Jump to content

Methods of detecting exoplanets: Revision history


For any version listed below, click on its date to view it. For more help, see Help:Page history and Help:Edit summary. (cur) = difference from current version, (prev) = difference from preceding version, m = minor edit, → = section edit, ← = automatic edit summary

(newest | oldest) View (newer 50 | ) (20 | 50 | 100 | 250 | 500)

26 June 2025

23 June 2025

20 June 2025

13 June 2025

12 June 2025

11 June 2025

9 June 2025

4 June 2025

3 June 2025

2 June 2025

29 April 2025

31 March 2025

3 March 2025

16 December 2024

9 December 2024

8 December 2024

30 November 2024

25 November 2024

23 November 2024

  • curprev 04:1404:14, 23 November 2024 Citation bot talk contribs 139,922 bytes +315 Alter: title, date, template type. Add: doi, pages, issue, volume, journal, doi-access, bibcode, arxiv, authors 1-1. Removed URL that duplicated identifier. Removed parameters. Some additions/deletions were parameter name changes. | Use this bot. Report bugs. | Suggested by Jay8g | #UCB_toolbar undo
  • curprev 04:0504:05, 23 November 2024 Hd163296 talk contribs 139,607 bytes +1,039 Fixed a couple of misconceptions in the previous description, like the fact that the previous description only mentioned gaps and not the fact that disk kinematics is based on detecting velocity perturbations in the gas of protoplanetary disks. Also, added 2 references to the original theoretical papers proposing the method. undo Tag: Visual edit

5 November 2024

17 October 2024

11 October 2024

22 September 2024

20 September 2024

30 August 2024

26 August 2024

22 August 2024

17 August 2024

30 July 2024

18 July 2024

(newest | oldest) View (newer 50 | ) (20 | 50 | 100 | 250 | 500)