V BAND PHOTOMETRY OF THE SN 2003gf SUPERNOVA UTILIZING THE 2MASS CATALOG
We obtained several images of SN 2003gf at the Marangani Observatory (Peru) on the night 3-4 July 2003 from which we have estimated its brightness in the V band, as 15.10 ± 0.09 mag. This was obtained after a proper calibration of the starfield, considering the photometric data of the infrared bands...
I tiakina i:
| I whakaputaina i: | Revista Mexicana de Astronomía y Astrofísica |
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| Ngā kaituhi matua: | , , , |
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
Universidad Nacional Autónoma de México
2013
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| Ngā marau: | |
| Urunga tuihono: | https://www.redalyc.org/articulo.oa?id=57128966016 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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