[{"scopus_import":"1","month":"03","intvolume":" 20","abstract":[{"lang":"eng","text":"Interpretation of extracellular recordings can be challenging due to the long range of electric field. This challenge can be mitigated by estimating the current source density (CSD). Here we introduce kCSD-python, an open Python package implementing Kernel Current Source Density (kCSD) method and related tools to facilitate CSD analysis of experimental data and the interpretation of results. We show how to counter the limitations imposed by noise and assumptions in the method itself. kCSD-python allows CSD estimation for an arbitrary distribution of electrodes in 1D, 2D, and 3D, assuming distributions of sources in tissue, a slice, or in a single cell, and includes a range of diagnostic aids. We demonstrate its features in a Jupyter Notebook tutorial which illustrates a typical analytical workflow and main functionalities useful in validating analysis results."}],"oa_version":"Published Version","issue":"3","volume":20,"related_material":{"link":[{"url":"https://github.com/Neuroinflab/kCSD-python","relation":"software"}]},"publication_identifier":{"issn":["1553-734X"],"eissn":["1553-7358"]},"publication_status":"published","language":[{"iso":"eng"}],"article_type":"original","type":"journal_article","status":"public","_id":"15169","department":[{"_id":"TiVo"}],"date_updated":"2024-03-25T07:54:23Z","publisher":"Public Library of Science","quality_controlled":"1","acknowledgement":"The Python implementation of kCSD was started by Grzegorz Parka during Google Summer of Code project through the International Neuroinformatics Coordinating Facility. Jan Mąka implemented the first Python version of skCSD class. This work was supported by the Polish National Science Centre (2013/08/W/NZ4/00691 to DKW; 2015/17/B/ST7/04123 to DKW). ","date_published":"2024-03-14T00:00:00Z","doi":"10.1371/journal.pcbi.1011941","date_created":"2024-03-24T23:00:59Z","year":"2024","day":"14","publication":"PLoS Computational Biology","article_number":"e1011941","author":[{"id":"E4EDB536-3485-11EA-98D2-20AF3DDC885E","first_name":"Chaitanya","full_name":"Chintaluri, Chaitanya","last_name":"Chintaluri"},{"last_name":"Bejtka","full_name":"Bejtka, Marta","first_name":"Marta"},{"first_name":"Wladyslaw","full_name":"Sredniawa, Wladyslaw","last_name":"Sredniawa"},{"first_name":"Michal","full_name":"Czerwinski, Michal","last_name":"Czerwinski"},{"last_name":"Dzik","full_name":"Dzik, Jakub M.","first_name":"Jakub M."},{"first_name":"Joanna","last_name":"Jedrzejewska-Szmek","full_name":"Jedrzejewska-Szmek, Joanna"},{"full_name":"Wojciki, Daniel K.","last_name":"Wojciki","first_name":"Daniel K."}],"article_processing_charge":"Yes","title":"kCSD-python, reliable current source density estimation with quality control","citation":{"chicago":"Chintaluri, Chaitanya, Marta Bejtka, Wladyslaw Sredniawa, Michal Czerwinski, Jakub M. Dzik, Joanna Jedrzejewska-Szmek, and Daniel K. Wojciki. “KCSD-Python, Reliable Current Source Density Estimation with Quality Control.” PLoS Computational Biology. Public Library of Science, 2024. https://doi.org/10.1371/journal.pcbi.1011941.","ista":"Chintaluri C, Bejtka M, Sredniawa W, Czerwinski M, Dzik JM, Jedrzejewska-Szmek J, Wojciki DK. 2024. kCSD-python, reliable current source density estimation with quality control. PLoS Computational Biology. 20(3), e1011941.","mla":"Chintaluri, Chaitanya, et al. “KCSD-Python, Reliable Current Source Density Estimation with Quality Control.” PLoS Computational Biology, vol. 20, no. 3, e1011941, Public Library of Science, 2024, doi:10.1371/journal.pcbi.1011941.","ama":"Chintaluri C, Bejtka M, Sredniawa W, et al. kCSD-python, reliable current source density estimation with quality control. PLoS Computational Biology. 2024;20(3). doi:10.1371/journal.pcbi.1011941","apa":"Chintaluri, C., Bejtka, M., Sredniawa, W., Czerwinski, M., Dzik, J. M., Jedrzejewska-Szmek, J., & Wojciki, D. K. (2024). kCSD-python, reliable current source density estimation with quality control. PLoS Computational Biology. Public Library of Science. https://doi.org/10.1371/journal.pcbi.1011941","ieee":"C. Chintaluri et al., “kCSD-python, reliable current source density estimation with quality control,” PLoS Computational Biology, vol. 20, no. 3. Public Library of Science, 2024.","short":"C. Chintaluri, M. Bejtka, W. Sredniawa, M. Czerwinski, J.M. Dzik, J. Jedrzejewska-Szmek, D.K. Wojciki, PLoS Computational Biology 20 (2024)."},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87"},{"status":"public","article_type":"original","type":"journal_article","_id":"15167","department":[{"_id":"MiLe"}],"date_updated":"2024-03-25T07:36:55Z","intvolume":" 109","month":"03","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2311.14536"}],"scopus_import":"1","oa_version":"Preprint","abstract":[{"lang":"eng","text":"We perform a diagrammatic analysis of the energy of a mobile impurity immersed in a strongly interacting two-component Fermi gas to second order in the impurity-bath interaction. These corrections demonstrate divergent behavior in the limit of large impurity momentum. We show the fundamental processes responsible for these logarithmically divergent terms. We study the problem in the general case without any assumptions regarding the fermion-fermion interactions in the bath. We show that the divergent term can be summed up to all orders in the Fermi-Fermi interaction and that the resulting expression is equivalent to the one obtained in the few-body calculation. Finally, we provide a perturbative calculation to the second order in the Fermi-Fermi interaction, and we show the diagrams responsible for these terms."}],"volume":109,"issue":"3","language":[{"iso":"eng"}],"publication_status":"published","publication_identifier":{"eissn":["2469-9934"],"issn":["2469-9926"]},"article_number":"033315","title":"Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy","article_processing_charge":"No","external_id":{"arxiv":["2311.14536"]},"author":[{"first_name":"Ragheed","id":"d1c405be-ae15-11ed-8510-ccf53278162e","full_name":"Al Hyder, Ragheed","last_name":"Al Hyder"},{"full_name":"Chevy, F.","last_name":"Chevy","first_name":"F."},{"first_name":"X.","full_name":"Leyronas, X.","last_name":"Leyronas"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","citation":{"mla":"Al Hyder, Ragheed, et al. “Exploring Beyond-Mean-Field Logarithmic Divergences in Fermi-Polaron Energy.” Physical Review A, vol. 109, no. 3, 033315, American Physical Society, 2024, doi:10.1103/PhysRevA.109.033315.","apa":"Al Hyder, R., Chevy, F., & Leyronas, X. (2024). Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy. Physical Review A. American Physical Society. https://doi.org/10.1103/PhysRevA.109.033315","ama":"Al Hyder R, Chevy F, Leyronas X. Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy. Physical Review A. 2024;109(3). doi:10.1103/PhysRevA.109.033315","short":"R. Al Hyder, F. Chevy, X. Leyronas, Physical Review A 109 (2024).","ieee":"R. Al Hyder, F. Chevy, and X. Leyronas, “Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy,” Physical Review A, vol. 109, no. 3. American Physical Society, 2024.","chicago":"Al Hyder, Ragheed, F. Chevy, and X. Leyronas. “Exploring Beyond-Mean-Field Logarithmic Divergences in Fermi-Polaron Energy.” Physical Review A. American Physical Society, 2024. https://doi.org/10.1103/PhysRevA.109.033315.","ista":"Al Hyder R, Chevy F, Leyronas X. 2024. Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy. Physical Review A. 109(3), 033315."},"oa":1,"publisher":"American Physical Society","quality_controlled":"1","acknowledgement":"We thank Félix Werner and Kris Van Houcke for interesting discussions.","date_created":"2024-03-24T23:00:59Z","date_published":"2024-03-19T00:00:00Z","doi":"10.1103/PhysRevA.109.033315","publication":"Physical Review A","day":"19","year":"2024"},{"date_published":"2024-03-19T00:00:00Z","doi":"10.1016/j.disc.2024.113962","date_created":"2024-03-24T23:00:58Z","year":"2024","day":"19","publication":"Discrete Mathematics","quality_controlled":"1","publisher":"Elsevier","oa":1,"acknowledgement":"We wish to thank Dániel Marx and András Sebő for making us aware of the results in [8] and some clarifications on them.","author":[{"last_name":"Campbell","full_name":"Campbell, Rutger","first_name":"Rutger"},{"first_name":"Florian","last_name":"Hörsch","full_name":"Hörsch, Florian"},{"id":"6dc1a1be-bf1c-11ed-8d2b-d044840f49d6","first_name":"Benjamin","last_name":"Moore","full_name":"Moore, Benjamin"}],"article_processing_charge":"No","external_id":{"arxiv":["2301.11615"]},"title":"Decompositions into two linear forests of bounded lengths","citation":{"chicago":"Campbell, Rutger, Florian Hörsch, and Benjamin Moore. “Decompositions into Two Linear Forests of Bounded Lengths.” Discrete Mathematics. Elsevier, 2024. https://doi.org/10.1016/j.disc.2024.113962.","ista":"Campbell R, Hörsch F, Moore B. 2024. Decompositions into two linear forests of bounded lengths. Discrete Mathematics. 347(6), 113962.","mla":"Campbell, Rutger, et al. “Decompositions into Two Linear Forests of Bounded Lengths.” Discrete Mathematics, vol. 347, no. 6, 113962, Elsevier, 2024, doi:10.1016/j.disc.2024.113962.","ama":"Campbell R, Hörsch F, Moore B. Decompositions into two linear forests of bounded lengths. Discrete Mathematics. 2024;347(6). doi:10.1016/j.disc.2024.113962","apa":"Campbell, R., Hörsch, F., & Moore, B. (2024). Decompositions into two linear forests of bounded lengths. Discrete Mathematics. Elsevier. https://doi.org/10.1016/j.disc.2024.113962","short":"R. Campbell, F. Hörsch, B. Moore, Discrete Mathematics 347 (2024).","ieee":"R. Campbell, F. Hörsch, and B. Moore, “Decompositions into two linear forests of bounded lengths,” Discrete Mathematics, vol. 347, no. 6. Elsevier, 2024."},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_number":"113962","issue":"6","volume":347,"publication_identifier":{"issn":["0012-365X"]},"publication_status":"epub_ahead","language":[{"iso":"eng"}],"scopus_import":"1","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2301.11615"}],"month":"03","intvolume":" 347","abstract":[{"text":"For some k∈Z≥0∪{∞}, we call a linear forest k-bounded if each of its components has at most k edges. We will say a (k,ℓ)-bounded linear forest decomposition of a graph G is a partition of E(G) into the edge sets of two linear forests Fk,Fℓ where Fk is k-bounded and Fℓ is ℓ-bounded. We show that the problem of deciding whether a given graph has such a decomposition is NP-complete if both k and ℓ are at least 2, NP-complete if k≥9 and ℓ=1, and is in P for (k,ℓ)=(2,1). Before this, the only known NP-complete cases were the (2,2) and (3,3) cases. Our hardness result answers a question of Bermond et al. from 1984. We also show that planar graphs of girth at least nine decompose into a linear forest and a matching, which in particular is stronger than 3-edge-colouring such graphs.","lang":"eng"}],"oa_version":"Preprint","department":[{"_id":"MaKw"}],"date_updated":"2024-03-25T08:09:43Z","article_type":"original","type":"journal_article","status":"public","_id":"15163"},{"acknowledgement":"We thank the anonymous referee for constructive comments that helped improve the manuscript. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program Nos. 1243 and 1895. The specific observations analyzed can be accessed via doi:10.17909/4xx0-zj76. Funded by the European Union (ERC, AGENTS, 101076224). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them. R.P.N. acknowledges funding from JWST programs GO-1933 and GO-2279. Support for this work for R.P.N. was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. Support for this work for G.I. was provided by NASA through grant JWST-GO-01895 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. This work has received funding from the Swiss State Secretariat for Education, Research and Innovation (SERI) under contract No. MB22.00072, as well as from the Swiss National Science Foundation (SNSF) through project grant 200020_207349. The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant No. 140.\r\nFacility: JWST - James Webb Space Telescope, HST - Hubble Space Telescope satellite\r\nSoftware: Python, matplotlib (Hunter 2007), numpy (Harris et al. 2020), scipy (Virtanen et al. 2020), Astropy (Astropy Collaboration et al. 2013, 2018), Imfit (Erwin 2015).","oa":1,"quality_controlled":"1","publisher":"American Astronomical Society","year":"2024","has_accepted_license":"1","publication":"The Astrophysical Journal","day":"07","date_created":"2024-03-25T08:54:47Z","doi":"10.3847/1538-4357/ad2345","date_published":"2024-03-07T00:00:00Z","article_number":"129","project":[{"grant_number":"101076224","name":"Young galaxies as tracers and agents of cosmic reionization","_id":"bd9b2118-d553-11ed-ba76-db24564edfea"}],"citation":{"chicago":"Matthee, Jorryt J, Rohan P. Naidu, Gabriel Brammer, John Chisholm, Anna-Christina Eilers, Andy Goulding, Jenny Greene, et al. “Little Red Dots: An Abundant Population of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys.” The Astrophysical Journal. American Astronomical Society, 2024. https://doi.org/10.3847/1538-4357/ad2345.","ista":"Matthee JJ, Naidu RP, Brammer G, Chisholm J, Eilers A-C, Goulding A, Greene J, Kashino D, Labbe I, Lilly SJ, Mackenzie R, Oesch PA, Weibel A, Wuyts S, Xiao M, Bordoloi R, Bouwens R, van Dokkum P, Illingworth G, Kramarenko I, Maseda MV, Mason C, Meyer RA, Nelson EJ, Reddy NA, Shivaei I, Simcoe RA, Yue M. 2024. Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys. The Astrophysical Journal. 963(2), 129.","mla":"Matthee, Jorryt J., et al. “Little Red Dots: An Abundant Population of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys.” The Astrophysical Journal, vol. 963, no. 2, 129, American Astronomical Society, 2024, doi:10.3847/1538-4357/ad2345.","ama":"Matthee JJ, Naidu RP, Brammer G, et al. Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys. The Astrophysical Journal. 2024;963(2). doi:10.3847/1538-4357/ad2345","apa":"Matthee, J. J., Naidu, R. P., Brammer, G., Chisholm, J., Eilers, A.-C., Goulding, A., … Yue, M. (2024). Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys. The Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/ad2345","ieee":"J. J. Matthee et al., “Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys,” The Astrophysical Journal, vol. 963, no. 2. American Astronomical Society, 2024.","short":"J.J. Matthee, R.P. Naidu, G. Brammer, J. Chisholm, A.-C. Eilers, A. Goulding, J. Greene, D. Kashino, I. Labbe, S.J. Lilly, R. Mackenzie, P.A. Oesch, A. Weibel, S. Wuyts, M. Xiao, R. Bordoloi, R. Bouwens, P. van Dokkum, G. Illingworth, I. Kramarenko, M.V. Maseda, C. Mason, R.A. Meyer, E.J. Nelson, N.A. Reddy, I. Shivaei, R.A. Simcoe, M. Yue, The Astrophysical Journal 963 (2024)."},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"Yes","author":[{"full_name":"Matthee, Jorryt J","orcid":"0000-0003-2871-127X","last_name":"Matthee","id":"7439a258-f3c0-11ec-9501-9df22fe06720","first_name":"Jorryt J"},{"full_name":"Naidu, Rohan P.","last_name":"Naidu","first_name":"Rohan P."},{"first_name":"Gabriel","last_name":"Brammer","full_name":"Brammer, Gabriel"},{"last_name":"Chisholm","full_name":"Chisholm, John","first_name":"John"},{"first_name":"Anna-Christina","last_name":"Eilers","full_name":"Eilers, Anna-Christina"},{"last_name":"Goulding","full_name":"Goulding, Andy","first_name":"Andy"},{"first_name":"Jenny","last_name":"Greene","full_name":"Greene, Jenny"},{"first_name":"Daichi","full_name":"Kashino, Daichi","last_name":"Kashino"},{"first_name":"Ivo","full_name":"Labbe, Ivo","last_name":"Labbe"},{"first_name":"Simon J.","full_name":"Lilly, Simon J.","last_name":"Lilly"},{"first_name":"Ruari","last_name":"Mackenzie","full_name":"Mackenzie, Ruari"},{"last_name":"Oesch","full_name":"Oesch, Pascal A.","first_name":"Pascal A."},{"first_name":"Andrea","last_name":"Weibel","full_name":"Weibel, Andrea"},{"first_name":"Stijn","full_name":"Wuyts, Stijn","last_name":"Wuyts"},{"first_name":"Mengyuan","last_name":"Xiao","full_name":"Xiao, Mengyuan"},{"full_name":"Bordoloi, Rongmon","last_name":"Bordoloi","first_name":"Rongmon"},{"full_name":"Bouwens, Rychard","last_name":"Bouwens","first_name":"Rychard"},{"full_name":"van Dokkum, Pieter","last_name":"van Dokkum","first_name":"Pieter"},{"first_name":"Garth","last_name":"Illingworth","full_name":"Illingworth, Garth"},{"full_name":"Kramarenko, Ivan","last_name":"Kramarenko","first_name":"Ivan"},{"last_name":"Maseda","full_name":"Maseda, Michael V.","first_name":"Michael V."},{"first_name":"Charlotte","full_name":"Mason, Charlotte","last_name":"Mason"},{"first_name":"Romain A.","last_name":"Meyer","full_name":"Meyer, Romain A."},{"full_name":"Nelson, Erica J.","last_name":"Nelson","first_name":"Erica J."},{"first_name":"Naveen A.","last_name":"Reddy","full_name":"Reddy, Naveen A."},{"first_name":"Irene","last_name":"Shivaei","full_name":"Shivaei, Irene"},{"last_name":"Simcoe","full_name":"Simcoe, Robert A.","first_name":"Robert A."},{"first_name":"Minghao","last_name":"Yue","full_name":"Yue, Minghao"}],"title":"Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys","abstract":[{"lang":"eng","text":"Characterizing the prevalence and properties of faint active galactic nuclei (AGNs) in the early Universe is key for understanding the formation of supermassive black holes (SMBHs) and determining their role in cosmic reionization. We perform a spectroscopic search for broad Hα emitters at z ≈ 4–6 using deep JWST/NIRCam imaging and wide field slitless spectroscopy from the EIGER and FRESCO surveys. We identify 20 Hα lines at z = 4.2–5.5 that have broad components with line widths from ∼1200–3700 km s−1, contributing ∼30%–90% of the total line flux. We interpret these broad components as being powered by accretion onto SMBHs with implied masses ∼107–8M⊙. In the UV luminosity range MUV,AGN+host = −21 to −18, we measure number densities of ≈10−5 cMpc−3. This is an order of magnitude higher than expected from extrapolating quasar UV luminosity functions (LFs). Yet, such AGN are found in only <1% of star-forming galaxies at z ∼ 5. The number density discrepancy is much lower when compared to the broad Hα LF. The SMBH mass function agrees with large cosmological simulations. In two objects, we detect complex Hα profiles that we tentatively interpret as caused by absorption signatures from dense gas fueling SMBH growth and outflows. We may be witnessing early AGN feedback that will clear dust-free pathways through which more massive blue quasars are seen. We uncover a strong correlation between reddening and the fraction of total galaxy luminosity arising from faint AGN. This implies that early SMBH growth is highly obscured and that faint AGN are only minor contributors to cosmic reionization."}],"oa_version":"Published Version","scopus_import":"1","intvolume":" 963","month":"03","publication_status":"published","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"language":[{"iso":"eng"}],"file":[{"success":1,"file_id":"15184","checksum":"dc7af4694f9f94a551417ab49fa43edf","content_type":"application/pdf","relation":"main_file","access_level":"open_access","file_name":"2024_AstrophysicalJourn_Matthee.pdf","date_created":"2024-03-25T09:31:58Z","file_size":6047536,"date_updated":"2024-03-25T09:31:58Z","creator":"dernst"}],"volume":963,"issue":"2","_id":"15180","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"type":"journal_article","article_type":"original","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"status":"public","date_updated":"2024-03-25T09:37:27Z","ddc":["550"],"file_date_updated":"2024-03-25T09:31:58Z","department":[{"_id":"JoMa"}]},{"_id":"15179","status":"public","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"article_type":"original","type":"journal_article","ddc":["580"],"date_updated":"2024-03-25T09:44:53Z","file_date_updated":"2024-03-25T09:42:10Z","department":[{"_id":"FyKo"}],"oa_version":"Published Version","abstract":[{"text":"The fungal bioluminescence pathway can be reconstituted in other organisms allowing luminescence imaging without exogenously supplied substrate. The pathway starts from hispidin biosynthesis—a step catalyzed by a large fungal polyketide synthase that requires a posttranslational modification for activity. Here, we report identification of alternative compact hispidin synthases encoded by a phylogenetically diverse group of plants. A hybrid bioluminescence pathway that combines plant and fungal genes is more compact, not dependent on availability of machinery for posttranslational modifications, and confers autonomous bioluminescence in yeast, mammalian, and plant hosts. The compact size of plant hispidin synthases enables additional modes of delivery of autoluminescence, such as delivery with viral vectors.","lang":"eng"}],"intvolume":" 10","month":"03","scopus_import":"1","language":[{"iso":"eng"}],"file":[{"content_type":"application/pdf","relation":"main_file","access_level":"open_access","success":1,"file_id":"15185","checksum":"a19c43b260ea0bbaf895a29712e3153c","file_size":1499302,"date_updated":"2024-03-25T09:42:10Z","creator":"dernst","file_name":"2024_ScienceAdv_Palkina.pdf","date_created":"2024-03-25T09:42:10Z"}],"publication_status":"published","publication_identifier":{"issn":["2375-2548"]},"volume":10,"issue":"10","article_number":"adk1992","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","citation":{"ista":"Palkina KA, Karataeva TA, Perfilov MM, Fakhranurova LI, Markina NM, Gonzalez Somermeyer L, Garcia-Perez E, Vazquez-Vilar M, Rodriguez-Rodriguez M, Vazquez-Vilriales V, Shakhova ES, Mitiouchkina T, Belozerova OA, Kovalchuk SI, Alekberova A, Malyshevskaia AK, Bugaeva EN, Guglya EB, Balakireva A, Sytov N, Bezlikhotnova A, Boldyreva DI, Babenko VV, Kondrashov F, Choob VV, Orzaez D, Yampolsky IV, Mishin AS, Sarkisyan KS. 2024. A hybrid pathway for self-sustained luminescence. Science Advances. 10(10), adk1992.","chicago":"Palkina, Kseniia A., Tatiana A. Karataeva, Maxim M. Perfilov, Liliia I. Fakhranurova, Nadezhda M. Markina, Louisa Gonzalez Somermeyer, Elena Garcia-Perez, et al. “A Hybrid Pathway for Self-Sustained Luminescence.” Science Advances. American Association for the Advancement of Science, 2024. https://doi.org/10.1126/sciadv.adk1992.","ama":"Palkina KA, Karataeva TA, Perfilov MM, et al. A hybrid pathway for self-sustained luminescence. Science Advances. 2024;10(10). doi:10.1126/sciadv.adk1992","apa":"Palkina, K. A., Karataeva, T. A., Perfilov, M. M., Fakhranurova, L. I., Markina, N. M., Gonzalez Somermeyer, L., … Sarkisyan, K. S. (2024). A hybrid pathway for self-sustained luminescence. Science Advances. American Association for the Advancement of Science. https://doi.org/10.1126/sciadv.adk1992","ieee":"K. A. Palkina et al., “A hybrid pathway for self-sustained luminescence,” Science Advances, vol. 10, no. 10. American Association for the Advancement of Science, 2024.","short":"K.A. Palkina, T.A. Karataeva, M.M. Perfilov, L.I. Fakhranurova, N.M. Markina, L. Gonzalez Somermeyer, E. Garcia-Perez, M. Vazquez-Vilar, M. Rodriguez-Rodriguez, V. Vazquez-Vilriales, E.S. Shakhova, T. Mitiouchkina, O.A. Belozerova, S.I. Kovalchuk, A. Alekberova, A.K. Malyshevskaia, E.N. Bugaeva, E.B. Guglya, A. Balakireva, N. Sytov, A. Bezlikhotnova, D.I. Boldyreva, V.V. Babenko, F. Kondrashov, V.V. Choob, D. Orzaez, I.V. Yampolsky, A.S. Mishin, K.S. Sarkisyan, Science Advances 10 (2024).","mla":"Palkina, Kseniia A., et al. “A Hybrid Pathway for Self-Sustained Luminescence.” Science Advances, vol. 10, no. 10, adk1992, American Association for the Advancement of Science, 2024, doi:10.1126/sciadv.adk1992."},"title":"A hybrid pathway for self-sustained luminescence","article_processing_charge":"Yes","author":[{"first_name":"Kseniia A.","full_name":"Palkina, Kseniia A.","last_name":"Palkina"},{"first_name":"Tatiana A.","full_name":"Karataeva, Tatiana A.","last_name":"Karataeva"},{"full_name":"Perfilov, Maxim M.","last_name":"Perfilov","first_name":"Maxim M."},{"full_name":"Fakhranurova, Liliia I.","last_name":"Fakhranurova","first_name":"Liliia I."},{"last_name":"Markina","full_name":"Markina, Nadezhda M.","first_name":"Nadezhda M."},{"last_name":"Gonzalez Somermeyer","orcid":"0000-0001-9139-5383","full_name":"Gonzalez Somermeyer, Louisa","first_name":"Louisa","id":"4720D23C-F248-11E8-B48F-1D18A9856A87"},{"last_name":"Garcia-Perez","full_name":"Garcia-Perez, Elena","first_name":"Elena"},{"full_name":"Vazquez-Vilar, Marta","last_name":"Vazquez-Vilar","first_name":"Marta"},{"first_name":"Marta","full_name":"Rodriguez-Rodriguez, Marta","last_name":"Rodriguez-Rodriguez"},{"last_name":"Vazquez-Vilriales","full_name":"Vazquez-Vilriales, Victor","first_name":"Victor"},{"full_name":"Shakhova, Ekaterina S.","last_name":"Shakhova","first_name":"Ekaterina S."},{"first_name":"Tatiana","last_name":"Mitiouchkina","full_name":"Mitiouchkina, Tatiana"},{"full_name":"Belozerova, Olga A.","last_name":"Belozerova","first_name":"Olga A."},{"full_name":"Kovalchuk, Sergey I.","last_name":"Kovalchuk","first_name":"Sergey I."},{"last_name":"Alekberova","full_name":"Alekberova, Anna","first_name":"Anna"},{"last_name":"Malyshevskaia","full_name":"Malyshevskaia, Alena K.","first_name":"Alena K."},{"last_name":"Bugaeva","full_name":"Bugaeva, Evgenia N.","first_name":"Evgenia N."},{"last_name":"Guglya","full_name":"Guglya, Elena B.","first_name":"Elena B."},{"first_name":"Anastasia","last_name":"Balakireva","full_name":"Balakireva, Anastasia"},{"first_name":"Nikita","full_name":"Sytov, Nikita","last_name":"Sytov"},{"first_name":"Anastasia","full_name":"Bezlikhotnova, Anastasia","last_name":"Bezlikhotnova"},{"first_name":"Daria I.","last_name":"Boldyreva","full_name":"Boldyreva, Daria I."},{"last_name":"Babenko","full_name":"Babenko, Vladislav V.","first_name":"Vladislav V."},{"last_name":"Kondrashov","full_name":"Kondrashov, Fyodor","orcid":"0000-0001-8243-4694","id":"44FDEF62-F248-11E8-B48F-1D18A9856A87","first_name":"Fyodor"},{"full_name":"Choob, Vladimir V.","last_name":"Choob","first_name":"Vladimir V."},{"full_name":"Orzaez, Diego","last_name":"Orzaez","first_name":"Diego"},{"last_name":"Yampolsky","full_name":"Yampolsky, Ilia V.","first_name":"Ilia V."},{"first_name":"Alexander S.","last_name":"Mishin","full_name":"Mishin, Alexander S."},{"first_name":"Karen S.","last_name":"Sarkisyan","full_name":"Sarkisyan, Karen S."}],"acknowledgement":"We thank Milaboratory (milaboratory.com) for the access to computing and storage infrastructure. We thank J. Petrasek for providing the BY-2 cell culture line. We thank Konstantin Lukyanov laboratory and Sergey Deyev laboratory for assistance with experiments.\r\nThis study was partially funded by Light Bio and Planta. The Synthetic biology Group is funded by the MRC London Institute of Medical Sciences (UKRI MC-A658-5QEA0). Cloning and luminescent assays performed in BY-2 were partially supported by RSF, project number 22-14-00400, https://rscf.ru/project/22-14-00400/. Plant transformations were funded by RFBR and MOST, project number 21-54-52004. Plant imaging experiments were funded by RSF, project number 22-74-00124, https://rscf.ru/project/22-74-00124/. Viral delivery experiments were funded by the grant PID2019-108203RB-I00 Plan Nacional I + D from the Ministerio de Ciencia e Innovación (Spain) through the Agencia Estatal de Investigación (cofinanced by the European Regional Development Fund).","oa":1,"publisher":"American Association for the Advancement of Science","quality_controlled":"1","publication":"Science Advances","day":"01","year":"2024","has_accepted_license":"1","date_created":"2024-03-25T08:54:33Z","doi":"10.1126/sciadv.adk1992","date_published":"2024-03-01T00:00:00Z"}]