RA/DEC (2000)
10:44:11.710 -59:44:26.59
161.048792 -59.740719
Type
Varstar
Redshift
0
Discovery ReportClassification Report
Reporting Group
GaiaAlerts
Discovering Data Source
GaiaAlerts
Discovery Date
2022-03-02 06:04:19.200
TNS AT
Y
Public
Y
Discovery Mag
13.92
Filter
G-Gaia
Reporter/s
S.T. Hodgkin, E. Breedt, A. Delgado, D.L. Harrison, M. van Leeuwen, G. Rixon, T. Wevers, A. Yoldas (IoA Cambridge), N. Ihanec, K. Kruszyńska, K.A. Rybicki, Ł. Wyrzykowski (Warsaw University Astronomical Observatory), Z. Kostrzewa-Rutkowska (Leiden Observatory), D. Eappachen (SRON/RU), G. Marton (Konkoly Observatory), on behalf of the Gaia Alerts team
NEDSIMBADDECaLSPanSTARRS-1SkyMapperVizieRWISEDSSADS

Spectra

 ▌AT_2022etv - 2022-03-31 19:07:55 SALT / RSS (WTFU)z=
▌Show H at z=vexp= km/s
▌Show He at z=vexp= km/s
▌Show He II at z=vexp= km/s
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▌Show N II at z=vexp= km/s
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▌Show N IV at z=vexp= km/s
▌Show N V at z=vexp= km/s
▌Show O at z=vexp= km/s
▌Show [O I] at z=vexp= km/s
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▌Show [O II] at z=vexp= km/s
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▌Show O V at z=vexp= km/s
▌Show O VI at z=vexp= km/s
▌Show Na at z=vexp= km/s
▌Show Mg at z=vexp= km/s
▌Show Mg II at z=vexp= km/s
▌Show Si II at z=vexp= km/s
▌Show S II at z=vexp= km/s
▌Show Ca II at z=vexp= km/s
▌Show [Ca II] at z=vexp= km/s
▌Show Fe II at z=vexp= km/s
▌Show Fe III at z=vexp= km/s
▌Show Å at z=vexp= km/s
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▌Show Tellurics 
▌Show Galaxy lines at z=
▌Show WR-WN at z=vexp= km/s
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   Binning factor: (rounded to nearest integer >1)
Mouse hovers at WL: 0 (rest),

Light curves

 ▌Gaia_Gaia-photometric_G
   
Pointer position (MJD, Mag, Abs.Mag): (0.00, 0.00, 0.00)
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
12312 2022-03-31 19:07:55 SALT / RSS 300 SALT J. Brink WTFU tns_2022etv_2022-03-31_19-07-55_SALT_RSS_WTFU.txt tns_2022etv_2022-03-31_19-07-55_SALT_RSS_WTFU.fits Object Spectrum is not flux calibrated due to lack of observation of standard star taken with the same setup as a science target.
Light Curves
Filter Tel / Inst Obs-date range JD Range Photometry
G-Gaia Gaia_Gaia-photometric 2021-11-11 01:19:12 - 2022-03-02 06:04:19 2459529.555 - 2459640.753 2
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
272062 2022-03-02 06:04:19 2459640.753 13.92 0.2 ABMag G-Gaia Gaia_Gaia-photometric 60 Robot
272061 2021-11-11 01:19:12 2459529.555 21.5 ABMag G-Gaia Gaia_Gaia-photometric Robot [Last non detection]
AT Reports
ID Time received (UT) Sender Reporter/s Reporting group Disc. Data Source RA DEC Discovery date (UT) Discovery Mag. Filter Related files AT Type Host name Internal name Assoc. Groups End prop. period Remarks ADS Bibcode Unreal Auto classification
142022 2022-03-14 10:51:33 Gaia_Bot1 S.T. Hodgkin, E. Breedt, A. Delgado et al. GaiaAlerts GaiaAlerts 10:44:11.710 -59:44:26.59 2022-03-02 06:04:19.200 13.92 G-Gaia Other Gaia22axt GaiaAlerts ~0.3 mag rise in Gaia source and YSO candidate 2022TNSTR.704....1H N
Classification Reports
ID Time received (UT) Sender Classifier/s Group Classification Redshift Spectra Related files Assoc. Groups End prop. period Remarks ADS Bibcode
12254 2022-04-12 17:44:08 Mariusz Gromadzki Mariusz Gromadzki WTFU Varstar 0 1 WTFU Spectrum shows stellar continuum affected by Galactic and Interstellar extinction with absorption lines of hydrogen (Balmer series), He I and few diffuse interstellar bands. This suggests that the transient is a brightening of an early B-type stars.The transient is located just 4 arcsec away from a Young Stellar Object candidate found in Povich et al. 2011, as reported by Simbad. We suspect the brightening detected by Gaia is actually a signature of the YSO identified earlier, but the coordinates in Simbad are incorrect and the star Cl* Trumpler 14 Y 340 is the actual YSO. 2022TNSCR.954....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
12312 2022-03-31 19:07:55 SALT / RSS 300 SALT J. Brink WTFU tns_2022etv_2022-03-31_19-07-55_SALT_RSS_WTFU.txt tns_2022etv_2022-03-31_19-07-55_SALT_RSS_WTFU.fits Object Spectrum is not flux calibrated due to lack of observation of standard star taken with the same setup as a science target.

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