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5 protocols using di02 r488

1

Single-particle fluorescence imaging of Bi4NbO8Cl

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To obtain isolated Bi4NbO8Cl particles, a well-dispersed methanol suspension of Bi4NbO8Cl in low concentration was spin-coated onto a cleaned cover glass. The particle-coated cover glass was annealed at 363 K for 30 min to immobilize the particles on the glass surface, and then placed in a chamber filled with an Ar-saturated aqueous methanol solution of MS-DN-BODIPY (1 μM). A 488 nm CW laser (OBIS 488LX, Coherent; 10 mW cm−2) passing through an objective lens (CFI Plan Apo λ100 × H, Nikon; NA 1.45) after reflection by a dichroic mirror (Di02-R488, Semrock) was reflected completely at the cover glass–solution interface to generate an evanescent field, which made it possible to detect the fluorescent products selectively on the bottom surface of the crystal. The emission from the sample was collected by the same objective lens, after which it was magnified by a 1.5× built-in magnification changer, and passed through a band-pass filter (FF01-535/50, Semrock) to remove undesired scattered light. The emission images were recorded using an electron-multiplying charge-coupled device (EMCCD) camera (Evolve 512, Roper Scientific) using Micro-Manager (https://www.micro-manager.org/). All experimental data were obtained at room temperature.
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2

Bi4NbO8Cl Optoelectronic Characterization

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PL microscopy measurement was also conducted based on a Nikon Ti-E inverted fluorescence microscope. For wide-field microscopy, the 405 nm CW laser (OBIS 405LX, Coherent; 30 mW cm−2) was used to excite the Bi4NbO8Cl. The emission images were recorded on an EMCCD at a rate of 30 frames s−1. A suitable dichroic mirror (Di02-R488, Semrock) and a long-pass filter (BLP01-488R, Semrock) were used to improve the signal-to-noise ratio. For confocal microscopy, the 405 nm pulsed diode laser (Advanced Laser Diode System, PiL040X; 45 ps FWHM, 1 MHz repetition rate) was used to excite the samples. The emitted photons were passed through a 100 μm pinhole and then directed onto a single-photon avalanche diode (Micro Photon Devices, SPD-050). The signals from the detector were sent to a time-correlated single photon counting module (Becker & Hickl, SPC-130EM) for further analysis. A dichroic mirror (Semrock, Di02-R405) and a longpass filter (Semrock, BLP01-458R) were used to remove the scattering from the excitation light. PL spectra were obtained by directing the emission into an imaging spectrograph (SOL instruments, MS3504i) equipped with a CCD camera (Andor, DU416A-LDC-DD) through a slit. All experimental data were obtained at room temperature in air. The data were analyzed using the open source image software ImageJ (http://rsb.info.nih.gov/ij/) and Origin 2015 (Origin-Lab).
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3

Quantifying Nanoparticle Brightness via FCS

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FCS measurements were used to determine the average brightness per particle (BPP) of the gQD/SiO2 before and after Au shelling. On an Olympus IX71 microscope, each sample was excited using a pulsed (10 MHz) 485 nm laser at 5 μW (PicoQuant PDL 800-B) through an Olympus 60× NA 1.2 water-immersion objective. The diffraction-limited probe volume was focused 25 μm above the coverslip into the solution. After passing through a 488 nm long-pass dichroic (Di02-R488, Semrock), the emission was filtered with a 640 nm band pass (FF01-641/75, Semrock), split by a 50/50 beam splitter (BS016, ThorLabs), and collected by two fiber-coupled single photon counting avalanche photodiodes (SPCM-AQ4C, Excelitas). The reflected and transmitted channels were cross-correlated using ALV5000 hardware correlators. The correlation function was averaged from at least three 5 second measurements. The BPP was determined by multiplying the average count rate by the amplitude of the correlation function, which is inversely equal to the number of particles in the probe volume.
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4

Multiphoton Imaging with Customized Setup

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It is taken with a commercial multiphoton microscope with both 2P and 3P light path (Bergamo II, Thorlabs). A high numerical aperture (NA) water immersion microscope objective (Olympus XLPLN25XWMP2, 25 X, NA 1.05) is used. For GFP and THG imaging, fluorescence and THG signals are separated and directed to the detector by a 488 nm dichronic mirror (Di02-R488, Semrock) and 562 nm dichronic mirror (FF562-Di03). Then the GFP and THG signals are further filtered by a 525/50 nm band-pass filter (FF03-525/50, Semrock) and 447/60 nm (FF02-447/60, Semrock) band-pass filter, respectively. The signals are finally detected by GaAsP photomultiplier tubes (PMTs) (PMT2101, Thorlabs).
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5

Custom Multichannel Fiber Photometry System

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The framework of our custom-built multichannel fiber photometry system is shown in Fig. 1(a). Four individual multimode fibers were integrated into a bundle and then glued into a subminiature version A connector. The excitation light from a 488-nm semiconductor laser (Coherent, OBIS 488 LX, 50 mW) was coupled into each fiber through an objective (Olympus, Plan N, 10× , NA 0.25) after being collimated with a beam expander [Fig. 1(a)]. The emitted fluorescence was separated from the excitation light through a dichroic mirror (Semrock, Di02-R488) and a bandpass emission filter (Semrock, FF01-535/22). The images of the fiber end faces were captured by a scientific complementary metal-oxide semiconductor (sCMOS) camera (Hamamatsu, C11440-22C) with a sampling frequency of 100  frames/s [Figs. 1(b) and 1(c)]. The image of each fiber end-face was circled as a region of interest (ROI) and the averaged fluorescent intensity of each ROI was acquired as Ca2+ signal for each channel. The control of light excitation and the data acquisition were implemented by a custom-written software on the LabVIEW platform (National Instruments).
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