Daniele Bjørn Malesani

基本信息

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职业迁徙

个人简介

I am an observational astronomer, interested in the field of transients. These are objects that vary catastrophically in the sky. Many are related to the deaths of stars, such as supernovae and gamma-ray bursts. Kilonovae are a newly discovered type of transients, connected to gravitational wave sources, originated when orbiting pairs of compact stars (black holes and neutron stars) smash against each other and merge, usually forming a (bigger) black hole.
Transients can be very bright, and while they’re active we can see them further away in the universe. As such, they are important probes of their environments. For example, gamma-ray bursts allow to test the composition of the medium of high-redshift galaxies. Kilonovae are an important site where elements heavier than iron are produced: everybody’s jewelry may come from a pair of colliding neutron stars.
I am involved in international programs, such as the Stargate and ENGRAVE consortia, aimed at exploiting every aspect of these transient sources.

研究兴趣

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Multi-Wavelength Analysis of AT 2023sva: a Luminous Orphan Afterglow with Evidence for a Structured Jet

Gokul P. Srinivasaragavan, Daniel A. Perley,Anna Y. Q. Ho, Brendan O'Connor, Antonio de Ugarte Postigo,Nikhil Sarin,S. Bradley Cenko,Jesper Sollerman,Lauren Rhodes, David A. Green,Dmitry S. Svinkin,Varun Bhalerao,Gaurav Waratkar,A. J. Nayana, Poonam Chandra, M. Coleman Miller,Daniele B. Malesani,Geoffrey Ryan, Suryansh Srijan, Eric C. Bellm, Eric Burns,David J. Titterington, Maria B. Stone,Josiah Purdum, Tomás Ahumada, G. C. Anupama, Sudhanshu Barway,Michael W. Coughlin,Andrew Drake,Rob Fender, José F. AgüÍ Fernández,Dmitry D. Frederiks,Stefan Geier, Matthew J. Graham, Mansi M. Kasliwal, S. R. Kulkarni,Harsh Kumar, Maggie L. Li, Russ R. Laher,Alexandra L. Lysenko, Gopal Parwani,Richard A. Perley,Anna V. Ridnaia, Anirudh Salgundi,Roger Smith,Niharika Sravan,Vishwajeet Swain,Christina C. Thöne,Anastasia E. Tsvetkova,Mikhail V. Ulanov, Jada Vail, Jacob L. Wise,Avery Wold

arxiv（2025）

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Soft X-ray Prompt Emission from the High-Redshift Gamma-Ray Burst EP240315a

Y. Liu,H. Sun,D. Xu,D. S. Svinkin, J. Delaunay,N. R. Tanvir,H. Gao,C. Zhang,Y. Chen,X. -F. Wu, B. Zhang,W. Yuan,J. An, G. Bruni,D. D. Frederiks,G. Ghirlanda,J. -W. Hu, A. Li,C. -K. Li,J. -D. Li,D. B. Malesani,L. Piro,G. Raman,R. Ricci,E. Troja,S. D. Vergani, Q. -Y. Wu,J. Yang, B. -B. Zhang,Z. -P. Zhu,A. de Ugarte Postigo, A. G. Demin,D. Dobie,Z. Fan,S. -Y. Fu,J. P. U. Fynbo,J. -J. Geng,G. Gianfagna,Y. -D. Hu,Y. -F. Huang,S. -Q. Jiang,P. G. Jonker, Y. Julakanti,J. A. Kennea,A. A. Kokomov,E. Kuulkers,W. -H. Lei,J. K. Leung,A. J. Levan,D. -Y. Li,Y. Li,S. P. Littlefair, X. Liu,A. L. Lysenko,Y. -N. Ma,A. Martin-Carrillo,P. O'Brien,T. Parsotan,J. Quirola-Vasquez,A. V. Ridnaia,S. Ronchini,A. Rossi,D. Mata-Sanchez,B. Schneider,R. -F. Shen,A. L. Thakur,A. Tohuvavohu,M. A. P. Torres,A. E. Tsvetkova,M. V. Ulanov,J. -J. Wei, D. Xiao, Y. -H. I. Yin,M. Bai,V. Burwitz,Z. -M. Cai,F. -S. Chen,H. -L. Chen,T. -X. Chen,W. Chen,Y. -F. Chen,Y. -H. Chen,H. -Q. Cheng,C. -Z. Cui,W. -W. Cui,Y. -F. Dai,Z. -G. Dai,J. Eder,D. -W. Fan,C. Feldman,H. Feng, Z. Feng,P. Friedrich, X. Gao,J. Guan,D. -W Han, J. Han,D. -J. Hou,H. -B. Hu,T. Hu,M. -H. Huang,J. Huo,I. Hutchinson,Z. Ji,S. -M. Jia,Z. -Q. Jia,B. -W. Jiang,C. -C. Jin,G. Jin,J. -J. Jin, A. Keereman,H. Lerman,J. -F. Li,L. -H. Li,M. -S. Li,W. Li,Z. -D. Li,T. -Y. Lian,E. -W. Liang,Z. -X. Ling,C. -Z. Liu,H. -Y. Liu,H. -Q. Liu,M. -J. Liu,Y. -R. Liu,F. -J. Lu,H. -J. LU,L. -D. Luo,F. L. Ma, J. Ma,J. -R. Mao, X. Mao, M. McHugh,N. Meidinger,K. Nandra,J. P. Osborne,H. -W. Pan,X. Pan,M. E. Ravasio,A. Rau,N. Rea, U. Rehman,J. Sanders, A. Santovincenzo,L. -M. Song,J. Su,L. -J. Sun,S. -L. Sun, X. -J. Sun, Y. -Y. Tan,Q. -J. Tang, Y. -H. Tao,J. -Z. Tong,H. Wang,J. Wang,L. Wang,W. -X. Wang,X. -F. Wang,X. -Y. Wang,Y. -L. Wang,Y. -S. Wang,D. -M. Wei,R. Willingale,S. -L. Xiong,H. -T. Xu,J. -J. Xu,X. -P. Xu,Y. -F. Xu, Z. Xu,C. -B. Xue,Y. -L. Xue,A. -L. Yan,F. Yang, H. -N. Yang, X. -T. Yang,Y. -J Yang,Y. -W. Yu,J. Zhang, M. Zhang, S. -N. Zhang,W. -D. Zhang,W. -J. Zhang, Y. -H. Zhang, Z. Zhang, Z. -L. Zhang,D. -H. Zhao,H. -S. Zhao,X. -F. Zhao,Z. -J. Zhao,L. -X. Zhou,Y. -L. Zhou,Y. -X. Zhu,Z. -C. Zhu,X. -X. Zuo

Nature Astronomypp.1-13, (2025)

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The Einstein Probe Transient EP240414a: Linking Fast X-ray Transients, Gamma-ray Bursts and Luminous Fast Blue Optical Transients

The Astrophysical Journal Lettersno. 2 (2025): L47

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EP240801a/XRF 240801B: an X-ray Flash Detected by the Einstein Probe and Implications of Its Multiband Afterglow

Shuai-Qing Jiang,Dong Xu, Agnes P. C. van Hoof,Wei-Hua Lei, Yuan Liu,Hao Zhou,Yong Chen, Shao-Yu Fu,Jun Yang, Xing Liu, Zi-Pei Zhu,Alexei V. Filippenko, Peter G. Jonker, A. S. Pozanenko,He Gao,Xue-Feng Wu,Bing Zhang,Gavin P Lamb,Massimiliano De Pasquale,Shiho Kobayashi,Franz Erik Bauer, Hui Sun,Giovanna Pugliese, Jie An, Valerio D'Elia, Johan P. U. Fynbo,WeiKang Zheng, Alberto J. C. Tirado, Yi-Han Iris Yin,Yuan-Chuan Zou,Adam T. Deller, N. S. Pankov, A. A. Volnova, A. S. Moskvitin, O. I. Spiridonova, D. V. Oparin, V. Rumyantsev, O. A. Burkhonov, Sh. A. Egamberdiyev, V. Kim, M. Krugov, A. M. Tatarnikov, R. Inasaridze, Andrew J. Levan,Daniele Bjørn Malesani, Maria E. Ravasio, Jonathan Quirola-Vásquez, Joyce N. D. van Dalen, Javi Sánchez-Sierras, Daniel Mata Sánchez, Stuart P. Littlefair, Jennifer A. Chacón, Manuel A. P. Torres, Ashley A. Chrimes, Nikhil Sarin,Antonio Martin-Carrillo,Vik Dhillon,Yi Yang,Thomas G. Brink,Rebecca L. Davies,Sheng Yang,Amar Aryan, Ting-Wan Chen, Albert K. H. Kong,Wen-Xiong Li, Rui-Zhi Li,Jirong Mao, Ignacio Pérez-García, Emilio J. Fernández-García, Moira Andrews,Joseph Farah,Zhou Fan, Estefania Padilla Gonzalez,D. Andrew Howell,Dieter Hartmann, Jing-Wei Hu, Páll Jakobsson, Cheng-Kui Li,Zhi-Xing Ling,Curtis McCully,Megan Newsome,Benjamin Schneider, Kaew Samaporn Tinyanont, Ning-Chen Sun, Giacomo Terreran,Qing-Wen Tang, Wen-Xin Wang, Jing-Jing Xu,Wei-Min Yuan,Bin-Bin Zhang,Hai-Sheng Zhao,Juan Zhang

arxiv（2025）

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GRB 241030A: a Prompt Thermal X-ray Emission Component and Diverse Origin of the Very Early UVOT WHITE and U Band Emission