M51 with SN2011dh
M51 with SN2011dh
Just a personal record of this supernova while weather permits. Unfortunately seeing was really poor and clouds roll in quickly after the object passed meridian last night.
M51 with SN2011dh
Tai Po, 5-Jun-2011, 20:21-22:31 HKT
11 x 300s L Channel, Astrodon filter
TOA-130 f/7.7, QSI-583, EM-200
Autoguide via Lodestar + OAG
CCDStack, PS CS5, cropped and resized
M51 with SN2011dh
Tai Po, 5-Jun-2011, 20:21-22:31 HKT
11 x 300s L Channel, Astrodon filter
TOA-130 f/7.7, QSI-583, EM-200
Autoguide via Lodestar + OAG
CCDStack, PS CS5, cropped and resized
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- 110605_M51_11x300s_L.jpg (104.22 KiB) 已瀏覽 3926 次
Re: M51 with SN2011dh
Congratulations!anguslau 寫:Just a personal record of this supernova while weather permits. Unfortunately seeing was really poor and clouds roll in quickly after the object passed meridian last night.
M51 with SN2011dh
Tai Po, 5-Jun-2011, 20:21-22:31 HKT
11 x 300s L Channel, Astrodon filter
TOA-130 f/7.7, QSI-583, EM-200
Autoguide via Lodestar + OAG
CCDStack, PS CS5, cropped and resized
I went to PTC last night, transparency was quite good while the Polaris was not visible. The clouds rolled in after the equipment was set up.
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Took more images of the object on 9-Jun. Sky conditions were similar: transparancy good, seeing poor. Managed to get some RGB data as well. Also used LPS-P2 filter this time. Below are the LRGB and L versions of the image.
I noticed that the SN seemed to have brightened up! Not sure if this make sense at all. Or was it affected by the use of the LPS filter. Did some rough measurement using MaxIm. I got a reading of Mag 14.5 on 5-Jun and Mag 13.4 on 9-Jun.
M51 with SN2011dh
Tai Po, 9-Jun-2011, 23:30-00:51 HKT
8 x 300s L channel, 3 x 5 x 300s RGB channels
Astrodon filters, LPS-P2 filter
TOA-130 f/7.7, QSI-583, EM-200
Autoguide via miniBORG50 + Lodestar
CCDStack, PS CS5, cropped and resized
I noticed that the SN seemed to have brightened up! Not sure if this make sense at all. Or was it affected by the use of the LPS filter. Did some rough measurement using MaxIm. I got a reading of Mag 14.5 on 5-Jun and Mag 13.4 on 9-Jun.
M51 with SN2011dh
Tai Po, 9-Jun-2011, 23:30-00:51 HKT
8 x 300s L channel, 3 x 5 x 300s RGB channels
Astrodon filters, LPS-P2 filter
TOA-130 f/7.7, QSI-583, EM-200
Autoguide via miniBORG50 + Lodestar
CCDStack, PS CS5, cropped and resized
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- 110609_M51_8x300s_L1crop.jpg (97.45 KiB) 已瀏覽 3375 次
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- 110609_M51_8-5-5-5x300s_LRGB1.jpg (76.71 KiB) 已瀏覽 3375 次
最後由 anguslau 於 週六 11 6月, 2011 15:43 編輯,總共編輯了 2 次。
Just checked other records. Indeed the SN is brightening up!
http://www.rochesterastronomy.org/sn2011/sn2011dh.html
http://www.rochesterastronomy.org/sn2011/sn2011dh.html
Yes, this time the SN is obviously brighter than the one you took 5th Jun.anguslau 寫:Took more images of the object on 9-Jun. Sky conditions were similar: transparancy good, seeing poor. Managed to get some RGB data as well. Also used LPS-P2 filter this time. Below are the LRGB and L versions of the image.
I noticed that the SN seemed to have brightened up! Not sure if this make sense at all. Or was it affected by the use of the LPS filter. Did some rough measurement using MaxIm. I got a reading of Mag 14.5 on 5-Jun and Mag 13.4 on 9-Jun.
M51 with SN2011dh
Tai Po, 9-Jun-2011, 23:30-00:51 HKT
8 x 300s L channel, 3 x 5 x 300s RGB channels
Astrodon filters, LPS-P2 filter
TOA-130 f/7.7, QSI-583, EM-200
Autoguide via miniBORG50 + Lodestar
CCDStack, PS CS5, cropped and resized
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