Claypaky Xtylos, the first Beam fixture with RGB Laser sources

Claypaky Xtylos

Presented at Prolight+Sound 2019, where it was very well received by lighting designers (it was like a honey pot in the middle of a bunch of hungry bear cubs), the Xtylos heralds itself as a revolution in the world of motorized Beam fixtures.
An evolution of the Sharpy, it is based on a brand new technology using three RGB LASER sources. Let’s have a look at this unit!

A trade show is not always the most appropriate place to assess the quality of a beam, so we asked to borrow this innovative fixture to test it at the Impact Evénement studios, but also at night in Dimatec’s parking lot, alongside the Sharpy, of course, and the Sharpy Plus.
We also asked our colleague Jean-Pierre Landragin, a laser specialist, to provide more details on the source technology on board (see the box at the end of this article).

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The Xtylos features a design that is reminiscent of the aesthetic styling of the Axcor range, with a rounded head, a kind of smooth, matte egg, decorated with pretty golden stripes on its sides and topped with an enormous 15 cm output lens, a yoke with rounded arms and a small, thin and compact base. This unit is beautiful!

The beam aperture, from the smallest reducer to the largest “wide focus”.

In terms of safety, although it is equipped with very powerful laser sources normally corresponding to Class 4 (prohibited for use indoors and highly regulated outdoors), thanks to its optical system, Xtylos is classified as a Class 1 laser source device, in other words safe for use, including direct viewing into the beam over extended periods of time. Everyone can rest assured!

Effects with gobos, prisms and pastel colors.

The Xtylos’ beam is indeed that of a beam fixture (and not that of a laser), very tight at 1.1° of divergence, and it cuts through the air like a fine and precise blade. The light is extremely bright and intense, as if it were covered with glittering colored dust.

From a purely optical point of view, the focal length extends far beyond the head of the fixture. The focal point can be several tens of centimeters from the output lens, forming a converging and then diverging radius. This is how, in the absence of a zoom, the widest beam can be obtained: about 8°.

Prisms and frost at the widest aperture.

The very coherence of the beam is completely new and its uniformity over its length is much more significant than that of a Beam from a lamp. It remains highly concentrated with little alteration over long distances.
The dimmer of Xtylos is electronic. The curve we have plotted is quite impressive. Claypaky has mastered the independent management of the three sources.

Lend me your Xtylos 3 colors!

Also in terms of colors, the Xtylos offers completely new possibilities. The sum of the three RGB sources yields a white that can be regarded as a “full-color”. It will be up to you to calibrate your own reference white in your color presets. Indeed, the Xtylos is controlled like any other automated fixture, with a very conventional CMY library that provides access to all the power of the sources.

Some hues with both pure and mixed colors.

If the pure colors – Red, Blue or Green – are really effective, the mixes can be surprising. The color can be slightly varied depending on the length of the beam, and how it is focused. For example, it may be that with an orange mixture, a brighter and more vivid beam is obtained before the focal point than after it.
It produces an almost yellow beam, which becomes more orange beyond the focal point, becoming deep gold in the projected field a few meters down. Be aware that this is not a matter of color mixing but of a property inherent to its technology. The sources don’t necessarily have the same focusing properties.

But let’s go back to the three basic RGB colors to underline their exceptional intensity. Never has a red been so intense on a beam fixture, with a flux that corresponds to nearly 36% of the total white flux. That’s something we’ve never seen before!
The same goes for green, and as for the blue, no need to talk about it… The colors are really intense.

New since its launch, the Xtylos offers a variable white from 8000K to 2500K that, logically, must be an electronic emulation of the three laser sources . This is good news that should reassure lighting technicians disappointed at Prolight + Sound by the white.

Video tests of beams, gobos, colors and prisms


The gobos

Xtylos features two gobo wheels. One of them includes 14 fixed gobos, directly (and precisely) cut from sheet metal with aperture reducers and a few gobos – that are already well known from the Sharpy – which can sculpt the beam.
The second wheel includes seven interchangeable, indexable rotating gobos: a bar, a cone, a “colander” and a few others, all very impressive in terms of aerial effects, which can truly be used on the wide open beam (which was not the case with the Sharpy) and multiplied by the prisms. The two wheels are mixable and, by playing with the focus, you can create nice effects.

Some of the fixed gobos. We start with the beam reducers.

The rotating gobos, in “wide focus” mode.

The prisms!

Several optical effects can be used to animate and shape the beam. First of all, a prism with 16 facets arranged in a “flower”, rotating and indexable, allows the beam to be scattered: it diverges at an angle of nearly 12°. It is independent and can be mixed with the effects wheel, which has a 6-facet radial prism, a prism to spread the beam in a linear plane and a 6-facet linear prism, all of which can be rotated and indexed. A frost filter is also located on this wheel.

The prisms and the frost.

The movements of the head.

Xtylos, like Sharpy, is extremely quick. Even though the head is more massive than that of its elder, it is quite comparable in speed. The slow movements are excellent and the movements are precise and smooth.

The construction of the fixture

The inside of the unit.

The housing of the head can be dismantled into three parts. Two cowlings that cover the effects section, i.e. two thirds of the way forward towards the lens. Each cowling is opened by turning two discreet screws, hidden in the ventilation grill, a quarter turn.

The front part is held by a tab that is fixed under the plastic housing of the head. It is secured by a small safety cable. The entire rear is enclosed by a large hood, which can also be removed by removing four quarter-turn screws and is likewise held in place by a small safety cable.

The back of the unit features a complex assembly that houses the laser sources and their cooling system. It is a sealed module that allows the heat pipe radiators to protrude. The technology in question is highly confidential.

The micrometric precision it requires for the adjustment of its sensitive semiconductors and their optical path requires that any internal intervention on the source be performed only by Claypaky’s technical services. The service life of the sources is declared to be 10,000 hours.

The module containing the laser sources.

After passing through a cylindrical light guide about ten centimeters long, the light is emitted through a small window a few centimeters wide, from which the beam emerges in the direction of the effects.

The light guide at the exit of the source, with its output window, once the modules have been removed.

The large focus lens.


The internal disassembly is all done with two removable effects modules, each with a set of captive quarter-turn screws, and by unplugging a few plastic connectors from a control PCB, and two large Sub-D connectors, which are also held in place by two small, captive flat screws.
It is necessary to remove two small plates that seem designed to avoid any light leakage towards the ventilation grills. These are also fixed with two captive screws. It takes a little meticulousness but everything can be disassembled quite well.
The first module holds the gobo wheels. On the underside of the second module is the effect wheel with the 6-facet and linear prisms plus the frost, while on the other side is the mechanism that inserts the large 16-facet prism into the beam.

The effects module (prisms and frost).

The gobo module.


Both of the yoke arms are traversed by the routing of the wiring to the head. Only one of them is equipped with the tilt drive – with the motor in the base of the arm transmitting its movement via a belt to the pulley – while the other is fitted with the pan motor, the electronics that appear to manage the pan and tilt drive, and the tilt lock of the head.
It should be noted that the tilt belt seems difficult to remove without completely dismantling the entire unit… The alignment of all these cowlings is impeccable. Very nice construction.

The connection panel.

The power supply is connected through True1 input and output sockets. The output allows you to daisy-chain up to three Xtylos units on the same mains line. DMX input and output on XLR5, plus an RJ45 port receive the control signals. The base is flanked by two large handles that integrate into the extremely refined design of the entire unit.

The bottom of the base is equipped with the usual receptacles to accommodate the quarter-turn cam-lock fasteners of the two omega brackets (supplied with the unit, of course!) and the safety cable. These models of omega brackets are common to all Claypaky units and allow an “offset” clamping position.

I would like to take a few lines to express my heartfelt thanks to the person who designed and conceived this feature, which allows the fixture to be fixed anywhere on a truss without being hindered by a junction or a crossbeam. I can’t count the number of times this system has saved me. Anyway…

The menu and options

The display for configuring the fixture.

The Xtylos has more or less the same interface as the latest Claypaky models: a small bright display and five keys arranged in a circle. This system works pretty well.
The menu provides access to the usual addressing functions, operating mode (in this case, there are two: a Standard mode and a “Vector” mode), the control options, the run-time information of the unit and the sources, and so on.

Photometric measurements

We start by measuring the derating in full-color white, that is to say with the three RGB laser sources running at full power. The illuminance in the center stabilizes in five minutes with an attenuation of 11%, which will have a negligible impact on the performance of the beam. This is an excellent result for an effects projector.


Beam measurements

This is the perfect opportunity for us to debut the filter that we had produced specially for us in Japan, by Minolta, and which, combined with our CL 500 A spectrometer (normally limited to 100,000 lux), now allows us to measure up to 10 million lux of illuminance.
To obtain a higher number of measurement points, this time we place the fixture 10 meters from the target, which compared to the usual 5 meters of distance, multiplies the diameter of the projection by a factor of 2.

Thus, at 10 m the projected field of the beam extends to 19 cm in diameter, which corresponds to an angle of 1.1°. The illuminance at the center before derating reaches 137,900 lumens (122,300 lm after derating) which translates into a flux of 3,250 lumens (2,880 lm after derating).


Using the Xtylos

The Xtylos is an amazing machine. The light it emits is extremely powerful, very concentrated, yet at the same time it can appear very soft in some respects. One of the characteristics that caught our attention was that the beam heats very little, for example, compared to lamp-based beams that could almost melt materials nearby. The temperature of the Xtylos beam is lower, but at 10 meters, pointing at a light surface, it burns your eyes! The light density is astounding.
The fixture itself responds admirably well. The functions are simple and straightforward. It will take a little time to fully grasp all that can be done with it, and to familiarize yourself with the hues and effects that can be obtained. The ventilation is somewhat audible, but it remains within reasonable limits and, quite unusually, the sound emitted at the back of the head is very directional. From the front, the noise is much less noticeable.

Night-time outdoor tests

We wanted to assess the benefits of this new source over long distances compared to the lamp-based beams we are familiar with today from Claypaky. We meet at Dimatec with Antony Cals, Claypaky Product Manager, and Stéphane Samama, from Sales, who were delighted to be able to spend the night with us. Antony has prepared the three fixtures we requested in the company’s parking lot: a Sharpy, a Sharpy Plus and, of course, the Xtylos.

We use the Sharpy because it is the reference that everyone has in mind (or in their eyes, if you will). The Sharpy Plus, a hybrid Beam fixture with a more powerful lamp, is also capable of a multipurpose spot-type beam, but it is its Beam that interests us here.

Now it’s dark. Come on, let’s fire up the lights!

Tests in “white”

The first test, with the beams aligned, in white for the two lamp-based fixtures, and in “full-color” for the Xtylos. As mentioned above, in full-color the beam is not exactly white. It emits a slightly purplish light, but we have chosen to push the fixtures to their maximum.

White beams. In the image on the left, seen from behind, the Sharpy Plus is to the left, Xtylos in the centre and Sharpy on the right. Viewed from the front, the Sharpy is on the left and the Sharpy Plus is on the right.

The Xtylos projects an infinitely sharper and more precise beam than the other two. We can hardly say that it is more powerful, because we have observed in the measurements that in terms of center illuminance and flux, it is the Sharpy that wins. The perfect edges of Xtylos’ beam give it a certain advantage. It is as “striking” to the eye, if not more so, than its neighbor. The good old Sharpy is not doing so badly but is clearly behind the other two, both in terms of brilliance and in terms of “visibility”.

Tests in blue

Blue beams, same disposition as above.

The same results. The Xtylos shows a remarkable ability to amaze us with a beam so narrow and sharp that, even though it is less luminous than the Sharpy Plus, we are noticing it more. It has a much more visual “presence”.

Tests in green

Green beams, same disposition as above. In the picture on the left, seen from behind, the Sharpy Plus is on the left, Xtylos in the center and Sharpy on the right. Viewed from the front, the Sharpy is on the left and the Sharpy Plus on the right.

This is a textbook case, because we arrive in a color domain where the laser is inevitably the winner. Green filtering is always delicate with lamp-based fixtures, whereas for a laser, especially with fairly acidic and “hot” greens (a bit over 500 nm), we are in the most sensitive range of the human eye.
This is why entertainment lasers, with powers that are sometimes quite low in green, have always proved to be extremely brilliant (especially with 532 nm DPSS sources, which have been successful for years, since the arrival of semiconductor-based lasers). Unsurprisingly, the Xtylos crushes the others in green.

Tests in red

Red beams.

The two lamp fixtures are in the zone where they have the most difficulty emitting light. Filtering their very cool source allows very little flux to pass through. Here, only the Xtylos beam is present, its red laser source showing its superiority hands down.

In short, after this very interesting test, it appears that the Xtylos has many advantages, which are not necessarily tied to a notion of raw luminous output. In the areas where the Sharpy Plus is superior, the Xtylos takes the game to the next level with another technology. The beam is so sharp and defined that it is much easier to distinguish and catches the eye more than any other Beam in some colors.

Conclusion

Xtylos represents a real breakthrough in the world of automated lighting. No one knows today whether or not this technology will be the standard in the near future or whether it is a clever solution for a unique product, but in any case, it is truly interesting. It is the only one that produces colors (such as red, blue or green) with this level of intensity. I can’t wait to see what lighting designers will do with this one.


Lasers in show lighting

Xtylos uses an RGB laser source. Unlike some fleeting attempts, this is not a laser+phosphor system (in which the primary source is a set of blue laser diodes and the rest or even the entire spectrum is created by phosphors arranged on a rotating disc, re-emitting lights of different wavelengths under the excitation of blue radiation), but a set of laser diodes emitting in red, green and blue, which are blended to achieve the whole spectrum of colors by additive synthesis.

It is therefore a “true laser” source that is emitted directly without any conversion, and the beam therefore maintains some of the very specific characteristics of laser light that have surprised our testers. The manufacturer is rather evasive about the exact characteristics of the sources, which are presumably the result of recent research by Osram… We know, however, that these are three sets of laser diodes mounted in arrays, with an electrical power of less than 100 W per color. Everything is in a sealed optical module, and the secret remains intact.

The essential characteristic of laser light is its coherence. This means that all photons are emitted in phase or, in other words, that all seem to come from the same sinusoidal wave. But since nothing is perfect, this aspect is characterized by the coherence length, which corresponds to the beam length over which the light can be considered to come from a single wave.

This characteristic has two ramifications:

A laser source is very monochromatic and this is all the more true when the coherence length is long (indeed, the spectral width and the coherence length are linked by the relation Lc = c/Δγ, where Lc is the coherence length[in m], c is the speed of light [c = 3.108 m/s] and Δγ is the spectral width of the emission[in Hz]). There is nothing here comparable to an LED source. As a result, an RGB laser source is able to reproduce a large color space, which is very well suited for video projection but may not be sufficient in lighting – we will see why later on.

Interference occurs inside the beam, especially when the light is very coherent. This causes the beams of laboratory lasers and the images they produce to have a granular, glittering or scintillating appearance. This is why we always have the impression that the space through which the beam passes is very dusty, the visible grains are not the effect of dust, but the effect of these interferences (called speckles). With three laser sources in the same beam, the interference of each color does not occur in the same place, so the beam is adorned with “grains” of different colors. It goes without saying that this effect could cause significant inconvenience in some applications.

Without any smoke, one gets the impression of dust particles in the beam.

Another result is that the emitted light does not contain any infrared (except, of course, if it is an infrared laser!), so the beam is “cool”. But, make no mistake, it is a concentrated energy that can be formidable when the illuminated object absorbs the radiation received (such as in medical applications). As such, it is normally necessary to take all necessary precautions to avoid receiving this type of beam in the eyes. In the case of Xtylos, the optics developed for the Beam application eliminate this risk.

Finally, laser sources generally emit parallel or very slightly divergent beams (hence the possibility of projecting laser beams onto the moon without scattering along the path) and their light distribution is very uniform. In the case of Xtylos, the light guide through which the beam exits the source probably acts as an integrating tube, allowing the beams from the diode arrays to be homogenized.
This yields a luminous distribution curve across the diameter of the beam that has very steeply ascending sides and a flat top, thus giving this solid and compact aspect to the beam, which is unrivaled by other types of sources. This particular characteristic also justifies the absence of any zoom, which is not necessary to change the width of the beam, as its edges are naturally perfectly defined.

From the point of view of colorimetry, each diode array is controlled using pulse width modulation (PWM), with the software adjusting the duration of the pulses applied to each to ensure the brightness (dimmer) and balance (color) of the mixture by emulating the more traditional controls. This is the only way to fine-tune the characteristics of the light emitted. However, when it comes to producing white, it is necessary to be able to precisely and independently adjust the power and color temperature.

With LEDs, it’s easy: you just need to have white LEDs, and you can fine-tune the balance with the other LEDs, and it’s even easier when you have a set of amber LEDs. This possibility does not exist with lasers because there is no such thing as a white laser (“white laser” is, in itself, an oxymoron), and the manufacturer did not choose to include a group of white LEDs (which would probably also have been technical and industrial nonsense).

For this reason, the RGB white is undoubtedly difficult to adjust, its fineness is limited by the resolution (i.e. the bit depth) of the PWM controls, and the software must “do its best” to achieve the desired “white” and try to maintain it over the entire dimming range. Paradoxically, having only three source colors is less of a problem for the range of colors than it is for the refinement of the whites. That being said, one could certainly call into question the use of this fixture in trying to create sophisticated white lighting, rather than using it to produce brightly colored beams in the air!

For further details, please refer to the articles in the SoundLightUp series on video projection regarding laser sources.


On aime :

  • The beam
  • The intensity of the colors
  • The construction quality

On regrette :

  • Not having 30 of them to play with on a stage!

Xtylos general

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Defender® Presents the MICRO 2 Cable Protector Series

Following the launch of the MICRO cable protector series at this year’s Prolight + Sound show in Frankfurt, Defender® is now doubling the stakes: The new MICRO 2 series provides space for two cable runs and ensures even greater protection for people and cables with its newly developed 3-D LaserGrip® surface.

Produced from over 90% recyclable materials, the MICRO 2 Cable protectors don’t only stand out thanks to their environmentally sustainability but feature a reengineered, ergonomic design.

MICRO 2 Features

The larger and more spacious an area, the higher the safety requirements are for both people and materials.
Nowhere else is this truer than at trade fairs, exhibitions, malls, and other public indoor and outdoor facilities, where there are lots of pedestrians walking around, as well as many smaller vehicles, trolleys, scooters, and wheelchairs out and about.


That’s why Defender has developed the compact MICRO 2 cable protectors for use in these areas. Built to withstand up to two tons per 7.8 × 7.8 inches, their two 1.4 × 1.2-inch cable runs protect power cables and water hoses from external influences.

A maximum level of grip and slip resistance is guaranteed by the innovative LaserGrip® surface, which features a special ergonomic design and surface structure to reduce the risk of an entire cable protector line accidentally moving out of place.

Sustainability

From shredding to granulation, 90% of Defender materials are recycled in-house, and the same goes for the new MICRO 2 series too! Since the whole process is monitored in-house, the type and origin of the individual materials can be traced at all times, which allows for exclusive proof to be provided that everything has been sourced from certified companies in Germany.
Defender is therefore the official recycler of materials from Bayer®, BASF®, and DOW® Chemical and as such plays an important role in the sustainable reuse of granulate.
Defender cable protectors and ramps are DEKRA certified (DIN 31000, EN 61537), comply with fire protection class B2 (DIN 4102, B1 also available), and meet the requirements of the Low Voltage Directive.

Video presentation of the product in situations.


New Brand Website : The Defender website underwent a complete overhaul and was launched at the same time as the rollout of the MICRO 2 cable protector series. In line with the new Defender brand slogan “Protect Your World”, the website provides users and prospective customers with all the key facts about products from Adam Hall’s prestigious private line.

Defender is a brand of the Adam Hall Group and more information on the Defender website

 

Oz LED followspots at the New National Theatre, Tokyo

Four of Robert Juliat Oz LED Followspots have recently replaced conventional followspots at the New National Theatre, Tokyo as part of an upgrade of the inventory for this arts venue.

Robert Juliat Oz in The Pit at New National Theatre, Tokyo © RJ Industry Japan

New National Theatre, Tokyo is Japan’s foremost national theatre dedicated to the contemporary performing arts of ballet, opera, dance and drama. The NNTT comprises 3 performance venues, Opera Palace, Playhouse, The Pit, and hosts over 300 performances a year to around 200,000 spectators.

Four of Robert Juliat’s Oz 7°-14° LED Top Control followspots were supplied by Sogo Butai, RJ distributor, initially chosen to be use in the small Pit Theatre, but also with the intention of relocating them to the Playhouse and Opera Palace as needed. This demonstrates the versatility of this zoom fixture whose 600W cool white LED engine generates an output equal to 1200W discharge fixtures.

Opera Palace at New National Theatre, Tokyo © Photo provided by New National Theatre, Tokyo

“Oz is extremely suitable for the open space within the smaller Pit Theatre, because of its silent operation,” says Takehito Suzuki, from NNTT’s technical lighting department.
“In venues where many theatrical shows and contemporary dance performances are presented, like those of the New National Theatre, we found Oz is the best followspot for lighting the performers at every distance.”

Suzuki also stresses that Oz was chosen because, above all others, its quality met the high standards of the New National Theatre, Tokyo; its Top Control option was a prime example of this, enabling the operators to control both the dimming and iris smoothly and easily from the top of the fixture.

ThePit (small theatre) at New National Theatre, Tokyo © Photo provided by New National Theatre, Tokyo

“Amongst many LED followspots, what makes this fixture remarkable is the Top Control,” Suzuki says. “I’m impressed by the minimum size of the iris shutter as well; the accuracy of the iris cassette is really incredible – it is great to see how RJ can make a spot so tiny that it seems like a hole pierced by a needle. We can see the RJ quality in these kinds of details.”

NNTT’s followspot operators agree and have enjoyed using the new arrivals, commenting: “Oz is highly operational with the double function of smooth dimming and iris control with the top controls. The body is well designed with a good balance of functionality, which makes it an extremely operator-friendly fixture.”

NNTT is familiar with Robert Juliat, having invested in Robert Juliat profiles when it first opened its doors in 1997. “Since the beginning we have used Robert Juliat Athos 914SNX and 910SNX profiles,” says Suzuki. “At the time these fixtures with discharge lamps were fully appreciated by every lighting designer who used them. ”

Playhouse at New National Theatre, Tokyo © Photo provided by New National Theatre, Tokyo

“The majority of New National Theatre profiles are still halogen-based, although most manufacturers are stopping production of these models, and we need to find new fixtures with alternative sources before these become outmoded. So we are now interested in LED sources which are powerful enough to match halogen fixtures, and Robert Juliat is already ahead of the game with LED models that perform as well as discharge fixtures.”

More on the Robert Juliat website

 

Meyer Sound Compass 4.6 is available and Offers Milan Integration

Meyer Sound has announced release of version 4.6 of its Compass® control software package, incorporating new feature sets for full control of Meyer Sound devices, including the Milan™ AVB certified GALAXY processors.

Compass 4.6 is the keystone component of a complete update package that also includes new firmware for the Galileo® GALAXY™ network platform processors, CAL™ beam-steering column array loudspeakers, and the RMServer for remote system monitoring.

Todd Meier

“This release marks an important milestone in the long history of Compass control software,” states Meyer Sound Director of Product Management Todd Meier, “as it is the first version to incorporate the new Milan networking protocol. It changes everything, as our goal is to make all of our digital products Milan-certified going forward.”

With the software and firmware upgrades in place, all existing Meyer Sound GALAXY processors will be immediately capable of upgrading to Milan-certified devices. Thousands of GALAXY devices are currently in the field, and all future GALAXY processors will be shipped with the new Milan-certified firmware installed.

The Milan protocol guarantees interoperability of networked devices by standardizing the implementation of AVB technology. Every Milan-certified device will discover and operate with any other certified device. No custom network configuration is necessary and all benefits of AVB networks are retained.
In conjunction with the companion update to GALAXY firmware, the Compass 4.6 software release offers other new features. Delay Integration and Starting Points are now accessible in one dialog and available from the Overview and Output Processing tabs.

Meyer leopard

New Starting Points have been added for LYON™ and LEO®loudspeaker arrays, eliminating the need to start configurations from “square one” and thus offering the quick setup of typical systems already available with Native Mode in LEOPARD™ and LINA™ line arrays.

The new software/firmware updates streamline the integration of LEO Family products with many prior generation products, allowing rental companies to maximize inventory use by, for example, using LEO Family main arrays with legacy fills and delays. New Starting Points also facilitate configuration of cardioid and directional gradient subwoofer arrays, and also include EQ and delay profiles that automatically tune legacy subwoofers to emulate the characteristics of the new LFC family of low frequency control elements.

“This level of seamless integration across product generations used to require time-consuming custom configuration and repeated measurements,” notes Todd Meier. “With this new release, the capability is built into the software.”
The new Compass 4.6 software requires a simultaneous firmware update for the controlled hardware devices: GALAXY network platform (v 2.1.0), CAL (2.1.0) and RMServer (2.7.0). An update of the Compass Go app also is required for full functionality of the iPad remote control features.

The proud Galaxy family

The complete software and firmware update package will be available for download at this link https://meyersound.com/product/compass/#software. The download is free for all registered users.
Available for Windows and Mac operating systems, Compass control software provides comprehensive and intuitive control of Meyer Sound self-powered loudspeakers systems either via the Galileo GALAXY network platform or by direct communication to CAL column array loudspeakers.
Compass provides a graphical user interface that displays detailed information and controls all device settings including GALAXY control pages, parametric and U-Shaping™ EQ, AVB network settings, delay integration, high and low pass filters, and CAL beam control.

Check for more and have a look on the brand new Meyer website

LIGHT PARTNER NEW DANISH DISTRIBUTOR FOR ALLEN & HEATH

Light Partner owners, Stig Meyer Jensen (Left) and Johan Kvartborg (Right)

The British professional audio mixing consoles brand Allen & Heath, has named Light Partner as its exclusive distributor for Denmark.

A&H EMEA Sales Manager Frédéric Cresson.

Allen & Heath’s EMEA Sales Manager, Fred Cresson, commented, “Allen & Heath has a strong, loyal following in Denmark, particularly in live sound and installation.
We are therefore delighted to be working with Light Partner to continue providing first-class support to our Danish customers, and to explore the opportunities to keep developing the brand.”

Stig Meyer Jensen, Light Partner’s CEO, commented, “With the new Avantis adding to an already unbeatable line-up of consoles, Allen & Heath is the mixer brand everybody is talking about right now.
We’re proud to be appointed to distribute A&H in Denmark and we’ve invested in a highly experienced team to deliver the outstanding backup that our customers deserve.”

The brand new Avantis.

The new distribution partnership is active with immediate effect.

More information on Allen&Heath website

 

Allianz Arena upgrades audio with a new L-Acoustics system

Famous German Munich’s Allianz Arena stadium upgrades audio for EURO 2020 in line with UEFA stadium standards, installing an extensive Kara system from L-Acoustics, in cooperation with Müller-BBM and Wilhelm & Willhalm.

Inaugurated in 2005, the Allianz Arena is one of the best-known football stadiums in the world. Inside, the three-tiered stadium construction leaves an impression on the 75,000 plus spectators who come to support home football team Bayern Munich.

For this season, the sound system in the Allianz Arena has stepped up its game. In cooperation with the engineering and planning office Müller-BBM, L-Acoustics Certified Provider System Integrator, Wilhelm & Willhalm event technology group, have installed an extensive Kara system from L-Acoustics.

Since the Arena opened, Wilhelm & Willhalm has been the infotainment technology service provider to the venue, and won the upgrade project when Müller-BBM launched a tender for the new sound system which would provide optimized, uniform sound level distribution across all three tiers, improve of the transmission quality for music playback, as well as increase speech intelligibility for announcements.

In addition, the new system needed to anticipate the upcoming EURO 2020 where, as part of the first pan-European European Football Championship, the only matches in Germany will be staged in there. Three preliminary round matches and a quarter-final are already scheduled and the venue’s sound system needed to respond to strong UEFA stadium standards.

Müller-BBM, previously worked with the Arena and the Wilhelm & Willhalm event technology group to optimize room and building acoustics at the venue. This experience helped when it came time to the design of the new sound reinforcement system.
“The membrane roof of the Allianz Arena creates considerable reverberation in the spectator area. For this reason, care was taken to design a system that delivers sound to the spectators, minimizing reflections,” explains Thomas Dürrbeck, who was responsible for planning and construction at Wilhelm & Willhalm event technology group.

L-Acoustics Kara-i install line source elements along with SB18 subwoofers from the main PA for the Arena before being pulled up into position.

Weight restrictions also played a decisive role: “Due to the static restrictions in the roof area of the stadium, only an eight-inch array system was considered,” adds Harald Frisch, sound engineer at Müller-BBM.
“L-Acoustics’ Kara system offers an almost ideal ratio of weight, precision of coverage, achievable sound pressure level and sound quality.”

In total, the L-Acoustics installation in the Arena comprises 266 Kara line source elements as well as 54 SB18 subwoofers for the main PA, with 48 ARCS WiFo as delay arrays in the curved areas and 70 5XT coaxial compact loudspeakers under the balconies. The system is driven by 110 LA4X amplified controllers with a system output of 440,000 watts, which are distributed over ten central amplifiers, each with two 40U system racks.

“The cooperation with Müller-BBM was excellent right from the start, extremely flexible and professional in every single phase of the installation. From the very beginning it was clear that all parties involved were working together as a large team to implement the project optimally for the customer”.
Jürgen Muth, Managing Director Allianz Arena München Stadion GmbH, agrees, stating, “the new Kara PA system is the result of trusted cooperation with our technology partner Wilhelm & Willhalm, and Müller-BBM as the executive planning office. With L-Acoustics, we chose one of the world’s leading suppliers in the field of professional sound system technology, who offers a complete package of sound characteristics, flexibility and cost-effectiveness.”

The Kara and SB18 ready to roar under the stadium roof.

“We are delighted that the Allianz Arena Munich now has a Kara system that meets the stadium’s leadership requirements, as well as the requirements of UEFA,” concludes L-Acoustics Director of Business Development Jochen Frohn.
“The great cooperation between Mueller BBM, Wilhelm & Willhalm and the Allianz Arena enabled planning, installation and commissioning of the system within a very short time. Hearing the system when it was fired up for the first matches filled us with great joy and pride.”

D’autres informations sur le site L-Acoustics

Active Audio / APG has hired Mathieu Pobeda as R&D Director

Mathieu Pobeda is the new R&D director of Active Audio / APG. He will oversee the development and introduction of new products for both arms of the company, with particular attention being paid to acoustics and transducers.
Mathieu brings with him a strong knowledge base – gained both academically and practically – of the market, as well as a great deal of expertise in electro-acoustic research.

“Active Audio / APG’s vision – which was explained by CEO Régis Cazin – was very appealing to me,” says Pobeda.
“In addition, I know there to be a lot of clever and talented people at the company; some of whom I have been in contact with for the last decade. From a personal point of view, the prospect of being able to use both my technical and my recently sanctioned management skills was key factor in accepting a new challenge. I think all the ingredients were there and – when that happens – you must take your chance.”

Mathieu Pobeda

Pobeda’s interest in audio began at the age of 10. “After university and my military service, I got my first job in a well-renowned Hi-Fi French manufacturer. I learnt a lot there as they had both systems and drive unit manufacturing facilities, so we could do anything from scratch including playing with cone or diaphragm materials. I also carried on my study as a part time student to get a Msc in Signal Processing from the CNAM in Saint Etienne.”

Mathieu then moved to England with his family to work for a Pro and MI drive unit manufacturer for five years. This allowed him to deepen his knowledge of compression drivers, horns and other types of direct radiation loudspeakers than Hi-Fis. For the last eight years, Pobeda has been designing complete systems for a renowned French professional audio company and has just completed a Master’s in Business Unit Management at ESSEC Business School in Paris.

Although he’s keen to hit the ground running at Active Audio / APG, Mathieu also emphasises the need to listen and learn when it comes to the company’s philosophy and methodology. “There are a lot of on-going projects and some very creative people in both companies,” he says.
“Nobody wants to drop straight into a company and start changing everything overnight, especially when the structure has been established for some time. You need to make sure that the changes you want to implement are valid and will stand the test of time. I’m very confident that I’ll be backed up by the top management in that mission.”

Pobeda identifies the Step Array as a game changer in the Active Audio portfolio. He says: “It’s been built on Xavier Meynial’s rigorous scientific knowledge and really address the customer’s priorities. This is a great example of the well-defined, well-thought-out, and well-made products that the company can offer. This same compliment can be applied to the UniLine and UniLine Compact products from APG.”

He concludes: “The market has undergone some changes in recent years, particularly with deep-pockets coming from other industries to grab historical audio activities and knowledge, so anything can happen in the next five. In any case, I trust that the Active Audio / APG group will substantially grow over that period.
We have the knowledge, interesting existing products and a lot more to come, though the main priority is to ensure we continue to move forward organically in every aspect of the business.”

Visit APG website or on Active Audio website

 

Ayrton Khamsin arrives in Starlite inventories

Starlite, the rental company that has one of the biggest inventories of lighting, AV and control equipment on the East Coast of USA, has purchased a complement of Khamsin-S, Ayrton’s profile LED moving head, to provide its clients in the broadcast, concert touring, corporate and performing arts markets.

The Khamsin-S purchase represents Starlite’s first acquisition of Ayrton products. “ACT Lighting (Ayrton’s exclusive distributor for in North America) demo’d the Ayrton line for us, and we evaluated the Khamsins in our shop and use on our own productions,” says President and CEO, Dean Danowitz.

“There was a fair amount of debate internally regarding which profile fixture we should invest in next,” notes Jason Danowitz, Vice President of Event Technology.
“Ultimately, we chose the Khamsin-S because it checked so many boxes for our touring and staging clients, including an 8:1 zoom (7o to 58o), 40,000-lumen output, CMY colour mixing plus fixed colours, variable CTO, two frosts, two rotating gobo wheels, prisms, an animation wheel, rotatable framing shutters and an iris. In addition, they’re flicker-free, which is essential for our clients with broadcast applications.”

As soon as Starlite took delivery of the fixtures they were quickly dispatched on a broadcast project. “The minute they hit our docks, they were booked for a major televised awards show,” says Starlite’s Rental Manager, Matt Strickland. “The Khamsins will work for so many applications that they will never be here – which is ultimately my goal!”

Jason Danowitz points out that, “the Ayrton brand has a reputation for innovative and well-designed fixtures, and they have amassed a loyal following among designers. Also, we’ve enjoyed great support from ACT Lighting through the years, so we’re happy to embark on this venture with them.”

More information on Ayrton Khamsin can be found at Ayrton website

 

Celso Papadopulos is the new Nexo European Sales Manager

Following the departure of Alain Boone to pursue independent interests, NEXO is pleased to announce the appointment of the industry veteran Celso Papadopulos to the role of European Sales Manager.

Celso Papadopulos has been one of the leading lights of the NEXO sales team since 2003, tasked with building the company’s export network and sales in Mexico, Central and Latin America.
In that time, he has created one of NEXO’s most dynamic and successful territories from virtually nothing, and helped to bring highly valued education and training to this huge market.

An industry veteran of 40 years, Celso started out as a professional musician and has since worked as a recording engineer, front-of-house engineer and monitor engineer. He worked as a sound designer on many large-scale projects before fully entering the commercial environment to work in sales and distribution.

His first task as Europe Sales Manager will be the development of NEXO’s European commercial department. “It’s a new challenge, and challenge renews life!” says Celso. “In South America, I was working in many different countries with different cultures, so I recognise that every place offers new opportunity.
The skills of distributors are critical to our success, and I hope to boost our outstanding network to achieve great things, drawing on my own wide-ranging background in both of NEXO’s main markets, touring and fixed installation.”

More information on the Nexo website

 

Area Four Industries acquires Prolyte Group

The leading manufacturing group on the worldwide market for aluminium truss, support structures and other peripheral products Area Four Industries has acquired the dutch Prolyte Group.

On his FaceBook page, Prolyte announces : « A miracle happened ! Even when things looked in all kinds of ways, it ended up, all of a sudden, in an agreement. We have become part of the world’s number one. Area Four Industries. Yet we keep our name. On and on. Forever. PROLYTE. Our Blue heart beats stronger than ever. »

Area Four Industries adds : « The core of the Prolyte brand and its high quality products will remain, but a major reorganization will take place within its management, production processes and strategic direction. »

More information on Prolyte Group faceBook and on Area Four Industries

 

WIcreations acquires Visual act

WIcreations, entertainment technology automation specialist, based in Belgium, has acquired the assets of Visual Act Scandinavia AB, including all the IP, source coding, patents, related to computerized control systems used for events, installations and venues machinery.

Hans Willems, CEO of Wicreations

The move makes independently owned and operated WIcreations the largest automation rental provider in Europe.
The Wicreations CEO, Hans Willems, says, “This opportunity will support our planned medium-term progression and allow us to develop even more dynamic automation solutions for a wider range of clients, including full touring packages.
WIcreations has been using Visual act’s Stage Control System for moving our own stage / event wagon system since 2014, so this puts us in a great position to develop this software for future applications”.
The plan is to integrate the platform into new WImotion system, which offers a full range of motion control hardware and software to move any object safely in a 3D environment.

Founded in 2005, WIcreations, has already over 80 Visual act drive units for rental that makes this company an active provider of this specific programmable wireless wagon system.
Full access to the Visual act Wagon and Visual act 3D IP and codes will help WIcreations to provide its client base with unrivalled device, object, wagon and 3D flying control and management.

Hans adds, “Our ambition has always been to have one single software solution to run all automated aspects of a show or event – whether it is objects or flying people, moving wagons on a floor, etc. With the proven reliability and scope of the Visual act architecture, several elements are now aligned for this to happen imminently.” WIcreations will announce their new WImotion system development / rental opportunities in the coming weeks.

More infos on the Wicreations website

 

QSC KS118, the new member of KS subwoofers family

QSC has just introduced the KS118, an active subwoofer which is the newest member of the KS family, replacing the acclaimed KW181.
With its robust design, legendary QSC amplification and versatile DSP features, the KS118 is the perfect choice for mobile entertainment, AV rental, event production, clubs and performance venues for which very high output and commanding low frequency performance is needed.

Featuring a long excursion, tour-grade, 18-inch direct radiating driver powered by a 3600 Watt Class D amplifier, the KS118 delivers high sound pressure levels with dynamic and musical sound reproduction of very low frequencies.


QSC KS118 back

On-board DSP optimizes and protects system performance while also offering advanced capabilities such as the ability to array two units in a cardioid arrangement, maximizing low frequency output in front while minimizing unwanted energy around the sides and rear of the system. DEEP™ mode provides additional low frequency extension and driver excursion processing.

Highly transportable, the rugged premium birch enclosure features comfortable aluminum handles and four rear-mounted low-noise casters. A top-mounted M20 threaded pole receptacle accepts a 35 mm pole for easy vertical deployment with QSC K.2 Series and other full-range loudspeaker. The high performance KS118 addresses today’s requirements for dynamic, high-energy bass content reproduction.


Specifications :

– Frequency response (- 6 dB) : 41 Hz-98 Hz (35-111, -10 dB)
– SPL max (@ 1m pink noise with 10 dB crest factor) : 136 dB
– Amplifier : class D, 3600 W peak
– Cooling : low noise variable speed fan
– AC power input : 100 – 240 VAC, 50 – 60 Hz
– Enclosure : 18 mm birch plywood with 16-gauge black powder coated steel
– Dimensions (HxWxD) : 25.2 x 29.3 x 35.3 in (640 x520x785 mm)
– Net weight (included casters) : 47 kg


More information on the QSC website

 

Bertrand Billon, new Nexo STM Series engineering support specialist

NEXO just expanded its Engineering Support Division with the appointment of Bertrand Billon. He will assume special responsibility for the company’s top-of-the-range modular line array systems, the STM Series.

After spending the first years of his engineering career working with tours and events as a PA technician and engineer for the well-known French production services company Dispatch, later known as Dushow, Bertrand joined the newly-created Stage Entertainment France as Head of Sound.
He acquired a wide experience of managing crews and liaising with sound designers, dealing with rental inventory as well as permanent in-house equipment.
As well as specifying all of Stage Entertainment France’s audio equipment purchases, he also managed the technical and crewing aspects of the events staged in the company’s Mogador Theatre in Paris, numbering about 30 corporate events, tv shows and concerts per season.

“Coming to NEXO gives me the opportunity to focus once more on PA systems, which was my first occupation and passion,” says Billon. “I am excited to be doing this job on behalf of a manufacturer, which will raise my skill level and knowledge. A great support engineer should be a very good listener, reacting to customer requests and feedback, not only able to fix their problems, but able to avoid them in the first place, through proper training and communication.”

More information on the Nexo website

 

La Fête des Vignerons Part 2: The people in the shadows

I wanted to devote this second part to these men and women, whose technical skills make them essential for making a show run smoothly. They are not part of any team, but are attentive to the challenges that they face.

In the meantime… (Photo: Philipe Leblond)

Let’s meet these data controllers, these communication experts and timing managers in order to understand their world: that of the intercom system, signal topography, network administration and show control.
Let’s delve into the invisible world that reveals itself only if there is a technical problem.

Ground Control to Major Tom…

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The men in the shadows: stage managers, stagehands… (Photo: Claude Cellier)

Doum preparing for a second Watergate. (Photo: Emmanuelle Husson)

There is no specific name for this profession (“Commie”? Maybe not…), but oh, how important it is, as explained by Philipe Leblond, better known in the business as Doum.

This former TV sound engineer – accustomed to stadiums, opening ceremonies, sporting events such as the Dakar, concerts and conventions – has become an authority in communications.
Who’s talking to whom? Who hears what? These are the two questions he faces daily and he must be able to answer… instantly.

“First of all, we have to define the specifications. How many routes will we have to deploy, how many people will we have to equip with a wired or wireless connection and for which coverage area? Sound, lighting, video, stage, stage management, choreography, so many primary routes under which sub-networks are dissimulated, and private networks because a 2 hour and 45 minute show without a little banter can be long. Don’t ask. What is said on the comms stays on the comms!

Welcome to the matrix: 200 in/out… (Photo: Philipe Leblond) Clear-Com EHX MEDIAN matrix, 2 MVX-A16 cards, 1 E-Dante 64 card, 1 E-IPA 64 HX card, 1 IVC-32 card.

All essential information is routed via the Clear-Com Eclipse matrix, on which the Freespeak wireless system is interfaced via the IPA card and completed by the Helixnet network, all of which can be controlled remotely via the EHX software.
The system consists of 26 stations connected in IP or in analog with multiple keys, from 12 to 32 depending on the size of the traffic, scattered throughout the arena to equip each mixing position. In addition to this, there are 60 wireless beltpacks, 70 walkie talkies and about ten wired stations distributed from right to left.
For the 5,500 costumed extras, the dressing-rooms were scattered throughout the town. These eight remote sites, gymnasiums, and schools, were all interconnected by La Romande Energie using optical fibre.

This network layout allowed me to install an IP station in each location to ensure real-time communication with the logistics of the Arena. And in case the connection were ever to be interrupted for any reason, I set up a Ubiquiti router on the matrix. Thanks to a public IP address, this allows me to create virtual panels (IC agent) on tablets or smartphones, to control the matrix remotely and, most importantly, to connect to a SIP server.

I can provide a compatible phone number that can be used to communicate directly with the relevant station or beltpack. ” I can confirm that Doum possesses the gift of ubiquity: during the rehearsals he was absent for a few days. He was in Cannes for the Amfar Gala; in short, not with us at all. Being a professional, he had brought in Margaux to replace him. The director asked for a modification to a key and then, miraculously, Doum replied, made his modification, three little tricks and then disappeared, leaving us – Margaux and me – in awe.

Rehearsals, a long and peaceful river

Due to impending rain, the rehearsals were postponed. The artistic director’s table. (Photo: Philipe Leblond)

After six intense days of setup, Doum thought he would be able to sit comfortably in his chair to supervise the smooth operation of his network.
Well, yes… but no! That was all without counting on the magic of creativity!

“Usually during a show,” he explains to me, “the show caller is the one who is responsible for conducting the show.
It is up to him to give the cues at the right time and in the right way to all the technicians and artists.


Daniele in the heat of staging work. (Photo: Philipe Leblond)

Faced with the sheer magnitude of the task at hand – extras, singers, technicians, stage managers etc., all equipped with radio receivers, in-ear monitors or intercoms – Daniele, the stage director, personally handled the cues regarding the staging of the show.
He delegated the cues concerning the dancers to Bryn Walters, the lead choreographer, while Maria Bonzanigo, the principal composer, did the same for the various musical ensembles.

This unique configuration allowed me to push the Clear-Com system to its limits. With the help of the embedded control software EHX and Dynam, I was able to modify the key assignments on demand and almost in real time, according to the rehearsal schedules, or leave the possibility to do so, for example, to the stage managers.”

When asked why the UHF band wasn’t used, Philippe’s answer is indisputable: No way. All the available bandwidth between 470 and 698 MHz is in use by the RF links of the microphones and in-ear monitors. The only solution was to move out of this overcrowded portion of the spectrum, by using the DECT standard which operates between 1.880 and 1.920 GHz. This technology is based on the allocation and dynamic distribution of channels and bandwidth according to the number of connections. To put it simply, the operating principle is similar to that of our mobile phones.

The calm before the storm, but where is Priscille, Doum’s assistant? (Photo: Philippe Leblond)

Each beltpack is constantly searching for an available antenna, preferably the nearest one, while taking into account the user’s movement. This is what is referred to as “roaming”. The limitation of the system is that it is impossible to exceed ten simultaneous communications per antenna, which means that the 11th will automatically interconnect or not with another one, hence the importance of distributing them properly. Their placement will therefore depend on the distribution of Freespeak units. Of the 60 being used, 40 of them are dedicated to stage managers and stagehands.

These are located both at the rear of the four stages located on level 1 (5.5 m in height), and at level 0 where the two hydraulically operated stairways that can be fully opened are located, but also on the Field of Play through the four vomitories. The coverage area therefore includes the entire Arena, the backstage areas and the ambulatory hidden under the grandstands.

Ten Freespeak IP antennas were installed 30 meters away on the towers at the back of each stage, as well as at the North and South main gates. This latest generation of TCVR-IP antenna is connected to the base station via the AES67 network using configurable and, above all, compatible switches. So let’s meet a little guy who is rather tall, discreet but very efficient.

Sharing and interoperability: Where are we in 2019?

A new profession means a new opportunity for young people and Baptiste Huguet has everything it takes! With his degree as a network administrator in his pocket, he could have applied for a job in a bank. Instead, he wanted to do shows and be alive! He therefore enrolled in a two-year work-study program at the CFA in Paris, the well known CFPTS.
He was torn between sound, lighting and video, but he chose lighting. Now he is looking for an employer. This will be the Dushow group, which has understood very well its need to integrate this type of profile into its staff, in order to be able to look forward to the next twenty years with peace of mind.

At the Dushow facilities, the trial assembly of the four Gigacore 16 XTs and twelve Gigacore 14 Rs. All connected by optic fiber. (Photo: Baptiste Huguet)

Upon completing his degree, he was hired on a permanent contract. He will not only remain confined to the warehouse: his work is in the field. His job is to oversee the deployment of the lighting network and its proper operation.
Was it possible to combine the audio, lighting, video and intercom networks on this event, with a high technological added value? No one dared to take up the challenge. It was too soon. Maybe next time?
The audio – over – IP is distributed over two separate Dante networks, in a double star configuration. The first one is dedicated to live sources, outputs to the different amplification systems and to the intercom matrix. The second is dedicated to virtual soundcheck, daily recordings and the Ovation playback in AES67.

A debut of interoperability: one small step for Audinate, one giant leap for AES67. As you may have understood, there is no room for intercom channels and AES67 and even less for ArtNet, despite the use of 34 Cisco SG 350 managed switches with 24 ports – four of which are equipped with fiber – and eight SG 350 48-port switches. There will be sharing between lighting and intercom.

For our nearsighted readers, a closer look, red into red and blue into blue. (Photo: Baptiste Huguet)

722 fixtures, two grandMA2 Full Size, one grandMA2 Light and one Ultralight consoles, two Command Wings, eight NPUs, four Robe RoboSpot remotely controlled followspots and 12 Luminex Node8 MKIIs for data distribution will coexist on the network that was designed by Baptiste:
Two rings for ArtNet, MA-Net, RTSP for the RoboSpot cameras and IVC 32 of the Clear-Com matrix for wired intercoms, plus a third ring dedicated to AES67 for Clear-Com’s IP antennas and the new panels.

“I chose the Luminex Gigacore switches because I had 170 watts of manageable Power-over-Ethernet per port to power them,” says Baptiste. “On this LAN inside the arena, I also interconnected physical star sub-networks composed of PoE switches (Netgear GS110 TP) to supply power and data to the comms panels.
Faced with Doum’s need to connect all the remote sites, I created an external network with a star topology that I linked to the rings of the arena via Netgear GS724T switches using dark fibers provided by the local vendor.

To monitor the proper operation of the Gigacores, I used the manufacturer’s Araneo software, as well as The Dude server client software with a Mikrotik router implemented as a server in the network to check the status of all the switches, but also of the inverters and the bandwidth of the Trunks.

The monitoring software: when it’s green, everything is fine; if it’s red, it’s the beginning of the end, and what does the Dante Controller say? A screen shot during the test phase conducted in Nice in January by Ludovic Morin. (Photo: Ludovic Morin)

To run Clear-Com’s Agent IC application and the telephone number call system from mobile phones to the matrix, I requested a public IP address, which I administered using Ubiquiti’s Edge router.

The multi-core fibers were spliced to the required lengths on site by Hugo. (Photo: Hugo)

Thanks to this system, in the event of a station failure, for example, Doum could be reached via his matrix from anywhere in France.
Many thanks to Baptiste, because of you, we feel a little less helpless when faced with this nebula.

Time flexibility: Show Control

Now let’s look at what’s happening in terms of synchronization. It would have been inappropriate to conceal my very close relationship with Ovation, a tool that, in my opinion, has become an essential part of this kind of show. At some point in my working life, I made the choice to leave the business to become a product manager at SCV Audio (old French high tech distributor, now Freevox). One of the brands I was responsible for was Merging Technologies.
Studio and broadcast technicians are familiar with the Pyramix recording, editing and mixing software, which has made its mark in the elitist world of classical orchestra recording, thanks to its cards with analog preamps and very high-end converters.

Ovation, surrounded by its friends, the Mif4s from Rosendhal, and the Merging+ANUBIS – the latest addition from Merging Technologies – atop the Mackie console on the right. This is a network interface that ensures, among other things, that AES67 passes through the meanderings of the DANTE network (Photo: Florian Baume)

In 2011 I discovered Ovation. It meets the demand for cross-functionality between different players in sound, lighting and video, which is essential for a smooth-running show.
This tool is used on many shows, including all those at Puy du Fou and Le Roi Lion et les Rythmes de la Terre, the latest addition to the Disneyland Paris park.

The sound effects, lighting, video playback or character entries can be the triggers.
It is possible to coordinate all the sectors via the different command protocols proposed by Ovation (IP, Midi, TC, OSC), thus fulfilling the director’s requests. For the Fête des Vignerons, each scene uses a 25-frame LTC time code, calibrated at various times.

Then, this is distributed via the DANTE network to all of the audio and lighting consoles, as well as to the SMODE, which manages the distribution of all the media used in the FoP and the blades, the screens positioned at the bottom of the four stages to establish the boundaries of their space. The sequencing of the console memories, all sectors included, is dependent on the proper operation of time code.

The show callers, from left to right: Sébastien Fevre, Daniele and Pietro Paolucci on the day of the event. (Photo: Sebastien Fevre)

The key elements – usually visual staging placements – are coordinated by Sébastien Fevre and Pietro Paolucci, the two showcallers (topeur in French), as it is a live show.
The possibility to work with several time lines, one per cue list, allowed the simultaneous reproduction up to four different scenes, a very useful feature on rainy days.

Underneath each stage, we were able to improvise independent rehearsal rooms. In addition to ensuring that all the various and diverse events are synchronized, Ovation also provides a multitrack cue playback using Pyramix as a framework. At any time, it is possible to edit, combine or merge the sounds to be played. This is very useful in light of the many changes that were made!

The orchestra playback was progressively supplemented with the stereo stems of the various choirs, in order to enhance their intelligibility. The matrix function was very helpful for sending cue tracks, clicks and various counts in the different wireless channels, with independent level management, depending on the intended purposes.
An extra doesn’t need to hear the click, whereas it is essential for the various musicians. The same is true for orchestra playback in the wireless channel of choir members. So, the show must go on!

The cycle of life.

From the invisible we plunge into the world of creativity: the world of Alexis Bowles’ lights, the poetry of Roberto Vitalini’s images, which have sublimated this story, the story of the cycle of life.

I would like to thank all the video technicians from the company Alabama, whom I unfortunately cannot name for fear of forgetting one, as well as those from the lighting department. There is one who braved all the storms: special thanks to Jean-François Leclercq, the logistics liaison for the Dushow group.

I leave you with pictures, great pictures…

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Stardraw.com reaches 1,000th manufacturer milestone

Software provider Stardraw.com announces the addition of the 1,000th manufacturer to the library of their award-winning design and documentation software, Stardraw Design 7, currently in release version 7.3.
This hugely significant milestone is the result of dozens of man-years of work on what is the most comprehensive, high quality line-art symbol resource available to the pro AV industry.

The Symbols Library, which now contains an impressive total of over 110,000 symbols of some 40,000 products, has been an integral part of Stardraw’s design software since 1992, and has been one of the features that sets Stardraw.com products apart.
Each symbol is drawn in house by Stardraw.com’s professional drafting team to ensure a consistent qualitative standard. All symbols are vector-based line art and, thus, resolution-independent meaning that the more you zoom in, the more detail you see, and even at the highest zoom levels there is none of the ‘blockiness’ exhibited by bitmap (raster) images.

The addition of new products to the library is prioritized based on user requests submitted through Stardraw’s online Product Request Service; this is another feature that is unique to Stardraw and ensures that only products relevant to the user base feature in the library.
“Since we have an installed user base operating in different industry segments across nearly 90 countries worldwide, it’s impossible for us to guess what particular products might be important for any particular integrator,” explained CEO Rob Robinson.

“Requirements vary hugely from market to market and country to country, so rather than randomly scraping catalogue data for products that may or may not be useful to our users, we encourage our users to drive the process themselves via Product Requests to keep the libraries relevant to their needs. All we require is the manufacturer name and product model number and we’ll do the rest.
To ensure that the system remains democratic, we recently implemented a Fair Use policy by means of a Product Request Allowance based on the level of your subscription to ensure that product requests are properly and fairly prioritized. This speeds up the process for everyone and enables requested products to be published even faster.”

Symbols include technically accurate Block Schematic representations showing discrete inputs and outputs, Rack Layout and Pictorial Schematic representations showing, where data is available, graphically accurate front and rear view detail, side view depths and, where appropriate, Panel Layout symbols with high detail front and rear views for creating custom connection plates, and Plan View symbols that conform to the J-STD-710 standard, “Audio, Video and Control Architectural Drawing Symbols”.

For further information, please visit the Stardraw website