Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Anik Halder"'
Publikováno v:
Gynecologic Oncology Reports, Vol 55, Iss , Pp 101481- (2024)
Introduction: Cervical cancer is an important public health issue in Bangladesh. Despite government efforts, the awareness and healthcare utilization in rural areas are inadequate. Methodology: This cross-sectional study was conducted in six district
Externí odkaz:
https://doaj.org/article/ce924bde16594ca080dff5bd209b74f9
Publikováno v:
The Astrophysical Journal, Vol 971, Iss 2, p 156 (2024)
Modern cosmological research in large-scale structure has witnessed an increasing number of machine-learning applications. Among them, convolutional neural networks (CNNs) have received substantial attention due to their outstanding performance in im
Externí odkaz:
https://doaj.org/article/d46a894749c745088a6fec90c2320c17
Autor:
Oliver Friedrich, Anik Halder, Aoife Boyle, Cora Uhlemann, Dylan Britt, Sandrine Codis, Daniel Gruen, ChangHoon Hahn
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, 510 (4), pp.5069-5087. ⟨10.1093/mnras/stab3703⟩
Monthly Notices of the Royal Astronomical Society, 2022, 510 (4), pp.5069-5087. ⟨10.1093/mnras/stab3703⟩
We study the connection of matter density and its tracers from the PDF perspective. One aspect of this connection is the conditional expectation value $\langle \delta_{\mathrm{tracer}}|\delta_m\rangle$ when averaging both tracer and matter density ov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 506:2780-2803
We present the integrated 3-point shear correlation function $i\zeta_{\pm}$ -- a higher-order statistic of the cosmic shear field -- which can be directly estimated in wide-area weak lensing surveys without measuring the full 3-point shear correlatio
Autor:
Anik Halder, Alexandre Barreira
The integrated shear 3-point correlation function $\zeta_{\pm}$ is a higher-order statistic of the cosmic shear field that describes the modulation of the 2-point correlation function $\xi_{\pm}$ by long-wavelength features in the field. Here, we int
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::48f391126881bb86857487610eb02a1a
http://arxiv.org/abs/2201.05607
http://arxiv.org/abs/2201.05607