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资源简介：
cosmological model:nrunlcdm, dataset:bicep_keck_2018
应用场景：
创建时间：
2025-02-10
相关数据集
Parkes observations for project P1229 semester 2023OCTS_01
We propose a pulsar timing campaign of three millisecond pulsars discovered in previous pulsar searches of Fermi gamma-ray sources. Despite an original follow-up effort, it was not possible to produce
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Parkes observations for project P1229 semester 2023OCTS_08
We propose a pulsar timing campaign of three millisecond pulsars discovered in previous pulsar searches of Fermi gamma-ray sources. Despite an original follow-up effort, it was not possible to produce
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Parkes observations for project P895 semester 2019APRS_02
Since the year 2005, the Parkes Pulsar Timing Array (PPTA) project has been placing ever more stringent constraints on the amplitude of a gravitational wave background signal. Such upper bounds on the
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Parkes observations for project P456 semester 2010OCTS
The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of o
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Parkes observations for project P456 semester 2022OCTS_10
The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of o
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