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1. Two-pole microring weight banks

   https://doi.org/10.1364/OL.43.002276  

   Tait, Alexander N.; Wu, Allie X.; Ferreira de Lima, Thomas; Nahmias, Mitchell A.; Shastri, Bhavin J.; Prucnal, Paul R. (January 2018, Optics Letters)
2. Minimal pole representation for spectral functions

   https://doi.org/10.1063/5.0273763  

   Zhang, Lei; Erpenbeck, André; Yu, Yang; Gull, Emanuel (June 2025, The Journal of Chemical Physics)

   Representing spectral densities, real-frequency, and real-time Green’s functions of continuous systems by a small discrete set of complex poles is a ubiquitous problem in condensed matter physics, with applications ranging from quantum transport simulations to the simulation of strongly correlated electron systems. This paper introduces a method for obtaining a compact, approximate representation of these functions, based on their parameterization on the real axis and a given approximate precision. We show applications to typical spectral functions and results for structured and unstructured correlation functions of model systems. 

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3. POLE: polarized embedding for signed networks

   Z. Huang; A. Silva; A. K. Singh (January 2022, WSDM ’22: The Fifteenth ACM International Conference on Web Search and Data Mining)
4. HEROES: The Hawaii eROSITA Ecliptic Pole Survey Catalog

   https://doi.org/10.3847/1538-4365/accd70  

   Taylor, A. J.; Barger, A. J.; Cowie, L. L.; Hasinger, G.; Hu, E. M.; Songaila, A. (May 2023, The Astrophysical Journal Supplement Series)

   Abstract We present a seven-band (g,r,i,z,y, NB816, NB921) catalog derived from a Subaru Hyper Suprime-Cam (HSC) imaging survey of the North Ecliptic Pole (NEP). The survey, known as HEROES, consists of 44 deg²of contiguous imaging reaching median 5σdepths ofg: 26.5,r: 26.2,i: 25.7,z: 25.1,y: 23.9, NB816: 24.4, and NB921: 24.4 mag. We reduced these data with the HSC pipeline softwarehscPipe, and produced a resulting multiband catalog containing over 25 million objects. We provide the catalog in three formats: (1) a collection ofhscPipeformat forced photometry catalogs, (2) a single combined catalog containing every object in that data set with selected useful columns, and (3) a smaller variation of the combined catalog with only essential columns for basic analysis or low-memory machines. The catalog uses all the available HSC data on the NEP and may serve as the primary optical catalog for current and future NEP deep fields from instruments and observatories such as SCUBA-2, eROSITA, Spitzer, Euclid, and JWST. 

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5. SOAR PPT (Pensacola-Pole Transect) gridded aerogeophysical observations

   https://doi.org/10.18738/t8/smlowr  

   Blankenship, Donald; Holt, John; Kempf, Scott; Morse, David; Davis, Marcy; Bell, Robin; Arko, Robert; Young, Duncan A; Kempf, Scott D (January 2025, Texas Data Repository)

   {"Abstract":["The PPT survey extended from the Ross Ice Shelf, southward over the TAM along 150W between the Scott and Reedy Glaciers, and through the South Pole. Approximately 15,000 line km were flown. North-south oriented transects were flown 10 km apart and west-east tie lines were flown with a 30 km line spacing. Fifteen km long transect 'run-ins' and 'run-outs' were added to each line, thus ensuring data collection to survey boundaries. Laser altimetry, ice-penetrating radar, gravity and magnetic field intensity data were collected. This work was funded by NSF-OPP grant 9615832 with the project title: Collaborative Research: Contrasting Architecture and Dynamics of the Transantarctic Mountains (Pensacola-Pole Transect). Principal Investigators were D.D. Blankenship, University of Texas Institute for Geophysics, and R.E. Bell and W.R. Buck, Lamont-Doherty Earth Observatory.\n<br>\n<br>\nThis work was conducted by the Support Office for Aerogeophysical Research (SOAR) NSF facility under cooperative agreement OPP-9319379. The 1998/1999 field season <a href="http://hdl.handle.net/2152/65412"> report </a>(Holt et al 1999) describes the field work in more detail.\n<br>\n<br>\nThese data are gridded orthogonal data with a point every 850 m. Data is in a space delimited ASCII table with three columns: Longitude, Latitude and geophysical observation. Grids are smoothed using a Gaussian filter (2.125 km for gravity, magnetic field anomaly, surface elevation and 8.5 km for ice thickness) and surfaced using a bicubic spline method.\n<br>\nObservations include:\n<ol>\n<li> Bed elevation (m, WGS-84) </li> \n<li> Gravity disturbance (mGal, WGS-84) </li> \n<li> Ice Thickness (m) </li> \n<li> Laser Derived Surface Elevation (m, WGS-84) </li> \n<li> Magnetic Anomaly (nT, IGRF) </li> \n<li> Radar Derived Surface Elevation (m, WGS-84) </li> \n</ol>\nA browse image is included. \n<br><br>\n<i>Acknowledgement: </i><br>\nIn keeping with NSF Grant Policy, any publication using these data (including web documents) must contain the following acknowledgment: "This material is based on work supported by the National Science Foundation under cooperative agreement OPP-9319379." Also, any oral presentation utilizing these materials should acknowledge the support of the National Science Foundation. In addition, we request that any oral presentation, web page or publication also acknowledge SOAR and the University of Texas. A suitable citation for PPT data is:\n<br>\n<i>Davis, M.B., 2001, Subglacial Morphology and Structural Geology in the Southern Transantarctic Mountains from Airborne Geophysics, M.S. Thesis, Univ. of Texas, 133 pp.<a href="http://dx.doi.org/10.26153/tsw/2786">doi:10.26153/tsw/2786</a></i>\n<br>\nThese data represent the data that was hosted on the UTIG webpage at https://www-udc.ig.utexas.edu/external/facilities/aero/data/soar/PPT/SOAR_ppt.htm."]} 

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