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for Pd, [Eq. (1)], and (1Àz) for Pt, and these values were employed
in the catalyst nomenclature: Pd(z)Pt(1Àz). The suffixes -MicE, and
-IWI indicate the preparation method. For example, Pd(1.0)-MicE
stands for monometallic palladium prepared by the MicE method.
the photoelectron kinetic energy. The spectra were decomposed
with CasaXPS employing a Gaussian/Lorentzian (85/15) product
function after subtraction of a Shirley nonlinear sigmoid-type base-
line. The binding energy (BE) scale was corrected by using the C-
[C,H] component of the adventitious carbon peak at 284.8 eV as
a reference.[30] To determine the surface chemical state of palladi-
um, a contribution from metallic palladium (Pd0), Pd3d5/2 BEꢁ
335.0 eV,[25,37,40] and another from oxidized palladium (Pdd+),
Pd3d5/2 BE>335 eV,[18,25,36–37,40] were considered (Table S3). Peak de-
composition was performed with the following constraints: a) The
FWHM of all Pd components was fixed within the range 1.2–2.0 eV;
b) FWHM of Pd3d3/2 peaks=FWHM of Pd3d5/2 peaks, for the same
molPd
z ¼
ð1Þ
molðPd þ PtÞ
Crystallinity by XRD
An X-ray diffraction study was carried out with a Siemens D5000
diffractometer using CuKa radiation (l=1.5418 ). The 2q range
was scanned between 2 and 708 at a rate of 0.01 8sÀ1. The identifi-
cation of the crystalline phases was made with the ICDD-JCPDS da-
tabase after analyzing the recorded spectra with CasaXPS (Casa
Software Ltd.) where the position of the peaks and their full width
at half maximum (FWHM) was determined. A Gaussian/Lorentzian
(70/30) product function and a linear background were employed
for peak fitting. Catalysts were examined after preparation and
after reduction under the same conditions as the reaction tests.
XRD spectra were recorded at least twice to confirm the presence
of the identified crystalline phases. The Scherrer equation[26] was
employed for estimating the crystallite size of the detected phases.
considered species; c) area of Pd3d3/2 =2/3Pd3d5/2; d) a separa-
[36]
tion of 5.25 eV between the peaks Pd3d5/2 and Pd3d3/2
.
In addi-
tion, an asymmetry factor for Pd0 was introduced in the mathemat-
ical decomposition so as to reflect the asymmetry of the peak of
this species as observed in palladium foil samples.[25] Such a factor
corresponded to
a modified Gaussian/Lorentzian line shape:
A(0.25,0.25,0)GL(15) in CasaXPS. Finally, the contribution of elec-
trons coming from the Pt4d3/2 core level, BE=330–335 eV,[37] to the
Pd3d signal was not taken into account owing the very low inten-
sity of Pt4d3/2. Concerning platinum, the following constraints
were imposed for peak decomposition: a) the FWHM of the main
Pt4f7/2 peak was fixed within the range 1.5–2.0 eV; b) the FWHM of
the Pt4f5/2 peaks=FWHM of the Pt4f7/2 peaks; c) the area of the
Pt4f5/2 peaks=0.75area of the Pt4f7/2 peaks; d) a separation of
[25]
Nanoparticle identification, morphology, size, and composi-
tion by TEM
3.35 eV between Pt4f5/2 and Pt4f7/2
.
Although, as, in the case of
palladium, two species of platinum could be present on the sur-
face of the catalysts; namely, one corresponding to Pt0 with BE for
Pt4f7/2 <71 eV,[36,40] and another corresponding to Ptd+ with BE for
Pt4f7/2 >72,[36,40] it was considered reasonable to use only one
component owing to the low intensity of the signal and to peak
overlapping with the Ti 3s plasmon loss peak for the TiO2 support.
In the case of Pd(0.82)Pt(0.18)-IWI, it was not possible to add com-
ponents corresponding to platinum into the peak because the
signal from platinum was completely masked by the Ti 3s plasmon
loss peak. Selected XPS spectra of the Pd3d and Pt4f core levels
are presented in the Supporting Information (Figures S6–S9).
TEM measurements were performed with a JEOL JEM-2200FS/Cs-
corrected FEG TEM instrument operated at 200 kV and provided
with an in-column omega filter. Two modes or measurement were
employed: namely, high resolution (HRTEM) and scanning (STEM)
mode. The probe diameter was 0.5–1.0 nm. By combining STEM
with energy dispersive X-ray analysis (EDX), we performed a system-
atic measurement of the composition of the observed individual
metallic nanoparticles. On the basis of these measurements, Pd/
(Pd+Pt) molar ratios (zTEM) for the individual nanoparticles were
defined in the same fashion as in Equation (1). Similar approaches
have been previously presented in the literature.[23,27,28]
Catalytic tests
Chemical composition and oxidation state by XPS
The aerobic gas-phase oxidation of methanol was performed at at-
mospheric pressure in a metallic fixed-bed microreactor made of
an inconel tube of 1 cm internal diameter (PID ENG&Tech). The cat-
alytic bed (ꢀ0.5 cm3) was composed of 100 mg of catalyst powder
selected within the granular fraction 200–315 mm and diluted in
600 mg glass spheres that were previously confirmed inactive.
Before testing, all catalysts were treated under a 50 cm3 minÀ1 flow
of pure hydrogen (99.999%, Praxair) at 573 K (heating ramp=
10 KminÀ1) for 1 h, to reduce them under the same conditions.
After this treatment, the reactor was cooled down to the reaction
temperature: 323 K. The reactor feed consisted in 100 cm3 minÀ1 of
a gas mixture of 5 vol.% MeOH (anhydrous, 99.995%, Sigma–Al-
drich) and 2.5 vol.% O2 (99.999%, Praxair) diluted in He (99.999%,
Praxair). The gas mixture was prepared by passing the stream of
He through a container with liquid methanol, which was, in turn,
placed in a saturator maintained at 278 K. Once the flows of MeOH
and O2 were stable, as verified by carrying out several injections of
this stream into the online GC system, the reactants were allowed
into the reactor and the catalytic test was begun. Reaction prod-
ucts were analyzed each 30 min by using a CP3800 Varian GC pro-
vided with TCD detector. CP-Pora-PLOT Q (25 m; 0.53 mm) and CP-
Molsieve 5 (25 m; 0.53 mm) columns were used for the separa-
XPS measurements were carried out with an SSI-X-probe spectrom-
eter (SSX-100/206, Surface Science Instruments) equipped with
a monochromatic microfocused AlKa (1486.6 eV) X-ray source
(10 kV; 22 mA). Both the fresh and spent catalysts were analyzed.
At least three samples of the fresh catalysts were analyzed to test
the reproducibility of the measurements. Catalyst particles were
pressed into small stainless steel troughs mounted on a multi-
specimen ceramic sample holder. The analysis chamber was oper-
ated under ultrahigh vacuum with a pressure close to 510À7 Pa.
Charge stabilization was achieved by using an electron flood gun
adjusted at 8 eV and by placing a nickel grid 3 mm above the sam-
ples. The following sequence of spectra was recorded: general
spectrum, O1s, C1s+K2p, Ti 2p, P2p, Ca2p, Pd3d, Pt4f, and
C1s+K2p again to check the stability of charge compensation as
a function of time. General spectra were recorded at a pass energy
of 150 eV whereas the elements spectra were recorded at a pass
energy of 50 eV. The analyzed area was approximately 1.4 mm2 as
estimated from an elliptic spot of 1000 mm1700 mm. Surface
molar concentrations were calculated by correcting peak intensi-
ties with theoretical sensitivity factors based on Scofield cross sec-
tions[29] and the mean free path varying according to 0.7 power of
ChemCatChem 2016, 8, 1157 – 1166
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