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Images (S479) |
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Images (S481) |
Objects Session Notes
M101 - Spiral Galaxy with Supernova 2011fe Photometric Monitoring - Variables - R CrB
- CI Cyg, S Cyg, SS Cyg failed due to wind)Astrometric Monitoring - Nearby Stars - None
- 61 Cyg attempt (failed due to wind)
- Evening session (1.3 hrs), windy, cut short due to wind/cloud - Session operated under semi-automated control, with remote monitoring from indoors computer. - Ambient Temperature: 8.5°C (minimum) - CCD operation -20°C (at 69% average cooling). - main objective of the session to obtain follow-up images of bright supernovae in nearby galaxy M101 secondary objective was to image project stars for ongoing photometric analysis
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M101 with supernova 2011fe (Ursa
Major) |
SN 2011fe is reported as being the nearest Type Ia supernova seen in decades |
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M101 with SN 2011fe (fading slowly) | ||
New Image (T+54d) 2011-10-16.83 54 days after SN discovery SN Est. Mag +11.2 Annotated CCD Image (58% size, cropped) 7 x 60 sec exposure (average combine), 3x3 binning, C Filter 2011-10-16 20:00 h UT (#480169-78) 12" LX200R (at f/9.7) + ST-10XME |
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M101 with SN 2011fe - Earlier Image (2011-10-03) | ||
Earlier Image (T+41d) 2011-10-03.85 41 days after SN discovery SN Est. Mag +10.5 Annotated CCD Image (58% size, cropped) 11 x 60 sec exposure (average combine), 3x3 binning, C Filter 2011-10-03 20:28 h UT (#479003-14) 12" LX200R (at f/9.7) + ST-10XME |
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Images of SN 2011fe (in M101) on Supernova 2011 Page >> |
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This Web Page: | Images - Session 480 (2011-10-16) |
Last Updated : | 2024-06-16 |
Site Owner : | David Richards |
Home Page : | David's Astronomy Web Site |