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We present a novel approach for classifying stars as binary or exoplanet using deep learning techniques. Our method utilizes feature extraction, wavelet transformation, and a neural network on the light curves of stars to achieve…

Instrumentation and Methods for Astrophysics · Physics 2023-05-22 Aman Kumar , Sarvesh Gharat

A procedure is described for estimating an optimum kernel for the detection by convolution of signals among Poissonian noise. The technique is applied to the detection of x-ray point sources in XMM-Newton data, and is shown to yield an…

Astrophysics · Physics 2009-11-11 Ian Stewart

The Euclid Space Telescope will provide deep imaging at optical and near-infrared wavelengths, along with slitless near-infrared spectroscopy, across ~15,000 sq deg of the sky. Euclid is expected to detect ~12 billion astronomical sources,…

Instrumentation and Methods for Astrophysics · Physics 2023-03-15 Euclid Collaboration , A. Humphrey , L. Bisigello , P. A. C. Cunha , M. Bolzonella , S. Fotopoulou , K. Caputi , C. Tortora , G. Zamorani , P. Papaderos , D. Vergani , J. Brinchmann , M. Moresco , A. Amara , N. Auricchio , M. Baldi , R. Bender , D. Bonino , E. Branchini , M. Brescia , S. Camera , V. Capobianco , C. Carbone , J. Carretero , F. J. Castander , M. Castellano , S. Cavuoti , A. Cimatti , R. Cledassou , G. Congedo , C. J. Conselice , L. Conversi , Y. Copin , L. Corcione , F. Courbin , M. Cropper , A. Da Silva , H. Degaudenzi , M. Douspis , F. Dubath , C. A. J. Duncan , X. Dupac , S. Dusini , S. Farrens , S. Ferriol , M. Frailis , E. Franceschi , M. Fumana , P. Gomez-Alvarez , S. Galeotta , B. Garilli , W. Gillard , B. Gillis , C. Giocoli , A. Grazian , F. Grupp , L. Guzzo , S. V. H. Haugan , W. Holmes , F. Hormuth , K. Jahnke , M. Kummel , S. Kermiche , A. Kiessling , M. Kilbinger , T. Kitching , R. Kohley , M. Kunz , H. Kurki-Suonio , S. Ligori , P. B. Lilje , I. Lloro , E. Maiorano , O. Mansutti , O. Marggraf , K. Markovic , F. Marulli , R. Massey , S. Maurogordato , H. J. McCracken , E. Medinaceli , M. Melchior , M. Meneghetti , E. Merlin , G. Meylan , L. Moscardini , E. Munari , R. Nakajima , S. M. Niemi , J. Nightingale , C. Padilla , S. Paltani , F. Pasian , K. Pedersen , V. Pettorino , S. Pires , M. Poncet , L. Popa , L. Pozzetti , F. Raison , A. Renzi , J. Rhodes , G. Riccio , E. Romelli , M. Roncarelli , E. Rossetti , R. Saglia , D. Sapone , B. Sartoris , R. Scaramella , P. Schneider , M. Scodeggio , A. Secroun , G. Seidel , C. Sirignano , G. Sirri , L. Stanco , P. Tallada-Crespi , D. Tavagnacco , A. N. Taylor , I. Tereno , R. Toledo-Moreo , F. Torradeflot , I. Tutusaus , L. Valenziano , T. Vassallo , Y. Wang , J. Weller , A. Zacchei , J. Zoubian , S. Andreon , S. Bardelli , A. Boucaud , R. Farinelli , J. Gracia-Carpio , D. Maino , N. Mauri , S. Mei , N. Morisset , F. Sureau , M. Tenti , A. Tramacere , E. Zucca , C. Baccigalupi , A. Balaguera-Antolinez , A. Biviano , A. Blanchard , S. Borgani , E. Bozzo , C. Burigana , R. Cabanac , A. Cappi , C. S. Carvalho , S. Casas , G. Castignani , C. Colodro-Conde , A. R. Cooray , J. Coupon , H. M. Courtois , O. Cucciati , S. Davini , G. De Lucia , H. Dole , J. A. Escartin , S. Escoffier , M. Fabricius , M. Farina , F. Finelli , K. Ganga , J. Garcia-Bellido , K. George , F. Giacomini , G. Gozaliasl , I. Hook , M. Huertas-Company , B. Joachimi , V. Kansal , A. Kashlinsky , E. Keihanen , C. C. Kirkpatrick , V. Lindholm , G. Mainetti , R. Maoli , S. Marcin , M. Martinelli , N. Martinet , M. Maturi , R. B. Metcalf , G. Morgante , A. A. Nucita , L. Patrizii , A. Peel , J. E. Pollack , V. Popa , C. Porciani , D. Potter , P. Reimberg , A. G. Sanchez , M. Schirmer , M. Schultheis , V. Scottez , E. Sefusatti , J. Stadel , R. Teyssier , C. Valieri , J. Valiviita , M. Viel , F. Calura , H. Hildebrandt

The discovery and subsequent study of optical counterparts to transient sources is crucial for their complete astrophysical understanding. Various gamma ray burst (GRB) detectors, and more notably the ground--based gravitational wave…

Instrumentation and Methods for Astrophysics · Physics 2022-09-29 Javed Rana , Akshat Singhal , Bhooshan Gadre , Varun Bhalerao , Sukanta Bose

Future space telescopes may be able to directly image $\sim$10 - 100 planets with sizes and orbits consistent with habitable surface conditions ("exo-Earth candidates" or EECs), but observers will face difficulty in distinguishing these…

Earth and Planetary Astrophysics · Physics 2020-02-27 Alex Bixel , Dániel Apai

The launch of the \textit{Einstein Probe} unleashed a new era of high-energy transient discovery in the largely unexplored soft X-ray band. The \textit{Einstein Probe} has detected a significant number of fast X-ray transients that display…

In modern astrophysics, the machine learning has increasingly gained more popularity with its incredibly powerful ability to make predictions or calculated suggestions for large amounts of data. We describe an application of the supervised…

Astrophysics of Galaxies · Physics 2018-12-26 Yu Bai , JiFeng Liu , Song Wang , Fan Yang

Because of the electromagnetic radiation produced during the merger, compact binary coalescences with neutron stars may result in multi-messenger observations. In order to follow up on the gravitational-wave signal with electromagnetic…

Energy dispersive X-ray (EDX) spectrum imaging yields compositional information with a spatial resolution down to the atomic level. However, experimental limitations often produce extremely sparse and noisy EDX spectra. Under such…

Stars are ubiquitous X-ray emitters and will be a substantial fraction of the X-ray sources detected in the on-going all-sky survey performed by the eROSITA instrument aboard the Spectrum Roentgen Gamma (SRG) observatory. We use the X-ray…

Solar and Stellar Astrophysics · Physics 2022-05-18 P. C. Schneider , S. Freund , S. Czesla , J. Robrade , M. Salvato , J. H. M. M. Schmitt

We report the discovery of a peculiar X-ray transient, EP240408a, by Einstein Probe (EP) and follow-up studies made with EP, Swift, NICER, GROND, ATCA and other ground-based multi-wavelength telescopes. The new transient was first detected…

High Energy Astrophysical Phenomena · Physics 2024-10-30 Wenda Zhang , Weimin Yuan , Zhixing Ling , Yong Chen , Nanda Rea , Arne Rau , Zhiming Cai , Huaqing Cheng , Francesco Coti Zelati , Lixin Dai , Jingwei Hu , Shumei Jia , Chichuan Jin , Dongyue Li , Paul O'Brien , Rongfeng Shen , Xinwen Shu , Shengli Sun , Xiaojin Sun , Xiaofeng Wang , Lei Yang , Bing Zhang , Chen Zhang , Shuang-Nan Zhang , Yonghe Zhang , Jie An , David Buckley , Alexis Coleiro , Bertrand Cordier , Liming Dou , Rob Eyles-Ferris , Zhou Fan , Hua Feng , Shaoyu Fu , Johan P. U. Fynbo , Lluis Galbany , Saurabh W. Jha , Shuaiqing Jiang , Albert Kong , Erik Kuulkers , Weihua Lei , Wenxiong Li , Bifang Liu , Mingjun Liu , Xing Liu , Yuan Liu , Zhu Liu , Chandreyee Maitra , Alessio Marino , Itumeleng Monageng , Kirpal Nandra , Jeremy Sanders , Roberto Soria , Lian Tao , Junfeng Wang , Song Wang , Tinggui Wang , Zhongxiang Wang , Qingwen Wu , Xuefeng Wu , Dong Xu , Yanjun Xu , Suijian Xue , Yongquan Xue , Zijian Zhang , Zipei Zhu , Hu Zou , Congying Bao , Fansheng Chen , Houlei Chen , Tianxiang Chen , Wei Chen , Yehai Chen , Yifan Chen , Chenzhou Cui , Weiwei Cui , Yanfeng Dai , Dongwei Fan , Ju Guan , Dawei Han , Dongjie Hou , Haibo Hu , Maohai Huang , Jia Huo , Zhenqing Jia , Bowen Jiang , Ge Jin , Chengkui Li , Junfei Li , Longhui Li , Maoshun Li , Wei Li , Zhengda Li , Tianying Lian , Congzhan Liu , Heyang Liu , Huaqiu Liu , Fangjun Lu , Laidan Luo , Jia Ma , Xuan Mao , Haiwu Pan , Xin Pan , Liming Song , Hui Sun , Yunyin Tan , Qingjun Tang , Yihan Tao , Hao Wang , Juan Wang , Lei Wang , Wenxin Wang , Yilong Wang , Yusa Wang , Qinyu Wu , Haitao Xu , Jingjing Xu , Xinpeng Xu , Yunfei Xu , Zhao Xu , Changbin Xue , Yulong Xue , Ailiang Yan , Haonan Yang , Xiongtao Yang , Yanji Yang , Juan Zhang , Mo Zhang , Wenjie Zhang , Zhen Zhang , Zhen Zhang , Ziliang Zhang , Donghua Zhao , Haisheng Zhao , Xiaofan Zhao , Zijian Zhao , Hongyan Zhou , Yilin Zhou , Yuxuan Zhu , Zhencai Zhu

Power systems are developing very fast nowadays, both in size and in complexity; this situation is a challenge for Early Event Detection (EED). This paper proposes a data- driven unsupervised learning method to handle this challenge.…

Methodology · Statistics 2015-09-16 Xing He , Robert Caiming Qiu , Qian Ai , Yinshuang Cao , Jie Gu , Zhijian Jin

With the coming data deluge from synoptic surveys, there is a growing need for frameworks that can quickly and automatically produce calibrated classification probabilities for newly-observed variables based on a small number of time-series…

XMM-Newton provides unprecedented insight into the X-ray Universe, recording variability information for hundreds of thousands of sources. Manually searching for interesting patterns in light curves is impractical, requiring an automated…

Instrumentation and Methods for Astrophysics · Physics 2022-03-14 Miloš Kovačević , Mario Pasquato , Martino Marelli , Andrea De Luca , Ruben Salvaterra , Andrea Belfiore Mondoni

Wildfires present intricate challenges for prediction, necessitating the use of sophisticated machine learning techniques for effective modeling\cite{jain2020review}. In our research, we conducted a thorough assessment of various machine…

Machine Learning · Computer Science 2024-04-03 Di Fan , Ayan Biswas , James Paul Ahrens

Convolution Neural Networks trained for the task of lens finding with similar architecture and training data as is commonly found in the literature are biased classifiers. An understanding of the selection function of lens finding neural…

Cosmology and Nongalactic Astrophysics · Physics 2023-07-21 A. Herle , C. M. O'Riordan , S. Vegetti

With the advent of new spectroscopic surveys from ground and space, observing up to hundreds of millions of galaxies, spectra classification will become overwhelming for standard analysis techniques. To prepare for this challenge, we…

Astrophysics of Galaxies · Physics 2022-06-08 Fucheng Zhong , Rui Li , Nicola R. Napolitano

Despite being operational for only a short time, the Einstein Probe mission, with its large field of view and rapid localisation capabilities, has already significantly advanced the study of rapid variability in the soft X-ray sky. We…

Learning at the edge is a challenging task from several perspectives, since data must be collected by end devices (e.g. sensors), possibly pre-processed (e.g. data compression), and finally processed remotely to output the result of…

Signal Processing · Electrical Eng. & Systems 2022-04-26 Mattia Merluzzi , Claudio Battiloro , Paolo Di Lorenzo , Emilio Calvanese Strinati

The search for atmospheric biosignatures in Earth-like exoplanets is one of the most pressing challenges in observational astrobiology. Detecting biogenic gases in terrestrial planets requires high-resolution observations and long…

Earth and Planetary Astrophysics · Physics 2025-04-03 David S. Duque-Castaño , Jorge I. Zuluaga , Lauren Flor-Torres
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