Please visit the International Supernovae Network (I.S.N.) web pages and VSNET (An International Mailing List of Variable Stars).
Image of SN 2002ap has been taken by Astronomical Mitja Šiška
5th of February 2002, at 18:41 UTC with CCD ST7 (no Filter), exposure: 120s,
telescope SC 10", f/6.3".
We estimate CCD magnitude near value 12.9.
Image of SN 2002ap has been taken by Astronomical group of Gymnasium Šentvid-Ljubljana
4th of February 2002, at 19:30 UTC with CCD ST7 (no Filter), exposure: 100s,
telescope SC 10", f/6.3".
We estimate CCD magnitude near value 13.0.
Members of our astronomical group are:
Kristina Meršak 1.a,
Dejan Kolarič 2.f,
Mitja Šiška 4.c,
Klemen Blokar 2.f,
Matija Kastelic 3.c,
Peter Mihor student,
Nejc Dolinšek 1.c,
Grega Hlupič 1.b,
Matjaž Alič 2.a,
Igor Prešern 4.c,
David Božič 1.c,
Nina Pogačnik 1.a,
Nejc Janež 2.f,
Mina Hiršman 3.f,
Rok Mališnik 1.c,
Tadej Gregl 1.c,
Šiška Igor 1.c,
Zorko Vičar.
Image of SN 2002ap has been taken by Matija Kastelic and Mitja Šiška
3rd of February 2002, at 20:59 UTC with CCD ST7 (no Filter), exposure:120s,
telescope SC 10", f/6.3".
We estimate CCD magnitude near value 13.0.
Image of SN 2002ap has been taken by Zorko Vičar
2nd of February 2002, at 19:03 UTC with CCD ST7 (no Filter), exposure:100s,
telescope SC 10", f/6.3".
I estimate CCD magnitude near value 13.1.
Supernova 2002ap (Type Ib/c-pec),
IAUC 7810 discovered Jan 29.4 2002 by Yoji Hirose
Found in M74 at R.A. = 1h36m23s.87, Decl. = +15o45'13".0 (AAVSO finder chart)
(Reinder Bouma finder chart)
Located 258" west and 108" south of the center of NGC 628 (= M74) (Yasuo Sano image)
Mag 13.3 and rising, Type Ib/c-pec (Hypernova?) (References: IAUC 7811)
Located 258" west and 108" south of the center of
NGC 628 (= M74)
Photos of
SN 2002ap have been taken by Zorko Vičar and Peter Mihor
1st of February 2002, at 19:18 UTC with CCD ST7 (no Filter), exposure:120s,
telescope SC 10", f/6.3", city Ljubljana, state Slovenia.
We estimate CCD magnitude near value 13.5.
See
Photometry Reference Images.
Picture is bad quality because image has been done from city Ljubljana,
where light pollution is very strong.
 |
| Supernova type criteria | |||||
| No Balmer Lines Type I |
Balmer Lines Type II | ||||
| Si II 6150 | No Si | Plateau |
Linear | ||
| He I 5876 | Weak He | then linear | |||
| Ia | Ib | Ic | IIP | IIL | |
URL: http://www2.arnes.si/guest/gljsentvid10/index.html
Secondary school
Gimnazija Šentvid-Ljubljana (astronomical group):
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