Low Temperature Microscopy
CLOSED-CYCLE BOTTOM LOADING CRYOSTAT
CONFOCAL MICROSCOPY
LT-SCM works by passing a laser beam through a light source aperture which is focused by an objective lens into a small area on the surface of the sample and an image is built up pixel-by-pixel by collecting the emitted photons from sample surface.
LOW TEMPERATURE XYZ PIEZO SCANNER
Low temperature piezo scanner
LT-AFM/MFM
The LT-AFM/MFM is an alignment-free Atomic Force Microscopy system equipped with a Fibre Interferometer operating at 1310 nm, 15 fm/√Hz noise level with an operation range of 20mK-300K, and up to 16T magnetic field.
LT-APO OBJECTIVES
Low Temperature APO Objectives
LT-SHPM/STM
With the help of a micron-sized semiconductor Hall sensor probe, our LT-SHPM enables user to map the surface Hall voltage V H as a function of position, which directly gives the spatial distribution of the local magnetic induction.
LT-sSNOM
LT-sSNOM has the capability of near-field imaging and spectroscopy together with other AFM modes such as contact, dynamic, MFM, cAFM, KPFM, PRFM. The tip-sample interface is illuminated by off axis parabolic mirror and scattered light is detected by heterodyne interferometer.
NMI CRYOSTAT: CRYOGEN FREE ULTRA LOW VIBRATION CRYOSTAT
Break free from the logistical challenges and rising costs of liquid helium. NanoMagnetics Instruments designs and manufactures a leading portfolio of cryogen-free cryostats, also known as closed-cycle cryostats. Our systems are engineered to provide an unparalleled ultra-low vibration environment, making them the ideal solution for the most sensitive microscopy, spectroscopy, and transport measurements.
Experience outstanding temperature stability, exceptionally low acoustic noise, and the freedom of a completely cryogen-free laboratory.
NV-CENTRE MICROSCOPE
LT-SNVCM uses a single NV Centre to image magnetic domains. The NV Centre is excited with a green laser through Low Temperature Apochromatic Objective with 0.82NA & 0.95mm WD. Single photons emitted by the NV centre are filtered and counted by an APD to obtain ODMR spectra with an RF antenna. Magnetic image is built up pixel-by-pixel by counting the number of emitted photons from the NV centre.
mK-CONFOCAL/RAMAN MICROSCOPE (mK-CFM/RAMAN)
0.82 NA / 0.95mm WD Low Temperature Compatible Objective