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+48V Phantom Power and Phase Reverse switch. Dedicated input Gain controls and output Trim controls on both channels. Exclusive Neve® Marinair™ transformers used on input and output stages. Hand-crafted and hand-wired by Neve in Burnley, UK. Two legendary 1073® microphone preamps in a convenient 1U rackmount design. This stereo unit is the perfect solution for studios looking to bring in the very essence of the legendary 1073® sound. Class A analogue outputs in XLR format are also found on the rear panel, controlled via adjustable front-panel ☑0dB Trim controls. Two rear-panel Mic inputs and Line inputs feed dual Class A gain stages, with adjustable Gain control and selectable 48V available on the Mic inputs. The 1073®DPA provides the legendary sound of Neve in a remarkably simple format. With the 1073®DPA, the highly sought-after 1073® mic amp sound is now available in a cost-effective 1U stereo rackmount solution, without the additional EQ found on the classic 1073 unit. Its lush sound with classic Neve® signature makes it the consummate mic pre for recording vocals, guitars, and acoustic instruments of all descriptions. The big, punchy sound of the 1073® compliments any musical genre, from rock to pop, hip-hop to rap, thrash to classical. The 1073® is the mic preamp of choice for numerous leading producers and artists, delivering the unique Neve® sound featured on some of the most famous recordings of the past 40 years.Ī superb addition to the Neve® outboard range, providing two of our world-famous Class A 1073® microphone preamplifiers in a single rackspace. 
EQL Button: Switches the equaliser in or out of circuit.Here's what Neve have to say about the 1073 Preamp:. High Pass Filter: 18dB per octave slope, switchable between 50Hz, 80Hz, 160Hz & 300Hz. Low Frequency: Smooth +/- 16dB shelving with selectable frequencies of 35Hz, 60Hz, 110Hz & 220Hz. Mid Frequency: Smooth +/- 18dB peaking, fixed 'Q' with selectable centre frequencies of 0.36kHz, 0.7kHz, 1.6kHz, 3.2kHz, 4.8kHz & 7.2kHz. High Frequency: Smooth +/- 16dB fixed frequency shelving at 12kHz. Noise: Not more than -83dBu at all Line gain settings, EQ In/Out (22Hz to 22kHz bandwidth). Frequency Response: '+/-0.5dB 20Hz to 20kHz, -3dB at 40kHz, EQ out. Distortion: Not more than 0.07% from 50Hz to 10kHz at +20dBu output (80kHz bandwidth) into 600 Ohms. Output impedance is 75 Ohms 1kHzOutput is transformer balanced and earth free. Output: Maximum output is >+26dBu into 600 Ohms. DI Input: Input impedance 10M Ohms (PAD off) / 10K Ohms (PAD on)Gain +80dB to +20dB in 5dB steps. Line Input: Input impedance 10K Ohms bridging, gain +20dB to -10dB in 5dB steps.Input is transformer balanced and earth free. Microphone Input: Input impedance 300 Ohms or 1200 Ohms, gain +80dB to +20dB in 5dB steps.Input is transformer balanced and earth free. The 19” rack-mount 2U unit includes an external multi-voltage PSU #How to use neve 1073 preamp plus#
The 1073DPX has two channels of Neve 1073 Class A design microphone preamplifiers, each with 3-band EQ (fixed HF plus two switchable bands with cut/boost capability) and high pass filter, adding warmth and depth to recordings, bringing out subtle ambience, maintaining spatial positioning, and capturing a more precise image – embodying, think many engineers and producers, the essence of the genuine Neve sound.īuilding on the 1073 classic module features, the 1073DPX introduces extra functionality with integrated DI input, phantom power, selectable Insert feature, level meters, selectable headphone monitoring and I/O connectors on each channel for easy and direct connection of microphones and instruments. Designed and built in England, the modern-day 1073DPX is produced to the exact specifications of the original with matched components to ensure the sound remains true. Found on some of the most famous recordings of the past 40 years, the big, punchy sound of the 1073 complements any musical genre – from rock to rap to classical. Launched in 1970, the Neve 1073 Classic soon became the first choice mic preamp for leading producers and artists.
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