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Images (S511) |
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Images (S513) |
Objects Session Notes
M101 - Spiral Galaxy with Supernova 2011fe Photometric Monitoring - Variables - R CrB, S Cyg, AM Her, SS Her, U Her
(CY Cyg, SS Cyg, DY Per ER UMa attempts - failed due to cloud/dew)Astrometric Monitoring - Nearby Stars - None
- Evening session (1.7 hrs duration). - Session operated under semi-automated control, with remote monitoring from indoors computer. - Ambient Temperature: 10.0°C (minimum) - CCD operation -20°C (at 79% average cooling). - main objectives of the session were to acquire images of selected project stars for ongoing photometric and astrometric analysis. - Notes from 2012-08-03 (updated flats)
M101 with SN 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+346d) 2012-08-03 346 days after SN discovery SN Est. Mag +16.5 Annotated CCD Image (58% size, cropped) 5 x 60 sec exposure (average combine), 3x3 binning, C Filter 2012-08-03 22:26 h UT (#512215-19) 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 >> | ||
SN 2011fe Light Curve | ||
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This Web Page: | Images - Session 512 (2012-08-03) |
Last Updated : | 2024-06-16 |
Site Owner : | David Richards |
Home Page : | David's Astronomy Web Site |