Forum der Vereinigung der Sternfreunde
https://forum.vdsastro.de/

WR 140 13.5.08
https://forum.vdsastro.de/viewtopic.php?f=17&t=2475
Seite 1 von 1

Autor:  Robin Leadbeater [ 14. Mai 2008, 19:31:15 PM ]
Betreff des Beitrags:  WR 140 13.5.08

A result from last night compared with Dec07-Jan08

LHIRES 600 l/mm 90min (18x5min) R~3200 S/N 120

(Vega used as "flat". Normalised using linear fit through Marchenko "continuum" wavelengths)

Robin

Dateianhänge:
wr140_13may08_mean_Dec07-Jan08_continfit.png
wr140_13may08_mean_Dec07-Jan08_continfit.png [ 10.51 KiB | 5033 mal betrachtet ]

Autor:  Thomas Eversberg [ 14. Mai 2008, 19:34:58 PM ]
Betreff des Beitrags: 

Great, Robin! That looks quite reliable, stable and solid. I'm impressed! :D
I believe that is a god baseline for the periastron passage.

Bye, Thomas

Autor:  Lothar Schanne [ 14. Mai 2008, 20:07:16 PM ]
Betreff des Beitrags: 

Hello Robin,

for comparison a spectrum of 12.5.2008, without any normalization. There are some variations around 570 nm.


C14, Lhires III, 40 um slit, 1200 g/mm grating, Sigma 1603ME, 1x1 binning, 4x20min. = 80 min exposition, not normalized, roughly calibrated, S/N = 170 [5970:5990].
FWHM of Na lines(D, 5890 und 5896) 1.52 A -> R >= 3875.

Dateianhänge:
WR140_20080512.png
WR140_20080512.png [ 55.03 KiB | 5025 mal betrachtet ]

Autor:  Robin Leadbeater [ 14. Mai 2008, 20:56:40 PM ]
Betreff des Beitrags: 

Zitat:
Hello Robin,

for comparison a spectrum of 12.5.2008, without any normalization. There are some variations around 570 nm.
hello Lothar,

That is interesting. I do not think I am seeing any significant change in my spectrum but your resolution and S/N is a bit better so perhaps you are seeing more than me. Do you have the spectrum as a fits file? I could normalize it in the same way and compare the two.

Best Regards
Robin

Autor:  Robin Leadbeater [ 15. Mai 2008, 12:05:47 PM ]
Betreff des Beitrags: 

Hello Lothar,

Thank you for the FITS file. I have made a comparison of the area of interest. (Normalized using points at 5635 and 5755A.)

Are there any real changes yet? I am not sure.

Note 5635 is not a Marchenko continuum point. This is the reason for the slope in the top of the emission line but I do not have the Marchenko point below this in my spectrum and I did not get a good comparison by extrapolating from the higher points. (I think there is a problem with the way Vspec calculates the spline fit. It sometimes includes points at the edges of the profile which it should not. I need to talk to Valerie about it)

Best Regards
Robin

Dateianhänge:
wr140_RL13may08_RLmeanDec07-Jan08_LS12may08.png
wr140_RL13may08_RLmeanDec07-Jan08_LS12may08.png [ 12.77 KiB | 5009 mal betrachtet ]

Autor:  Lothar Schanne [ 15. Mai 2008, 17:06:32 PM ]
Betreff des Beitrags: 

Zitat:
Are there any real changes yet? I am not sure.
Hi Robin,

no, I believe also, there is no significant change.

But ist is interesting to see the good overlapping of our spectra in spite of the different setups. That makes me happy ! :D

Seite 1 von 1 Alle Zeiten sind UTC+02:00
Powered by phpBB® Forum Software © phpBB Limited
https://www.phpbb.com/