Revision history of "Ew(Hα) of one star forming galaxy in LAMOST survey"

View logs for this page

Jump to navigation Jump to search

Diff selection: Mark the radio boxes of the revisions to compare and hit enter or the button at the bottom.
Legend: (cur) = difference with latest revision, (prev) = difference with preceding revision, m = minor edit.

curprev 01:48, 25 December 2013‎ Cluster talk contribs‎ 2,462 bytes −4‎ →‎SDSS image
curprev 01:47, 25 December 2013‎ Cluster talk contribs‎ 2,466 bytes +693‎
curprev 07:44, 24 December 2013‎ Cluster talk contribs‎ 1,773 bytes +6‎
curprev 07:43, 24 December 2013‎ Cluster talk contribs‎ 1,767 bytes +4‎
curprev 07:42, 24 December 2013‎ Cluster talk contribs‎ 1,763 bytes +274‎
curprev 07:18, 24 December 2013‎ Cluster talk contribs‎ 1,489 bytes +43‎
curprev 07:11, 24 December 2013‎ Cluster talk contribs‎ 1,446 bytes 0‎ →‎Exercise: measure the Ew(Hα) of one SFing galaxy in the Lamost survey
curprev 07:11, 24 December 2013‎ Cluster talk contribs‎ 1,446 bytes +6‎
curprev 07:08, 24 December 2013‎ Cluster talk contribs‎ 1,440 bytes +8‎
curprev 02:44, 24 December 2013‎ Cluster talk contribs‎ 1,432 bytes +100‎
curprev 02:23, 24 December 2013‎ Cluster talk contribs‎ 1,332 bytes +16‎ →‎Exercise: measure the Ew(Hα) of one SFing galaxy in the Lamost survey
curprev 02:15, 24 December 2013‎ Cluster talk contribs‎ 1,316 bytes +1,316‎ 以“=== Equivalent Width : EW(Hα) === Recall EW(Hα) measures the relative strength of Hα to the continuum under the line It therefore acts like a long baseline color...”为内容创建页面

Retrieved from "http://cluster.shao.ac.cn/wiki/index.php?title=Ew(Hα)_of_one_star_forming_galaxy_in_LAMOST_survey"