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200,000 Quasars Confirm Einstein's Prediction
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That does appear to be one aspect of the intrinsic redshift arguement that was quantified sufficiently in this study to be applicable. Edit: typo correction
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Would one of you gents be good enough to explain the idea of "intrinsic" red shift and why this quasar study may put it to rest. I understand the concept of redshift and blueshift of light (basicaly dopler effect translated to light) but the intrinsic part is lost to me.
Also if someone could briefly explain how quasars are expected to magnify light that would be great. Is it a gravitational lensing sort of deal? Thanks in advance. K |
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[hand on forehead, shielding eyes]
Hmm. I don't see any John Kiernan around. Odd. John Kiernan? John? Hmmf. [shrug] ;-) CJSF
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Two years ago moved from my town I was looking up past the city lights But the city lights got in my way See the constellation ride across the sky No cigar, no lady on his arm Just a guy made of dots and lines -from "See The Constellation" by They Might Be Giants |
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I'll try to keep the explanation short. In mainstream cosmology it is assumed that almost the entire observed redshift of a quasar or galaxy is cosmological - resulting from expansion of the universe. However, shortly after quasars were discovered the Astronomer Halton Arp noticed that many of the quasars appeared to be placed in the sky near active and disturbed low redshift galaxies. Since some of the quasars were aligned in pairs across the galaxies Arp put forward the interpretation that the quasars were ejected from the nuclei of the active galaxies. Since quasars have very large redshifts in mainstream theory they are interpreted to be very distant. If Arp is right, they are not very distant – they are local. However that would mean that most of their redshift is not from expansion but must have some other cause. This other cause is generically referred to as “intrinsic redshift” by those of us that support this interpretation because the redshift would most likely be due to some intrinsic property of the quasars. If intrinsic redshifts are real, the cause is unknown. Asking what intrinsic redshifts are is similar to asking what dark energy or dark matter is in that there is some theory and speculation, but a specific answer has not been scientifically proven. At any rate, there have been numerous papers published by Arp and others presenting evidence supporting the interpretation that some high redshift objects can be associated with much lower redshift objects. The mainstream response is that these associations are not real, but simply accidental alignments of background objects with nearby lower redshift galaxies. Here are two recent papers that discuss several of the strongest candidates for real associations between high and low redshift objects. You can download the papers by clicking on “PDF” and look at the images in the papers to get the quick picture of the evidence: NGC 7603 and NEQ3 Quote:
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It is also important to note that the study does not present evidence that this or that specific quasar is lensed. Rather they can conclude that if the quasars are background objects, their distribution is consistent with the concordance model parameters. There are two tests that could definitively falsify Arp's hypothesis that quasars are local. Time dilation - which it has been found quasars do not exhibit - a result consistent with them being local. If time dilation was identified in QSO's that would place them at cosmological distances and therefore falsify Arp's proposal. Proper motions provide another test. If quasars are local ejected objects, then proper motions will be detected in reasonable time frames. If Arp is wrong than such studies will not find proper motions. |
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* Ryan Scranton, Brice M´enard, Gordon T. Richards, Robert C. Nichol, Adam D. Myers, Bhuvnesh Jain, Alex Gray, Matthias Bartelmann, Robert J. Brunner, Andrew J. Connolly, James E. Gunn3, Ravi K. Sheth, Neta A. Bahcall, John Brinkman, Jon Loveday, Donald P. Schneider, Aniruddha Thakar, Donald G. York
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Which is also why their results do not make the local quasar hypothesis unnecessary. Their paper has absolutely no implications for the local quasar hypothesis one way or the other. What their paper indicates is that if the quasars are background to the galaxies, then their distribution is consistent with GR. I've specified above which tests can verify/refute the local quasars hypothesis. |
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Everyone is entitled to his own opinion, but not his own facts. |
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Your use of the word dissembling is an accusation that I am being misleading. Once again you're walking that line between discussion and ad-hominem. Quote:
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This is something you're constantly doing. It happened in this thread and now you're doing it again here. Here let me help you for future reference: I'm not saying: Big Bang is wrong. Universe is not expanding. I am saying: Evidence exists that there may be a component of intrinsic redshifts in normal galaxies superimposed upon the cosmological component (which could be from expansion). See my papers. Evidence exists that QSO's and some other very high redshift objects may be local rather than at cosmological distances. I've specifically defined (on this thread again) tests that could falsify this possibility for local QSO's: (1) Time dilation; (2) QSO proper motions. Quote:
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Scranton's paper does not assume quasars are at cosmological distances, but the paper's findings do provide significant support for that view. The key foundation of your argument is incorrect. That Scranton's paper supports the view that quasars are at cosmological distances is not circular reasoning. Scranton's findings explain Arp's anecdotal quasar-galaxy associations better than Arp's attempts at explanation. This paper does indeed damage the local-quasar, intrinsic-redshift hypotheses.
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Dgruss, to explain why I felt this study might provide ammunition to refute intrinsic redshift. One of the arguements I've heard repeatedly with Arp was that there always seemed to be a line of sight correlation with a known, low red shift galaxy and a known quasar or two. I acknowledge full well that the necessary direct observations needed to determine specific redshifts were not taken, but I was reaching for the idea that with over 200,000 different data points to use, the so-called line of site correlation arguement could be refuted.
If it could be determined by this study that the apparent relationship between quasars and low red shift galaxies is not statistically consistent, one of Arp's legs could be abruptly removed from beneath him.
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Cougar emailed me about this thread and I thought it would be appropriate to comment on the discussion here.
Contrary to the dgruss23's reading of the paper, our measurement does not implicitly assume that the quasars were background objects. Rather, we merely selected the quasars based on photometric redshifts so that they were distintinctly separated in redshift from our galaxy sample (see our Figure 1). The cross-correlation is based on angular distance on the the sky, so there's no assumption of cosmology there. Likewise, the weighting scheme we used in the second series of measurements was based on the slope of the quasar number counts as a function of magnitude. As with the redshift selection, this was done because it's relevant to the lensing hypothesis, but we don't have to assume anything about cosmology to measure the slope. Now, when it comes to calculating the expected weak lensing signal to compare to the measurement, yes, we are assuming a standard cosmological redshift relation for quasars. Obviously, we could have calculated the expected signal based on a non-cosmological model, but the main thrust of this paper was to address the discrepancy between the various previous measurements of this cross-correlation. If anyone were interested in doing such a calculation to compare to our measurements, I'd be happy to share the raw numbers from our results for a comparison along the lines of our Figures 3, 7 and 8. Without doing such a calculation, however, my guess is that, if quasars were physically associated with galaxies, the cross-correlation between galaxies and quasars should be on order the auto-correlation of galaxies, rather than down by at least two orders of magnitude as we found in our measurement. Likewise, I wouldn't expect the amplitude of the signal to scale with the slope of the quasar number counts, as we demonstrated in our paper, although I'm not familar enough with the details of Arp's model to say for certain. Hope this helps to clarify things... |
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Let me qualify my previous statement. Considering the cross-correlation of galaxies and quasars, Scranton et al found a positive correlation with bright quasars and a negative correlation with faint quasars. This correlation makes no assumption about foreground galaxies/background quasars. It may have been expected, but it was not assumed.
Q. What is the natural explanation for such a finding? A. Gravitational lensing. Thereafter, Scranton et al did suppose, "Well, if this finding is due to lensing, we would have certain mathematical expectations according to the physics of lensing." So they tried weighting each quasar by the expected lensing signal and found that the result matched the expected lensing signature extremely well. I continue to assert that this finding does serious damage to the idea that quasars are physically associated with local galaxies.
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I'm just glad to see people interested in the paper; the disagreements between the various earlier attempts kept the measurement kind of obscure. Lensing people had originally looked at the magnification effect because the optics necessary to measure lensing shear weren't widely available. When it turned out that the non-uniformities in galaxy and quasar selection were really difficult to overcome, people lost interest.
The primary authors on the paper have been working on the measurement on and off for the last five years, so we've all been very pleased by the results we got when we switched from using spectroscopically selected quasars to the photometric sample in the paper. The behavior was the same in both cases, but the much, much larger photometric sample shrunk the error bars considerably. Now that we've shown it can be done reliably and basically comes for free for all of the planned multi-band large-area surveys that will follow the SDSS, we're busy working out new applications and making predictions for its future use in larger surveys. |
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I understand that your correlation analysis is a matter of quasar/galaxy distribution on the sky and can be analyzed independently of cosmological models. However, as you noted above - when you calculated the lensing signal - which is what Cougar and others seem to think refutes the local quasars hypothesis, then you did have to assume the standard cosmological redshift-distance relation for the quasars. I obviously was not specific enough as to when that assumption was brought into play in your analysis. My apologies for that. But my point to Cougar is that your conclusions about the lensing are dependent upon the quasars being at cosmological distances. So the lensing part of the analysis is not designed to refute the local quasars hypothesis. Yet he keeps insisting that it does refute the local quasars hypothesis. As for the correlation analysis, since Arp expects a correlation between the distribution of galaxies and higher redshift quasars, it would depend upon specific theoretical predictions as to whether the correlations in your paper specifically refute local quasars. In our discussions on this board I've tried to make clear the distinction between Arp's empirical model for ejection of quasars and the development of a theoretical explanation if he's right. What seems to get lost in these discussions is that the specific mathematical predictions such as those in your lensing analysis require a theoretical model. Unfortunately, Arp lacks a theoretical model that would allow such specific predictions about QSO-galaxy associations. The best that can be done at this time is general trends from the empirical relationships. However, as I did point out in an earlier post above (and on plenty of other threads in which I've discussed this with Cougar), there are several tests that can falsify the possibility of local quasars even without developing a specifical theoretical mechanism for ejection of quasars and intrinsic redshifts. Those tests are Time dilation and proper motions. Hawkins found that quasar variability does not exhibit time dilation as expected if they are at cosmological distances. Microlensing was initially advanced as an explanation, but more recent studies have shown microlensing is too small a player in QSO variability to account for the lack of time dilation. So this test is consistent with quasars being local - or at least the quasars studied by Hawkins. The proper motion test should be relatively simple but will probably take a decade or two if somebody actually conducts the study. The best candidates would be the quasars in the vicinity of M-82 which Arp has suggested are ejected from that galaxy. Since M-82 is a local galaxy, the proper motions will be detectable much sooner if the quasars are in fact local. Personally, I wouldn't be surprised if the basic cosmological picture is correct, but that intrinsic redshifts are an additional phenomenon superimposed upon any cosmological redshift from expansion. Anyway, congratulations on your results! It is obviously no small task to conduct the analysis and reductions on 200,000 QSO's and 13 million galaxies. |
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It also helps if you know the distances to the proposed parent galaxies of the quasars. That requires redshift independent distances - which for very distant galaxies are hard to come by. |
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Everyone is entitled to his own opinion, but not his own facts. |
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[Skipping a bit; I agree that this whole discussion would be easier if Arp had some concrete mechanism to test.] Quote:
By coincidence, I'm also part of a group working on a project tracking quasar variability using the repeat scans that have been done with the SDSS (an earlier attempt with SDSS data was done by Vanden Berk et al, 2004, ApJ, 601, 692, but we'll have many more epochs per object). We won't have quite the time base line (only 5-6 years), but we should be able to do much better on number of quasars and photometric accuracy. Time dilation should definitely be on the list of things to check, but one could easily imagine something like quasar duty cycle variations screwing things up. Given enough quasars, you could probably find a set where you're matching a lot of emission line strengths, but you'd have a hard time getting much redshift range. Tough problem. |
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One thing I think should also be considered here is that Arp's model doesn't prohibit gravitational lensing. Even though quasars are said to be "local", they are not all very local, they are just generally closer than their redshift distance. What I'm wondering is that would this same result be obtained due to gravitational lensing even if we assume that local quasar hypothesis is correct? There would be small subset of closeby quasars that would probably cause some deviation to the result, but would they cause too much deviation?
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Greetings, Scranton. Much thanks for your comments here in helping us to understand your research!
There is one aspect I was interested in regarding the use of photometric redshift data. There are an abundance of studies concerning the differences in spectroscopic and photometric redshift data, but I definitely don't speak the language of any of their authors! #-o I understand that photometric obesrvation is much more convenient, and that spectroscopy is much more accurate, but I don't understand what the specific errors are that need to be accounted for in order to 'calibrate' the photometric data to spectroscopic results. It can be seen in a number of spectroscopic versus photometric observation studies that correcting these errors may not be so easy! Are these aberrations the result of fundamental problems related to standard earth-based astronomy; atmosphere, etc? Did you encounter any interesting problems related this sort of calibration? If anyone else is interested, I found one readable reference on this subject: Photometric Redshifts: A Comparison of Methods Another interesting link came up while studying this: Hyperz: a new and public photometric redshift code The flow-chart introduction is very amusing =D>
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Ari: That's true, but runs into a couple problems. The primary one is that the gravitational clustering signal is intrinsically much stronger than the weak lensing signal. If the true distribution of quasars and galaxies was not two distinct annuli, but rather two annuli blended together, you'd quickly see the lensing signal swamped by the clustering signal (and measurements of the quasar auto-correlation function in redshift and angular space lead us to believe that quasars cluster gravitationally in much the same way as galaxies).
This leads to the second big problem, which is that the weak lensing signal is expected to change amplitude and sign as a function of quasar magnitude, while the clustering signal is always going to be positive. If you had overlap in physical space, you'd expect to see two effects (assuming that the overlap was such that you weren't completely dominating the lensing signal). At the bright end, you'd see a much stronger positive signal as you're adding both the positive clustering and lensing signals. However, the angular dependence of these two signals isn't quite the same, though, so the shape would look odd (admittedly, the error bars are probably big enough that this wouldn't be show-stopper by itself). At the faint end, you're adding two signals of opposite sign (positive clustering and negative lensing), so it's going to be a mess. Depending on how things are balanced, you could get a negative signal at small angles, transitioning to a positive signal at intermediate angles or a positive signal all around with a strong dip at small angles. In either case, if you do use the optimal weighting as we did in section 4.2 of the paper, then any physical overlap should show up as a strong deviation from the pure lensing signal we compare against in Figure 8. akirabakabaka: The biggest challenge in dealing with photometric redshifts is that you don't know the spectral shape a priori. Which is to say that, while all galaxy spectra are roughly similar, there is a fair bit of variation due to star formation activity and the like. As such, you can easily run into cases where you don't know if a galaxy is intrinsically a bit bluer and at a higher redshift or is intrinsically red and at a lower redshift. The ability of a photometric system to resolve these dilemma comes down to how the filters end up interacting with the space spanned by the galaxy spectra. For example, the SDSS filters have a problem with photometric redshifts around z ~ 0.4. It's not a defect, per se, just where this particular problem happened to crop up; if the filters were slightly different, then we'd have a similar problem at some other redshift. For the quasars, you've gotta slightly different problem. Ignoring the spectrum blue-ward of the Lyman alpha break, the main spectral shape of a quasar is a power-law. This is terrible for photometric redshifts since a red-shifted power-law remains the same power-law. Instead, the quasar photometric redshifts are mostly determined by the presence or absence of the strong emission lines. As such, instead of seeing a gradual reddening of all of the colors (g-r becoming larger and larger) as you might with galaxies, individual colors bounce around with increasing redshift, sometimes getting redder, sometimes getting bluer. When you combine all of the color information (u-g, g-r, r-i, i-z, etc.), you can get a sense of what's going on, but it's not as accurate as galaxy photometric redshifts. You also run into a lot more cases where you've gotta a good match to the colors at one redshift and but also a secondary match at another redshift. This added complication is why we adopted the method for selecting and weighting the quasars we described in the paper. |
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