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pejuangcod · 4 years ago

Text

beatbind

Ecosystem for Music Events

BeatBind Platform

BeatBind is the industry's long overdue platform for music event organization. We’re developing a multi-stage business, each level standing on top of the other, to tackle each of the industry's 4 prevailing issues:

BeatBidder - A platform for connecting venues, DJs, artists, and all other parties involved in the music event organization process. We connect DJs, artists, venue owners, and everybody else involved in the music event organization process in order to provide the best opportunities for all. Leveraging auction systems, we strive to both increase revenue for the most in-demand DJs and venues, while the sheer size of the market cuts costs and lowers entry barriers for virtually everyone who takes part in creating music events. BeatBind also counts promotions, sponsorships and event organization outsourcing among the services that can eventually be exchanged on the platform.

BeatBuy - Ticketing will be a default feature of any event created on BeatBind, which will directly be sold and offered to our fanbase, massively decreasing entry barriers. This prevents ticket scalping, forgery, and the rise secondary markets that steal $8 billion annually from the creators of events. BeatBuy will eliminate this problem and bring that money back to the pockets of artists, organizers, and all businesses that actually create the experiences..

BeatX - App giving fans the impact they need to shape the even they're attending, and event-oriented experiences like dating. Fans will have access to newsfeeds and will be engaged in multiple ways to help the organizers better shape the very events that those same fans are attending. In order to ensure the integrity of all transactions and to protect all parties, we plan to introduce a rigorous escrow protocol for refunding money in case of failed transactions and handling disputes

BeatAI - Providing revenue projections and other heuristics that helps all platform users to decide whom to hire, where to perform, etc. Our platform will use machine learning to produce revenue estimations to help you justify decisions in any part of the music event organization process. This will greatly reduce risk and spur even more growth. We believe this is just the step the industry needs to take to step out of the dark caused by the lack of data, and make better decisions.

The Solution: BeatBidder

4 stage platform

Artists are paired with venues and organizers.

Let's say you're a DJ, and you want the best deal for a Friday night performance. Let venues compete for you! Show off your portfolio, choose when you're available for a show, and let event organizers outbid each other as you get better and better offers.

BeatBind Platform benefits all parties in the music events industry:

Music groups - let venues & organizers bid on you, increasing your revenue

Event organizers - let musicians bid on your opportunity, so you lower your expenses, and get the best

Venue owners - outsource event organization to the most passionate managers

BEATBUY FOR FANSFANS

"Ticket reseller sites illegally inflate prices by up to 500%.” ―Choice, Consumer Rights Group

Seamless Ticketing for BeatBind Events

Direct access to tickets for all BeatBind events

Transparent pricing, no chance of fraud, forgery, or ticket scalping

Fans have the ability to return tickets and get refunded

Fans can pre-purchase tickets as an event is organized

Seamless Crowdfunding for BeatBind Events

Our superior ticketing system supports purchase of tickets for currently organizing events, allowing an initial inflow of capital to organizers

This form of seamless crowdfunding gives smaller venues the means to bring in big stars

All money is refunded to fans if the event doesn’t materialize

BEATX

“We see our customers as invited guests to a party, and we are the hosts. It’s our job every day to make every important aspect of the customer experience a little bit Better.” - Jeff Bezos, Founder @ Amazon

BeatBind Mobile App will help fans keep up with what their favorite artists and venues have in store for them. They will be drawn to any available ticket sales, events, or updates relevant to them immediately. But BeatBind offers much more than just buying tickets: they will be able to access much more value in terms of bidding for backstage access to artists.

BeatAI

"There are no statistics. We just advertise and hope they come." ―Anonymous industry insider

The above quote is what we heard when we asked one of our big music industry contacts to share his marketing know-how. This quote summarizes the current approach in the entire industry to estimations, from determining the profitability of promotions to hiring the very artists central to events. It resembles shooting in the dark more than the empirical data-driven approach that has consistently proven to produce best results.

TOKEN

The utility token of the BeatBind ecosystem. The ultimate vision of BBND is to be a universal medium of exchange for the music events industry. Ethereum blockchain provides all the privacy, security and decentralization that such a token deserves. BBND will be traded on public exchanges, but BeatBind platform users are protected from the price volatility during everyday use. The full list of BBND use cases is described in the whitepaper.

Pre IEO - Start: Jan 15, 2021

Pre-Sale Discount: 40% to the IEO launch price of 0.05 USD

Pre IEO - End: March 15, 2021

Pre - IEO Price: 0.03 USD

Available Supply: 1 Billion BBND utility tokens

Acceptable currencies: ETH, BTC, LTC, USDT, BSV

Use of Proceeds

ROADMAP

TEAM

Bosko Gasic: Founder/CEO

Dale Baeten: Co-Founder/COO

Akash Syed: Chief Technology Officer

Doc Ish: Chief Innovation Officer

Ivica Panic: Chief Marketing Officer

Goran Beko: Chief Design Officer

ADVISORS

William Scott Boatman

Daryl Naidoo

Nebojsa Sataric

DEVELOPERS TEAM

Tapendra Shee: Blockchain Architect

Rasel Mahmud: UI/UX Developer

Andrey Romanov: Coin Offering Specialist

Glennbert Ferrer: Community manager

Uros Jovanovic: Copywriter

Elza Hovhannisyan: Junior Marketing Specialist

For More Information Click Links Bellow:

Website: https://www.beatbind.io/

Whitepaper: https://www.beatbind.io/public/template/assets/whitepaper.pdf

Telegram: https://t.me/beatbindutilitytoken

Facebook: https://www.facebook.com/beatbind/

Twitter: https://twitter.com/beat_bind

Author: pejuang cod

My Bitcointalk Profile: https://bitcointalk.org/index.php?action=profile;u=2699227

ETH Address: 0x29AF24D027E5A0A74427A2A4D5dDFe09803D5F93

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khanshiqqheil · 4 years ago

Text

beatbind

Ecosystem for Music Events

BeatBind Platform

The Solution: BeatBidder

4 stage platform

Artists are paired with venues and organizers.

BeatBind Platform benefits all parties in the music events industry:

Music groups - let venues & organizers bid on you, increasing your revenue

Event organizers - let musicians bid on your opportunity, so you lower your expenses, and get the best

Venue owners - outsource event organization to the most passionate managers

BEATBUY FOR FANSFANS

"Ticket reseller sites illegally inflate prices by up to 500%.” ―Choice, Consumer Rights Group

Seamless Ticketing for BeatBind Events

Direct access to tickets for all BeatBind events

Transparent pricing, no chance of fraud, forgery, or ticket scalping

Fans have the ability to return tickets and get refunded

Fans can pre-purchase tickets as an event is organized

Seamless Crowdfunding for BeatBind Events

Our superior ticketing system supports purchase of tickets for currently organizing events, allowing an initial inflow of capital to organizers

This form of seamless crowdfunding gives smaller venues the means to bring in big stars

All money is refunded to fans if the event doesn’t materialize

BEATX

BeatAI

"There are no statistics. We just advertise and hope they come." ―Anonymous industry insider

TOKEN

Pre IEO - Start: Jan 15, 2021

Pre-Sale Discount: 40% to the IEO launch price of 0.05 USD

Pre IEO - End: March 15, 2021

Pre - IEO Price: 0.03 USD

Available Supply: 1 Billion BBND utility tokens

Acceptable currencies: ETH, BTC, LTC, USDT, BSV

Use of Proceeds

ROADMAP

TEAM

Bosko Gasic: Founder/CEO

Dale Baeten: Co-Founder/COO

Akash Syed: Chief Technology Officer

Doc Ish: Chief Innovation Officer

Ivica Panic: Chief Marketing Officer

Goran Beko: Chief Design Officer

ADVISORS

William Scott Boatman

Daryl Naidoo

Nebojsa Sataric

DEVELOPERS TEAM

Tapendra Shee: Blockchain Architect

Rasel Mahmud: UI/UX Developer

Andrey Romanov: Coin Offering Specialist

Glennbert Ferrer: Community manager

Uros Jovanovic: Copywriter

Elza Hovhannisyan: Junior Marketing Specialist

For More Information Click Links Bellow:

Website: https://www.beatbind.io/

Whitepaper: https://www.beatbind.io/public/template/assets/whitepaper.pdf

Telegram: https://t.me/beatbindutilitytoken

Facebook: https://www.facebook.com/beatbind/

Twitter: https://twitter.com/beat_bind

Author: KHAN SHIQ QHEIL

My Bitcointalk Profile: https://bitcointalk.org/index.php?action=profile;u=2550289

ETH Address: 0xa809395b84354d256302D97d5C68AaEE9EF84005

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batupermata · 4 years ago

Text

beatbind

Ecosystem for Music Events

BeatBind Platform

The Solution: BeatBidder

4 stage platform

Artists are paired with venues and organizers.

BeatBind Platform benefits all parties in the music events industry:

Music groups - let venues & organizers bid on you, increasing your revenue

Event organizers - let musicians bid on your opportunity, so you lower your expenses, and get the best

Venue owners - outsource event organization to the most passionate managers

BEATBUY FOR FANSFANS

"Ticket reseller sites illegally inflate prices by up to 500%.” ―Choice, Consumer Rights Group

Seamless Ticketing for BeatBind Events

Direct access to tickets for all BeatBind events

Transparent pricing, no chance of fraud, forgery, or ticket scalping

Fans have the ability to return tickets and get refunded

Fans can pre-purchase tickets as an event is organized

Seamless Crowdfunding for BeatBind Events

Our superior ticketing system supports purchase of tickets for currently organizing events, allowing an initial inflow of capital to organizers

This form of seamless crowdfunding gives smaller venues the means to bring in big stars

All money is refunded to fans if the event doesn’t materialize

BEATX

BeatAI

"There are no statistics. We just advertise and hope they come." ―Anonymous industry insider

TOKEN

Pre IEO - Start: Jan 15, 2021

Pre-Sale Discount: 40% to the IEO launch price of 0.05 USD

Pre IEO - End: March 15, 2021

Pre - IEO Price: 0.03 USD

Available Supply: 1 Billion BBND utility tokens

Acceptable currencies: ETH, BTC, LTC, USDT, BSV

Use of Proceeds

ROADMAP

TEAM

Bosko Gasic: Founder/CEO

Dale Baeten: Co-Founder/COO

Akash Syed: Chief Technology Officer

Doc Ish: Chief Innovation Officer

Ivica Panic: Chief Marketing Officer

Goran Beko: Chief Design Officer

ADVISORS

William Scott Boatman

Daryl Naidoo

Nebojsa Sataric

DEVELOPERS TEAM

Tapendra Shee: Blockchain Architect

Rasel Mahmud: UI/UX Developer

Andrey Romanov: Coin Offering Specialist

Glennbert Ferrer: Community manager

Uros Jovanovic: Copywriter

Elza Hovhannisyan: Junior Marketing Specialist

For More Information Click Links Bellow:

Website: https://www.beatbind.io/

Whitepaper: https://www.beatbind.io/public/template/assets/whitepaper.pdf

Telegram: https://t.me/beatbindutilitytoken

Facebook: https://www.facebook.com/beatbind/

Twitter: https://twitter.com/beat_bind

Author: Batu permata

My Bitcointalk Profile: https://bitcointalk.org/index.php?action=profile;u=1875984

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cryptonewsmanuelakanji · 4 years ago

Text

BeatBind

BeatBind aims to become the long-awaited platform for music event organization, with BBND being the cryptocurrency token used for all its transactions.

#crypto #beatbind #bbnd #trade #invest #ethereum

Beatbind Ecosystem for Music Events

BeatBind connects musicians, venues, event organizers and fans to create the most memorable music events on Earth.

BeatBind aims to become the long-awaited platform for music event organization, with BBND being the cryptocurrency token used for all its transactions.

The current state of the music events industry is highly fragmented, everyone's individual networks limiting their reach. The Internet proved that's not how the world needs to operate - as other industries move toward open digital solutions, the music event industry is lagging heavily behind. Scalping and ticket forgery steal value from organizers, and a lack of data mining and collection in the industry makes revenue predictions inaccurate, which in turn makes events risky ventures - hurting artists, venues, and fans equally

The Problem

Organizing an event of any size remains a slow and manual process, with high cost and connection barriers

Quality performers or venues are hard to reach

Lack of connections limits rising artists and new venues

Agencies and middlemen are slow, inflexible, and expensive

The Solution

stage platform

Artists are paired with venues and organizers.

BeatBind Platform benefits all parties in the music events industry:

Music groups - let venues & organizers bid on you, increasing your revenue

Event organizers - let musicians bid on your opportunity, so you lower your expenses, and get the best

Venue owners - outsource event organization to the most passionate managers

BeatBind Platform

1. BeatBidder

A platform for connecting venues, DJs, artists, and all other parties involved in the music event organization process. We connect DJs, artists, venue owners, and everybody else involved in the music event organization process in order to provide the best opportunities for all. Leveraging auction systems, we strive to both increase revenue for the most in-demand DJs and venues, while the sheer size of the market cuts costs and lowers entry barriers for virtually everyone who takes part in creating music events. BeatBind also counts promotions, sponsorships and event organization outsourcing among the services that can eventually be exchanged on the platform

2. BeatBuy

Ticketing will be a default feature of any event created on BeatBind, which will directly be sold and offered to our fanbase, massively decreasing entry barriers. This prevents ticket scalping, forgery, and the rise secondary markets that steal $8 billion annually from the creators of events. BeatBuy will eliminate this problem and bring that money back to the pockets of artists, organizers, and all businesses that actually create the experiences..

3. BeatX

App giving fans the impact they need to shape the even they're attending, and event-oriented experiences like dating. Fans will have access to newsfeeds and will be engaged in multiple ways to help the organizers better shape the very events that those same fans are attending. In order to ensure the integrity of all transactions and to protect all parties, we plan to introduce a rigorous escrow protocol for refunding money in case of failed transactions and handling disputes..

4. BeatAI

Providing revenue projections and other heuristics that helps all platform users to decide whom to hire, where to perform, etc. Our platform will use machine learning to produce revenue estimations to help you justify decisions in any part of the music event organization process. This will greatly reduce risk and spur even more growth. We believe this is just the step the industry needs to take to step out of the dark caused by the lack of data, and make better decisions.

FANS

"Ticket reseller sites illegally inflate prices by up to 500%.” ―Choice, Consumer Rights Group

Seamless Ticketing for BeatBind Events

Direct access to tickets for all BeatBind events

Transparent pricing, no chance of fraud, forgery, or ticket scalping

Fans have the ability to return tickets and get refunded

Fans can pre-purchase tickets as an event is organized

Seamless Crowdfunding for BeatBind Events

Our superior ticketing system supports purchase of tickets for currently organizing events, allowing an initial inflow of capital to organizers

This form of seamless crowdfunding gives smaller venues the means to bring in big stars

All money is refunded to fans if the event doesn’t materialize

Beatx APP

Beatbind AI

"There are no statistics. We just advertise and hope they come." ―Anonymous industry insider

Token Sale

Pre IEO - Start

Jan 15, 2021

Pre-Sale Discount

40% to the IEO launch price of 0.05 USD

Pre IEO - End

March 15, 2021

Pre - IEO Price

0.03 USD

Available Supply

1 Billion BBND utility tokens

Acceptable currencies

ETH, BTC, LTC, USDT, BSV

BeatBind Token Details:

● Ticker: BBND

● Platform: Ethereum

● Token Type: ERC-20

● Available for sale: 500,000,000 BBND (50%)

● Total supply: 1,000,000,000 BBND

● Pre-sale Price : 1 BBND = 0.03 USD

● Accepting: ETH, BTC, LTC, USDT, BSV

● Soft cap: 250,000 USD

● Hard cap: 5,000,000 USD

● Bonuses: Presale – 40%

BeatBind Roadmap

Q1 2021

Whitepaper

Seed Investments

Office & Incorporation

Platform Development Start

Q2 2021

Private Token Sale

BeatBind Community

Establishment

Platform POC Public Beta

Public Token Sale

BBND Exchange Listings

Q3 2021

Team Expansion

Feature Experimentation Start

Q4 2021

Platform Public Beta

EOY Status Report

Q1 2022+

Mobile App & Ticketing

Development Start

Platform Early Adoption

Community Quarterly Status Reports

BeatBind Team

Bosko Gasic – Founder/CEO

Dale Baeten – Co-Founder/COO

Akash Syed – Chief Technology Officer

Doc Ish – Chief Innovation Officer

Ivica Panic – Chief Marketing Officer

Goran Beko – Chief Design Officer

Advisors

William Scott Boatman – Legal & Business Advisor

Daryl Naidoo – IEO & Blockchain Advisor

Nebojsa Sataric – Business Development Advisor

Developers Team

Tapendra Shee – Blockchain Architect

Rasel Mahmud – UI/UX Developer

Andrey Romanov – Coin Offering Specialist

Glennbert Ferrer – Community manager

Uros Jovanovic – Copywriter

Elza Hovhannisyan – Junior Marketing Specialist

Conclusion

BeatBind and its corresponding BBND Tokens are not intended or offered as a security in any jurisdiction. This Whitepaper is not intended to constitute an offering of securities, a solicitation of investment, a prospectus or offering document in any jurisdiction. This Whitepaper neither represents any opinion or advice to purchase or sell tokens nor shall it or any part of it be relied upon for any contract or transaction decision. This Whitepaper is not a contract and is not binding any person or entity into any Agreement in relation to the purchase and sale of BeatBind Tokens. Any agreement for the the purchase of BeatBind Tokens shall be governed by a separate contract setting out the specific terms and conditions applicable to that transaction.

Here is how you can reach us:

Website: http://www.beatbind.io/

LinkedIN: https://www.linkedin.com/company/14055885/admin/

Medium: https://beatbind.medium.com/

Twitter: https://twitter.com/beat_bind

Instagram: https://www.instagram.com/beatbindgram/

FaceBook: https://www.facebook.com/beatbind/

Watch our Video: https://www.youtube.com/watch?v=dfkXPNsJrRA

Reddit: https://www.reddit.com/r/BeatBind_Master/comments/l97uv5/rbeatbind_master_lounge/

Bitcointalk.org: https://bitcointalk.org/index.php?topic=5187388

AUTHOR: Manuel Akanji

Bitcointalk Profile: https://bitcointalk.org/index.php?action=profile;u=2954998

Telegram Username: @Manuelakanji777

#crypto beatbind bbnd trade invest ethereum

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theuniversitychallengereview · 5 years ago

Text

UC 49.28-32, QF Mega-Blog

What better thing to do, when forced to stay at home during the outbreak of a global virus that threatens not only millions of peoples lives but the very fabric of society as we know it, than catch up on watching and writing about the quiz show whose previous four episodes you had missed for various reasons, all of which seem frivolous following the outbreak of a global virus that threatens not only millions of peoples lives but the very fabric of society as we know it. Also, I kept seeing that Twitter meme about Shakespeare having written King Lear during the plague quarantine and fancied getting involved.

Its also the only sport of any kind that can be found on TV for love nor money (apart from the Turkish Superlig, which for some reason thinks itself immune). Maybe the Premier League should try out pre-recording like the Challenge, for precisely this kind of situation. Just get Salah, De Bruyne and all the boys together for a few kick-abouts, film a few goals and slide tackles and all that, and keep the footage for a rainy day. Or send a camera round Serena Williams’ gaff, log a couple of serves and forehands, cut it together - BOOM, there’s your Wimbledon final if Greta decides tennis is too carbon-heavy.

All I’m saying is, you’ve never seen University Challenge postponed due to a global virus that threatens not only millions of peoples lives but the very fabric of society as we know it (although, as I write this I’m realising that the recordings of next years show will probably be delayed. Shit)

Episode 28 - Courtauld vs Imperial

Whenever I’ve not written one of these for a while it takes me a while to figure out what the heck it is I’m doing. Like, what do I usually write about? How have I managed to put out 118 of these? Do you reckon Shakespeare felt the same way when he was between plays - would he sit down with his quill and parchment and wonder aloud, ‘What the fuck is an iambic pentameter and how do I find one?’ (If I 1: knew the answer to that question; and 2: could be bothered, then I would have written that question in iambic pentameter, but you should know by now you’re dealing with one lazy blogger).

Anyway, Imperial had blazed aside all before them in the opening two rounds, thanks in no small part to the efforts of mercurial star Brandon, whose laconic style has drawn unfair criticism as arrogance. Thats how it always goes with the social media juries though - if a contestant displays any level of confidence above the bare minimum then they’re too big for their boots. But then if they grin and seem really happy when they get an answer that’ll probably annoy some people too. Almost as if they can’t win and there’s no point playing this game to appease the kind of people who get annoyed at kids on quiz shows.

The Courtauld side fall into the grinning category. They all four of them seem genuinely delighted to be on the show, and even more delighted that they managed to win two matches and make it to the quarter finals - their second round defeat of Glasgow a particularly impressive performance.

Glasgow were a good side, but Imperial are a different gravy, and Courtauld, after a neg on the opening question, seem like rabbits in the headlights (when they should have been at home, the whole country’s on lockdown, dammit Peter!) as Brandon sycthes down question after question, fearful to fall further below zero in case they can’t make it back up again.

For a while it looked as though that might end up being the case, as Imperial pranced into a hundred point lead within six questions, but Haigh finally stopped the rot, and Courtauld would add some respectability over the rest of the episode. In truth, it was clear from that point onwards that the race had been run, and Brandon seemed to relax from thereon out, and his teammates picked up the slack, though that seems like doing them a disservice, as they all seem very accomplished in their own right.

Final Score: Courtauld 75 - 240 Imperial

Episode 29 - Trinity, Cam vs Corpus Christi, Cam

Right, on to the next, and for Ep 29 we had our first Cam-Cam slugfest of the series. There had already been plenty of Ox-Cam derbies of course, you can’t move for them half the time, but no inter-collegiate battles thus far. Whoever won would become the first side to reach the semi-finals, with Trinity having beaten Manchester and Corpus Wolfson in their respective opening quarter final clashes.

Stewart, who doesn’t look like he would be out of place in the Byzantine Empire, gets Corpus off the mark with ‘Byzantine’ (I have basically no idea what this comparison would actually mean, or if it is in fact a sick burn, but I feel like he has an old-timey medieval look about him and felt like this should not go unaddressed. Like, he wouldn’t look strange wearing a tunic, would he?).

Russell and Wang increased the lead before Hughes got Trinity into the game with what looked like a semi-guess on a maths-y starter. Paxman, who clearly enjoys toying with the Corpus captain, then gets Wang for the second match in a row with a double serving of Boomer sarcasm. When Wang rather dejectedly says, ‘Its not Isaac Asimov, is it? No’, the quizmaster further interrogates him as to whether he was giving a question or an answer, much in the way an irritating geography teacher would parrot ‘Of course you can go to the toilet, the question is whether or not you may’. He’s right though, and Corpus gobble up two more bonuses on sci-fi writers.

Another starter went to Stewart, and a first for Gunasekera. Corpus were starting to look comfortable, but a brief flurry from Trinity around the music round looks like it might bring them into contention. But that’s all it was, the briefest of flurries, like that random day in April or October where someone says ‘is it snowing?, and you all look out of the window, but before you can actually work out if it really was snowing or if it was some sort of white rain, its stopped.

Corpus stretch their legs now, and find themselves beyond two hundred points before Trinity turn themselves back on, which they eventually do, building up to a not-disgraceful 80 before the gong.

Final Score: Trinity 80 - 245 Corpus

Episode 30 - Manchester vs Wolfson, Ox

Because I do this on Tumblr, one of the most annoying things about doing this (and I know its dumb), and something that I think might subconsciously play into me not doing these more regularly, is that when I try and add the pictures of the teams to the post it quite often takes ages and sometimes causes the page to freeze so that I can’t save/post it. This problem is exacerbated when there are multiple episodes to get through, which makes it one of those snowballing problems that only gets worse the longer you leave it - like when you put off repying to an email until it becomes almost a monolithic entitiy in your mind.

It only takes a few minutes to fix this - you copy and paste the text and then add the images in a different window (though there is another annoying thing where the hashtags don’t save anyway, so you have to retype the hashtags - and for some reason I always add loads of hashtags, including #JeremyPaxman - which also feels like it takes an epoch) - but its one of those few minute periods that feel like fifteen minutes. So basically, what I’m saying is that I can’t be assed adding the pictures to the post at this point. I might add them later, but for now you’re just getting words, so, so many rambling words.

Manchester are back in the last eight for the first time in donkeys, but they stand on the precipice following a trouncing by Trinity in their QF-opener (I’ve already mentioned this in the last review, which normally wouldn’t matter, but since its directly above this one then it might seem a bit repetitive, but I don’t know if I can rely on your having remembered). Wolfson were likewise (likewise were? Are both okay) baeten by Corpus Christi (which is also referenced above, sorry) so this one was an ELIMINATOR!

Neither side seemed to realise this from the off though (I say though too much don’t I? If I had more time I’d probably edit a few down. But I’m doing a 5-episode mega-post so I don’t, though. Shit. Actually, that one was on purpose winky face) and sort of stumble through the first few questions with some atrocious work on the bonuses.

Green thought he’d pulled a great answer out of the bag to kick start the match, but Fanny Burney Fanny Burnett is not, and Paxo decries the crowd for being amused at how close Green had come (they having let out a collective ‘oooh’, much in the same way their footballing equivalent may have done at a smashed crossbar).

Even Jones, so electric in her previous appearances, was a bit slow off the mark tonight. On one occasion she even overruled her teammates conferred and agreed upon answer at the last moment, giving her own guess which they had dismissed, but fortunately for her they had both been wrong, so she did not look a fool.

Manchester were ahead, but couldn’t get far ahead. Wolfson were within touching distance, but couldn’t touch. Not until the very end that is. Caple took the final starter to draw them level and the gong sounded before th first bonus could be asked. DEADLOCK.

A #DEADLOCKELIMINATOR no less.

Paxman explains that a Neg on this question would hand victory to the other team without them lifting a buzzer-finger. He starts reading, no one buzzes. He continues to read. Everyone continues to not buzz. He carries on r- BUZZ.

Manchester Rogers. Three words left on Paxo’s lips. He better be right. Kaiser Wilhelm. He isn’t. Otto Von Bismarck. An easy mistake to make, says Paxo.

I reckon Wolfson would have picked up the drop anyway, but you can’t be sure.

My fellow UC blog, jacksonlinewritings, says that its the first time a neg has lost a tiebreak since 2002/03.

Final Score: Manchester 125 - 130 Wolfson.

Episode 31 - Durham vs Imperial.

I don’t know if this is the first time I’ve written about the same team twice in one post before, but it may well be. Either way, you can (and probably already have) read everything I had to say about Imperial Brandon, my favourite contestant this series, further up this very page, so I don’t need to reiterate.

Durham’s Tams beats him to what I thought was a relatively easy starter on the Magna Carta (just spent a few minutes trying to come up with another word to rhyme with carta, thought it would be easy, but it was a bit harda). He gets the next one though (though) and his Captain Rich the third to give them the lead. Their opponents proved a tougher nut to crack than Courtauld though (though, and I’m not doing this on purpose. I’m just not removing them when I probably should be. They’re all coming up naturally. This is just how much I apparently use the word. If there are any others then please let me know) and cling on whenever Brandon threatens to zoom away.

Please forgive me for going on about Brandon, by the way. He’s just (I think ‘just’ is probably one, and probably ‘probably’ too) so captivating to watch. There were several times in this episode when I stopped watching the whole screen during a starter and focussed on him, expecting him to buzz in, which he duly did. Especially on the starters which are that bit more important, when Durham were (I need to do something about my tenses too, they’re all over the shop) threatening to make a comeback, you could feel certain that he was going to get it.

When the game has been won, he relaxes, so his personal scores haven’t been as high as those of others in past series, but he hasn’t needed to get more than he has done, so why would he bother? I expect if a team were to push Imperial close over a whole match then he’d easily post double figures.

Imperial join Corpus Christi in the semis. Durham live to fight another day.

Final Score: Durham 115 - 185 Imperial

Episode 32 - Jesus, Ox vs Courtauld

Phew! I’ve never written four in a night before. That was quite something. Wait, whats that, I have another one to go? Okay, lets do this - an advance warning, this one will probably (probably! Why do I feel the need to never be absolute about anything. I know for certain that this will be very short, so why must I try and placate some imaginary reader who might scold me for its being so?) be very short.

So, another ELIMINATOR. Courtauld were my favourite team of the series, but I harboured little hope for them, after such a crushing defeat by Imperial last time out, and Jesus were quick to crush what little I had left. Lucy Clarke, who absolutely relishes a buzz on the opening starter of a match, came in with an early buzz, as is her wont, and fortunately for the Oxonians she was right this time. She got the next one too, and Jesus were 45 up.

Three in a row for Courtauld captain Prance, who looks shocked every time he gets a starter correct, despite the fact that when he got the third of this hat-trick, he had quite clearly proved to himself that he knows how to answer starter questions by the fact that (the fact that Ducks, Newburyport) he had got the previous two. They were ahead now. Dare I dream?

No, I daren’t. Jesus quickly stole it back, and did not let it go. Courtauld stayed fairly close, but could never again broach the gap, struggling on the bonus questions whenever they got in. Perhaps on another night they might have stood a better chance (with a bonus set on collage art, which Paxman reckoned they would have knocked out of the park, going to Jesus), but tonight (its not tonight at all is it, not for me and not for you) was not their night.

And breathe...

Final Score: Jesus, Ox 135 - 90 Courtauld

If you’ve stuck with me through all of this, I’m frankly amazed. Thank you, and if you need something to do during self-isolation, there are like 6 whole series of the Challenge on YouTube. I haven’t reviewed them all, but thats probably for the best though.

#university challenge #bbc2 #manchester #jesus #oxford #wolfson #cambridge #corpus christi #durham #imperial #london #trinity #Courtauld #Jeremy Paxman

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brajeshupadhyay · 4 years ago

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Marlins’ coronavirus outbreak has sports world on edge

Fans may have been caught off guard when, just four days into a new season, a COVID-19 outbreak among the Miami Marlins team forced the postponement of several pro baseball games, but the news did not surprise public health officials.

With cases surging in many parts of the country, experts say Major League Baseball’s predicament shows that anyone can catch the novel coronavirus.

“This is something we knew would happen,” said Anne Rimoin, an epidemiology professor at UCLA’s Fielding School of Public Health. “Baseball has taught us that nobody is immune.”

Eleven players on Miami’s roster tested positive, forcing the postponement of the team’s scheduled home opener Monday and an ensuing game Tuesday. MLB officials also postponed a game in Philadelphia, where the Marlins had played over the weekend, so the Phillies could be tested and their locker rooms disinfected.

Monday’s announcement stirred memories of March, when the NBA abruptly halted its season, a precursor to widespread shutdowns. This time, amid national debate over masks, social distancing and other aspects of the COVID-19 pandemic, experts wonder whether sports might once again serve as a bellwether.

“There are absolutely lessons to be learned from this,” said Dr. Jared Baeten, a vice dean at the University of Washington’s School of Public Health. “If sports makes this real for everyone, that would be great.”

Six months after its first reported COVID-19 case, the United States has seen a significant increase in infections. The seven-day average dipped Monday, according to data from Johns Hopkins University, but still totaled more than 60,000 cases.

The Marlins figured to be at particular risk because they play in Florida, a state hit hard by the coronavirus. Rimoin noted that the team traveled to Pennsylvania, where officials and the public have worked to flatten the curve.

“You’ve got people going from a high-risk area to lower-risk area,” she said. “Hopefully they were not mixing with the community.”

The outbreak called into question baseball’s strategy for its shortened, 66-day season.

The NHL chose to conclude its schedule in “bubble” conditions, with 12 teams sequestered in Toronto and 12 in Edmonton. On Monday, the league reported no positive results among 4,256 tests. Other sports leagues, such as the NBA and Major League Soccer, also are keeping players in quarantine and holding games at a central location.

The NBA even has established an anonymous tip hotline — dubbed “the Snitch Line” — to report players who violate coronavirus protocol inside its bubble near Orlando, Fla.. And Clippers guard Lou Williams must stay in quarantine for 10 days, missing two games, after he was caught visiting a strip club during an excused absence for a funeral.

“What we’re doing and what they’re doing is so different,” Clippers coach Doc Rivers said in reference to baseball. “I like what we’re doing.”

MLB executives have insisted their season is too long and requires too many ballparks for sequestration, although plans to contain games to spring-training areas in Florida and Arizona were considered at one point. “The longer you go, the more people you have, the less likely it is that you can make the bubble work,” baseball Commissioner Rob Manfred said Monday during an interview on MLB Network.

Franchises have been grouped in geographical divisions to reduce travel but are playing in their own stadiums with no fans present. Players are on the honor system, allowed to go home after work.

A view of Citizens Bank Park on Sunday in Philadelphia, where the Miami Marlins played the Phillies. On Monday, the Marlins’ next two games were postponed because of a coronavirus outbreak on the team.

(Chris Szagola / Associated Press)

“I think it’s really important to trace how it occurred,” Angels manager Joe Madden said during a videoconference call before his team’s 3-0 loss to the Athletics in Oakland on Monday. “That’s the one thing we need to know first before we jump to a lot of different conclusions. I mean, to me, if there was a breach of protocol by any of those players, then it’s more easily explainable. And if not, then it becomes more problematic.”

MLB officials said they expected some positive tests, with teams keeping a larger-than-usual 30-man roster and 30 more players who are continuing to train in a separate area and would be ready to replace anyone who becomes infected. On Monday, Dodger President Stan Kasten expressed confidence in the approach.

“I don’t believe there is going to be any panic just yet,” he told MLB Network Radio. “I think we understood that there might be occasions like this.”

But earlier this month, Manfred discussed the possibility of more-significant outbreaks during a radio interview.

“If we have a team or two that’s really decimated with a number of people who had the virus and can’t play for any significant period of time, it could have a real impact on the competition and we’d have to think very, very hard about what we’re doing,” Manfred said on “The Dan Patrick Show.”

Washington Nationals manager Dave Martinez, who has a heart condition, acknowledged feeling scared about the prospect of traveling with his team to face Miami in a three-game series scheduled to start Friday.

“My level of concern went from about an 8 to a 12,” he said. “This thing really hits home now that you see half a team get infected.”

Baseball’s dilemma might have an impact on the NFL and college football, both of which have adopted similar protocols for their upcoming seasons in the fall. NFL camps officially open Tuesday, and, like baseball, the league’s teams are using their own facilities to train.

Bruce Arians, coach of the Tampa Bay Buccaneers, believes the league and its teams are doing all they can to be safe. “I don’t think anybody’s going to get sick at work, because we test every day and everybody is clean,” he said during an interview by phone Monday. “So it’s just, ‘What are you doing away from home, away from the office.’ ”

Said Baeten: “Only the bubble can prevent cases. What was really striking about the Marlins was that they went from zero to 14 cases so fast. That’s not 14 cases coming into the team. That’s transmission within the team and its coaches.”

It would be a mistake to downplay the danger of the coronavirus for athletes who are young and fit enough to be at low risk for severe symptoms. Public health experts cited cases of COVID-19 leading to long-term heart and lung problems even among young patients.

The potential for lasting effects has been particularly worrisome to NBA players. “We’re trying to be extra careful and not have a bad outcome because all it takes is one bad outcome before there’s a lot of regret,” said Dr. Jonathan Kim, a sports cardiologist at Emory University and specialist for the Atlanta Hawks. “Better to be safe and let the science guide.”

Some medical experts are calling for the entire Miami roster to be quarantined for 14 days. Though it remains to be seen how baseball will respond, Kasten said he hopes the outbreak “will teach us things to avoid the repetition of this going forward.”

If nothing else, Baeten wonders whether Monday’s news will send a message to fans across the nation about the importance of wearing masks, washing hands and practicing social distancing.

“We’ll have to see if the Marlins are enough,” he said. “If we’re six weeks out from now and the NFL closes down two teams, maybe that will hit even harder.”

Times staff writers Andrew Greif, Bill Shaikin, Helene Elliott, Dan Woike, Sam Farmer and Maria Torres contributed to this article.

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yonoise · 6 years ago

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Featuring Asemic Writing & Book Art from: Tim Gaze, Rosaire Appel, Luigi Serafini, Carlos M. Luis, Israel F Haros Lopez, Paul A Toth, Alain Satié, Jose Parlá, John M. Bennett, Marco Giovenale, Cecil Touchon, Scott Helmes, Derek Beaulieu, Brion Gysin, Satu Kaikkonen, Cheryl Penn, Raymond Queneau, Logan K. Young, Steve McCaffery, Xu Bing, Geof Huth, Gene Kannenberg Jr., Christopher Skinner, Max Ernst, Timothy Ely, Charles Stein, Gazaliel, Lucinda Sherlock, Volodymyr Bilyk, Catherine M. Bennett, Henri Michaux, Spencer Selby, Jim Leftwich, Louise Tournay, Abdourahamane Diarra, Joe Maneri, Michael Jacobson, Robyn Ellenbogen, Donna Maria De Creeft, Marilyn R Rosenberg, Francesco Aprile, Bill Beamer, Nuno De Matos, Lynn Alexander, Tony Burhouse, Scott Ross, Axel Calatayud, Henry Denander, Jean-christophe Giacottino, Lin Tarczynski, Tom Cassidy, Ricky Brett, Edward Kulemin, Phil Openshaw, Kerri Pullo, Anneke Baeten, Benji Friedman, Laura Ortiz, John McConnochie, Kimm Kiriako, Sam Roxas Chua, Steven J Fowler, Tatiana Roumelioti, Ekaterina Samigulina & Yuli Ilyshchanska, Nico Vassilakis, mIEKAL aND, Eckhard Gerdes & Domonic Ward, the unknown author of The Voynich Manuscript, all the authors & artists in Asemic Magazine, everyone in John Moore William's asemic issue of The Bleed, & including everyone in Paul A. Toth's ALPHA BET A TEST: The Eye Am Eye Asemic Anthology: Language In The Act of Disappearing.

http://thenewpostliterate.blogspot.com/2017/02/asemic-writing-offline-and-in-gallery.html

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jurnaldeoltenia · 2 years ago

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Marius Croitoru, Gabriel Enache si Kyriakos Papadopoulos au prefatat meciul cu Petrolul Ploiesti.

Azi a avut loc o conferinta de presa sustinuta de Marius Croitoru, Gabriel Enache si Kyriakos Papadopoulos. FCU Craiova intalneste maine la Targu Jiu echipa Petrolul Ploiesti. William Baeten și Benjamin Van Durmen revin in lotul Stiintei pentru meciul cu Petrolul Ploiesti in schimb Paramatti nu este recuperat complet , Radu Negru este suspendat iar Bauza se recupereaza dupa accidentarea din…

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#Bauza #Benjamin Van Durmen #Craiova #fcu craiova #Fotbal #fotbal craiova #Gabriel Enache #KYRIAKOS PAPADOPOULOS #Liga 1 #Marius Croitoru #Paramatti #Petrolu Ploiesti #Radu Negru #Stiinta #superliga #targu-jiu #William Baeten

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maxisama · 8 years ago

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30.4.2.3 ESTRELLAS DE WOLF-RAYET: TIPOS DE GALAXIAS STARBUST WOLF-RAYET.

2 .Galaxias compactas azules (BCGs):

b) Galaxias del Guisante Verde (2da. Parte): Historia del Descubrimiento de las Galaxias del Guisante Verde.

Años 2007 a 2010

Galaxy Zoo (GZ) es un proyecto en línea desde julio de 2007 que busca clasificar hasta un millón de galaxias. En julio de 2007, pocos días después del inicio de GZ, se inició una discusión en el foro de Internet de GZ, Hanny Van Arkel, llamado "Dar a los guisantes una oportunidad", en la que se publicaron varios objetos verdes. Este tema comenzó con humor, ya que el nombre es un juego de palabras del título de la canción de John Lennon " Give Peace a Chance”, pero para diciembre de 2007, se había puesto de manifiesto que algunos de estos objetos inusuales eran un grupo distinto de galaxias. Estas "galaxias de guisantes" aparecen en el SDSS como imágenes verdes no resueltas. Esto se debe a que los guisantes tienen una línea espectral muy brillante o poderosa en sus espectros de oxígeno altamente ionizado, que en los compuestos de color SDSS aumenta la luminosidad o brillo de la banda de color "r" con respecto a los otros dos colores Bandas "g" e "i". La banda de color "r" aparece como verde en las imágenes SDSS.] Los entusiastas, llamándose a sí mismos "el Cuerpo de los Guisantes" (otro juego humorístico en el Cuerpo de Paz ), recogieron más de un centenar de estos guisantes, que finalmente fueron colocados juntos en un hilo de discusión dedicado iniciado por Carolin Cardamone en julio de 2008 La colección, una vez refinada, proporcionó valores que podrían utilizarse en una búsqueda sistemática por ordenador de la base de datos GZ de un millón de objetos, lo que dio como resultado una muestra de 251 galaxias de guisantes, también conocidos como guisantes verdes.

En noviembre de 2009, los autores C. Cardamone, Kevin Schawinski, M. Sarzi, S. Bamford, N. Bennert, C. Urry, Chris Lintott, W. Keel y otros 9 publicaron un artículo en los Avisos Mensuales de la Real Sociedad Astronómica titulado "Galaxy Zoo Green Peas: Descubrimiento de una clase de galaxias compactas que forman estrellas". En este artículo, se reconoce que 10 voluntarios del Zoo Galaxy han hecho una contribución particularmente significativa. Ellos son: Elisabeth Baeten, Gemma Coughlin, Dan Goldstein, Brian Legg, Mark McCallum, Christian Manteuffel, Richard Nowell, Richard Proctor, Alice Sheppard y Hanny Van Arkel. Se les agradece por "dar a los guisantes una oportunidad". Las citas para 2009MNRAS.399.1191C están disponibles en el SAO / NASA Astrophysics Data System.

Sería erróneo suponer que los 80 GPs eran nuevos descubrimientos. De los 80 originales, 46 GPs tienen citas anteriores fechadas antes de noviembre de 2009 en la base de datos extragaláctica NASA / IPAC. Los 80 GPs originales formaban parte de una muestra de la liberación de datos SDSS 7 (DR7), pero no incluían galaxias de otras fuentes. Algunas de estas otras fuentes incluían objetos que bien podrían haber sido clasificados como GP si estuvieran en la muestra SDSS. Un ejemplo de un trabajo que demuestra esto es: En abril de 2009, los autores JJ Salzer, AL Williams y C. Gronwall publicaron un artículo en el Astrophysical Journal Letters titulado "Una Población de Metal-Poor Galaxias con L Luminosidades en Redshifts Intermedio". En este trabajo, se presentaron "nuevas estimaciones de espectroscopia y metalicidad para una muestra de 15 galaxias formadoras de estrellas con desplazamientos hacia el rojo en el rango de 0.29 - 0.42". Estos objetos fueron seleccionados utilizando la KPNO International Spectroscopic Survey (KISS). Ciertamente 3 de estos 15 cuando se ven como objetos en SDSS son verdes (KISSR 1516, KISSR 2042 y KISSRx 467). De hecho, citando de Salzer et al. Dada la gran cantidad de estudios de abundancias de metales en galaxias con desplazamiento al rojo intermedio y alto mencionados en la Introducción, puede parecer extraño que no se hayan reconocido sistemas similares a los descritos aquí previamente."

En junio de 2010, los autores R. Amorin, E. Perez-Montero y J. Vilchez publicaron un artículo en The Astrophysical Journal Letters titulado "Sobre las abundancias químicas de oxígeno y nitrógeno y la evolución de las galaxias" guisantes verdes” . En él se exploran cuestiones relativas a la metalicidad de 79 GPs, disputando los hallazgos originales en Cardamone et al. Concluyen, "argumentando que la reciente entrada de gas inducida por la interacción, posiblemente junto con una pérdida de gas rica en metales selectiva por los vientos de supernova, puede explicar nuestros hallazgos y las propiedades de la galaxia conocidas"

AÑO 2011

En febrero de 2011, los autores Y. Izotov, N. Guseva y T. Thuan publicaron un artículo en el Astrophysical Journal titulado "Galaxias y cohortes de guisantes verdes: Luminous Compact Emission-line Galaxies en Sloan Digital Sky Survey". Ellos encuentran que los 80 GPs no son una clase rara de galaxias por sí mismos, sino más bien un subconjunto de una clase conocida como "Luminous Compact Galaxies" (LCGs), de los cuales hay 803.

En noviembre de 2011, los autores Y. Izotov, N. Guseva, K. Fricke y C. Henkel publicaron un artículo en Astronomía y Astrofísica titulado " Galaxias de formación de estrellas con emisión de polvo caliente en el SDSS descubierto por el Explorador de Infrarrojos de Campo Amplio SABIO)'. En este artículo, encuentran cuatro galaxias que tienen colores muy rojos en el rango de longitud de onda 3,4 micrómetros (W1) y 4,6 micrómetros (W2). Esto implica que el polvo en estas galaxias está a temperaturas de hasta 1000 Kº. Estas cuatro galaxias son GPs y más del doble del número de galaxias conocidas con estas características.

AÑO 2012

En enero de 2012, los autores R. Amorin, R. Perez-Montero y J.Vilchez publicaron un "Procedimiento de la Conferencia" titulado "Descubriendo la Naturaleza de las Galaxias del Guisante Verde". En esta publicación, anuncian que han realizado un conjunto de observaciones utilizando el Sistema Óptico de Imágenes y Espectroscopía Integrada de Baja Resolución (OSIRIS) en el Gran Telescopio Canarias, y que hay un próximo trabajo sobre su investigación. Estas observaciones "aportarán nuevas perspectivas sobre el estado evolutivo de los guisantes verdes, en particular, seremos capaces de ver si los guisantes verdes muestran una prolongada y antigua población estelar subyacente a los jóvenes arrancadores de estrellas, como los típicamente dominantes en términos de masa estelar En la mayoría de las galaxias compactas azules ".

En enero de 2012, los autores L. Pilyugin, J. Vilchez, L. Mattsson y T. Thuan publicaron un artículo en el MNRAS titulado: "Determinación de la abundancia de los espectros SDSS de la línea de emisión global: explorando objetos con altas relaciones N / O". En ellos se comparan las abundancias de oxígeno y nitrógeno derivadas de los espectros SDSS de líneas de emisión globales de galaxias usando (1) el método de temperatura electrónica y (2) dos calibraciones de líneas fuertes recientes: las calibraciones O / N y N / S. Se compararon tres conjuntos de objetos: nebulosas compuestas ricas en hidrógeno, 281 galaxias SDSS y una muestra de GPs con líneas aurorales detectables [OIII] -4363. Entre las preguntas que rodean a los GPs se encuentra la cantidad de nebulosas que influyen en sus espectros y resultados. A través de las comparaciones de los tres objetos utilizando la metodología probada y el análisis de la metalicidad, concluyen que "las altas proporciones de nitrógeno a oxígeno derivadas en algunas galaxias de guisantes verdes pueden ser causadas por el hecho de que sus espectros SDSS son espectros de nebulosas compuestas compuestas de Varios componentes con diferentes propiedades físicas (como la metalicidad), pero para las galaxias de guisantes verdes más calientes, que parecen ser galaxias enanas, esta explicación no parece plausible ".

En enero de 2012, el autor S. Hawley publicó un artículo en las Publicaciones de la Sociedad Astronómica del Pacífico titulado "Abundancias en" Green Pea "Star-forming Galaxies". En este artículo, el ex astronauta de la NASA, Steven Hawley, compara los resultados de los anteriores artículos del GP con respecto a sus metalicidades. Hawley compara diferentes maneras de calibrar e interpretar los diversos resultados, principalmente de Cardamone et al. Y Amorin et al. Pero algunos de Izotov et al., Y sugiere por qué las diferentes discrepancias entre los resultados de estos documentos podrían ser. También considera detalles tales como la contribución de las estrellas de Wolf-Rayet a la ionización de gas y qué conjuntos de líneas de emisión dan los resultados más precisos para estas galaxias. Termina escribiendo: "Las calibraciones derivadas de los guisantes verdes difieren de las utilizadas comúnmente y serían útiles si las galaxias formadoras de estrellas como los guisantes verdes con fuentes ionizantes extremadamente calientes son más comunes".

En febrero de 2012, los autores S. Chakraborti, N. Yadav, C. Cardamone y A. Ray publicaron un artículo en The Astrophysical Journal Letters titulado 'Radio Detection of Green Peas: Implications for Magnetic Fields in Young Galaxies'. En este artículo, los estudios de magnetismo usando nuevos datos del Telescopio de Metrierave Gigante describen varias observaciones basadas en los GPs. Demuestran que las tres galaxias starburst "muy jóvenes" que se estudiaron tienen campos magnéticos más grandes que la Vía Láctea. Esto está en desacuerdo con la comprensión actual de que las galaxias acumulan sus propiedades magnéticas en el tiempo.

En abril de 2012, los autores R. Amorin, E. Perez-Montero, J. Vilchez y P. Papaderos publicaron un artículo en el Astrophysical Journal titulado "Historia de la formación estelar y contenido de metales de los guisantes". Espectrofotometría de Tres Galaxias ". Ellos dan los resultados para la imagen de banda ancha profunda y la espectroscopia de hendidura larga para 3 GPs que se han observado con el instrumento OSIRIS, montado en el Gran Telescopio Canarias de 10,4 m en el Observatorio Roque de los Muchachos.

En agosto de 2012, los autores R. Amorín, J. Vílchez, G. Hägele, V. Firpo, E. Pérez-Montero y P. Papaderos publicaron un artículo en el Astrophysical Journal Letters titulado "Compleja cinemática de gas en compacto, Formando galaxias ". Usando el espectrógrafo de ISIS en el telescopio de William Herschel, publican los resultados del espectro de alta calidad que tomaron de seis galaxias, cinco de los cuales son GPs. Después de estudiar las líneas de emisión de hidrógeno alfa (ELs) en los espectros de los seis, se muestra que estos ELs están formados por múltiples líneas, lo que significa que los GPs tienen varios trozos de gas y estrellas que se mueven a grandes velocidades entre sí.Estos ELs también muestran que los GPs son efectivamente un "lío turbulento", con partes (o grumos) que se mueven a velocidades de más de 500 km / s (quinientos km / s) entre sí.

AÑO 2013

En enero de 2013, los autores S. Parnovsky, I. Izotova y Y. Izotov publicaron un artículo en Astrofísica y Ciencias Espaciales titulado "H alfa y UV luminosidades y tasas de formación de estrellas en una gran muestra de galaxias compactas luminosas". En ellos, se presenta un estudio estadístico de las tasas de formación estelar (SFR) derivadas de las observaciones GALEX en el continuo Ultravioleta y en la línea de emisión H alpha para una muestra de ~ 800 galaxias compactas luminosas (LCGs). Dentro del conjunto más grande de LCGs, incluyendo los GPs, se encuentran SFR de hasta ~ 110 M ☉ / año (~ 110 masas solares al año), así como estimaciones de las edades de los starbursts.

En abril de 2013, los autores A. Jaskot y M. Oey publicaron un artículo en el Astrophysical Journal titulado "El Origen y la Profundidad Óptica de la Radiación Ionizante en el" Guisante Verde "Galaxias". Se estudian seis GP "extremos". Usando éstos, los autores procuran reducir la lista de posibilidades sobre qué está produciendo la radiación y las cantidades substanciales del fotón de la alta energía que podrían escaparse de los GPs. Siguiendo con este artículo, las observaciones sobre el Telescopio Espacial Hubble, que totalizan 24 órbitas, fueron tomadas en diciembre de 2013. El Espectrógrafo de Orígenes Cósmicos y la Cámara Avanzada de Encuestas se utilizaron en cuatro GPs "extremos".

AÑO 2014

En enero de 2014, los autores Y. Izotov, N. Guseva, K. Fricke y C. Henkel publicaron un artículo en Astronomía y Astrofísica titulado "Estudio de múltiples longitudes de onda de 14000 galaxias formadoras de estrellas de la Sloan Digital Sky Survey". En él, usan una variedad de fuentes para demostrar: "que la emisión que emerge de las jóvenes regiones formadoras de estrellas es la fuente dominante de calentamiento del polvo para temperaturas de varios centenares de grados en la muestra de galaxias formadoras de estrellas". La primera fuente de datos es SDSS a partir de la cual se seleccionan 14.610 espectros con líneas de emisión fuertes. Estos 14.610 espectros se identificaron entonces de forma cruzada con fuentes procedentes de levantamientos fotométricos en otros rangos de longitud de onda. Éstos son: 1) GALEX para el ultravioleta; 2) la encuesta 2MASS para el infrarrojo cercano; 3) el Catálogo Wide-field Infrared Survey Explorer All-Sky para infrarrojos en diferentes longitudes de onda; 4) la encuesta IRAS para el infrarrojo lejano y la 5) Encuesta NVSS a longitudes de onda radioeléctricas. Sólo una pequeña fracción de los objetos SDSS se detectaron en las dos últimas encuestas. Entre los resultados está una lista de veinte galaxias con las magnitudes más altas que tienen polvo caliente de varios cientos de grados. De estos veinte, todos podrían ser clasificados como GPs y / o LCGs. También entre los resultados, la luminosidad se obtiene en las galaxias de muestra en un amplio rango de longitudes de onda. En las luminosidades más altas, las galaxias de muestra tenían luminosidades que se acercaban a las de la galaxia de alto-desplazamiento al rojo Lyman-break.

En enero de 2014, los autores A. Jaskot, M. Oey, J. Salzer, A. Van Sistine y M. Haynes hicieron una presentación titulada "Gas neutro y desbordamientos de bajo desplazamiento al rojo: de infall a ionización" a la Sociedad Astronómica Americana en su Reunión # 223. En la presentación se incluyeron datos de la Encuesta Rápida de ALFA del Observatorio de Arecibo (ALFALFA). Los autores analizaron los espectros ópticos de los GPs y concluyeron: "Mientras que la encuesta de ALFALFA demuestra el papel de los procesos externos en el desencadenamiento de arranques estelares, los guisantes muestran que la radiación de los starbursts puede escapar para afectar su ambiente externo", encontrando que los guisantes son probables Ópticamente delgada a Lyman continuum (LyC) radiación. "

En junio de 2014, los autores A. Jaskot y M. Oey publicaron un informe de la conferencia titulado "El origen y la profundidad óptica de los fotones ionizantes en las galaxias de guisantes verdes". Esto aparece en "Grandes Clusters de Estrellas Jóvenes Cerca y Lejos: De la Vía Láctea a la Reionización", basado en la Conferencia de Guillermo Haro 2013.

AÑO 2015

En mayo de 2015, los autores A. Henry, C. Scarlata, CL Martin y D. Erb publicaron un artículo en la revista Astrophysical Journal titulada "Lyα Emission from Green Peas: El Papel de la Densidad, Cubrimiento y Cinemática de los gases Circumgalácticos". En este artículo, diez guisantes verdes fueron estudiados en el ultravioleta, usando la espectroscopia de alta resolución con el telescopio espacial de Hubble usando el espectrógrafo de los orígenes cósmicos. Este estudio demostró, por primera vez, que los guisantes verdes tienen una emisión de Lya fuerte como las galaxias distantes, de alto desplazamiento al rojo observadas en un universo más joven. Henry et al. Exploró los mecanismos físicos que determinan cómo Lyα escapa de los Guisantes, y concluyó que las variaciones en la densidad de la columna de hidrógeno neutral eran el factor más importante.

AÑO 2016

En mayo de 2016, la autora Miranda CP Straub publicó un trabajo de investigación en la revista de acceso abierto Ciencia Ciudadana: Teoría y Práctica denominada "Dar a los Científicos Ciudadanos una Oportunidad: Un Estudio de Descubrimiento Científico dirigido por Voluntarios". El resumen afirma: "El descubrimiento de una clase de galaxias llamadas Green Peas proporciona un ejemplo de trabajo científico realizado por voluntarios.Esta situación única surgió de un sitio web de crowdsourcing de la ciencia llamado Galaxy Zoo. Dio la capacidad de investigar la investigación Proceso utilizado por los voluntarios El proceso de los voluntarios fue analizado en términos de tres modelos de investigación científica y un modelo de trabajo iterativo para mostrar el camino a este descubrimiento.Como se ha ilustrado en estos modelos de la ciencia, el camino fue iterativo, no predeterminado , Y conducido por datos empíricos.Este artículo da una narración de los 11 meses, el voluntario conducido por el proceso de descubrimiento de las galaxias Green Pea y la transición a la participación del Galaxy Zoo equipo científico para analizar e informar sobre una nueva clase de galaxia. Estudio identificó los ciclos de trabajo de los voluntarios y los situó en el modelo integrado propuesto del proceso de investigación científica para mostrar que los voluntarios participaban en investigaciones científicas significativas investigación."

En abril de 2016, Yang et al. Publicado "Las Galaxias de Guisante Verde Revelan Secretos de Lya Escape". Los espectros de Lyman-alpha de 12 GPs que utilizaron el HST_COS (Henry GO: 12928, Jaskot GO: 13293 y Heckman GO: 11727) fueron analizados y modelados con modelos de transferencia radiativa. Se exploró la dependencia de las fracciones de escape Lyman-alfa (LyA) en varias propiedades. Todos los 12 GPs muestran líneas de LyA en emisión, con una distribución de ancho similar a LyA similar a los emisores de alto-redshift. Entre los hallazgos se encuentra que la fracción de escape LyA depende fuertemente de la metalicidad y moderadamente de la extinción del polvo. Los resultados de los trabajos sugieren que la baja densidad de la columna H1 y la baja metalicidad son esenciales para el escape de LyA. "En conclusión, los médicos generales ofrecen una oportunidad inigualable para estudiar LyA escape en LyA Emitters".

AÑO 2017

Finalmente en enero de 2017, Yang et al. Presentó un estudio en el Astrophysical Journal titulado: "Perfil de Lyα, polvo y predicción de la fracción de escape Lyα en galaxias de guisantes verdes". Los autores afirman que los GPs son análogos cercanos de las galaxias emisoras de Lyman-alfa (LyA) de alto desplazamiento al rojo. Utilizando datos espectrales del archivo MAST de HST-COS, 24 GPs fueron estudiados para su escape de LyA y los perfiles espaciales de las emisiones de LyA y UV continuum. Los resultados incluyen: 1) Habiendo comparado los tamaños de LyA y UV de los espectros 2D y perfiles espaciales 1D, se observa que la mayoría de los GPs muestran una emisión de LyA más extendida que el continuo UV. 2) 8 GPs tuvieron sus perfiles espaciales de fotones LyA en blueshifted y velocidades redshifted en comparación. 3) La fracción de escape LyA se comparó con la proporción de tamaño de LyA a UV. Se encontró que los GP que tienen fracciones de escape de LyA mayores del 10% "tienden a tener una morfología de LyA más compacta".

En marzo de 2017, Yang et al. Publicó un artículo en el Astrophysical Journal titulado "Lyα y UV Sizes of Green Pea Galaxies". Los autores estudiaron el escape de Lyman-alfa (LyA) en una muestra estadística de 43 GP con espectros HST / COS LyA. Los 43 GPs y sus datos fueron tomados de programas de 6 HST (GO: 14201, GO: 12928, GO: 11727, GO: 13017, GO: 13293 y GO: 13744). Sus conclusiones incluyen: 1) El uso de GPs que cubren toda la gama de extinción de polvo y la metalicidad, que encuentran alrededor de dos tercios son fuertes LyA emisores. Esto confirma que los GPs generalmente son "los mejores análogos de los emisores Lyman-alpha (LAEs) de alto z (redshift) en el universo cercano". Las fracciones de escape de LyA muestran anti-correlaciones con algunas características cinemáticas de LyA 3) Los autores encuentran muchas correlaciones con respecto a la dependencia del escape de LyA en las propiedades galácticas, tales como la extinción del polvo y la metalicidad. ) El modelo de transferencia radiativa de una sola envoltura puede reproducir la mayoría de los perfiles de LyA de GPs. LyA fracción de escape, la extinción de polvo y el LyA rojo pico de velocidad.

En enero de 2017, Lofthouse et al. Presentó un estudio a los Avisos Mensuales de la Real Sociedad Astronómica denominados: "Análogos locales de las galaxias que forman estrellas de alto desplazamiento al rojo: espectroscopía de campo integral de guisantes". Los autores utilizaron la espectroscopía de campo integral, de los instrumentos SWIFT y Palm 3K, para realizar un análisis espectroscópico espacialmente resuelto de cuatro GPs, numerados 1,2,4 y 5. Entre los resultados se encuentran los GPs 1 & 2 están soportados rotativamente (tienen un centro giratorio), mientras que los GPs 4 y 5 son sistemas dominados por dispersión. Los GP 1 y 2 muestran morfologías indicativas de las fusiones en curso. Sin embargo, los GPs 4 y 5 no muestran signos de interacciones recientes y tienen tasas de formación de estrellas similares. Esto indica que las fusiones no son "un requisito necesario para conducir la alta formación estelar en este tipo de galaxias".

En una presentación a la American Astronomical Society Meeting # 229 en enero de 2017, Matt Brorby y Philip Kaaret describen las observaciones de dos GPs y su emisión de rayos X. Usando ambos programas de telescopio espacial Chandra GO: 16400764 y Hubble GO: 13940, examinan las Galaxias Compactas Luminosas, ambos GPs, J0842 + 1150 y SHOC 486. Concluyen: 1) Estas son las primeras observaciones de rayos X de GPs. 2) Los dos GPs estudiados son la primera prueba de la relación planar Lx-SFR-Z y que son consistentes con esto. 3) Las galaxias de baja metalicidad exhiben una emisión de rayos X mejorada con respecto a las galaxias de formación de estrellas de metalicidad normales. 4) GPs son útiles para las predicciones de la salida de rayos X en el universo temprano.

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