Discovery Gaming Community - Ageira Innovations

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Flight log: Jay Anderson

This is a report from Dark Matter Survey mission to Kepler system. Samples were collected from all three dark matter clouds in the system. Spectral analysis of particles was conducted and results are uploaded to Neural Net.

Mission log attached.

824-02-03 15:50 Departed from Dortmund station, load out for research mission [link][link]
824-02-03 15:55 Entered Hudson system.
824-02-03 15:57 Passing Texas system.
824-02-03 16:02 Passing New York system.
824-02-03 16:08 Jumped to Kepler system.
824-02-03 16:12 Moved on to waypoint #1 in Denko cloud.
824-02-03 16:12 Collecting samples at waypoint #1.
824-02-03 16:15 Moved on to waypoint #2 in Denko cloud.
824-02-03 16:15 Collecting samples at color=LightSkyBlue]waypoint #2.
824-02-03 16:17 Moved on to waypoint #3 in Denko cloud. Nome base on scanners at waypoint #3.
824-02-03 16:18 Collecting samples at waypoint #3.
824-02-03 16:33 Moved on to waypoint #4 in Matsuo cloud.
824-02-03 16:33 Collecting samples at waypoint #4.
824-02-03 16:34 Located wreck of Kusari transport with cargo of Semiconductors.
824-02-03 16:38 Moved on to waypoint #5 in Matsuo cloud.
824-02-03 16:38 Collecting samples at waypoint #5.
824-02-03 16:40 Visual on wreck of trade lane ring.
824-02-03 16:40 Moved on to waypoint #6 in Matsuo cloud.
824-02-03 16:40 Collecting samples at waypoint #6.
824-02-03 16:42 Visual on wreck of trade lane ring.
824-02-03 16:48 Moved on to waypoint #7 in Kuryo cloud. Unknown battlecruiser spotted, might be damaged, transponder is unreadable.
824-02-03 16:48 Collecting samples at waypoint #7.
824-02-03 17:07 Scanned jump anomaly connected to Cassini system. Reading uploaded.
824-02-03 17:10 Moved on to waypoint #8 in Kuryo cloud. Collecting samples at waypoint #8.
824-02-03 17:12 Readings of transport McKinley spotted. Cargo recovered, samples taken.
824-02-03 17:12 Returned to Pueblo Station in Colorado system.

Flight log: Jay Anderson

New report from Dark Matter survey mission just arrived. Ageira~Oort successfully completed sampling of Dark Matter clouds present in Galileo system. Something interesting was found along the way related to Lane Hackers presence in the system.

Mission log attached.

824-03-16 7:05 Departed from Pueblo station [loadout][loadout]
824-03-16 7:12 Entered Galileo system.
824-03-16 7:12 Survey plan for Reppu cloud.
824-03-16 7:16 Moved on to waypoint #1 in Reppu cloud. Collecting samples at waypoint #1.
824-03-16 7:21 Moved on to waypoint #2 in Reppu cloud. Collecting samples at waypoint #2.
824-03-16 7:25 Moved on to waypoint #3 in Reppu cloud. Collecting samples at waypoint #3.
824-03-16 7:33 Survey plan for Komatsu cloud.
824-03-16 7:35 Moved on to waypoint #1 in Komatsu cloud. Collecting samples at waypoint #1.
824-03-16 7:38 Moved on to waypoint #2 in Komatsu cloud. Collecting samples at waypoint #2.
824-03-16 7:38 Lane Hackers installation on long range scanners, identification uncertain.
824-03-16 7:38 Lane Hackers Leiden Base on long range scanners. Coordinates corrupted by the dark matter cloud field.
824-03-16 7:43 Moved on to waypoint #3 in Komatsu cloud. Collecting samples at waypoint #3.
824-03-16 7:47 Survey plan for Raiden cloud.
824-03-16 7:49 Moved on to waypoint #1 in Raiden cloud. Collecting samples at waypoint #1.
824-03-16 7:52 Moved on to waypoint #2 in Raiden cloud. Collecting samples at waypoint #2.
824-03-16 7:56 Moved on to waypoint #3 in Raiden cloud. Collecting samples at waypoint #3.
824-03-16 8:12 Returned to Pueblo Station in Colorado system.

To: Jay Anderson, Chief Executive Officer, Ageira Innovations

Dear Mr Anderson,

The Legal Department has received an information that you were looking for a certain documentation dating back to the founding and early days of our branch of Ageira Technologies. I am happy to inform you that I have all the information you seek.

Ageira Innovations was founded on 821-03-14 A.S. by Mr Sebastian Haart ^{[security profile]} and Mr Anthony Hall ^{[security profile]}. While Mr Hart designed almost entire structure of the company, including transmission protocols, internal procedures and overall structure we do still use today, Mr Hall focused on building our transportation wing and strengthening our exports. Shortly after initial organization, Mr Hart decided to focus his energy solely on scientific endevours and limited his role to a Director of R&D Department, while Mr Hall became Director of Jump Gate and Trade Lane Network Department. In order to strengthen the company management Mr Haart and Mr Hall decided to hire a professional Chief Executive Officer on 821-03-28 A.S., Mr John White ^{[security profile]}. As you know Mr White was successfully holding this position until 823-04-17 A.S. excluding period between 822-04-10 A.S. and 822-11-21 A.S., during which time Mr Haart shortly served a role as an Acting Chief Executive Officer ^[resource]. After Mr White's return Mr Haart returned to his personal lab and did not hold any official posts in Ageira Innovations ever since.

Should you need them Mr Anderson, The Legal Department has a copy of all documents ^[resource] prepared by Mr Haart. Should you have further questions you may try to reach Mr Haart directly. While I was told that he does not wish to be disturbed, I am more than sure he will respond to the current CEO of Ageira Innovations.

Kind regards,
Edison Lawrence,
Managing Director of Legal Department,
Ageira Innovations

To: Edison Lawrence, Legal Department

Mr. Lawrence, your level of awareness is just as impressive as the accuracy and level of details in your report. You confirm my confidence that our legal affairs are handled with utmost excellence.

I can only admire the brilliance of the members of Ageira once more, and I'm proud to be in charge of such superior organization.

Jay Anderson,
Ageira Innovations

Flight log: Tango-11

Today I got report from Ageira Tango wing unit. It was given a task to pick up certain materials from Mr. Finnugor. The unit met Mr. Finnugor near Durango planetoid in Colorado space. The following materials were passed:

824-04-26 15:21- Nomad Countermeasure Ammo

Tango-11 then proceeded to Alberta system and delivered the materials to Anomalous Materials Lab arranged on board of Leduc Station.

824-04-26 15:40 - Delivery manifest

Jay Anderson,
Ageira Innovations

Flight log: Jay Anderson

Today I took Leonov to mission in remote corner of Sirius sector: Omicron Delta system. My vessel delivered 780 Gravity Field Stabilizers ordered by The Core. The journey was remarkably uneventful for such high risk route.

824-04-30 05:40 Arrived in Omicron Rho via Sigma-15
824-04-30 05:42 Jumped to Omicron Delta
824-04-30 05:43 Delivered 780 Gravity Field Stabilizers to Yaren base
824-04-30 06:19 Delivered 3920 Iridium from Yaren base to Fort Severn

Jay Anderson,
Ageira Innovations

To: Ageira Innovations Executive Leadership
Sender ID: Otto Muller
Encryption: Dual alphanumeric anaglyph
Encryption level: High
Signal strength: High

::/Loading message...

Gentlemen,

We all remember the terrible tragedy in Kepler system. The storm of dark matter, which began deep in Omicrons, caused significant damage in the inhabited systems too. But now we shouldn't take this as a tragedy. This is a huge field for experiments. To discover new knowledge. After some discussions with Dr. Fairchild, the head of Dark Matter projects, and Mr.Anderson, the first of us, who seriously engaged in the problem of dark matter, we decided to send an expedition deep into the Kuryo cloud.

Expedition ship:

Ship's ID: Ageira~Rontgen
Class: Research vessel][Cargo vessel
Captain: Otto Muller
Crew: 4 people (+3 surveys team)
Short history: The "Rentgen" began life in the 800th A.S. Initially, it was a fully cargo ship belonging to a small trading company "Frame Works". In 817th A.S the company went bankrupt and was forced to sell the ship to the Junkers, who used it for collecting scrap. In 820th A,S the ship was seriously damaged by an unknown pilot with LSF-signature. In the 824th A.S the ship was bought by Ageira corp and was re-equipped as a research vessel.

Subject of interest:

Mr.Anderson Wrote:Being engulfed in dark matter storms in the past, these systems represent the aftermath of such cataclysmic event and give us a chance to study the long-term effects of it. Dark Matter Lab is interested in samples from the fragments of clouds that fill those two systems for comparison analysis with samples from other systems.

Kuryo Cloud

Dark matter cloud known as Kuryo Cloud is one of the three dark matter clouds, located in Kepler and this is the biggest one. In addition to the size, the cloud is ineresting for us because many multiple signatures were detected deep inside. Remains of trade lanes are interesting for Ageira too. On the other hand... There are many hostile signatures. We are not sure, but we think there is a wormhole inside the cloud. We reached this cloud at 8:52, 825 A.S, 04, 20. We detected, that scanners range is reduced in this cloud, so it's a great opportunity for Lane Hackers and others.

Cassini Jumphole

Wormhole (Is a natural phenomenom in spacemaking possible to make a jump from one system to another in Sirius) connected with Cassini system was found in this cloud at 5E sector. It explains the increased activity of hackers in this place. I scanned this wormhole and got this information...

::/Opening file: Report_X452-B.rpr...

Type: STABLE
Maximum permissible class of the ship: CRUISER (Battleships are allowed too, but it can be dangerous)
Closing time: UNKNOWN

McKinley

We found remains of The Universal large transport McKinley at 09:09. Looks like, that it was hauling superconductors. All systems of the ship were disabled, we didn't find any crew's remains. We take the samples from cargo and got some scrap from the armor. Weapons were unmounted and placed in cargohold of the "Rontgen". We don't say even something without careful analysis, but we found some logs in the black boxes. I will send it a bit later. The hull of the ship is covered with an unknown substance... I think, that it is the result of the interaction of the alloy in the hull and dark matter. We left these debris and continued on our way...

Remains of trade lanes

Spoiler

We found requested remains of trade lanes. Power core is destroyed or blown up, so nothing surprising, that they are out of action. Unfortunately, nothing more can be said without laboratory analysis.

Battlecruiser Wyoming

During the preparation of samples from the last ring of trade lane located in Kuryo we found unknown signature. When we flew closer, we found that it was Battlecruiser "Wyoming". We thought that it was located here to protect this area from pirates, but when we tried to contact... It opened fire on us. I have no idea why. We covered and activated long-range scanners...

::/Opening file: Report_X453-G.rpr...

CLASS: Interdictor
ARMAMENT: CLASSIFIED
CREW: CLASSIFIED
Date of building: 820 A.S
Signature: ERROR UNKNOWN SIGNATURE WAS DETECTED

Results

All samples were delivered to Pueblo Station. We have already started working with them and we will show the first results as soon as possible. In addition, 32 hackers were captured with help of pilots from Bounty Hunters Guild. The researching of black matter is important for all of us. Its potential is huge. We can create engines based on black matter, research possible reactions with metals. Kepler is a huge field of experiments and new discoveries for us. We hope that other clouds of the system will be so rich for surprises.

To: Otto Muller

Once again I'm glad to see you doing excellent job, Mr. Muller. The samples you collected, especially the materials exposed to dark matter over time, are invaluable to Science Department. Dr. Fairchild shared the results of the initial tests with me just yesterday, and I must admit that they look extremely promising. As you know, our plans regarding research mission in Kepler are on track, and the survey you conducted will help to advance them further.

You will be rewarded for the assignments you completed and your employee dossier will be updated accordingly. Please, keep it up.

Jay Anderson,
Ageira Innovations

Flight Log: Clarissa Fairchild, Ageira~Oort

As you know, I'm currently on a mission in Munich system, a part of Dark Matter Survey initiative. The system proved to be quite interesting and have real good potential for goals of our research. Today I report the first series of sampling and tests conducted within dark matter cloud that surrounds Planet Bodensee. More reports are pending for our ongoing activities in the system.

824-06-11 22:42 Survey plan for Bodensee cloud.
824-06-11 22:42 Moved on to waypoint #1 in Bodensee cloud. Collecting samples at waypoint #1.
824-06-11 22:47 Scanning atmosphere of Planet Bodensee with spectrometers and scanners in all wavelengths.
824-06-11 22:49 Moved on to waypoint #2 in Bodensee cloud. Collecting samples at waypoint #2.
824-06-11 22:54 Moved on to waypoint #3 in Bodensee cloud. Collecting samples at waypoint #3.
824-06-11 22:57 Observing anomalous particles outside boundaries of mass for dark matter particles.
824-06-11 23:00 Moved on to waypoint #4 in Bodensee cloud. Collecting samples at waypoint #1.
824-06-11 23:02 Scanners detected wreck of trade lane rings, position marked for later detailed inspection.

Clarissa Fairchild,
Ageira Innovations

Flight Log: Clarissa Fairchild, Ageira~Oort

This is the second report from Munich survey mission. This time it was long range observation flight to the outer edge of heliopause of Munich sun. The goal is to explore configuration of dark matter clouds in the system.

The cloud of dark matter that engulfs Munich assumed form of sphere, approx. 80K radius with a center on the Munich main star. The cloud contains no larger bodies, but emits intense radiation. The spectral analysis of the radiation is usual for the dark matter nebulae.

The cloud itself doesn't seem homogeneous upon initial analysis. There are turbulent zones with varied density of dark matter particles and intensity of radiation. The form of the cloud and the streams observed within it make it evident that the dark matter masses were dragged by the gravity of the central star and formed a kind of maelstrom, with the dark matter moving around the start in spiral.

During two dives into the cloud, we measured the radiation, density gradients and relative speeds of different parts of the maelstrom.

824-06-24 06:01 45K to zenith from Neu Augsburg Outpost. Inside the dark matter cloud. Radiation A = 12*10^8 Bq
824-06-24 06:05 135K to zenith from Neu Augsburg. Outside the main cloud formation.
824-06-24 06:06 Walker nebula observed through secondary outcroppings of the cloud for spectral analysis.
824-06-24 06:07 Moving on to waypoint #1 in Schwarzwald cloud.
824-06-24 06:10 95K to waypoint. Close to the upper boundary of the dark matter cloud. Edge nebula observed through cloud matter for spectral analysis.
824-06-24 06:11 External radius of the cloud ~80K from the main star of Munich system.
824-06-24 06:12 Particles of dark matter on spectral scanners in external layers of the upper region of the cloud.
824-06-24 06:15 Internal radius of the dark matter cloud ~45K from the main star. Particles of dark matter observed by spectral scanners.
824-06-24 06:19 On the waypoint #1. A = 7.3*10^8 Bq.
824-06-24 06:25 External radius of the nadir portion of the cloud is ~80K from the central star.
824-06-24 06:28 Both stars of Munich system observed through the dark matter cloud for spectral analysis of the dark matter.
824-06-24 06:33 Internal border of the cloud at ~30K from the main star. A = 9.1*10^8 Bq.

Clarissa Fairchild,
Ageira Innovations

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