The final programme can also be downloaded here.
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9.30
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Manchado, Arturo: Welcome address
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9.40
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Aggarwal, Kanti: Atomic data and their applications and assessment
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10.35
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Bautista, Manuel: Atomic data for neutral and singly ionized species. problems and limitations |
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11.30
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Coffee break
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12.00
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Shaw, Richard: Toward precision abundances in nebular Astrophysics
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12.30
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Wesson, Roger: Estimating uncertainties in analyses of ionised nebulae
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13.00
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Organization of work groups
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13.30
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Lunch
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15.30
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Aggarwal, Bautista, Shaw, Wesson. Panel discussion:
• How reliable are uncertainties in atomic data?
• Where are the breakthroughs in atomic data generation likely to be? • How do current uncertainties limit applications to nebular astrophysics? • What precision is attainable?
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17.00
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Coffee break
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17.30
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Work groups
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9.30
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Mendoza, Claudio: Uncertainties in the Ne V infrared diagnostics
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10.00
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Ferland, Gary: Uncertainties in theoretical He I emissivities
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10.30
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Luridiana, Valentina: The new nebular software |
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11.00
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Coffee break
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11.30
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Shaw, Richard: A comparison between the ELSA and nebular abundance codes |
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12.10
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Bergemann, Maria: Role of input atomic data in spectroscopic analyses of the Sun and metal-poor stars |
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12.50
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Lind, Karin: The impact of new collisional data on stellar abundance determination of Li and Na |
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13.30
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Lunch
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15.30
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Mendoza, Ferland, Shaw, Simón-Díaz. Panel discussion:
• For which ions (including s-process elements) are new, better atomic data urgently required? • Which observations might serve as feedback to atomic data calculations? • Can we trust atomic data? Paradigmatic cases.
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17.00
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Coffee break
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17.30
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Work groups
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20.30
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Dinner
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| 9.30 | Ferland, Gary: The Cloudy atomic data base - future goals |
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10.00
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Mendoza, Claudio: VAMDC: Virtual Atomic and Molecular Data Centre
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10.30
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Del Zanna, Giulio: Atomic data for astrophysics: calculations, benchmarks and distribution |
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11.00
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Coffee break
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11.30
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Ferland, Mendoza, Aggarwal, Del Zanna. Panel discussion: Creation of a database and organization of data user communities. • Is a database a la Mendoza 1983 feasible? • How should uncertainties be included? • Which functionalities should be added to allow comparison? • How can the interaction between users and producers be made more efficient? |
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12.45
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Concluding remarks
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13.15
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Lunch
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14.30
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Visit to the Teide Observatory
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1) Organization of a user-friendly database
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2) Preparation of a quick start guide for atomic data users: general introduction to the topic, what is what, where to choose, how to assess data, etc. The following is a (very approximate) example of draft: |
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• The atom
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• Level diagrams of main ions
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• Spectroscopic notation
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• What is reported in papers
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• Experimental vs. theoretical data
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• Atomic data: how they are determined, typical uncertainties |
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• Collisional data: theoretical vs experimental; how they are computed; different methods; typical uncertainties |
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• What is published in papers; collision strengths vs effective collision strengths. |
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• Databases
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