The mass function of IC 4665 revisited by the UKIDSS Galactic Clusters Survey

N. Lodieu; W.-J. de Wit; G. Carraro; E. Moraux; J. Bouvier; N. C. Hambly

doi:10.1051/0004-6361/201116883

Home

All issues

Volume 532 (August 2011)

A&A, 532 (2011) A103

Full HTML

Free Access

Table 1

Log of the observations.

Tile^a	RA^b	dec^b	Date

1	17^h44^m	+06°02′	2006-05-10
2	17^h44^m	+05°10′	2006-05-10
3	17^h45^m	+06°55′	2006-05-11
4	17^h47^m	+06°02′	2006-05-10
5	17^h47^m	+05°10′	2006-05-10
6	17^h49^m	+06°56′	2006-05-11
7	17^h51^m	+06°02′	2006-05-11
8	17^h51^m	+05°10′	2006-05-10

Notes.

^(a)

Each WFCAM tile is 54 by 54 arcmin aside and was observed in all five passbands (ZYJHK). Average seeing measured on the images and in each individual filter ranged from 0.75 to 1.0 arcsec.

^(b)

Central coordinates (in J2000) of each tile from UKIDSS GCS DR8.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.