Talk:List of gravitational wave observations

Table entries/organizations
Despite WP:CRYSTALBALL, We might want to rethink entries/columns in the table. Several issues:
 * 1) The columns seem tuned to black hole merger events. Most of the columns do not really make sense for likely future observations such as continuous sources, GW background, etc.
 * 2) On the other hand, as a table of a binary merger events some properties are weighted more heavily (like energy) while being the least important.

Suggestions: TR 20:09, 27 September 2016 (UTC)
 * It is probably a good idea (for the future) to have separate tables for different types of events: binary mergers, continuous sources, burst sources, etc. (For now we only need the first).
 * In the table for binary mergers have separate columns for masses, spins, and nature of primary and secondary.
 * Probably include the LVT(s) in the same table but note their speculative nature.


 * I agree. I notice that the scholarly journals refer to these events as a "compact binary coalescence (CBC)".  Perhaps that could be the name of a list page with links to the different tables. Fantasticawesome (talk) 04:23, 17 March 2018 (UTC)

Would it be appropriate to include Joseph Weber's claims that he (and the Gran Sasso National Labs in Italy) observed gravitational waves from Supernova 1987A as a "candidate event"?
As references, see, , etc.

69.140.36.53 (talk) 03:15, 30 September 2016 (UTC)
 * I do not think that that would be appropriate, as those claims are widely disputed.TR 07:48, 30 September 2016 (UTC)

Unit conversions in table
I think we should remove the unit conversions from the table. They add a lot of clutter making the table harder to read. We can add a note to the column heading with conversions to other relevant units? As this involves a rather large change to the table, I'd rather get some feedback before being WP:BOLD about it.TR 08:36, 29 September 2017 (UTC)

"Remnant" for a merger?
I know that "remnant" is the term used to describe the collapsed object left behind by a supernovae explosion. But, does it also fit for the product of a collapsed object merger, in which only a small fraction of the mass is lost? WolfmanSF (talk) 14:44, 29 September 2017 (UTC)
 * This is the terminology that is used in for example all LIGO produced "fact sheets" (e.g. ). The use of this terminology becomes more obvious when you start looking binary neutron star mergers, where besides GWs some amount of matter may be ejected from the system at merger.TR 14:51, 29 September 2017 (UTC)

Spin
I removed the "spin" data from the table, as there was no information in, or near, the table to describe what this is, nor the units, e.g. Hz, rpm. If you put it back please state the units. GW150914 $0.68$ spin GW151226 $0.74$ spin GM170104 $0.64$ spin GW170814 $0.7$ spin Nick Beeson (talk) 21:31, 2 October 2017 (UTC)


 * It's a dimensionless parameter that ranges from 0 to 1. WolfmanSF (talk) 02:46, 3 October 2017 (UTC)

Primary, Secondary, Remnant columns
Should these columns be split into individual columns for the mass, spin, and "nature" (e.g. black hole, white dwarf, neutron star, etc.)?TR 08:18, 3 October 2017 (UTC)

Size of table and wiki code
When we use a display screen 21" or larger this table looks good, but when using a smaller display it becomes ugly, can anyone help to use additional wiki code to make the table has a horizontal scroll bar when using a small dispaly to keep it size like when using 21" or larger display? Does it affect when using on a smartphone? Earthandmoon (talk) 08:37, 9 November 2017 (UTC)
 * I set a global minimum width for the table. Does this help?TR 18:51, 9 November 2017 (UTC)
 * It looks ok, thank you. Earthandmoon (talk) 03:43, 10 November 2017 (UTC)

Table entries without full articles?
LIGO-SC just put out a preprint on a new, low-mass BH merger ([]). Would it be appropriate to add an entry to this table, without having the event name (GW170608) be a link to an article? Presumably this will become more relevant in the future, as statistics increase. Kelseymh (talk) 06:41, 16 November 2017 (UTC)
 * Makes sense to me, but a stub article looks quick to make as well. Tom Ruen (talk) 07:18, 16 November 2017 (UTC)

Chirp masses?
Should we add chirp masses to the table? The advantage is that they are much more accurately measurable. WolfmanSF (talk) 23:33, 16 November 2017 (UTC)

Wikidata Query / List of Gravitational Wave events
given that the list of gravitational wave events might somewhat grow in the future the following query might be useful: WikiData Query / List of Gravitational Wave events and wikipedia articles sorted by lang

--WolfgangFahl (talk) 11:34, 15 October 2018 (UTC)

Table entries for old events are outdated
The recent announcement also included updated values for all the previously announced events, usually slightly different from the previous values. Still more work to update everything. --mfb (talk) 11:08, 3 December 2018 (UTC)
 * Now updated. WolfmanSF (talk) 18:02, 6 December 2018 (UTC)

O3 candidates
There are too many... what a nice problem to have. Here is a neutron star merger candidate, and here is a list of all candidates (5 in the last 3 weeks). The information in that database is very rudimentary and likely to change with further analysis. I suggest to not include GraceDb candidates and wait for a proper analysis unless the candidates get significant media attention. --mfb (talk) 16:15, 25 April 2019 (UTC)
 * As the primary curator for those, what I've been doing is (by intention at least) only including events with a false alarm rate of less than 1 in 100 years, giving brief mention of events with a false alarm rate of 1-100 years, and ignoring sub-1-year-FAR objects unless there's some other notable quality. LIGO predicts that they'll be getting one every week or so, which has held quite true so far. Considering these events are virtually confirmed to exist- but the specifics haven't been hashed out yet- I'd say we should include them and, worst case scenario, we make a separate listing of preliminary GW reports until they can be formally reviewed in a paper. No point in holding off for weeks or months on something that's both in public accessibility and virtually confirmed to exist as a very first point of analysis. exoplanetaryscience (talk) 02:31, 26 April 2019 (UTC)
 * The main problem is not the question if these events are real (although we shouldn't neglect that: The false positive rate is purely from statistics, it doesn't include other causes). The problem is the poor knowledge about these events. We don't get much more than "we saw something", everything else is uncertain. --mfb (talk) 03:04, 26 April 2019 (UTC)
 * While I agree that that could potentially result in an overload of (non)information, I think that at the moment it's decently balanced and meaningful to list these. For the recent events, we have not only the fact that 'we saw something' but about where in the sky it is, what kind of object it probably came from, about how far away it is, and an indicator of whether that's something interesting or not. If this preliminary info weren't informational enough to be useful, then we wouldn't have just had a bunch of news outlets posting about the neutron star merger. exoplanetaryscience (talk) 20:51, 26 April 2019 (UTC)
 * See "unless the candidates get significant media attention". The GraceDB entries are primary sources meant for astronomers. If you think they absolutely have to be in the article put them in - I don't think it is a good idea but I won't remove them. --mfb (talk) 07:12, 27 April 2019 (UTC)
 * I think they should be here. I came here looking for exactly this. Fig (talk) 21:19, 27 April 2019 (UTC)

Looks like 0421 has been upgraded to 97% BBH... Fig (talk) 09:54, 4 May 2019 (UTC)

Primary vs secondary sourcing
I am concerned about basing an article largely on primary sources and whether your decisions on which reports to include count as original research or synthesis. I'm not going to take any action, as I don't see any conclusion being drawn, other than the interesting one that there is a lot going on. TomS TDotO (talk) 10:41, 4 May 2019 (UTC)
 * Correct me if I'm wrong, but I don't see what's wrong with using primary sources for an article if they're reliable and decently informative? exoplanetaryscience (talk) 19:56, 4 May 2019 (UTC)
 * WP:PSTS "Do not base an entire article on primary sources, and be cautious about basing large passages on them." WP:SYN "...do not combine different parts of one source to reach or imply a conclusion not explicitly stated by the source." I know that SYN does not exactly apply, for there is no conclusion stated. ANd I want to make it clear that I am not thinking of objecting, I'm just noting the topic. I am amazed at the large number and frequency of observatons. TomS TDotO (talk) 22:22, 4 May 2019 (UTC)
 * Since there is only one LIGO it’s perfectly obvious that all detections be will from their primary source, unless there is multi-messenger detection as in GW170817. The current frequency of detections, however, is exactly in line with theoretical predictions from multiple sources. Fig (talk) 08:11, 5 May 2019 (UTC)
 * WP:PRIMARY

"Policy: Unless restricted by another policy, primary sources that have been reputably published may be used in Wikipedia, but only with care, because it is easy to misuse them.[d] Any interpretation of primary source material requires a reliable secondary source for that interpretation. A primary source may only be used on Wikipedia to make straightforward, descriptive statements of facts that can be verified by any educated person with access to the primary source but without further, specialized knowledge. For example, an article about a novel may cite passages to describe the plot, but any interpretation needs a secondary source.


 * Do not analyze, evaluate, interpret, or synthesize material found in a primary source yourself; instead, refer to reliable secondary sources that do so.


 * Do not base an entire article on primary sources, and be cautious about basing large passages on them.


 * Do not add unsourced material from your personal experience, because that would make Wikipedia a primary source of that material. Use extra caution when handling primary sources about living people; see WP:Biographies of living persons § Avoid misuse of primary sources, which is policy."  TomS TDotO (talk) 17:08, 5 May 2019 (UTC)
 * This policy is less applicable to science than say, history or literature. Recent, ground-breaking scientific findings obviously need to be reported, and it could be a while before suitable secondary sources appear. WolfmanSF (talk) 17:26, 5 May 2019 (UTC)

The qualifier 'candidate' must be applied to all immediate claims for LVC triggers, with lapses in confirmatory discourse rampant throughout LIGO-Virgo social media and popular science articles during O3. Many non-astrophysical transients produce virtually identical waveforms as those assumed to be unique to GW events. No records of magnetometer or power mains fluctuations are presented by LVC, and their mention is avoided, despite that LIGO events are accompanied by unsettled magnetospheric-ionospheric conditions (substorms, particle injections, magnetospheric sawtooth events, unusual radio bursts, pulse-coupled global CG lightning mode).

Some non-rejected events still show a significant probability for terrestrial sources (the very fact of this ambiguity highlights the inexact and bias-prone nature of LIGO-Virgo phenomenology), and three (as of June 4, 2019 12:57 UTC) claimed events have been retracted (including the first reported event for O3, S190405ar, which was not effectively publicized as being a rejected event until the arrival of a second non-rejected candidate, S190412m. In addition to S190405ar, S190518bb and S190524q have been retracted. All three are considered terrestrial noise, yet met criteria for consideration as candidate events. https://gracedb.ligo.org/latest/ False alarm rate is considered virtually meaningless by LIGO, which calls into question yet again the neutrality of any motivation for nearly immediate updates for LVC events on Wikipedia - unprecedented in science, and potentially dangerous/misleading.

Systematic error likely affects parameters, as extremes in values for consecutive events for DL suggest: S190602aq FAR 1/T=16.673 yrs, DL 797±238 S190524q FAR 1/T=4.5458 yrs, [event retracted], DL 192±101 S190521g FAR 1/T=8.3367 yrs, furthest claimed LIGO DL 3931±953 S190519bj FAR 1/T=5.56 yrs, former furthest claimed LIGO DL 3154±791 S190518bb FAR 1/T=3.16 yrs, closest claimed DL [event retracted] 28±15 S190517h FAR 1/T=13.35 yrs, former furthest LIGO DL 2950±1038 S190426c FAR 1/T=1.63 yrs, DL 377±100 S190421ar FAR 1/T=2.13 yrs; DL 1628±535 S190405ar FAR 6756.4/T=1 yrs, [event retracted] DL 268±129. Fulguritics 13:16, 4 June 2019 (UTC)


 * Fulguritics I have seen your posts on Twitter responding to LIGO announcements. You are one of the tiny number of people who think that LIGO is not detecting gravitational waves, and your entire online presence seems geared towards this. As such you are promoting fringe science and therefore I do not believe your tagging of this page as NPOV is valid or itself impartial. This page is not the page for fighting ideological battles on gravitational wave detectors. If you want to do that you should do it at the LIGO talk page...but good luck finding any independent references for the ideas you are promoting.


 * I believe the NPOV tag should be removed from this page. Fig (talk) 08:56, 7 July 2019 (UTC)

At this point, NPOV tag should remain until independent assessment of O3 LIGO results is published, and realize that no peer-reviewed O3 LIGO publications yet exist. LIGO-Virgo would be unprecedented in their unchecked confidence given that this Wikipedia table is updated as soon as *candidate* signals are presented by LVC collab. here https://gracedb.ligo.org/. This page implies certainty. Candidates are uncertain. Therefore, the presentation of non-reviewed possible false alarms as equivalent to past, peer reviewed findings does not qualify as an unbiased approach.

There is no ideology behind appropriate criticism. One admits their inability to distinguish ideology from criticism when they sacrifice their logical consistency and disinterest. Any beliefs or personal sentiments regarding the capability of LIGO-Virgo to detect gravitational waves has no bearing on the applicability of the NPOV tag, as technically, we adhere to standards that LIGO has no control over. Opposition to equivocal criteria by which LIGO findings are vetted is not a fringe view. My role is purely to apply due controls to an experiment that has demonstrated no concern to publicize magnetometer data, power mains data, and other key onsite control system datasets that are essential to the rejection of LIGO signals, and must be maintained during findings regardless of Bayesian priors. LEt me remind one that LIGO noise floor in the best case for N=28 LIGO-Virgo triggers is 3 orders of magnitude above desired signal, and Numerical Relativity templates do not exist for all candidate transient signals.

There are many "independent" references and new studies in multiple geophysical/heliophysical contexts that are producing findings about the solar-terrestrial neighborhood and its energetic behavior that lead one to think twice regarding instantaneous acceptance of LIGO-Virgo signals, especially as three claimed triggers for O3 have been retracted as noise, and the distinctions between any number of upchirp-producing sources, most terrestrial, that trigger the LVC network are purely statistical, with rejection due to non-presence/"independence" of particular classes of "glitches." Most LIGO signals are accompanied by glitches, and their bearing on LIGO-Virgo signal rejection is weighted by apparent"network SNR." Fulguritics (Fulguritics) 11:49, 7 July 2019 (UTC)


 * Since these are labelled "preliminary" it should not instill certainty as you suggest. But perhaps we could have en extra sentence in the O3 introduction to say that the observations have not yet been published in a peer reviewed journal yet. Graeme Bartlett (talk) 12:04, 7 July 2019 (UTC)

Table formatting
How about colourising the primary and secondary ‘type’ cells - according to content - as with the o1, o2 and o3 runs? Fig (talk) 19:15, 12 May 2019 (UTC)
 * Done, how does that look? exoplanetaryscience (talk) 22:33, 13 May 2019 (UTC)
 * Good - nice one :) Fig (talk) 13:04, 14 May 2019 (UTC)

Moved O3 alerts to separate table
I moved the O3 alerts to a separate table. This are fundamentally different in nature than the confirmed events. They have not (yet) been subjected to the same detailed analysis as the confirmed events. Their primary function is to allow EM astronomers to follow up on events if they wish. As such the provided information is tailored such that they can make an informed decision on which events events to follow up. Added advantage is that we can now change the columns that we have for these alerts. Things like components and final masses and spins will not be published for alerts during O3, hence we don't need those columns for these events. Instead we can have dedicated columns for the information that is provided (such as the FAR).(TR 10:17, 5 July 2019 (UTC))

S190728q
GraceDB, 52% mass gap, 34% binary black hole, 14% neutron star black hole, IceCube has seen a neutrino that would be consistent with this event. Forbes article, search for S190728q to skip the irrelevant parts before. --mfb (talk) 11:42, 30 July 2019 (UTC)

S190814bv
S190814bv looks exciting - predicted to be almost certainly a "mass gap" observation. Tayste (edits) 23:52, 14 August 2019 (UTC)
 * Almost certainly NS/BH, an update changed the expectation completely. --mfb (talk) 04:51, 16 August 2019 (UTC)

S190828j/S190828l
Just 21 minutes apart, very similar sky localization. Let's look if a reliable source discusses potential gravitational lensing. --mfb (talk) 15:52, 28 August 2019 (UTC)
 * Very unlikely. News article, Blog article (Dutch). --mfb (talk) 01:01, 31 August 2019 (UTC)

2030s
Was informed in a talk yesterday that if things develop as planned, by the 2030s we'll get ~10,000 NS/NS and ~100,000 BH/BH merger detections per annum. WolfmanSF (talk) 20:22, 5 November 2019 (UTC)


 * By whom? In which talk? And on a substantial note: How are supposed to measure these? --MGChecker (talk) 21:35, 5 November 2019 (UTC)
 * You can find Samaya Nissanke's talk (starting at 3h 15', with that prediction made at 3h 35') here. WolfmanSF (talk) 22:15, 5 November 2019 (UTC)
 * Just like Lists of stars, we'll have to restrict lists to the notable ones. Gaia has data about nearly two billion objects, mainly stars and galaxies. --mfb (talk) 01:09, 6 November 2019 (UTC)
 * Well, at some point, we will have to think about this. However, at the moment we do not have to many observations yet. Let's wait how much is left from O3 after we have actual observations confirmed by the collaboration instead of some mere candidates. --MGChecker (talk) 15:44, 6 November 2019 (UTC)

what are "events" and "superevents"?
I think these terms have a technical meaning here and should be defined. "Event" is used in the "Nomenclature" section without definition and in a figure caption; "superevent" is used in a figure caption. For "superevent", I find a definition at ligo.org but it is too technical and I'm not sure I would get it right. Are events something "in the data" or"the real thing"? --Qcomp (talk) 21:27, 12 November 2019 (UTC)
 * The "superevent" nomenclature is particular to how things are reported in graceDB, and does not have any deeper physical meaning. (It is just a way of distinguishing different types of entries in the database. )TR 16:33, 13 November 2019 (UTC)
 * So is the difference between the "events" in the figure for O1 and O2 and the "superevents" for O3 that the latter are not yet confirmed? Would it be correct to extend the first sentence of the Nomenclature-paragraph to read
 * Gravitational wave events are named starting with the prefix GW, while observations that trigger a event alert but have not (yet) been confirmed are named starting with the prefix S and sometimes referred to as "superevents".
 * ? I think the article text should explain the technical terms (including those used in the figures) so that lay readers (like myself) know what to make of them.--Qcomp (talk) 13:18, 14 November 2019 (UTC)
 * Apparently you haven't noticed that the offending term has been removed from the article. WolfmanSF (talk) 20:29, 14 November 2019 (UTC)
 * no, it is still in the figure (the one displaying "LIGO & Virgo O3 Superevents" - that was where I stumbled across the term in the first place... --Qcomp (talk) 20:36, 14 November 2019 (UTC)

S200114f
where did you get its comment from? A three digit number for the frequency makes no sense if the whole event was only one period long. Its frequency spectrum must be extremely broad if that time is correct. --mfb (talk) 04:33, 14 January 2020 (UTC)
 * The report is from graceDB's initial.xml file: https://gracedb.ligo.org/apiweb/superevents/S200114f/files/S200114f-3-Initial.xml,0 I'm a bit skeptical myself of the cited frequency, but they seem to know what they're doing. I don't think I could confidently change the significant digits of the frequency without seeing any info on LIGO-Virgo's temporal resolution. exoplanetaryscience (talk) 04:54, 14 January 2020 (UTC)
 * That's the central frequency, a signal that short can't have a frequency that well-defined, and the database just reports the best fit with a silly number of digits in all cases. I rounded it to produce a useful statement. --mfb (talk) 20:56, 14 January 2020 (UTC)

Column ordering
Ideally, the Massgap column in O3 should come before the BH/BH column to preserve the order of increasing mass. I realise that’s a lot of work though... Fig (talk) 10:08, 19 January 2020 (UTC)

controversies
There are lots of controversies about the so-called discoveries of so-called gravitational waves. They should be discussed here. — Preceding unsigned comment added by 178.122.67.240 (talk) 00:19, 12 February 2020 (UTC)
 * Please add new sections at the bottom, not at the top. There isn't really a controversy in science. There is the science, and then there are a few people who can't accept it (most of the time for ideological reasons, as far as I can see) and make up stuff. --mfb (talk) 06:39, 12 February 2020 (UTC)

Events from non-LIGO analyses
At least two groups (in Princton, and the former LIGO group in Hannover) have re-analyzed the O1 and O2 data, finding a few more high significance events. How should we include them in this list?TR 22:54, 12 March 2020 (UTC)
 * One option might be to treat them the same, except adding a note to the publication date indicating the event was found in a later re-analysis. WolfmanSF (talk) 23:12, 12 March 2020 (UTC)
 * As a test, I've added the one extra event for O1.TR 09:35, 13 March 2020 (UTC)


 * For reference some of the relevant references:
 * Hanover group:
 * 1811.01921
 * 1910.05331
 * Princeton group:
 * 1902.10341
 * 1904.07214
 * 1910.09528
 * TR 08:51, 13 March 2020 (UTC)
 * I'm somewhat hesitant to put all of these in as observations due to their hesitant nature- LTV151012 was held from the list until last year because the 2.4% chance of a false signal wasn't considered strong enough evidence on its own. I propose we make a separate list of marginal detections whose existence is unconfirmed. exoplanetaryscience (talk) 22:16, 24 March 2020 (UTC)
 * Or we could add a false alarm rate column to the table. WolfmanSF (talk) 22:29, 24 March 2020 (UTC)
 * The last two of these preprints haven't been published either. &#32; Headbomb {t · c · p · b} 22:31, 24 March 2020 (UTC)
 * What do you guys think of this edit I made? exoplanetaryscience (talk) 00:22, 25 March 2020 (UTC)
 * I'm not sure I see much value in listing events with less than a 50% probability of being astrophysical in origin. Is there something interesting about them I'm missing? WolfmanSF (talk) 07:45, 25 March 2020 (UTC)
 * Well I thought about it this way: say you've got 7 different events with a 90% chance of being terrestrial noise. Statistically, one of them is probably a bona fide event. Sure, a lot of them have pretty low probabilities even below 10%, but nevertheless the fact that a possible signal was detected makes them worthy of at least a footnote to me. exoplanetaryscience (talk) 18:11, 25 March 2020 (UTC)
 * Given that we will be drowning in detections fairly soon, my preference would be to focus on the most meaningful events. WolfmanSF (talk) 23:33, 25 March 2020 (UTC)
 * what do you think? >50% p_astro detections only? exoplanetaryscience (talk) 20:45, 26 March 2020 (UTC)
 * I would suggest to limit it to only events that have been identified as "real" events by at least two sources. I.e. for O1+02 this would be the LIGO sources plus GW170121, GW170304, and GW170727.TR 14:53, 27 March 2020 (UTC)
 * I'd personally just make a tally of what's been reported in peer-reviewed venues, e.g. "In addition, 42 sources are considered potential observations at a lesser significance" or something. But I don't have any strong feelings on this. &#32; Headbomb {t · c · p · b} 20:05, 27 March 2020 (UTC)

probability
candidate events with a probability of near 1 to be terrestrial should not be listed here. i think a fair threshold would be either .9 or .5. this should not be a comprehensive academic review, and there are plenty of detections by now to try to be limiting the number of low relevancy events. — Preceding unsigned comment added by 2601:602:9200:1310:F86F:2D18:D52:FD1A (talk) 10:07, 4 June 2020 (UTC)

Published 03 events
I think we should move the published events from O3 to a separate table, either the same one used for O1/O2, or a new one. One of the many reasons is that the current table with public triggers does not have columns for listing the inferred source parameters.TR 18:25, 4 June 2020 (UTC)
 * Sounds reasonable. Maybe a new table, at least while the run is ongoing? At some point, we should also greatly trim the "Marginal detections" table. WolfmanSF (talk) 19:48, 4 June 2020 (UTC)

2023/O4 inclusion criteria
So: with O3 well behind us and O4 just began, it's time to start up a new discussion on how this page should change.

O4 event numbers O4 is clearly going to have a LOT of events over its duration - almost certainly in the hundreds, and possibly in the thousands. I've already trimmed previous detections with a >50% chance of being terrestrial, but that's not going to stop the many, many high-confidence events published otherwise. How should we deal with this fact? Include all events with a >50% chance of being real? Separate them into a different article - 'gravitational waves in 2023' for example? Most exclusion criteria I imagine would be fairly arbitrary, so limiting to only a small fraction of events would also need some justification for what can be considered truly 'notable'.

Confirmed events We currently have sections for event 'candidates' and a section for definitely confirmed events. Although in the past that's been pretty clear-cut, several years after O3's end we're now faced with at least one paper covering the rough parameters of just about every single O3 candidate. What should the policy be moving these to the confirmed events section? Some very insignificant ones (such as the 2019/04/26 event, so low-confidence that it's not even currently listed in the candidates section) have astrophysical parameters published in papers that acknowledge their insignificance and hedge their characterizations with "if it is a real signal, then-" So should anything, however insignificant, with a paper giving the relevant source parameters, be included? Should we wait for LIGO or some other authoritative body to make a press release on it? Bearing in mind that depending on how that question is answered, the section may inflate from its current 22 events to nearly 100 at the present moment, let alone in the near future.

---

Personally, I would still consider every single >50% astro-origin event notable on the grounds that we're seeing a decent portion of the entire observable universe: we're quite satisfied to cover events that happen billions of times a day in the universe because we can only see a couple, so why shouldn't we cover events that happen only once or twice a day in the universe that we're able to spot most of? The latter is objectively far more notable in the universe than the former. As for the 'confirmed' events section, I truly have no idea what to do there. I feel like, ideally, anything that can be classified as a candidate should ideally be moved to the top section whenever we're able to characterize it, but like I said, there's nothing stopping researchers characterizing improbable, low-SNR events just the same as ~100% astrophysical events. So I'm not sure of the best strategy. exoplanetaryscience (talk) 02:40, 2 June 2023 (UTC)


 * Yeh it's a conundrum with no obvious answer. Clearly O4 could end up being huge. I actually think that maybe the best looking-term solution is to have the sections based on the observing runs rather than the detection/candidate dichotomy. I would maybe merge O1 and O2 because they are small, but then O3, O4 etc have their own section, and inside, subsections for the detections and then candidates. Fig (talk) 20:52, 13 June 2023 (UTC)
 * I'm very iffy about the approach you have taken here ; 50% pAstro is not a very good criterion here. It leads you to include events like S230528a, S231025a or S231124z which are pretty dubious ; you should restrict that section to the ones labelled "Significant" and which were not retracted, as those have been manually vetted. Even among those, I expect a few not to make it to the final catalogues. Thuiop (talk) 12:57, 17 February 2024 (UTC)
 * @Exoplanetaryscience I would like to reiterate that the methodology you use for recent O4 events is very dubious to me. On what grounds do you include S240420ax as a candidate event ? The FAR is somewhat high at around 2/year, while for this kind of event we would expect to have tighter constraints than for CBC; as far as I am aware, no one seriously expects this event to be real (or at least to be confident enough to say it is).
 * You also mislabeled S240420da (should be dc), but it should not even be there ! These are events that basically nobody looked at, for which alerts are sent just in case but which are unlikely to make it in catalogs, and for which you have little guarantee against glitches. Same for 0407v, and plenty of the ones you put there for O4a. The only reason the pAstro can be high even with such a high FAR is that BBH are expected to be quite common (at the scale of the universe), meaning that a fair share of them are expected to be actual events, but without a way to tell which is which it is not very useful. There may be some science to be done using these events but I would certainly not put them in a Wikipedia page, especially considering that this puts them on an equal footing with catalogued events (for which there are much more thorough checks and thresholds). Thuiop (talk) 14:28, 24 April 2024 (UTC)
 * Hi, sorry I did not see your previous message here... you make valid points. For me personally, I see it as a debate about mindset; I know that many of the events may well not be real, but I would personally rather include events which are "probably" real than omit them. You on the other hand don't want the confident events muddied by uncertain ones, which I get. I did try to add some indicators of how confident an event was (like the "chance in O4" indicator) but I can see those being difficult for a casual reader to interpret.
 * So, thus far, I had been considering my full inclusion criteria as "is PAstro >50%?", and for unmodeled events checking for a FAR under 1e-7. Would your criteria be events under the label SIGNIF_LOCKED (FAR <8e-8) then? I'm open to the concept, though I would ask what of events like the edge-case S230609a, which has a PAstro of ~96% but isn't considered significant? exoplanetaryscience (talk) 00:52, 25 April 2024 (UTC)
 * Yes, using SIGNIF_LOCKED (or ADVOK) would be much better, as these are events that have been human-vetted (as catalog events are). These "edge" events still fall on the wrong side of the threshold, meaning that nobody looked at them. It might be that they are found significantly offline, or that a pAstro threshold is used instead of FAR for the catalog, but it is only at that point that they should go into the page. Thuiop (talk) 07:59, 25 April 2024 (UTC)
 * I've thought on it overnight, and you make a good point. I'll remove the low_signif events, though just listing them as a footnote. Considering 240420ax has a relatively low FAR on the same level as signif_locked events, I'll probably keep that for completeness (S200114f was later identified as probably at least partially astrophysical). exoplanetaryscience (talk) 03:27, 26 April 2024 (UTC)
 * Ok, thanks ! Thuiop (talk) 07:59, 26 April 2024 (UTC)

Hertz
The hertz is used for regular cyclical events, not for random events. Ehrenkater (talk) 07:24, 9 June 2023 (UTC)
 * Any rate can be given in Hz, doesn't have to be with constant times between events. You can find background rates given in Hz for a large range of different experiments. --mfb (talk) 11:32, 9 June 2023 (UTC)

Detection using pulsar timing
It isn’t clear to me about the detection using pulsar timing, the various Nanohertz observatories contribution to detection of gravitational waves. Is that sort of thing repressed here? Should it be? —— TomS TDotO (talk) 17:38, 1 July 2023 (UTC)


 * Sorry, I meant to say “represented” (not “repressed”!) ———- TomS TDotO (talk) 17:40, 1 July 2023 (UTC)


 * I believe it should be included - it's still a gravitational wave observation, even if it's not in the same frequency as LIGO detects. Unfortunately enough of the article is structured around LIGO detections, it's a bit difficult to say where exactly this would fit... It certainly deserves some better real estate than one sentence in the 'marginal detections' section, at the very least. exoplanetaryscience (talk) 21:49, 3 July 2023 (UTC)
 * Thank you. I was reluctant to write up what I did, because I didn’t know the proper terminology etc., or where to place it - or maybe I just missed the mention. But then I decided to “be bold”. TomS TDotO (talk) 22:44, 3 July 2023 (UTC)

Missing neutron-star detections
I'm calling it: there's a problem with the LIGO detectors that's made them not sensitive to neutron-star frequency signals. Yes, this is original research. But the probability of there only being a single NS detection at the current advertised sensitivity range, over 5 months, is essentially zero. It's a big shame; but the GW community is notoriously secretive about problems (it took KAGRA over a year to admit there was a problem with their detector). Fig (talk) 08:55, 5 October 2023 (UTC)
 * They have a few detections, it's not a very frequent event and the range is small. Anyway, if you don't have any suggestion for changes to the article then this talk page is not the right place. WP:NOTFORUM. --mfb (talk) 11:53, 5 October 2023 (UTC)
 * I've put plenty of suggestions up-page, thanks. Are you going to implement them? Fig (talk) 15:14, 5 October 2023 (UTC)
 * How have my changes been of late? Is there anything that still needs addressing? I thought I'd covered most of the outstanding to-do's. exoplanetaryscience (talk) 08:38, 17 October 2023 (UTC)
 * My outstanding suggestions, if you agree with them, are in the section "Column ordering" (which is think makes a lot of sense but is probably a lot of text manipulation); and the end of section "2023/O4 inclusion criteria", where I think in the long run the page should be divided by observation run rather than by events vs candidate events...(but this one is more of an opinion). Fig (talk) 12:02, 17 October 2023 (UTC)
 * I've fixed the mass gap ordering- it wasn't really that hard, which I am not complaining about. I'll think some more on the idea of separating the tables. exoplanetaryscience (talk) 01:37, 19 October 2023 (UTC)
 * Great work, thanks! Fig (talk) 19:29, 23 October 2023 (UTC)
 * Just for your information as this has nothing to do with the page : the probability of not detecting any BNS during O4a is definitely non-zero. And there is no issue with the detectors preventing specifically the detection of BNS. Thuiop (talk) 13:06, 17 February 2024 (UTC)