Hello all, During the processing of my last image I fount a faint object - looks like a faint cloud of gas. I tried to identify it in the registers (used Aladdin lite) but was unable to find a reference. Can you please help me identify it.  Thank you in advance! CS, Ivan
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
In what constellation are you looking at?
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Would that be at 8:52:46 +9:11:10? Do yoy have an Oiii only image?
No CSPN in PanSTARSS DR1 Nothing registered in HASH.
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Sven Eklund: Would that be at 8:52:46 +9:11:10? Do yoy have an Oiii only image?
No CSPN in PanSTARSS DR1 Nothing registered in HASH. Yes, that are the coordinates of the object. I imaged with a color camera so here are the separate channels. G and B should show OIII signal.  Thank you for the help. CS, Ivan
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
What is the total exposure time and at what f-number?
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
It would be worthwhile to collect some OIII data on the object. There is a "hot-enough" GALEX object nearby.  |
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Sven Eklund: What is the total exposure time and at what f-number? I am imaging with RASA8 at F2. Exposure time is 17 hours.
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Ivan Raichev:
Sven Eklund: What is the total exposure time and at what f-number? I am imaging with RASA8 at F2. Exposure time is 17 hours. Ohh, then you have plenty of photons! Still, I concur with Randy, try to get some Oiii data.
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Here is the GALEX UV color panel on that object with the cross hairs moved slightly off the object to see that it has a visible flux signal in the GALEX UV bands. The actual UV magnitudes collected by GALEX indicate a flux source right at the 18,000-20,000 degrees Kelvin threshhold where it is just hot enough to ionize any nearby nebulosity.  |
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Thank you for your support. I will collect more data the first chance I get.
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Excellent attention to the details in your image! Will look forward to your results.
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Ivan Raichev: Thank you for your support. I will collect more data the first chance I get. I am in Ha right now (Hyperstar 14") but the techs in Spain will change filter to Oiii late next week. I might be able to help you out then, given CS.
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Sven Eklund:
Ivan Raichev: Thank you for your support. I will collect more data the first chance I get. I am in Ha right now (Hyperstar 14") but the techs in Spain will change filter to Oiii late next week. I might be able to help you out then, given CS. This would be great. Thank you!
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Randy Lindstrom: Here is the GALEX UV color panel on that object with the cross hairs moved slightly off the object to see that it has a visible flux signal in the GALEX UV bands. The actual UV magnitudes collected by GALEX indicate a flux source right at the 18,000-20,000 degrees Kelvin threshhold where it is just hot enough to ionize any nearby nebulosity.
 Randy, may I ask where or how you can determine the temperature? Is it simply that stars with lower temperatures just wont be picked up by GALEX UV and since it is visible here it has to be that hot? /Sven
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Ivan Raichev:
Sven Eklund:
Ivan Raichev: Thank you for your support. I will collect more data the first chance I get. I am in Ha right now (Hyperstar 14") but the techs in Spain will change filter to Oiii late next week. I might be able to help you out then, given CS. This would be great. Thank you! Ivan, I just had a look at my Oiii data (5h, f/1.9, 4nm Baader Ultrahighspeed filter) and I cannot see any signal in that area. /Sven
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Thank you for your effort Sven. Then its a processing artifact of some sort. Sorry to waste your time  CS, Ivan
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.
Ivan Raichev: Thank you for your effort Sven.
Then its a processing artifact of some sort. Sorry to waste your time 
CS, Ivan Maybe. Or maybe you need more exposure time than 5h.
|
You cannot like this item. Reason: "ANONYMOUS".
You cannot remove your like from this item.
Editing a post is only allowed within 24 hours after creating it.
You cannot Like this post because the topic is closed.
Copy the URL below to share a direct link to this post.