AT 2016blf
RA/DEC (2000)
06:34:12.716 -32:59:49.62
98.552983 -32.997117
Type
CV
Redshift
Source Group
ASAS-SN
Discovery Date
2016-03-30 02:52:48
TNS AT
Y
Public
Y
Discovery Mag
16.1
Filter
V-Johnson
Discoverer/s
J. S. Brown, for the ASAS-SN team

Spectra

 AT_2016blf - 2016-04-17 01:44:50 SOAR / Goodman (ASAS-SN)z=
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   Binning factor: (rounded to nearest integer >1)
Mouse hovers at WL: 0 (rest),
Spectra
SelectIDObs-date (UT)Tel / InstExp-TimeObserver/sReducer/sGroupSpectrum ascii fileSpectrum fits fileSpec. TypeAssoc. GroupsEnd prop. periodRemarks
6342016-04-17 01:44:50SOAR / GoodmanJay Strader, Laura Chomiuk, Laura Shishkovsky (MSU) ASAS-SN tns_2016blf_2457495.5728104_SOAR_Goodman_ASAS-SN.txt tns_2016blf_2457495.5728104_SOAR_Goodman_ASAS-SN.fitsObjectASAS-SN
Light Curves
FilterTel / InstObs-date rangePhotometry
V-JohnsonASASSN-2_Cassius2016-03-23 03:21:36 - 2016-03-30 02:52:483
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
19742016-03-30 02:52:4816.1VegaMagV-JohnsonASASSN-2_Cassius270ASASSN
19752016-03-24 01:26:2416.4VegaMagV-JohnsonASASSN-2_Cassius270ASASSN
19732016-03-23 03:21:3617.1VegaMagV-JohnsonASASSN-2_Cassius270ASASSN[Last non detection]
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
17652016-03-31 22:44:05brojonatJ. S. Brown, for the ASAS-SN teamASAS-SN06:34:12.716-32:59:49.622016-03-30 02:52:4816.1V-JohnsonPSNASASSN-16doASAS-SN
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
6252016-12-06 13:37:49jlprieto Jay Strader, Laura Chomiuk, Laura Shishkovsky (MSU)ASAS-SNCVASAS-SNWe obtained an optical spectrum of ASASSN-16do/AT2016blf (ATel #8888) on UT 2016 April 17.07 with the Goodman Spectrograph on the SOAR telescope. The source has a blue continuum and broad double-peaked Balmer and He 5875 emission at z~0, with an H-alpha FWHM of about 2400 km/s. This value is high for a CV and suggests the source is observed close to edge-on.

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