000641203 001__ 641203
000641203 005__ 20260209135949.0
000641203 0247_ $$2arXiv$$aarXiv:2509.26110
000641203 0247_ $$2doi$$a10.22323/1.501.0753
000641203 0247_ $$2datacite_doi$$a10.3204/PUBDB-2025-04934
000641203 0247_ $$2openalex$$aopenalex:W4414530566
000641203 037__ $$aPUBDB-2025-04934
000641203 041__ $$aEnglish
000641203 082__ $$a530
000641203 088__ $$2arXiv$$aarXiv:2509.26110
000641203 1001_ $$0P:(DE-H253)PIP1085187$$aKostunin, Dmitriy$$b0$$eCorresponding author
000641203 1112_ $$a39th International Cosmic Ray Conference$$cGeneva$$d2025-07-14 - 2025-07-24$$gICRC2025$$wSwitzerland
000641203 245__ $$aAgent-based code generation for the Gammapy framework
000641203 260__ $$aTrieste$$bSISSA$$c2025
000641203 300__ $$a7
000641203 3367_ $$2ORCID$$aCONFERENCE_PAPER
000641203 3367_ $$033$$2EndNote$$aConference Paper
000641203 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$mjournal
000641203 3367_ $$2BibTeX$$aINPROCEEDINGS
000641203 3367_ $$2DRIVER$$aconferenceObject
000641203 3367_ $$2DataCite$$aOutput Types/Conference Paper
000641203 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1770289200_693812
000641203 500__ $$aICRC2025 proceedings PoS(ICRC2025)753
000641203 520__ $$aSoftware code generation using Large Language Models (LLMs) is one of the most successful applications of modern artificial intelligence. Foundational models are very effective for popular frameworks that benefit from documentation, examples, and strong community support. In contrast, specialized scientific libraries often lack these resources and may expose unstable APIs under active development, making it difficult for models trained on limited or outdated data. We address these issues for the Gammapy library by developing an agent capable of writing, executing, and validating code in a controlled environment. We present a minimal web demo and an accompanying benchmarking suite. This contribution summarizes the design, reports our current status, and outlines next steps.
000641203 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000641203 588__ $$aDataset connected to DataCite
000641203 693__ $$0EXP:(DE-H253)HESS-20170101$$5EXP:(DE-H253)HESS-20170101$$eHigh Energy Stereoscopic System$$x0
000641203 693__ $$0EXP:(DE-H253)CTA-20150101$$5EXP:(DE-H253)CTA-20150101$$eCherenkov Telescope Array$$x1
000641203 7001_ $$aSotnikov, Vladimir$$b1
000641203 7001_ $$aGolovachev, Sergo$$b2
000641203 7001_ $$0P:(DE-H253)PIP1102748$$aMehta, Abhay$$b3$$eCorresponding author$$udesy
000641203 7001_ $$0P:(DE-H253)PIP1022858$$aHolch, Tim Lukas$$b4
000641203 7001_ $$0P:(DE-H253)PIP1097858$$aJones, Elisa$$b5
000641203 773__ $$0PERI:(DE-600)2642026-0$$a10.22323/1.501.0753$$p753$$tProceedings of Science / International School for Advanced Studies$$v(ICRC2025)$$x1824-8039$$y2025
000641203 7870_ $$0PUBDB-2026-00668$$aKostunin, Dmitriy et.al.$$d2025$$iIsParent$$rarXiv:2509.26110$$tAgent-based code generation for the Gammapy framework
000641203 8564_ $$uhttps://bib-pubdb1.desy.de/record/641203/files/2509.26110v1.pdf$$yOpenAccess
000641203 8564_ $$uhttps://bib-pubdb1.desy.de/record/641203/files/2509.26110v1.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000641203 909CO $$ooai:bib-pubdb1.desy.de:641203$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000641203 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1085187$$aDeutsches Elektronen-Synchrotron$$b0$$kDESY
000641203 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1102748$$aDeutsches Elektronen-Synchrotron$$b3$$kDESY
000641203 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1022858$$aDeutsches Elektronen-Synchrotron$$b4$$kDESY
000641203 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1097858$$aDeutsches Elektronen-Synchrotron$$b5$$kDESY
000641203 9131_ $$0G:(DE-HGF)POF4-613$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vMatter and Radiation from the Universe$$x0
000641203 9141_ $$y2025
000641203 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2025-01-02
000641203 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0
000641203 915__ $$0StatID:(DE-HGF)0501$$2StatID$$aDBCoverage$$bDOAJ Seal$$d2021-04-20T14:42:38Z
000641203 915__ $$0StatID:(DE-HGF)0500$$2StatID$$aDBCoverage$$bDOAJ$$d2021-04-20T14:42:38Z
000641203 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000641203 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bDOAJ : Editorial review$$d2021-04-20T14:42:38Z
000641203 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2025-01-02
000641203 9201_ $$0I:(DE-H253)Z_DV-20210408$$kZ_DV$$lDatenverarbeitung$$x0
000641203 9201_ $$0I:(DE-H253)Z_HESS-20210408$$kZ_HESS$$lHigh Energy Steroscopic System$$x1
000641203 980__ $$acontrib
000641203 980__ $$aVDB
000641203 980__ $$aUNRESTRICTED
000641203 980__ $$ajournal
000641203 980__ $$aI:(DE-H253)Z_DV-20210408
000641203 980__ $$aI:(DE-H253)Z_HESS-20210408
000641203 9801_ $$aFullTexts