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The EuAuGe-type CaAuSn phase has been synthesized and single-crystal X-ray diffraction analysis reveals that it has an ortho­rhom­bic symmetry (space group Imm2), with a = 4.5261 (7) Å, b = 7.1356 (11) Å and c = 7.8147 (11) Å. The structure features puckered layers that are connected by homoatomic Au-Au and Sn-Sn inter­layer bonds. This structure is one of the two parent structures of its high-temperature polymorph (ca 873 K), which is an inter­growth structure of the EuAuGe- and SrMgSi-type structures in a 2:3 ratio.

Supporting information

cif

Crystallographic Information File (CIF) https://doi.org/10.1107/S205322961401612X/fn3175sup1.cif
Contains datablocks I, global

hkl

Structure factor file (CIF format) https://doi.org/10.1107/S205322961401612X/fn3175Isup2.hkl
Contains datablock I

CCDC reference: 1013352

Introduction top

During exploratory syntheses of quasicrystals and approximants in the Ca–Au–Tr system (Tr = Ga, In, Ge, Sn; Lin & Corbett, 2007, 2008a,b, 2010a,b), the 1:1:1 phases were sometimes the minor products in inter­esting e/a (electron count per atom) regions. These phases were generally well characterized by single-crystal X-ray diffraction. According to the literature, both CaAuGa (Cordier et al., 1993) and CaAuIn (Kußmann et al., 1998) show SrMgSi-type (or TiNiSi-type) structures (space group Pnma). In comparison, the same 1:1:1 ratio yielded polymorphs when group 13 elements (Ga, In) were replaced by group 14 elements (Ge, Sn). For example, two polymorphs of CaAuGe were reported, i.e. a threefold superstructure (space group Pnma) of the SrMgSi-type (Merlo et al., 1998; Kußmann et al., 1998) and a monoclinic derivative (space group C2/m) (Merlo et al., 1998), whereas CaAuSn exhibits a fivefold superstructure (space group Pnma) of the SrMgSi-type parent structure (Kußmann et al., 1998). The formation of all these superstructures is incurred by different ordering between Au and Sn. In this work, we report another CaAuSn phase, which belongs to the EuAuGe-type (space group Imm2) structure (Pöttgen, 1995) and can also be considered as a parent of the CaAuSn superstructure.

Experimental top

High-purity elements of Ca, Au and Sn (all from Alfa Aesar, >99.99%) were weighed in the desired stoichiometries in an Ar-filled glove-box, and the mixtures were sealed in Ta containers using an arc melter under Ar. The Ta containers were then enclosed in SiO2 tubes, which were evacuated down to 10 -6 Torr (1 Torr = 133.322 Pa). The samples were heated from room temperature to 1123 K at a rate of 120 K h-1, kept at 1073 K for 1 d, slowly cooled to 773 K at a rate of 2 K h-1, annealed at this temperature for three weeks and finally quenched in water. High-yield (> 95%) phase products were obtained from various loadings of CaAu1+xSn1-x (x ±0.2) proportions. All products are fragile, inert to air at room temperature and with a metallic luster.

Refinements top

A single crystal attached to a glass fiber was mounted on a Bruker SMART APEX CCD area-detector diffractometer equipped with Mo Kα (λ = 0.71069 Å) radiation. An exposure time of 10 s per frame at room temperature was adopted. The reflection intensities were integrated using the SAINT-Plus program in the SMART software package (Bruker, 2013). Empirical absorption corrections were accomplished with the aid of the SADABS subprogram (Sheldrick, 1996). The noncentrosymmetric space group was determined by the |E2 - 1| test in XPREP within SHELXTL (Sheldrick, 2008). The structure was solved with the aid of direct methods and subsequently refined on |F2| with a combination of least-squares refinement and difference Fourier maps.

The Au and Sn sites were directly identified by direct methods. After a few cycles of least-square refinements, two independent sites with distances to the Au and Sn sites of ~3.05–3.10 Å were yielded by the difference Fourier map, so Ca was assigned to both sites. Final least-square refinements, with anisotropic displacement parameters, a secondary extinction correction and a constraint of an inversion twin for the noncentric symmetry, yielded R1 = 0.0276, wR2 = 0.0720 and a goodness-of-fit of 1.171 for 23 parameters refined from 330 observed independent data.

Results and discussion top

The present CaAuSn structure features two puckered layers, in which Au and Sn alterate along the c axis. There are two sets of Au—Sn bond distances in the puckered layers, i.e. 2.628 (1) and 2.663 (3) Å, the two shortest inter­atomic separations in the structure. Viewed along the a axis, adjacent puckered layers are connected by homo-atomic Au—Au [3.090 (2) Å] and Sn—Sn [2.746 (5) Å] inter­layer bonds, as shown in Fig. 1(a), whereas the electropositive Ca atoms are located in the large eight-membered rings. From another viewpoint, the Au–Sn three-dimensional framework can be considered as inter­linked ladders (circled with a red line in Fig. 1a), which consist of the above-mentioned inter­layer bonds. This structure differs from the SrMgSi-type by the `coloring' with regard to the inter­layer bonds (or ladders). As shown in Fig. 1(b), the SrMgSi-type structure consists only of hetero-atomic inter­layer bonds.

It turns out that the EuAuGe- and SrMgSi-type structures, both ordered derivatives of the KHg2-type (or CeCu2-type) structure (Hoffmann & Pöttgen, 2001), represent the two basic structural motifs for all the above-mentioned superstructures and others, which are actually inter­growth structures consisting of various proportions of the building blocks of the EuAuGe- and SrMgSi-type structures. Using A and B to represent the ladders of the EuAuGe- and SrMgSi-type structures, respectively, CaAuGe (Merlo et al., 1998; Kußmann et al., 1998) can be considered as a 4A+2B inter­growth structure, as shown in Fig. 2(a). Similarly, the structure of CaAuSn (Kußmann et al., 1998) is a 4A+6B inter­growth structure (Fig. 2b), EuAuSn (Pöttgen et al., 1997) is a 6A+4B inter­growth (Fig. 2c) and YPdSi (Prots' et al., 1998) is a 2A+2B inter­growth structure (Fig. 2d). Apparently, similar phases with other A+B combinations could exist and are to be discovered.

Related literature top

For related literature, see: Bruker (2013); Cordier et al. (1993); Hoffmann & Pöttgen (2001); Kußmann, Hoffmann & Pöttgen (1998); Lin & Corbett (2007, 2008a, 2008b, 2010a, 2010b); Merlo et al. (1998); Pöttgen (1995); Pöttgen et al. (1997); Sheldrick (1996, 2008).

Computing details top

Data collection: SMART (Bruker, 2002); cell refinement: SAINT-Plus (Bruker, 2013); data reduction: SAINT-Plus (Bruker, 2013); program(s) used to solve structure: SHELXS97 (Sheldrick, 2008); program(s) used to refine structure: SHELXL2013 (Sheldrick, 2008); molecular graphics: DIAMOND (Brandenburg, 2000); software used to prepare material for publication: SHELXTL2013 (Sheldrick, 2008).

Figures top
[Figure 1] Fig. 1. Views of the 2 × 2 unit cells of (a) the EuAuGe-type CaAuSn along the a axis and (b) the SrMgSi-type EuZnSn along the b axis. In both plots, the areas circled by red lines mark the major coloring differences with regard to interlayer bonds or ladders.
[Figure 2] Fig. 2. The crystal structures of (a) CaAuGe, (b) CaAuSn, (c) EuAuSn and (d) YPdSi. The symbols `A' and `B' are used to show the differences among these intergrowth structures.
Calcium gold stannide top
Crystal data top
CaAuSnDx = 9.362 Mg m3
Mr = 355.74Mo Kα radiation, λ = 0.71073 Å
Orthorhombic, Imm2Cell parameters from 330 reflections
a = 4.5261 (7) Åθ = 3.9–28.2°
b = 7.1356 (11) ŵ = 69.58 mm1
c = 7.8147 (11) ÅT = 273 K
V = 252.39 (7) Å3Irregular, metallic
Z = 40.03 × 0.02 × 0.02 mm
F(000) = 596
Data collection top
Bruker SMART APEXII CCD area-detector
diffractometer
326 reflections with I > 2σ(I)
Radiation source: Mo KaRint = 0.024
ω scansθmax = 28.2°, θmin = 3.9°
Absorption correction: empirical (using intensity measurements)
(SADABS; Sheldrick, 1996)
h = 55
Tmin = 0.16, Tmax = 0.27k = 49
769 measured reflectionsl = 109
330 independent reflections
Refinement top
Refinement on F2Secondary atom site location: difference Fourier map
Least-squares matrix: full w = 1/[σ2(Fo2) + (0.036P)2 + 7.6305P]
where P = (Fo2 + 2Fc2)/3
R[F2 > 2σ(F2)] = 0.028(Δ/σ)max < 0.001
wR(F2) = 0.072Δρmax = 2.68 e Å3
S = 1.17Δρmin = 1.85 e Å3
330 reflectionsExtinction correction: SHELXL2013 (Sheldrick, 2008), Fc*=kFc[1+0.001xFc2λ3/sin(2θ)]-1/4
23 parametersExtinction coefficient: 0.0072 (10)
1 restraintAbsolute structure: Refined as an inversion twin (Flack, 1983)
Primary atom site location: structure-invariant direct methodsAbsolute structure parameter: 0.31 (3)
Crystal data top
CaAuSnV = 252.39 (7) Å3
Mr = 355.74Z = 4
Orthorhombic, Imm2Mo Kα radiation
a = 4.5261 (7) ŵ = 69.58 mm1
b = 7.1356 (11) ÅT = 273 K
c = 7.8147 (11) Å0.03 × 0.02 × 0.02 mm
Data collection top
Bruker SMART APEXII CCD area-detector
diffractometer
330 independent reflections
Absorption correction: empirical (using intensity measurements)
(SADABS; Sheldrick, 1996)
326 reflections with I > 2σ(I)
Tmin = 0.16, Tmax = 0.27Rint = 0.024
769 measured reflections
Refinement top
R[F2 > 2σ(F2)] = 0.0281 restraint
wR(F2) = 0.072Δρmax = 2.68 e Å3
S = 1.17Δρmin = 1.85 e Å3
330 reflectionsAbsolute structure: Refined as an inversion twin (Flack, 1983)
23 parametersAbsolute structure parameter: 0.31 (3)
Special details top

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. Refined as an inversion twin.

Fractional atomic coordinates and isotropic or equivalent isotropic displacement parameters (Å2) top
xyzUiso*/Ueq
Au0.00000.21650 (14)0.68259 (7)0.0106 (5)
Sn0.00000.3076 (4)0.0130 (3)0.0163 (6)
Ca10.50000.50000.8058 (15)0.0083 (18)
Ca20.00000.50000.3876 (16)0.0109 (19)
Atomic displacement parameters (Å2) top
U11U22U33U12U13U23
Au0.0111 (6)0.0074 (6)0.0133 (6)0.0000.0000.0007 (7)
Sn0.0145 (14)0.0191 (10)0.0153 (13)0.0000.0000.0004 (9)
Ca10.010 (5)0.006 (4)0.009 (4)0.0000.0000.000
Ca20.014 (6)0.007 (4)0.012 (5)0.0000.0000.000
Geometric parameters (Å, º) top
Au—Sni2.6282 (13)Ca1—Snxvi3.103 (7)
Au—Snii2.6282 (13)Ca1—Sniii3.103 (7)
Au—Sniii2.663 (3)Ca1—Snxvii3.103 (7)
Au—Ca23.067 (9)Ca1—Snii3.171 (9)
Au—Auiv3.090 (2)Ca1—Snxviii3.171 (9)
Au—Ca2v3.174 (6)Ca1—Auxix3.185 (4)
Au—Ca2vi3.174 (6)Ca1—Auxii3.185 (4)
Au—Ca1vii3.185 (4)Ca1—Auxx3.185 (4)
Au—Ca13.185 (4)Ca1—Auxviii3.325 (11)
Au—Ca1viii3.325 (11)Ca1—Auii3.325 (11)
Sn—Auix2.6282 (13)Ca2—Auxii3.067 (9)
Sn—Aux2.6282 (13)Ca2—Aux3.174 (6)
Sn—Auxi2.663 (3)Ca2—Auxxi3.174 (6)
Sn—Snxii2.746 (5)Ca2—Auxxii3.174 (6)
Sn—Ca1xiii3.103 (7)Ca2—Auix3.174 (6)
Sn—Ca1xi3.103 (7)Ca2—Snxii3.233 (12)
Sn—Ca1viii3.171 (9)Ca2—Snxviii3.301 (4)
Sn—Ca23.233 (12)Ca2—Sni3.301 (4)
Sn—Ca2viii3.301 (4)Ca2—Snii3.301 (4)
Sn—Ca2xiv3.301 (4)Ca2—Snxxiii3.301 (4)
Ca1—Snxv3.103 (7)
Sni—Au—Snii118.87 (9)Snxv—Ca1—Auxix50.09 (5)
Sni—Au—Sniii120.33 (5)Snxvi—Ca1—Auxix85.44 (6)
Snii—Au—Sniii120.33 (5)Sniii—Ca1—Auxix163.2 (3)
Sni—Au—Ca270.38 (8)Snxvii—Ca1—Auxix113.27 (9)
Snii—Au—Ca270.38 (8)Snii—Ca1—Auxix102.8 (3)
Sniii—Au—Ca2124.60 (17)Snxviii—Ca1—Auxix48.85 (10)
Sni—Au—Auiv86.25 (6)Au—Ca1—Auxix144.8 (4)
Snii—Au—Auiv86.25 (6)Snxv—Ca1—Auxii113.27 (9)
Sniii—Au—Auiv104.13 (6)Snxvi—Ca1—Auxii163.2 (3)
Ca2—Au—Auiv131.27 (15)Sniii—Ca1—Auxii85.44 (6)
Sni—Au—Ca2v146.78 (8)Snxvii—Ca1—Auxii50.09 (5)
Snii—Au—Ca2v66.97 (18)Snii—Ca1—Auxii102.8 (3)
Sniii—Au—Ca2v68.2 (2)Snxviii—Ca1—Auxii48.85 (10)
Ca2—Au—Ca2v134.46 (14)Au—Ca1—Auxii78.87 (11)
Auiv—Au—Ca2v60.88 (7)Auxix—Ca1—Auxii90.57 (13)
Sni—Au—Ca2vi66.97 (18)Snxv—Ca1—Auxx85.44 (6)
Snii—Au—Ca2vi146.78 (8)Snxvi—Ca1—Auxx50.09 (5)
Sniii—Au—Ca2vi68.2 (2)Sniii—Ca1—Auxx113.27 (9)
Ca2—Au—Ca2vi134.46 (14)Snxvii—Ca1—Auxx163.2 (3)
Auiv—Au—Ca2vi60.88 (7)Snii—Ca1—Auxx48.85 (10)
Ca2v—Au—Ca2vi91.0 (2)Snxviii—Ca1—Auxx102.8 (3)
Sni—Au—Ca1vii65.30 (16)Au—Ca1—Auxx90.57 (13)
Snii—Au—Ca1vii143.71 (12)Auxix—Ca1—Auxx78.87 (11)
Sniii—Au—Ca1vii63.4 (2)Auxii—Ca1—Auxx144.8 (4)
Ca2—Au—Ca1vii78.95 (14)Snxv—Ca1—Auxviii48.12 (15)
Auiv—Au—Ca1vii129.44 (6)Snxvi—Ca1—Auxviii75.1 (2)
Ca2v—Au—Ca1vii131.5 (4)Sniii—Ca1—Auxviii75.1 (2)
Ca2vi—Au—Ca1vii69.50 (12)Snxvii—Ca1—Auxviii48.12 (15)
Sni—Au—Ca1143.71 (12)Snii—Ca1—Auxviii163.9 (3)
Snii—Au—Ca165.30 (16)Snxviii—Ca1—Auxviii108.51 (7)
Sniii—Au—Ca163.4 (2)Au—Ca1—Auxviii124.3 (2)
Ca2—Au—Ca178.95 (14)Auxix—Ca1—Auxviii88.43 (13)
Auiv—Au—Ca1129.44 (6)Auxii—Ca1—Auxviii88.43 (13)
Ca2v—Au—Ca169.50 (12)Auxx—Ca1—Auxviii124.3 (2)
Ca2vi—Au—Ca1131.5 (4)Snxv—Ca1—Auii75.1 (2)
Ca1vii—Au—Ca190.57 (14)Snxvi—Ca1—Auii48.12 (15)
Sni—Au—Ca1viii61.51 (5)Sniii—Ca1—Auii48.12 (15)
Snii—Au—Ca1viii61.51 (5)Snxvii—Ca1—Auii75.1 (2)
Sniii—Au—Ca1viii166.45 (12)Snii—Ca1—Auii108.51 (7)
Ca2—Au—Ca1viii69.0 (2)Snxviii—Ca1—Auii163.9 (3)
Auiv—Au—Ca1viii62.31 (10)Au—Ca1—Auii88.43 (13)
Ca2v—Au—Ca1viii102.76 (15)Auxix—Ca1—Auii124.3 (2)
Ca2vi—Au—Ca1viii102.76 (15)Auxii—Ca1—Auii124.3 (2)
Ca1vii—Au—Ca1viii124.3 (2)Auxx—Ca1—Auii88.43 (13)
Ca1—Au—Ca1viii124.3 (2)Auxviii—Ca1—Auii55.4 (2)
Auix—Sn—Aux118.87 (9)Auxii—Ca2—Au82.5 (3)
Auix—Sn—Auxi118.23 (5)Auxii—Ca2—Aux134.46 (13)
Aux—Sn—Auxi118.23 (5)Au—Ca2—Aux93.35 (6)
Auix—Sn—Snxii93.75 (6)Auxii—Ca2—Auxxi93.35 (6)
Aux—Sn—Snxii93.75 (6)Au—Ca2—Auxxi134.46 (13)
Auxi—Sn—Snxii104.13 (6)Aux—Ca2—Auxxi119.4 (4)
Auix—Sn—Ca1xiii156.94 (10)Auxii—Ca2—Auxxii93.35 (6)
Aux—Sn—Ca1xiii70.37 (16)Au—Ca2—Auxxii134.46 (13)
Auxi—Sn—Ca1xiii66.55 (19)Aux—Ca2—Auxxii58.25 (13)
Snxii—Sn—Ca1xiii63.74 (7)Auxxi—Ca2—Auxxii91.0 (2)
Auix—Sn—Ca1xi70.37 (16)Auxii—Ca2—Auix134.46 (13)
Aux—Sn—Ca1xi156.94 (10)Au—Ca2—Auix93.35 (6)
Auxi—Sn—Ca1xi66.55 (19)Aux—Ca2—Auix91.0 (2)
Snxii—Sn—Ca1xi63.74 (7)Auxxi—Ca2—Auix58.25 (13)
Ca1xiii—Sn—Ca1xi93.7 (3)Auxxii—Ca2—Auix119.4 (4)
Auix—Sn—Ca1viii65.84 (7)Auxii—Ca2—Sn163.9 (3)
Aux—Sn—Ca1viii65.84 (7)Au—Ca2—Sn113.61 (8)
Auxi—Sn—Ca1viii122.06 (18)Aux—Ca2—Sn48.42 (14)
Snxii—Sn—Ca1viii133.81 (16)Auxxi—Ca2—Sn75.5 (2)
Ca1xiii—Sn—Ca1viii133.07 (11)Auxxii—Ca2—Sn75.5 (2)
Ca1xi—Sn—Ca1viii133.07 (11)Auix—Ca2—Sn48.42 (14)
Auix—Sn—Ca264.61 (6)Auxii—Ca2—Snxii113.61 (8)
Aux—Sn—Ca264.61 (6)Au—Ca2—Snxii163.9 (3)
Auxi—Sn—Ca2169.01 (14)Aux—Ca2—Snxii75.5 (2)
Snxii—Sn—Ca264.88 (11)Auxxi—Ca2—Snxii48.42 (14)
Ca1xiii—Sn—Ca2106.53 (16)Auxxii—Ca2—Snxii48.42 (14)
Ca1xi—Sn—Ca2106.53 (16)Auix—Ca2—Snxii75.5 (2)
Ca1viii—Sn—Ca268.9 (2)Sn—Ca2—Snxii50.2 (2)
Auix—Sn—Ca2viii134.14 (13)Auxii—Ca2—Snxviii48.58 (11)
Aux—Sn—Ca2viii61.05 (16)Au—Ca2—Snxviii102.4 (3)
Auxi—Sn—Ca2viii63.2 (2)Aux—Ca2—Snxviii164.2 (3)
Snxii—Sn—Ca2viii131.67 (7)Auxxi—Ca2—Snxviii48.51 (4)
Ca1xiii—Sn—Ca2viii68.86 (12)Auxxii—Ca2—Snxviii108.36 (8)
Ca1xi—Sn—Ca2viii129.7 (4)Auix—Ca2—Snxviii89.12 (6)
Ca1viii—Sn—Ca2viii75.76 (15)Sn—Ca2—Snxviii123.4 (3)
Ca2—Sn—Ca2viii123.4 (3)Snxii—Ca2—Snxviii89.22 (13)
Auix—Sn—Ca2xiv61.05 (16)Auxii—Ca2—Sni102.4 (3)
Aux—Sn—Ca2xiv134.14 (13)Au—Ca2—Sni48.58 (11)
Auxi—Sn—Ca2xiv63.2 (2)Aux—Ca2—Sni48.51 (4)
Snxii—Sn—Ca2xiv131.67 (7)Auxxi—Ca2—Sni164.2 (3)
Ca1xiii—Sn—Ca2xiv129.7 (4)Auxxii—Ca2—Sni89.12 (6)
Ca1xi—Sn—Ca2xiv68.86 (12)Auix—Ca2—Sni108.36 (8)
Ca1viii—Sn—Ca2xiv75.76 (15)Sn—Ca2—Sni89.22 (13)
Ca2—Sn—Ca2xiv123.4 (3)Snxii—Ca2—Sni123.4 (3)
Ca2viii—Sn—Ca2xiv86.54 (14)Snxviii—Ca2—Sni145.5 (4)
Snxv—Ca1—Snxvi52.52 (15)Auxii—Ca2—Snii102.4 (3)
Snxv—Ca1—Sniii117.1 (4)Au—Ca2—Snii48.58 (11)
Snxvi—Ca1—Sniii93.7 (3)Aux—Ca2—Snii108.36 (8)
Snxv—Ca1—Snxvii93.7 (3)Auxxi—Ca2—Snii89.12 (6)
Snxvi—Ca1—Snxvii117.1 (4)Auxxii—Ca2—Snii164.2 (3)
Sniii—Ca1—Snxvii52.52 (15)Auix—Ca2—Snii48.51 (4)
Snxv—Ca1—Snii133.07 (11)Sn—Ca2—Snii89.22 (13)
Snxvi—Ca1—Snii94.03 (5)Snxii—Ca2—Snii123.4 (3)
Sniii—Ca1—Snii94.03 (5)Snxviii—Ca2—Snii83.34 (14)
Snxvii—Ca1—Snii133.07 (11)Sni—Ca2—Snii86.55 (14)
Snxv—Ca1—Snxviii94.03 (5)Auxii—Ca2—Snxxiii48.58 (11)
Snxvi—Ca1—Snxviii133.07 (11)Au—Ca2—Snxxiii102.4 (3)
Sniii—Ca1—Snxviii133.07 (11)Aux—Ca2—Snxxiii89.12 (6)
Snxvii—Ca1—Snxviii94.03 (5)Auxxi—Ca2—Snxxiii108.36 (7)
Snii—Ca1—Snxviii87.6 (3)Auxxii—Ca2—Snxxiii48.51 (4)
Snxv—Ca1—Au163.2 (3)Auix—Ca2—Snxxiii164.2 (3)
Snxvi—Ca1—Au113.27 (9)Sn—Ca2—Snxxiii123.4 (3)
Sniii—Ca1—Au50.09 (5)Snxii—Ca2—Snxxiii89.22 (13)
Snxvii—Ca1—Au85.44 (6)Snxviii—Ca2—Snxxiii86.55 (14)
Snii—Ca1—Au48.85 (10)Sni—Ca2—Snxxiii83.34 (14)
Snxviii—Ca1—Au102.8 (3)Snii—Ca2—Snxxiii145.5 (4)
Symmetry codes: (i) x1/2, y+1/2, z+1/2; (ii) x+1/2, y+1/2, z+1/2; (iii) x, y, z+1; (iv) x, y, z; (v) x+1/2, y1/2, z+1/2; (vi) x1/2, y1/2, z+1/2; (vii) x1, y, z; (viii) x1/2, y1/2, z1/2; (ix) x+1/2, y+1/2, z1/2; (x) x1/2, y+1/2, z1/2; (xi) x, y, z1; (xii) x, y+1, z; (xiii) x1, y, z1; (xiv) x+1/2, y1/2, z1/2; (xv) x+1, y+1, z+1; (xvi) x+1, y, z+1; (xvii) x, y+1, z+1; (xviii) x+1/2, y+1/2, z+1/2; (xix) x+1, y+1, z; (xx) x+1, y, z; (xxi) x+1/2, y+1/2, z1/2; (xxii) x1/2, y+1/2, z1/2; (xxiii) x1/2, y+1/2, z+1/2.

Experimental details

Crystal data
Chemical formulaCaAuSn
Mr355.74
Crystal system, space groupOrthorhombic, Imm2
Temperature (K)273
a, b, c (Å)4.5261 (7), 7.1356 (11), 7.8147 (11)
V3)252.39 (7)
Z4
Radiation typeMo Kα
µ (mm1)69.58
Crystal size (mm)0.03 × 0.02 × 0.02
Data collection
DiffractometerBruker SMART APEXII CCD area-detector
diffractometer
Absorption correctionEmpirical (using intensity measurements)
(SADABS; Sheldrick, 1996)
Tmin, Tmax0.16, 0.27
No. of measured, independent and
observed [I > 2σ(I)] reflections
769, 330, 326
Rint0.024
(sin θ/λ)max1)0.664
Refinement
R[F2 > 2σ(F2)], wR(F2), S 0.028, 0.072, 1.17
No. of reflections330
No. of parameters23
No. of restraints1
Δρmax, Δρmin (e Å3)2.68, 1.85
Absolute structureRefined as an inversion twin (Flack, 1983)
Absolute structure parameter0.31 (3)

Computer programs: SMART (Bruker, 2002), SAINT-Plus (Bruker, 2013), SHELXS97 (Sheldrick, 2008), SHELXL2013 (Sheldrick, 2008), DIAMOND (Brandenburg, 2000), SHELXTL2013 (Sheldrick, 2008).

 

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