The following is an archived discussion of a featured article nomination. Please do not modify it. Subsequent comments should be made on the article's talk page or in Wikipedia talk:Featured article candidates. No further edits should be made to this page.

The article was promoted by Karanacs 19:29, 14 April 2009 [1].


GRB 970508[edit]

Nominator(s): Cryptic C62 · Talk 22:35, 29 March 2009 (UTC)[reply]

I've successfully brought this article through a very rigorous GA review by the very vigorous Wronkiew. It is a very short article, but I believe it is sufficiently comprehensive without going into the absurdly technical details. There are no gamma-ray bursts which have been brought to FA yet (this is even the first GA, I believe), so I don't really have a reference point. Oh well. It's good to WP:BEBOLD, eh? --Cryptic C62 · Talk 22:35, 29 March 2009 (UTC)[reply]

  • Fix the disambiguation links, found with the links checker tool in the toolbox.
  • External links check out fine with the links checker tool in the toolbox.
  • Book refs that use multiple pages should be formatted as pp. not p.
  • Other ref formatting checks out fine with the WP:REFTOOLS script.--Best, RUCӨ 22:43, 29 March 2009 (UTC)[reply]
Struck resolved issues. --Cryptic C62 · Talk 22:49, 29 March 2009 (UTC)[reply]
  • this was the first measurement of the distance of a gamma-ray burst. - shouldn't that be the distance to a gamma-ray burst?
  • Until this burst, astronomers were in disagreement over how far away GRBs were occurring. - tense - don't they still occur?
  • Unambiguously - wouldn't 'unequivocally' be better?
  • Dale Frail should be announced as an astronomer
  • There are more instances of minor grammatical problems throughout the article. Parrot of Doom (talk) 23:57, 29 March 2009 (UTC)[reply]
I've fixed the comments you've mentioned. Any other issues? --Cryptic C62 · Talk 00:31, 30 March 2009 (UTC)[reply]
I'll have a read through the article. Parrot of Doom (talk) 17:43, 30 March 2009 (UTC)[reply]


Otherwise, sources look okay, links checked out with the link checker tool. Ealdgyth - Talk 15:48, 30 March 2009 (UTC)[reply]
I've expanded the circular citation, though I'm still not entirely sure what the correct format for a circular is. I've also corrected those dates from 1999 to 1997; that was my mistake. --Cryptic C62 · Talk 16:00, 30 March 2009 (UTC)[reply]
Looks good. When in doubt, cite it like a web page... Ealdgyth - Talk 16:03, 30 March 2009 (UTC)[reply]
  1. The lead contains information that is not mentioned in the main text (A gamma-ray burst is a highly luminous flash of gamma rays, the most energetic form of electromagnetic radiation, often followed by a longer-lived "afterglow" emitting at longer wavelengths (X-ray, ultraviolet, optical, infrared, and radio).) and thus violates WP:LEAD.
    Now included in the first paragraph of Discovery.
  2. The article is not fully complaint with 1(b). In particular it should provide better context for this discovery. I want to see a short section about BeppoSAX satellite (and possible about Ulysses) and more information about GRBs in general.
    Hrm, do you suggest I just plop a pargraph into Observations? Or should I start a new section called Background or some such?
    I will be satisfied with a paragraph. One of the main goals of BeppoSAX was investigation of the nature GRBs. This discovery was not accidental, it was planned. Ruslik (talk) 06:29, 2 April 2009 (UTC)[reply]
    I've added an introductory paragraph. I decided not to include Ulysses, but I did expand upon that bit later on.
  3. What was the energy of gamma-rays detected by BeppoSAX and Ulysses?
    The Ulysses detection wasn't published. It was cited in Pian's article as a private communication from Kevin Hurley. I will try to find more information about the gamma-ray detection.
    Whew! I managed to find some information on the energy according to BeppoSAX and BATSE. --Cryptic C62 · Talk 00:03, 5 April 2009 (UTC)[reply]
  4. Regarding optical afterglow. What was the spectral range, in which it was observed?
    I've added a paragraph about this. I must admit that I understood very little of what I read, so I may not have found exactly what you were looking for. --Cryptic C62 · Talk 22:32, 2 April 2009 (UTC)[reply]
    If I could interrupt here—this added paragraph is a bit jargon-heavy. I would suggest something like
    About 5 hours after the burst, the apparent magnitude of the object—a measure of its brightness—was 20.3 ± 0.3 in the U-band (the ultraviolet region of the spectrum) and 21.2 ± 0.1 in the R-band (the red region of the spectrum). This is approximately the same apparent magnitude as the moons of Pluto.Citation needed, see Apparent magnitudeThe afterglow reached its peak luminosity in both bands approximately 2 days after the burst was detected—19.6 ± 0.3 in the U-band at 02:13 UTC on May 11, and 19.8 ± 0.2 in the R-band at 20:55 UTC on May 10. (A lower apparent magnitude corresponds to a greater brightness)Citation needed Several optical spectra were obtained at the Calar Alto Observatory at wavelength ranges of 4300-7100 Å and 3500-8000 Å, though no emission lines were identified in any of these spectra.[1]
    There is probably a better choice of object for the apparent magnitude comparison though.Dr pda (talk) 00:04, 3 April 2009 (UTC)[reply]
    I like your paragraph, it's much more user-friendly than the crap that I churned out. However, I have two problems with making a magnitude comparison: First, comparing a specific band's magnitude with a the total magnitude of another might be misleading or confusing. Second, I haven't found any mention of a comparison in the journals. To come up with our own comparison would be WP:OR. Besides, if the reader really wants to get a better sense of this scale, s/he can just follow the link to apparent magnitude. --Cryptic C62 · Talk 00:56, 3 April 2009 (UTC)[reply]
    Fair enough. Dr pda (talk) 01:49, 3 April 2009 (UTC)[reply]
    Alright, changed. What do you think, Ruslik? --Cryptic C62 · Talk 02:08, 3 April 2009 (UTC)[reply]
    I actually do not think that a simple comparison is an OR. Ruslik (talk) 07:39, 5 April 2009 (UTC)[reply]
  5. Although the Caltech team and a competing team in Amsterdam were hesitant to publish... What is "Amsterdam team"? Is this the team of Djorgovski?
    It actually refers to Jan van Paradijs, Titus Galama, and Paul Groot. Later tonight I'll try expanding the observations section to include more about what they did. If it doesn't seem to fit, we can just delete it altogether, I suppose. --Cryptic C62 · Talk 20:11, 1 April 2009 (UTC)[reply]
    Done. --Cryptic C62 · Talk 00:46, 2 April 2009 (UTC)[reply]
  6. Further analysis of the burst by Frail, Waxman, and Kulkarni indicated that the total energy released by the burst was approximately 5×1050 erg, They assumed that the radiation was isotropic, did not they? This should be clarified.
    I'm fairly certain that they assumed it was isotropic, but the source doesn't explicitly say one way or the other. It does mention Rhoads's paper and his previous analysis of the beaming, so I've added that. --Cryptic C62 · Talk 20:11, 1 April 2009 (UTC)[reply]
  7. Although the isotropic distribution of bursts suggested that they do not occur within or nearby the Milky Way This is wrong. Isotropic distribution is fully compatible with the Milky Way origin of GRBs, provided that they are located in the halo, not in the disk.
    Whoops, you're quite right. Don Lamb made it very clear in his debate with Paczynski that the isotropic distribution only excludes the disk. Corrected. --Cryptic C62 · Talk 20:11, 1 April 2009 (UTC)[reply]
  8. Was the host galaxy of this GRB investigated? And what results were obtained?
    Woot, I added a nice little section about the host galaxy and incorporated some information from Observations. Is this what you had in mind? --Cryptic C62 · Talk 23:28, 1 April 2009 (UTC)[reply]
    So the red shift of the host coincides with the first redshift determined from the absorption lines? Ruslik (talk) 06:29, 2 April 2009 (UTC)[reply]
    Yes, I've clarified that. --Cryptic C62 · Talk 17:28, 2 April 2009 (UTC)[reply]

images Academia is a rich source of free images, the image can be illustrated with images of the observatory, diagrams of red shift, equipment... the graphical content to brighten up the article is here on wp, you dont even have to look for it. Fasach Nua (talk) 18:54, 3 April 2009 (UTC)[reply]

Okey doke, I've added pictures of BeppoSAX and the VLA. Do you think it needs any more? --Cryptic C62 · Talk 22:51, 4 April 2009 (UTC)[reply]
The new images look great, however the two Hubble images are indistinguishable unless they are right next to each other, giving the appearance that you have included the same image twice. You could try cropping the galaxy in the second image so it displays at full resolution as a thumbnail. Not a major issue though. Wronkiew (talk) 05:07, 9 April 2009 (UTC)[reply]
Hmm, the problem with cropping either image is that it might give the false impression that the host galaxy was significantly larger than the afterglow (or vice versa). The value of having both images at the same size is that it allows the reader to make an accurate comparison between the two, but I suppose that's hard to do when they're not next to each other... --Cryptic C62 · Talk 14:25, 9 April 2009 (UTC)[reply]
Fasach Nua has responded here, he will not revisit. For all purposes of discussion, this concern was addressed. Dabomb87 (talk) 15:56, 13 April 2009 (UTC)[reply]

Comment I'm very close to supporting but I'd like to see each sentence that mentions a number or figure have an inline cite per WP:V. --mav (talk) 16:19, 12 April 2009 (UTC)[reply]

Done. --Cryptic C62 · Talk 20:12, 12 April 2009 (UTC)[reply]

Support Great article. --mav (talk) 03:33, 13 April 2009 (UTC)[reply]

The above discussion is preserved as an archive. Please do not modify it. No further edits should be made to this page.
  1. ^ Castro-Tirado 1998