Details on Acronym: WMH | |
| WMH | (Willott+McLure+Hibon+, 2013) |
| ***** | Avoid the usage of WMH, prefer [WMH2013] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [WMH2013] | |
| [WMH2013] | (Willott+McLure+Hibon+, 2013)= (WMH) |
| Write: | <<[WMH2013] NN>> <<[WMH2013] Serendip>> |
| N: | 40+1 |
| Object: | Poss. LBG (SIMBAD class: Galaxy) |
| Stat: | is completely incorporated in Simbad |
| Note: | N=40 z∼6 LBG candidates in CFHTLS data. Gemini GMOS spectroscopy for 7 of the candidates. |
| Ref: | =2013AJ....145....4W |
| by | WILLOTT C.J. , McLURE R.J., HIBON P., BIELBY R., McCRACKEN H.J., KNEIB J.-P., ILBERT O., BONFIELD D.G., BRUCE V.A., JARVIS M.J. |
| Astron. J., 145, 4 (2013) | |
| An exponential decline at the bright end of the z = 6 galaxy luminosity function. | |
| o | Fig. 1, Table 1: <[WMH2013] NN> (Nos 1-40). Fig 3, Table 2: <[WMH2013] Serendip> N=1. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |