Legal Aspects of Open Science: the EU Perspective, Krzysztof Siewicz, University of Warsaw

•

0 likes•722 views

Conference Opening Science to Meet Future Challenges, Warsaw, March 11, 2014, organized by Interdisciplinary Centre for Mathematical and Computational Modelling, University of Warsaw.

Science

Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl
4

Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl
4
Horizon
2020
EC
Recommendations
Amended PSI
Directive
Copyright
framework

Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl

Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl
gratis, not necessarily libre
details in grant agreements
(MGA not too elaborate)
open data not mandatory, but Open Data Pilot

Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl
NO MANDATE FOR LIBRARIES
If "IPRs" held by libraries (including university libraries, museums and
archives), the re-use is possible only if it is allowed (not clear by whom)
SOFT OBLIGATIONS
(open formats, cf. definition; transparent fees; no unreasonable limitations in
license)

Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl
mandate, not just encourage, libre
liberalize copyright
harmonize PSI & set it free

Credits:
- https://ec.europa.eu/programmes/horizon2020/sites/horizon2020/files/FactSheet_Open_Access.pdf
- The unnamed, Freedom, http://www.flickr.com/photos/unnamed/47093936/ (CC BY-SA 2.0)
- Unhindered by Talent, Free Beer, http://www.flickr.com/photos/nicmcphee/2345633527/ (CC BY SA 2.0)
- http://ec.europa.eu/research/participants/data/ref/h2020/legal_basis/rules_participation/
h2020-rules-participation_en.pdf
- http://ec.europa.eu/research/science-society/document_library/pdf_06/
recommendation-access-and-preservation-scientific-information_en.pdf
- http://ec.europa.eu/digital-agenda/en/european-legislation-reuse-public-sector-information
- http://ec.europa.eu/internal_market/consultations/2013/copyright-rules/index_en.htm
- http://ec.europa.eu/internal_market/consultations/2013/copyright-rules/docs/
consultation-document_en.pdf

Thank You for Your attention
The content of this presentation is available under Creative Commons
Attribution 3.0 PL License
(http://creativecommons.org/licenses/by/3.0/pl/legalcode)

More from Platforma Otwartej Nauki

Umowy dot. autorskich praw majątkowych w praktyce wydawców książek naukowych

Platforma Otwartej Nauki

Prawne aspekty otwartego dostępu

Platforma Otwartej Nauki

Monografie Naukowe - Uniwersytet Śląski

Platforma Otwartej Nauki

DSpace - doświadczenia Repozytorium Uniwersytetu Łódzkiego

Platforma Otwartej Nauki

Platforma czasopism Wydawnictwa Uniwersytetu Łódzkiego

Platforma Otwartej Nauki

Biblioteka Nauki - techniczne możliwości wymiany metadanych

Platforma Otwartej Nauki

Monografie w Bibliotece Nauki

Platforma Otwartej Nauki

Open Science Platform

Platforma Otwartej Nauki

OpenAIRE Services for Open Science

Platforma Otwartej Nauki

Publikacje Ośrodka Badawczego Facta Ficta w Bibliotece Nauki

Platforma Otwartej Nauki

PRESSto Platfoma otwartych czasopism naukowych UAM

Platforma Otwartej Nauki

Publikacje Instytutu Historii Ukrainy w Bibliotece Nauki

Platforma Otwartej Nauki

Polska Akademia Nauk a otwarta nauka

Platforma Otwartej Nauki

Otwarty dostęp do publikacji naukowych GUS - doświadczenia i wyzwania

Platforma Otwartej Nauki

Making Open Access Book Funding Work Fairly

Platforma Otwartej Nauki

UCL Press. The UK's first fully open access university press

Platforma Otwartej Nauki

Funding open access books at Open Book Publishers

Platforma Otwartej Nauki

Discussion panel during the conference celebrating the public launch of the new platform of the Library of Science (https://bibliotekanauki.pl), developed by the Interdisciplinary Centre for Mathematical and Computational Modelling, University of Warsaw, in cooperation with publishers, journal editorial boards, and indexing databases. The Library of Science is an Open Access collection of Polish scientific journals and books. All the resources are available as full texts with metadata. Panelists presented their individual experiences from the development of local and regional infrastructures for Open Access to scientific journals. Panelists: Arianna Becerril García (Redalyc) Miroslav Milinović (HRČAK) Susan Murray (AJOL) Ritsuko Nakajima (J-STAGE) Abel L Packer (SciELO) moderator: Krzysztof Siewicz (ICM UW) Recording: https://youtu.be/q8bfstI5vpE The new version of the platform was developed in the framework of the “Platform of Polish Scientific Publications” project, co-financed from the European Regional Development Fund, 2nd priority axis of the Operational Program Digital Poland 2014-2020, Measure 2.3 (total project value: PLN 5,164,777.78, co-financing from European Funds: PLN 4,370,951.43).

Arianna Becerril García – Redalyc: A platform to advance non-commercial Open ...

Platforma Otwartej Nauki

Abel L Packer – SciELO advances as an Open Science program

Platforma Otwartej Nauki

Prezentacja: dr Laura Bandura-Morgan (Narodowe Centrum Nauki) Krajowe Warsztaty Otwartego Dostępu OpenAIRE 2020, Polska Polityki otwartości w Polsce Cześć 2: dane badawcze 25 listopada 2020, online OpenAIRE National Workshop in Poland (2020), organized as part of the OpenAIRE Advance project, was be devoted to the implementation of open access policies in Polish scientific institutions. http://pon.edu.pl/politykiotwartosci/

Open Data - zarządzanie danymi w projektach badawczych NCN

Platforma Otwartej Nauki

More from Platforma Otwartej Nauki (20)

Umowy dot. autorskich praw majątkowych w praktyce wydawców książek naukowych

Prawne aspekty otwartego dostępu

Monografie Naukowe - Uniwersytet Śląski

DSpace - doświadczenia Repozytorium Uniwersytetu Łódzkiego

Platforma czasopism Wydawnictwa Uniwersytetu Łódzkiego

Biblioteka Nauki - techniczne możliwości wymiany metadanych

Monografie w Bibliotece Nauki

Open Science Platform

OpenAIRE Services for Open Science

Publikacje Ośrodka Badawczego Facta Ficta w Bibliotece Nauki

PRESSto Platfoma otwartych czasopism naukowych UAM

Publikacje Instytutu Historii Ukrainy w Bibliotece Nauki

Polska Akademia Nauk a otwarta nauka

Otwarty dostęp do publikacji naukowych GUS - doświadczenia i wyzwania

Making Open Access Book Funding Work Fairly

UCL Press. The UK's first fully open access university press

Funding open access books at Open Book Publishers

Arianna Becerril García – Redalyc: A platform to advance non-commercial Open ...

Abel L Packer – SciELO advances as an Open Science program

Open Data - zarządzanie danymi w projektach badawczych NCN

Recently uploaded

BooK Now Call us at +918448380779 to hire a gorgeous and seductive call girl for sex. Take a Delhi Escort Service. The help of our escort agency is mostly meant for men who want sexual Indian Escorts In Delhi NCR. It should be noted that any impersonator will get 100 attention from our Young Girls Escorts in Delhi. They will assume the position of reliable allies. VIP Call Girl With Original Photos Book Tonight +918448380779 Our Cheap Price 1 Hour not available 2 Hours 5000 Full Night 8000 TAG: Call Girls in Delhi, Noida, Gurgaon, Ghaziabad, Connaught Place, Greater Kailash Delhi, Lajpat Nagar Delhi, Mayur Vihar Delhi, Chanakyapuri Delhi, New Friends Colony Delhi, Majnu Ka Tilla, Karol Bagh, Malviya Nagar, Saket, Khan Market, Noida Sector 18, Noida Sector 76, Noida Sector 51, Gurgaon Mg Road, Iffco Chowk Gurgaon, Rajiv Chowk Gurgaon All Delhi Ncr Free Home Deliver

Stunning ➥8448380779▻ Call Girls In Panchshil Enclave Delhi NCR

Delhi Call girls

Jupiter’s moon Io hosts extensive volcanism, driven by tidal heating. The isotopic composition of Io's inventory of volatile chemical elements, including sulfur and chlorine, reflects its outgassing and mass loss history, and thus records information about its evolution. We used millimeter observations of Io’s atmosphere to measure sulfur isotopes in gaseous SO2 and SO, and chlorine isotopes in gaseous NaCl and KCl. We find 34S/32S = 0.0595 ± 0.0038 (equivalent to δ34S = +347 ± 86‰), which is highly enriched compared to average Solar System values and indicates that Io has lost 94 to 99% of its available sulfur. Our measurement of 37Cl/35Cl = 0.403 ± 0.028 (δ37Cl = +263 ± 88‰) shows that chlorine is similarly enriched. These results indicate that Io has been volcanically active for most (or all) of its history, with potentially higher outgassing and mass-loss rates at earlier times.

Isotopic evidence of long-lived volcanism on Io

Sérgio Sacani

Mustard, as a crop, is susceptible to a variety of pests that can affect its growth and yield. Here’s a rundown of some common pests that target mustard plants: Aphids: These small, sap-sucking insects can cause significant damage by feeding on the leaves and stems. Aphids also excrete a sticky substance known as honeydew, which can lead to the growth of sooty mold on the plants. Flea Beetles: These tiny beetles jump like fleas when disturbed and chew small holes in the leaves. They are particularly damaging in the early growth stages of the plant. Cabbage Loopers: The larvae of a type of moth, these caterpillars are known for their distinctive looping movement. They chew large holes in the leaves and can defoliate plants if present in large numbers. Diamondback Moth Larvae: Another caterpillar pest, these larvae chew small holes in the leaves and can cause extensive damage, especially when infestations are heavy. Whiteflies: These are tiny, winged insects that feed on plant sap and can quickly become a problem in greenhouse or close planting conditions. Like aphids, they also secrete honeydew. Cutworms: These are the larvae of certain types of moths and are known for cutting young plants at the stem base at ground level. They are most destructive during the night. Root Maggots: The larvae of root maggot flies, these pests attack the roots of mustard plants, causing wilting and potentially killing young plants. Harlequin Bugs: These are colorful stink bugs that suck the sap from mustard plant stems and leaves, causing the leaves to become stippled, wilt, and eventually die if the infestation is severe. Mustard Sawfly: The larvae of the mustard sawfly can cause considerable defoliation, as they feed voraciously on the leaves. Clubroot: Caused by a fungus-like organism, clubroot affects the roots, causing them to swell and distort. While technically a disease, it is often associated with pest management because controlling it involves similar preventative strategies. Control Measures: Managing pests in mustard involves a combination of cultural, biological, and chemical methods. Crop rotation, resistant varieties, timely sowing, maintaining plant health, and using natural predators like ladybugs and parasitic wasps can help keep pest populations under control. Chemical pesticides should be used as a last resort due to their potential impact on the environment and non-target species.

Pests of mustard_Identification_Management_Dr.UPR.pdf

PirithiRaju

Pulmonary drug delivery system M.pharm -2nd sem P'ceutics

sakshisoni2385

HotJupiters are amongthebest-studied exoplanets, but it is still poorly understood how their chemical composition and cloud properties vary with longitude. Theoretical models predict that clouds may condense on the nightside and that molecular abundances can be driven out of equilibrium by zonal winds. Here we report a phase-resolved emission spectrum of the hot Jupiter WASP-43b measured from 5–12µ 5–12µ 5–12µm with JWST’s Mid-Infrared Instrument (MIRI). 1524 ±35 1524 ±35 and 863±23 The spectra reveal a large day–night temperature contrast (with average brightness temperatures of 1524 ± 35 863 ±23 863 ±23Kelvin, respectively) and evidence for water absorption at all orbital phases. Comparisons with three-dimensional atmospheric models show that both the phase curve shape and emission spectra strongly suggest the presence of nightside clouds which become optically thick to thermal emission at pressures greater than ∼100mbar. The dayside is consistent with a cloudless atmosphere above the mid-infrared photosphere. Con3trary to expectations from equilibrium chemistry but consistent with disequilibrium kinetics models, methane is not detected on the nightside (2σ upper limit of 1–6 parts per million, depending on model assumptions).

Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b

Sérgio Sacani

Raman spectroscopy.pptx M Pharm, M Sc, Advanced Spectral Analysis

Diwakar Mishra

Small size (20-300 nm) / bacteria (size measured in μm) Viral genome – single type of nucleic acid: DNA – dezoxyriboviruses RNA - riboviruses Totally dependant on living cells for all metabolic processes May infect humans, animals, plants, bacteria, fungi,parasites, insects Virion = viral corpuscle = elementary, infectious unit. Only visible by electron microscopy. Laboratory diagnosis of viral infections Methods: • Cytology • Electron microscopy • Cultivation • Detection of viral proteins • Serology • Molecular diagnosis (detection of genetic material i.e. nucleic acids) PPT prepared by Dr. Prince C P

VIRUSES structure and classification ppt by Dr.Prince C P

PRINCE C P

Chromatin Structure | EUCHROMATIN | HETEROCHROMATIN

sankalpkumarsahoo174

GBSN - Biochemistry (Unit 1)

Areesha Ahmad

A botany file is similar to a chemistry practical file but specifically focuses on experiments and observations related to plants. It typically includes detailed descriptions of plant-related experiments, such as germination studies, growth experiments, tissue culture techniques, plant anatomy investigations, and ecological surveys. The file may contain records of plant specimens collected, their classification, characteristics, and ecological significance. Additionally, it may include diagrams, photographs, drawings, tables, and data analysis related to plant research. Like a chemistry practical file, a botany file serves as a documentation of practical work conducted in the field of botany and is often used for assessment and educational purposes.

Botany 4th semester file By Sumit Kumar yadav.pdf

Sumit Kumar yadav

Cotton crops are vulnerable to a variety of sucking pests, which can severely impact plant health, yield, and fiber quality. These pests primarily feed on plant sap, extracting nutrients directly from the plant's vascular system. Here's a breakdown of some of the most significant sucking pests in cotton cultivation: Aphids: Cotton aphids or melon aphids can cause direct damage by sucking sap and indirect damage by secreting honeydew, which encourages sooty mold growth. This can interfere with photosynthesis and weaken the plant. Aphids can also transmit viral diseases. Whiteflies: Two species, the silverleaf whitefly and the bandedwinged whitefly, are particularly troublesome. They not only suck sap from the underside of leaves, causing yellowing and leaf drop, but their honeydew excretion promotes sooty mold and they can transmit several plant viruses. Thrips: While thrips can chew on plants, their primary damage to cotton is through sucking. They attack the cotton plant during its seedling stage, which can stunt growth and reduce vigor. Thrips are also capable of transmitting the Cotton Bud disease. Spider Mites: These are not insects but arachnids. Spider mites, such as the two-spotted spider mite, suck cell contents from the leaves, leading to speckled discoloration and potentially significant leaf loss if infestations are severe. Leafhoppers: Including various species, leafhoppers can cause direct damage through feeding, which results in leaf curling and stunted growth. They can also be vectors for plant diseases. Mealybugs: These pests are less common but can be problematic, especially in clustered planting conditions. They suck sap and secrete honeydew, which leads to sooty mold. Mealybugs can also spread viruses. Stink Bugs: Although primarily known for their chewing mouthparts, certain stink bugs can cause damage similar to sucking pests by injecting saliva into the plant and sucking out nutrients, leading to boll damage and stained lint. Management Strategies: Cultural Controls: This includes practices such as crop rotation, using resistant varieties, and managing planting and harvesting times to avoid peak pest populations. Biological Controls: Beneficial insects like lady beetles, lacewings, and predatory mites can naturally control sucking pest populations. Parasitic wasps also play a role in controlling aphid and whitefly populations. Chemical Controls: Insecticides may be used but should be chosen carefully to minimize resistance development and preserve beneficial insects. Systemic insecticides can be particularly effective against sucking pests. Integrated Pest Management (IPM): Combining multiple control strategies based on monitoring and thresholds to apply the most effective and environmentally sensitive approach. Effective management of sucking pests in cotton requires a thorough understanding of the pest species present, their life cycles, and the ecological balance of the field environment.

Pests of cotton_Sucking_Pests_Dr.UPR.pdf

PirithiRaju

fundamental of entomology all in one topics of entomology

DrAnita Sharma

Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Available Now New Year Offer Best Call Girl Site Lucknow Call Us – 8923113531 ★ *Doggie (Sex style from behind)* ★ *Duo (Sex with two *escorts; Threesome with the client)* ★ *S-GFE *(*Special Girl Friend Experience*)* ★ *HJ (*Hand Job*) ★ *Special Massage* ★ *O-Level* *(*Oral sex*)* ★ *Tour (Internationaly*) ★ *sex)* ★ *BJ (Blowjob With Condom*) ★ *GFE (Girl Friend Experience*) ★ *CBJ (Covered Blow Job; Oral sex with a condom) Full on escorts Service by High Profile 28/April/2024 {{🎗️SCH🎗️}} 8923113531

Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...

anilsa9823

Recombinant DNA technology (Immunological screening)

PraveenaKalaiselvan1

Biological Classification BioHack (3).pdf

muntazimhurra

We explore different scenarios to explain the chemical difference found in the remarkable giant-giant binary system HD138202+CD−3012303. For the first time, we suggest how to distinguish these scenarios by taking advantage of the extensive convective envelopes of giant stars. Methods. We carried out a high-precision determination of stellar parameters and abundances by applying a full line-by-line differential analysis on GHOST high-resolution spectra. We used the FUNDPAR program with ATLAS12 model atmospheres and specific opacities calculated for an arbitrary composition through a doubly iterated method. Physical parameters were estimated with the isochrones package and evolutionary tracks were calculated via MIST models. Results. We found a significant chemical difference between the two stars (∆[Fe/H]∼0.08dex), which is largely unexpected considering the insensitivity of giant stars to planetary ingestion and diffusion effects. We tested the possibility of engulfment events by using several different combinations of stellar mass, ingested mass, metallicity of the engulfed object and different convective envelopes. However, the planetary ingestion scenario does not seem to explain the observed differences. For the first time, we distinguished the source of chemical differences using a giant-giant binary system. By ruling out other possible scenarios such as planet formation and evolutionary effects between the two stars, we suggest that primordial inhomogeneities might explain the observed differences. This remarkable result implies that the metallicity differences that were observed in at least some main-sequence binary systems might be related to primordial inhomogeneities rather than engulfment events. We also discuss the important implications of finding primordial inhomogeneities, which affect chemical tagging and other fields such as planet formation. We strongly encourage the use of giantgiant pairs. They are a relevant complement to main-sequence pairs for determining the origin of the observed chemical differences in multiple systems.

Disentangling the origin of chemical differences using GHOST

Sérgio Sacani

Context. Determining the size distribution of asteroids is key to understanding the collisional history and evolution of the inner Solar System. Aims. We aim to improve our knowledge of the size distribution of small asteroids in the main belt by determining the parallaxes of newly detected asteroids in the Hubble Space Telescope (HST) archive and subsequently their absolute magnitudes and sizes. Methods. Asteroids appear as curved trails in HST images because of the parallax induced by the fast orbital motion of the spacecraft. Taking into account the trajectory of this latter, the parallax effect can be computed to obtain the distance to the asteroids by fitting simulated trajectories to the observed trails. Using distance, we can obtain the absolute magnitude of an object and an estimation of its size assuming an albedo value, along with some boundaries for its orbital parameters. Results. In this work, we analyse a set of 632 serendipitously imaged asteroids found in the ESA HST archive. Images were captured with the ACS/WFC and WFC3/UVIS instruments. A machine learning algorithm (trained with the results of a citizen science project) was used to detect objects in these images as part of a previous study. Our raw data consist of 1031 asteroid trails from unknown objects, not matching any entries in the Minor Planet Center (MPC) database using their coordinates and imaging time. We also found 670 trails from known objects (objects featuring matching entries in the MPC). After an accuracy assessment and filtering process, our analysed HST asteroid set consists of 454 unknown objects and 178 known objects. We obtain a sample dominated by potential main belt objects featuring absolute magnitudes (H) mostly between 15 and 22 mag. The absolute magnitude cumulative distribution logN(H > H0) ∝ αlog(H0) confirms the previously reported slope change for 15 < H < 18, from α ≈ 0.56 to α ≈ 0.26, maintained in our case down to absolute magnitudes of around H ≈ 20, and therefore expanding the previous result by approximately two magnitudes. Conclusions. HST archival observations can be used as an asteroid survey because the telescope pointings are statistically randomly oriented in the sky and cover long periods of time. They allow us to expand the current best samples of astronomical objects at no extra cost in regard to telescope time.

Hubble Asteroid Hunter III. Physical properties of newly found asteroids

Sérgio Sacani

Recombination DNA Technology (Nucleic Acid Hybridization )

aarthirajkumar25

The presentation first gives the brief introduction about the animal communication covering the reasons for communication. It then describes the important types of animal communication emphasizing the important points regarding auditory and visual communication. With respect to auditory communication, it covers the uses of it and mechanisms of auditory communication along with examples. Later the presentation discusses the various forms of visual communication such as gestures, postures, facial expressions, color changes , bioluminescent communication. It then describes the visual communication in bees in the form of bee dance . In bee dance it gives a brief overview of round dance , sickle dance and waggle dance .

Animal Communication- Auditory and Visual.pptx

UmerFayaz5

Botany is the branch of biology that deals with the scientific study of plants, including their structure, growth, reproduction, metabolism, development, and classification. It encompasses a wide range of topics, from the molecular biology of plant cells to the ecological relationships between plants and their environments. Botany is essential for understanding plant diversity, ecology, evolution, and the roles plants play in ecosystems and human societies.

Botany 4th semester series (krishna).pdf

Sumit Kumar yadav

Recently uploaded (20)

Stunning ➥8448380779▻ Call Girls In Panchshil Enclave Delhi NCR

Isotopic evidence of long-lived volcanism on Io

Pests of mustard_Identification_Management_Dr.UPR.pdf

Pulmonary drug delivery system M.pharm -2nd sem P'ceutics

Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b

Raman spectroscopy.pptx M Pharm, M Sc, Advanced Spectral Analysis

VIRUSES structure and classification ppt by Dr.Prince C P

Chromatin Structure | EUCHROMATIN | HETEROCHROMATIN

GBSN - Biochemistry (Unit 1)

Botany 4th semester file By Sumit Kumar yadav.pdf

Pests of cotton_Sucking_Pests_Dr.UPR.pdf

fundamental of entomology all in one topics of entomology

Lucknow 💋 Russian Call Girls Lucknow Finest Escorts Service 8923113531 Availa...

Recombinant DNA technology (Immunological screening)

Biological Classification BioHack (3).pdf

Disentangling the origin of chemical differences using GHOST

Hubble Asteroid Hunter III. Physical properties of newly found asteroids

Recombination DNA Technology (Nucleic Acid Hybridization )

Animal Communication- Auditory and Visual.pptx

Botany 4th semester series (krishna).pdf

Legal Aspects of Open Science: the EU Perspective, Krzysztof Siewicz, University of Warsaw

1. Legal Aspects of Open Science: the EU Perspective dr Krzysztof Siewicz

2. Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl 4

3. Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl 4 Horizon 2020 EC Recommendations Amended PSI Directive Copyright framework

7. Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl

10.

11. Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl gratis, not necessarily libre details in grant agreements (MGA not too elaborate) open data not mandatory, but Open Data Pilot

12.

13.

14.

15.

16. Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl NO MANDATE FOR LIBRARIES If "IPRs" held by libraries (including university libraries, museums and archives), the re-use is possible only if it is allowed (not clear by whom) SOFT OBLIGATIONS (open formats, cf. definition; transparent fees; no unreasonable limitations in license)

17.

18.

19.

20. Platforma Otwartej Nauki ul. Prosta 69, 00 ― 838 Warszawa tel: +48 (22) 874 94 29 pon@icm.edu.pl pon.edu.pl mandate, not just encourage, libre liberalize copyright harmonize PSI & set it free

21. Credits: - https://ec.europa.eu/programmes/horizon2020/sites/horizon2020/files/FactSheet_Open_Access.pdf - The unnamed, Freedom, http://www.flickr.com/photos/unnamed/47093936/ (CC BY-SA 2.0) - Unhindered by Talent, Free Beer, http://www.flickr.com/photos/nicmcphee/2345633527/ (CC BY SA 2.0) - http://ec.europa.eu/research/participants/data/ref/h2020/legal_basis/rules_participation/ h2020-rules-participation_en.pdf - http://ec.europa.eu/research/science-society/document_library/pdf_06/ recommendation-access-and-preservation-scientific-information_en.pdf - http://ec.europa.eu/digital-agenda/en/european-legislation-reuse-public-sector-information - http://ec.europa.eu/internal_market/consultations/2013/copyright-rules/index_en.htm - http://ec.europa.eu/internal_market/consultations/2013/copyright-rules/docs/ consultation-document_en.pdf

22. Thank You for Your attention The content of this presentation is available under Creative Commons Attribution 3.0 PL License (http://creativecommons.org/licenses/by/3.0/pl/legalcode)

Legal Aspects of Open Science: the EU Perspective, Krzysztof Siewicz, University of Warsaw

Recommended

Recommended

More Related Content

More from Platforma Otwartej Nauki

More from Platforma Otwartej Nauki (20)

Recently uploaded

Recently uploaded (20)

Legal Aspects of Open Science: the EU Perspective, Krzysztof Siewicz, University of Warsaw