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Single crystals of the barium trigallium tin, BaGa3.11 (2)Sn0.89 (2), have been obtained by a reaction of the elements in a sealed Nb tube. The title compound crystallizes with the BaAl4-type (Pearson's code tI10), and some of the Ga atoms are replaced by Sn atoms. All atoms occupy special positions: Ba (4/mmm), Ga1/Sn1 (\overline{4}m2) and Ga2/Sn2 (4mm). The refined composition has also been confirmed by means of elemental microanalysis.

Supporting information

cif

Crystallographic Information File (CIF) https://doi.org/10.1107/S1600536807000359/wm2086sup1.cif
Contains datablocks global, I

hkl

Structure factor file (CIF format) https://doi.org/10.1107/S1600536807000359/wm2086Isup2.hkl
Contains datablock I

Key indicators

  • Single-crystal X-ray study
  • T = 120 K
  • Mean [sigma]() = 0.000 Å
  • Disorder in main residue
  • R factor = 0.018
  • wR factor = 0.039
  • Data-to-parameter ratio = 10.3

checkCIF/PLATON results

No syntax errors found



Alert level C PLAT041_ALERT_1_C Calc. and Rep. SumFormula Strings Differ .... ? PLAT045_ALERT_1_C Calculated and Reported Z Differ by ............ 0.50 Ratio PLAT066_ALERT_1_C Predicted and Reported Transmissions Identical . ? PLAT068_ALERT_1_C Reported F000 Differs from Calcd (or Missing)... ? PLAT077_ALERT_4_C Unitcell contains non-integer number of atoms .. ? PLAT301_ALERT_3_C Main Residue Disorder ......................... 25.00 Perc.
0 ALERT level A = In general: serious problem 0 ALERT level B = Potentially serious problem 6 ALERT level C = Check and explain 0 ALERT level G = General alerts; check 4 ALERT type 1 CIF construction/syntax error, inconsistent or missing data 0 ALERT type 2 Indicator that the structure model may be wrong or deficient 1 ALERT type 3 Indicator that the structure quality may be low 1 ALERT type 4 Improvement, methodology, query or suggestion 0 ALERT type 5 Informative message, check

Computing details top

Data collection: SMART (Bruker, 2003); cell refinement: SAINT (Bruker, 2003); data reduction: SAINT; program(s) used to solve structure: SHELXTL (Sheldrick, 2001); program(s) used to refine structure: SHELXTL; molecular graphics: XP in SHELXTL; software used to prepare material for publication: SHELXTL.

barium trigallium tin top
Crystal data top
BaGa3.11Sn0.89Dx = 6.425 Mg m3
Mr = 459.80Mo Kα radiation, λ = 0.71073 Å
Tetragonal, I4/mmmCell parameters from 620 reflections
Hall symbol: -I 4 2θ = 3.9–27.3°
a = 4.7455 (14) ŵ = 29.97 mm1
c = 10.554 (6) ÅT = 120 K
V = 237.68 (17) Å3Plate, metallic grey
Z = 20.07 × 0.07 × 0.06 mm
F(000) = 394
Data collection top
Bruker SMART APEX CCD area-detector
diffractometer
103 independent reflections
Radiation source: fine-focus sealed tube92 reflections with I > 2σ(I)
Graphite monochromatorRint = 0.019
Detector resolution: 8.3 pixels mm-1θmax = 27.3°, θmin = 3.9°
ω scansh = 65
Absorption correction: multi-scan
(SADABS; Sheldrick, 2003)
k = 56
Tmin = 0.142, Tmax = 0.165l = 1311
651 measured reflections
Refinement top
Refinement on F20 restraints
Least-squares matrix: fullPrimary atom site location: structure-invariant direct methods
R[F2 > 2σ(F2)] = 0.018Secondary atom site location: difference Fourier map
wR(F2) = 0.039 w = 1/[σ2(Fo2) + (0.0205P)2 + 0.0192P]
where P = (Fo2 + 2Fc2)/3
S = 1.21(Δ/σ)max < 0.001
103 reflectionsΔρmax = 0.86 e Å3
10 parametersΔρmin = 1.67 e Å3
Special details top

Experimental. Data collection was performed with four batch runs at φ = 0.00° (450 frames), at φ = 90.00° (450 frames), at φ = 180.00° (450 frames), and at φ = 270.00° (450 frames). Frame width = 0.40° in ω. Data were merged and treated with multi-scan absorption corrections.

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 covariance matrix. The cell e.s.d.'s are taken into account individually in the estimation of e.s.d.'s in distances, angles and torsion angles; correlations between e.s.d.'s in cell parameters are only used when they are defined by crystal symmetry. An approximate (isotropic) treatment of cell e.s.d.'s is used for estimating e.s.d.'s involving l.s. planes.

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) top
xyzUiso*/UeqOcc. (<1)
Ba0.00000.00000.00000.0114 (3)
Ga10.00000.50000.25000.0147 (3)0.824 (8)
Sn10.00000.50000.25000.0147 (3)0.176 (8)
Ga20.00000.00000.37537 (10)0.0128 (3)0.731 (9)
Sn20.00000.00000.37537 (10)0.0128 (3)0.269 (9)
Atomic displacement parameters (Å2) top
U11U22U33U12U13U23
Ba0.0112 (3)0.0112 (3)0.0119 (5)0.0000.0000.000
Ga10.0172 (4)0.0172 (4)0.0095 (6)0.0000.0000.000
Sn10.0172 (4)0.0172 (4)0.0095 (6)0.0000.0000.000
Ga20.0147 (4)0.0147 (4)0.0090 (5)0.0000.0000.000
Sn20.0147 (4)0.0147 (4)0.0090 (5)0.0000.0000.000
Geometric parameters (Å, º) top
Ba—Sn1i3.5485 (13)Ga1—Ga2i2.7167 (9)
Ba—Ga1i3.5485 (13)Ga1—Ga22.7167 (9)
Ba—Ga13.5485 (13)Ga1—Baix3.5485 (13)
Ba—Sn1ii3.5485 (13)Ga1—Bax3.5485 (13)
Ba—Ga1ii3.5485 (13)Ga1—Baviii3.5485 (13)
Ba—Sn1iii3.5485 (13)Ga2—Sn2xi2.631 (3)
Ba—Ga1iii3.5485 (13)Ga2—Ga2xi2.631 (3)
Ba—Sn1iv3.5485 (13)Ga2—Sn1iv2.7168 (9)
Ba—Ga1v3.5485 (13)Ga2—Sn1v2.7168 (9)
Ba—Ga1vi3.5485 (13)Ga2—Ga1iv2.7168 (9)
Ba—Sn1vii3.5485 (13)Ga2—Ga1v2.7168 (9)
Ga1—Sn2iv2.7167 (9)Ga2—Sn1i2.7167 (9)
Ga1—Ga2iv2.7167 (9)Ga2—Ga1i2.7167 (9)
Ga1—Sn2viii2.7167 (9)Ga2—Baix3.6042 (10)
Ga1—Ga2viii2.7167 (9)Ga2—Baxii3.6042 (10)
Ga1—Sn2i2.7167 (9)
Sn1i—Ba—Ga156.43 (2)Sn2iv—Ga1—Baix161.11 (2)
Sn1i—Ba—Sn1ii123.57 (2)Sn2viii—Ga1—Baix68.77 (2)
Ga1—Ba—Sn1ii180.0Ga2iv—Ga1—Baix161.11 (2)
Sn1i—Ba—Sn1iii180.0Ga2viii—Ga1—Baix68.77 (2)
Ga1—Ba—Sn1iii123.57 (2)Sn2i—Ga1—Baix77.18 (4)
Sn1ii—Ba—Sn1iii56.43 (2)Ga2i—Ga1—Baix77.18 (4)
Sn1i—Ba—Ga1i0.0Ga2—Ga1—Baix68.77 (2)
Ga1—Ba—Ga1i56.43 (2)Ba—Ga1—Baix123.57 (2)
Sn1ii—Ba—Ga1i123.57 (2)Sn2iv—Ga1—Bax77.18 (4)
Sn1iii—Ba—Ga1i180.0Sn2viii—Ga1—Bax68.77 (2)
Sn1i—Ba—Ga1ii123.57 (2)Ga2iv—Ga1—Bax77.18 (4)
Ga1—Ba—Ga1ii180.0Ga2viii—Ga1—Bax68.77 (2)
Sn1ii—Ba—Ga1ii0.0Sn2i—Ga1—Bax161.11 (2)
Sn1iii—Ba—Ga1ii56.43 (2)Ga2i—Ga1—Bax161.11 (2)
Ga1i—Ba—Ga1ii123.57 (2)Ga2—Ga1—Bax68.77 (2)
Sn1i—Ba—Ga1iii180.0Ba—Ga1—Bax123.57 (2)
Ga1—Ba—Ga1iii123.57 (2)Baix—Ga1—Bax83.93 (4)
Sn1ii—Ba—Ga1iii56.43 (2)Sn2iv—Ga1—Baviii68.77 (2)
Sn1iii—Ba—Ga1iii0.0Sn2viii—Ga1—Baviii77.18 (4)
Ga1i—Ba—Ga1iii180.0Ga2iv—Ga1—Baviii68.77 (2)
Ga1ii—Ba—Ga1iii56.43 (2)Ga2viii—Ga1—Baviii77.18 (4)
Sn1i—Ba—Sn1iv83.93 (4)Sn2i—Ga1—Baviii68.77 (2)
Ga1—Ba—Sn1iv56.43 (2)Ga2i—Ga1—Baviii68.77 (2)
Sn1ii—Ba—Sn1iv123.57 (2)Ga2—Ga1—Baviii161.11 (2)
Sn1iii—Ba—Sn1iv96.07 (4)Ba—Ga1—Baviii83.93 (4)
Ga1i—Ba—Sn1iv83.93 (4)Baix—Ga1—Baviii123.57 (2)
Ga1ii—Ba—Sn1iv123.57 (2)Bax—Ga1—Baviii123.57 (2)
Ga1iii—Ba—Sn1iv96.07 (4)Sn2xi—Ga2—Ga2xi0.0
Sn1i—Ba—Ga1v56.43 (2)Sn2xi—Ga2—Sn1iv119.15 (3)
Ga1—Ba—Ga1v83.93 (4)Ga2xi—Ga2—Sn1iv119.15 (3)
Sn1ii—Ba—Ga1v96.07 (4)Sn2xi—Ga2—Sn1v119.15 (3)
Sn1iii—Ba—Ga1v123.57 (2)Ga2xi—Ga2—Sn1v119.15 (3)
Ga1i—Ba—Ga1v56.43 (2)Sn1iv—Ga2—Sn1v76.28 (2)
Ga1ii—Ba—Ga1v96.07 (4)Sn2xi—Ga2—Ga1iv119.15 (3)
Ga1iii—Ba—Ga1v123.57 (2)Ga2xi—Ga2—Ga1iv119.15 (3)
Sn1iv—Ba—Ga1v56.43 (2)Sn1iv—Ga2—Ga1iv0.0
Sn1i—Ba—Ga1vi96.07 (4)Sn1v—Ga2—Ga1iv76.28 (2)
Ga1—Ba—Ga1vi123.57 (2)Sn2xi—Ga2—Ga1v119.15 (3)
Sn1ii—Ba—Ga1vi56.43 (2)Ga2xi—Ga2—Ga1v119.15 (3)
Sn1iii—Ba—Ga1vi83.93 (4)Sn1iv—Ga2—Ga1v76.28 (2)
Ga1i—Ba—Ga1vi96.07 (4)Sn1v—Ga2—Ga1v0.0
Ga1ii—Ba—Ga1vi56.43 (2)Ga1iv—Ga2—Ga1v76.28 (2)
Ga1iii—Ba—Ga1vi83.93 (4)Sn2xi—Ga2—Ga1119.15 (3)
Sn1iv—Ba—Ga1vi180.0Ga2xi—Ga2—Ga1119.15 (3)
Ga1v—Ba—Ga1vi123.57 (2)Sn1iv—Ga2—Ga176.28 (2)
Sn1i—Ba—Sn1vii123.57 (2)Sn1v—Ga2—Ga1121.71 (5)
Ga1—Ba—Sn1vii96.07 (4)Ga1iv—Ga2—Ga176.28 (2)
Sn1ii—Ba—Sn1vii83.93 (4)Ga1v—Ga2—Ga1121.71 (5)
Sn1iii—Ba—Sn1vii56.43 (2)Sn2xi—Ga2—Sn1i119.15 (3)
Ga1i—Ba—Sn1vii123.57 (2)Ga2xi—Ga2—Sn1i119.15 (3)
Ga1ii—Ba—Sn1vii83.93 (4)Sn1iv—Ga2—Sn1i121.71 (5)
Ga1iii—Ba—Sn1vii56.43 (2)Sn1v—Ga2—Sn1i76.28 (2)
Sn1iv—Ba—Sn1vii123.57 (2)Ga1iv—Ga2—Sn1i121.71 (5)
Ga1v—Ba—Sn1vii180.0Ga1v—Ga2—Sn1i76.28 (2)
Ga1vi—Ba—Sn1vii56.43 (2)Ga1—Ga2—Sn1i76.28 (2)
Sn2iv—Ga1—Sn2viii103.72 (2)Sn2xi—Ga2—Ga1i119.15 (3)
Sn2iv—Ga1—Ga2iv0.0Ga2xi—Ga2—Ga1i119.15 (3)
Sn2viii—Ga1—Ga2iv103.72 (2)Sn1iv—Ga2—Ga1i121.71 (5)
Sn2iv—Ga1—Ga2viii103.72 (2)Sn1v—Ga2—Ga1i76.28 (2)
Sn2viii—Ga1—Ga2viii0.00 (4)Ga1iv—Ga2—Ga1i121.71 (5)
Ga2iv—Ga1—Ga2viii103.72 (2)Ga1v—Ga2—Ga1i76.28 (2)
Sn2iv—Ga1—Sn2i121.71 (5)Ga1—Ga2—Ga1i76.28 (2)
Sn2viii—Ga1—Sn2i103.72 (2)Sn1i—Ga2—Ga1i0.0
Ga2iv—Ga1—Sn2i121.71 (5)Sn2xi—Ga2—Baix68.59 (2)
Ga2viii—Ga1—Sn2i103.72 (2)Ga2xi—Ga2—Baix68.59 (2)
Sn2iv—Ga1—Ga2i121.71 (5)Sn1iv—Ga2—Baix138.827 (7)
Sn2viii—Ga1—Ga2i103.72 (2)Sn1v—Ga2—Baix138.827 (7)
Ga2iv—Ga1—Ga2i121.71 (5)Ga1iv—Ga2—Baix138.827 (7)
Ga2viii—Ga1—Ga2i103.72 (2)Ga1v—Ga2—Baix138.827 (7)
Sn2i—Ga1—Ga2i0.00 (4)Ga1—Ga2—Baix66.60 (2)
Sn2iv—Ga1—Ga2103.72 (2)Sn1i—Ga2—Baix66.60 (2)
Sn2viii—Ga1—Ga2121.71 (5)Ga1i—Ga2—Baix66.60 (2)
Ga2iv—Ga1—Ga2103.72 (2)Sn2xi—Ga2—Baxii68.59 (2)
Ga2viii—Ga1—Ga2121.71 (5)Ga2xi—Ga2—Baxii68.59 (2)
Sn2i—Ga1—Ga2103.72 (2)Sn1iv—Ga2—Baxii66.60 (2)
Ga2i—Ga1—Ga2103.72 (2)Sn1v—Ga2—Baxii66.60 (2)
Sn2iv—Ga1—Ba68.77 (2)Ga1iv—Ga2—Baxii66.60 (2)
Sn2viii—Ga1—Ba161.11 (2)Ga1v—Ga2—Baxii66.60 (2)
Ga2iv—Ga1—Ba68.77 (2)Ga1—Ga2—Baxii138.827 (7)
Ga2viii—Ga1—Ba161.11 (2)Sn1i—Ga2—Baxii138.827 (7)
Sn2i—Ga1—Ba68.77 (2)Ga1i—Ga2—Baxii138.827 (7)
Ga2i—Ga1—Ba68.77 (2)Baix—Ga2—Baxii137.19 (4)
Ga2—Ga1—Ba77.18 (4)
Symmetry codes: (i) x+1/2, y+1/2, z+1/2; (ii) x, y, z; (iii) x1/2, y1/2, z1/2; (iv) x1/2, y+1/2, z+1/2; (v) x, y1, z; (vi) x+1/2, y1/2, z1/2; (vii) x, y+1, z; (viii) x, y+1, z; (ix) x+1/2, y+1/2, z+1/2; (x) x1/2, y+1/2, z+1/2; (xi) x, y, z+1; (xii) x1/2, y1/2, z+1/2.
 

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