Talk:Kitt Peak H-alpha Data

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--NicholasJamesKelley 07:20, 22 December 2007 (PST) H-Alpha images taken with the Kitt Peak Observatory has been Beneficial because it allows us to see Active Stars, T-Tauris' fortunately are very active. The two targets that I am monitoring are labeled as 415 and 416, and can be seen in this image.

  H-Alpha.jpg

This images alone allows me to make the statement that these objects emit H-Alpha. To take this idea to a new level we have developed a new way to look at H-Alpha intensity in comparision using simple photometry. The work and final products of this new approach are below.

  Star
415 (05 07 30.63,-06 11 00.1)
416 (05 07 30.21, -06 10 15.8)
ref1 (05 07 46.75,   -06 09 10.2
Ref2  (05 07 47.14   -06 09 46.1)
ref3  (05 07 37.40   -06 11 43.7)
ref4 (05 07 45.95   -06 13 13.2
ref5 (05 07 49.39   -06 11 39.4
ref6 (05 07 46.06   -06 12 20.2
ref7 (05 07 32.54   -06 13 07.0
  hA Intensity
415  158647.28
416  167325.391
Ref1  26830.305
Ref2  51520.008
Ref3   9200.643
Ref4 134461.094
Ref5  34399.918
Ref6  24596.813
Ref7  12920.03


R1	           R2	           R3	           R4
415 43521.02	  39019.879	39840.48	32770.988
416 13763.399	  17767.584	14823.522	14634.927
Ref1 4880.869	  5976.293	5184.819	5415.333
Ref2 11846.153	  11857.752	11317.155	10557.247
Ref3 2033.761	  2071.625	1948.087	1384.457
ref4 29362.744	  30389.764	26979.943	26288.033
ref5 7797.505	  8393.399	7646.638	7870.902
ref6 6451.765	  5386.33	 5251.918       4545.934
ref7 2509.687 	  3354.988	4532.651	2456.102
3/5/2007	  2/21/2007	2/27/2007	03/082007
Avg R	         Ratio(H/AvgR)
38788.09175	4.090102731
15247.358	10.974058
5364.3285	5.001614834
11394.57675	4.521449908
1859.4825	4.947958908
28255.121	4.758822091
7927.111	4.33952773
5408.98675	4.547397532
3213.357	4.020726611

RCC.jpg

The I band

--NicholasJamesKelley 08:16, 22 December 2007 (PST) This is the same proceedure that i used for for the R band in Comparison to H-Alpha this time though I used the I band as a Comparison.

Star	                              hA Intensity
415 (05 07 30.63,-06 11 00.1)	       158647.28
416 (05 07 30.21, -06 10 15.8)	       167325.391
ref1 (05 07 46.75 -06 09 10.2	        26830.305
Ref2  (05 07 47.14   -06 09 46.1)	51520.008
ref3  (05 07 37.40   -06 11 43.7)	 9200.643
ref4 (05 07 45.95   -06 13 13.2)       134461.094
ref5 (05 07 49.39   -06 11 39.4)        34399.918
ref6 (05 07 46.06   -06 12 20.2)        24596.813
ref7 (05 07 32.54   -06 13 07.0)	12920.03
I intensity	I intensity	I inetensity	I intensity
83941.086	82039.164	79750.445	86310.219
38087.754	39591.254	43700.785	37208.473
6738.003	6250.884	6566.5	         7151.164
9816.58       10866.196	10564.864	10967.834
2285.85	2566.026	2180.912	2767.535
26221.172	27226.857	27333.27	30301.652
6382.668	7225.333	6022.346	7721.122
4993.719	6441.247	4672.51	        4703.471
5098.407	4902.227	4184.837	5040.592
3/12/2007	3/11/2007	3/9/2007	2/21/2007
Avg I	         Avg H/I
83010.2285	1.911177488
39647.0665	4.220372546
6676.63775	4.018535377
10553.8685	4.881623075
2450.08075	3.75524072
27770.73775	4.841826501
6837.86725	5.030796408
5202.73675	4.727668183
4806.51575	2.688024064

ICC.JPG

Final Color Color plot

--NicholasJamesKelley 10:03, 22 December 2007 (PST) This is the final product of the other two posts, to understand stand this how this is benificial to my project you must first understand that H-Alpha is contained within the R Band. Therefore if one was to take the ratio of H-Alpha/R than you could seperate out the excess in H-Alpha from the R-Band. By comparing this to I/R we are compareing the amount of H-Alpha given off by an object to how much brighter the object is in the I band compared to the R band. T-Tauris' should not only have an excess in H-Alpha they should also appear brighter in the I band. Because a color color plot done on these two ideas would hopefully show where my targets would fall if it be in the area of a yso or a main sequence star.

Color color plot.JPG

As you can see in this plot both targets 415 and 416 both seperate from the other " Normal Stars" This shows that these two are indeed bright in H-Alpha and brighter in the I band than the R band.