![](/images/gifchars/gamma.gif)
-L
nL
n'S
3 (L
n = La, Ce; L
n' = Er, Tm, Yb) have bee
n prepared as dark red to black si
ngle crystalsby the reactio
n of the respective la
ntha
nides with sulfur i
n a Sb
2S
3 flux at 1000
![](/images/e<font color=)
ntities/deg.gif">C. This isotypic seriesof compou
nds adopts a layered structure that co
nsists of the smaller la
ntha
nides (Er, Tm, a
nd Yb) bou
ndby sulfide i
n six- a
nd seve
n-coordi
nate e
nviro
nme
nts that are co
nnected together by the larger la
ntha
nides(La a
nd Ce) i
n eight- a
nd
ni
ne-coordi
nate e
nviro
nme
nts. The layers ca
n be broke
n dow
n i
nto three disti
ncto
ne-dime
nsio
nal substructures co
ntai
ni
ng three crystallographically u
nique L
n' ce
nters. The first of theseis co
nstructed from o
ne-dime
nsio
nal chai
ns of edge-shari
ng [L
n'S
7] mo
nocapped trigo
nal prisms that arejoi
ned to equivale
nt chai
ns via edge shari
ng to yield ribbo
ns. There are parallel chai
ns of [L
n'S
6] distortedoctahedra that are li
nked to the first ribbo
ns through cor
ner shari
ng. These latter u
nits also share cor
nerswith a o
ne-dime
nsio
nal ribbo
n composed of parallel chai
ns of [L
n'S
6] polyhedra that edge-share both i
nthe directio
n of chai
n propagatio
n a
nd with adjace
nt ide
ntical chai
ns. Mag
netic susceptibility measureme
ntsshow Curie-
Weiss behavior from 2 to 300 K with a
ntiferromag
netic coupli
ng a
nd
no evide
nce formag
netic orderi
ng. The
p values ra
nge from -0.4 to -37.5 K, a
nd spi
n-frustratio
n may be i
ndicated forthe Yb-co
ntai
ni
ng compou
nds. All compou
nds show mag
netic mome
nts substa
ntially reduced from thosecalculated for the free io
ns. The optical ba
nd gaps for
![](/images/gifchars/gamma.gif)
-LaL
n'S
3 (L
n' = Er, Tm, Yb) are approximately1.6 eV, whereas
![](/images/gifchars/gamma.gif)
-CeL
n'S
3 (L
n' = Er, Tm, Yb) are approximately 1.3 eV.