I am looking to find galaxy spectra of early type elliptical galaxies in the SDSS catalog by the objects name. See: https://dr12.sdss.org/advancedSearch. I dont know how to find out the PLATEID of my objects of interest, e.G. NGC 4125, NGC 4472 (Messier 49) or NGC 4649 (Messier 60), in the advanced search. I have tried to work with the constrains for redshift and sky position, but in the sdss library the objects name never turn up so I dont know if the found spectra are the spectra of the galaxies i mentioned. I am new to working with astrophysical data and the sdss catalogue in particular so please forgive me if this should be approached completely different. Can anyone tell me how to find these galaxy spectra fits files on the sdss website ? I am planning to further work with these fits files in python and extract kinematical parameters.
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$\begingroup$ Hi! Have you tried doing an SQL query of the catalogued data using SkyServer? skyserver.sdss.org/dr16/en/tools/search/sql.aspx $\endgroup$– Daddy KropotkinApr 30, 2021 at 16:16
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$\begingroup$ You might find this SkySearch SQL tutorial helpful cas.sdss.org/dr7/en/help/howto/search $\endgroup$– Daddy KropotkinApr 30, 2021 at 16:18
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1$\begingroup$ thank you very much for the hint I will have a look into it $\endgroup$– trynerrorApr 30, 2021 at 17:41
1 Answer
One thing you might try doing is to use the SkyServer Navigate interface to see if the object was imaged by SDSS. Enter the name in the "name" box in the upper left and then click on the "Resolve" button. If an image with the galaxy shows up, click on the "Object with spectra" checkbox in the "Drawing options" panel on the left, and red squares will appear for objects with spectra. If there's a red square associated with the center of your galaxy, then there's a spectrum. (You can click on the links on the right-hand side to find out more; there may even be a little graphic of the spectrum you can click on.)
Here's an example for the elliptical galaxy NGC 6066, which does have an SDSS spectrum (as indicated by the spectrum-plot graphic to the lower right):
Something you should be aware of: in many cases, very nearby and luminous galaxies like your three examples simply don't have SDSS spectra. (This is true for your three galaxies, in fact.) Since such galaxies were known to already have plenty of spectra (including redshift measurements), there was little need to get SDSS spectra of them, so they were ignored. So you may end up needing to focus on more distant elliptical galaxies (NGC 6066 has a redshift of 0.034, while your example galaxies all have redshifts $< 0.005$.)
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$\begingroup$ @DaddyKropotkin I rejected the proposed edit but accidentally clicked the wrong reason why. I think that is better posted as an additional and different answer by its author rather than edited in to someone else's answer, though that's just my view and (at)PeterErwin may disagree. $\endgroup$– uhohMay 1, 2021 at 3:52
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$\begingroup$ Thank you this tool is very handy and for my application easier to use then SQL querrys, since I am only interested in the method and not particular in big data analysis. Can you recommend a different spectra catalog for these kind of galaxies? I am looking specificly for these galaxies since I want to further compare results obtained by my implementation and earlier research. $\endgroup$ May 1, 2021 at 8:53
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$\begingroup$ Try to 2MASS option instead of SDSS $\endgroup$ May 1, 2021 at 14:01
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$\begingroup$ @DaddyKropotkin What does "2MASS option" mean? 2MASS was an imaging survey. $\endgroup$ May 1, 2021 at 18:33
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$\begingroup$ Oh yes sorry, that's only for an image. I tried editing your answer but it didn't go through - I think using a SkyServer SQL query is the optimal solution. Such a query does not require a big data analysis project: the query just requires a few lines of code and can output in many types of files, for example as a spreadsheet or a .txt It's really not a difficult thing, it takes a couple of hours, at most, to learn the lines of code you need to get the data you want, but once you learn it, it's a handy thing to know. The tutorial in the OP comments I left is very helpful, I used it myself $\endgroup$ May 2, 2021 at 16:21