MediaWiki API 结果
这是JSON格式的HTML实现。HTML对调试很有用，但不适合应用程序使用。
指定format参数以更改输出格式。要查看JSON格式的非HTML实现，设置format=json。
{
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"logid": 2741,
"ns": 0,
"title": "Compact group",
"pageid": 703,
"logpage": 703,
"params": {},
"type": "create",
"action": "create",
"user": "Shen",
"timestamp": "2025-03-19T03:14:00Z",
"comment": "\u521b\u5efa\u9875\u9762\uff0c\u5185\u5bb9\u4e3a\u201c*arXiv:2503.13761 \u534a\u89e3\u6790\u6a21\u578b\u4e2d\u7684CG\u201d"
},
{
"logid": 2740,
"ns": 0,
"title": "Ring galaxy",
"pageid": 702,
"logpage": 702,
"params": {},
"type": "create",
"action": "create",
"user": "Shen",
"timestamp": "2025-02-17T07:49:21Z",
"comment": "\u521b\u5efa\u9875\u9762\uff0c\u5185\u5bb9\u4e3a\u201c* LEDA 1313424 (\u201cBullseye\u201d)\uff1a Collisional Ring Galaxies\uff1awith nine readily-identified rings \u2014\u201d"
},
{
"logid": 2739,
"ns": 0,
"title": "Filament",
"pageid": 701,
"logpage": 701,
"params": {},
"type": "create",
"action": "create",
"user": "Shen",
"timestamp": "2025-01-21T09:05:40Z",
"comment": "\u521b\u5efa\u9875\u9762\uff0c\u5185\u5bb9\u4e3a\u201c*Filfinder [https://fil-finder.readthedocs.io/en/latest/index.html]\u201d"
},
{
"logid": 2738,
"ns": 0,
"title": "EMU",
"pageid": 700,
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"params": {},
"type": "create",
"action": "create",
"user": "Shen",
"timestamp": "2024-11-28T06:45:18Z",
"comment": "\u521b\u5efa\u9875\u9762\uff0c\u5185\u5bb9\u4e3a\u201cPilot Survey of the Evolutionary Map of the Universe (EMU), observed at 944 MHz with the Australian Square Kilometre Array Pathnder (ASKAP) telescope. The survey covers 270 deg2of an area covered by the Dark Energy Survey, reaching a depth of 2530 \u00b5Jy/beam rms at a spatial resolution of \u223c 1118 arcsec,\u201d"
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{
"logid": 2737,
"ns": 0,
"title": "\u6df1\u5ea6\u5b66\u4e60",
"pageid": 699,
"logpage": 699,
"params": {},
"type": "create",
"action": "create",
"user": "Shen",
"timestamp": "2024-11-03T13:29:34Z",
"comment": "\u521b\u5efa\u9875\u9762\uff0c\u5185\u5bb9\u4e3a\u201c==\u53d8\u5206\u81ea\u7f16\u7801\u5668VAE== *\u91c7\u7528flow match\u7684\u65b9\u6cd5\u6765\u9884\u8a00\u661f\u7cfb\u4e2dex situ\u7684\u6bd4\u4f8b\uff08\u56fe\u751f\u56fe\uff09\u201d"
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{
"logid": 2736,
"ns": 0,
"title": "XUV disk",
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"params": {},
"type": "create",
"action": "create",
"user": "Shen",
"timestamp": "2024-10-20T06:46:00Z",
"comment": "\u521b\u5efa\u9875\u9762\uff0c\u5185\u5bb9\u4e3a\u201c* extended ultraviolet (XUV) disks beyond the optical disk of galaxies * arXiv:2312.06031 * \u5e74\u8f7b\u6052\u661f\u201d"
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{
"logid": 2735,
"ns": 0,
"title": "Bar",
"pageid": 697,
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"params": {},
"type": "create",
"action": "create",
"user": "Shen",
"timestamp": "2024-09-23T14:17:07Z",
"comment": "\u521b\u5efa\u9875\u9762\uff0c\u5185\u5bb9\u4e3a\u201c*\u63cf\u8ff0\u68d2\u661f\u7cfb\u7684\u4e09\u4e2a\u53c2\u6570\uff0c\u957f\u5ea6\uff0c\u5f3a\u5ea6\uff0c\u548cpattern speed [https://arxiv.org/pdf/1501.05498] ==strength== The bar strength is a parameter that measures the non-axisymmetric forces produced by the bar potential in the disc of galaxies (see, e.g., Laurikainen & Salo, 2002). * measure the torques of the bar (e.g., Combes & Sanders , 1981; Quillen et al. , 1994; Buta & Block , 2001; Laurikainen et al. , 2007; Salo et al. , 2010) * bar ellipticity Martin\u2026\u201d"
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"title": "\u77e9\u9635",
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"logpage": 696,
"params": {},
"type": "create",
"action": "create",
"user": "Shen",
"timestamp": "2024-09-22T11:30:18Z",
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{
"logid": 2733,
"ns": 0,
"title": "\u9ad8\u65af\u6df7\u5408\u6a21\u578b",
"pageid": 695,
"logpage": 695,
"params": {},
"type": "create",
"action": "create",
"user": "Shen",
"timestamp": "2024-09-22T09:31:51Z",
"comment": "\u521b\u5efa\u9875\u9762\uff0c\u5185\u5bb9\u4e3a\u201c* Gaussian Mixture Model [https://www.astroml.org/book_figures/chapter4/fig_GMM_1D.html]\u201d"
},
{
"logid": 2732,
"ns": 0,
"title": "\u661f\u56e2",
"pageid": 694,
"logpage": 694,
"params": {},
"type": "create",
"action": "create",
"user": "Shen",
"timestamp": "2024-09-10T13:51:43Z",
"comment": "\u521b\u5efa\u9875\u9762\uff0c\u5185\u5bb9\u4e3a\u201c**SPISEA: A Python-based Simple Stellar Population Synthesis Code for Star Clusters [https://iopscience.iop.org/article/10.3847/1538-3881/aba533?msclkid=eb4df8cac15a11ecbebd4b509b9bb140]\u201d"
}
]
}
}