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The dataset likely contains user authentication details such as emails and passwords, as indicated by the presence of login prompts for SARAO, including options to reset passwords and instructions for new users to register using their Gmail accounts. This suggests the dataset may be used for managing user access or analyzing login patterns. The purpose appears to facilitate user registration and authentication processes, ensuring secure access to the SARao platform while providing flexibility through integration with external services like Gmail.

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相关论文

5

A persistent bow shock in a diskless magnetized accreting white dwarf

Krystian IłkiewiczSimone ScaringiDomitilla de MartinoChristian KniggeSara E. Motta12
Nature Astronomy
2026
2026/1/12
Vol.10 No.3 p.391-400
Stellar bow shocks form when an outflow interacts with the interstellar medium. In white dwarfs accreting from a binary companion, outflows are associated with strong winds from the donor star, the accretion disk or a thermonuclear runaway explosion on the white dwarf surface. To date, only six accr...
Astrophysical disksAstrophysical magnetic fieldsCompact astrophysical objects
10.1038/S41550-025-02748-8
ISSN:2397-3366

Periodic radio and X-ray emission from an accreting white dwarf binary

Kovi RoseJoshua PritchardTara MurphyL. N. DriessenD. L. Kaplan29
Nature Astronomy
2026
2026/6/1
00 p.1-13
Long-period radio transients (LPTs) are coherent bursts of polarized radio emission that repeat periodically on timescales of minutes to hours. Little is known about the physical origins of these systems. Astronomers have proposed magnetars that rotate slowly and white dwarfs that rapidly orbit with...
Compact astrophysical objectsStarsStellar evolutionTransient astrophysical phenomena
10.1038/S41550-026-02882-X
ISSN:2397-3366

Jets from MRC 0600-399 bent by magnetic fields in the cluster Abell 3376

James O. ChibuezeHaruka SakemiTakumi OhmuraMami MachidaHiroki Akamatsu10
Nature
2021
2021/5/5
Vol.593 No.7857 p.47-50
Galaxy clusters are known to harbour magnetic fields, the nature of which remains unresolved. Intra-cluster magnetic fields can be observed at the density contact discontinuity formed by cool and dense plasma running into hot ambient plasma1,2, and the discontinuity exists3 near the second-brightest...
Astrophysical magnetic fieldsGalaxies and clusters
10.1038/S41586-021-03434-1
ISSN:0028-0836

The emission of interpulses by a 6.45-h-period coherent radio transient

Y. W. J. LeeM. CalebTara MurphyE. LencD. L. Kaplan32
Nature Astronomy
2025
2025/1/15
00 p.1-13
Long-period radio transients are a new class of astronomical objects characterized by prolonged periods ranging from 18 min to 54 min. They exhibit highly polarized, coherent, beamed radio emission lasting only 10–100 s. The intrinsic nature of these objects is subject to speculation, with highly ma...
Compact astrophysical objectsTime-domain astronomyTransient astrophysical phenomena
10.1038/S41550-024-02452-Z
ISSN:2397-3366

Detection of X-ray emission from a bright long-period radio transient

Ziteng WangNanda ReaTong BaoDavid L. KaplanEmil Lenc49
Nature
2025
2025/5/28
00 p.1-4
Recently, a class of long-period radio transients (LPTs) has been discovered, exhibiting emission thousands of times longer than radio pulsars1–5. These findings, enabled by advances in wide-field radio surveys, challenge existing models of rotationally powered pulsars. Proposed models include highl...
Compact astrophysical objectsTime-domain astronomyTransient astrophysical phenomena
10.1038/S41586-025-09077-W
ISSN:0028-0836