2026fhe | Transient Name Server

RA/DEC (2000)

13:59:17.520 -37:52:42.30

209.823 -37.878417

Type

Redshift

0.001256

Discovery Report Classification Report

Reporting Group

MASTER

Discovering Data Source

MASTER

Discovery Date

2026-03-11 00:46:42.816

TNS AT

Public

Discovery Mag

16.1

Filter

Other-

Reporter/s

V.Shumkov, M.A.Kuznetsova, V.Lipunov, E.Gorbovskoy, A.Kuznetsov, K.Zhirkov, I.Panchenko, N.Tiurina, P.Balanutsa, V.Topolev, D.Vlasenko, G.Antipov, A.Sankovich, Yu.Tselik, Ya.Kechin, V.Senik, A.Chasovnikov, K.Labsina, I. Gorbunov (Lomonosov MSU), O.Gress, N.Budnev (ISU), C.Francile, F. Podesta, R.Podesta, E. Gonzalez (Observatorio Astronomico Felix Aguilar (OAFA), A. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory), A.Sosnovskij (CrAO), A. Gabovich, V.Yurkov (Blagoveschensk Educational StateUniversity), D.Buckley (SAAO), R.Rebolo (The Instituto de Astrofisica de Canarias), L.Carrasco, J.R.Valdes, V.Chavushyan, V.M.Patino Alvarez, J.Martinez, A.R.Corella, L.H.Rodriguez (INAOE, Guillermo Haro Astrophysics Observatory)

NED SIMBAD DECaLS PanSTARRS-1 SkyMapper VizieR WISE DSS ADS

Select	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
	23209	2026-03-11 22:26:23	Lesedi / Mookodi	600	io_robot SAAO	Moses Mlangeni	BlackGEM	tns_2026fhe_2026-03-11_22-26-23_Lesedi_Mookodi_BlackGEM.txt		Object			The spectrum is characterised by a blue continuum with a prominent emission feature consistent with Hα (6563 Å). The shorter-wavelength region of the spectrum is relatively noisy, and while weak structure is present, additional Balmer lines such as Hβ and Hγ are not unambiguously detected in the current spectrum. The combination of a blue continuum together with strong Hα emission is commonly observed in accreting cataclysmic variable systems, particularly dwarf novae during or near outburst phases. No spectral features consistent with supernovae are present.
Binning factor: (rounded to nearest integer >1) Mouse hovers at WL: 0 (rest), 0 (observed) ▌Show H at z=v_exp= km/s ▌Show He at z=v_exp= km/s ▌Show He II at z=v_exp= km/s ▌Show C II at z=v_exp= km/s ▌Show C III at z=v_exp= km/s ▌Show C IV at z=v_exp= km/s ▌Show N II at z=v_exp= km/s ▌Show N III at z=v_exp= km/s ▌Show N IV at z=v_exp= km/s ▌Show N V at z=v_exp= km/s ▌Show O at z=v_exp= km/s ▌Show [O I] at z=v_exp= km/s ▌Show O II at z=v_exp= km/s ▌Show [O II] at z=v_exp= km/s ▌Show [O III] at z=v_exp= km/s ▌Show O V at z=v_exp= km/s ▌Show O VI at z=v_exp= km/s ▌Show Na at z=v_exp= km/s ▌Show Mg at z=v_exp= km/s ▌Show Mg II at z=v_exp= km/s ▌Show Si II at z=v_exp= km/s ▌Show S II at z=v_exp= km/s ▌Show Ca II at z=v_exp= km/s ▌Show [Ca II] at z=v_exp= km/s ▌Show Fe II at z=v_exp= km/s ▌Show Fe III at z=v_exp= km/s ▌Show Å at z=v_exp= km/s ▌Show Å at z=v_exp= km/s ▌Show Å at z=v_exp= km/s ▌Show Å at z=v_exp= km/s ▌Show Tellurics ▌Show Galaxy lines at z= ▌Show WR-WN at z=v_exp= km/s ▌Show WR-WC/O at z=v_exp= km/s Remarks The spectrum is characterised by a blue continuum with a prominent emission feature consistent with Hα (6563 Å). The shorter-wavelength region of the spectrum is relatively noisy, and while weak structure is present, additional Balmer lines such as Hβ and Hγ are not unambiguously detected in the current spectrum. The combination of a blue continuum together with strong Hα emission is commonly observed in accreting cataclysmic variable systems, particularly dwarf novae during or near outburst phases. No spectral features consistent with supernovae are present.

AT 2026fhe

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