[Aavso-photometry] [AAVSO-DIS] Close stars and aperture photometry
Michael Newberry
mnewberry at mirametrics.com
Fri Jan 18 20:58:25 EST 2008
Absolutely, you're right, it is. But rather than doing PSF fitting for the
star being measured, the tool is used for removing stars using the template.
It is called "star editing".
Michael
----- Original Message -----
From: "Doug Welch" <welch at physics.mcmaster.ca>
To: <aavso-discussion at mira.aavso.org>
Sent: Friday, January 18, 2008 4:21 PM
Subject: Re: [AAVSO-DIS] Close stars and aperture photometry
>
> Michael,
>
> This sounds like PSF fitting to me!
>
> Cheers,
> Doug
>
> Michael Newberry wrote:
>> Hi Michael and Nicola,
>>
>> In addition to PSF fitting, there's another way. By coincidence, we've
>> been
>> developing a Star Removal module for Mira, which is almost ready. There's
>> also one in IRAF---it's been some years since I used it, I think it is
>> called SEdit, or something like that. The way this method works is that
>> the
>> software creates a template of the star profile and then uses it to
>> subtract
>> the overlapping star(s) from the image. Then you can measure the target
>> object without any confusion.
>>
>> Michael Newberry
>>
>> ----- Original Message -----
>> From: "Michael Koppelman" <lolife at bitstream.net>
>> To: "Nicola Montecchiari" <superpolaris at gmail.com>
>> Cc: <aavso-discussion at mira.aavso.org>
>> Sent: Friday, January 18, 2008 12:29 PM
>> Subject: Re: [AAVSO-DIS] Close stars and aperture photometry
>>
>>
>>> Yes. You need to do PSF photometry if you want to untangle stars that
>>> are blended.
>>>
>>> M.
>>>
>>>
>>> On Jan 18, 2008, at 11:44 AM, Nicola Montecchiari wrote:
>>>
>>>> Let's say we have two stars Aand B and the ring of an aperture
>>>> photometry of star A overlaps the gaussian shape of star B and that I
>>>> can not have a smaller ring. Is this going to invalidate the measure?
>>>> I think so, but would like to know for sure.
>>> _______________________________________________
>>>
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>>>
>>>
>>
>>
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