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48 results for “Aquila”
Figure 2 in Diet of Dasyatis pastinaca and Myliobatis aquila (Myliobatiformes) from the Azores, NE Atlantic
Figure 2. - Cumulated trophic diversity and number of sampled stomachs from Dasyatis pastinaca from Terceira Island, Azores, NE Atlantic.
Figure 1 in Diet of Dasyatis pastinaca and Myliobatis aquila (Myliobatiformes) from the Azores, NE Atlantic
Figure 1. - Sampling sites of Dasyatis pastinaca and Myliobatis aquila in Terceira Island, Azores, NE Atlantic. BI: Biscoitos; CR: Cinco Ribeiras; VM: Vila Maria Bay.
The supporting data for the paper "Synergistic Enhancement of LSTM Time Series Prediction via Companion Strategy and Decay Operator-Improved Aquila Optimization"
<p>数据生成程序</p> <p>该数据集是使用 The Investor's Exchange API 生成的,脚本会定期获取标准普尔 500 指数中所有公司的历史股价。详细说明和脚本可以在 GitHub 存储库中找到。该数据每5年更新一次,最近一次更新于2018年2月。</p> <p> </p> <p>数据处理方法和步骤</p> <p>数据处理的主要步骤包括:</p> <p> </p> <p>数据采集:使用 API 获取每只股票的历史数据,存储在.csv文件中。</p> <p>数据清理:删除重复条目,纠正格式错误,确保数据完整性。</p> <p>数据合并:将单个股票数据合并到一个大.csv文件中,以便于使用。</p> <p>数据验证:通过检查时间序列的连续性和完整性来验证数据的准确性。</p> <p>使用的设备和工具</p> <p>数据采集工具:Python 脚本</p> <p>数据处理工具:用于数据清洗和处理的 Pandas 库</p> <p>数据存储:CSV文件格式</p> <p>时间和地理范围</p> <p>时间范围:数据涵盖过去 5 年的历史股票价格,最新更新于 2018 年 2 月。</p> <p>地理范围:数据涵盖标准普尔500指数中的所有公司,主要是美国市场数据。</p> <p>时间和空间分辨率</p> <p>时间分辨率:每日数据,每个交易日一条记录。</p> <p>空间分辨率:无地理空间分辨率;数据按公司分组。</p> <p>表格数据</p> <p>条目总数:条目总数取决于标准普尔500指数中的公司数量和总交易日数。</p> <p>行标题和列标题:</p> <p>日期:交易日期格式为yy-mm-dd</p> <p>开盘价:开盘价(美元)</p> <p>最高价:当日最高价(美元)</p> <p>最低价:当日最低价格(美元)</p> <p>收盘价:收盘价(美元)</p> <p>交易量:成交股数</p> <p>名称:以股票代码的名义</p> <p>缺失数据</p> <p>数据集在某些交易日可能缺少数据,主要是由于非交易日(例如节假日)或API数据采集过程中的临时网络问题。这些缺失的数据通常不会影响整体分析结果。</p> <p> </p> <p>数据错误</p> <p>由于数据源是第三方 API,因此数据错误的可能性很低。如果发现错误,通常是由于 API 数据采集过程中的临时网络问题造成的。数据清理过程旨在最大限度地减少和纠正这些错误。</p> <p> </p> <p>数据文件说明</p> <p>数据文件类型:</p> <p>all_stocks_5yr.csv:包含所有股票的合并数据文件。</p> <p>individual_stocks_5yr文件夹:包含每个股票的单个.csv文件。</p> <p>文件内容和格式:文件采用 CSV 格式,每个文件包含日期、开盘价、最高价、最低价、收盘价、成交量和股票名称列。</p> <p>文件大小:文件大小取决于特定股票的交易数据量,通常从几MB到几十MB不等。</p> <p>文件格式说明</p> <p>数据以通用的 CSV 格式存储,可以使用 Excel、Notepad++ 或任何支持 CSV 文件的工具打开和查看。对于进一步的数据处理和分析,可以使用 Python Pandas 库。</p> <p> </p> <p>总结</p> <p>该数据集提供过去5年标准普尔500指数中所有公司的历史股价数据,包括开盘价、最高价、最低价、收盘价、交易量等详细信息。它适用于各种财务数据分析和建模应用。数据通过 API 获取并处理,以确保准确性和完整性。</p>
"Aquila della Vittoria". Santomero (TE).
My 3D reconstruction generated with photogrammetry software 3DF Zephyr v5.007 processing 161 immagini. Modello realizzato per tirocinio tenuto in collaborazione con il Dott. Rocco D'Errico, nell'attvità del Master Universitario di 2° Liv. STArch Scienze e tecnologie per i beni culturali a rischio. Disputer Università G. d'Annunzio. Source: Objaverse 1.0 / Sketchfab
Rocca dell' Aquila - Altopiano dell' Argimusco
Source: Objaverse 1.0 / Sketchfab
Santa Maria di Collemaggio (L'Aquila - Italy)
S. Maria di Collemaggio is a large medieval church in L'Aquila, central Italy. It was the site of the original Papal Jubilee, a penitential observation devised by Pope Celestine V, who is buried there. The church, which therefore ranks as a basilica because of its importance in religious history, sits in isolation at the end of a long rectangular sward of grass at the southwest edge of the town. The church is a masterpiece of Abruzzese Romanesque and Gothic architecture and one of the chief sights of L'Aquila. The striking jewel-box effect of the exterior is due to a pattern of blocks of alternating pink and white stone; the interior, on the other hand, is massive and austere. Outbuildings include a colonnaded cloister, with the central fountain typical of many other similar Italian cloisters, and the former monastic refectory. Parts of the structure were significantly damaged in the 2009 earthquake in L'Aquila. coordinates: 42.342890, 13.404106 photogrammetry: 167 photos Source: Objaverse 1.0 / Sketchfab
eHOPS Aquila SED Fits Catalog
The Extension of HOPS Out to 500 ParSecs (eHOPS) project used archival data to survey all the major star forming molecular clouds within 500 pc of the Sun, except Orion (which was surveyed by HOPS). The first eHOPS data release covers the Aquila molecular clouds (d ~ 436 pc). For every source detected in the Herschel/PACS bands, the eHOPS-Aquila catalog contains 1-850 micron SEDs assembled from 2MASS, Spitzer, Herschel, WISE, and JCMT/SCUBA-2 data. A total of 172 protostars are found in Aquila, tightly concentrated in the molecular filaments that thread the clouds. Of these, 72 (42%) are Class 0 protostars, 53 (31%) Class I protostars, 43 (25%) are flat-spectrum protostars, and 4 (2%) are Class II sources. Ten of the Class 0 protostars are young PACS Bright Red Sources similar to those discovered in Orion. eHOPS compares the SEDs to a grid of radiative transfer models to constrain the luminosities, envelope densities, and envelope masses of the protostars.
eHOPS Aquila SED Data Catalog
The Extension of HOPS Out to 500 ParSecs (eHOPS) project used archival data to survey all the major star forming molecular clouds within 500 pc of the Sun, except Orion (which was surveyed by HOPS). The first eHOPS data release covers the Aquila molecular clouds (d ~ 436 pc). For every source detected in the Herschel/PACS bands, the eHOPS-Aquila catalog contains 1-850 micron SEDs assembled from 2MASS, Spitzer, Herschel, WISE, and JCMT/SCUBA-2 data. A total of 172 protostars are found in Aquila, tightly concentrated in the molecular filaments that thread the clouds. Of these, 72 (42%) are Class 0 protostars, 53 (31%) Class I protostars, 43 (25%) are flat-spectrum protostars, and 4 (2%) are Class II sources. Ten of the Class 0 protostars are young PACS Bright Red Sources similar to those discovered in Orion. eHOPS compares the SEDs to a grid of radiative transfer models to constrain the luminosities, envelope densities, and envelope masses of the protostars.
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