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Large, Bright Galaxy at z ~ 11
http://arxiv.org/abs/1603.00461
Oesch et al Some Commentary: However, the discovery also raises many new questions as the existence of such a bright and large galaxy is not predicted by theory. "It's amazing that a galaxy so massive existed only 200 million to 300 million years after the very first stars started to form. It takes really fast growth, producing stars at a huge rate, to have formed a galaxy that is a billion solar masses so soon," explains Garth Illingworth of the University of California, Santa Cruz. (From Science Daily 3/3/16) RLO http://ww3.amherst.edu/~rloldershaw |
#2
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Large, Bright Galaxy at z ~ 11
In article , "Robert L.
Oldershaw" writes: Some Commentary: However, the discovery also raises many new questions as the existence of such a bright and large galaxy is not predicted by theory. "It's amazing that a galaxy so massive existed only 200 million to 300 million years after the very first stars started to form. It takes really fast growth, producing stars at a huge rate, to have formed a galaxy that is a billion solar masses so soon," explains Garth Illingworth of the University of California, Santa Cruz. (From Science Daily 3/3/16) Since s.a.r contributor is a co-author, I'm sure he will comment. :-) Maybe he can counter the argument that the big bang didn't happen, or that this proves the fractal structure of the universe. |
#3
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Large, Bright Galaxy at z ~ 11
On Saturday, March 5, 2016 at 4:29:59 AM UTC-5, Phillip Helbig (undress to reply) wrote:
Since s.a.r contributor is a co-author, I'm sure he will comment. :-) Maybe he can counter the argument that the big bang didn't happen, or that this proves the fractal structure of the universe. Are you claiming that I argue "that the big bang didn't happen, or that this proves the fractal..."? If so I regret to inform you that your claim is completely false. If you had made a slightest bit of effort to learn what it is I do specifically propose, and we have been arguing about for over a decade, it would be impossible to make such a false accusation. Could you please candidly explain yourself on this comment? [Mod. note: further comments in this thread should be of general interest or taken to private e-mail -- mjh] RLO http://www3.amherst.edu/~rloldershaw |
#4
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Large, Bright Galaxy at z ~ 11
http://arxiv.org/abs/1603.00461
In article , "Robert L. Oldershaw" writes: the existence of such a bright and large galaxy is not predicted by theory. Neither is its absence predicted by theory. There is no theory that predicts high-z galaxy luminosity functions. Or low-z galaxy luminosity functions, for that matter. People who are interested should read the preprint (or eventually the paper, which is accepted but not published quite yet) to understand the uncertainties in the derived parameters. The redshift seems secure to me, but the stellar mass and star formation rate depend on assumptions. As an example, the longest wavelength observation at 4.5 microns corresponds to a rest-frame (i.e., emitted) wavelength of 375 nm, which is not an ideal indicator of stellar mass. What we really need is a proper survey to _measure_ the luminosity function at z = 11. That could be done with a properly instrumented 1.5-m telescope at L2. Last year Japan (JAXA) rejected a proposal for such a mission. A similar mission may be proposed to ESA later this year, but even if accepted, it probably wouldn't fly until 2027-2029. There seems to be no suitable funding opportunity at NASA: the mission is too expensive to fit in the Explorer category but too specialized to qualify as a Flagship mission. Some of us would like to see a new funding line for "Probe-class missions," but it will probably take a Decadal Survey recommendation to establish one. -- Help keep our newsgroup healthy; please don't feed the trolls. Steve Willner Phone 617-495-7123 Cambridge, MA 02138 USA |
#5
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Large, Bright Galaxy at z ~ 11
On Tuesday, March 8, 2016 at 3:16:42 AM UTC-5, Steve Willner wrote:
http://arxiv.org/abs/1603.00461 Neither is its absence predicted by theory. There is no theory that predicts high-z galaxy luminosity functions. Or low-z galaxy luminosity functions, for that matter. People who are interested should read the preprint (or eventually the paper, which is accepted but not published quite yet) to understand the uncertainties in the derived parameters. The redshift seems secure to me, but the stellar mass and star formation rate depend on assumptions. As an example, the longest wavelength observation at 4.5 microns corresponds to a rest-frame (i.e., emitted) wavelength of 375 nm, which is not an ideal indicator of stellar mass. What we really need is a proper survey to _measure_ the luminosity function at z = 11. That could be done with a properly instrumented 1.5-m telescope at L2. Last year Japan (JAXA) rejected a proposal for such a mission. A similar mission may be proposed to ESA later this year, but even if accepted, it probably wouldn't fly until 2027-2029. There seems to be no suitable funding opportunity at NASA: the mission is too expensive to fit in the Explorer category but too specialized to qualify as a Flagship mission. Some of us would like to see a new funding line for "Probe-class missions," but it will probably take a Decadal Survey recommendation to establish one. Also what we need are fully general relativistic modeling to supersede crude toy models that use the Newtonian approximations. For hints that this work is in progress, see: https://www.sciencedaily.com/release...0307112935.htm RLO http://www3.amherst.edu/~rloldershaw Keep science and our newsgroups healthy - question authority and hand-waving |
#6
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Large, Bright Galaxy at z ~ 11
Robert L. Oldershaw wrote:
Also what we need are fully general relativistic modeling to supersede crude toy models that use the Newtonian approximations. For hints that this work is in progress, see: https://www.sciencedaily.com/release...0307112935.htm See also Sabino Matarrese "Computational cosmology: A general relativistic approach" Nature Physics (2016) http://dx.doi.org/10.1038/nphys3706 It's unclear to me whether this commentary is open-access or behind the usual Nature paywall. -- -- "Jonathan Thornburg [remove -animal to reply]" Dept of Astronomy & IUCSS, Indiana University, Bloomington, Indiana, USA "There was of course no way of knowing whether you were being watched at any given moment. How often, or on what system, the Thought Police plugged in on any individual wire was guesswork. It was even conceivable that they watched everybody all the time." -- George Orwell, "1984" |
#7
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Large, Bright Galaxy at z ~ 11
In article , "Robert L.
Oldershaw" writes: Also what we need are fully general relativistic modeling to supersede crude toy models that use the Newtonian approximations. Yes, GR is more correct than Newtonian theory. However, one has to make many approximations. In many cases, Newtonian theory is good enough, since relativistic effects or small and/or cancel out. Note that "toy model" does not apply here. The term "toy model" has a specific meaning: a model which is as simple as possible in order to illustrate a certain point, with no claim to being realistic in general, even approximately. It is not a term for any approximate model, nor for any which you don't like. |
#8
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Large, Bright Galaxy at z ~ 11
On Wednesday, March 9, 2016 at 3:18:06 AM UTC-5, Phillip Helbig (undress to reply) wrote:
In article , "Robert L. Oldershaw" Also what we need are fully general relativistic modeling to supersede crude toy models that use the Newtonian approximations. Yes, GR is more correct than Newtonian theory. However, one has to make many approximations. In many cases, Newtonian theory is good enough, since relativistic effects or small and/or cancel out. Note that "toy model" does not apply here. The term "toy model" has a specific meaning: a model which is as simple as possible in order to illustrate a certain point, with no claim to being realistic in general, even approximately. It is not a term for any approximate model, nor for any which you don't like. ---------------------------- Well, both the quark model and the the Big Bang model started out as toy models and then they were developed and refined until they are now considered well-established mature theories/models. Having been taught as near fact to generations of students, they are regarded "the way nature works". We could waste considerable time and effort arguing about whether we have sufficient evidence to say that no further fundamental modification to these models is required, so let's skip that and agree to disagree on that issue. But a question I will ask is how, exactly do we get from toy model to mature model. Was and is Newtonian gravitation a toy model of gravitation? To paraphrase Shakespere again: Is it possible that "a toy by any other name is still a toy", until it gets superseded by a better toy model? RLO http://www3.amherst.edu/~rloldershaw |
#9
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Large, Bright Galaxy at z ~ 11
In article , "Robert L.
Oldershaw" writes: Also what we need are fully general relativistic modeling to supersede crude toy models that use the Newtonian approximations. Note that "toy model" does not apply here. The term "toy model" has a specific meaning: a model which is as simple as possible in order to illustrate a certain point, with no claim to being realistic in general, even approximately. It is not a term for any approximate model, nor for any which you don't like. ---------------------------- Well, both the quark model and the the Big Bang model started out as toy models and then they were developed and refined until they are now considered well-established mature theories/models. True. However, LCDM is not a "toy model", as you claimed. Was and is Newtonian gravitation a toy model of gravitation? No. It is an approximation. |
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