RA/DEC (2000)
01:48:43.210 -48:39:00.68
27.18004 -48.65019
Type
SN Ia
Redshift
0.02072
Discovery Date
2010-02-09 00:00:00.000
Public
Y
Host Name
NGC 692
Comments
[Discoverer=Monard; DiscoveryRef=CBET 2171; PositionRef=CBET 2171; Orig Type=Unknown]
Discovery Mag
16.4
IAU name
sn2010aa

Spectra

 SN_2010aa - 2010-02-15 00:00:00 VLT-UT3 / VIMOS (None)z=
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   Binning factor: (rounded to nearest integer >1)
Mouse hovers at WL: 0 (rest),0 (observed)
Spectra
ID Obs-date (UT) Tel / Inst Exp-Time Observer/s Reducer/s Group Spectrum ascii file Spectrum fits file Spec. Type Assoc. Groups End prop. period Remarks
3457 2010-02-15 00:00:00 VLT-UT3 / VIMOS 600 J. P. Anderson L. Galbany None tns_2010aa_2010-02-15_VLT-UT3_VIMOS.dat Object Host galaxy emission lines have been removed.
No Data
No Data
Classification Reports
ID Time received (UT) Sender Classifier/s Group Classification Redshift Spectra Related files Assoc. Groups End prop. period Remarks ADS Bibcode
3450 2019-01-28 20:58:37 Lluís Galbany Lluís Galbany, J. P. Anderson None SN Ia 0.02072 1 While looking at archival VIMOS data of SN host galaxies in the ESO archive, we found that one of the observations of NGC 0692 had a bright source that was not present in archival DSS images. We extracted a 2-arcsec aperture spectrum (4850-10000 A) at that location, and it clearly showed the main features of a type Ia supernovae at maximum light (S II W, Si II 5972 A, and Si II 6355 A). Host galaxy emission lines were superposed to the SN spectrum, and we measured a redshift of 0.02072 from H-alpha (in agreement with the galaxy redshift reported in NED, 0.02118). We estimate a Si II 6355 velocity of 12100 km/s. Comparing the SN spectrum with templates of several SNe of different types, GELATO (Harutyunyan et al., 2008, A&A, 488, 383) found the best fit to SNIa 2005am at +2.7 days past B-band maximum. 2019TNSCR.158....1G
Spectra
ID Obs-date (UT) Tel / Inst Exp-Time Observer/s Reducer/s Group Spectrum ascii file Spectrum fits file Spec. Type Assoc. Groups End prop. period Remarks
3457 2010-02-15 00:00:00 VLT-UT3 / VIMOS 600 J. P. Anderson L. Galbany None tns_2010aa_2010-02-15_VLT-UT3_VIMOS.dat Object Host galaxy emission lines have been removed.

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