PSN J12355230+2755559 (= AT 2016blu) campaign - Alert Notice 847

weo
Affiliation
American Association of Variable Star Observers (AAVSO)
Tue, 01/23/2024 - 19:05

AAVSO Alert Notice 847 announces an observing campaign beginning immediately on the very interesting SDOR variable PSN J12355230+2755559 (= AT 2016blu) (Com). Please see the notice for details and observing instructions.

There are threads for this campaign under the following AAVSO forums:

- Campaigns & Observation Reports: https://www.aavso.org/psn-J-12355230-2755559-2024
- Cataclysmic Variables: https://www.aavso.org/psn-J-12355230-2755559-2024-01

Please subscribe to these threads if you are participating in the campaign so you can be updated. Join in the discussion or ask questions there!

Many thanks, and Good observing,

Elizabeth O. Waagen, AAVSO HQ

MZK
Affiliation
American Association of Variable Star Observers (AAVSO)
Detection??

My image tonight seems to show a detectable brightening? Needs confirmation.

Ken

Aghakhanloo
Affiliation
American Association of Variable Star Observers (AAVSO)
Based on the magnitude you…

Based on the magnitude you reported (16.776), it is very likely that it is undergoing the predicted eruption. Unfortunately, being new to this platform, I am unsure of how to view the image you took.

MZK
Affiliation
American Association of Variable Star Observers (AAVSO)
Needs Confirmation

This target is not easy to measure due to the very small adjacent contaminant nebulosity. We should get another confirmation. The are 2 other recent observers, so hopefully they will image again soon.

I'm planning to take another image tonight if weather cooperates. I'll try to get the image to you via email?

Ken

Aghakhanloo
Affiliation
American Association of Variable Star Observers (AAVSO)
Yes, it would be great if…

Yes, it would be great if you send them to me via email. Thank you.

MZK
Affiliation
American Association of Variable Star Observers (AAVSO)
Not outburst?

Probably a false alarm after second image 2 hours later? Really a tough target due to small contaminant nebulosity and faintness?

Should probably use a larger scope than the 12" I used (iT18) to get better resolution? I'll try again!  ;-)

Ken

BHarrisHBB
Affiliation
American Association of Variable Star Observers (AAVSO)
My Photometry

I have just submitted 3 days of photometry:

1/29/24  16.886R

1/31/24  16.794R

2/1/24    16.981R

Cloudy last night.

 

Barbara

BHarrisHBB
Affiliation
American Association of Variable Star Observers (AAVSO)
Redo photometry

I decided to redo my photometry after looking closer at the DSS chart. My initial photometry included this wide complex. I repeated the photometry and used an annulus that only included that portion of the star that is close to the galaxy's core. With that annulus, these are my results:

 

1/29/24    17.544(R)  ERR 0.022

1/31/24    17.654(R) ERR 0.030

21/25       17.710(R) ERR 0.027

 

Barbara

Aghakhanloo
Affiliation
American Association of Variable Star Observers (AAVSO)
Thanks for sharing the image…

Thanks for sharing the image. Yes, AT 2016blu is the star closer to the galaxy.

BHarrisHBB
Affiliation
American Association of Variable Star Observers (AAVSO)
FEB 3 Photometry

Mag       18.181R, ERR 0.055,  JD 343.810

 

Barbara

cdk
Affiliation
American Association of Variable Star Observers (AAVSO)
No AT 2016 blu found adjacent to HII region of IC 3550

On JD 343.71, a stack of 24 x 90sec exposure images with my 14 inch telescope reveals no star at expected position near the HII region (IC 3550)

I found an annotated SLOAN image on web page: https://cseligman.com/text/atlas/ic35a.htm which shows a close-up of the IC 3550 region (Courtney Seligman).  I assume the AT2016blu is one of the two stars at the lower right of the main HII region, SE of the main HII region adjoining the main nebulosity.  My stacked CCD images show no distinct stars there which I interpret as no flare-up of AT 2016 blu.  Any comments?

 

Don Collins (CDK)

Aghakhanloo
Affiliation
American Association of Variable Star Observers (AAVSO)
Yes, AT 2016blu is one of…

Yes, AT 2016blu is one of the two stars, the one closer to the galaxy is AT 2016blu. If AT 2016blu is very faint, then, as you said, it means it is not experiencing an eruption. However, if it is bright, then it is experiencing an eruption.

cdk
Affiliation
American Association of Variable Star Observers (AAVSO)
By "the galaxy" do you mean…

By "the galaxy" do you mean IC 3550 or the big near-by galaxy NGC 4959?

 

Thanks, CDK

DEY_VAR
Affiliation
American Association of Variable Star Observers (AAVSO)
"Big galaxy" ID was wrong

Greetings,

The "Big Galaxy" nearby this object with the long name, PSN J12355230+2755559 (= AT 2016blu), is NGC 4559. It is located in Coma Berenicis and is of Sc type.

Ahhh, the wonders of real-time editing... I'll play along... subject line "is" is now "was".  Have fun, we are getting well paid for this.

Jim (DEY)
 

Aghakhanloo
Affiliation
American Association of Variable Star Observers (AAVSO)
Sorry for the typo; I meant…

Sorry for the typo; I meant NGC 4559. Most likely, CDK also meant NGC 4559, not NGC 4959.

cdk
Affiliation
American Association of Variable Star Observers (AAVSO)
I also made a typo.  I see…

I also made a typo.  I see from my telescope program that the "big Galaxy" is NGC 4559 (also Caldwell 36).

Star AT 2016 blu is next to IC 3550

The link below is an image of IC 3550 I've download from the web (a sloan image).  I have marked a star within the IC 3550 with hatch marks.  Is the marked star our target: AT 2015 blu?

https://aavso-cdk.blogspot.com/2024/02/ic-3550-hii-region-near-ngc-4559.html

Thanks,

CDK

cdk
Affiliation
American Association of Variable Star Observers (AAVSO)
Thank you.  I clearly did…

Thank you.  I clearly did not see it on JD 343.7.

 

Don (CDK)

MDJ
Affiliation
Liga Iberoamericana de Astronomia (South America) (LIADA)
PSN J12355230+2755559

Dear All, my photometry

 

PSN J12355230+27555592460347.7258832024 Feb. 07.22588 17.387 0.069 R MDJ

Image:

https://drive.google.com/file/d/1dDcnOV74C2N16HG9QIKe8O29XR9RXHgv/view?usp=drive_link

 

Regards.

 

Prof. Daniel J. Mendicini

SEV-CODE/LIADA.

Santa Fe, Argentina.