I have found some academic papers regarding the scientific instruments on Chang'e 4 from Chinese forums and other websites. Here's a list and some technical specifications of all of them: (info from JIA Yingzhuo, ZOU Yongliao, XUE Changbin, PING Jinsong, YAN Jun, NING Yuanming.
Scientific objectives and payloads of
Chang’E-4 mission (in Chinese). Chin. J. Space Sci., 2018,
38(1): 118-130.; doi 10.11728/cjss2018.01.118)
Lander:1. Landing Camera (LCAM)
2. Terrain Camera (TCAM)
3. Low Frequency Radio Spectrometer (LFS)
A. Lunar Lander Neutrons and Dosimetry (LND) (Kiel University, Germany)
Rover:1. Panoramic Camera (PCAM)
2. Visible and Near-Infrared Imaging Spectrometer (VNIS)
3. Lunar Penetrating Radar (LPR)
B. Advanced Small Analyzer for Neutrals(ASAN) (Swedish Institute of Space Physics)
Relay satellite:C. Netherlands-China Low-frequency Explorer (NCLE) (Radboud University Nijmegen, Netherlands)
Of the 6 Chinese instruments, 5 of them are apparently the same model as the ones from Chang'e 3. Only the Low Frequency Radio Spectrometer for radio astronomy observations is new.
The specifications of the instruments are as follows (not sure about some of the translations of the technical terms - I did badly with my undergraduate physics!

):
Landing Camera (LCAM)Observation Wavelength - 419-777 nm
Focal distance - 4 m - infinity
Effective pixels - >= 1024 x 1024
Observation field - 45 x 45° (error <5%)
Modulation Transfer Function - >=0.20 (all fields)
Signal to noise ratio - >= 40 dB at highest SNR; >= 30 dB for albedo 0.09 and Sun angle 30°)
Terrain Camera (TCAM)Observation Wavelength - 420-700 nm (with RGB capability)
Focal distance - 5 m - infinity
Effective pixels - >= 2352 x 1728
Observation field - 22.9 x 16.9° (error <5%)
Modulation Transfer Function - >=0.20 (all fields)
Signal to noise ratio - >= 40 dB at highest SNR; >= 30 dB for albedo 0.09 and Sun angle 30°)
Panoramic Camera (PCAM)Observation Wavelength - 420-700 nm (with RGB and full color capability)
Focal distance - 3 m - infinity
Observation field - 19.7 x 14.5° (error <5%)
Modulation Transfer Function - >=0.20 (all fields)
Signal to noise ratio - >= 40 dB at highest SNR; >= 30 dB for albedo 0.09 and Sun angle 30°)
Low Frequency Radio Spectrometer (LFS)Observation frequency - 0.1-40 MHz
Receiver Sensitivity - <= 10 nV·Hz^−1/2
Dynamic Range - >= 75 dB
Frequency resolution - 1-10 kHz for 0.1-1.0 MHz range and 100-200 kHz at 1.0-40 MHz range
Visible and Near-Infrared Imaging Spectrometer (VNIS)Observation Wavelength - 450-950 nm (visual - NIR channel) & 900-2400 nm (NIR - short wave IR channel)
Spectral resolution - 2-10 nm (visual - NIR channel) & 3-12 nm (NIR - short wave IR channel)
Observation field - >= 6 x 6° (visual - NIR channel) & >= 2 x 2° (NIR - short wave IR channel)
Modulation Transfer Function - >0.1
Signal to noise ratio - >= 40 dB at highest SNR; >= 30 dB for albedo 0.09 (Sun angle 45° for visual - NIR channel & 15° for NIR - short wave IR channel)
Lunar Penetrating Radar (LPR)Channel 1
Transmitter Voltage - 1000 V (error <5%)
Transmitter Pulse frequency - 0.5, 1, 2 kHz
Transmitter Pulse time of arrival - <= 5 ns
Receiver frequency - 10-175 MHz
Receiver input dynamic range - >90 dB
Antenna central frequency - 60 MHz
Antenna bandwidth - >=40 MHz
Standing wave function - <= 3
Maximum detection depth - >= 100 m
Depth resolution - 1 m
Channel 2
Transmitter Voltage - >= 400 V (error <5%)
Transmitter Pulse frequency - 5, 10, 20 kHz
Transmitter Pulse time of arrival - <= 1 ns
Receiver frequency - 10-1000 MHz
Receiver input dynamic range - >90 dB
Antenna central frequency - 500 MHz
Antenna bandwidth - >=450 MHz
Standing wave function - <= 2.5
Maximum detection depth - >= 30 m
Depth resolution - <= 30 cm
And here are the specifications of the European instruments:
Lunar Lander Neutrons and Dosimetry (LND)Detection capability for:
Fast neutrons - 2-20 MeV (32 channels)
Neutron flux rate - 10-104 min^-1
Protons - 7-30 MeV (32 channels)
Electrons - 60-500 keV (32 channels)
Alpha Particles - 7-20 MeV/n (32 channels)
Heavy ions - 10-30 MeV/n (32 x 32 array)
LET - 0.1-430 keV/μm (64 channels)
Time resolution - 1 min for flux rate; 5 min for protons and electrons; 30 min for heavy ions
Advanced Small Analyzer for Neutrals(ASAN)Observation range - 10 eV - 10 keV
Mass resolution - Neutral atoms - capable of distinguishing H atoms and +ve ions of mass to charge ratio of 1, 2, 4, 8, 16, 32
Energy resolution - 7% (+ve ions) and 30% (Neutral atoms)
Time resolution - 10 s
Netherlands-China Low-frequency Explorer (NCLE)Observation frequency/Frequency resolution - 100 kHz∼1MHz/1 kHz; 1∼10MHz/10 kHz; 10∼80MHz/100 kHz
Clock stability - <5 x 10^-11
Receiver Sensibility - <-160 dBm.Hz^-1 (10 MHz)
Dynamic Range - >= 84 dB
Interferometer base line - >400000 km
Interferometer resolution - <= 1 Mbit.s^-1
I'll translate other details mentioned in the paper when I have time.