1 Introduction

Titanium oxide is a well-known photocatalyst working in the ultraviolet (UV) region of light with a band gap of 3.2 eV. Numerous reports are available regarding the shifting of wavelength corresponding to the onset of absorption from UV to visible region of light in TiO2 as a consequence of doping with cationic or anionic dopants. Anionic dopants such as nitrogen, sulphur, carbon, and fluorine lead to narrowing of the band gap of TiO2 which results in visible light absorption and improved photo-catalytic activity [1–3]. Doping TiO2 with antimony and chromium results in the shifting of absorption band from UV to visible light region and exhibits photo-catalytic activity for O2 generation from aqueous silver nitrate solution under visible light irradiation [4]. TiO2 doped with Ce, V, Cu, Sn, Nd, Fe, Cr, or Co shows a red shift in the absorption band compared to pure TiO2, and considerable photo-catalytic activity under visible light irradiation [5–11]. Doping with lanthanide ions such as Eu3+, Pr3+ and Yb3+ in TiO2 was found to improve the photo-catalytic activity for the photo degradation of salicylic acid and t-cinnamic acid [12]. The enhanced degradation was attributed to the formation of Lewis acid–base complex between the lanthanide ions and the reactants at the photocatalyst interface. The photo-excited wavelength of the TiO2–SnO2 prepared by ball milling shows a red shift of 20 nm in its absorption spectrum and increase in the photo-catalytic activity for the degradation of monocrotophos compared to pure TiO2 [13]. The increased photo-catalytic activity was explained on the basis of the photo generated charge separation efficiency of the coupled TiO2–SnO2. Sensitization of Cu doped TiO2 with eosin improved the photo-catalytic activity for water splitting under visible light irradiation [7]. Doping TiO2 with 0.1 % Nd and impregnation with Pt produced enhanced photo-catalytic activity for water splitting due to the prevention of phase transformation of TiO2 from anatase to rutile and inhibition of particle growth [14]. Some recent studies have revealed that the oxygen deficient sites play a crucial role in the visible light induced photo-catalytic activity of TiO2. Ihara et al. [15] have reported that the low temperature H2 plasma treated TiO2 and nitrogen doped TiO2 [16] show visible light photo-catalytic activity due to the presence of oxygen deficient sites. Visible light absorption of TiO2, reduced in different polymeric media, originates from colour centers (defects associated with oxygen vacancies) rather than due to a narrowing of the original band gap of TiO2 [17]. Prokes et al. [18] have proposed that the visible light absorption of titanium oxynitride is due to the oxygen hole centre created during the surface modification process by nitrogen near the surface of the nano colloid. The visible light photo-catalytic activity observed due to the oxygen vacancies in TiO2 is found to decrease after an optimum value [19].

Among the advantages of titania as a photocatalyst, its excellent (photo) chemical stability, low cost, and non-toxicity can be cited. However, its wide band-gap energy (ca. 3.0 eV for rutile and 3.2 eV for anatase) means that only 5 % of solar spectrum is used. Moreover, TiO2 presents a relatively high electron–hole recombination rate which is detrimental to its photoactivity. In this sense, doping with metals or metal oxides could make a double effect:

  1. 1.

    It could reduce the band gap energy, thus shifting the absorption band to the visible region.

  2. 2.

    Metals could provoke a decrease in electron–hole recombination rate, acting as electron traps.

In our previous research we studied the effect of doping Sn (up to 30 mol%) and Nb (up to 20 mol%) on photo-catalytic behavior of titania based thin films. We found that 15 mol% of Sn and 1 mol% on Nb shows the most significant improvement on photo-catalytic behavior of TiO2 under UV irradiation [20, 21]. In the present study, Sn and Nb have been selected as co dopnats to increase the photo-catalytic activity of thin films at the solar light wavelengths. The thin films were applied by sol–gel dip-coating process. The effect of the dopant cations on the structure and the phase stability was studied in a systematic way. The efficiency of these samples as photocatalysts for the degradation of MB, as organic compound model, under solar excitation, was investigated.

2 Experimental procedures

2.1 Preparation of the thin films

The preparation of precursor solution for Sn/Nb co-doped TiO2 thin films is described as follows: TiO2, SnO2 and Nb2O5 sols were prepared, separately. For the preparation of TiO2 sol, titanium (IV) butoxide (TBT = Ti (OC4H9)4, Aldrich) was selected as titanium source. First, 0.35 mol ethanol (EtOH, Merck) and 0.04 mol ethyl acetoacetate (EAcAc is as a sol stabilizer during preparation of sol and also chelating agent during coating, Merck) were mixed, and then 0.01 mol TBT was added by the rate of 1 ml/min to the mixture at the ambient temperature (25 °C). The solution was continuously stirred for 45 min, followed by the dropping of HNO3 as catalyst to the solution until pH of 3. De-ionized water was added to the solution slowly to initiate hydrolysis process. Solution was aged for 24 h in order to complete all reactions. The chemical composition of the resultant alkoxide solution was TBT:H2O:HNO3:EAcAc:EtOH = 1:10:1:4:35 in molar ratio. In order to prepare SnO2·sol and Nb2O5·sol, stannous chloride (SnCl2·2H2O, Merck) and Niobium chloride were dissolved in EtOH with molar ratio of SnCl2·2H2O:EtOH = 1:35 and NbCl5:EtOH = 2:35 at ambient temperature with continuous stirring. Solutions were aged for 24 h in order to complete all reactions. Then, mixtures of TiO2, SnO2, and Nb2O5 were made with different mol ratios of Sn and Nb (Ti-15 %Sn-1 %Nb) at the ambient temperature. The Sn/Nb co-doped thin films were applied on the glazed porcelain substrates with the prepared sol solutions by dipping-withdrawing at room temperature with withdrawal speed of 10 mm/min.

The porcelain substrate composition was Al2O3: 45.12, SiO2: 43.83, BaO: 6.18, K2O: 3.63, Na2O: 0.58, MgO: 0.39, CaO: 0.27 wt%. Glazed composition contained SiO2: 64.45, Al2O3: 16.56, CaO: 6.07, K2O: 5.1 MgO: 4.36, Fe2O3: 3.46 wt%. Porcelain and glaze compositions were reported by substrate manufacturer with formal report.

Substrate dimensions were 30 × 15 × 1 mm. The substrates were degreased in ethanol and cleaned in de-ionized water for 15 min and acetone with supersonic wave. The treated substrate samples were dried at 80 °C for 1 h. In order to prevent diffusion of porcelain substrate and glaze elements to final thin film, one interlayer (buffer layer) SiO2 thin film with withdrawal speed of 10 mm/min was applied. Silica sol contains tetra ethyl orthosilicate (TEOS, Merck): EtOH:H2O:HCl with 1:3.8:1:0.01 molar ratios and calcined at 400 °C for 1 h. Samples were dried at 100 °C for 1 h after each coating cycle and finally heated at a rate of 2 °C/min and calcined at 475 °C for 1 h in air atmosphere.

Substrates were coated with one SiO2 (buffer layer) and two Sn/Nb co-doped TiO2 layers.

2.2 Characterization methods

Differential thermal analysis (DTA) and thermogravimetric (TG) were used in order to determine crystallization temperature with a heating rate of 10 °C/min (STA 1,460 equipment). XRD pattern and phase identification of thin films were recorded using X-ray diffraction analysis (Philips, MPD-XPERT, λ: Cukα = 0.154 nm). The samples were scanned in the 2θ range of 20–70°. Morphology of the thin films was observed using scanning electron microscopy (SEM, XL30 Series) with an accelerating voltage of 10–15 kV. X-ray photoelectron spectroscopy (XPS) spectra were recorded by a PHI 5000C ESCA spectrometer using Mg Ka radiation (hυ = 1,253.6 eV). The pressure of the analyzer chamber was maintained at 5 × 10−8 Pa. Spectra were calibrated with respect to the C1s peak at 284.6 eV.

N2 adsorption–desorption isotherms were determined in a surface analyzer equipment (BEL Japan Inc., Osaka, Japan) at 77 K. BET surface area and BJH analyses were used to determine the total specific surface area and the pore size distribution.

In order to make TEM foils, the films were removed from the substrates by water flotation. Droplets of the sol–gel material were also deposited on plain (un-coated) copper grids so as to form free-standing films for in situ hot-stage experiments in the TEM. Conventional TEM imaging and electron diffraction analysis was carried out using an EM-2100F-JEOL-Tokyo-Japan with acceleration voltage of 200 kV.

2.3 Photo-catalytic activity measurement

The photo-catalytic activity was evaluated by monitoring the degradation of MB solution (5 ppm) under UV and solar illumination. The samples were placed in 20 ml aqueous MB solution and were kept in dark for 2 h. They were then irradiated from top using a UV lamp (Philips 8 W, 360 nm) and solar irradiation (the total accumulated UV light (350–400 nm) and the total accumulated visible light (400–750 nm) were 6.786 and 78.834 kJ/L, respectively) using costume made apparatus. The intensity of the MB characteristic band at 660 nm (I660) in the obtained UV–vis spectrum (Varian cary 50 spectrophotometer) was used to determine the concentration of MB in the solution (Ct).

The degradation rate of MB, which represents the photo-catalytic efficiency of the films, can be determined by Eq. 1.

$$ d(\% ) = \left( {C_{0} - C_{t} } \right)/C_{0} \times 100 $$
(1)

Where d is degradation rate, Ct is concentration after radiation and C0 is concentration before radiation [22].

3 Results and discussion

Figure 1 shows the XRD patterns of the films without and with Sn, Nb dopant heat treated at 475 °C for 1 h. X-ray diffraction peak at 25.5° corresponds to characteristic peak of crystal plane (1 0 1) of anatase, at 27.6° corresponds to characteristic peak of crystal plane (1 1 0) of rutile in films. According to the XRD patterns, the pure TiO2 (T) constituted of pure anatase phase.

Fig. 1
figure 1

XRD spectra of the pure and doping TiO2 films

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All thin films were identified as the mixture polymorphs of anatase (JCPDS: No. 21-1272) and rutile (JCPDS: No.21-1276), without any impurity phase. In the phase composition, anatase appeared as the main phase, and rutile crystallization was promoted by Sn4+ doping but was inhibited by Nb5+ doping. With the addition of Sn 15 % and Nb 1 %, the intensity of the (101) diffraction peak became weaker than that of the pure TiO2 film, suggesting that the film with Sn and Nb co-doping experienced lower crystallization. Other co-doped samples were also rutile TiO2 and no signs of metal or oxide phases of Tin or Niobium were detected. This suggests the incorporation of Sn4+ and Nb5+ in TiO2 lattice [23, 24].

The diffraction peaks of rutile crystallites appeared in X-ray profiles with increasing Sn dopant in thin films. The addition of Sn has a promoting effect on the transformation of anatase to rutile crystalline phase [25, 26], due to the rutile like structure of SnO2-cassiterite phase. It is also found that the peak position of (1 0 1) anatase and (1 1 0) rutile planes shift to a smaller diffraction angle with increasing Sn content in TiO2 thin films. This may results from the exchange of Ti with Sn in the TiO2 lattice.

The average crystallite size of thin films (D) was determined from the XRD patterns, according to the Scherrer Eq. (2) [27]

$$ D = {{k\lambda } \mathord{\left/ {\vphantom {{k\lambda } {\beta \,\cos \,\theta }}} \right. \kern-0pt} {\beta \,\cos \,\theta }} $$
(2)

where k is a constant (shape factor, about 0.9), λ the X-ray wavelength (0.154 nm), β the full width at half maximum (FWHM) of the diffraction peak, and θ is the diffraction angle. The values of β and θ of anatase and rutile phases were taken from anatase (1 0 1) and rutile (1 1 0) planes diffraction lines, respectively.

The amount of rutile in the samples was calculated using the following equation [28]

$$ X_{R} = (1 + 0.8{{I_{A} } \mathord{\left/ {\vphantom {{I_{A} } {I_{R} }}} \right. \kern-0pt} {I_{R} }})^{ - 1} $$
(3)

where XR is the mass fraction of rutile in the samples, and IA and IR are the X-ray integrated intensities of (101) reflection of the anatase and (110) reflection of rutile, respectively. The diffraction peaks of crystal planes (101) (200), and (105) of Anatase phase in XRD patterns were selected to determine the lattice parameters of the TiO2 and doped TiO2 thin films. The lattice parameters were obtained by using the Eq. (4) [27]

$$ \begin{gathered} (Bragg's\,law):2d_{(hkl)} \sin \theta = {{\uplambda}} \hfill \\ ({1 \mathord{\left/ {\vphantom {1 {d_{(hkl)} }}} \right. \kern-0pt} {d_{(hkl)} }})^{2} = ({h \mathord{\left/ {\vphantom {h a}} \right. \kern-0pt} a})^{2} + ({k \mathord{\left/ {\vphantom {k b}} \right. \kern-0pt} b})^{2} + ({l \mathord{\left/ {\vphantom {l c}} \right. \kern-0pt} c})^{2} \hfill \\ \end{gathered} $$
(4)

where d (hkl) is the distance between the crystal planes of (hkl); λ is the wavelength of X-ray used in the experiment; θ is the diffraction angle of the crystal plane (hkl); hkl is the crystal plane index; and a, b, and c are lattice parameters (in Anatase form, a = b ≠ c).

The characteristic of all thin films after thermal treatment at 475 °C is reported at Table 1. By increasing Sn dopant, transformation of anatase to rutile phase was promoted, the amount of rutile phase structure was increased, and a decrease in the crystalline size was detected. The decrease in crystal size can be attributed to the presence of Sn–O–Ti in the Sn-doped TiO2 thin films which inhibits the growth of crystal grains [29].

Table 1 The characteristic of dip-coated thin films after thermal treatment at 475 °C
Full size table

Compared with those of pure TiO2 films, for doped TiO2 films, average anatase crystallite sizes decreased. It is found that the Nb dopants can inhibit the anatase grain growth. The Nb5+ radius (0.70 Å) is slightly bigger than Ti4+ radius (0.64 Å) and this means that Nb5+ induces slight stress in TiO2 lattice, which may hinder the growth of the TiO2 crystallites as was found by Sharma and Bhatnagar [23].

Also, the lattice parameters and cell volume of the TiO2 and doped TiO2 thin films are summarized in Table 1.

It is obvious that the lattice parameters and cell volume of the doped TiO2 thin films increase with increasing amount of Sn an Nb substitution for Ti4+ in titania lattice.

XPS is a highly sensitive technique of surface analysis, and is an effective method to investigate the surface composition and chemical states of solid samples. XPS measurements were carried out to determine the surface composition and chemical state of Sn/Nb co-doped TiO2 thin film calcined at 475 °C. The XPS survey spectrum in Fig. 2 demonstrates the presence of titanium, oxygen, carbon, tin, and Nb on the surface (Fig. 2a). All the binding energies were referenced to the adventitious C 1s peak at 284.6 eV.

Fig. 2
figure 2

XPS analysis of calcined Sn/Nb co-doped TiO2 thin film. a Survey analysis (Broad scan), b Ti 2p, c Sn 3d, d Nb 3d

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The binding energy of Ti 2p3/2 and Ti 2p1/2 were observed at approximately 458.8 and 464.1 eV, respectively, indicating that the Ti element mainly existed as the chemical state of Ti4+ [30]. XPS spectra of Sn 3d region are given in Fig. 2c. Two peaks corresponding to Sn 3d5/2 and Sn 3d3/2 are observed. The peak position corresponding to Sn 3d5/2 is located between those of Sn 3d5/2 in SnO2 (486.5 eV) and Sn 3d5/2 in metallic Sn (485.0 eV), which is ascribed to incorporated Sn4+ in the lattice of TiO2 [31].

Figure 2d shows the Nb 3d spectrum for the doped film exhibiting two peaks at 206.3 and 208.8 eV [32]. The peaks represent the 3d5/2 and 3d3/2 components, respectively, with a spin–orbit splitting of 2.5 eV. The center of the Nb 3d3/2 peak corresponds to that of Nb5+ oxidation state.

The nitrogen adsorption–desorption isotherm at 77 K and the BJH pore size distribution of sample calcined at 475 °C are showed in Fig. 3. It can be observed that the sample exhibits the classical shape of a type IV isotherm according to the IUPAC classification, typical for mesoporous solids [33]. The existence of the hysteresis loop in the isotherms is due to the capillary condensation of N2 gas occurring in the mesopores. The surface area and the mean pore diameter of co-doped film calcined at 475 °C are 262.34 m2/g and 5.7 nm, respectively.

Fig. 3
figure 3

Nitrogen adsorption–desorption isotherm

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Table 2 shows the results from surface area measurements of the different samples. As can be seen, the co-doped TiO2 film has larger surface area.

Table 2 Surface area measurement of the different samples
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Figure 4 shows the UV–vis spectra of the pure TiO2 and the doped TiO2 thin films deposited on glazed porcelain substrates in the wavelength range of 250–600 nm. In this figure, the absorption edge of Sn-doped TiO2 thin films shifts towards longer wavelengths, whereas absorption edge of Nb-doped TiO2 thin films shifts towards shorter wavelengths. It indicates a decrease (Sn doping) or increase (Nb doping) in the energy band gap (inset in Fig. 4).

Fig. 4
figure 4

UV–vis absorption spectra of pure TiO2 and doped thin films deposited on glazed porcelain substrate (calcined at 475 °C) with calculated energy band gaps of samples

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The energy band gap corresponds to the absorption limit and can be roughly evaluated by using following equation:

$$ E_{g} = \frac{1240}{{\lambda_{edge} }}(eV) $$
(5)

where λedge represents the absorption limit of the semiconductor. λedge can be extracted from the absorption spectrum by carrying out the first derivative of absorbance with respect to wavelength near the absorption edge and finding the point at which the derivative spectrum reaches its minimum value. This point is actually the reflection point of the absorption curve. The tangent line of the absorption curve at the reflection point intersects with the x-axis on which absorbance reaches 0 and indicates λedge.

Doping Sn4+ has been found to be located approaching and below the conduction band [8]. Therefore, the red shift of the absorption edge for the Sn-doped TiO2 should be the result of the electronic transition from the valance band to the doping energy level. On the other hand, according to the XRD results, doping with Sn had accelerated the transformation from anatase to rutile phase of TiO2, and the rutile phase has a band gap smaller than that of anatase, so this transformation should be another reason for the red shift.

The band gap of the pure TiO2 thin film was about 3.22 eV and had increased to 3.25 eV with increasing Nb content. The widening of the band gap can be explained by the Burstein-Moss (BM) effect [34], in which the lowest states in the conduction band were blocked, and transitions can take place only to energies higher than Fermi energy. Thus, the band gap became widened with increasing Nb content. The observed values were higher than the band gap of both bulk and thin film TiO2 in the anatase phase. The reported values were 3.18 eV [35] for bulk material and in the range 3.2–3.23 eV for thin films [36].

The absorption spectrum of co-doped TiO2 shows that co-doping not only leads to a red-shift of absorption edge but also significantly enhances the absorption of visible light. The absorption of Sn/Nb co-doping samples in visible region is much higher than those of single doped samples (Nb-doped TiO2) and lesser than Sn-doped TiO2.

Figure 5 shows the normalized concentration at 660 nm absorption of the MB solutions separated from the TiO2 thin film as a photocatalyst under various time irradiations (0–120 min) to determine the photo-catalytic degradation: a under the UV irradiation and b under the visible light irradiation.

Fig. 5
figure 5

Normalized concentration at 660 nm absorption of the MB solutions under various time irradiations, a under the UV irradiation and b under the sun light irradiation

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According to Figure 5a, the order of photo-catalytic activity of TiO2 thin films at 120 min under the UV irradiation was as following: T-15 %Sn-1 %Nb > T-1 %Nb > T-15 %Sn > T, but under the sun light irradiation (Fig. 5b), was T-15 %Sn-1 %Nb > T-15 %Sn > T-1 %Nb > T which suggests that the doping enhances the photo-catalytic activity of TiO2 under both conditions. Non-doped Titania has lowest response in all irradiation ranges. T coatings have better response under UV light because of Eg around 3.22 eV. This energy band is in UV light range. Near 90.4 % of MB was decomposed in the presence of T-15 %Sn-1 %Nb film after UV irradiation for 120 min, while the values in the presence of T-1 %Nb, T-15 %Sn and T film are 76.2, 42.4 and 36.4 %, respectively. Also, photo-catalytic activity of TiO2 thin films at 120 min under the sun light irradiation obtained 96.5, 78.1, 37.8 and 24.7 % in the presence of T-15 %Sn-1 %Nb, T-15 %Sn, T-1 %Nb and T thin film, respectively.

Some studies indicated that the photo-catalytic activity of TiO2 catalysts depends strongly on two factors: adsorption behavior and the separation efficiency of electron–hole pairs [37, 38]. On the one hand, the BET results showed that the specific surface areas of the catalysts increased from 85.93 m2/g for undoped TiO2 to 262.34 m2/g for co-doped TiO2, significantly (shown in Table 2). The larger specific surface area of co-doped TiO2 catalysts would be beneficial to achieve better adsorption of MB in aqueous suspension. Therefore, the increase of dopant content seems to be helpful for the photo-catalytic activity. According to Fig. 5 and Table 2, the photo-catalytic reactivity of doped TiO2 thin film is higher than that of undoped TiO2, which is consistent with the larger specific surface area of doped TiO2 than undoped TiO2.

The increase in photoactivity may be attributed to the combination of different processes: (1) decrease of the energy gap favoring higher photo excitation efficiency under solar radiation, and giving rise to a larger population of excited species (hole–electron pairs); (2) the small particles size favoring the increase in the surface per volume ratio, the scavenging action of photogenerated electrons by Sn4+ or Nb5+ ions thus preventing the recombination of electron–hole pairs and increasing the lifetime of charge carriers, so that they can take part in photo-catalytic processes; (3) the doping ions Sn4+ or Nb5+ can act as electron traps, thus facilitating the electron–hole separation and subsequent transfer of trapped electron to the adsorbed O2 which acts as an electron acceptor on the surface of the TiO2; (4) the dopant contribute to prevent the recombination of electron–hole pairs, increasing the lifetime of charge carriers, so that they can take part in photo-catalytic processes. Higher photo-catalytic behavior of Sn/Nb codoped thin film can be the result of higher specific surface area and a band gap in visual and UV wave lengths ranges. Based on Fig. 5a, under UV irradiation T-1 %Nb has better decomposition ability than T-15 %Sn while T-15 %Sn has better decomposition ability under sun light irradiation. This can be caused by higher sun light absorbance of T-15 %Sn and higher UV light absorbance on T-1 %Nb.

TEM micrographs of T-15 %Sn-1 %Nb thin film are shown in Fig. 6a. Surface was consisted of highly dense and uniform nanocrystalline TiO2, with a porous structure and particle size around 10 nm. This figure also shows formation of crack-free thin film on glazed porcelain substrate.

Fig. 6
figure 6

a TEM image and b FE-SEM cross-section image of T-15 %Sn-1 %Nb the thin film calcined at 475 °C for 1 h

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Figure 6b shows the cross-section image of the prepared coating captured by FE-SEM. As the figure shows, the thickness of thin film is about 200 nm. Thin film structure shows a parallel columnar like structure.

TEM images for Sn/Nb co-doped TiO2 thin film is shown in Fig. 7. As seen, both rutile and anatase grains were detected in TEM bright field image. The fringe spacing (d) of (101) crystallographic plane is 3.5 Å for undoped TiO2 film [20] and is detected to be 3.55 Å for co-doped TiO2. This implies that Sn4+ and Nb5+ ions are doped into TiO2 lattice in substitutional space in co-doped TiO2, since the ionic radius of Sn4+ (0.71 Å) and the ionic radius of NB5+ (0.7 Å) are larger than that of the lattice Ti4+ (0.6 Å), a fringe spacing of 3.37 Å corresponding to the (110) planes of rutile TiO2 is observed in co-doped TiO2. All of these are consistent with the aforementioned XRD results.

Fig. 7
figure 7

Bright field TEM image of Sn/Nb co-doped TiO2 thin film. SAED pattern from this sample is shown in the right panel (Anatase TiO2 (solid lines) and Rutile TiO2 (dotted lines) is shown in the inset)

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SAED pattern (Fig. 7-Top right) from a finely dispersed region of Sn/Nb co-doped sample showed continuous rings, which indicate the polycrystalline nature of thin film.

The detailed HR-TEM image analysis of Sn/Nb co-doped TiO2 thin film indicated uniformly substituted Sn and Nb in TiO2 structure. The Sn and Nb ions are incorporated into the structure of titania coatings, which has been confirmed by SAED analysis. No rings corresponding of secondary phases, like SnO2 or Nb2O5, were observed in SAED pattern for co-doped TiO2 samples.

4 Conclusion

In this research, Sn/Nb co-doped TiO2 thin films with photo-catalytic properties have been prepared by a sol–gel dip-coating method. The thickness of the applied thin films on porcelain substrates was about 200 nm. The photo-catalytic activity of the co-doped thin film is higher than that of pure TiO2 thin films. Sn4+ and Nb5+ substitution for Ti4+ in the titania lattice results in a decrease in the rate of photogenerated electron–hole recombination that is responsible for the enhancement in photo-catalytic degradation rate. The anatase to rutile phase transformation was promoted by Sn4+ doping but inhibited by Nb5+ doping. Photo-catalytic activity of the co-doped thin film under solar irradiation was improved comparing to single doped thin films.