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Topas c

Manufactured by Light Conversion
Sourced in Lithuania

TOPAS-C is a tunable optical parametric amplifier system designed for scientific research applications. It generates coherent, tunable radiation across a wide range of wavelengths, from the ultraviolet to the mid-infrared region of the electromagnetic spectrum. The system utilizes nonlinear optical processes to convert a fixed-wavelength laser input into a pair of tunable output beams.

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19 protocols using topas c

1

Time-resolved infrared spectroscopy of samples

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The time-resolved infrared spectroscopy measurements were performed using a setup described in detail previously,42 (link) and based on an amplified Ti:Sapphire system (Spectra-Physics, Solstice, 100 fs, 800 nm, 1 kHz). The pump pulses were generated from the second harmonic of the output of an optical parametric amplifier (Light Conversion, TOPAS-C). Probing was achieved using the output of an optical parametric amplifier (TOPAS C, Light Conversion) combined with a non-collinear difference-frequency-mixing module (NDFG, Light Conversion). These pulses were dispersed in a Triax 190 spectrograph (Horiba, 150 lines per mm) and detected with a 2 × 64 elements MCT array (Infrared Systems Development). The samples were flowed through a cell with CaF2 windows and a 500 μm spacer and had an absorbance of less than 0.3 at the excitation wavelength.
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2

Transient Absorption Spectroscopy of Excited-State Lifetimes

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Excited-state lifetimes were measured by transient absorption spectroscopy using a home built set up.54 (link) Pump-pulses with a temporal duration of 110 fs are generated by converting the fundamental of a Ti:Sapphire laser by a TOPAS C (Light Conversion Ltd). The pump pulse energy was adjusted to 100 μW at the sample position. The excited-state dynamics were probed by a white light supercontinuum, generated by focusing a small portion of the fundamental laser into a CaF2 plate. The polarisation between the pump beam and the probe beam was set to magic angle (54.7°). The samples were placed in a 1 mm cuvette with PBS as solvent. The sample concentration was adjusted to yield an OD between 0.1 and 0.2 at the excitation wavelength. To ensure sample integrity, absorption spectra of the samples were measured before and after each experiment.
The transient absorption data were analysed using the Python-based KiMoPack software. Prior to analysis, the data was chirp corrected and globally fit using a sum of exponentials.
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3

Ultrafast Transient Absorption Spectroscopy

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Absorption spectra of the samples were measured using a Shimadzu UV-3600 UV-VIS-NIR spectrophotometer. The sample morphology was investigated using a field emission SEM (FE-SEM; Carl Zeiss Ultra 55). Ultrafast transient absorption (TA) responses of the samples were measured using a pump–probe system described previously [20 (link),22 (link)]. Briefly, samples were excited at 695 nm (pump) by roughly 100 fs pulses at a repetition rate of 1 kHz (Libra F, Coherent Inc., coupled with Topas C, Light Conversion Ltd). White continuum probe pulses were generated by a small fraction of fundamental pulses produced by the generator (Libra F) focused on a sapphire crystal. The time-resolved transient absorption spectra were recorded using an ExciPro TA spectrometer (CDP, Inc.) in two wavelength ranges: 460–770 nm and 850–1050 nm. Home-developed software (decfit.py) was used to process and analyse the pump–probe measurements. The program carries out group velocity dispersion compensation, convolution with an instrument response function and a global data fit to a sum of exponential, stretched exponential and distributed decay functions [23 (link)].
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4

Transient absorption spectroscopy of colloidal quantum dots

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Transient absorption signal was recorded using the pump-probe setup described in our previous study35 (link). Laser pulses (800 nm, 80 fs pulse length, 1 kHz repetition rate) were generated by a regenerative amplifier (Spitfire XP) seeded by a femtosecond oscillator (Tsunami, both Spectra Physics).
Excitation pulses at the wavelength of 380, 390, 400, 420, 460, and 480 nm were acquired using an optical parametric amplifier (Topas C, Light Conversion). The used excitation photon flux at 480 nm was 1 × 1014 photons/cm2/pulse corresponds to <N> ~ 0.1 (the mean number of excited e-h pairs per QD). The intensity for all excitation wavelengths was adjusted to lead to approximately the same TA signal of the colloidal sample of 5–7.10−3 change in OD (measured in 1-mm static cell).
Probe pulses (broad supercontinuum spectrum) were generated from the 800-nm pulses in a sapphire plate and split by a beam splitter into probe pulse and a reference pulse. The probe pulse and the reference pulse were dispersed in a spectrograph and detected by two diode arrays (Pascher Instruments). The analysis of kinetics was done by averaging over 8 nm wide spectral bands of the probe spectra.
Thin film samples (typical OD of 0.02 at first exciton peak) were measured in a nitrogen atmosphere to avoid possible oxidation of QDs36 .
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5

Time-Resolved Photoluminescence Spectroscopy

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Excitation was performed with 100 fs pulses at 400 nm generated by frequency doubling part of the output of a standard 1 kHz Ti:Sapphire amplified system. The pump intensity on the sample was below 1 mJ cm−2. The gate pulses were at 1340 nm and were produced by an optical parametric amplifier (TOPAS-C, Light Conversion). Detection of the up-converted spectra was performed with a CCD camera (Andor, DV420ABU). The FWHM of the cross correlation of the gate with the solvent Raman signal was ~170 fs. Corrected time-resolved emission spectra were obtained by calibration with secondary emissive standards. The temporal chirp was determined measuring the instantaneous response of BBOT (Radiant Dyes) in all the solvents used.
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6

Ultrafast Transient Absorption Spectroscopy

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Transient absorption measurements were performed with a pump–probe differential spectrometer (Ultrafast Systems HELIOS-EOS), with both pump and probe wavelengths generated by a Ti:Sapphire regenerative amplifier (Coherent Libra-F-1K-HE-230), which delivers 100 fs long pulses at 800 nm with 1 KHz repetition rate. The main emission from the regenerative amplifier was split into two branches: one sent to an optical parametric amplifier (Light Conversion TOPAS C), in order to generate the pump wavelengths, and the other sent to the sapphire plate of the HELIOS spectrometer, where multi-color probe beam was generated by means of white light supercontinuum generation. The probe pulses were time delayed with respect to the pump pulses, by passing through a variable digitally controlled optical delay line. The pump and probe beams were then non-collinearly focused and overlapped on the sample surface, with the pump being chopped at 500 Hz, so that half of the transmission spectra were recorded with the pump on and half with pump off. The transmission spectra from the probe beam were recorded as a function of the relative delay time, by means of CCD spectrometers
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7

Ultrafast Transient Absorption Spectroscopy

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Transient absorption spectra were measured as described before. 38 Briefly, a modular laser system was used, consisting of an ultrafast Ti:sapphire regenerative amplifier (Spitfire Ace-100F, Spectra-Physics, USA) seeded with a Ti:sapphire oscillator (MaiTai SP, Spectra-Physics, USA), and pumped by Nd: YLF laser (Empower 30, Spectra-Physics, USA). The generated ∼100 fs pulses (800 nm) at 1 kHz repetition rate were divided into excitation and probe beams by a beam splitter. Tunable excitation pulses were generated by an optical parametric amplifier (TOPAS-C, Light Conversion, Lithuania). A 2 mm sapphire plate was used to generate a broadband (450-750 nm) white light pulse. The probe beam was focused to the sample, overlapping with the excitation beam. Probe and reference beams were then focused to the entrance slit of a spectrograph where the beams were dispersed onto a double CCD detection system (Pascher Instruments, Sweden). The time delay between the excitation and probe pulses was introduced by a computer-controlled delay line. The mutual polarisation of the excitation and probe beams was set to the magic angle (54.7°).
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8

Ultrafast Transient Absorption Spectroscopy

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A Libra F laser system (Coherent,
Inc.) produced 800 nm light pulses at a repetition rate of 1 kHz,
which was split for the excitation and probe pulse generation in a
roughly 90:10 ratio, respectively. The pulse width was ∼70
fs. The pump wavelength was tuned to 400 nm by a Topas C optical parametric
amplifier (Light Conversion Ltd.) followed by decreasing the excitation
energy density to 20 μJ cm–2 using neutral
density filters. The white light continuum for the probe pulses was
obtained by directing ∼10% of the primary 800 nm pulse energy
to a water-filled cuvette. The measurement system (ExciPro, CDP, Inc.)
comprised a silicon CCD, using an optical chopper for the pump pulses
for reference measurements.
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9

Time-Resolved Infrared Spectroscopy Setup

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Time-resolved IR (TRIR) measurements were carried out with the same setup as described in [33 (link),37 (link)]. Excitation was achieved with 400 nm pulses generated by frequency doubling part of the output of a 1 kHz amplified Ti:Sapphire system (Solstice, Spectra-Physics). Probing was achieved with the output of an optical parametric amplifier (TOPAS-C, Light Conversion) connected to a difference-frequency mixing module (NDFG, Light Conversion) and polarised at magic angle relative to the pump pulse. Detection was performed with a 2 × 64 element MCT array (Infrared Systems Development) connected with a spectrograph (Triax190, 150 lines per mm, Horiba), resulting in a spectral resolution of 1.5 cm−1. Sample handling and data acquisitions were the same as described in [33 (link)].
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10

SFG Measurements of Second-Order Nonlinear Susceptibility

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HD-SFG71 (link) measurements were performed in a collinear beam geometry using a Ti:sapphire regenerative amplifier (centred at 800 nm, ∼40-fs pulse duration, 5-µJ pulse energy, 1-kHz repetition rate, Spitfire Ace, Spectra Physics). Part of the output was used to generate a broadband IR pulse in an OPA (TOPAS-C, Light Conversion) with a DFG crystal. The other part of the output was directed through a pulse shaper consisting of a grating-cylindrical mirror system to generate a narrowband visible pulse with a bandwidth of ∼10 cm−1. The IR and visible beam were first focused into a 20-μm y-cut quartz plate as the local oscillator (LO). These beams were collinearly passed through a 2-mm SrTiO2 plate for phase modulation and focused on the sample surface at an angle of incidence of 45°. The SFG signal from the sample interfered with the SFG signal from the LO, generating the SFG interferogram. The SFG interferogram was dispersed in a spectrometer (HRS-300, Princeton Instrument) and detected by a liquid nitrogen-cooled CCD camera (PyLoN, Princeton Instruments). The data were analysed using a previously described procedure79 (link). Briefly, the complex spectra of the second-order nonlinear susceptibility χeff(2) were obtained via Fourier analysis of the interferogram and normalization by a z-cut quartz crystal. All measurements were performed using the ssp polarization combination.
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