vaccari (MV) Gabriele Mainetti (GM) & Giulia Rodighiero (GR) University of Padova – Department of Astronomy ASI Review Padova ICC Contribution 1 WP 3000.1 - Partecipazione all'ICC di PACS : fase di sviluppo WP 3000.2 - Partecipazione all'ICC di PACS : fase operativa WP 3000.3 - Partecipazione all'ICC di SPIRE : fase di sviluppo WP 3000.4 - Partecipazione all'ICC di SPIRE : fase operativa

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Page 1: WP3000 : Padova ICC Contribution 2007-2010 Mattia Vaccari (MV) Gabriele Mainetti (GM) & Giulia Rodighiero (GR) University of Padova – Department of Astronomy

WP3000 : Padova ICC Contribution

2007-2010

Mattia Vaccari (MV)Gabriele Mainetti (GM) & Giulia Rodighiero (GR)

University of Padova – Department of Astronomy

ASI Review Padova ICC Contribution 1

WP 3000.1 - Partecipazione all'ICC di PACS : fase di sviluppo

WP 3000.2 - Partecipazione all'ICC di PACS : fase operativa

WP 3000.3 - Partecipazione all'ICC di SPIRE : fase di sviluppo

WP 3000.4 - Partecipazione all'ICC di SPIRE : fase operativa

Page 2: WP3000 : Padova ICC Contribution 2007-2010 Mattia Vaccari (MV) Gabriele Mainetti (GM) & Giulia Rodighiero (GR) University of Padova – Department of Astronomy

PACS & SPIRE ICC Activities

Testing of PACS Instrument Simulator, Pipeline and AOTs

Definition of user requirements for Herschel Data Processing system

Development of Visualization Tools for SPIRE Interactive Analysis

Testing of Herschel Data Processing system at the astronomer level

Following the full Instrument and Data Processing Development Cycle

ASI Review Padova ICC Contribution 2

Page 3: WP3000 : Padova ICC Contribution 2007-2010 Mattia Vaccari (MV) Gabriele Mainetti (GM) & Giulia Rodighiero (GR) University of Padova – Department of Astronomy

A) Test del simulatore strumentale di PACS per l’identificazione di eventuali bachi del software, dal punto di vista di un utente.

B) Sono stati individuati e riportati al working group vari problemi negli output del simulatore. Le frequenti telecon hanno permesso di riportare in modo continuativo le problematiche individuate e di riportarle agli sviluppatori per individuare una soluzione.

C) Le expertise acquisite dal team italiano (GR) nell’utilizzo del software hanno permesso di utilizzarlo come strumento nella preparazione delle osservazioni di Guaranteed e Open Time, creando mappe simulate con le diverse configurazioni richieste dai diversi proposal.

160 μm simulated image

PACS Instrument Simulator

ASI Review 3Padova ICC Contribution

Page 4: WP3000 : Padova ICC Contribution 2007-2010 Mattia Vaccari (MV) Gabriele Mainetti (GM) & Giulia Rodighiero (GR) University of Padova – Department of Astronomy

PACS Pipeline

ASI Review Padova ICC Contribution 4

A) Utilizzo del simulatore per testare alcuni moduli della pipeline del fotometro di PACS

B) - Generazione di timeline simulate corrispondenti alle osservazioni del GT PACS- Esecuzione e test della pipeline sulle timeline simulate- Applicazione dei moduli High-Pass Filtering e PhotProject per produrre mappe del cielo- Utilizzo di dati SOVT2 come input alla pipeline- Partecipazione ai meeting tecnici del GT per la validazione dei vari test della pipeline

C) Questi impegni hanno contribuito ad un’estesa validazione sia del simulatore dello strumento PACS che al software di Data Processing dai raw data al Map Making

Page 5: WP3000 : Padova ICC Contribution 2007-2010 Mattia Vaccari (MV) Gabriele Mainetti (GM) & Giulia Rodighiero (GR) University of Padova – Department of Astronomy

ASI Review Padova ICC Contribution 5

A) Test degli Astronomical Observing Templates (i.e. Observing Modes) per ottimizzare l’esecuzione delle osservazioni per le survey extragalattiche sia nei programmi di Guaranteed Time che di Open Time

B) Individuazione delle migliori strategie osservative, validate dalle successive osservazioni PEP

C) Particolare contributo italiano alla pianificazione del campo COSMOS

A scan mapping strategy with perpendicular “cross-linked” scans was

adopted to homogeneously cover the field and remove correlated noise during data

reduction

Screenshot detailing the coverage of the COSMOS field as observed by the PEP

Guaranteed Time Key Program

PACS AOTs

Page 6: WP3000 : Padova ICC Contribution 2007-2010 Mattia Vaccari (MV) Gabriele Mainetti (GM) & Giulia Rodighiero (GR) University of Padova – Department of Astronomy

Visualization Tools for SPIRE Interactive Analysis

ASI Review Padova ICC Contribution 6

Aim of the work : developing Visualization Tools for Interactive Analysis of SPIRE raw and reduced data (from level 0 to level 2).• Understand the goodness of an observation• Understand any problems of the detectors• Use/manage/visualize the data for further processing

DTMosaic

•DetectorTimelineExplorer is the default viewer for the SPIRE Detector Timeline product within HIPE. In HIPE from version 1 .0.•TimelineSimplePlot in HIPE from version 4.0.•DTMosaic in HIPE from version 5.0 •GM is the owner of the spire_ia_gui package

TimelineSimplePlot

DetectorTimelineExplorerComponent

• Intuitive view of detector arrays• Powerful plotting tools• No Jython involved

Padova efforts focuesd on:1.DetectorTimelineExplorer2.TimelineSimplePlot3.DTMosaic

Level 0.5-1 productDetector Timelines

Two ways : script (Jython) or Graphical User Interface (GUI)

Page 7: WP3000 : Padova ICC Contribution 2007-2010 Mattia Vaccari (MV) Gabriele Mainetti (GM) & Giulia Rodighiero (GR) University of Padova – Department of Astronomy

One of the GUIs at a glance

ASI Review Padova ICC Contribution 7

Page 8: WP3000 : Padova ICC Contribution 2007-2010 Mattia Vaccari (MV) Gabriele Mainetti (GM) & Giulia Rodighiero (GR) University of Padova – Department of Astronomy

SPIRE : Pipeline How-To

ASI Review Padova ICC Contribution 8

Herschel Science Archivehttp://herschel.esac.esa.int/Science_Archive.shtmlGet the data

Explore the data HIPE

Level 0 - Raw dataLevel 0.5Level 1Level 2 - Reduced data

Reprocess (if you need) HIPE + JYTHON Official Pipeline scriptYour pipeline scripts

ScienceImage Credit : ESA / SPIRE / HerMES

http://herschel.cf.ac.uk/results/lockman-hole

Page 9: WP3000 : Padova ICC Contribution 2007-2010 Mattia Vaccari (MV) Gabriele Mainetti (GM) & Giulia Rodighiero (GR) University of Padova – Department of Astronomy

Herschel DP CCB & Users Group Activities

MV represented SPIRE within the Herschel Data Processing (DP) Configuration Control Board (CCB) and Users Group (UG) and chaired the SPIRE DP UG

– Assembling and coordinating DP feedback from SPIRE consortium members– Participating into DP CCB telecons and DP UG meetings– Supervising (Mentoring) DP development related to a number of WPs

ASI Review Padova ICC Contribution 9

Development of Herschel DP has benefited from the exposure to a larger pool of dedicated users, stimulating ICC members to take action on issues raised by KPs

The Herschel DP UG has recently spawned a number of DP Interest Groups (IGs), including the “PACS and SPIRE Large Maps & Source Extraction” IG coordinated by Mattia Vaccari as mentor for the related DP WPs

Following SDP papers and the AO for OT, the Herschel DP UG will include new members from the IGs, supporting the newly established Herschel Users Group

Page 10: WP3000 : Padova ICC Contribution 2007-2010 Mattia Vaccari (MV) Gabriele Mainetti (GM) & Giulia Rodighiero (GR) University of Padova – Department of Astronomy

Conclusion : Padova ICC Contribution

GM, GR, MV have represented Padova within the PACS and SPIRE ICCs throughout the 2007-2010 pre-to-post launch timeframe

They have provided a substantial contribution to:– pre-launch development and testing of the Herschel general DP and SPG system– post-launch improvements to general DP and SPG following community feedback– execution of PACS and SPIRE SPG pipelines as part of the HerMES and PEP GT KPs– involvement by the general astronomical community

ASI Review Padova ICC Contribution 10

Their work has ensured that Padova is recognized as an important player within the largest PACS and SPIRE GT KPs, thus continuing its long-time involvement in IRAS, ISO, Spitzer and now Herschel extragalactic survey science

They are now in a position to provide expert knowledge about the instruments and data processing system but also to carry out ground-breaking science with them

They have greatly contributed to providing the ICCs with early astronomers feedback on one hand and to popularizing Herschel and its data processing system within the extragalactic astronomical community at large on the other