[Mr Jack Martin]

Robin,

Are you monitoring the H alpha line ?

Regards,

Jack

Essex UK

[Mr Jack Martin]

Robin,

I have followed your instructions and opened the file in BASS.

Thank you,

Jack

Essex UK 

[Mr Jack Martin]

Paul,

Thank you for your encouragement, its good to know others are following the forums.

Onwards and upwards.

Regards,

Jack

Essex UK

[Mr Jack Martin]

No changes in H Alpha emission profile as of 2017-08-13, I am continuing to monitor.

Jack

Essex UK

[Mr Jack Martin]

Robin,

I will open your fits file in my other computer which has the appropriate program.

Regards,

Jack

Essex UK

[Mr Jack Martin]

Robin,

This was just a 300 s raw exposure uncalibrated, no dark or flat frames just to check if the h alpha line has changed.

Regards,

Jack

Essex UK

[Mr Jack Martin]

Robin,

The response I am waiting for is if you are able to do a comparison between the spectra obtained by Marc and my spectra, as taken with Marcs C11 and my C14.

Please refer to Marcs previous post for info.

Regards,

Jack

Essex UK

[Mr Jack Martin]

Robin,

I can’t open your attachment.

Regards,

Jack

Essex UK 

[Mr Jack Martin]

Andy,

You mean like this, the latest ‘quick’ spectrum of vv cep taken around 22.00 hr 2017-08-10 revealing no changes in the h alpha profile yet.

Regards,

Jack

Essex UK

[Mr Jack Martin]

Andy,

In our last communication I measured the resolution and inserted it the fits file.

I have posted a png file of my latest ‘quick’ spectrum of the h alpha profile of vv cep.

Regards,

Jack

Essex UK   

[Mr Jack Martin]

Marc,

I am awaiting Robins response on this one.

Also, just a minor point to resolve before I can upload spectra to the database.

Regards,

Jack

Essex UK

[Mr Jack Martin]

Marc,

I can send data to Robin for analysis who can post comparative results on this forum for the benefit of all. 

Jack

Essex UK

[Mr Jack Martin]

Steve,

I will follow your instructions.

Thanks for your response.

Jack

Essex UK 

[Mr Jack Martin]

Robin,

I am keen to submit my data for further analysis as suggested by Marc, BUT I use BASS not ISIS to do my data reduction.

Thank you for your input, any further comments welcome.

Jack

Essex UK

[Mr Jack Martin]

Marc,

I use Shelyak SE0002B Lhires III 4 position slit NOT the photometric slit as advised by Olivier Thizzy sometime ago.

Regards,

Jack

Essex UK

[Mr Jack Martin]

Hello all,

I would attach a calibration lamp spectrum.

But bigger than 2 MB is there any way round this ?

Regards,

Jack

Essex UK 

[Mr Jack Martin]

Marc,

Perhaps the difference between our spectra is due to the fact that you use Angstrom units and I use nanometers so a factor of 10 out.

Ernst take note but I am sure you account for this when combining our results.

Regards,

Jack

Essex UK

[Mr Jack Martin]

Marc,

I am using a 23 micron slit as opposed to 35 micron.

So would the difference in slit width account for changes in the baseline ?

The weather here in the UK is not good.

Regards,

Jack

Essex UK

[Mr Jack Martin]

Attached is last nights 2017-07-25 result.

Still no change in the V H alpha emission line.

Regards,

Jack

Essex UK

 

[Mr Jack Martin]

[Author]

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