Details on Acronym: SDSS | |
SDSS | (Sloan Digital Sky Survey) |
***** | Avoid the usage of SDSS, prefer [YNG2003] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [YNG2003] | |
[YNG2003] | (Yanny+Newberg+Grebel+, 2003)= (SDSS) |
Write: | <<[YNG2003] NNNN-N-N-NNN-NNNN>> <<[YNG2003] SpLLL+BB-NN.N>> |
N: | 392+4 |
Object: | * + Region (SIMBAD class: Star) |
Stat. | in SIMBAD: Table 1 is completely incorporated. |
Note: | Sloan Digital Sky Survey (SDSS) observations. Study of large structures with concentration of stars in the Milky Way N=4 'Sp' regions. N=392 blue stars in these regions, with a SDSS format: 'Run-Rerun-Camcol-Field-ID'. See paper II: [NYR2002]. |
Ref: | =2003ApJ...588..824Y |
by | YANNY B. , NEWBERG H.J., GREBEL E.K., KENT S., ODENKIRCHEN M., ROCKOSI C.M., SCHLEGEL D., SUBBARAO M., BRINKMANN J., FUKUGITA M., IVEZIC Z., LAMB D.Q., SCHNEIDER D.P., YORK D.G. |
Astrophys. J., 588, 824-841 (2003) | |
A low-latitude halo stream around the Milky Way. | |
o | (Erratum) erratum vol. 605, p. 575 (2004) |
o | Table 1: <[YNG2003] NNNN-N-N-NNN-NNNN> N=392. Table 2: <[YNG2003] SpLLL+BB-NN.N> N=4. |
=E= | Catalogue in electronic form as J/ApJ/588/824 |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |