RA/DEC (2000)
15:03:05.190 +22:02:04.10
225.771625 +22.034472
Type
CV
Redshift
0
Related AstroNotes: 2026-134
Reporting Group
None
Discovering Data Source
None
Discovery Date
2026-05-08 07:49:26.400
TNS AT
Y
Public
Y
Discovery Mag
13.9
Filter
Clear-
Reporter/s
Kirill Sokolovsky, Katie Barnhart, Darien Perla, Vallia Antoniou, Elias Aydi (Texas Tech University)

Spectra

 AT_2026lxf - 2026-05-09 22:45:07 Galileo / BC-Asi (Padova-Asiago)z=
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Light curves

 Other_Other_Clear
   
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
23682 2026-05-09 22:45:07 Galileo / BC-Asi 1200 D. Carli, P. Ochner P. Ochner Padova-Asiago tns_2026lxf_2026-05-09.948_Galileo_BC-Asi_Padova-Asiago.txt Object
Light Curves
Filter Tel / Inst Obs-date range JD Range Photometry
Clear- Other_Other 2026-05-07 10:55:12 - 2026-05-08 07:49:26 2461167.955 - 2461168.826 2
Photometry
ID Obs-date JD Mag. / Flux Err Lim. Mag./Flux Units Filter Tel / Inst Exp-time Observer/s Remarks
580954 2026-05-08 07:49:26 2461168.826 13.9 VegaMag Clear- Other_Other Dwarf nova candidate found with the NMW-TexasTech survey using two identical 135mm telephoto lenses + unfiltered QHY600M CMOS cameras. The transient was first detected on 2026-05-08.3260 UTC at CV=13.95 with one camera and confirmed in images taken with the second camera 78 minutes later on 2026-05-08.3803 at CV=14.01. The magnitude difference is not significant given the expected photometric uncertainty of 0.06 mag. The object was not detected above the magnitude limit of CV~15 on the images taken the previous night on 2026-05-07.4551. A blue Pan-STARRS 1 DR2 source PS1 134442257714871804 (g=21.38 +/-0.04, r=21.50 +/-0.05) is located at 15:03:05.16 +22:02:03.6 J2000, just 0.6" from the measured position of the transient (NMW-TexasTech image scale is 5.9"/pix). The plate-solved FITS images, finder charts and animations produced from the NMW-TexasTech images are available at https://tau.kirx.net/img/TCPJ15030519+2202041/ The NMW-TexasTech survey operates at TTU Preston Gott Skyview Observatory (Shallowater, Texas).
580953 2026-05-07 10:55:12 2461167.955 15 VegaMag Clear- Other_Other [Last non detection] The object was not detected above the magnitude limit of CV~15 on the images taken the previous night on 2026-05-07.4551.
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
302961 2026-05-10 14:11:35 Claudio Balcon Kirill Sokolovsky, Katie Barnhart, Darien Perla et al. 15:03:05.190 +22:02:04.10 2026-05-08 07:49:26.400 13.9 Clear- PNV Dwarf nova candidate found with the NMW-TexasTech survey using two identical 135mm telephoto lenses + unfiltered QHY600M CMOS cameras. The transient was first detected on 2026-05-08.3260 UTC at CV=13.95 with one camera and confirmed in images taken with the second camera 78 minutes later on 2026-05-08.3803 at CV=14.01. The magnitude difference is not significant given the expected photometric uncertainty of 0.06 mag. The object was not detected above the magnitude limit of CV~15 on the images taken the previous night on 2026-05-07.4551. A blue Pan-STARRS 1 DR2 source PS1 134442257714871804 (g=21.38 +/-0.04, r=21.50 +/-0.05) is located at 15:03:05.16 +22:02:03.6 J2000, just 0.6" from the measured position of the transient (NMW-TexasTech image scale is 5.9"/pix). The plate-solved FITS images, finder charts and animations produced from the NMW-TexasTech images are available at https://tau.kirx.net/img/TCPJ15030519+2202041/ The NMW-TexasTech survey operates at TTU Preston Gott Skyview Observatory (Shallowater, Texas). 2026TNSTR2027....1S N
Classification Reports
ID Time received (UT) Sender Classifier/s Group Classification Redshift Spectra Related files Assoc. Groups End prop. period Remarks ADS Bibcode
23679 2026-05-10 16:40:09 Andrea Reguitti Vittorio Andreoli (UniTn), Deborah Carli (UniPd), Andrea Farina (UniPd), Paolo Ochner (UniPd), Claudio Balcon (ISSP), Andrea Reguitti (INAF-OAPd) Padova-Asiago CV 0 1 Padova-Asiago A low-resolution spectrum was obtained with the 1.22-m Galilei telescope and B&C spectrograph (dispersion 2.25 Å/pixel) located in Asiago (Italy) on 2026-05-9.948 UT. The spectrum shows a blue continuum without Balmer lines, instead there are He I emissions 706.5 and 667.8 nm and He I absorption at 587.6; 447.1; 438.8; 414.4; 402.6; 381.9; 370.5 and 363.4 nm. A possible progenitor was found in GAIA DR3 database (Gaia collaboration et al. 2023) DR3 1261910766509656448 with an estimated g-mag 21.2 ± 0.1 that means Δmag ≈ 7.3.These characteristics are consistent with a Helium-rich cataclysmic variable. We propose to classify this target as a Helium-rich dwarf nova. 2026TNSCR2036....1A
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
23682 2026-05-09 22:45:07 Galileo / BC-Asi 1200 D. Carli, P. Ochner P. Ochner Padova-Asiago tns_2026lxf_2026-05-09.948_Galileo_BC-Asi_Padova-Asiago.txt Object

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