SN 2018ata
RA/DEC (2000)
12:41:31.344 +26:01:59.16
190.3806 +26.0331
Type
SN Ia
Redshift
0.19
Discovery ReportClassification Report
Reporting Group
SNHunt
Discovering Data Source
SNHunt
Discovery Date
2018-04-10 06:30:17.000
TNS AT
Y
Public
Y
Host Name
NGC 4614
Host Redshift
0.0161
Discovery Mag
20.1
Filter
V-crts-CRTS
Reporter/s
Mirco Villi with CRTS
NEDSIMBADDECaLSPanSTARRS-1SkyMapperVizieRWISEDSSADS

Spectra

 ▌SN_2018ata - 2018-04-20 00:43:12 Ekar / AFOSC (Padova-Asiago)z=
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▌Show Tellurics 
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   Binning factor: (rounded to nearest integer >1)
Mouse hovers at WL: 0 (rest),0 (observed)
Spectra
SelectIDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
18852018-04-20 00:43:12Ekar / AFOSC2700S. Chen, Y. Cai, A. Reguitti, E. Congiu A. PastorelloPadova-Asiago tns_2018ata_2018-04-20.03_Ekar_AFOSC_Padova-Asiago. tns_2018ata_2018-04-20.03_Ekar_AFOSC_Padova-Asiago.fitsObjectPadova-Asiago
Light Curves
FilterTel / InstObs-date rangePhotometry
V-crts-CRTSOther_Other2018-03-22 07:51:42 - 2018-04-10 06:30:172
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
269092018-04-10 06:30:1720.1ABMagV-crts-CRTSOther_OtherSeen in four images.
269082018-03-22 07:51:4221.5ABMagV-crts-CRTSOther_Other[Last non detection] MLS 10K CCD. It would be nice if I didn't have to enter this same info every single time.
AT Reports
IDTime received (UT)SenderReporter/sReportting groupDisc. Data SourceRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
177212018-04-10 18:06:38ajdMirco Villi with CRTSSNHuntSNHunt12:41:31.344+26:01:59.162018-04-10 06:30:17.00020.1V-crts-CRTSPSNCRTS, SNHunt
Classification Reports
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarksADS Bibcode
18802018-04-20 14:22:57pastoS. Chen, Y. Cai, E. Congiu, A. Reguitti (Padova University), A. PastorelloPadova-AsiagoSN Ia0.191Padova-AsiagoThe spectrum resembles that of a normal Type Ia SN at about the B-band maximum light. The redshift is estimated through the broad SN features. We also note that although SNhunt368 is projected near NGC 4614 (z=0.016), it is associated to a much more distant foreground galaxy.2018TNSCR.520....1C
Related files
FileFile TypeCommentsLast Modified (UT)Modified By
tns_2018ata_classrep_1880_Padova-Asiago.pngGraphics2018-04-20 14:22:57pasto