inorganic papers
Acta Cryst.(2006). E62, i83–i85 doi:10.1107/S1600536806007446 Salloumet al. Ho
0.76In1.68Mo15Se19
i83
Acta Crystallographica Section E
Structure Reports
Online
ISSN 1600-5368
Ho
0.76In
1.68Mo
15Se
19D. Salloum, P. Gougeon* and M. Potel
Laboratoire de Chimie du Solide et Inorganique Mole´culaire, URA CNRS No. 6511, Universite´ de Rennes I, Avenue du Ge´ne´ral Leclerc, 35042 Rennes Cedex, France
Correspondence e-mail: [email protected]
Key indicators
Single-crystal X-ray study
T= 293 K
Mean(Mo–Se) = 0.007 A˚ Disorder in main residue
Rfactor = 0.040
wRfactor = 0.088
Data-to-parameter ratio = 36.9
For details of how these key indicators were automatically derived from the article, see http://journals.iucr.org/e.
Received 14 February 2006 Accepted 1 March 2006
#2006 International Union of Crystallography All rights reserved
The structure of holmium indium molybdenum selenide, Ho0.76In1.68Mo15Se19, isotypic with In2.9Mo15Se19 [Gru¨ttner,
Yvon, Chevrel, Potel, Sergent & Seeber (1979). Acta Cryst.
B35, 285–292], is characterized by two cluster units Mo6Se
i
8Se
a
6
and Mo9Se
i
11Se
a
6 (where i = inner and a = apical) that are
present in a 1:1 ratio. The cluster units are centered at Wyckoff
positions 2band 2cand have point-group symmetry 3 and 6,
respectively. The clusters are interconnected through
addi-tional Mo—Se bonds. In the title compound, Ho3+ cations
replace the trivalent indium observed in In2.9Mo15Se19, and a
deficiency is observed on the monovalent indium site.
Comment
In 1979, Gru¨ttner et al. reported the crystal structures of
In2.9Mo15Se19 and In3.3Mo15Se19 as the first compounds
containing a transition metal cluster with a nuclearity higher
than 6, viz. the bioctahedral Mo9 cluster. The latter cluster,
which results from the face-sharing of two Mo6 octahedra,
coexists with the octahedral Mo6cluster in equal proportions.
Another interesting feature in these compounds concerns the In atoms that occupy two crystallographically different posi-tions depending on their formal oxidation state of +I or +III,
[image:1.610.208.457.455.724.2]respectively. While the InIsite is fully occupied, the InIIIsite
Figure 1
presents a non-stoichiometry that leads to broad composition ranges from In2.9Mo15Se19 to In3.3Mo15Se19. We present here
the crystal structure of Ho0.76In1.68Mo15Se19 in which Ho
replaces the trivalent In site.
The Mo–Se framework of the title compound consists of the
cluster units Mo6Se
i
8Se
a
6and Mo9Se
i
11Se
a
6in a 1:1 ratio. These
units are interconnected through additional Mo—Se bonds
(Figs. 1 and 2); for details of thei- anda-type ligand notation,
see Scha¨fer & von Schnering (1964). The first unit can be
described as an Mo6 octahedron surrounded by eight
face-capping inner Seiand six apical Sealigands. The Mo9cluster is
surrounded by 11 Seiatoms capping the faces of the
biocta-hedron and six Sea ligands above the apical Mo atoms. The
Mo6Sei8Sea6 and Mo9Se11iSea6 units are centered at Wyckoff
positions 2band 2cand have point-group symmetry 3 and 6,
respectively. The Mo—Mo distances within the Mo6 cluster
are 2.7001 (7) A˚ for the distances of the Mo3triangles formed
by the Mo atoms related through the threefold axis, and
2.7104 (8) A˚ for the distances between these triangles. The
Mo—Mo distances within the Mo9clusters are 2.6470 (7) and
2.719 (1) A˚ for the intra-triangle distances between atoms
Mo2 and Mo3, respectively, and 2.7179 (5) and 2.7673 (6) A˚
for those between the Mo3 triangles. The Se atoms bridge
either one (Se1, Se2, Se4 and Se5) or two (Se3) triangular faces of the Mo clusters. Moreover, atoms Se1 and Se2 are linked to an Mo atom of a neighboring cluster. The Mo—Se
bond distances range from 2.5469 (9) to 2.6587 (7) A˚ within
the Mo6Se8iSea6unit, and from 2.5290 (8) to 2.6928 (6) A˚ within
the Mo9Se11i Sea6 unit. Each Mo9Se11iSea6 cluster is
inter-connected to six Mo6Se
i
8Se
a
6units (andvice versa)viaMo2—S1
bonds (and Mo1—S2 bonds, respectively), forming the three-dimensional Mo—S framework, the connective formula of
which is Mo9S
i
5S
i-a 6/2S
a-i
6/2, Mo6S
i
2S
i-a 6/2S
a-i
6/2. It results from this
arrangement that the shortest intercluster Mo1—Mo2
distance is 3.4666 (6) A˚ , indicating only weak metal–metal
interaction. The In+cations are surrounded by seven Se atoms
forming a distorted tricapped tetrahedron, as is the case in
In2.9Mo15Se19. The Se5 and Se2 atoms forming the tetrahedron
are at 3.0647 (15) and 3.1591 (5) A˚ from the In atom, and the
capping Se1 atoms are at 3.5079 (7) A˚ . While in In2.9Mo15Se19
the latter site is fully occupied by monovalent In, in the title compound it is only 0.842 (3) occupied. This probably results from the higher temperature used during the crystal-growth process which led to a loss of InSe because of its high volatility
at 1773 K. The Ho3+ cations, as the In3+ cations in the
In3xMo15Se19 compounds, occupy partially [25.5 (2)%]
occupied distorted octahedral cavities around the threefold
axis, which are formed by two Mo6Se
i
8Se
a
6 and three
Mo9Se
i
11Se
a
6 units. The Ho—Se distances are in the range
2.5689 (13)–2.9690 (16) A˚ .
Experimental
Single crystals of Ho0.76In1.68Mo15Se19were prepared from a mixture of Ho2Se3, MoSe2, InSe and Mo with the nominal composition HoIn2Mo15Se19. Before use, Mo powder was reduced under flowing H2gas at 1273 K over a period 10 h in order to eliminate any trace of oxygen. The binaries Ho2Se3, MoSe2, InSe were obtained by heating stoichiometric mixtures of the elements in sealed evacuated silica tubes over a period of about 2 d. All handling of materials was carried out in an argon-filled glove-box. The initial mixture (ca5 g) was cold-pressed and loaded into a molybdenum crucible, which was sealed under a low argon pressure using an arc-welding system. The charge was heated at a rate of 300 K h1up to 1773 K, the temperature which was held there for 48 h, then cooled at a rate of 100 K h1to 1373 K and finally allowed to cool in the switched-off furnace. On the basis of the X-ray powder diagram, the product was a single phase.
Crystal data
Ho0.76In1.68Mo15Se19 Mr= 3258.98
Hexagonal,P63=m a= 9.7969 (1) A˚
c= 19.3973 (4) A˚
V= 1612.31 (4) A˚3 Z= 2
Dx= 6.713 Mg m3
MoKradiation
Cell parameters from 31521 reflections
= 2.0–35.0
= 30.08 mm1
T= 293 (2) K Irregular block, black 0.080.050.03 mm
Data collection
Nonius KappaCCD diffractometer ’and!scans
Absorption correction: analytical (de Meulenaer & Tompa, 1965)
Tmin= 0.094,Tmax= 0.345
28264 measured reflections 2436 independent reflections
1625 reflections withI> 2(I)
Rint= 0.092
max= 35.1 h=11!15
k=15!15
l=31!31
Refinement
Refinement onF2 R[F2> 2(F2)] = 0.040
wR(F2) = 0.088 S= 1.07 2436 reflections 66 parameters
w= 1/[2(F
o2) + (0.0398P)2
+ 0.2653P]
whereP= (Fo2+ 2Fc2)/3
(/)max= 0.001
max= 2.64 e A˚3
min=2.69 e A˚3
inorganic papers
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Salloumet al. Ho [image:2.610.48.294.70.314.2]0.76In1.68Mo15Se19 Acta Cryst.(2006). E62, i83–i85
Figure 2
Plot showing the atom-numbering scheme and the inter-unit linkage of the Mo9Se11Se6and Mo6Se8Se6cluster units. Displacement ellipsoids are
Table 1
Selected bond lengths (A˚ ).
Mo1—Se4 2.5469 (9)
Mo1—Se1i
2.5526 (7)
Mo1—Se1 2.5765 (7)
Mo1—Se1ii
2.6163 (6)
Mo1—Se2 2.6587 (7)
Mo1—Mo1iii 2.7001 (7)
Mo1—Mo1iv
2.7104 (8)
Mo2—Se5 2.5290 (8)
Mo2—Se2 2.5862 (6)
Mo2—Se2v
2.6275 (7)
Mo2—Mo2v
2.6470 (7) Mo2—Se1vi
2.6675 (7)
Mo2—Se3v 2.6928 (6)
Mo2—Mo3v
2.7179 (5)
Mo2—Mo3 2.7673 (5)
Mo3—Se3v
2.5836 (9)
Mo3—Se2 2.5851 (6)
Mo3—Se2vii
2.5851 (6)
Mo3—Se3 2.5908 (9)
Mo3—Mo3viii 2.7193 (10)
In—Se5 3.0647 (15)
In—Se2ix
3.1591 (5) In—Se1ix
3.5079 (7) Ho—Se4vii
2.5689 (13) Ho—Se3ii
2.7270 (16) Ho—Se2iii
2.8314 (11)
Ho—Se2x 2.8314 (11)
Ho—Se3iii
2.9690 (16)
Symmetry codes: (i) xy;x;zþ1; (ii) y;xy;z; (iii) xþy;x;z; (iv)
y;xþy;zþ1; (v)yþ1;xy;z; (vi)xþyþ1;x;z; (vii)x;y;zþ3 2; (viii)
xþyþ1;xþ1;z; (ix)xþ1;y;zþ1; (x)xþy;x;zþ3 2.
The occupation factors for the Ho and In atoms were refined freely. The highest peak and the deepest hole in the final Fourier map are located 0.20 A˚ from In and 0.64 A˚ from Se4, respectively.
Data collection: COLLECT (Nonius, 1998); cell refinement:
COLLECT; data reduction: EVALCCD (Duisenberg et al., 2003);
program(s) used to solve structure: SIR97 (Altomare et al., 1999; program(s) used to refine structure:SHELXL97(Sheldrick, 1997); molecular graphics:DIAMOND(Brandenburg, 2001); software used to prepare material for publication:SHELXL97.
Intensity data were collected on the Nonius KappaCCD X-ray diffactometer system of the Centre de diffractome´trie de l’Universite´ de Rennes I (URL: www.cdifx.univ-rennes1. fr).
References
Altomare, A., Burla, M. C., Camalli, M., Cascarano, G., Giacovazzo, C., Guagliardi, A., Moliterni, A. G. G., Polidori, G. & Spagna, R. (1999).J. Appl. Cryst.32, 115–119.
Brandenburg, K. (2001). DIAMOND. Version. 2.1e. Crystal Impact GbR, Bonn, Germany.
Duisenberg, A. J. M., Kroon-Batenburg, L. M. J. & Schreurs, A. M. M. (2003).
J. Appl. Cryst.36, 220–229.
Gru¨ttner, A., Yvon, K., Chevrel R., Potel, M., Sergent, M. & Seeber, B. (1979).
Acta Cryst.B35, 285–292.
Meulenaer, J. de & Tompa, H. (1965).Acta Cryst.19, 1014–1018. Nonius (1998).COLLECT. Nonius BV, Delft, The Netherlands. Scha¨fer, H. & von Schnering, H. G. (1964).Angew. Chem.76, 833–845. Sheldrick, G. M. (1997).SHELXL97. University of Go¨ttingen, Germany.
inorganic papers
Acta Cryst.(2006). E62, i83–i85 Salloumet al. Ho
supporting information
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Acta Cryst. (2006). E62, i83–i85
supporting information
Acta Cryst. (2006). E62, i83–i85 [https://doi.org/10.1107/S1600536806007446]
Ho
0.76In
1.68Mo
15Se
19D. Salloum, P. Gougeon and M. Potel
holmium indium molybdenum selenide
Crystal data Ho0.76In1.68Mo15Se19
Mr = 3258.98 Hexagonal, P63/m
Hall symbol: -P 6c a = 9.7969 (1) Å c = 19.3973 (4) Å V = 1612.31 (4) Å3
Z = 2
F(000) = 2820
Dx = 6.713 Mg m−3
Mo Kα radiation, λ = 0.71069 Å Cell parameters from 31521 reflections θ = 2.0–35.0°
µ = 30.08 mm−1
T = 293 K
Irregular block, black 0.08 × 0.05 × 0.03 mm
Data collection Nonius Kappa CCD
diffractometer
Radiation source: fine-focus sealed tube Horizontally mounted graphite crystal
monochromator
Detector resolution: 9 pixels mm-1
φ and ω scans
Absorption correction: analytical (de Meulenaar & Tompa, 1965)
Tmin = 0.094, Tmax = 0.345
28264 measured reflections 2436 independent reflections 1625 reflections with I > 2σ(I) Rint = 0.092
θmax = 35.1°, θmin = 3.2°
h = −11→15 k = −15→15 l = −31→31
Refinement Refinement on F2
Least-squares matrix: full R[F2 > 2σ(F2)] = 0.040
wR(F2) = 0.088
S = 1.07 2436 reflections 66 parameters 0 restraints
Primary atom site location: structure-invariant direct methods
Secondary atom site location: difference Fourier map
w = 1/[σ2(F
o2) + (0.0398P)2 + 0.2653P]
where P = (Fo2 + 2Fc2)/3
(Δ/σ)max = 0.001
Δρmax = 2.64 e Å−3
Δρmin = −2.69 e Å−3
Special details
Geometry. All e.s.d.'s (except the e.s.d. in the dihedral angle between two l.s. planes) are estimated using the full
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Acta Cryst. (2006). E62, i83–i85
Refinement. Refinement of F2 against ALL reflections. The weighted R-factor wR and goodness of fit S are based on F2,
conventional R-factors R are based on F, with F set to zero for negative F2. The threshold expression of F2 > σ(F2) is used
only for calculating R-factors(gt) etc. and is not relevant to the choice of reflections for refinement. R-factors based on F2
are statistically about twice as large as those based on F, and R- factors based on ALL data will be even larger.
Fractional atomic coordinates and isotropic or equivalent isotropic displacement parameters (Å2)
x y z Uiso*/Ueq Occ. (<1)
Mo1 0.16651 (5) 0.01597 (5) 0.55715 (2) 0.00634 (10) Mo2 0.68338 (5) 0.18637 (5) 0.63335 (2) 0.00570 (10) Mo3 0.51229 (7) 0.16779 (7) 0.7500 0.00581 (12) Se1 0.03516 (6) −0.28658 (6) 0.55165 (3) 0.00840 (11) Se2 0.38029 (6) 0.00931 (6) 0.63934 (3) 0.00904 (12) Se3 0.35216 (8) 0.31290 (9) 0.7500 0.00907 (15) Se4 0.0000 0.0000 0.66099 (5) 0.0201 (2) Se5 0.6667 0.3333 0.52947 (5) 0.00926 (18)
In 0.6667 0.3333 0.37147 (6) 0.0356 (4) 0.842 (3) Ho −0.20999 (18) −0.17299 (16) 0.7500 0.0135 (4) 0.2553 (16)
Atomic displacement parameters (Å2)
U11 U22 U33 U12 U13 U23
Mo1 0.0079 (2) 0.00649 (19) 0.0046 (2) 0.00365 (16) 0.00012 (15) 0.00014 (14) Mo2 0.00623 (19) 0.00645 (19) 0.00453 (19) 0.00325 (16) −0.00007 (15) −0.00021 (14) Mo3 0.0071 (3) 0.0067 (3) 0.0044 (2) 0.0040 (2) 0.000 0.000
Se1 0.0092 (2) 0.0081 (2) 0.0082 (2) 0.0046 (2) 0.00081 (18) 0.00175 (18) Se2 0.0073 (2) 0.0080 (2) 0.0107 (3) 0.00297 (19) −0.00287 (18) −0.00156 (18) Se3 0.0070 (3) 0.0119 (4) 0.0094 (3) 0.0055 (3) 0.000 0.000
Se4 0.0280 (4) 0.0280 (4) 0.0043 (4) 0.01399 (18) 0.000 0.000 Se5 0.0115 (3) 0.0115 (3) 0.0047 (4) 0.00577 (13) 0.000 0.000 In 0.0373 (5) 0.0373 (5) 0.0324 (7) 0.0186 (2) 0.000 0.000 Ho 0.0151 (8) 0.0096 (7) 0.0147 (7) 0.0053 (6) 0.000 0.000
Geometric parameters (Å, º)
Mo1—Se4 2.5469 (9) Se3—Mo2x 2.6928 (6)
Mo1—Se1i 2.5526 (7) Se3—Mo2v 2.6928 (6)
Mo1—Se1 2.5765 (7) Se3—Hoiii 2.7270 (16)
Mo1—Se1ii 2.6163 (6) Se3—Hoii 2.9690 (16)
Mo1—Se2 2.6587 (7) Se3—Inxii 4.2704 (9)
Mo1—Mo1iii 2.7001 (7) Se3—Inxiii 4.2704 (9)
Mo1—Mo1ii 2.7001 (7) Se4—Mo1iii 2.5469 (9)
Mo1—Mo1iv 2.7104 (8) Se4—Mo1ii 2.5469 (9)
Mo1—Mo1i 2.7104 (8) Se4—Hoiii 2.5689 (13)
Mo1—Mo2v 3.4666 (6) Se4—Hoii 2.5689 (13)
Mo1—Invi 4.6789 (5) Se4—Ho 2.5689 (13)
Mo2—Se5 2.5290 (8) Se5—Mo2vii 2.5290 (8)
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Acta Cryst. (2006). E62, i83–i85
Mo2—Se2vii 2.6275 (7) In—Se5 3.0647 (15)
Mo2—Mo2vii 2.6470 (7) In—Se2vi 3.1591 (5)
Mo2—Mo2v 2.6470 (7) In—Se2xiv 3.1591 (5)
Mo2—Se1viii 2.6675 (7) In—Se2i 3.1591 (5)
Mo2—Se3vii 2.6928 (6) In—Se1vi 3.5079 (7)
Mo2—Mo3vii 2.7179 (5) In—Se1i 3.5079 (7)
Mo2—Mo3 2.7673 (5) In—Se1xiv 3.5079 (7)
Mo2—Invi 4.4980 (4) In—Se3iv 4.2704 (9)
Mo3—Se3vii 2.5836 (9) In—Se3xv 4.2704 (9)
Mo3—Se2 2.5851 (6) In—Se3xiii 4.2704 (9)
Mo3—Se2ix 2.5851 (6) In—Mo2xiv 4.4980 (4)
Mo3—Se3 2.5908 (9) In—Mo2vi 4.4980 (4)
Mo3—Mo2x 2.7179 (5) In—Mo2i 4.4980 (4)
Mo3—Mo2v 2.7179 (5) In—Hoxvi 4.5834 (15)
Mo3—Mo3v 2.7193 (10) In—Hoxvii 4.5834 (15)
Mo3—Mo3vii 2.7193 (10) In—Hoxviii 4.5834 (15)
Mo3—Mo2ix 2.7673 (5) Ho—Se4ix 2.5689 (13)
Mo3—Hoii 2.8993 (15) Ho—Se3ii 2.7270 (16)
Se1—Mo1iv 2.5526 (7) Ho—Se2iii 2.8314 (11)
Se1—Mo1iii 2.6163 (6) Ho—Se2xix 2.8314 (11)
Se1—Mo2xi 2.6675 (7) Ho—Mo3iii 2.8993 (15)
Se1—Invi 3.5079 (7) Ho—Se3iii 2.9690 (16)
Se2—Mo2v 2.6275 (6) Ho—Hoiii 3.295 (3)
Se2—Hoii 2.8314 (11) Ho—Hoii 3.295 (3)
Se2—Invi 3.1591 (5) Ho—Inxvii 4.5834 (15)
Se3—Mo3v 2.5836 (9) Ho—Inxx 4.5834 (15)
Se4—Mo1—Se1i 176.38 (3) Inxii—Se3—Inxiii 66.97 (3)
Se4—Mo1—Se1 91.489 (17) Mo1iii—Se4—Mo1ii 64.02 (3)
Se1i—Mo1—Se1 89.250 (17) Mo1iii—Se4—Mo1 64.02 (3)
Se4—Mo1—Se1ii 90.580 (17) Mo1ii—Se4—Mo1 64.02 (3)
Se1i—Mo1—Se1ii 88.377 (17) Mo1iii—Se4—Hoiii 148.11 (3)
Se1—Mo1—Se1ii 174.56 (3) Mo1ii—Se4—Hoiii 95.32 (2)
Se4—Mo1—Se2 90.72 (2) Mo1—Se4—Hoiii 130.75 (3)
Se1i—Mo1—Se2 92.86 (2) Mo1iii—Se4—Hoii 130.75 (3)
Se1—Mo1—Se2 86.74 (2) Mo1ii—Se4—Hoii 148.11 (3)
Se1ii—Mo1—Se2 98.27 (2) Mo1—Se4—Hoii 95.32 (2)
Se4—Mo1—Mo1iii 57.990 (13) Hoiii—Se4—Hoii 79.77 (4)
Se1i—Mo1—Mo1iii 119.638 (17) Mo1iii—Se4—Ho 95.32 (2)
Se1—Mo1—Mo1iii 59.39 (2) Mo1ii—Se4—Ho 130.75 (3)
Se1ii—Mo1—Mo1iii 117.90 (2) Mo1—Se4—Ho 148.11 (3)
Se2—Mo1—Mo1iii 130.04 (2) Hoiii—Se4—Ho 79.77 (4)
Se4—Mo1—Mo1ii 57.990 (13) Hoii—Se4—Ho 79.77 (4)
Se1i—Mo1—Mo1ii 118.656 (17) Mo2vii—Se5—Mo2 63.11 (2)
Se1—Mo1—Mo1ii 119.34 (2) Mo2vii—Se5—Mo2v 63.11 (2)
Se1ii—Mo1—Mo1ii 57.95 (2) Mo2—Se5—Mo2v 63.11 (2)
Se2—Mo1—Mo1ii 137.221 (19) Mo2vii—Se5—In 142.822 (15)
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Se4—Mo1—Mo1iv 118.092 (16) Mo2v—Se5—In 142.822 (15)
Se1i—Mo1—Mo1iv 59.53 (2) Se5—In—Se2vi 93.80 (2)
Se1—Mo1—Mo1iv 57.673 (15) Se5—In—Se2xiv 93.80 (2)
Se1ii—Mo1—Mo1iv 116.97 (2) Se2vi—In—Se2xiv 119.564 (5)
Se2—Mo1—Mo1iv 132.37 (2) Se5—In—Se2i 93.80 (2)
Mo1iii—Mo1—Mo1iv 60.125 (11) Se2vi—In—Se2i 119.564 (5)
Mo1ii—Mo1—Mo1iv 90.0 Se2xiv—In—Se2i 119.564 (5)
Se4—Mo1—Mo1i 118.092 (16) Se5—In—Se1vi 64.840 (19)
Se1i—Mo1—Mo1i 58.53 (2) Se2vi—In—Se1vi 65.026 (13)
Se1—Mo1—Mo1i 117.42 (2) Se2xiv—In—Se1vi 64.880 (14)
Se1ii—Mo1—Mo1i 57.236 (15) Se2i—In—Se1vi 158.64 (4)
Se2—Mo1—Mo1i 139.85 (2) Se5—In—Se1i 64.840 (19)
Mo1iii—Mo1—Mo1i 90.0 Se2vi—In—Se1i 64.880 (14)
Mo1ii—Mo1—Mo1i 60.125 (11) Se2xiv—In—Se1i 158.64 (4)
Mo1iv—Mo1—Mo1i 59.75 (2) Se2i—In—Se1i 65.026 (13)
Se4—Mo1—Invi 99.688 (19) Se1vi—In—Se1i 103.23 (2)
Se1i—Mo1—Invi 83.419 (19) Se5—In—Se1xiv 64.840 (19)
Se1—Mo1—Invi 47.705 (14) Se2vi—In—Se1xiv 158.64 (4)
Se1ii—Mo1—Invi 136.719 (18) Se2xiv—In—Se1xiv 65.026 (13)
Se2—Mo1—Invi 40.278 (15) Se2i—In—Se1xiv 64.880 (14)
Mo1iii—Mo1—Invi 102.863 (18) Se1vi—In—Se1xiv 103.23 (2)
Mo1ii—Mo1—Invi 156.315 (16) Se1i—In—Se1xiv 103.23 (2)
Mo1iv—Mo1—Invi 94.923 (17) Se5—In—Se3iv 123.487 (14)
Mo1i—Mo1—Invi 140.93 (2) Se2vi—In—Se3iv 55.274 (16)
Se5—Mo2—Se2 92.189 (17) Se2xiv—In—Se3iv 141.57 (4)
Se5—Mo2—Se2vii 91.227 (17) Se2i—In—Se3iv 71.125 (17)
Se2—Mo2—Se2vii 174.78 (3) Se1vi—In—Se3iv 119.728 (14)
Se5—Mo2—Mo2vii 58.444 (12) Se1i—In—Se3iv 59.375 (11)
Se2—Mo2—Mo2vii 120.20 (2) Se1xiv—In—Se3iv 135.828 (14)
Se2vii—Mo2—Mo2vii 58.72 (2) Se5—In—Se3xv 123.487 (14)
Se5—Mo2—Mo2v 58.444 (12) Se2vi—In—Se3xv 71.125 (17)
Se2—Mo2—Mo2v 60.26 (2) Se2xiv—In—Se3xv 55.274 (16)
Se2vii—Mo2—Mo2v 118.66 (2) Se2i—In—Se3xv 141.57 (4)
Mo2vii—Mo2—Mo2v 60.0 Se1vi—In—Se3xv 59.375 (11)
Se5—Mo2—Se1viii 90.55 (2) Se1i—In—Se3xv 135.828 (14)
Se2—Mo2—Se1viii 86.15 (2) Se1xiv—In—Se3xv 119.728 (14)
Se2vii—Mo2—Se1viii 97.77 (2) Se3iv—In—Se3xv 92.49 (2)
Mo2vii—Mo2—Se1viii 137.526 (19) Se5—In—Se3xiii 123.487 (14)
Mo2v—Mo2—Se1viii 130.30 (2) Se2vi—In—Se3xiii 141.57 (4)
Se5—Mo2—Se3vii 175.06 (3) Se2xiv—In—Se3xiii 71.125 (17)
Se2—Mo2—Se3vii 85.50 (2) Se2i—In—Se3xiii 55.274 (15)
Se2vii—Mo2—Se3vii 90.79 (2) Se1vi—In—Se3xiii 135.829 (14)
Mo2vii—Mo2—Se3vii 119.183 (18) Se1i—In—Se3xiii 119.727 (14)
Mo2v—Mo2—Se3vii 116.678 (19) Se1xiv—In—Se3xiii 59.375 (11)
Se1viii—Mo2—Se3vii 93.64 (2) Se3iv—In—Se3xiii 92.49 (2)
Se5—Mo2—Mo3vii 120.52 (2) Se3xv—In—Se3xiii 92.49 (2)
Se2—Mo2—Mo3vii 116.98 (2) Se5—In—Mo2xiv 91.190 (16)
supporting information
sup-5
Acta Cryst. (2006). E62, i83–i85
Mo2vii—Mo2—Mo3vii 62.086 (16) Se2xiv—In—Mo2xiv 34.134 (11)
Mo2v—Mo2—Mo3vii 91.285 (15) Se2i—In—Mo2xiv 153.608 (13)
Se1viii—Mo2—Mo3vii 138.15 (2) Se1vi—In—Mo2xiv 36.333 (10)
Se3vii—Mo2—Mo3vii 57.21 (2) Se1i—In—Mo2xiv 139.26 (2)
Se5—Mo2—Mo3 118.65 (2) Se1xiv—In—Mo2xiv 94.266 (12)
Se2—Mo2—Mo3 57.630 (18) Se3iv—In—Mo2xiv 126.11 (2)
Se2vii—Mo2—Mo3 117.19 (2) Se3xv—In—Mo2xiv 35.650 (9)
Mo2vii—Mo2—Mo3 90.204 (15) Se3xiii—In—Mo2xiv 100.888 (15)
Mo2v—Mo2—Mo3 60.216 (15) Se5—In—Mo2vi 91.190 (16)
Se1viii—Mo2—Mo3 131.91 (2) Se2vi—In—Mo2vi 34.134 (11)
Se3vii—Mo2—Mo3 56.463 (19) Se2xiv—In—Mo2vi 153.608 (13)
Mo3vii—Mo2—Mo3 59.43 (2) Se2i—In—Mo2vi 85.861 (11)
Se5—Mo2—Invi 113.462 (19) Se1vi—In—Mo2vi 94.266 (12)
Se2—Mo2—Invi 43.269 (13) Se1i—In—Mo2vi 36.333 (10)
Se2vii—Mo2—Invi 137.970 (17) Se1xiv—In—Mo2vi 139.26 (2)
Mo2vii—Mo2—Invi 163.303 (19) Se3iv—In—Mo2vi 35.649 (9)
Mo2v—Mo2—Invi 103.341 (19) Se3xv—In—Mo2vi 100.888 (15)
Se1viii—Mo2—Invi 51.183 (17) Se3xiii—In—Mo2vi 126.11 (2)
Se3vii—Mo2—Invi 67.56 (2) Mo2xiv—In—Mo2vi 119.957 (1)
Mo3vii—Mo2—Invi 123.41 (2) Se5—In—Mo2i 91.190 (16)
Mo3—Mo2—Invi 81.293 (19) Se2vi—In—Mo2i 153.608 (13)
Se3vii—Mo3—Se2 87.80 (2) Se2xiv—In—Mo2i 85.861 (11)
Se3vii—Mo3—Se2ix 87.80 (2) Se2i—In—Mo2i 34.134 (11)
Se2—Mo3—Se2ix 112.27 (3) Se1vi—In—Mo2i 139.26 (2)
Se3vii—Mo3—Se3 176.59 (3) Se1i—In—Mo2i 94.266 (12)
Se2—Mo3—Se3 94.09 (2) Se1xiv—In—Mo2i 36.333 (10)
Se2ix—Mo3—Se3 94.09 (2) Se3iv—In—Mo2i 100.888 (15)
Se3vii—Mo3—Mo2x 118.011 (16) Se3xv—In—Mo2i 126.11 (2)
Se2—Mo3—Mo2x 150.76 (3) Se3xiii—In—Mo2i 35.650 (9)
Se2ix—Mo3—Mo2x 59.337 (15) Mo2xiv—In—Mo2i 119.957 (1)
Se3—Mo3—Mo2x 60.904 (15) Mo2vi—In—Mo2i 119.957 (1)
Se3vii—Mo3—Mo2v 118.011 (16) Se5—In—Hoxvi 120.935 (16)
Se2—Mo3—Mo2v 59.337 (15) Se2vi—In—Hoxvi 37.513 (19)
Se2ix—Mo3—Mo2v 150.76 (3) Se2xiv—In—Hoxvi 90.18 (2)
Se3—Mo3—Mo2v 60.904 (15) Se2i—In—Hoxvi 133.45 (3)
Mo2x—Mo3—Mo2v 112.72 (3) Se1vi—In—Hoxvi 64.173 (16)
Se3vii—Mo3—Mo3v 118.43 (3) Se1i—In—Hoxvi 100.582 (19)
Se2—Mo3—Mo3v 120.47 (2) Se1xiv—In—Hoxvi 155.19 (2)
Se2ix—Mo3—Mo3v 120.47 (2) Se3iv—In—Hoxvi 64.13 (2)
Se3—Mo3—Mo3v 58.17 (3) Se3xv—In—Hoxvi 35.66 (2)
Mo2x—Mo3—Mo3v 61.188 (17) Se3xiii—In—Hoxvi 113.45 (3)
Mo2v—Mo3—Mo3v 61.188 (17) Mo2xiv—In—Hoxvi 62.630 (18)
Se3vii—Mo3—Mo3vii 58.43 (3) Mo2vi—In—Hoxvi 65.238 (19)
Se2—Mo3—Mo3vii 116.97 (2) Mo2i—In—Hoxvi 147.84 (3)
Se2ix—Mo3—Mo3vii 116.97 (2) Se5—In—Hoxvii 120.935 (16)
Se3—Mo3—Mo3vii 118.17 (3) Se2vi—In—Hoxvii 90.18 (2)
Mo2x—Mo3—Mo3vii 89.748 (15) Se2xiv—In—Hoxvii 133.45 (3)
supporting information
sup-6
Acta Cryst. (2006). E62, i83–i85
Mo3v—Mo3—Mo3vii 60.0 Se1vi—In—Hoxvii 155.19 (2)
Se3vii—Mo3—Mo2ix 60.314 (14) Se1i—In—Hoxvii 64.172 (16)
Se2—Mo3—Mo2ix 145.40 (3) Se1xiv—In—Hoxvii 100.582 (19)
Se2ix—Mo3—Mo2ix 57.667 (15) Se3iv—In—Hoxvii 35.66 (2)
Se3—Mo3—Mo2ix 118.486 (16) Se3xv—In—Hoxvii 113.45 (3)
Mo2x—Mo3—Mo2ix 57.698 (17) Se3xiii—In—Hoxvii 64.13 (2)
Mo2v—Mo3—Mo2ix 145.81 (3) Mo2xiv—In—Hoxvii 147.84 (3)
Mo3v—Mo3—Mo2ix 88.722 (14) Mo2vi—In—Hoxvii 62.630 (18)
Mo3vii—Mo3—Mo2ix 59.383 (16) Mo2i—In—Hoxvii 65.238 (18)
Se3vii—Mo3—Mo2 60.314 (14) Hoxvi—In—Hoxvii 95.95 (2)
Se2—Mo3—Mo2 57.667 (15) Se5—In—Hoxviii 120.935 (16)
Se2ix—Mo3—Mo2 145.40 (3) Se2vi—In—Hoxviii 133.45 (3)
Se3—Mo3—Mo2 118.486 (16) Se2xiv—In—Hoxviii 37.513 (19)
Mo2x—Mo3—Mo2 145.81 (3) Se2i—In—Hoxviii 90.18 (2)
Mo2v—Mo3—Mo2 57.698 (17) Se1vi—In—Hoxviii 100.582 (19)
Mo3v—Mo3—Mo2 88.722 (14) Se1i—In—Hoxviii 155.19 (2)
Mo3vii—Mo3—Mo2 59.383 (16) Se1xiv—In—Hoxviii 64.173 (16)
Mo2ix—Mo3—Mo2 109.71 (3) Se3iv—In—Hoxviii 113.45 (3)
Se3vii—Mo3—Hoii 118.21 (4) Se3xv—In—Hoxviii 64.13 (2)
Se2—Mo3—Hoii 61.851 (19) Se3xiii—In—Hoxviii 35.66 (2)
Se2ix—Mo3—Hoii 61.851 (19) Mo2xiv—In—Hoxviii 65.238 (19)
Se3—Mo3—Hoii 65.19 (4) Mo2vi—In—Hoxviii 147.84 (3)
Mo2x—Mo3—Hoii 92.11 (2) Mo2i—In—Hoxviii 62.630 (18)
Mo2v—Mo3—Hoii 92.11 (2) Hoxvi—In—Hoxviii 95.95 (2)
Mo3v—Mo3—Hoii 123.36 (4) Hoxvii—In—Hoxviii 95.95 (2)
Mo3vii—Mo3—Hoii 176.64 (4) Se4ix—Ho—Se4 84.46 (5)
Mo2ix—Mo3—Hoii 119.517 (18) Se4ix—Ho—Se3ii 88.65 (4)
Mo2—Mo3—Hoii 119.517 (18) Se4—Ho—Se3ii 88.65 (4)
Mo1iv—Se1—Mo1 63.80 (2) Se4ix—Ho—Se2iii 163.32 (6)
Mo1iv—Se1—Mo1iii 63.24 (2) Se4—Ho—Se2iii 86.49 (2)
Mo1—Se1—Mo1iii 62.66 (2) Se3ii—Ho—Se2iii 105.14 (4)
Mo1iv—Se1—Mo2xi 131.54 (2) Se4ix—Ho—Se2xix 86.49 (2)
Mo1—Se1—Mo2xi 129.02 (2) Se4—Ho—Se2xix 163.32 (6)
Mo1iii—Se1—Mo2xi 82.00 (2) Se3ii—Ho—Se2xix 105.14 (4)
Mo1iv—Se1—Invi 134.69 (2) Se2iii—Ho—Se2xix 98.60 (5)
Mo1—Se1—Invi 99.386 (18) Se4ix—Ho—Mo3iii 120.75 (4)
Mo1iii—Se1—Invi 148.54 (3) Se4—Ho—Mo3iii 120.75 (4)
Mo2xi—Se1—Invi 92.48 (2) Se3ii—Ho—Mo3iii 138.15 (6)
Mo3—Se2—Mo2 64.703 (19) Se2iii—Ho—Mo3iii 53.61 (3)
Mo3—Se2—Mo2v 62.848 (18) Se2xix—Ho—Mo3iii 53.61 (3)
Mo2—Se2—Mo2v 61.02 (2) Se4ix—Ho—Se3iii 83.57 (4)
Mo3—Se2—Mo1 130.30 (3) Se4—Ho—Se3iii 83.57 (4)
Mo2—Se2—Mo1 127.66 (2) Se3ii—Ho—Se3iii 169.47 (6)
Mo2v—Se2—Mo1 81.96 (2) Se2iii—Ho—Se3iii 81.51 (3)
Mo3—Se2—Hoii 64.54 (3) Se2xix—Ho—Se3iii 81.51 (3)
Mo2—Se2—Hoii 129.24 (3) Mo3iii—Ho—Se3iii 52.38 (3)
Mo2v—Se2—Hoii 95.61 (4) Se4ix—Ho—Hoiii 50.12 (2)
supporting information
sup-7
Acta Cryst. (2006). E62, i83–i85
Mo3—Se2—Invi 117.17 (3) Se3ii—Ho—Hoiii 58.17 (5)
Mo2—Se2—Invi 102.597 (19) Se2iii—Ho—Hoiii 130.20 (3)
Mo2v—Se2—Invi 162.70 (2) Se2xix—Ho—Hoiii 130.20 (3)
Mo1—Se2—Invi 106.76 (2) Mo3iii—Ho—Hoiii 163.68 (7)
Hoii—Se2—Invi 99.69 (4) Se3iii—Ho—Hoiii 111.30 (5)
Mo3v—Se3—Mo3 63.41 (3) Se4ix—Ho—Hoii 50.12 (2)
Mo3v—Se3—Mo2x 63.224 (17) Se4—Ho—Hoii 50.12 (2)
Mo3—Se3—Mo2x 61.881 (17) Se3ii—Ho—Hoii 118.17 (5)
Mo3v—Se3—Mo2v 63.224 (17) Se2iii—Ho—Hoii 113.79 (5)
Mo3—Se3—Mo2v 61.881 (17) Se2xix—Ho—Hoii 113.79 (5)
Mo2x—Se3—Mo2v 114.35 (3) Mo3iii—Ho—Hoii 103.68 (7)
Mo3v—Se3—Hoiii 163.64 (5) Se3iii—Ho—Hoii 51.30 (5)
Mo3—Se3—Hoiii 132.95 (5) Hoiii—Ho—Hoii 60.0
Mo2x—Se3—Hoiii 121.145 (17) Se4ix—Ho—Inxvii 153.40 (5)
Mo2v—Se3—Hoiii 121.145 (17) Se4—Ho—Inxvii 101.72 (3)
Mo3v—Se3—Hoii 125.83 (4) Se3ii—Ho—Inxvii 65.90 (3)
Mo3—Se3—Hoii 62.42 (3) Se2iii—Ho—Inxvii 42.80 (2)
Mo2x—Se3—Hoii 91.10 (2) Se2xix—Ho—Inxvii 92.62 (4)
Mo2v—Se3—Hoii 91.10 (2) Mo3iii—Ho—Inxvii 78.51 (3)
Hoiii—Se3—Hoii 70.53 (6) Se3iii—Ho—Inxvii 122.64 (3)
Mo3v—Se3—Inxii 87.95 (2) Hoiii—Ho—Inxvii 115.19 (5)
Mo3—Se3—Inxii 136.807 (19) Hoii—Ho—Inxvii 149.064 (16)
Mo2x—Se3—Inxii 76.790 (18) Se4ix—Ho—Inxx 101.72 (3)
Mo2v—Se3—Inxii 134.33 (3) Se4—Ho—Inxx 153.40 (5)
Hoiii—Se3—Inxii 78.44 (3) Se3ii—Ho—Inxx 65.90 (3)
Hoii—Se3—Inxii 134.15 (2) Se2iii—Ho—Inxx 92.62 (4)
Mo3v—Se3—Inxiii 87.95 (2) Se2xix—Ho—Inxx 42.80 (2)
Mo3—Se3—Inxiii 136.807 (19) Mo3iii—Ho—Inxx 78.51 (3)
Mo2x—Se3—Inxiii 134.33 (3) Se3iii—Ho—Inxx 122.64 (3)
Mo2v—Se3—Inxiii 76.790 (18) Hoiii—Ho—Inxx 115.19 (5)
Hoiii—Se3—Inxiii 78.44 (3) Hoii—Ho—Inxx 149.064 (16)
Hoii—Se3—Inxiii 134.15 (2) Inxvii—Ho—Inxx 61.87 (3)