AT 2019akv
RA/DEC (2000)
06:15:34.190 -29:14:31.31
93.892458 -29.242031
Type
CV
Redshift
Source Group
GaiaAlerts
Discovery Date
2019-02-02 05:49:55
TNS AT
Y
Public
Y
Discovery Mag
17.56
Filter
G-Gaia
Discoverer/s
A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts team

Spectra

 AT_2019akv - 2019-02-04 07:12:51 UH88 / SNIFS (SCAT)z=
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Show Tellurics 
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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
34992019-02-04 07:12:51UH88 / SNIFS1800TuckerSCAT tns_2019akv_2458518.8006_UH88_SNIFS_SCAT.datObjectSCATReduced with a summit quick reduction pipeline, care should be taken before reusing this data for future studies.
Light Curves
FilterTel / InstObs-date rangePhotometry
G-GaiaGaia_Gaia-photometric2018-12-16 06:12:57 - 2019-02-02 05:49:552
Photometry
IDObs-dateMag. / FluxErrLim. Mag./FluxUnitsFilterTel / InstExp-timeObserver/sRemarks
529642019-02-02 05:49:5517.560.2ABMagG-GaiaGaia_Gaia-photometric60Robot
529632018-12-16 06:12:5721.5ABMagG-GaiaGaia_Gaia-photometricRobot[Last non detection]
AT Reportings
IDTime received (UT)SenderReporter/s (Discoverer/s)GroupRADECDiscovery date (UT)Discovery Mag.FilterRelated filesAT TypeInternal nameAssoc. GroupsEnd prop. periodRemarks
295382019-02-03 18:52:48Gaia_Bot1A. Delgado, D. Harrison, S. Hodgkin, M. van Leeuwen, G. Rixon, A. Yoldas (University of Cambridge), on behalf of Gaia Alerts teamGaiaAlerts06:15:34.190-29:14:31.312019-02-02 05:49:5517.56G-GaiaPSNGaia19akcGaiaAlertsapparently hostless blue transient
Classification Reportings
IDTime received (UT)SenderClassifier/sGroupClassificationRedshiftRelated filesAssoc. GroupsEnd prop. periodRemarks
34922019-02-04 12:17:24tuckermaM A Tucker, A V Payne, A Do, M E Huber, B J Shappee (IfA UH Manoa)SCATCVSCATBlue spectrum with Halpha in emission and Hbeta+Hdelta+CaII in absorption at z=0. Likely CV but could also be another stellar variable, no obvious HeI/II or metal emission.