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  1. Book ; Online: The Tiny Time-series Transformer

    Allam Jr., Tarek / Peloton, Julien / McEwen, Jason D.

    Low-latency High-throughput Classification of Astronomical Transients using Deep Model Compression

    2023  

    Abstract: A new golden age in astronomy is upon us, dominated by data. Large astronomical surveys are broadcasting unprecedented rates of information, demanding machine learning as a critical component in modern scientific pipelines to handle the deluge of data. ... ...

    Abstract A new golden age in astronomy is upon us, dominated by data. Large astronomical surveys are broadcasting unprecedented rates of information, demanding machine learning as a critical component in modern scientific pipelines to handle the deluge of data. The upcoming Legacy Survey of Space and Time (LSST) of the Vera C. Rubin Observatory will raise the big-data bar for time-domain astronomy, with an expected 10 million alerts per-night, and generating many petabytes of data over the lifetime of the survey. Fast and efficient classification algorithms that can operate in real-time, yet robustly and accurately, are needed for time-critical events where additional resources can be sought for follow-up analyses. In order to handle such data, state-of-the-art deep learning architectures coupled with tools that leverage modern hardware accelerators are essential. We showcase how the use of modern deep compression methods can achieve a $18\times$ reduction in model size, whilst preserving classification performance. We also show that in addition to the deep compression techniques, careful choice of file formats can improve inference latency, and thereby throughput of alerts, on the order of $8\times$ for local processing, and $5\times$ in a live production setting. To test this in a live setting, we deploy this optimised version of the original time-series transformer, t2, into the community alert broking system of FINK on real Zwicky Transient Facility (ZTF) alert data, and compare throughput performance with other science modules that exist in FINK. The results shown herein emphasise the time-series transformer's suitability for real-time classification at LSST scale, and beyond, and introduce deep model compression as a fundamental tool for improving deploy-ability and scalable inference of deep learning models for transient classification.

    Comment: 16 pages, 11 figures
    Keywords Astrophysics - Instrumentation and Methods for Astrophysics ; Computer Science - Machine Learning
    Subject code 006
    Publishing date 2023-03-15
    Publishing country us
    Document type Book ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  2. Book ; Online: Fink

    Leoni, Marco / Ishida, Emille E. O. / Peloton, Julien / Möller, Anais

    early supernovae Ia classification using active learning

    2021  

    Abstract: We describe how the Fink broker early supernova Ia classifier optimizes its ML classifications by employing an active learning (AL) strategy. We demonstrate the feasibility of implementation of such strategies in the current Zwicky Transient Facility ( ... ...

    Abstract We describe how the Fink broker early supernova Ia classifier optimizes its ML classifications by employing an active learning (AL) strategy. We demonstrate the feasibility of implementation of such strategies in the current Zwicky Transient Facility (ZTF) public alert data stream. We compare the performance of two AL strategies: uncertainty sampling and random sampling. Our pipeline consists of 3 stages: feature extraction, classification and learning strategy. Starting from an initial sample of 10 alerts (5 SN Ia and 5 non-Ia), we let the algorithm identify which alert should be added to the training sample. The system is allowed to evolve through 300 iterations. Our data set consists of 23 840 alerts from the ZTF with confirmed classification via cross-match with SIMBAD database and the Transient name server (TNS), 1 600 of which were SNe Ia (1 021 unique objects). The data configuration, after the learning cycle was completed, consists of 310 alerts for training and 23 530 for testing. Averaging over 100 realizations, the classifier achieved 89% purity and 54% efficiency. From 01/November/2020 to 31/October/2021 Fink has applied its early supernova Ia module to the ZTF stream and communicated promising SN Ia candidates to the TNS. From the 535 spectroscopically classified Fink candidates, 459 (86%) were proven to be SNe Ia. Our results confirm the effectiveness of active learning strategies for guiding the construction of optimal training samples for astronomical classifiers. It demonstrates in real data that the performance of learning algorithms can be highly improved without the need of extra computational resources or overwhelmingly large training samples. This is, to our knowledge, the first application of AL to real alerts data.

    Comment: accepted for publication in Astronomy and Astrophysics
    Keywords Astrophysics - Instrumentation and Methods for Astrophysics ; Astrophysics - Cosmology and Nongalactic Astrophysics ; Computer Science - Machine Learning
    Subject code 006
    Publishing date 2021-11-22
    Publishing country us
    Document type Book ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  3. Article ; Online: Internal Delensing of Cosmic Microwave Background Polarization B-Modes with the POLARBEAR Experiment.

    Adachi, S / Aguilar Faúndez, M A O / Akiba, Y / Ali, A / Arnold, K / Baccigalupi, C / Barron, D / Beck, D / Bianchini, F / Borrill, J / Carron, J / Cheung, K / Chinone, Y / Crowley, K / El Bouhargani, H / Elleflot, T / Errard, J / Fabbian, G / Feng, C /
    Fujino, T / Goeckner-Wald, N / Hasegawa, M / Hazumi, M / Hill, C A / Howe, L / Katayama, N / Keating, B / Kikuchi, S / Kusaka, A / Lee, A T / Leon, D / Linder, E / Lowry, L N / Matsuda, F / Matsumura, T / Minami, Y / Namikawa, T / Navaroli, M / Nishino, H / Peloton, J / Pham, A T P / Poletti, D / Puglisi, G / Reichardt, C L / Segawa, Y / Sherwin, B D / Silva-Feaver, M / Siritanasak, P / Stompor, R / Tajima, O / Takatori, S / Tanabe, D / Teply, G P / Vergès, C

    Physical review letters

    2020  Volume 124, Issue 13, Page(s) 131301

    Abstract: Using only cosmic microwave background polarization data from the polarbear experiment, we measure B-mode polarization delensing on subdegree scales at more than 5σ significance. We achieve a 14% B-mode power variance reduction, the highest to date for ... ...

    Abstract Using only cosmic microwave background polarization data from the polarbear experiment, we measure B-mode polarization delensing on subdegree scales at more than 5σ significance. We achieve a 14% B-mode power variance reduction, the highest to date for internal delensing, and improve this result to 22% by applying for the first time an iterative maximum a posteriori delensing method. Our analysis demonstrates the capability of internal delensing as a means of improving constraints on inflationary models, paving the way for the optimal analysis of next-generation primordial B-mode experiments.
    Language English
    Publishing date 2020-04-17
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.124.131301
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  4. Article ; Online: Measurement of the cosmic microwave background polarization lensing power spectrum with the POLARBEAR experiment.

    Ade, P A R / Akiba, Y / Anthony, A E / Arnold, K / Atlas, M / Barron, D / Boettger, D / Borrill, J / Chapman, S / Chinone, Y / Dobbs, M / Elleflot, T / Errard, J / Fabbian, G / Feng, C / Flanigan, D / Gilbert, A / Grainger, W / Halverson, N W /
    Hasegawa, M / Hattori, K / Hazumi, M / Holzapfel, W L / Hori, Y / Howard, J / Hyland, P / Inoue, Y / Jaehnig, G C / Jaffe, A / Keating, B / Kermish, Z / Keskitalo, R / Kisner, T / Le Jeune, M / Lee, A T / Linder, E / Leitch, E M / Lungu, M / Matsuda, F / Matsumura, T / Meng, X / Miller, N J / Morii, H / Moyerman, S / Myers, M J / Navaroli, M / Nishino, H / Paar, H / Peloton, J / Quealy, E / Rebeiz, G / Reichardt, C L / Richards, P L / Ross, C / Schanning, I / Schenck, D E / Sherwin, B / Shimizu, A / Shimmin, C / Shimon, M / Siritanasak, P / Smecher, G / Spieler, H / Stebor, N / Steinbach, B / Stompor, R / Suzuki, A / Takakura, S / Tomaru, T / Wilson, B / Yadav, A / Zahn, O

    Physical review letters

    2014  Volume 113, Issue 2, Page(s) 21301

    Abstract: Gravitational lensing due to the large-scale distribution of matter in the cosmos distorts the primordial cosmic microwave background (CMB) and thereby induces new, small-scale B-mode polarization. This signal carries detailed information about the ... ...

    Abstract Gravitational lensing due to the large-scale distribution of matter in the cosmos distorts the primordial cosmic microwave background (CMB) and thereby induces new, small-scale B-mode polarization. This signal carries detailed information about the distribution of all the gravitating matter between the observer and CMB last scattering surface. We report the first direct evidence for polarization lensing based on purely CMB information, from using the four-point correlations of even- and odd-parity E- and B-mode polarization mapped over ∼30 square degrees of the sky measured by the POLARBEAR experiment. These data were analyzed using a blind analysis framework and checked for spurious systematic contamination using null tests and simulations. Evidence for the signal of polarization lensing and lensing B modes is found at 4.2σ (stat+sys) significance. The amplitude of matter fluctuations is measured with a precision of 27%, and is found to be consistent with the Lambda cold dark matter cosmological model. This measurement demonstrates a new technique, capable of mapping all gravitating matter in the Universe, sensitive to the sum of neutrino masses, and essential for cleaning the lensing B-mode signal in searches for primordial gravitational waves.
    Language English
    Publishing date 2014-07-11
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.113.021301
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  5. Article ; Online: Evidence for gravitational lensing of the cosmic microwave background polarization from cross-correlation with the cosmic infrared background.

    Ade, P A R / Akiba, Y / Anthony, A E / Arnold, K / Atlas, M / Barron, D / Boettger, D / Borrill, J / Borys, C / Chapman, S / Chinone, Y / Dobbs, M / Elleflot, T / Errard, J / Fabbian, G / Feng, C / Flanigan, D / Gilbert, A / Grainger, W /
    Halverson, N W / Hasegawa, M / Hattori, K / Hazumi, M / Holzapfel, W L / Hori, Y / Howard, J / Hyland, P / Inoue, Y / Jaehnig, G C / Jaffe, A / Keating, B / Kermish, Z / Keskitalo, R / Kisner, T / Le Jeune, M / Lee, A T / Leitch, E M / Linder, E / Lungu, M / Matsuda, F / Matsumura, T / Meng, X / Miller, N J / Morii, H / Moyerman, S / Myers, M J / Navaroli, M / Nishino, H / Paar, H / Peloton, J / Poletti, D / Quealy, E / Rebeiz, G / Reichardt, C L / Richards, P L / Ross, C / Rotermund, K / Schanning, I / Schenck, D E / Sherwin, B D / Shimizu, A / Shimmin, C / Shimon, M / Siritanasak, P / Smecher, G / Spieler, H / Stebor, N / Steinbach, B / Stompor, R / Suzuki, A / Takakura, S / Tikhomirov, A / Tomaru, T / Wilson, B / Yadav, A / Zahn, O

    Physical review letters

    2014  Volume 112, Issue 13, Page(s) 131302

    Abstract: We reconstruct the gravitational lensing convergence signal from cosmic microwave background (CMB) polarization data taken by the Polarbear experiment and cross-correlate it with cosmic infrared background maps from the Herschel satellite. From the cross ...

    Abstract We reconstruct the gravitational lensing convergence signal from cosmic microwave background (CMB) polarization data taken by the Polarbear experiment and cross-correlate it with cosmic infrared background maps from the Herschel satellite. From the cross spectra, we obtain evidence for gravitational lensing of the CMB polarization at a statistical significance of 4.0σ and indication of the presence of a lensing B-mode signal at a significance of 2.3σ. We demonstrate that our results are not biased by instrumental and astrophysical systematic errors by performing null tests, checks with simulated and real data, and analytical calculations. This measurement of polarization lensing, made via the robust cross-correlation channel, not only reinforces POLARBEAR auto-correlation measurements, but also represents one of the early steps towards establishing CMB polarization lensing as a powerful new probe of cosmology and astrophysics.
    Language English
    Publishing date 2014-04-04
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.112.131302
    Database MEDical Literature Analysis and Retrieval System OnLINE

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