Details on Acronym: DANCe | |
DANCe | (Dynamical Analysis of Nearby Clusters) |
Write: | <<DANCe JHHMMSSss+DDMMSSs>> |
N: | about 30.106 |
Object: | ? (SIMBAD class: Unknown = Object of Unknown Nature) |
Note: | The DANCe surveys measured proper motions by combining archival and new wide field images. The main scientific goal of the survey focuses on nearby associations and clusters, but the catalogs include the astrometry, multi-wavelength (optical and near-infrared) photometry for millions of sources in the field of view. The survey encompasses areas of typically 5 to 100 square degrees around each cluster, and reaches optical magnitudes of the order of 24mag. The accuracy on the proper motion reaches 0.3mas/yr in the best cases, depending on the observational history. Website: http://project-dance.com |
in source: | NAME Pleiades |
in source: | NGC 2168 = M 35 |
in source: | NAME VI CYG = Ass Cyg OB 2 |
Ref: | =2015A&A...575A.120B |
by | BOUY H. , BERTIN E., BARRADO D., SARRO L.M., OLIVARES J., MORAUX E., BOUVIER J., CUILLANDRE J.-C., RIBAS A., BELETSKY Y. |
Astron. Astrophys., 575A, 120-120 (2015) | |
Messier 35 (NGC 2168) DANCe. I. Membership, proper motions, and multiwavelength photometry. | |
o | Table 3: <DANCe JHHMMSSss+DDMMSSs> N=337522. |
Ref: | =2015A&A...577A.148B |
by | BOUY H. , BERTIN E., SARRO L.M., BARRADO D., MORAUX E., BOUVIER J., CUILLANDRE J.-C., BERIHUETE A., OLIVARES J., BELETSKY Y. |
Astron. Astrophys., 577A, 148-148 (2015) | |
The Seven Sisters DANCe. I. Empirical isochrones, luminosity, and mass functions of the Pleiades cluster. | |
o | <DANCe JHHMMSSss+DDMMSSs> N=1969890. |
Ref: | =2016MNRAS.460.2593W |
by | WRIGHT N.J. , BOUY H., DREW J.E., SARRO L.M., BERTIN E., CUILLANDRE J.-C., BARRADO D. |
Mon. Not. R. Astron. Soc., 460, 2593-2610 (2016) | |
Cygnus OB2 DANCe: A high-precision proper motion study of the Cygnus OB2 association. | |
o | Table 2: <DANCe JHHMMSSss+DDMMSSs> N=873. CAB CSIC |
Origin | of the Acronym: p = Pre-registered to IAU Comm.5 |
Details on Acronym: DANCe | |
DANCe | (Dynamical Analysis of Nearby Clusters) |
***** | Avoid the usage of DANCe, prefer [SBB2014] |
Origin | of the Acronym: A = Assigned by the author(s) |