This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.24 21:59:12.69 +42:08:23.3
91.98149 -10.15213 galactic Lac Second-epoch detections are separated by 7.4" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.8004+42.1419 | 21:59:12.69 +42:08:23.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:12.69 +42:08:23.3: 12.38 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:12.69 +42:08:23.3: 14.46 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.8004+42.1419,2461172.8579,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.8004+42.1419 20260512.3579 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.60 21:56:43.44 +37:32:19.1
88.66477 -13.44775 galactic Cyg Second-epoch detections are separated by 1.4" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.1826+37.5389 | 21:56:43.44 +37:32:19.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:43.44 +37:32:19.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:43.44 +37:32:19.1: 13.95 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1826+37.5389,2461172.8579,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1826+37.5389 20260512.3579 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.48 21:41:34.32 +34:36:23.6
84.31044 -13.66421 galactic Cyg Second-epoch detections are separated by 1.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:34.32 +34:36:23.6 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.237+/-0.050 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:34.32 +34:36:23.6: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:34.32 +34:36:23.6: 14.61 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.29 21:42:11.57 +36:19:08.9
85.58878 -12.48166 galactic Cyg Second-epoch detections are separated by 0.4" and 2.7 pix
The object was found in VSX 1" Gaia DR3 1950901384257092480
Type: ROT
# Max. Min./Amp. JD0 Period
14.420 G 14.450 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:11.57 +36:19:08.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:11.57 +36:19:08.9: 14.55 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950901384257092480,2461172.8579,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950901384257092480 20260512.3579 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.36 22:02:54.20 +40:44:54.5
91.66868 -11.67530 galactic Lac Second-epoch detections are separated by 1.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:54.20 +40:44:54.5 (user input) | T | P | (position from user input) J-Ks=0.641+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:54.20 +40:44:54.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:54.20 +40:44:54.5: 14.38 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.43 21:48:53.93 +36:09:36.7
86.52058 -13.49618 galactic Cyg Second-epoch detections are separated by 0.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:53.93 +36:09:36.7 (user input) | T | P | (position from user input) J-Ks=0.729+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:53.93 +36:09:36.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:53.93 +36:09:36.7: 14.87 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.38 21:37:06.39 +33:54:16.9
83.12344 -13.55018 galactic Cyg Second-epoch detections are separated by 2.1" and 3.1 pix
The object was found in VSX24" WISE J213705.8+335440
Type: EW
# Max. Min./Amp. JD0 Period
14.054 r Y 0.401 r 2458374.83370 0.390860800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:06.39 +33:54:16.9: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:06.39 +33:54:16.9: 14.95 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J213705.8+335440,2461172.8579,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J213705.8+335440 20260512.3579 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.27 21:38:16.22 +34:33:06.6
83.75909 -13.24311 galactic Cyg Second-epoch detections are separated by 3.0" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.5744+34.5531 | 21:38:16.22 +34:33:06.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.575+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:16.22 +34:33:06.6: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:16.22 +34:33:06.6: 14.69 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.5744+34.5531,2461172.8579,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.5744+34.5531 20260512.3579 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.35 21:48:57.03 +38:28:35.1
88.07612 -11.74661 galactic Cyg Second-epoch detections are separated by 2.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:57.03 +38:28:35.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.766+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:57.03 +38:28:35.1: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:57.03 +38:28:35.1: 14.14 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.26 21:50:40.99 +39:31:45.3
89.03275 -11.16118 galactic Cyg Second-epoch detections are separated by 1.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:40.99 +39:31:45.3 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:40.99 +39:31:45.3: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:40.99 +39:31:45.3: 14.53 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.21 21:32:45.94 +37:06:19.5
84.72111 -10.62025 galactic Cyg Second-epoch detections are separated by 1.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:32:45.94 +37:06:19.5 (user input) | T | P | (position from user input) J-Ks=0.194+/-0.069 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:45.94 +37:06:19.5: 12.53 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:45.94 +37:06:19.5: 14.39 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.29 22:10:18.73 +41:32:58.6
93.29964 -11.86906 galactic Lac Second-epoch detections are separated by 2.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:10:18.73 +41:32:58.6 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:18.73 +41:32:58.6: 13.23 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:18.73 +41:32:58.6: 15.05 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.24 21:59:20.80 +39:40:39.1
90.44826 -12.10161 galactic Lac Second-epoch detections are separated by 1.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959210531060529664 | 21:59:23.76 +39:41:05.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:20.80 +39:40:39.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:20.80 +39:40:39.1: 14.20 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959210531060529664,2461172.8579,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959210531060529664 20260512.3579 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.48 21:55:29.67 +36:36:05.8
87.85759 -14.01639 galactic Cyg Second-epoch detections are separated by 1.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:29.67 +36:36:05.8 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:29.67 +36:36:05.8: 12.71 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:29.67 +36:36:05.8: 14.91 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.39 21:56:43.41 +41:51:09.7
91.43231 -10.09024 galactic Cyg Second-epoch detections are separated by 0.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.1700+41.8569 | 21:56:43.41 +41:51:09.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.515+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:43.41 +41:51:09.7: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:43.41 +41:51:09.7: 15.00 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.00 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1700+41.8569,2461172.8579,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1700+41.8569 20260512.3579 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.14 21:40:11.20 +37:48:07.1
86.30211 -11.11366 galactic Cyg Second-epoch detections are separated by 2.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.0467+37.8006 | 21:40:11.20 +37:48:07.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:11.20 +37:48:07.1: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:11.20 +37:48:07.1: 13.99 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.0467+37.8006,2461172.8579,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.0467+37.8006 20260512.3579 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.29 22:03:12.09 +37:15:34.4
89.52134 -14.46846 galactic Lac Second-epoch detections are separated by 0.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:12.09 +37:15:34.4 (user input) | T | P | (position from user input) J-Ks=0.522+/-0.079 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:12.09 +37:15:34.4: 13.47 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:12.09 +37:15:34.4: 14.33 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.35 21:54:14.01 +35:39:31.5
87.03323 -14.57826 galactic Peg Second-epoch detections are separated by 3.0" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:14.01 +35:39:31.5 (user input) | T | P | (position from user input) J-Ks=0.451+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:14.01 +35:39:31.5: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:14.01 +35:39:31.5: 14.65 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.21 21:55:25.02 +39:42:15.4
89.86309 -11.60741 galactic Cyg Second-epoch detections are separated by 2.1" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:25.02 +39:42:15.4 (user input) | T | P | (position from user input) J-Ks=0.398+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:25.02 +39:42:15.4: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:25.02 +39:42:15.4: 14.40 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.18 21:35:34.81 +41:02:12.4
87.85101 -8.12647 galactic Cyg Second-epoch detections are separated by 4.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:34.81 +41:02:12.4 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.311+/-0.042 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:34.81 +41:02:12.4: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:34.81 +41:02:12.4: 14.43 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.11 21:40:22.44 +39:00:37.6
87.15476 -10.24205 galactic Cyg Second-epoch detections are separated by 0.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.0801+39.0061 | 21:40:22.44 +39:00:37.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.721+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:22.44 +39:00:37.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:22.44 +39:00:37.6: 14.11 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.0801+39.0061,2461172.8579,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.0801+39.0061 20260512.3579 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.22 22:01:48.31 +39:56:08.6
90.99123 -12.19012 galactic Lac Second-epoch detections are separated by 1.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:01:48.31 +39:56:08.6 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.054 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:48.31 +39:56:08.6: 12.84 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:48.31 +39:56:08.6: 14.27 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.24 21:50:17.67 +42:04:59.5
90.64135 -9.15588 galactic Cyg Second-epoch detections are separated by 3.1" and 2.3 pix
The object was found in VSX17" Gaia DR3 1960632160939763456
Type: RS
# Max. Min./Amp. JD0 Period
18.120 G 18.340 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:17.67 +42:04:59.5: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:17.67 +42:04:59.5: 14.50 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960632160939763456,2461172.8579,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960632160939763456 20260512.3579 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.23 21:31:25.66 +35:04:07.5
83.08236 -11.90013 galactic Cyg Second-epoch detections are separated by 2.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:25.66 +35:04:07.5 (user input) | T | P | (position from user input) J-Ks=0.315+/-0.034 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:25.66 +35:04:07.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:25.66 +35:04:07.5: 14.20 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.98 21:48:34.08 +42:19:14.2
90.54781 -8.76850 galactic Cyg Second-epoch detections are separated by 2.5" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:34.08 +42:19:14.2 (user input) | T | P | (position from user input) J-Ks=0.331+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:34.08 +42:19:14.2: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:34.08 +42:19:14.2: 13.81 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.23 21:29:26.32 +37:55:02.9
84.81010 -9.57764 galactic Cyg Second-epoch detections are separated by 4.3" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.3596+37.9165 | 21:29:26.32 +37:55:02.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:26.32 +37:55:02.9: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:26.32 +37:55:02.9: 14.19 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.3596+37.9165,2461172.8579,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.3596+37.9165 20260512.3579 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.15 21:51:41.33 +39:11:41.9
88.96557 -11.54222 galactic Cyg Second-epoch detections are separated by 1.3" and 2.7 pix
The object was found in VSX24" Gaia DR3 1953335290682076416
Type: ROT
# Max. Min./Amp. JD0 Period
14.110 G 14.150 G 3.239490000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:41.33 +39:11:41.9: 13.41 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:41.33 +39:11:41.9: 14.12 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953335290682076416,2461172.8579,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953335290682076416 20260512.3579 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.22 22:06:06.12 +38:12:56.7
90.59248 -14.06169 galactic Lac Second-epoch detections are separated by 4.1" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1955089458405516032 | 22:06:06.12 +38:12:56.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:06.12 +38:12:56.7: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:06.12 +38:12:56.7: 14.58 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1955089458405516032,2461172.8579,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1955089458405516032 20260512.3579 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.96 21:51:41.89 +34:07:05.8
85.59079 -15.41616 galactic Peg Second-epoch detections are separated by 1.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:41.89 +34:07:05.8 (user input) | T | P | (position from user input) J-Ks=0.576+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:41.89 +34:07:05.8: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:41.89 +34:07:05.8: 14.41 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.10 22:02:38.66 +37:44:29.0
89.73772 -14.02081 galactic Lac Second-epoch detections are separated by 2.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:38.66 +37:44:29.0 (user input) | T | P | (position from user input) J-Ks=0.356+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:38.66 +37:44:29.0: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:38.66 +37:44:29.0: 15.08 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.09 21:36:58.24 +37:51:38.0
85.86577 -10.64136 galactic Cyg Second-epoch detections are separated by 1.2" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.2508+37.8632 | 21:36:58.24 +37:51:38.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.640+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:58.24 +37:51:38.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:58.24 +37:51:38.0: 14.48 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.2508+37.8632,2461172.8579,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.2508+37.8632 20260512.3579 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.04 22:06:54.87 +41:38:25.6
92.83218 -11.41944 galactic Lac Second-epoch detections are separated by 1.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:54.87 +41:38:25.6 (user input) | T | P | (position from user input) J-Ks=0.698+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:54.87 +41:38:25.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:54.87 +41:38:25.6: 14.44 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.05 22:02:56.21 +40:46:06.2
91.68621 -11.66338 galactic Lac Second-epoch detections are separated by 4.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:56.21 +40:46:06.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:56.21 +40:46:06.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:56.21 +40:46:06.2: 14.04 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.96 21:43:44.26 +34:49:10.4
84.79704 -13.80567 galactic Cyg Second-epoch detections are separated by 2.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:44.26 +34:49:10.4 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:44.26 +34:49:10.4: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:44.26 +34:49:10.4: 14.64 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.97 22:07:48.88 +34:48:04.2
88.72298 -16.98297 galactic Peg Second-epoch detections are separated by 2.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:07:48.88 +34:48:04.2 (user input) | T | P | (position from user input) J-Ks=0.686+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:48.88 +34:48:04.2: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:48.88 +34:48:04.2: 14.49 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.97 22:08:33.12 +35:58:49.2
89.59417 -16.13697 galactic Lac Second-epoch detections are separated by 0.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:33.12 +35:58:49.2 (user input) | T | P | (position from user input) J-Ks=0.291+/-0.039 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:33.12 +35:58:49.2: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:33.12 +35:58:49.2: 14.32 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.82 22:10:57.06 +37:02:42.5
90.65913 -15.57423 galactic Lac Second-epoch detections are separated by 1.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:10:57.06 +37:02:42.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:57.06 +37:02:42.5: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:57.06 +37:02:42.5: 14.01 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.02 21:50:25.14 +38:28:30.2
88.29891 -11.93386 galactic Cyg Second-epoch detections are separated by 0.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:25.14 +38:28:30.2 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.539+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:25.14 +38:28:30.2: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:25.14 +38:28:30.2: 13.94 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.02 22:09:56.44 +39:05:40.5
91.75342 -13.80804 galactic Lac Second-epoch detections are separated by 0.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:09:56.44 +39:05:40.5 (user input) | T | P | (position from user input) J-Ks=0.397+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:56.44 +39:05:40.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:56.44 +39:05:40.5: 14.30 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.90 21:44:37.46 +38:02:18.1
87.12812 -11.52083 galactic Cyg Second-epoch detections are separated by 1.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:37.46 +38:02:18.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:37.46 +38:02:18.1: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:37.46 +38:02:18.1: 14.04 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.98 21:57:31.30 +38:48:29.4
89.61020 -12.56022 galactic Cyg Second-epoch detections are separated by 3.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.3824+38.7999 | 21:57:31.30 +38:48:29.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.520+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:31.30 +38:48:29.4: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:31.30 +38:48:29.4: 14.45 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.3824+38.7999,2461172.8579,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.3824+38.7999 20260512.3579 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.14 22:02:38.78 +37:13:44.8
89.41213 -14.42432 galactic Lac Second-epoch detections are separated by 2.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:38.78 +37:13:44.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:38.78 +37:13:44.8: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:38.78 +37:13:44.8: 14.16 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.94 22:09:04.27 +36:22:36.8
89.92997 -15.88390 galactic Lac Second-epoch detections are separated by 1.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:09:04.27 +36:22:36.8 (user input) | T | P | (position from user input) J-Ks=0.651+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:04.27 +36:22:36.8: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:04.27 +36:22:36.8: 14.31 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.76 22:09:49.48 +37:06:45.4
90.51388 -15.38601 galactic Lac Second-epoch detections are separated by 1.0" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:09:49.48 +37:06:45.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:49.48 +37:06:45.4: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:49.48 +37:06:45.4: 14.19 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.88 21:40:15.55 +37:50:21.5
86.33848 -11.09563 galactic Cyg Second-epoch detections are separated by 0.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.0657+37.8384 | 21:40:15.55 +37:50:21.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.793+/-0.051 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:15.55 +37:50:21.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:15.55 +37:50:21.5: 13.70 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.0657+37.8384,2461172.8579,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.0657+37.8384 20260512.3579 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.94 21:45:03.10 +36:40:08.6
86.26655 -12.60357 galactic Cyg Second-epoch detections are separated by 5.6" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:03.10 +36:40:08.6 (user input) | T | P | (position from user input) J-Ks=0.529+/-0.043 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:03.10 +36:40:08.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:03.10 +36:40:08.6: 13.82 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.78 22:07:19.75 +40:15:15.6
92.04909 -12.57734 galactic Lac Second-epoch detections are separated by 1.7" and 2.7 pix
The object was found in VSX22" Gaia DR3 1956579812056615680
Type: VAR
# Max. Min./Amp. JD0 Period
15.280 G 15.440 G 0.014165500000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:19.75 +40:15:15.6: 13.09 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:19.75 +40:15:15.6: 14.03 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956579812056615680,2461172.8579,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956579812056615680 20260512.3579 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.94 21:52:04.60 +34:41:09.5
86.03519 -15.03603 galactic Peg Second-epoch detections are separated by 0.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:04.60 +34:41:09.5 (user input) | T | P | (position from user input) J-Ks=0.783+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:04.60 +34:41:09.5: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:04.60 +34:41:09.5: 14.26 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.96 21:55:46.12 +35:47:06.6
87.36425 -14.68063 galactic Peg Second-epoch detections are separated by 0.7" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:46.12 +35:47:06.6 (user input) | T | P | (position from user input) J-Ks=0.596+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:46.12 +35:47:06.6: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:46.12 +35:47:06.6: 14.28 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.91 22:05:32.42 +38:58:34.1
90.97688 -13.39028 galactic Lac Second-epoch detections are separated by 2.6" and 3.1 pix
The object was found in VSX 4" Gaia DR3 1955944191256830592
Type: ROT
# Max. Min./Amp. JD0 Period
14.100 G 14.150 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:32.42 +38:58:34.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:32.42 +38:58:34.1: 13.93 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955944191256830592,2461172.8579,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955944191256830592 20260512.3579 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.75 21:48:31.26 +41:08:43.0
89.77236 -9.66046 galactic Cyg Second-epoch detections are separated by 2.1" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.1211+41.1406 | 21:48:31.26 +41:08:43.0 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.389+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:31.26 +41:08:43.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:31.26 +41:08:43.0: 13.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.1211+41.1406,2461172.8579,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.1211+41.1406 20260512.3579 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.77 21:53:31.13 +33:46:50.1
85.66065 -15.91823 galactic Peg Second-epoch detections are separated by 2.3" and 3.0 pix
The object was found in VSX17" Gaia DR3 1948095842897373440
Type: E+ROT
# Max. Min./Amp. JD0 Period
15.750 G 15.920 G 1.253330000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:31.13 +33:46:50.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:31.13 +33:46:50.1: 14.15 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948095842897373440,2461172.8579,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948095842897373440 20260512.3579 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.69 21:58:49.48 +40:53:49.1
91.14119 -11.08366 galactic Lac Second-epoch detections are separated by 5.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.7091+40.8974 | 21:58:52.17 +40:53:35.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:49.48 +40:53:49.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:49.48 +40:53:49.1: 13.80 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.7091+40.8974,2461172.8579,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.7091+40.8974 20260512.3579 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.82 21:42:14.31 +37:22:59.4
86.32368 -11.69688 galactic Cyg Second-epoch detections are separated by 2.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:14.31 +37:22:59.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:14.31 +37:22:59.4: 12.29 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:14.31 +37:22:59.4: 14.26 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.77 21:53:53.60 +41:17:52.3
90.65985 -10.18921 galactic Cyg Second-epoch detections are separated by 2.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:53:53.60 +41:17:52.3 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:53.60 +41:17:52.3: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:53.60 +41:17:52.3: 13.81 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.82 21:43:02.43 +34:00:50.1
84.12978 -14.30643 galactic Cyg Second-epoch detections are separated by 1.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1947542582391081344 | 21:43:00.64 +34:00:23.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:02.43 +34:00:50.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:02.43 +34:00:50.1: 13.25 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1947542582391081344,2461172.8579,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947542582391081344 20260512.3579 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.78 22:00:24.41 +39:57:07.7
90.78562 -12.01211 galactic Lac Second-epoch detections are separated by 0.9" and 2.5 pix
The object was found in VSX 6" Gaia DR3 1959243104097280768
Type: ROT
# Max. Min./Amp. JD0 Period
15.910 G 15.960 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:24.41 +39:57:07.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:24.41 +39:57:07.7: 13.81 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959243104097280768,2461172.8579,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959243104097280768 20260512.3579 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.78 21:56:29.02 +37:56:47.0
88.89164 -13.10169 galactic Cyg Second-epoch detections are separated by 1.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.1061+37.9513 | 21:56:29.02 +37:56:47.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.617+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:29.02 +37:56:47.0: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:29.02 +37:56:47.0: 13.68 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1061+37.9513,2461172.8579,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1061+37.9513 20260512.3579 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.74 21:55:57.26 +40:10:25.0
90.24644 -11.30787 galactic Cyg Second-epoch detections are separated by 1.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.9858+40.1754 | 21:55:57.26 +40:10:25.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.373+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:57.26 +40:10:25.0: 13.12 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:57.26 +40:10:25.0: 13.84 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.9858+40.1754,2461172.8579,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.9858+40.1754 20260512.3579 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.76 21:29:16.58 +34:43:05.5
82.50965 -11.84212 galactic Cyg Second-epoch detections are separated by 3.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:16.58 +34:43:05.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:16.58 +34:43:05.5: 11.95 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:16.58 +34:43:05.5: 13.59 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.68 21:44:03.16 +37:47:35.8
86.87625 -11.62989 galactic Cyg Second-epoch detections are separated by 1.9" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:03.16 +37:47:35.8 (user input) | T | P | (position from user input) J-Ks=0.479+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:03.16 +37:47:35.8: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:03.16 +37:47:35.8: 13.57 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.69 21:39:53.76 +37:58:52.8
86.38169 -10.94232 galactic Cyg Second-epoch detections are separated by 2.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1953496811513244032 | 21:39:53.19 +37:58:30.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.542+/-0.097 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:53.76 +37:58:52.8: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:53.76 +37:58:52.8: 13.50 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953496811513244032,2461172.8579,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953496811513244032 20260512.3579 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.65 21:53:17.50 +41:45:59.3
90.87249 -9.75514 galactic Cyg Second-epoch detections are separated by 0.9" and 2.6 pix
The object was found in VSX 4" Gaia DR3 1960367457816371328
Type: ROT
# Max. Min./Amp. JD0 Period
14.130 G 14.170 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:17.50 +41:45:59.3: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:17.50 +41:45:59.3: 13.45 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960367457816371328,2461172.8579,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960367457816371328 20260512.3579 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.81 21:55:39.50 +36:53:22.5
88.07251 -13.81518 galactic Cyg Second-epoch detections are separated by 2.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:39.50 +36:53:22.5 (user input) | T | P | (position from user input) J-Ks=0.641+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:39.50 +36:53:22.5: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:39.50 +36:53:22.5: 13.96 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.57 22:10:45.32 +40:14:53.9
92.58473 -12.97041 galactic Lac Second-epoch detections are separated by 1.7" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:10:45.32 +40:14:53.9 (user input) | T | P | (position from user input) J-Ks=0.703+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:45.32 +40:14:53.9: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:45.32 +40:14:53.9: 13.99 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.52 22:09:47.58 +36:16:45.8
89.98984 -16.04921 galactic Lac Second-epoch detections are separated by 1.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.4409+36.2868 | 22:09:47.21 +36:17:07.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.715+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:47.58 +36:16:45.8: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:47.58 +36:16:45.8: 13.49 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.4409+36.2868,2461172.8579,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.4409+36.2868 20260512.3579 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.53 21:26:12.88 +41:49:13.0
87.11159 -6.34958 galactic Cyg Second-epoch detections are separated by 5.7" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.5536+41.8236 | 21:26:12.88 +41:49:13.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:12.88 +41:49:13.0: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:12.88 +41:49:13.0: 13.64 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.5536+41.8236,2461172.8579,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.5536+41.8236 20260512.3579 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.34 21:40:12.45 +37:22:52.0
86.01668 -11.42796 galactic Cyg Second-epoch detections are separated by 1.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952694649060067840 | 21:40:13.14 +37:22:20.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.354+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:12.45 +37:22:52.0: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:12.45 +37:22:52.0: 13.16 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952694649060067840,2461172.8579,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952694649060067840 20260512.3579 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.39 21:40:43.80 +37:23:00.4
86.09670 -11.49599 galactic Cyg Second-epoch detections are separated by 0.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1759+37.3947 | 21:40:43.80 +37:23:00.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.217+/-0.038 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:43.80 +37:23:00.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:43.80 +37:23:00.4: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1759+37.3947,2461172.8579,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1759+37.3947 20260512.3579 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.35 21:57:14.44 +42:01:04.2
91.61324 -10.02110 galactic Cyg Second-epoch detections are separated by 2.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.3064+42.0125 | 21:57:14.44 +42:01:04.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.753+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:14.44 +42:01:04.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:14.44 +42:01:04.2: 13.41 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.3064+42.0125,2461172.8579,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.3064+42.0125 20260512.3579 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.48 21:30:55.05 +34:30:59.6
82.61161 -12.22255 galactic Cyg Second-epoch detections are separated by 1.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.7144+34.5154 | 21:30:55.05 +34:30:59.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.354+/-0.078 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:55.05 +34:30:59.6: 13.19 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:55.05 +34:30:59.6: 13.35 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.7144+34.5154,2461172.8579,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.7144+34.5154 20260512.3579 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.27 22:02:05.96 +36:06:27.4
88.60463 -15.23701 galactic Peg Second-epoch detections are separated by 4.3" and 3.4 pix
The object was found in VSX18" Gaia DR3 1948807192560317824
Type: ROT
# Max. Min./Amp. JD0 Period
14.030 G 14.060 G 8.170100000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:05.96 +36:06:27.4: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:05.96 +36:06:27.4: 13.23 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948807192560317824,2461172.8579,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948807192560317824 20260512.3579 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.17 21:26:50.52 +37:00:11.8
83.78749 -9.86982 galactic Cyg Second-epoch detections are separated by 4.6" and 2.5 pix
The object was found in VSX 4" Gaia DR3 1963749143269434240
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.840 G 13.860 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:50.52 +37:00:11.8: 12.30 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:50.52 +37:00:11.8: 13.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1963749143269434240,2461172.8579,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963749143269434240 20260512.3579 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.15 22:02:11.35 +35:32:42.6
88.25660 -15.68885 galactic Peg Second-epoch detections are separated by 1.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1948505887717109376 | 22:02:11.25 +35:33:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-0.030 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:11.35 +35:32:42.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:11.35 +35:32:42.6: 13.35 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948505887717109376,2461172.8579,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948505887717109376 20260512.3579 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.95 22:05:39.86 +34:53:39.2
88.41802 -16.63934 galactic Peg Second-epoch detections are separated by 1.6" and 2.7 pix
The object was found in VSX19" Gaia DR3 1900468744392395008
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.160 G 13.190 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:39.86 +34:53:39.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:39.86 +34:53:39.2: 13.22 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1900468744392395008,2461172.8579,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1900468744392395008 20260512.3579 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.87 21:59:59.27 +36:08:34.1
88.28226 -14.94349 galactic Peg Second-epoch detections are separated by 1.8" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.9994+36.1363 | 21:59:59.86 +36:08:10.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:59.27 +36:08:34.1: 12.14 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:59.27 +36:08:34.1: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.9994+36.1363,2461172.8579,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.9994+36.1363 20260512.3579 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.88 21:59:20.92 +36:56:49.6
88.69958 -14.23618 galactic Lac Second-epoch detections are separated by 2.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:20.92 +36:56:49.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.647+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:20.92 +36:56:49.6: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:20.92 +36:56:49.6: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.80 21:44:09.56 +37:55:03.4
86.97645 -11.55072 galactic Cyg Second-epoch detections are separated by 1.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.0405+37.9120 | 21:44:11.54 +37:55:07.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.406+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:09.56 +37:55:03.4: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:09.56 +37:55:03.4: 12.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.0405+37.9120,2461172.8579,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.0405+37.9120 20260512.3579 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.53 21:28:09.20 +41:14:36.6
86.96876 -7.01605 galactic Cyg Second-epoch detections are separated by 1.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.0200+41.2443 | 21:28:07.89 +41:14:23.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.370+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:09.20 +41:14:36.6: 12.20 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:09.20 +41:14:36.6: 12.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0200+41.2443,2461172.8579,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0200+41.2443 20260512.3579 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.76 21:33:13.75 +37:12:43.5
84.86399 -10.60670 galactic Cyg Second-epoch detections are separated by 1.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952077135843691520 | 21:33:13.84 +37:13:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.344+/-0.031 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:13.75 +37:12:43.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:13.75 +37:12:43.5: 12.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952077135843691520,2461172.8579,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952077135843691520 20260512.3579 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.54 21:30:32.04 +35:46:44.8
83.45461 -11.26391 galactic Cyg Second-epoch detections are separated by 0.7" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:32.04 +35:46:44.8 (user input) | T | P | (position from user input) J-Ks=0.719+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:32.04 +35:46:44.8: 12.75 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:32.04 +35:46:44.8: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.53 22:06:01.48 +39:10:17.5
91.17530 -13.29159 galactic Lac Second-epoch detections are separated by 1.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:01.48 +39:10:17.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:01.48 +39:10:17.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:01.48 +39:10:17.5: 12.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.50 21:28:11.90 +34:45:26.3
82.37691 -11.65858 galactic Cyg Second-epoch detections are separated by 0.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:11.90 +34:45:26.3 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:11.90 +34:45:26.3: 10.87 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:11.90 +34:45:26.3: 12.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,10.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 10.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 9.74 21:59:06.37 +34:00:18.2
86.73706 -16.48952 galactic Peg Second-epoch detections are separated by 1.1" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1947975824331378048 | 21:59:07.15 +34:00:38.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.727+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:06.37 +34:00:18.2: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:06.37 +34:00:18.2: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1947975824331378048,2461172.8579,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947975824331378048 20260512.3579 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 9.53 22:01:18.73 +41:30:28.0
91.90005 -10.89118 galactic Lac Second-epoch detections are separated by 1.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959759393525967360 | 22:01:19.91 +41:30:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.219+/-0.030 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:18.73 +41:30:28.0: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:18.73 +41:30:28.0: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959759393525967360,2461172.8579,9.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959759393525967360 20260512.3579 9.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 8.37 22:01:14.46 +38:33:47.2
90.03616 -13.20398 galactic Lac Second-epoch detections are separated by 2.5" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.3181+38.5754 | 22:01:16.11 +38:33:57.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.852+/-0.052 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:14.46 +38:33:47.2: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:14.46 +38:33:47.2: 10.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.13 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.3181+38.5754,2461172.8579,8.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.3181+38.5754 20260512.3579 8.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.54 22:04:54.79 +40:37:24.8
91.90054 -12.00586 galactic Lac Second-epoch detections are separated by 0.7" and 2.7 pix
The object was found in VSX16" Gaia DR3 1956652654701605504
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.420 G 13.470 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:54.79 +40:37:24.8: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:54.79 +40:37:24.8: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956652654701605504,2461172.8579,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956652654701605504 20260512.3579 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.87 22:02:13.89 +41:47:07.9
92.21129 -10.77632 galactic Lac Second-epoch detections are separated by 1.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.5515+41.7805 | 22:02:12.37 +41:46:50.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.975+/-0.036 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:13.89 +41:47:07.9: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:13.89 +41:47:07.9: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.5515+41.7805,2461172.8579,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.5515+41.7805 20260512.3579 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 10.94 21:40:41.03 +36:19:20.7
85.36052 -12.27504 galactic Cyg Second-epoch detections are separated by 0.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1711+36.3226 | 21:40:38.96 +36:19:21.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:41.03 +36:19:20.7: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:41.03 +36:19:20.7: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1711+36.3226,2461172.8579,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1711+36.3226 20260512.3579 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.14 22:02:14.84 +34:37:08.9
87.66561 -16.42037 galactic Peg Second-epoch detections are separated by 0.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.5676+34.6142 | 22:02:14.84 +34:37:08.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.389+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:14.84 +34:37:08.9: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:14.84 +34:37:08.9: 13.59 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.5676+34.6142,2461172.8579,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.5676+34.6142 20260512.3579 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.10 22:02:42.09 +37:09:00.8
89.37077 -14.49316 galactic Lac Second-epoch detections are separated by 1.8" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:42.09 +37:09:00.8 (user input) | T | P | (position from user input) J-Ks=0.360+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:42.09 +37:09:00.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:42.09 +37:09:00.8: 13.58 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.20 22:00:24.20 +35:58:54.0
88.24556 -15.12170 galactic Peg Second-epoch detections are separated by 2.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1948721361934626432 | 22:00:23.05 +35:59:18.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:24.20 +35:58:54.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:24.20 +35:58:54.0: 13.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948721361934626432,2461172.8579,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948721361934626432 20260512.3579 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.18 22:02:42.59 +41:44:10.6
92.25277 -10.86971 galactic Lac Second-epoch detections are separated by 1.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959859277284333312 | 22:02:40.01 +41:44:42.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:42.59 +41:44:10.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:42.59 +41:44:10.6: 13.60 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959859277284333312,2461172.8579,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959859277284333312 20260512.3579 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.41 22:06:31.88 +34:33:33.2
88.34998 -17.01313 galactic Peg Second-epoch detections are separated by 1.0" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:31.88 +34:33:33.2 (user input) | T | P | (position from user input) J-Ks=0.631+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:31.88 +34:33:33.2: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:31.88 +34:33:33.2: 14.31 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.44 21:47:33.64 +37:22:56.1
87.13371 -12.39701 galactic Cyg Second-epoch detections are separated by 0.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:47:33.64 +37:22:56.1 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:33.64 +37:22:56.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:33.64 +37:22:56.1: 13.81 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.40 21:58:18.40 +39:26:01.3
90.13253 -12.16760 galactic Lac Second-epoch detections are separated by 2.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.5793+39.4473 | 21:58:21.67 +39:26:22.2 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.814+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:18.40 +39:26:01.3: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:18.40 +39:26:01.3: 13.94 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.5793+39.4473,2461172.8579,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.5793+39.4473 20260512.3579 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.52 22:02:04.56 +37:45:27.6
89.65695 -13.93869 galactic Lac Second-epoch detections are separated by 1.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:04.56 +37:45:27.6 (user input) | T | P | (position from user input) J-Ks=0.260+/-0.038 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:04.56 +37:45:27.6: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:04.56 +37:45:27.6: 14.36 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.58 22:07:43.40 +37:37:06.9
90.48286 -14.73070 galactic Lac Second-epoch detections are separated by 1.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.9384+37.6117 | 22:07:43.40 +37:37:06.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:43.40 +37:37:06.9: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:43.40 +37:37:06.9: 14.15 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.9384+37.6117,2461172.8579,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.9384+37.6117 20260512.3579 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.63 21:48:57.90 +37:42:53.1
87.57182 -12.32702 galactic Cyg Second-epoch detections are separated by 2.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.2399+37.7077 | 21:48:57.59 +37:42:28.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:57.90 +37:42:53.1: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:57.90 +37:42:53.1: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.2399+37.7077,2461172.8579,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.2399+37.7077 20260512.3579 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.62 21:51:57.54 +37:11:56.1
87.69320 -13.10490 galactic Cyg Second-epoch detections are separated by 0.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949874199877180800 | 21:51:57.22 +37:12:35.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.432+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:57.54 +37:11:56.1: 12.53 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:57.54 +37:11:56.1: 13.80 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949874199877180800,2461172.8579,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949874199877180800 20260512.3579 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.60 21:49:41.28 +37:43:30.9
87.69002 -12.41200 galactic Cyg Second-epoch detections are separated by 2.4" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.4213+37.7226 | 21:49:42.64 +37:43:55.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.682+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:41.28 +37:43:30.9: 12.80 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:41.28 +37:43:30.9: 13.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.4213+37.7226,2461172.8579,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.4213+37.7226 20260512.3579 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.60 22:10:20.04 +38:44:22.5
91.59975 -14.13917 galactic Lac Second-epoch detections are separated by 0.3" and 2.7 pix
The object was found in VSX 4" Gaia DR3 1955512632942240128
Type: ROT
# Max. Min./Amp. JD0 Period
13.880 G 13.920 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:20.04 +38:44:22.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:20.04 +38:44:22.5: 14.35 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955512632942240128,2461172.8579,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955512632942240128 20260512.3579 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.69 22:04:54.72 +35:49:32.8
88.88834 -15.81025 galactic Peg Second-epoch detections are separated by 2.1" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.2245+35.8493 | 22:04:53.90 +35:50:15.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:54.72 +35:49:32.8: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:54.72 +35:49:32.8: 14.07 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.2245+35.8493,2461172.8579,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.2245+35.8493 20260512.3579 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.71 22:09:33.60 +41:54:58.6
93.40424 -11.49006 galactic Lac Second-epoch detections are separated by 1.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:09:33.60 +41:54:58.6 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:33.60 +41:54:58.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:33.60 +41:54:58.6: 14.26 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.57 21:29:32.26 +33:48:21.6
81.89322 -12.52912 galactic Cyg Second-epoch detections are separated by 2.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:32.26 +33:48:21.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:32.26 +33:48:21.6: 11.70 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:32.26 +33:48:21.6: 13.98 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.70 21:38:38.20 +33:58:31.1
83.41119 -13.71603 galactic Cyg Second-epoch detections are separated by 2.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:38:38.20 +33:58:31.1 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:38.20 +33:58:31.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:38.20 +33:58:31.1: 14.04 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.73 22:05:42.75 +35:53:01.4
89.05844 -15.86397 galactic Lac Second-epoch detections are separated by 0.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.4278+35.8836 | 22:05:42.75 +35:53:01.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.451+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:42.75 +35:53:01.4: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:42.75 +35:53:01.4: 14.45 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.4278+35.8836,2461172.8579,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.4278+35.8836 20260512.3579 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.71 22:11:12.63 +37:18:42.5
90.86681 -15.39059 galactic Lac Second-epoch detections are separated by 2.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:12.63 +37:18:42.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:12.63 +37:18:42.5: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:12.63 +37:18:42.5: 14.38 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.72 21:59:28.80 +37:59:47.4
89.39619 -13.43344 galactic Lac Second-epoch detections are separated by 2.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.8746+37.9877 | 21:59:28.80 +37:59:47.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:28.80 +37:59:47.4: 13.63 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:28.80 +37:59:47.4: 14.19 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.8746+37.9877,2461172.8579,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.8746+37.9877 20260512.3579 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.71 22:06:23.67 +41:39:57.7
92.76837 -11.34085 galactic Lac Second-epoch detections are separated by 3.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.5987+41.6659 | 22:06:24.91 +41:40:32.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.311+/-0.043 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:23.67 +41:39:57.7: 13.58 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:23.67 +41:39:57.7: 13.87 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.5987+41.6659,2461172.8579,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.5987+41.6659 20260512.3579 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.70 22:09:11.52 +36:46:06.6
90.19481 -15.58562 galactic Lac Second-epoch detections are separated by 1.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.2936+36.7689 | 22:09:11.52 +36:46:06.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.423+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:11.52 +36:46:06.6: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:11.52 +36:46:06.6: 14.71 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.2936+36.7689,2461172.8579,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.2936+36.7689 20260512.3579 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.76 21:59:01.83 +36:26:59.1
88.32612 -14.58345 galactic Peg Second-epoch detections are separated by 0.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949636430486534272 | 21:59:02.65 +36:26:18.3 (Gaia DR3) | VAR (local) | F (local) | Gaia3var=VARIABLE J-Ks=0.738+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:01.83 +36:26:59.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:01.83 +36:26:59.1: 13.92 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949636430486534272,2461172.8579,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949636430486534272 20260512.3579 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.76 22:06:38.32 +41:43:55.3
92.84588 -11.31523 galactic Lac Second-epoch detections are separated by 2.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:38.32 +41:43:55.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:38.32 +41:43:55.3: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:38.32 +41:43:55.3: 14.35 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.61 21:58:43.07 +42:11:58.0
91.94587 -10.04872 galactic Lac Second-epoch detections are separated by 5.9" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.6664+42.1926 | 21:58:43.07 +42:11:58.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:43.07 +42:11:58.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:43.07 +42:11:58.0: 13.94 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.6664+42.1926,2461172.8579,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.6664+42.1926 20260512.3579 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.72 21:56:29.21 +36:52:35.9
88.19587 -13.93038 galactic Cyg Second-epoch detections are separated by 0.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.1195+36.8762 | 21:56:29.21 +36:52:35.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.385+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:29.21 +36:52:35.9: 12.14 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:29.21 +36:52:35.9: 14.29 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1195+36.8762,2461172.8579,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1195+36.8762 20260512.3579 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.77 22:00:26.18 +37:37:17.9
89.30788 -13.84434 galactic Lac Second-epoch detections are separated by 1.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.1316+37.6258 | 22:00:28.91 +37:37:12.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:26.18 +37:37:17.9: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:26.18 +37:37:17.9: 13.53 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.1316+37.6258,2461172.8579,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.1316+37.6258 20260512.3579 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.72 21:57:23.01 +41:48:54.3
91.50613 -10.19630 galactic Cyg Second-epoch detections are separated by 2.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:23.01 +41:48:54.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:23.01 +41:48:54.3: 12.34 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:23.01 +41:48:54.3: 14.22 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.78 22:01:04.06 +41:04:57.6
91.59743 -11.19877 galactic Lac Second-epoch detections are separated by 1.8" and 2.3 pix
The object was found in VSX 5" Gaia DR3 1959714932024123904
Type: ROT
# Max. Min./Amp. JD0 Period
14.280 G 14.310 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:04.06 +41:04:57.6: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:04.06 +41:04:57.6: 13.92 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959714932024123904,2461172.8579,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959714932024123904 20260512.3579 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.71 21:56:00.49 +37:10:56.8
88.31953 -13.63336 galactic Cyg Second-epoch detections are separated by 1.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:00.49 +37:10:56.8 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:00.49 +37:10:56.8: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:00.49 +37:10:56.8: 14.42 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.73 21:36:48.58 +38:51:42.1
86.53288 -9.88481 galactic Cyg Second-epoch detections are separated by 0.5" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.1997+38.8630 | 21:36:48.58 +38:51:42.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:48.58 +38:51:42.1: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:48.58 +38:51:42.1: 13.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.1997+38.8630,2461172.8579,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.1997+38.8630 20260512.3579 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.77 21:27:10.32 +36:53:17.9
83.75300 -9.99792 galactic Cyg Second-epoch detections are separated by 4.2" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1951737902147573376 | 21:27:12.98 +36:53:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:10.32 +36:53:17.9: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:10.32 +36:53:17.9: 13.98 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951737902147573376,2461172.8579,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951737902147573376 20260512.3579 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.79 21:50:34.31 +37:11:03.4
87.46714 -12.93749 galactic Cyg Second-epoch detections are separated by 2.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:34.31 +37:11:03.4 (user input) | T | P | (position from user input) J-Ks=0.683+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:34.31 +37:11:03.4: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:34.31 +37:11:03.4: 14.52 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.89 22:02:19.99 +34:02:56.0
87.30803 -16.87659 galactic Peg Second-epoch detections are separated by 3.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:19.99 +34:02:56.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:19.99 +34:02:56.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:19.99 +34:02:56.0: 14.32 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.83 22:05:11.32 +41:31:54.9
92.50239 -11.31275 galactic Lac Second-epoch detections are separated by 2.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.2992+41.5224 | 22:05:09.23 +41:31:24.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.597+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:11.32 +41:31:54.9: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:11.32 +41:31:54.9: 14.47 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.2992+41.5224,2461172.8579,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.2992+41.5224 20260512.3579 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.85 21:49:23.30 +36:27:43.5
86.80011 -13.33208 galactic Peg Second-epoch detections are separated by 3.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949440133303961728 | 21:49:24.50 +36:27:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:23.30 +36:27:43.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:23.30 +36:27:43.5: 13.94 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949440133303961728,2461172.8579,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949440133303961728 20260512.3579 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.02 21:48:46.74 +35:26:23.2
86.01569 -14.02449 galactic Cyg Second-epoch detections are separated by 1.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:46.74 +35:26:23.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:46.74 +35:26:23.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:46.74 +35:26:23.2: 14.54 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.80 22:01:12.15 +35:17:06.7
87.92488 -15.76661 galactic Peg Second-epoch detections are separated by 1.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:01:12.15 +35:17:06.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:12.15 +35:17:06.7: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:12.15 +35:17:06.7: 14.21 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.86 21:50:58.71 +36:44:36.8
87.23737 -13.32578 galactic Cyg Second-epoch detections are separated by 1.7" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:58.71 +36:44:36.8 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:58.71 +36:44:36.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:58.71 +36:44:36.8: 14.41 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.95 21:39:40.89 +34:24:59.7
83.88327 -13.54021 galactic Cyg Second-epoch detections are separated by 1.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:40.89 +34:24:59.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:40.89 +34:24:59.7: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:40.89 +34:24:59.7: 14.48 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.80 21:50:58.46 +39:25:04.2
89.00354 -11.28263 galactic Cyg Second-epoch detections are separated by 1.3" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:58.46 +39:25:04.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:58.46 +39:25:04.2: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:58.46 +39:25:04.2: 14.32 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.88 21:57:10.69 +42:10:42.9
91.70565 -9.88809 galactic Cyg Second-epoch detections are separated by 2.7" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:10.69 +42:10:42.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:10.69 +42:10:42.9: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:10.69 +42:10:42.9: 14.30 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.79 21:54:38.63 +36:53:54.3
87.91739 -13.67911 galactic Cyg Second-epoch detections are separated by 2.5" and 2.4 pix
The object was found in VSX 2" Gaia DR3 1949813864175891072
Type: ROT
# Max. Min./Amp. JD0 Period
14.220 G 14.240 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:38.63 +36:53:54.3: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:38.63 +36:53:54.3: 13.72 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949813864175891072,2461172.8579,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949813864175891072 20260512.3579 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.88 21:46:54.19 +39:15:20.8
88.28569 -10.89573 galactic Cyg Second-epoch detections are separated by 0.9" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:46:54.19 +39:15:20.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:54.19 +39:15:20.8: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:54.19 +39:15:20.8: 14.29 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.98 21:46:14.75 +37:25:08.7
86.95692 -12.19775 galactic Cyg Second-epoch detections are separated by 1.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952554912304902528 | 21:46:16.92 +37:24:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.795+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:14.75 +37:25:08.7: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:14.75 +37:25:08.7: 14.23 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952554912304902528,2461172.8579,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952554912304902528 20260512.3579 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.94 21:29:56.13 +35:08:34.3
82.91210 -11.63397 galactic Cyg Second-epoch detections are separated by 1.8" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.4990+35.1416 | 21:29:56.13 +35:08:34.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:56.13 +35:08:34.3: 12.82 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:56.13 +35:08:34.3: 14.74 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.4990+35.1416,2461172.8579,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.4990+35.1416 20260512.3579 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.88 21:42:07.42 +39:04:10.8
87.45210 -10.42473 galactic Cyg Second-epoch detections are separated by 5.2" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5244+39.0636 | 21:42:07.42 +39:04:10.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:07.42 +39:04:10.8: 11.99 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:07.42 +39:04:10.8: 14.17 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5244+39.0636,2461172.8579,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5244+39.0636 20260512.3579 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.07 22:06:12.38 +39:36:05.5
91.47053 -12.96992 galactic Lac Second-epoch detections are separated by 3.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:12.38 +39:36:05.5 (user input) | T | P | (position from user input) J-Ks=0.466+/-0.041 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:12.38 +39:36:05.5: 13.25 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:12.38 +39:36:05.5: 14.77 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.15 21:51:11.60 +37:00:46.2
87.45012 -13.14838 galactic Cyg Second-epoch detections are separated by 4.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949490156780126336 | 21:51:09.14 +37:01:09.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:11.60 +37:00:46.2: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:11.60 +37:00:46.2: 14.34 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949490156780126336,2461172.8579,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949490156780126336 20260512.3579 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.97 21:56:34.45 +37:00:27.0
88.29520 -13.84021 galactic Cyg Second-epoch detections are separated by 3.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949631375305780480 | 21:56:30.58 +37:00:26.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:34.45 +37:00:27.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:34.45 +37:00:27.0: 14.33 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949631375305780480,2461172.8579,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949631375305780480 20260512.3579 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.90 21:48:07.30 +36:02:35.7
86.31983 -13.48163 galactic Cyg Second-epoch detections are separated by 2.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949333446315971968 | 21:48:07.96 +36:02:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.657+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:07.30 +36:02:35.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:07.30 +36:02:35.7: 13.65 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949333446315971968,2461172.8579,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949333446315971968 20260512.3579 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.98 21:57:57.47 +34:05:54.2
86.60741 -16.26633 galactic Peg Second-epoch detections are separated by 0.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1948022278697534208 | 21:57:57.80 +34:06:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.476+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:57.47 +34:05:54.2: 12.93 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:57.47 +34:05:54.2: 14.76 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948022278697534208,2461172.8579,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948022278697534208 20260512.3579 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.99 22:04:30.42 +41:26:44.9
92.34558 -11.30444 galactic Lac Second-epoch detections are separated by 2.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:04:30.42 +41:26:44.9 (user input) | T | P | (position from user input) J-Ks=0.591+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:30.42 +41:26:44.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:30.42 +41:26:44.9: 14.93 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.97 21:42:33.76 +41:45:51.2
89.32613 -8.46246 galactic Cyg Second-epoch detections are separated by 0.8" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:33.76 +41:45:51.2 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:33.76 +41:45:51.2: 13.04 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:33.76 +41:45:51.2: 14.17 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.14 21:50:44.43 +36:27:35.9
87.01090 -13.51064 galactic Peg Second-epoch detections are separated by 3.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949413745022587008 | 21:50:47.19 +36:27:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.606+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:44.43 +36:27:35.9: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:44.43 +36:27:35.9: 14.24 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949413745022587008,2461172.8579,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949413745022587008 20260512.3579 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.02 21:35:27.29 +35:03:48.3
83.68690 -12.47450 galactic Cyg Second-epoch detections are separated by 4.4" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1950544695813049600 | 21:35:29.09 +35:04:22.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:27.29 +35:03:48.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:27.29 +35:03:48.3: 14.61 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950544695813049600,2461172.8579,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950544695813049600 20260512.3579 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.13 22:06:29.23 +39:32:47.9
91.48091 -13.04633 galactic Lac Second-epoch detections are separated by 4.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956338228735784064 | 22:06:32.74 +39:32:33.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.667+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:29.23 +39:32:47.9: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:29.23 +39:32:47.9: 14.62 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956338228735784064,2461172.8579,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956338228735784064 20260512.3579 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.16 21:48:57.14 +34:21:32.4
85.30998 -14.86252 galactic Cyg Second-epoch detections are separated by 3.5" and 2.8 pix
The object was found in VSX 3" ASASSN-V J214856.87+342131.6
Type: ROT
# Max. Min./Amp. JD0 Period
14.710 V 14.830 V 2458390.85000 20.268000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:57.14 +34:21:32.4: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:57.14 +34:21:32.4: 14.83 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214856.87+342131.6,2461172.8579,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214856.87+342131.6 20260512.3579 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.14 22:08:10.51 +39:02:03.1
91.43312 -13.65222 galactic Lac Second-epoch detections are separated by 0.6" and 2.8 pix
The object was found in VSX 6" Gaia DR3 1956262018836200448
Type: ROT
# Max. Min./Amp. JD0 Period
16.600 G 16.710 G 2.137180000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:10.51 +39:02:03.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:10.51 +39:02:03.1: 14.94 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956262018836200448,2461172.8579,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956262018836200448 20260512.3579 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.02 21:50:31.56 +38:39:10.8
88.43265 -11.81150 galactic Cyg Second-epoch detections are separated by 1.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:31.56 +38:39:10.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.422+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:31.56 +38:39:10.8: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:31.56 +38:39:10.8: 14.65 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.99 21:27:00.73 +33:45:03.0
81.47284 -12.19771 galactic Cyg Second-epoch detections are separated by 3.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.7555+33.7505 | 21:27:00.73 +33:45:03.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.381+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:00.73 +33:45:03.0: 12.57 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:00.73 +33:45:03.0: 14.55 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.7555+33.7505,2461172.8579,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.7555+33.7505 20260512.3579 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.99 21:27:07.35 +35:14:57.5
82.57139 -11.15434 galactic Cyg Second-epoch detections are separated by 5.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:27:07.35 +35:14:57.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:07.35 +35:14:57.5: 12.52 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:07.35 +35:14:57.5: 14.26 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.06 21:55:36.26 +35:51:33.8
87.38671 -14.60223 galactic Peg Second-epoch detections are separated by 2.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949126222734750080 | 21:55:33.00 +35:51:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.364+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:36.26 +35:51:33.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:36.26 +35:51:33.8: 14.51 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949126222734750080,2461172.8579,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949126222734750080 20260512.3579 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.20 21:42:31.24 +35:51:14.2
85.31966 -12.87134 galactic Cyg Second-epoch detections are separated by 2.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.6327+35.8537 | 21:42:31.24 +35:51:14.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:31.24 +35:51:14.2: 13.42 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:31.24 +35:51:14.2: 14.65 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.6327+35.8537,2461172.8579,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.6327+35.8537 20260512.3579 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.16 21:31:26.82 +33:46:07.4
82.15633 -12.83389 galactic Cyg Second-epoch detections are separated by 3.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:26.82 +33:46:07.4 (user input) | T | P | (position from user input) J-Ks=0.678+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:26.82 +33:46:07.4: 13.28 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:26.82 +33:46:07.4: 14.48 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.21 21:35:34.11 +34:35:52.7
83.37596 -12.82824 galactic Cyg Second-epoch detections are separated by 1.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:34.11 +34:35:52.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:34.11 +34:35:52.7: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:34.11 +34:35:52.7: 14.70 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.09 21:42:10.93 +39:16:11.0
87.59597 -10.28288 galactic Cyg Second-epoch detections are separated by 1.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1953715648687912064 | 21:42:11.55 +39:16:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.752+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:10.93 +39:16:11.0: 12.35 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:10.93 +39:16:11.0: 14.65 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953715648687912064,2461172.8579,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953715648687912064 20260512.3579 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.10 21:28:43.61 +35:11:03.8
82.76206 -11.43115 galactic Cyg Second-epoch detections are separated by 2.4" and 2.5 pix
The object was found in VSX 2" Gaia DR3 1951299235669161728
Type: ROT
# Max. Min./Amp. JD0 Period
14.400 G 14.440 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:43.61 +35:11:03.8: 13.25 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:43.61 +35:11:03.8: 14.40 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951299235669161728,2461172.8579,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951299235669161728 20260512.3579 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.08 21:28:15.22 +35:43:26.1
83.07851 -10.97947 galactic Cyg Second-epoch detections are separated by 3.4" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:15.22 +35:43:26.1 (user input) | T | P | (position from user input) J-Ks=0.487+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:15.22 +35:43:26.1: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:15.22 +35:43:26.1: 14.83 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.09 21:27:17.53 +34:59:18.0
82.40864 -11.36371 galactic Cyg Second-epoch detections are separated by 7.8" and 1.2 pix
The object was found in VSX 4" Gaia DR3 1951270579646729984
Type: ROT
# Max. Min./Amp. JD0 Period
14.690 G 14.720 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:17.53 +34:59:18.0: 12.66 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:17.53 +34:59:18.0: 14.40 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951270579646729984,2461172.8579,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951270579646729984 20260512.3579 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 11.99 21:58:19.49 +37:12:23.5
88.70348 -13.90605 galactic Lac Second-epoch detections are separated by 1.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949722261114407552 | 21:58:19.27 +37:12:00.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.343+/-0.049 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:19.49 +37:12:23.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:19.49 +37:12:23.5: 14.08 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949722261114407552,2461172.8579,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949722261114407552 20260512.3579 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.22 21:58:15.44 +33:46:39.2
86.44440 -16.55328 galactic Peg Second-epoch detections are separated by 0.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:15.44 +33:46:39.2 (user input) | T | P | (position from user input) J-Ks=0.441+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:15.44 +33:46:39.2: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:15.44 +33:46:39.2: 14.83 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.05 21:58:36.19 +41:09:24.0
91.27191 -10.85406 galactic Lac Second-epoch detections are separated by 1.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:36.19 +41:09:24.0 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:36.19 +41:09:24.0: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:36.19 +41:09:24.0: 14.77 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.02 21:31:29.58 +33:55:40.3
82.27740 -12.72676 galactic Cyg Second-epoch detections are separated by 2.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:29.58 +33:55:40.3 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:29.58 +33:55:40.3: 12.87 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:29.58 +33:55:40.3: 14.46 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.24 22:02:22.56 +41:34:47.3
92.10534 -10.95583 galactic Lac Second-epoch detections are separated by 0.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:22.56 +41:34:47.3 (user input) | T | P | (position from user input) J-Ks=0.752+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:22.56 +41:34:47.3: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:22.56 +41:34:47.3: 14.83 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.03 21:33:06.86 +34:09:51.6
82.69334 -12.79118 galactic Cyg Second-epoch detections are separated by 2.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:33:06.86 +34:09:51.6 (user input) | T | P | (position from user input) J-Ks=0.835+/-0.027 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:06.86 +34:09:51.6: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:06.86 +34:09:51.6: 14.96 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.22 21:37:58.70 +36:42:06.9
85.21357 -11.62783 galactic Cyg Second-epoch detections are separated by 2.9" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1951148426473260544 | 21:37:56.76 +36:42:19.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.544+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:58.70 +36:42:06.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:58.70 +36:42:06.9: 14.02 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951148426473260544,2461172.8579,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951148426473260544 20260512.3579 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.13 21:30:18.12 +34:13:06.9
82.30533 -12.34650 galactic Cyg Second-epoch detections are separated by 1.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.5813+34.2012 | 21:30:18.95 +34:12:23.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.297+/-0.036 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:18.12 +34:13:06.9: 12.86 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:18.12 +34:13:06.9: 14.54 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.5813+34.2012,2461172.8579,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.5813+34.2012 20260512.3579 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.32 21:51:16.57 +41:52:19.3
90.64663 -9.43489 galactic Cyg Second-epoch detections are separated by 3.2" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:16.57 +41:52:19.3 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.051 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:16.57 +41:52:19.3: 13.33 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:16.57 +41:52:19.3: 15.12 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.33 22:03:08.32 +41:49:51.3
92.37598 -10.84316 galactic Lac Second-epoch detections are separated by 1.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.7848+41.8332 | 22:03:08.32 +41:49:51.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.483+/-0.054 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:08.32 +41:49:51.3: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:08.32 +41:49:51.3: 15.20 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.20 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.7848+41.8332,2461172.8579,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.7848+41.8332 20260512.3579 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.13 22:07:22.82 +40:35:20.9
92.26218 -12.31486 galactic Lac Second-epoch detections are separated by 1.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:07:22.82 +40:35:20.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:22.82 +40:35:20.9: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:22.82 +40:35:20.9: 15.02 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.27 21:49:05.09 +37:22:34.0
87.36441 -12.59947 galactic Cyg Second-epoch detections are separated by 2.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:05.09 +37:22:34.0 (user input) | T | P | (position from user input) J-Ks=0.446+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:05.09 +37:22:34.0: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:05.09 +37:22:34.0: 14.69 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.15 22:00:11.35 +39:37:39.9
90.54686 -12.24120 galactic Lac Second-epoch detections are separated by 1.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:11.35 +39:37:39.9 (user input) | T | P | (position from user input) J-Ks=1.010+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:11.35 +39:37:39.9: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:11.35 +39:37:39.9: 14.85 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.19 21:52:15.38 +41:18:17.8
90.42308 -9.98863 galactic Cyg Second-epoch detections are separated by 2.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:15.38 +41:18:17.8 (user input) | T | P | (position from user input) J-Ks=0.455+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:15.38 +41:18:17.8: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:15.38 +41:18:17.8: 14.61 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.14 21:26:47.03 +37:17:35.4
83.98602 -9.65560 galactic Cyg Second-epoch detections are separated by 4.0" and 2.9 pix
The object was not found in VSX
The object was found in ASASSN-V 4" ASASSN-V J212647.19+371739.0
Type: EW
MeanMag 14.66 m Amp. 0.09 m Period 0.379175 d
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:47.03 +37:17:35.4: 13.18 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:47.03 +37:17:35.4: 14.60 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461172.8579,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260512.3579 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.32 21:35:46.59 +36:12:51.7
84.54345 -11.68241 galactic Cyg Second-epoch detections are separated by 5.4" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.9437+36.2099 | 21:35:46.59 +36:12:51.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:46.59 +36:12:51.7: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:46.59 +36:12:51.7: 14.52 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.9437+36.2099,2461172.8579,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.9437+36.2099 20260512.3579 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.23 22:00:10.35 +38:33:14.2
89.86196 -13.08176 galactic Lac Second-epoch detections are separated by 1.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:10.35 +38:33:14.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.413+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:10.35 +38:33:14.2: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:10.35 +38:33:14.2: 14.88 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.15 21:55:49.63 +34:16:14.3
86.36929 -15.85224 galactic Peg Second-epoch detections are separated by 1.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:49.63 +34:16:14.3 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:49.63 +34:16:14.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:49.63 +34:16:14.3: 14.77 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.22 21:36:08.46 +35:55:08.9
84.39172 -11.94797 galactic Cyg Second-epoch detections are separated by 2.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:08.46 +35:55:08.9 (user input) | T | P | (position from user input) J-Ks=0.537+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:08.46 +35:55:08.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:08.46 +35:55:08.9: 14.29 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.19 21:27:06.44 +33:44:11.4
81.47673 -12.22184 galactic Cyg Second-epoch detections are separated by 1.2" and 2.5 pix
The object was found in VSX 5" Gaia DR3 1854317224858662912
Type: ROT
# Max. Min./Amp. JD0 Period
15.320 G 15.350 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:06.44 +33:44:11.4: 12.59 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:06.44 +33:44:11.4: 14.67 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1854317224858662912,2461172.8579,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1854317224858662912 20260512.3579 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.14 21:57:33.35 +41:16:30.9
91.18994 -10.63873 galactic Cyg Second-epoch detections are separated by 1.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.3632+41.2762 | 21:57:29.83 +41:16:51.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:33.35 +41:16:30.9: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:33.35 +41:16:30.9: 14.53 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.3632+41.2762,2461172.8579,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.3632+41.2762 20260512.3579 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.18 21:43:05.94 +37:32:43.6
86.56412 -11.68979 galactic Cyg Second-epoch detections are separated by 2.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:05.94 +37:32:43.6 (user input) | T | P | (position from user input) J-Ks=0.764+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:05.94 +37:32:43.6: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:05.94 +37:32:43.6: 14.81 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.15 21:53:14.90 +36:41:34.9
87.56120 -13.65789 galactic Cyg Second-epoch detections are separated by 2.8" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.3156+36.6914 | 21:53:15.90 +36:42:09.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5) J-Ks=0.381+/-0.049 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:14.90 +36:41:34.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:14.90 +36:41:34.9: 14.66 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.3156+36.6914,2461172.8579,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.3156+36.6914 20260512.3579 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.15 21:29:18.02 +33:38:42.9
81.74141 -12.60862 galactic Cyg Second-epoch detections are separated by 2.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:18.02 +33:38:42.9 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.703+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:18.02 +33:38:42.9: 12.29 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:18.02 +33:38:42.9: 14.33 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.30 21:45:58.86 +39:55:48.1
88.59757 -10.26948 galactic Cyg Second-epoch detections are separated by 2.7" and 2.8 pix
The object was found in VSX 0" Gaia DR3 1954120926101711872
Type: ROT
# Max. Min./Amp. JD0 Period
14.530 G 14.550 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:58.86 +39:55:48.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:58.86 +39:55:48.1: 14.77 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1954120926101711872,2461172.8579,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1954120926101711872 20260512.3579 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.17 21:30:09.31 +35:59:14.0
83.54658 -11.06128 galactic Cyg Second-epoch detections are separated by 2.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:09.31 +35:59:14.0 (user input) | T | P | (position from user input) J-Ks=0.848+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:09.31 +35:59:14.0: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:09.31 +35:59:14.0: 14.70 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.06 21:33:16.35 +41:46:52.0
88.04209 -7.28660 galactic Cyg Second-epoch detections are separated by 5.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.3240+41.7774 | 21:33:16.35 +41:46:52.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:16.35 +41:46:52.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:16.35 +41:46:52.0: 14.35 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.3240+41.7774,2461172.8579,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.3240+41.7774 20260512.3579 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.15 22:06:09.36 +39:56:12.9
91.66990 -12.69644 galactic Lac Second-epoch detections are separated by 2.7" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956569401055456768 | 22:06:08.01 +39:56:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.517+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:09.36 +39:56:12.9: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:09.36 +39:56:12.9: 14.26 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956569401055456768,2461172.8579,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956569401055456768 20260512.3579 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.10 21:49:33.44 +39:24:22.7
88.78270 -11.11496 galactic Cyg Second-epoch detections are separated by 2.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:33.44 +39:24:22.7 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:33.44 +39:24:22.7: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:33.44 +39:24:22.7: 14.47 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.13 22:09:09.62 +38:13:27.4
91.09271 -14.41637 galactic Lac Second-epoch detections are separated by 4.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1955428726456072960 | 22:09:13.45 +38:13:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:09.62 +38:13:27.4: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:09.62 +38:13:27.4: 14.31 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955428726456072960,2461172.8579,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955428726456072960 20260512.3579 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.39 21:44:26.00 +38:03:30.2
87.11285 -11.48094 galactic Cyg Second-epoch detections are separated by 1.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952820238205138560 | 21:44:26.49 +38:04:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.363+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:26.00 +38:03:30.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:26.00 +38:03:30.2: 14.68 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952820238205138560,2461172.8579,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952820238205138560 20260512.3579 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.21 21:55:15.58 +37:52:02.2
88.64842 -13.00999 galactic Cyg Second-epoch detections are separated by 4.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1950001708865080960 | 21:55:16.23 +37:52:43.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.412+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:15.58 +37:52:02.2: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:15.58 +37:52:02.2: 14.65 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950001708865080960,2461172.8579,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950001708865080960 20260512.3579 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.31 22:07:19.28 +35:59:01.1
89.39018 -15.98345 galactic Lac Second-epoch detections are separated by 1.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:07:19.28 +35:59:01.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:19.28 +35:59:01.1: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:19.28 +35:59:01.1: 14.76 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.32 21:59:53.99 +34:16:51.1
87.05157 -16.37981 galactic Peg Second-epoch detections are separated by 2.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:53.99 +34:16:51.1 (user input) | T | P | (position from user input) J-Ks=0.389+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:53.99 +34:16:51.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:53.99 +34:16:51.1: 15.13 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.32 22:10:22.57 +40:43:10.2
92.80967 -12.54721 galactic Lac Second-epoch detections are separated by 0.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:10:22.57 +40:43:10.2 (user input) | T | P | (position from user input) J-Ks=0.627+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:22.57 +40:43:10.2: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:22.57 +40:43:10.2: 15.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.29 21:50:35.53 +37:36:20.2
87.75013 -12.61910 galactic Cyg Second-epoch detections are separated by 1.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:35.53 +37:36:20.2 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:35.53 +37:36:20.2: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:35.53 +37:36:20.2: 14.85 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.26 21:42:09.63 +36:32:21.6
85.73486 -12.31380 galactic Cyg Second-epoch detections are separated by 0.9" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952593631429313920 | 21:42:07.48 +36:32:40.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.377+/-0.051 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:09.63 +36:32:21.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:09.63 +36:32:21.6: 14.58 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952593631429313920,2461172.8579,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952593631429313920 20260512.3579 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.37 22:07:10.81 +38:37:35.0
91.02150 -13.86200 galactic Lac Second-epoch detections are separated by 1.3" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:07:10.81 +38:37:35.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.497+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:10.81 +38:37:35.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:10.81 +38:37:35.0: 14.93 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.17 21:54:17.27 +36:52:14.7
87.84284 -13.65490 galactic Cyg Second-epoch detections are separated by 1.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949793420131211520 | 21:54:15.63 +36:52:54.0 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.350+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:17.27 +36:52:14.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:17.27 +36:52:14.7: 14.58 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949793420131211520,2461172.8579,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949793420131211520 20260512.3579 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 22:09:48.87 +37:29:08.6
90.74341 -15.08573 galactic Lac Second-epoch detections are separated by 2.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:09:48.87 +37:29:08.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.688+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:48.87 +37:29:08.6: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:48.87 +37:29:08.6: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.26 21:35:30.92 +33:55:27.4
82.89108 -13.30876 galactic Cyg Second-epoch detections are separated by 1.0" and 2.6 pix
The object was found in VSX 2" Gaia DR3 1950223427957054848
Type: ROT
# Max. Min./Amp. JD0 Period
14.490 G 14.510 G 12.727600000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:30.92 +33:55:27.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:30.92 +33:55:27.4: 14.80 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950223427957054848,2461172.8579,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950223427957054848 20260512.3579 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.29 21:40:12.88 +34:16:56.2
83.87252 -13.71353 galactic Cyg Second-epoch detections are separated by 1.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:12.88 +34:16:56.2 (user input) | T | P | (position from user input) J-Ks=0.283+/-0.040 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:12.88 +34:16:56.2: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:12.88 +34:16:56.2: 14.74 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.23 21:52:15.51 +41:52:18.1
90.78932 -9.55167 galactic Cyg Second-epoch detections are separated by 1.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:15.51 +41:52:18.1 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:15.51 +41:52:18.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:15.51 +41:52:18.1: 14.73 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.73 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.18 21:47:59.25 +38:52:24.5
88.19407 -11.32279 galactic Cyg Second-epoch detections are separated by 3.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.0041+38.8701 | 21:47:59.25 +38:52:24.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.539+/-0.039 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:59.25 +38:52:24.5: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:59.25 +38:52:24.5: 14.71 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.0041+38.8701,2461172.8579,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.0041+38.8701 20260512.3579 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.18 21:36:58.81 +34:31:60.0
83.54707 -13.07487 galactic Cyg Second-epoch detections are separated by 2.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:58.81 +34:31:60.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.436+/-0.054 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:58.81 +34:31:60.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:58.81 +34:31:60.0: 14.71 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.26 21:58:49.50 +40:28:43.6
90.87661 -11.41161 galactic Lac Second-epoch detections are separated by 2.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:49.50 +40:28:43.6 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:49.50 +40:28:43.6: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:49.50 +40:28:43.6: 14.98 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.15 21:26:55.40 +38:03:54.9
84.55569 -9.12551 galactic Cyg Second-epoch detections are separated by 0.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1964230213966061824 | 21:26:54.89 +38:03:17.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:55.40 +38:03:54.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:55.40 +38:03:54.9: 14.51 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1964230213966061824,2461172.8579,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1964230213966061824 20260512.3579 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.32 21:41:28.54 +34:59:55.2
84.56748 -13.36143 galactic Cyg Second-epoch detections are separated by 0.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:28.54 +34:59:55.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.698+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:28.54 +34:59:55.2: 13.10 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:28.54 +34:59:55.2: 15.34 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.38 21:43:18.88 +42:12:56.5
89.73312 -8.21507 galactic Cyg Second-epoch detections are separated by 5.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:18.88 +42:12:56.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:18.88 +42:12:56.5: 12.95 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:18.88 +42:12:56.5: 14.64 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.30 21:38:19.66 +39:47:36.5
87.39106 -9.39636 galactic Cyg Second-epoch detections are separated by 1.2" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.5932+39.7857 | 21:38:19.66 +39:47:36.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.400+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:19.66 +39:47:36.5: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:19.66 +39:47:36.5: 14.89 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.5932+39.7857,2461172.8579,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.5932+39.7857 20260512.3579 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.31 21:35:04.40 +35:48:31.4
84.15345 -11.87991 galactic Cyg Second-epoch detections are separated by 0.7" and 2.5 pix
The object was found in VSX 1" Gaia DR3 1951001749052505088
Type: ROT
# Max. Min./Amp. JD0 Period
14.450 G 14.490 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:04.40 +35:48:31.4: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:04.40 +35:48:31.4: 14.59 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951001749052505088,2461172.8579,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951001749052505088 20260512.3579 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.23 21:36:20.55 +34:21:42.7
83.32808 -13.10934 galactic Cyg Second-epoch detections are separated by 2.8" and 2.5 pix
The object was found in VSX 4" Gaia DR3 1950309503404606080
Type: ROT
# Max. Min./Amp. JD0 Period
14.860 G 14.900 G 4.366990000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:20.55 +34:21:42.7: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:20.55 +34:21:42.7: 14.48 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950309503404606080,2461172.8579,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950309503404606080 20260512.3579 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.31 22:08:34.53 +37:33:23.8
90.58374 -14.88179 galactic Lac Second-epoch detections are separated by 0.9" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:34.53 +37:33:23.8 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:34.53 +37:33:23.8: 13.49 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:34.53 +37:33:23.8: 15.43 +/- 0.35 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.31 21:32:07.92 +37:19:43.0
84.78515 -10.37172 galactic Cyg Second-epoch detections are separated by 5.5" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:32:07.92 +37:19:43.0 (user input) | T | P | (position from user input) J-Ks=0.576+/-0.114 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:07.92 +37:19:43.0: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:07.92 +37:19:43.0: 14.66 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.27 22:00:30.51 +41:08:38.3
91.55117 -11.08568 galactic Lac Second-epoch detections are separated by 1.9" and 2.3 pix
The object was found in VSX 3" Gaia DR3 1959727232810436608
Type: ROT
# Max. Min./Amp. JD0 Period
15.060 G 15.090 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:30.51 +41:08:38.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:30.51 +41:08:38.3: 14.84 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959727232810436608,2461172.8579,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959727232810436608 20260512.3579 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:32:41.23 +35:18:26.0
83.44084 -11.90760 galactic Cyg Second-epoch detections are separated by 0.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.1712+35.3046 | 21:32:41.23 +35:18:26.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.753+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:41.23 +35:18:26.0: 12.97 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:41.23 +35:18:26.0: 15.20 +/- 0.29 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.1712+35.3046,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.1712+35.3046 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.21 21:32:35.87 +35:36:11.1
83.63702 -11.68180 galactic Cyg Second-epoch detections are separated by 2.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.1465+35.6027 | 21:32:35.87 +35:36:11.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:35.87 +35:36:11.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:35.87 +35:36:11.1: 14.75 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.1465+35.6027,2461172.8579,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.1465+35.6027 20260512.3579 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.33 22:05:26.20 +37:35:45.0
90.09632 -14.47437 galactic Lac Second-epoch detections are separated by 2.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:05:26.20 +37:35:45.0 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.054 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:26.20 +37:35:45.0: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:26.20 +37:35:45.0: 14.90 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.42 21:57:52.74 +34:06:47.3
86.60408 -16.24457 galactic Peg Second-epoch detections are separated by 2.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:52.74 +34:06:47.3 (user input) | T | P | (position from user input) J-Ks=0.389+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:52.74 +34:06:47.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:52.74 +34:06:47.3: 15.35 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.21 22:05:26.98 +41:32:29.9
92.54814 -11.33438 galactic Lac Second-epoch detections are separated by 2.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:05:26.98 +41:32:29.9 (user input) | T | P | (position from user input) J-Ks=0.282+/-0.109 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:26.98 +41:32:29.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:26.98 +41:32:29.9: 15.11 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.35 21:29:44.30 +35:02:50.1
82.81434 -11.67399 galactic Cyg Second-epoch detections are separated by 2.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1951246871423742464 | 21:29:44.30 +35:02:50.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.459+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:44.30 +35:02:50.1: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:44.30 +35:02:50.1: 15.18 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.18 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1951246871423742464,2461172.8579,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1951246871423742464 20260512.3579 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.23 21:52:19.85 +34:09:35.2
85.72190 -15.46993 galactic Peg Second-epoch detections are separated by 2.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:19.85 +34:09:35.2 (user input) | T | P | (position from user input) J-Ks=0.641+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:19.85 +34:09:35.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:19.85 +34:09:35.2: 14.63 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.38 21:56:45.73 +40:47:17.4
90.76131 -10.92572 galactic Cyg Second-epoch detections are separated by 2.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.1810+40.7921 | 21:56:45.73 +40:47:17.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.531+/-0.059 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:45.73 +40:47:17.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:45.73 +40:47:17.4: 14.94 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1810+40.7921,2461172.8579,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1810+40.7921 20260512.3579 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.30 21:58:48.24 +40:45:29.0
91.05022 -11.19018 galactic Lac Second-epoch detections are separated by 2.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959343125295495168 | 21:58:45.44 +40:45:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.410+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:48.24 +40:45:29.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:48.24 +40:45:29.0: 15.26 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959343125295495168,2461172.8579,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959343125295495168 20260512.3579 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.28 22:08:35.89 +37:44:55.1
90.70672 -14.73093 galactic Lac Second-epoch detections are separated by 1.9" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:35.89 +37:44:55.1 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:35.89 +37:44:55.1: 13.28 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:35.89 +37:44:55.1: 15.45 +/- 0.34 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.46 21:43:45.89 +35:25:54.1
85.22244 -13.35427 galactic Cyg Second-epoch detections are separated by 1.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:45.89 +35:25:54.1 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:45.89 +35:25:54.1: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:45.89 +35:25:54.1: 15.31 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.19 21:57:39.52 +41:25:20.8
91.29855 -10.53558 galactic Lac Second-epoch detections are separated by 1.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:39.52 +41:25:20.8 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:39.52 +41:25:20.8: 12.77 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:39.52 +41:25:20.8: 14.81 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.36 21:43:07.95 +37:05:02.1
86.25512 -12.03852 galactic Cyg Second-epoch detections are separated by 2.5" and 2.2 pix
The object was found in VSX 2" Gaia DR3 1952645484575159040
Type: ROT
# Max. Min./Amp. JD0 Period
15.120 G 15.150 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:07.95 +37:05:02.1: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:07.95 +37:05:02.1: 15.05 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952645484575159040,2461172.8579,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952645484575159040 20260512.3579 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.24 22:04:46.12 +42:08:02.3
92.80817 -10.78500 galactic Lac Second-epoch detections are separated by 2.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.1918+42.1233 | 22:04:46.12 +42:08:02.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.843+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:46.12 +42:08:02.3: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:46.12 +42:08:02.3: 14.34 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.1918+42.1233,2461172.8579,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.1918+42.1233 20260512.3579 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.19 21:44:35.13 +34:15:55.6
84.54862 -14.33430 galactic Cyg Second-epoch detections are separated by 2.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:35.13 +34:15:55.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:35.13 +34:15:55.6: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:35.13 +34:15:55.6: 14.67 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.67 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.30 21:51:49.79 +37:26:02.0
87.82850 -12.90870 galactic Cyg Second-epoch detections are separated by 2.2" and 2.5 pix
The object was found in VSX20" STSP J215151.42+372556.3
Type: EA
# Max. Min./Amp. JD0 Period
17.490 r 17.910 r 2458714.80500 5.787900000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:49.79 +37:26:02.0: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:49.79 +37:26:02.0: 14.95 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
STSP J215151.42+372556.3,2461172.8579,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
STSP J215151.42+372556.3 20260512.3579 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.23 21:41:03.69 +37:41:57.4
86.36254 -11.30584 galactic Cyg Second-epoch detections are separated by 2.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:03.69 +37:41:57.4 (user input) | T | P | (position from user input) J-Ks=0.773+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:03.69 +37:41:57.4: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:03.69 +37:41:57.4: 14.01 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.31 21:55:34.88 +36:37:37.0
87.88806 -14.00796 galactic Cyg Second-epoch detections are separated by 4.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949618941381943168 | 21:55:33.24 +36:38:09.4 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE J-Ks=0.324+/-0.046 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:34.88 +36:37:37.0: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:34.88 +36:37:37.0: 14.92 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949618941381943168,2461172.8579,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949618941381943168 20260512.3579 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.42 21:56:14.98 +41:22:12.1
91.05537 -10.41153 galactic Cyg Second-epoch detections are separated by 1.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:14.98 +41:22:12.1 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:14.98 +41:22:12.1: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:14.98 +41:22:12.1: 15.09 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.19 21:36:23.98 +37:34:32.5
85.58431 -10.77331 galactic Cyg Second-epoch detections are separated by 1.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:23.98 +37:34:32.5 (user input) | T | P | (position from user input) J-Ks=0.762+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:23.98 +37:34:32.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:23.98 +37:34:32.5: 14.42 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.30 21:26:51.55 +34:03:09.1
81.66855 -11.96232 galactic Cyg Second-epoch detections are separated by 2.2" and 2.8 pix
The object was found in VSX24" Gaia DR3 1855099733538948736
Type: ROT
# Max. Min./Amp. JD0 Period
16.960 G 17.080 G 0.491688000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:51.55 +34:03:09.1: 13.07 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:51.55 +34:03:09.1: 14.66 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1855099733538948736,2461172.8579,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1855099733538948736 20260512.3579 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.22 21:59:43.45 +35:08:54.3
87.59148 -15.68362 galactic Peg Second-epoch detections are separated by 0.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:43.45 +35:08:54.3 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:43.45 +35:08:54.3: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:43.45 +35:08:54.3: 14.85 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.30 21:54:32.73 +35:25:33.6
86.92902 -14.79744 galactic Peg Second-epoch detections are separated by 1.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:32.73 +35:25:33.6 (user input) | T | P | (position from user input) J-Ks=0.681+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:32.73 +35:25:33.6: 13.32 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:32.73 +35:25:33.6: 15.04 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.27 21:35:30.25 +38:08:37.0
85.84661 -10.23735 galactic Cyg Second-epoch detections are separated by 2.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.8631+38.1437 | 21:35:30.25 +38:08:37.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.586+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:30.25 +38:08:37.0: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:30.25 +38:08:37.0: 14.59 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.8631+38.1437,2461172.8579,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.8631+38.1437 20260512.3579 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.21 21:27:08.93 +35:52:28.6
83.02437 -10.71477 galactic Cyg Second-epoch detections are separated by 4.8" and 3.3 pix
The object was found in VSX 1" Gaia DR3 1951530717225138816
Type: ROT
# Max. Min./Amp. JD0 Period
14.560 G 14.590 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:08.93 +35:52:28.6: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:08.93 +35:52:28.6: 14.37 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951530717225138816,2461172.8579,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951530717225138816 20260512.3579 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.34 22:08:40.10 +38:50:08.0
91.38991 -13.86877 galactic Lac Second-epoch detections are separated by 0.4" and 2.8 pix
The object was found in VSX 2" Gaia DR3 1955508063096780544
Type: RS
# Max. Min./Amp. JD0 Period
14.480 G 14.530 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:40.10 +38:50:08.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:40.10 +38:50:08.0: 15.47 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.47 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955508063096780544,2461172.8579,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955508063096780544 20260512.3579 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.26 22:08:30.73 +37:04:05.1
90.26909 -15.26455 galactic Lac Second-epoch detections are separated by 3.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:30.73 +37:04:05.1 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:30.73 +37:04:05.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:30.73 +37:04:05.1: 14.79 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.42 21:29:09.49 +34:06:49.0
82.05747 -12.25511 galactic Cyg Second-epoch detections are separated by 1.4" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:09.49 +34:06:49.0 (user input) | T | P | (position from user input) J-Ks=0.573+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:09.49 +34:06:49.0: 13.04 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:09.49 +34:06:49.0: 14.82 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:58:43.76 +39:44:50.6
90.39760 -11.97307 galactic Lac Second-epoch detections are separated by 2.9" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.6842+39.7459 | 21:58:43.76 +39:44:50.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.402+/-0.056 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:43.76 +39:44:50.6: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:43.76 +39:44:50.6: 14.83 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.6842+39.7459,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.6842+39.7459 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.34 21:40:43.39 +37:37:29.1
86.26092 -11.31622 galactic Cyg Second-epoch detections are separated by 0.3" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:43.39 +37:37:29.1 (user input) | T | P | (position from user input) J-Ks=0.507+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:43.39 +37:37:29.1: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:43.39 +37:37:29.1: 14.79 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.47 22:00:33.04 +35:15:46.4
87.80262 -15.70067 galactic Peg Second-epoch detections are separated by 1.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:33.04 +35:15:46.4 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:33.04 +35:15:46.4: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:33.04 +35:15:46.4: 15.16 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.51 21:49:47.22 +34:12:11.0
85.33838 -15.09338 galactic Peg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:47.22 +34:12:11.0 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:47.22 +34:12:11.0: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:47.22 +34:12:11.0: 15.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.47 21:43:00.40 +34:57:39.2
84.78001 -13.60031 galactic Cyg Second-epoch detections are separated by 3.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.7527+34.9668 | 21:43:00.40 +34:57:39.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.373+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:00.40 +34:57:39.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:00.40 +34:57:39.2: 14.96 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.7527+34.9668,2461172.8579,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.7527+34.9668 20260512.3579 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.41 22:02:22.22 +33:59:02.7
87.27193 -16.93196 galactic Peg Second-epoch detections are separated by 3.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.5941+33.9856 | 22:02:22.22 +33:59:02.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:22.22 +33:59:02.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:22.22 +33:59:02.7: 15.33 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.5941+33.9856,2461172.8579,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.5941+33.9856 20260512.3579 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.27 21:53:00.60 +35:46:14.9
86.91143 -14.33265 galactic Peg Second-epoch detections are separated by 1.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:53:00.60 +35:46:14.9 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.571+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:00.60 +35:46:14.9: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:00.60 +35:46:14.9: 14.71 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.38 21:52:58.87 +39:47:12.8
89.54723 -11.24657 galactic Cyg Second-epoch detections are separated by 0.3" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:58.87 +39:47:12.8 (user input) | T | P | (position from user input) J-Ks=0.661+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:58.87 +39:47:12.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:58.87 +39:47:12.8: 14.68 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.38 21:31:04.27 +36:50:21.3
84.28519 -10.57796 galactic Cyg Second-epoch detections are separated by 1.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:04.27 +36:50:21.3 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:04.27 +36:50:21.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:04.27 +36:50:21.3: 14.45 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.19 21:29:56.56 +36:19:12.5
83.75192 -10.79291 galactic Cyg Second-epoch detections are separated by 4.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.4845+36.3132 | 21:29:56.56 +36:19:12.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:56.56 +36:19:12.5: 13.05 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:56.56 +36:19:12.5: 14.24 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.4845+36.3132,2461172.8579,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.4845+36.3132 20260512.3579 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.29 21:47:28.68 +39:11:54.5
88.33349 -11.01181 galactic Cyg Second-epoch detections are separated by 2.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:47:28.68 +39:11:54.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:28.68 +39:11:54.5: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:28.68 +39:11:54.5: 15.23 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.34 22:11:53.83 +39:29:36.8
92.31049 -13.70963 galactic Lac Second-epoch detections are separated by 0.9" and 2.8 pix
The object was found in VSX 9" Gaia DR3 1955632578489408128
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
18.360 G 18.680 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:53.83 +39:29:36.8: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:53.83 +39:29:36.8: 14.86 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955632578489408128,2461172.8579,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955632578489408128 20260512.3579 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.35 22:00:55.83 +36:53:37.8
88.92013 -14.47522 galactic Lac Second-epoch detections are separated by 5.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.2309+36.8928 | 22:00:55.83 +36:53:37.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:55.83 +36:53:37.8: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:55.83 +36:53:37.8: 15.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.2309+36.8928,2461172.8579,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.2309+36.8928 20260512.3579 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.31 21:59:13.18 +42:19:04.5
92.09434 -10.01291 galactic Lac Second-epoch detections are separated by 0.3" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:13.18 +42:19:04.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:13.18 +42:19:04.5: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:13.18 +42:19:04.5: 14.90 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.36 21:43:08.73 +40:49:38.0
88.78317 -9.23842 galactic Cyg Second-epoch detections are separated by 3.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.7962+40.8254 | 21:43:08.73 +40:49:38.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.461+/-0.046 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:08.73 +40:49:38.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:08.73 +40:49:38.0: 15.20 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.20 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.7962+40.8254,2461172.8579,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.7962+40.8254 20260512.3579 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.25 22:04:41.19 +40:20:52.3
91.69485 -12.19930 galactic Lac Second-epoch detections are separated by 1.8" and 2.7 pix
The object was found in VSX16" Gaia DR3 1956639769799538560
Type: ROT
# Max. Min./Amp. JD0 Period
15.840 G 15.880 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:41.19 +40:20:52.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:41.19 +40:20:52.3: 14.54 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956639769799538560,2461172.8579,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956639769799538560 20260512.3579 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.43 22:11:52.79 +40:52:48.9
93.14238 -12.58414 galactic Lac Second-epoch detections are separated by 2.6" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:52.79 +40:52:48.9 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:52.79 +40:52:48.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:52.79 +40:52:48.9: 14.72 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:56:01.47 +35:45:22.2
87.38645 -14.73606 galactic Peg Second-epoch detections are separated by 1.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:01.47 +35:45:22.2 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:01.47 +35:45:22.2: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:01.47 +35:45:22.2: 15.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.43 21:50:07.58 +42:10:53.8
90.68097 -9.06034 galactic Cyg Second-epoch detections are separated by 1.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.5325+42.1739 | 21:50:07.58 +42:10:53.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.441+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:07.58 +42:10:53.8: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:07.58 +42:10:53.8: 14.70 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.5325+42.1739,2461172.8579,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.5325+42.1739 20260512.3579 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:44:30.95 +38:50:13.2
87.64964 -10.90716 galactic Cyg Second-epoch detections are separated by 1.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:30.95 +38:50:13.2 (user input) | T | P | (position from user input) J-Ks=0.466+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:30.95 +38:50:13.2: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:30.95 +38:50:13.2: 15.29 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.29 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.39 21:51:39.60 +42:01:59.1
90.80646 -9.35636 galactic Cyg Second-epoch detections are separated by 3.6" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:39.60 +42:01:59.1 (user input) | T | P | (position from user input) J-Ks=0.493+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:39.60 +42:01:59.1: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:39.60 +42:01:59.1: 14.84 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.44 21:49:56.15 +36:30:34.0
86.91761 -13.36789 galactic Peg Second-epoch detections are separated by 3.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.4940+36.5046 | 21:49:56.15 +36:30:34.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.453+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:56.15 +36:30:34.0: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:56.15 +36:30:34.0: 14.70 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.4940+36.5046,2461172.8579,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.4940+36.5046 20260512.3579 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.39 21:59:29.65 +36:02:35.0
88.13711 -14.95860 galactic Peg Second-epoch detections are separated by 2.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.8768+36.0410 | 21:59:29.65 +36:02:35.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:29.65 +36:02:35.0: 12.79 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:29.65 +36:02:35.0: 14.96 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.8768+36.0410,2461172.8579,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.8768+36.0410 20260512.3579 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:37:37.21 +37:57:03.9
86.02403 -10.66181 galactic Cyg Second-epoch detections are separated by 3.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1953528254969388800 | 21:37:37.21 +37:57:03.9 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.431+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:37.21 +37:57:03.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:37.21 +37:57:03.9: 14.97 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1953528254969388800,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1953528254969388800 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.53 22:08:05.83 +41:53:32.3
93.16588 -11.34839 galactic Lac Second-epoch detections are separated by 0.8" and 2.5 pix
The object was found in VSX10" ZTF J220806.43+415340.2
Type: EW
# Max. Min./Amp. JD0 Period
17.111 g Y 0.534 g 2458272.97290 0.343266000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:05.83 +41:53:32.3: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:05.83 +41:53:32.3: 14.91 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J220806.43+415340.2,2461172.8579,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J220806.43+415340.2 20260512.3579 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.32 21:52:57.02 +41:56:24.6
90.93426 -9.58050 galactic Cyg Second-epoch detections are separated by 2.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:57.02 +41:56:24.6 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.056 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:57.02 +41:56:24.6: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:57.02 +41:56:24.6: 14.80 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:55:40.14 +42:12:52.4
91.50694 -9.68542 galactic Cyg Second-epoch detections are separated by 0.6" and 2.5 pix
The object was found in VSX18" Gaia DR3 1960777575653317120
Type: ROT
# Max. Min./Amp. JD0 Period
15.070 G 15.100 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:40.14 +42:12:52.4: 12.88 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:40.14 +42:12:52.4: 14.67 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960777575653317120,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960777575653317120 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.31 21:39:26.15 +34:58:47.9
84.23850 -13.09248 galactic Cyg Second-epoch detections are separated by 2.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:26.15 +34:58:47.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:26.15 +34:58:47.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:26.15 +34:58:47.9: 14.89 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.42 21:40:55.08 +37:27:31.1
86.17643 -11.46530 galactic Cyg Second-epoch detections are separated by 2.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2298+37.4563 | 21:40:55.08 +37:27:31.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.495+/-0.064 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:55.08 +37:27:31.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:55.08 +37:27:31.1: 14.93 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2298+37.4563,2461172.8579,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2298+37.4563 20260512.3579 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.53 22:00:48.39 +36:27:05.0
88.61508 -14.80577 galactic Peg Second-epoch detections are separated by 4.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:48.39 +36:27:05.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:48.39 +36:27:05.0: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:48.39 +36:27:05.0: 15.28 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.28 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.31 21:44:34.94 +33:59:27.3
84.35847 -14.53792 galactic Cyg Second-epoch detections are separated by 1.7" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:34.94 +33:59:27.3 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:34.94 +33:59:27.3: 12.74 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:34.94 +33:59:27.3: 15.09 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.36 21:54:18.94 +34:21:39.2
86.18138 -15.58236 galactic Peg Second-epoch detections are separated by 1.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:18.94 +34:21:39.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:18.94 +34:21:39.2: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:18.94 +34:21:39.2: 14.58 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.28 22:11:11.50 +41:48:09.4
93.58714 -11.76048 galactic Lac Second-epoch detections are separated by 0.1" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.7994+41.8054 | 22:11:11.50 +41:48:09.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.453+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:11.50 +41:48:09.4: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:11.50 +41:48:09.4: 15.31 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.7994+41.8054,2461172.8579,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.7994+41.8054 20260512.3579 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.53 21:59:19.84 +39:44:23.1
90.48531 -12.05092 galactic Lac Second-epoch detections are separated by 2.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:19.84 +39:44:23.1 (user input) | T | P | (position from user input) J-Ks=0.331+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:19.84 +39:44:23.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:19.84 +39:44:23.1: 15.42 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.42 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.25 21:29:38.93 +36:14:26.8
83.65235 -10.80838 galactic Cyg Second-epoch detections are separated by 3.0" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:38.93 +36:14:26.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:38.93 +36:14:26.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:38.93 +36:14:26.8: 14.81 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.32 21:52:13.78 +34:04:19.5
85.64619 -15.52289 galactic Peg Second-epoch detections are separated by 1.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:13.78 +34:04:19.5 (user input) | T | P | (position from user input) J-Ks=0.656+/-0.049 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:13.78 +34:04:19.5: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:13.78 +34:04:19.5: 15.05 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.44 21:45:59.71 +34:32:51.9
84.96654 -14.31774 galactic Cyg Second-epoch detections are separated by 2.1" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:59.71 +34:32:51.9 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:59.71 +34:32:51.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:59.71 +34:32:51.9: 15.24 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.30 22:01:32.44 +34:05:01.2
87.19718 -16.74664 galactic Peg Second-epoch detections are separated by 3.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:01:32.44 +34:05:01.2 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:32.44 +34:05:01.2: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:32.44 +34:05:01.2: 15.04 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.26 21:48:31.76 +39:16:35.8
88.54279 -11.08495 galactic Cyg Second-epoch detections are separated by 1.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.1228+39.2740 | 21:48:31.76 +39:16:35.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.531+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:31.76 +39:16:35.8: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:31.76 +39:16:35.8: 14.61 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.1228+39.2740,2461172.8579,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.1228+39.2740 20260512.3579 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.43 22:11:40.95 +38:00:40.6
91.37418 -14.88253 galactic Lac Second-epoch detections are separated by 3.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:40.95 +38:00:40.6 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.041 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:40.95 +38:00:40.6: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:40.95 +38:00:40.6: 14.96 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.28 21:28:56.61 +38:33:57.6
85.19715 -9.04458 galactic Cyg Second-epoch detections are separated by 4.4" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:56.61 +38:33:57.6 (user input) | T | P | (position from user input) J-Ks=0.677+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:56.61 +38:33:57.6: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:56.61 +38:33:57.6: 14.75 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.43 21:49:46.32 +40:24:29.2
89.47291 -10.37639 galactic Cyg Second-epoch detections are separated by 1.5" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:46.32 +40:24:29.2 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:46.32 +40:24:29.2: 13.53 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:46.32 +40:24:29.2: 14.91 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.39 21:56:21.42 +38:37:25.6
89.31043 -12.56064 galactic Cyg Second-epoch detections are separated by 2.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1950057474720955776 | 21:56:23.86 +38:36:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.489+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:21.42 +38:37:25.6: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:21.42 +38:37:25.6: 15.01 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950057474720955776,2461172.8579,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950057474720955776 20260512.3579 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.38 21:48:59.09 +35:21:20.3
85.99143 -14.11551 galactic Cyg Second-epoch detections are separated by 1.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:59.09 +35:21:20.3 (user input) | T | P | (position from user input) J-Ks=0.584+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:59.09 +35:21:20.3: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:59.09 +35:21:20.3: 15.09 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.35 21:50:11.78 +38:02:34.9
87.97907 -12.23510 galactic Cyg Second-epoch detections are separated by 0.8" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:11.78 +38:02:34.9 (user input) | T | P | (position from user input) J-Ks=0.568+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:11.78 +38:02:34.9: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:11.78 +38:02:34.9: 14.74 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.62 21:58:18.04 +34:23:37.9
86.85996 -16.08333 galactic Peg Second-epoch detections are separated by 0.8" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.5881+34.3875 | 21:58:18.04 +34:23:37.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.397+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:18.04 +34:23:37.9: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:18.04 +34:23:37.9: 15.37 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.37 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.5881+34.3875,2461172.8579,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.5881+34.3875 20260512.3579 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.44 22:03:45.00 +39:44:32.7
91.17257 -12.57139 galactic Lac Second-epoch detections are separated by 1.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956551602712257792 | 22:03:41.66 +39:44:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.789+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:45.00 +39:44:32.7: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:45.00 +39:44:32.7: 14.71 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956551602712257792,2461172.8579,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956551602712257792 20260512.3579 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.34 21:43:25.64 +36:45:53.6
86.08261 -12.31567 galactic Cyg Second-epoch detections are separated by 1.6" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:25.64 +36:45:53.6 (user input) | T | P | (position from user input) J-Ks=0.568+/-0.044 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:25.64 +36:45:53.6: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:25.64 +36:45:53.6: 15.01 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.52 22:10:04.13 +38:55:16.1
91.66798 -13.96240 galactic Lac Second-epoch detections are separated by 4.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:10:04.13 +38:55:16.1 (user input) | T | P | (position from user input) J-Ks=0.381+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:04.13 +38:55:16.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:04.13 +38:55:16.1: 14.95 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:28:31.39 +33:41:58.1
81.66305 -12.45619 galactic Cyg Second-epoch detections are separated by 2.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:31.39 +33:41:58.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:31.39 +33:41:58.1: 13.24 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:31.39 +33:41:58.1: 14.78 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.49 22:05:41.20 +41:02:04.2
92.27307 -11.76629 galactic Lac Second-epoch detections are separated by 1.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.4275+41.0304 | 22:05:41.20 +41:02:04.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.344+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:41.20 +41:02:04.2: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:41.20 +41:02:04.2: 15.18 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.18 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.4275+41.0304,2461172.8579,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.4275+41.0304 20260512.3579 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.35 21:54:13.78 +42:03:15.5
91.19423 -9.64235 galactic Cyg Second-epoch detections are separated by 0.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:13.78 +42:03:15.5 (user input) | T | P | (position from user input) J-Ks=0.806+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:13.78 +42:03:15.5: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:13.78 +42:03:15.5: 14.94 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.31 21:37:31.25 +35:02:48.5
83.99066 -12.77646 galactic Cyg Second-epoch detections are separated by 1.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:31.25 +35:02:48.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.847+/-0.035 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:31.25 +35:02:48.5: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:31.25 +35:02:48.5: 14.86 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.52 22:11:18.84 +39:15:07.6
92.07038 -13.83851 galactic Lac Second-epoch detections are separated by 0.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:18.84 +39:15:07.6 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:18.84 +39:15:07.6: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:18.84 +39:15:07.6: 14.93 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.41 21:44:37.79 +36:48:09.8
86.29251 -12.44747 galactic Cyg Second-epoch detections are separated by 1.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:37.79 +36:48:09.8 (user input) | T | P | (position from user input) J-Ks=0.381+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:37.79 +36:48:09.8: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:37.79 +36:48:09.8: 15.10 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.57 21:50:41.89 +37:37:59.7
87.78485 -12.61161 galactic Cyg Second-epoch detections are separated by 0.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:41.89 +37:37:59.7 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:41.89 +37:37:59.7: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:41.89 +37:37:59.7: 15.29 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.29 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.36 22:05:03.22 +41:23:49.0
92.39886 -11.40525 galactic Lac Second-epoch detections are separated by 3.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:05:03.22 +41:23:49.0 (user input) | T | P | (position from user input) J-Ks=0.731+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:03.22 +41:23:49.0: 13.07 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:03.22 +41:23:49.0: 15.16 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.52 21:50:23.40 +37:34:17.7
87.69627 -12.61909 galactic Cyg Second-epoch detections are separated by 1.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.5928+37.5712 | 21:50:23.40 +37:34:17.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.388+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:23.40 +37:34:17.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:23.40 +37:34:17.7: 15.26 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.5928+37.5712,2461172.8579,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.5928+37.5712 20260512.3579 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.47 21:58:27.10 +41:39:27.4
91.56539 -10.44350 galactic Lac Second-epoch detections are separated by 1.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.6163+41.6662 | 21:58:27.10 +41:39:27.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.795+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:27.10 +41:39:27.4: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:27.10 +41:39:27.4: 14.78 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.6163+41.6662,2461172.8579,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.6163+41.6662 20260512.3579 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.22 21:31:39.41 +36:46:29.7
84.32566 -10.70563 galactic Cyg Second-epoch detections are separated by 0.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:39.41 +36:46:29.7 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:39.41 +36:46:29.7: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:39.41 +36:46:29.7: 14.40 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.57 22:10:13.66 +36:21:54.4
90.11623 -16.03311 galactic Lac Second-epoch detections are separated by 2.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:10:13.66 +36:21:54.4 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:13.66 +36:21:54.4: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:13.66 +36:21:54.4: 15.45 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.45 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.45 21:42:21.27 +38:13:08.4
86.90985 -11.08947 galactic Cyg Second-epoch detections are separated by 2.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5860+38.2161 | 21:42:21.27 +38:13:08.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.355+/-0.046 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:21.27 +38:13:08.4: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:21.27 +38:13:08.4: 14.99 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5860+38.2161,2461172.8579,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5860+38.2161 20260512.3579 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.37 21:52:45.52 +42:15:34.6
91.11170 -9.31092 galactic Cyg Second-epoch detections are separated by 0.5" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:45.52 +42:15:34.6 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:45.52 +42:15:34.6: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:45.52 +42:15:34.6: 14.79 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.46 21:48:54.48 +37:26:43.2
87.38333 -12.52408 galactic Cyg Second-epoch detections are separated by 3.0" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:54.48 +37:26:43.2 (user input) | T | P | (position from user input) J-Ks=0.308+/-0.060 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:54.48 +37:26:43.2: 13.67 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:54.48 +37:26:43.2: 15.32 +/- 0.30 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.39 21:45:57.25 +39:56:07.7
88.59724 -10.26200 galactic Cyg Second-epoch detections are separated by 0.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:57.25 +39:56:07.7 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:57.25 +39:56:07.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:57.25 +39:56:07.7: 14.79 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.35 22:10:15.72 +41:34:00.8
93.30227 -11.84957 galactic Lac Second-epoch detections are separated by 0.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.5657+41.5671 | 22:10:15.72 +41:34:00.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.696+/-0.041 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:15.72 +41:34:00.8: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:15.72 +41:34:00.8: 14.87 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.5657+41.5671,2461172.8579,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.5657+41.5671 20260512.3579 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.41 21:50:24.73 +34:50:30.8
85.87204 -14.69499 galactic Peg Second-epoch detections are separated by 1.0" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:24.73 +34:50:30.8 (user input) | T | P | (position from user input) J-Ks=0.319+/-0.045 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:24.73 +34:50:30.8: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:24.73 +34:50:30.8: 15.16 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.53 21:47:39.91 +41:28:28.4
89.86424 -9.30544 galactic Cyg Second-epoch detections are separated by 0.3" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:47:39.91 +41:28:28.4 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:39.91 +41:28:28.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:39.91 +41:28:28.4: 14.88 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.44 21:58:30.14 +36:23:05.3
88.19856 -14.56709 galactic Peg Second-epoch detections are separated by 0.8" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.6267+36.3763 | 21:58:30.14 +36:23:05.3 (user input) | CBF (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:30.14 +36:23:05.3: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:30.14 +36:23:05.3: 14.81 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.6267+36.3763,2461172.8579,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.6267+36.3763 20260512.3579 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.38 21:58:01.30 +38:57:27.6
89.78385 -12.50469 galactic Lac Second-epoch detections are separated by 1.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:01.30 +38:57:27.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.818+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:01.30 +38:57:27.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:01.30 +38:57:27.6: 15.26 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.55 21:59:57.43 +36:55:02.7
88.77829 -14.33543 galactic Lac Second-epoch detections are separated by 0.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:57.43 +36:55:02.7 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:57.43 +36:55:02.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:57.43 +36:55:02.7: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.55 21:47:31.96 +35:11:22.3
85.64862 -14.04568 galactic Cyg Second-epoch detections are separated by 1.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:47:31.96 +35:11:22.3 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.048 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:31.96 +35:11:22.3: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:31.96 +35:11:22.3: 15.08 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.46 21:55:53.83 +37:45:14.8
88.67465 -13.17734 galactic Cyg Second-epoch detections are separated by 0.8" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.9635+37.7496 | 21:55:53.83 +37:45:14.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.786+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:53.83 +37:45:14.8: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:53.83 +37:45:14.8: 15.23 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.9635+37.7496,2461172.8579,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.9635+37.7496 20260512.3579 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.35 22:06:03.46 +41:22:06.3
92.53489 -11.54130 galactic Lac Second-epoch detections are separated by 1.3" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.5145+41.3685 | 22:06:03.46 +41:22:06.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.536+/- (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:03.46 +41:22:06.3: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:03.46 +41:22:06.3: 14.88 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.5145+41.3685,2461172.8579,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.5145+41.3685 20260512.3579 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.30 22:02:54.61 +40:29:58.1
91.51460 -11.87342 galactic Lac Second-epoch detections are separated by 2.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:54.61 +40:29:58.1 (user input) | T | P | (position from user input) J-Ks=0.466+/-0.039 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:54.61 +40:29:58.1: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:54.61 +40:29:58.1: 15.11 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.56 22:01:31.62 +37:57:47.2
89.70001 -13.71022 galactic Lac Second-epoch detections are separated by 0.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:01:31.62 +37:57:47.2 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:31.62 +37:57:47.2: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:31.62 +37:57:47.2: 15.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.34 22:04:28.27 +41:44:47.9
92.52534 -11.06063 galactic Lac Second-epoch detections are separated by 4.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:04:28.27 +41:44:47.9 (user input) | T | P | (position from user input) J-Ks=0.545+/-0.149 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:28.27 +41:44:47.9: 12.90 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:28.27 +41:44:47.9: 14.77 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.54 21:47:07.93 +39:07:42.5
88.23520 -11.02110 galactic Cyg Second-epoch detections are separated by 0.5" and 2.5 pix
The object was found in VSX21" Gaia DR3 1953285022384759936
Type: ROT
# Max. Min./Amp. JD0 Period
16.750 G 16.790 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:07.93 +39:07:42.5: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:07.93 +39:07:42.5: 14.77 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953285022384759936,2461172.8579,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953285022384759936 20260512.3579 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.43 21:43:18.36 +39:30:22.8
87.92061 -10.24986 galactic Cyg Second-epoch detections are separated by 2.0" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.8240+39.4965 | 21:43:18.36 +39:30:22.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.446+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:18.36 +39:30:22.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:18.36 +39:30:22.8: 14.52 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.8240+39.4965,2461172.8579,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.8240+39.4965 20260512.3579 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.46 22:03:45.74 +37:39:38.7
89.86645 -14.22036 galactic Lac Second-epoch detections are separated by 1.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.9357+37.6642 | 22:03:45.74 +37:39:38.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.651+/-0.044 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:45.74 +37:39:38.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:45.74 +37:39:38.7: 15.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.9357+37.6642,2461172.8579,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.9357+37.6642 20260512.3579 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.29 22:09:32.18 +42:04:31.1
93.49624 -11.35899 galactic Lac Second-epoch detections are separated by 1.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:09:32.18 +42:04:31.1 (user input) | T | P | (position from user input) J-Ks=0.845+/-0.036 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:32.18 +42:04:31.1: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:32.18 +42:04:31.1: 15.13 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.31 21:36:40.42 +34:18:58.2
83.34686 -13.18951 galactic Cyg Second-epoch detections are separated by 3.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:40.42 +34:18:58.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.670+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:40.42 +34:18:58.2: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:40.42 +34:18:58.2: 15.19 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.44 21:31:04.35 +38:40:11.5
85.57338 -9.25850 galactic Cyg Second-epoch detections are separated by 2.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:04.35 +38:40:11.5 (user input) | T | P | (position from user input) J-Ks=0.743+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:04.35 +38:40:11.5: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:04.35 +38:40:11.5: 14.93 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.28 21:39:12.74 +36:17:19.8
85.11362 -12.09961 galactic Cyg Second-epoch detections are separated by 1.5" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1951077168676950144 | 21:39:15.93 +36:17:28.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5) J-Ks=0.393+/-0.049 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:12.74 +36:17:19.8: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:12.74 +36:17:19.8: 14.75 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951077168676950144,2461172.8579,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951077168676950144 20260512.3579 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.43 21:59:59.28 +38:04:07.7
89.52295 -13.43924 galactic Lac Second-epoch detections are separated by 1.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:59.28 +38:04:07.7 (user input) | T | P | (position from user input) J-Ks=0.664+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:59.28 +38:04:07.7: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:59.28 +38:04:07.7: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.41 21:45:15.69 +35:22:23.0
85.41609 -13.60123 galactic Cyg Second-epoch detections are separated by 0.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:15.69 +35:22:23.0 (user input) | T | P | (position from user input) J-Ks=0.532+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:15.69 +35:22:23.0: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:15.69 +35:22:23.0: 15.24 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.29 21:58:32.55 +37:54:59.4
89.19651 -13.38034 galactic Lac Second-epoch detections are separated by 3.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949965493701517568 | 21:58:29.55 +37:54:46.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:32.55 +37:54:59.4: 12.79 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:32.55 +37:54:59.4: 14.56 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949965493701517568,2461172.8579,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949965493701517568 20260512.3579 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.57 21:51:40.80 +35:15:18.4
86.35371 -14.55055 galactic Peg Second-epoch detections are separated by 1.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:40.80 +35:15:18.4 (user input) | T | P | (position from user input) J-Ks=0.515+/-0.042 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:40.80 +35:15:18.4: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:40.80 +35:15:18.4: 15.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:49:29.14 +36:55:04.6
87.12051 -12.99913 galactic Cyg Second-epoch detections are separated by 1.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:29.14 +36:55:04.6 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.049 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:29.14 +36:55:04.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:29.14 +36:55:04.6: 14.72 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.61 21:58:40.75 +35:20:14.8
87.54337 -15.40236 galactic Peg Second-epoch detections are separated by 3.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.6626+35.3264 | 21:58:40.75 +35:20:14.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.351+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:40.75 +35:20:14.8: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:40.75 +35:20:14.8: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.6626+35.3264,2461172.8579,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.6626+35.3264 20260512.3579 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.38 22:02:16.99 +35:25:29.1
88.19430 -15.79502 galactic Peg Second-epoch detections are separated by 2.1" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:16.99 +35:25:29.1 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:16.99 +35:25:29.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:16.99 +35:25:29.1: 15.03 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.36 21:39:30.92 +37:21:42.5
85.89972 -11.34960 galactic Cyg Second-epoch detections are separated by 2.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:30.92 +37:21:42.5 (user input) | T | P | (position from user input) J-Ks=0.871+/-0.034 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:30.92 +37:21:42.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:30.92 +37:21:42.5: 14.73 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.73 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.48 21:45:18.26 +34:36:19.2
84.89656 -14.18013 galactic Cyg Second-epoch detections are separated by 2.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:18.26 +34:36:19.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:18.26 +34:36:19.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:18.26 +34:36:19.2: 15.15 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.49 21:44:17.40 +36:34:05.3
86.08078 -12.57765 galactic Cyg Second-epoch detections are separated by 0.1" and 2.6 pix
The object was found in VSX25" Gaia DR3 1952398266258269568
Type: ROT
# Max. Min./Amp. JD0 Period
16.710 G 16.770 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:17.40 +36:34:05.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:17.40 +36:34:05.3: 15.03 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952398266258269568,2461172.8579,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952398266258269568 20260512.3579 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.42 21:28:45.69 +39:40:27.0
85.95174 -8.22438 galactic Cyg Second-epoch detections are separated by 4.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:45.69 +39:40:27.0 (user input) | T | P | (position from user input) J-Ks=0.735+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:45.69 +39:40:27.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:45.69 +39:40:27.0: 14.92 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.51 21:56:54.99 +41:26:11.6
91.19688 -10.43782 galactic Cyg Second-epoch detections are separated by 2.1" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.2456+41.4395 | 21:56:54.99 +41:26:11.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.705+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:54.99 +41:26:11.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:54.99 +41:26:11.6: 15.24 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.2456+41.4395,2461172.8579,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.2456+41.4395 20260512.3579 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.54 21:50:02.20 +37:36:18.4
87.66393 -12.54819 galactic Cyg Second-epoch detections are separated by 1.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:02.20 +37:36:18.4 (user input) | T | P | (position from user input) J-Ks=0.508+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:02.20 +37:36:18.4: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:02.20 +37:36:18.4: 15.48 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.48 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.36 21:51:40.04 +38:49:50.4
88.72349 -11.81886 galactic Cyg Second-epoch detections are separated by 2.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:40.04 +38:49:50.4 (user input) | T | P | (position from user input) J-Ks=0.772+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:40.04 +38:49:50.4: 13.19 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:40.04 +38:49:50.4: 14.64 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.53 21:52:00.27 +36:48:32.6
87.44198 -13.40868 galactic Cyg Second-epoch detections are separated by 3.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:00.27 +36:48:32.6 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.050 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:00.27 +36:48:32.6: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:00.27 +36:48:32.6: 15.42 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.42 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.42 21:50:09.92 +40:20:09.6
89.48397 -10.47980 galactic Cyg Second-epoch detections are separated by 1.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:09.92 +40:20:09.6 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:09.92 +40:20:09.6: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:09.92 +40:20:09.6: 14.91 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.33 21:28:08.21 +36:20:37.8
83.50442 -10.52147 galactic Cyg Second-epoch detections are separated by 1.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.0319+36.3316 | 21:28:08.21 +36:20:37.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.579+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:08.21 +36:20:37.8: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:08.21 +36:20:37.8: 14.85 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0319+36.3316,2461172.8579,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0319+36.3316 20260512.3579 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.26 21:37:52.89 +35:41:21.5
84.49483 -12.35687 galactic Cyg Second-epoch detections are separated by 2.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:52.89 +35:41:21.5 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.049 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:52.89 +35:41:21.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:52.89 +35:41:21.5: 14.68 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.54 21:58:05.47 +36:02:57.0
87.91319 -14.77522 galactic Peg Second-epoch detections are separated by 1.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.5275+36.0583 | 21:58:05.47 +36:02:57.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.654+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:05.47 +36:02:57.0: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:05.47 +36:02:57.0: 15.46 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.46 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.5275+36.0583,2461172.8579,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.5275+36.0583 20260512.3579 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:55:36.85 +38:47:54.9
89.30843 -12.33358 galactic Cyg Second-epoch detections are separated by 1.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:36.85 +38:47:54.9 (user input) | T | P | (position from user input) J-Ks=0.547+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:36.85 +38:47:54.9: 13.25 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:36.85 +38:47:54.9: 15.24 +/- 0.30 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.52 21:51:39.69 +34:33:54.7
85.88667 -15.07221 galactic Peg Second-epoch detections are separated by 2.6" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:39.69 +34:33:54.7 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:39.69 +34:33:54.7: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:39.69 +34:33:54.7: 15.10 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.41 21:51:54.16 +39:30:23.0
89.20162 -11.32971 galactic Cyg Second-epoch detections are separated by 2.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:54.16 +39:30:23.0 (user input) | T | P | (position from user input) J-Ks=0.441+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:54.16 +39:30:23.0: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:54.16 +39:30:23.0: 15.03 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.39 21:55:20.73 +34:39:48.1
86.55194 -15.48732 galactic Peg Second-epoch detections are separated by 2.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:20.73 +34:39:48.1 (user input) | T | P | (position from user input) J-Ks=0.296+/- (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:20.73 +34:39:48.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:20.73 +34:39:48.1: 14.89 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.63 21:51:45.90 +37:59:55.3
88.19132 -12.46838 galactic Cyg Second-epoch detections are separated by 1.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:45.90 +37:59:55.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:45.90 +37:59:55.3: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:45.90 +37:59:55.3: 15.36 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.36 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.43 21:56:38.98 +41:55:31.3
91.46748 -10.02490 galactic Cyg Second-epoch detections are separated by 3.4" and 2.8 pix
The object was found in VSX 3" ASASSN-V J215638.98+415528.0
Type: ROT
# Max. Min./Amp. JD0 Period
14.930 V 15.070 V 2457550.98500 8.188900000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:38.98 +41:55:31.3: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:38.98 +41:55:31.3: 14.93 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J215638.98+415528.0,2461172.8579,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J215638.98+415528.0 20260512.3579 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.43 21:38:12.01 +37:42:55.4
85.94729 -10.91278 galactic Cyg Second-epoch detections are separated by 2.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.5379+37.7193 | 21:38:12.01 +37:42:55.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.437+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:12.01 +37:42:55.4: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:12.01 +37:42:55.4: 14.78 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.5379+37.7193,2461172.8579,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.5379+37.7193 20260512.3579 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.38 21:56:48.74 +40:07:52.5
90.34946 -11.44378 galactic Cyg Second-epoch detections are separated by 2.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:48.74 +40:07:52.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:48.74 +40:07:52.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:48.74 +40:07:52.5: 14.52 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.38 21:41:24.09 +39:05:05.1
87.35605 -10.32011 galactic Cyg Second-epoch detections are separated by 2.0" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:24.09 +39:05:05.1 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:24.09 +39:05:05.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:24.09 +39:05:05.1: 15.14 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:28:20.33 +36:35:54.5
83.71545 -10.36843 galactic Cyg Second-epoch detections are separated by 2.2" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.0756+36.6023 | 21:28:20.33 +36:35:54.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.262+/-0.050 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:20.33 +36:35:54.5: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:20.33 +36:35:54.5: 14.49 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0756+36.6023,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0756+36.6023 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.50 22:05:36.58 +41:17:42.1
92.42127 -11.54945 galactic Lac Second-epoch detections are separated by 0.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1959778944212475008 | 22:05:32.79 +41:17:29.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.674+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:36.58 +41:17:42.1: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:36.58 +41:17:42.1: 15.42 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.42 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1959778944212475008,2461172.8579,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1959778944212475008 20260512.3579 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:48:39.20 +37:49:36.7
87.59872 -12.20184 galactic Cyg Second-epoch detections are separated by 1.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:39.20 +37:49:36.7 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:39.20 +37:49:36.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:39.20 +37:49:36.7: 15.24 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.55 21:43:12.83 +35:46:27.1
85.37200 -13.02466 galactic Cyg Second-epoch detections are separated by 1.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:12.83 +35:46:27.1 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.049 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:12.83 +35:46:27.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:12.83 +35:46:27.1: 15.08 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.49 21:59:29.20 +39:40:34.1
90.46898 -12.11942 galactic Lac Second-epoch detections are separated by 2.1" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:29.20 +39:40:34.1 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:29.20 +39:40:34.1: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:29.20 +39:40:34.1: 15.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.53 22:00:32.74 +41:01:59.0
91.48723 -11.17741 galactic Lac Second-epoch detections are separated by 2.3" and 2.8 pix
The object was found in VSX24" Gaia DR3 1959713832512277376
Type: RS
# Max. Min./Amp. JD0 Period
17.330 G 17.440 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:32.74 +41:01:59.0: 12.91 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:32.74 +41:01:59.0: 15.32 +/- 0.33 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959713832512277376,2461172.8579,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959713832512277376 20260512.3579 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.45 21:46:56.51 +37:17:28.1
86.97746 -12.38509 galactic Cyg Second-epoch detections are separated by 1.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:46:56.51 +37:17:28.1 (user input) | T | P | (position from user input) J-Ks=0.535+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:56.51 +37:17:28.1: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:56.51 +37:17:28.1: 15.23 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.47 21:44:35.61 +34:37:03.7
84.79270 -14.07336 galactic Cyg Second-epoch detections are separated by 4.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.1587+34.6257 | 21:44:35.61 +34:37:03.7 (user input) | PULSE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.669+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:35.61 +34:37:03.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:35.61 +34:37:03.7: 15.04 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.1587+34.6257,2461172.8579,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.1587+34.6257 20260512.3579 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.44 21:30:41.20 +35:07:20.1
83.00953 -11.75607 galactic Cyg Second-epoch detections are separated by 1.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:41.20 +35:07:20.1 (user input) | T | P | (position from user input) J-Ks=0.710+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:41.20 +35:07:20.1: 13.42 +/- 0.35 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:41.20 +35:07:20.1: 15.31 +/- 0.34 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.50 21:53:17.71 +39:27:53.4
89.38544 -11.53331 galactic Cyg Second-epoch detections are separated by 1.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:53:17.71 +39:27:53.4 (user input) | T | P | (position from user input) J-Ks=0.875+/-0.034 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:17.71 +39:27:53.4: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:17.71 +39:27:53.4: 14.85 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.61 21:55:29.46 +39:55:36.7
90.01766 -11.44368 galactic Cyg Second-epoch detections are separated by 1.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.8704+39.9276 | 21:55:29.46 +39:55:36.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.461+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:29.46 +39:55:36.7: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:29.46 +39:55:36.7: 15.24 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.8704+39.9276,2461172.8579,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.8704+39.9276 20260512.3579 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.51 21:45:05.81 +37:10:31.4
86.61671 -12.23006 galactic Cyg Second-epoch detections are separated by 3.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.2616+37.1700 | 21:45:02.80 +37:10:12.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:05.81 +37:10:31.4: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:05.81 +37:10:31.4: 14.68 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.2616+37.1700,2461172.8579,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.2616+37.1700 20260512.3579 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.48 21:37:04.93 +35:55:02.5
84.53265 -12.07954 galactic Cyg Second-epoch detections are separated by 1.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:04.93 +35:55:02.5 (user input) | T | P | (position from user input) J-Ks=0.634+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:04.93 +35:55:02.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:04.93 +35:55:02.5: 14.85 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.54 21:53:44.10 +39:01:58.7
89.17158 -11.92049 galactic Cyg Second-epoch detections are separated by 0.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:53:44.10 +39:01:58.7 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:44.10 +39:01:58.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:44.10 +39:01:58.7: 15.36 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.36 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.37 21:40:19.76 +35:37:23.6
84.82313 -12.74277 galactic Cyg Second-epoch detections are separated by 1.0" and 2.5 pix
The object was found in VSX17" Gaia DR3 1950852765226527104
Type: ROT
# Max. Min./Amp. JD0 Period
17.130 G 17.160 G 0.454966000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:19.76 +35:37:23.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:19.76 +35:37:23.6: 15.19 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950852765226527104,2461172.8579,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950852765226527104 20260512.3579 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.40 21:54:41.38 +41:37:13.6
90.98423 -10.03320 galactic Cyg Second-epoch detections are separated by 2.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:41.38 +41:37:13.6 (user input) | T | P | (position from user input) J-Ks=0.884+/-0.030 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:41.38 +41:37:13.6: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:41.38 +41:37:13.6: 14.56 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.38 21:33:09.40 +37:05:57.4
84.77423 -10.67848 galactic Cyg Second-epoch detections are separated by 2.7" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:33:09.40 +37:05:57.4 (user input) | T | P | (position from user input) J-Ks=0.473+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:09.40 +37:05:57.4: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:09.40 +37:05:57.4: 15.08 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.39 21:38:56.80 +37:31:13.6
85.92396 -11.15636 galactic Cyg Second-epoch detections are separated by 2.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.7367+37.5110 | 21:38:56.80 +37:31:13.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.788+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:56.80 +37:31:13.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:56.80 +37:31:13.6: 14.85 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.7367+37.5110,2461172.8579,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.7367+37.5110 20260512.3579 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.3579 2461172.8579 12.35 21:34:40.41 +37:53:56.9
85.55543 -10.30397 galactic Cyg Second-epoch detections are separated by 2.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:40.41 +37:53:56.9 (user input) | T | P | (position from user input) J-Ks=0.608+/-0.057 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:40.41 +37:53:56.9: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:40.41 +37:53:56.9: 14.95 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461172.8579,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260512.3579 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
First image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Last image: 2461172.85814611 12.05.2026 08:35:33.824 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 24
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 10 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 20198
Objects passed selection criteria: 20193
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 19235.8
Average stars matched: 17071.5 (88.7488 %)
Memory usage VmPeak: 126280 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 12 04:31:55 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
First image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Last image: 2461172.85814611 12.05.2026 08:35:33.824 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 644
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 222 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 138952
Objects passed selection criteria: 138682
Measurements per detected object (mean, median, min, max): 3.3 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 3.0 2 4
Average stars detected per image: 131615
Average stars matched: 118736 (90.2152 %)
Memory usage VmPeak: 1978216 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 12 04:37:34 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461172.85766941
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
Entering WCS image calibration mode.
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Entering WCS image calibration mode.
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Entering WCS image calibration mode.
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits was not set. Trying to guess...
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
The guess is 605 arcmin.
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits was not set. Trying to guess...
The guess is 605 arcmin.
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits .... Determining astrometry method...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits was not set. Trying to guess...
The guess is 572 arcmin.
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits has a WCS header - will blindly trust it is good...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/lib/make_outxyls_for_astrometric_calibration found 22215 high-SNR stars for plate solving
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/lib/make_outxyls_for_astrometric_calibration found 22198 high-SNR stars for plate solving
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits' -> 'wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits was not set. Trying to guess...
Generating wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat from image00001.cat
The guess is 570 arcmin.
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
verification OK: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Generating wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat from image00002.cat
Catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits created.
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits created.
verification OK: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
verification OK: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Image size: 932.3'x637.3' 15.5(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.99"/pix along the Y axis
Image center: 21:48:57.820 +38:02:09.57 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out2571067.xyls"...
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:06.050 +38:00:21.02 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 28429 stars ###
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out2571071.xyls"...
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/correct_sextractor_wcs_catalog_usingxy2sky2571481.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
### Converted positions of 21746 stars ###
'wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/correct_sextractor_wcs_catalog_usingxy2sky2571480.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2571067.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Reading file "./out2571071.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
log-odds ratio 35.0077 (1.59823e+15), 9 match, 0 conflict, 28 distractors, 94 index.
RA,Dec = (327.223,38.0517), pixel scale 5.90819 arcsec/pix.
Hit/miss: Hit/miss: +----+--+-------+---+---+---+---+---+(best)-------------------+--------+--+-------------------+-----------
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1: solved with index index-4114.fits.
Field 1 solved: writing to file ./out2571067.solved to indicate this.
Field: out2571067.xyls
Field center: (RA,Dec) = (327.281055, 38.043158) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:07.453, +38:02:35.367).
Field size: 15.7339 x 10.5311 degrees
Field rotation angle: up is -0.844763 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits' -> 'fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits'
Field 1 did not solve (index index-4115.fits, field objects 1-10).
log-odds ratio 26.7131 (3.99331e+11), 6 match, 0 conflict, 19 distractors, 94 index.
RA,Dec = (327.218,38.0487), pixel scale 5.90825 arcsec/pix.
Hit/miss: Hit/miss: +----+--+-------+---+---+(best)---+-------+-------+-----------+--------+--+-------------------+-----------
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 12 04:31 fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
-rw-r--r-- 1 apache apache 12K May 12 04:31 out2571067.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits for reading... done!
Creating new image file (wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits)... done!
Field 1: solved with index index-4114.fits.
Field 1 solved: writing to file ./out2571071.solved to indicate this.
Field: out2571071.xyls
Field center: (RA,Dec) = (327.276891, 38.040464) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:06.454, +38:02:25.670).
Field size: 15.7338 x 10.531 degrees
Field rotation angle: up is -0.841402 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits' -> 'fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits'
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 12 04:31 fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
-rw-r--r-- 1 apache apache 12K May 12 04:31 out2571071.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits for reading... done!
Creating new image file (wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits)... done!
done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits (fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits (fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out2571067.xyls"...
Reading input file 1 of 1: "out2571071.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2571067.axy"...
Only searching for solutions within 15.6633 degrees of RA,Dec (327.282,38.044)
log-odds ratio 32.9557 (2.0535e+14), 7 match, 0 conflict, 34 distractors, 23 index.
RA,Dec = (327.272,38.0456), pixel scale 5.95693 arcsec/pix.
Hit/miss: Hit/miss: -+-----++-+-----------------+-----+-----+(best)---------------+-------------------------------------------
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2571071.axy"...
Only searching for solutions within 15.6633 degrees of RA,Dec (327.278,38.0413)
log-odds ratio 32.7457 (1.66451e+14), 7 match, 0 conflict, 34 distractors, 23 index.
RA,Dec = (327.268,38.043), pixel scale 5.95681 arcsec/pix.
Hit/miss: Hit/miss: -+----++--+---------------+-------+-----+(best)---------------+-------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2571067.solved to indicate this.
Field 1 solved: writing to file ./out2571071.solved to indicate this.
Field: out2571067.xyls
Field: out2571071.xyls
Field center: (RA,Dec) = (327.279945, 38.040913) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:07.187, +38:02:27.288).
Field size: 15.7147 x 10.5377 degrees
Field rotation angle: up is -0.85918 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 12 04:31 fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
-rw-r--r-- 1 apache apache 12K May 12 04:31 out2571071.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits for reading... done!
Creating new image file (wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits)... done!
done!
Field center: (RA,Dec) = (327.284059, 38.043653) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:08.174, +38:02:37.152).
Field size: 15.7148 x 10.5378 degrees
Field rotation angle: up is -0.861645 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 12 04:31 fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
-rw-r--r-- 1 apache apache 12K May 12 04:31 out2571067.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits for reading... done!
Creating new image file (wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 100000 sources.
simplexy: found 100000 sources.
Solving...
Reading file "./wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.axy"...
Verifying WCS using indices with quads of size [63.5068, 952.006] arcmin
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 8.02246
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 19.6686
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 79.9702 (5.37786e+34), 20 match, 0 conflict, 168 distractors, 49 index.
RA,Dec = (327.279,38.0401), pixel scale 5.96495 arcsec/pix.
Hit/miss: Hit/miss: -+--+-------+---+-----------+-----+----------+--------------+----+-+--------+---+--+----------------
--> log-odds 79.9702
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 375.184 (8.71214e+162), 51 match, 0 conflict, 248 distractors, 97 index.
RA,Dec = (327.279,38.0401), pixel scale 5.96495 arcsec/pix.
Hit/miss: Hit/miss: -+--+--++---+++-++-++--+----+-----++---+----++-------------++---++-+------+++---+--+----------------
--> log-odds 375.184
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 843.721 (inf), 104 match, 0 conflict, 305 distractors, 194 index.
RA,Dec = (327.279,38.0401), pixel scale 5.96495 arcsec/pix.
Hit/miss: Hit/miss: -+-++++++---+++-+++++--+----+---+-++++-++---++++++++------+++-+--+++------+++++-+--+---+-+++----+---
--> log-odds 843.721
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 1762.38 (inf), 206 match, 0 conflict, 234 distractors, 375 index.
RA,Dec = (327.279,38.0401), pixel scale 5.96495 arcsec/pix.
Hit/miss: Hit/miss: +++++++++-+++++++++++-++++-++---+++++++++++-+++++++++-++--+++++-++++-+-+--+++++-+-++-+-+-++++---+-++
--> log-odds 1762.38
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 3112.15 (inf), 378 match, 0 conflict, 227 distractors, 730 index.
RA,Dec = (327.279,38.0401), pixel scale 5.96495 arcsec/pix.
Hit/miss: Hit/miss: +++++++++++++++++++++-+++++++++++++++++++++++++++++++++++-++++++++++++++++++++++++++++++++++++-+++++
Solving...
Reading file "./wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.axy"...
Verifying WCS using indices with quads of size [63.5059, 951.991] arcmin
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
--> log-odds 3112.15
Verifying WCS of field 1.
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 5801.87 (inf), 777 match, 0 conflict, 607 distractors, 1449 index.
RA,Dec = (327.279,38.0401), pixel scale 5.96495 arcsec/pix.
Hit/miss: Hit/miss: ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
--> log-odds 14.554
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 110.222 (7.39202e+47), 25 match, 0 conflict, 244 distractors, 49 index.
RA,Dec = (327.283,38.0428), pixel scale 5.96486 arcsec/pix.
Hit/miss: Hit/miss: --++--+---+-------+-----+-+------+---+------+-------------+---------+------++-----------------------
--> log-odds 110.222
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 375.834 (1.66919e+163), 52 match, 0 conflict, 280 distractors, 97 index.
RA,Dec = (327.283,38.0428), pixel scale 5.96486 arcsec/pix.
Hit/miss: Hit/miss: --+++-+---+-----+-+-+-+-+-++--+--+--++----+-+-------------+++----+--+-----+++---+++-----------------
--> log-odds 375.834
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 704.264 (7.20863e+305), 90 match, 0 conflict, 255 distractors, 194 index.
RA,Dec = (327.283,38.0428), pixel scale 5.96486 arcsec/pix.
Hit/miss: Hit/miss: -++++-+-+-+-+---+-+-+-+-+-+++-+--+++++----+-+--+---+--+---+++----+--+--+-++++-+--++-----+--+++------
--> log-odds 5801.87
Got 6 solutions.
Field: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
Field center: (RA,Dec) = (327.279161, 38.040530) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:06.999, +38:02:25.909).
Field size: 15.7182 x 10.5337 degrees
Field rotation angle: up is -0.842172 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.new"...
--> log-odds 704.264
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 1606.58 (inf), 188 match, 0 conflict, 194 distractors, 375 index.
RA,Dec = (327.283,38.0428), pixel scale 5.96486 arcsec/pix.
Hit/miss: Hit/miss: +++++-+++++-+++++-+++-+-+-++++++++++++--+++++-++-+-++-+---+++++--++-+--+-++++++-+++++++-+--+++++--+-
--> log-odds 1606.58
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 2957.91 (inf), 363 match, 0 conflict, 293 distractors, 730 index.
RA,Dec = (327.283,38.0428), pixel scale 5.96486 arcsec/pix.
Hit/miss: Hit/miss: +++++++++++-++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
renamed 'wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.new' -> 'wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits'
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
Generating wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat from image00004.cat
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits created.
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
--> log-odds 2957.91
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 5551.94 (inf), 751 match, 0 conflict, 674 distractors, 1448 index.
RA,Dec = (327.283,38.0428), pixel scale 5.96486 arcsec/pix.
Hit/miss: Hit/miss: ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
Image size: 937.9'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:07.247 +38:02:28.93 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 23785 stars ###
'wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/correct_sextractor_wcs_catalog_usingxy2sky2580471.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
--> log-odds 5551.94
Got 6 solutions.
Field: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
Field center: (RA,Dec) = (327.283381, 38.043218) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:08.012, +38:02:35.584).
Field size: 15.7184 x 10.5338 degrees
Field rotation angle: up is -0.845912 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.new"...
renamed 'wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.new' -> 'wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits'
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
Generating wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat from image00003.cat
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits created.
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
Image size: 937.9'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:08.260 +38:02:38.61 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 23640 stars ###
'wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/correct_sextractor_wcs_catalog_usingxy2sky2580623.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits (1st reference image)
verification OK: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Image size: 932.3'x637.3' 15.5(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.99"/pix along the Y axis
Image center: 21:48:57.820 +38:02:09.57 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits (1st new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
Image size: 937.9'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:08.260 +38:02:38.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:48:57.820 +38:02:09.57
Second-epoch image center 21:49:08.260 +38:02:38.61
Angular distance between the image centers 0.0352 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits (2nd new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
Image size: 937.9'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:07.247 +38:02:28.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:48:57.820 +38:02:09.57
Second-epoch image center 21:49:07.247 +38:02:28.93
Angular distance between the image centers 0.0314 deg.
###################################
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits sigma_overall=N/A worst_q_ratio=N/A
ref2=wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits sigma_overall=N/A worst_q_ratio=N/A
new1=wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits sigma_overall=N/A worst_q_ratio=N/A
new2=wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits sigma_overall=N/A worst_q_ratio=N/A
reference average sigma_overall=N/A worst_q_ratio=N/A
warn-on-ratio threshold: 2.0x reference
###################################
INFO: WCS quality sigma_overall_arcsec not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality sigma_overall_arcsec not available for comparison (2nd new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (2nd new image new=N/A ref_avg=N/A)
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:49:08.260 +38:02:38.61
Second-epoch second image center 21:49:07.247 +38:02:28.93
Angular distance between the image centers 0.00428 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits &> /tmp/tmp.r8UBTvnBH2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits &> /tmp/tmp.EQc9cmpucg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits &> /tmp/tmp.WXqUKGwZ6i
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits &> /tmp/tmp.PZODImamxW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
The reference image (wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits) and catalog (wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat) found
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Read 28429 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8517 to 337.9501 deg, Dec +32.2173 to +43.3775 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.8517 to 337.9501 deg, Dec 32.2173 to 43.3775 deg
Loaded 21151 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 23 out of 30 total matches.
Matched with Tycho-2 30 out of 28429 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.968900
a=0.000000 b=1.000000 c=22.968900
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 28429 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8517 to 337.9501 deg, Dec +32.2173 to +43.3775 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.8517 to 337.9501 deg, Dec 32.2173 to 43.3775 deg
Loaded 21151 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 23 out of 30 total matches.
Matched with Tycho-2 30 out of 28429 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits:
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits (aperture=6.2)
Read 21746 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.5217 to 337.7622 deg, Dec +32.2988 to +43.2789 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.5217 to 337.7622 deg, Dec 32.2988 to 43.2789 deg
Loaded 21125 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 13298 out of 14228 total matches.
Matched with Tycho-2 14228 out of 21746 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits:
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits (aperture=7.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.9 pix Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
2.6 pix fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
2.6 pix fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
2.2 pix wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.9 pix wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Limiting magnitude estimates:
15.2 mag. Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
14.7 mag. Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
14.9 mag. fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
14.9 mag. fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.r8UBTvnBH2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2960, passed=28429
Got 28429 stars (including 25433 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 28429 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.3'
Seting catalog search parameters based on the expected field of view 932.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012949 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010359 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.4)
Done reading UCAC5 zone files...
Matched 424 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 377 matched stars entering correct_measured_positions(), 326 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 373 matched stars entering correct_measured_positions(), 11634 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.4)
Done reading UCAC5 zone files...
Matched 495 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 453 matched stars entering correct_measured_positions(), 11686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.41"
Accuracy estimation diagnostic: 452 matched stars entering correct_measured_positions(), 13987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.48"
Excluding outliers - 452 stars left (next iteration limit 410)
WCS_QUALITY_DIAG: file=Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits N_match=452 sigma_overall_arcsec=5.245 sigma_q1_arcsec=26.359 sigma_q2_arcsec=5.045 sigma_q3_arcsec=33.611 sigma_q4_arcsec=3.580 n_q1=17 n_q2=196 n_q3=13 n_q4=226 worst_quadrant_to_overall_ratio=6.408
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -region wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.EQc9cmpucg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits' -> 'wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1940, passed=21746
Got 21746 stars (including 19798 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat
util/solve_plate_with_UCAC5 got 21746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits N_match=958 sigma_overall_arcsec=0.836 sigma_q1_arcsec=0.742 sigma_q2_arcsec=0.917 sigma_q3_arcsec=0.784 sigma_q4_arcsec=1.358 n_q1=279 n_q2=165 n_q3=306 n_q4=208 worst_quadrant_to_overall_ratio=1.625
The image catalog is written to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits -region wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WXqUKGwZ6i (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1920, passed=23640
Got 23640 stars (including 21694 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat
util/solve_plate_with_UCAC5 got 23640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010421 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 23261 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 23263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 23263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits N_match=961 sigma_overall_arcsec=0.577 sigma_q1_arcsec=0.539 sigma_q2_arcsec=0.541 sigma_q3_arcsec=0.537 sigma_q4_arcsec=0.670 n_q1=225 n_q2=216 n_q3=286 n_q4=234 worst_quadrant_to_overall_ratio=1.161
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PZODImamxW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1918, passed=23785
Got 23785 stars (including 21850 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat
util/solve_plate_with_UCAC5 got 23785 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010421 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 23456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 23456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 23456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits N_match=960 sigma_overall_arcsec=0.587 sigma_q1_arcsec=0.496 sigma_q2_arcsec=0.626 sigma_q3_arcsec=0.537 sigma_q4_arcsec=0.678 n_q1=229 n_q2=215 n_q3=285 n_q4=231 worst_quadrant_to_overall_ratio=1.154
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-34-52_20.00sec_-5.00C_LIGHT_0344.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-12_CI_Cyg-07-Q2b1x1_034709_TTUQ2b1x1_1891922_fGzHoiPc/wcs_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345.fits'
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:01.87 +37:32:45.4: 14.87 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:47.54 +37:36:36.6: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:34.06 +39:25:50.2: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:02.61 +35:24:01.7: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:08.41 +38:04:10.6: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:16.27 +38:10:28.1: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:15.68 +37:46:30.9: 13.53 +/- 0.05 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:12.97 +34:04:37.4: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:28.02 +37:51:53.2: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:26.59 +37:53:17.2: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:01.87 +37:32:45.4: 12.13 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:47.54 +37:36:36.6: 12.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.02
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:02.61 +35:24:01.7: 12.24 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 21:46:01.87 +37:32:45.4: ref_mag=12.17 +/- 0.02 new_mean_mag=12.1530 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:56:47.54 +37:36:36.6: ref_mag=12.18 +/- 0.02 new_mean_mag=12.0384 delta=0.14 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:34.06 +39:25:50.2: 12.16 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:08.41 +38:04:10.6: 12.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:12.97 +34:04:37.4: 11.93 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:15.68 +37:46:30.9: 11.77 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 21:57:02.61 +35:24:01.7: ref_mag=12.24 +/- 0.02 new_mean_mag=12.1893 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Forced photometry reference-image weighted average: 12.02 +/- 0.02
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:16.27 +38:10:28.1: 12.18 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 21:50:34.06 +39:25:50.2: ref_mag=12.16 +/- 0.02 new_mean_mag=12.1351 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:40:08.41 +38:04:10.6: ref_mag=12.02 +/- 0.02 new_mean_mag=12.0674 delta=-0.05 (need > 0.90)
Forced photometry reference-image weighted average: 11.93 +/- 0.02
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter REJECTED candidate at 21:49:12.97 +34:04:37.4: ref_mag=11.93 +/- 0.02 new_mean_mag=12.1164 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:33:15.68 +37:46:30.9: ref_mag=11.90 +/- 0.01 new_mean_mag=12.1916 delta=-0.29 (need > 0.90)
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Forced photometry filter REJECTED candidate at 21:44:16.27 +38:10:28.1: ref_mag=12.18 +/- 0.02 new_mean_mag=12.2059 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:28.02 +37:51:53.2: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Forced photometry filter REJECTED candidate at 21:51:28.02 +37:51:53.2: ref_mag=12.25 +/- 0.02 new_mean_mag=12.2027 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:26.59 +37:53:17.2: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Forced photometry filter REJECTED candidate at 22:03:26.59 +37:53:17.2: ref_mag=12.38 +/- 0.02 new_mean_mag=12.2251 delta=0.16 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:24.02 +39:33:21.6: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:38.72 +38:55:22.5: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:52.39 +36:25:34.1: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:27.60 +40:44:01.2: 15.17 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:50.94 +36:42:27.6: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:06.41 +34:09:02.4: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:01.06 +34:19:09.6: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:00.29 +37:21:59.1: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:03.48 +37:37:18.4: 15.60 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:15.78 +35:14:24.2: 13.23 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:24.02 +39:33:21.6: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Forced photometry filter REJECTED candidate at 21:44:24.02 +39:33:21.6: ref_mag=12.16 +/- 0.02 new_mean_mag=12.2138 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:52.39 +36:25:34.1: 11.51 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:50.94 +36:42:27.6: 12.33 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:27.60 +40:44:01.2: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.01
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:01.06 +34:19:09.6: 12.53 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:38.72 +38:55:22.5: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Forced photometry filter REJECTED candidate at 21:54:52.39 +36:25:34.1: ref_mag=11.51 +/- 0.01 new_mean_mag=12.2166 delta=-0.71 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:00.29 +37:21:59.1: 12.34 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 21:54:50.94 +36:42:27.6: ref_mag=12.33 +/- 0.02 new_mean_mag=12.2786 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:06.41 +34:09:02.4: 12.41 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 21:44:27.60 +40:44:01.2: ref_mag=12.28 +/- 0.02 new_mean_mag=12.2303 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 12.53 +/- 0.03
Forced photometry reference-image weighted average: 12.29 +/- 0.02
Forced photometry reference-image weighted average: 12.34 +/- 0.02
Forced photometry filter REJECTED candidate at 21:58:38.72 +38:55:22.5: ref_mag=12.29 +/- 0.02 new_mean_mag=12.2153 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:05:01.06 +34:19:09.6: ref_mag=12.53 +/- 0.03 new_mean_mag=12.3058 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:53:00.29 +37:21:59.1: ref_mag=12.34 +/- 0.02 new_mean_mag=12.2346 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.41 +/- 0.02
Forced photometry filter REJECTED candidate at 21:53:06.41 +34:09:02.4: ref_mag=12.41 +/- 0.02 new_mean_mag=12.3115 delta=0.10 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:03.48 +37:37:18.4: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.02
Forced photometry filter REJECTED candidate at 21:50:03.48 +37:37:18.4: ref_mag=12.34 +/- 0.02 new_mean_mag=12.2876 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:15.78 +35:14:24.2: 12.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter REJECTED candidate at 22:09:15.78 +35:14:24.2: ref_mag=12.85 +/- 0.02 new_mean_mag=12.3145 delta=0.53 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:20.26 +35:38:42.6: 14.57 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:20.26 +35:38:42.6: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Forced photometry filter REJECTED candidate at 21:52:20.26 +35:38:42.6: ref_mag=12.52 +/- 0.02 new_mean_mag=12.3138 delta=0.20 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 37882_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37882_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37930_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37930_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:01:54.10 +36:57:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37943_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37943_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37946_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37946_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37954_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37954_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37960_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37960_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37961_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37961_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37966_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37966_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37968_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37968_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:41:12.72 +37:03:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37973_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37973_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37976_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37976_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37979_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37979_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37982_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37982_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37986_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37986_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37987_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37987_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37988_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37988_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37991_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37991_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 37996_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 37996_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 38000_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 38000_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 38001_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 38001_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 38007_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 38007_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 38012_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 38012_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 38016_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 38016_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 253004_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253004_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 253009_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253009_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253011_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253011_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253012_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253012_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253023_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253023_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253025_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253025_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253027_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253027_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253033_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253033_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253046_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253046_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253050_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253050_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253052_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253052_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 253053_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253053_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253055_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253055_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253057_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253057_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253058_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253058_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253065_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253065_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 253072_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253072_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253081_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253081_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253084_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253084_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253095_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253095_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253103_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253103_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253105_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253105_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253110_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253110_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 253117_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253117_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253125_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253125_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253133_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253133_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253135_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253135_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253136_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253136_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253140_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253140_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253153_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253153_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 253158_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253158_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 253169_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253169_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253194_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253194_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 253198_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253198_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 253201_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253201_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 253207_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253207_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253213_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253213_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253226_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253226_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253232_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253232_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253239_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253239_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253248_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253248_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 253253_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253253_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253262_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253262_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253264_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253264_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253268_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253268_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253273_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253273_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253281_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253281_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253283_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253283_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253291_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253291_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253302_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253302_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253308_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253308_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253313_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253313_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253345_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253345_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253346_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253346_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253348_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253348_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253351_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253351_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253373_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253373_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253376_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253376_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253387_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253387_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253393_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253393_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253397_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253397_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253410_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253410_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253413_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253413_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253423_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253423_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253438_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253438_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253439_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253439_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253448_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253448_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253449_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253449_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253478_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253478_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253491_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253491_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253525_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253525_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253575_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253575_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253606_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253606_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253612_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253612_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253613_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253613_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:10:36.31 +41:28:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253628_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253628_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253641_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253641_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253652_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253652_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:01:57.40 +35:42:31.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253657_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253657_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253672_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253672_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253685_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253685_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253711_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253711_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253724_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253724_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253740_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253740_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:59:46.44 +39:52:42.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253753_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253753_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253785_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253785_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:33:21.52 +38:02:44.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253786_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253786_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253804_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253804_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253814_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253814_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253825_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253825_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253828_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253828_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253839_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253839_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253847_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253847_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253849_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253849_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253850_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253850_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253851_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253851_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:05:08.07 +36:40:56.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253886_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253886_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253891_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253891_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253897_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 253897_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253907_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253907_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:01:07.98 +39:15:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253912_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253912_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253932_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253932_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253967_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253967_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253972_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253972_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253992_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 253992_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254015_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254015_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:56:49.76 +42:13:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254019_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254019_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254053_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254053_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254075_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254075_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:56:37.87 +37:20:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254076_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254076_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 254084_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254084_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:10:04.65 +41:24:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254085_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254085_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 254103_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254103_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 254110_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254110_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:08:09.94 +37:08:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254120_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254120_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254153_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254153_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254159_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254159_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 254161_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254161_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:57:40.54 +37:18:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254171_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254171_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:58:07.70 +38:56:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254186_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254186_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254200_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254200_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 254208_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254208_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254216_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254216_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 254236_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254236_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254237_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254237_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:01:53.26 +40:17:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254239_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254239_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 254240_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254240_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:06:46.57 +39:39:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254241_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254241_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 254255_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254255_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:42:46.47 +37:59:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254262_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254262_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:04:54.88 +37:38:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254263_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254263_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 254268_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254268_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:00:54.53 +41:16:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254270_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254270_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254273_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254273_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:05:15.55 +37:31:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254284_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254284_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 254286_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254286_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 254328_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254328_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:49:54.68 +34:54:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254329_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254329_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:50:52.32 +39:37:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254344_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254344_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 254351_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254351_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 254358_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254358_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254363_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254363_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 254365_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254365_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:09:21.07 +33:46:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254369_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254369_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:47:01.50 +35:15:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254373_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254373_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 254383_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254383_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:54:04.41 +37:39:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254390_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254390_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 254401_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254401_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:51:54.95 +33:54:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254408_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254408_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254413_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254413_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:59:59.45 +37:35:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254426_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254426_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254429_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254429_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 254431_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254431_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:49:54.42 +37:45:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254436_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254436_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 254437_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254437_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:09:23.77 +40:29:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254450_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254450_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254455_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254455_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:02:27.78 +42:04:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254466_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254466_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:55:07.28 +37:29:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254481_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254481_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 254482_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254482_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 254486_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254486_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:44:49.55 +35:31:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254503_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254503_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 254506_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254506_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254510_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254510_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 254514_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254514_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254520_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254520_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:55:01.61 +42:15:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254524_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254524_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 254537_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254537_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254549_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254549_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:58:13.61 +38:26:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254553_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254553_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254558_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254558_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 254567_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254567_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 254570_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254570_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 254571_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254571_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:59:00.17 +41:56:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254586_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254586_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 254589_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254589_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:49:18.25 +39:21:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254598_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254598_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254599_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254599_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 254605_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254605_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254626_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254626_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 254629_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254629_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 254645_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254645_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254652_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254652_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:00:00.03 +38:42:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254653_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254653_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254664_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254664_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254673_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254673_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:04:36.84 +38:54:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254674_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254674_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254681_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254681_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 254685_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254685_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 254695_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254695_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254754_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254754_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 254769_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254769_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 254770_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254770_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254791_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254791_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254794_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254794_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254801_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254801_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254806_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254806_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254809_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254809_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254812_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 254812_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:43:03.27 +37:32:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254855_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254855_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254879_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254879_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254893_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254893_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254905_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254905_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254948_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254948_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254998_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 254998_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255008_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 255008_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 255018_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255018_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255051_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255051_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255080_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255080_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255108_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255108_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255134_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255134_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255143_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 255143_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 255160_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 255160_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 255179_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255179_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255194_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255194_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255206_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255206_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255223_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255223_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255235_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 255235_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:41:50.95 +35:55:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255249_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 255249_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:46:08.76 +35:33:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255260_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255260_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255274_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255274_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255393_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255393_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255412_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255412_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255475_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255475_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255520_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255520_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 255524_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255524_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255528_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255528_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255536_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255536_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255541_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255541_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255567_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 255567_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 255575_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 255575_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 22:02:25.84 +38:25:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255609_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255609_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255747_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255747_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 255789_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255789_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 255852_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 255852_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 255865_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255865_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 255882_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255882_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255908_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255908_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 255909_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 255909_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 255918_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 255918_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 255919_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 255919_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 255976_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 255976_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256003_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256003_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256047_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256047_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256057_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 256057_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 256087_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256087_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256139_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256139_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256150_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256150_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256159_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256159_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256174_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256174_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256268_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256268_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256298_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256298_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256323_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256323_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256331_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256331_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256333_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256333_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256391_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 256391_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 256403_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256403_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256457_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256457_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256486_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256486_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256561_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256561_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256576_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256576_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256587_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 256587_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
**** FOUND 21:46:28.74 +39:28:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256599_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256599_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256606_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256606_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256612_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256612_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256654_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 256654_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 256684_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 256684_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 256692_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 256692_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 256698_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256698_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256777_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256777_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256781_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256781_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256783_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 256783_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 256804_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256804_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256817_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256817_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256820_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256820_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256833_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256833_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256836_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256836_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256852_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 256852_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 256857_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256857_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256866_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 256866_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 256873_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256873_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256876_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256876_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256891_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256891_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256938_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256938_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256963_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256963_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256976_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256976_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256983_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256983_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256988_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256988_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 256991_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256991_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256992_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 256992_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257000_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257000_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257024_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257024_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 257031_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257031_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257065_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257065_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257092_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257092_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 257099_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257099_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 257110_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257110_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257118_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257118_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257132_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257132_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257141_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257141_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257146_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257146_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257153_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257153_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257157_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257157_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257162_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257162_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257166_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257166_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257180_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257180_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257184_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257184_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257189_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257189_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257228_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257228_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257230_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257230_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257241_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257241_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257249_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257249_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257256_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257256_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257278_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257278_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257304_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257304_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257306_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257306_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257327_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257327_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257335_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257335_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257338_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257338_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257344_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257344_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257360_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257360_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257363_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257363_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257365_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257365_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257373_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257373_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257375_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257375_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257377_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257377_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257389_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257389_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 257391_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257391_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257431_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257431_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257438_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257438_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 257439_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257439_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257443_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257443_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257446_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257446_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257449_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257449_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257454_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257454_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257455_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257455_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257459_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257459_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257465_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257465_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257471_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257471_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257476_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257476_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257481_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257481_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257512_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257512_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257514_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257514_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257533_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257533_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257536_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257536_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257542_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257542_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257545_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257545_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 257548_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257548_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257556_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257556_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257576_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257576_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257581_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257581_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257592_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257592_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257611_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257611_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 257618_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257618_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257623_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257623_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257631_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257631_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257642_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257642_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257645_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257645_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257650_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257650_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 257662_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257662_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257664_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257664_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 257666_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257666_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257701_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257701_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257709_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257709_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 257711_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257711_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 257718_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257718_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257727_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257727_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257756_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257756_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257760_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257760_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257765_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257765_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257770_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257770_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257774_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257774_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257778_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257778_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 257792_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257792_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257798_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257798_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 257800_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257800_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257822_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257822_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257831_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257831_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257833_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257833_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257834_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257834_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257837_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257837_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257841_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257841_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257844_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257844_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257845_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257845_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257849_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257849_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257852_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257852_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257856_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257856_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257871_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257871_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257872_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257872_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257886_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257886_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257889_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257889_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257895_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257895_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257898_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257898_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257901_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257901_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 257911_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257911_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257912_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257912_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257931_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257931_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257932_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257932_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257933_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257933_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257939_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257939_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257942_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257942_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257946_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257946_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257960_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257960_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257962_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257962_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257967_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 257967_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257976_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257976_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257977_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257977_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257987_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257987_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257990_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257990_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257992_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 257992_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258008_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258008_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258010_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 258010_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258012_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258012_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258013_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258013_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258016_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258016_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258030_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258030_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258033_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258033_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258034_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258034_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258045_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258045_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258051_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258051_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258053_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258053_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258071_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258071_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258086_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258086_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258108_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258108_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258113_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258113_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258119_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258119_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258120_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258120_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258137_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 258137_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258143_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258143_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258164_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258164_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258166_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258166_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258171_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258171_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258188_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258188_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258195_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258195_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258196_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258196_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258204_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258204_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258206_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258206_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258221_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258221_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258223_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258223_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258230_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258230_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258233_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258233_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258235_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258235_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258242_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258242_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258243_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258243_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258244_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258244_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258248_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258248_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258251_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258251_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258253_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258253_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258256_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258256_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258265_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258265_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258267_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258267_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258272_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258272_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258275_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 258275_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 258283_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258283_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258286_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 258286_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 258292_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258292_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258294_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258294_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258300_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258300_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258306_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258306_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258328_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258328_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258333_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258333_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258345_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258345_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258358_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258358_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258370_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258370_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258375_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258375_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258376_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258376_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258412_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258412_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258415_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258415_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258419_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258419_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258424_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258424_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258428_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258428_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258446_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 258446_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 258449_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258449_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258450_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258450_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258452_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258452_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258453_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258453_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258457_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258457_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258467_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258467_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258481_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258481_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258485_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 258485_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 258488_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258488_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258493_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258493_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258511_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258511_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258532_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258532_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258543_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258543_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258551_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258551_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258569_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258569_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258575_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258575_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258580_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258580_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258581_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258581_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258584_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258584_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258594_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258594_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258604_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 258604_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 258610_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 258610_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
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Considering the candidate 258620_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258620_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258622_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258622_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258629_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258629_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258633_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258633_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258636_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258636_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258637_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258637_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258660_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258660_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258683_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258683_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258685_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258685_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 258776_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
Preparing report for the candidate 258776_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
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Considering the candidate 97092_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345
The candidate 97092_fd_Cyg-07-Q2b1x1_2026-05-12_03-35-33_20.00sec_-5.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 40s
make_report_in_HTML.sh TOTAL: 1065s
Prepared the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:59:12.69 +42:08:23.3
21:56:43.44 +37:32:19.1
21:41:34.32 +34:36:23.6
21:42:11.57 +36:19:08.9
22:02:54.20 +40:44:54.5
21:48:53.93 +36:09:36.7
21:37:06.39 +33:54:16.9
21:38:16.22 +34:33:06.6
21:48:57.03 +38:28:35.1
21:50:40.99 +39:31:45.3
21:32:45.94 +37:06:19.5
22:10:18.73 +41:32:58.6
21:59:20.80 +39:40:39.1
21:55:29.67 +36:36:05.8
21:56:43.41 +41:51:09.7
21:40:11.20 +37:48:07.1
22:03:12.09 +37:15:34.4
21:54:14.01 +35:39:31.5
21:55:25.02 +39:42:15.4
21:35:34.81 +41:02:12.4
21:40:22.44 +39:00:37.6
22:01:48.31 +39:56:08.6
21:50:17.67 +42:04:59.5
21:31:25.66 +35:04:07.5
21:48:34.08 +42:19:14.2
21:29:26.32 +37:55:02.9
21:51:41.33 +39:11:41.9
22:06:06.12 +38:12:56.7
21:51:41.89 +34:07:05.8
22:02:38.66 +37:44:29.0
21:36:58.24 +37:51:38.0
22:06:54.87 +41:38:25.6
22:02:56.21 +40:46:06.2
21:43:44.26 +34:49:10.4
22:07:48.88 +34:48:04.2
22:08:33.12 +35:58:49.2
22:10:57.06 +37:02:42.5
21:50:25.14 +38:28:30.2
22:09:56.44 +39:05:40.5
21:44:37.46 +38:02:18.1
21:57:31.30 +38:48:29.4
22:02:38.78 +37:13:44.8
22:09:04.27 +36:22:36.8
22:09:49.48 +37:06:45.4
21:40:15.55 +37:50:21.5
21:45:03.10 +36:40:08.6
22:07:19.75 +40:15:15.6
21:52:04.60 +34:41:09.5
21:55:46.12 +35:47:06.6
22:05:32.42 +38:58:34.1
21:48:31.26 +41:08:43.0
21:53:31.13 +33:46:50.1
21:58:49.48 +40:53:49.1
21:42:14.31 +37:22:59.4
21:53:53.60 +41:17:52.3
21:43:02.43 +34:00:50.1
22:00:24.41 +39:57:07.7
21:56:29.02 +37:56:47.0
21:55:57.26 +40:10:25.0
21:29:16.58 +34:43:05.5
21:44:03.16 +37:47:35.8
21:39:53.76 +37:58:52.8
21:53:17.50 +41:45:59.3
21:55:39.50 +36:53:22.5
22:10:45.32 +40:14:53.9
22:09:47.58 +36:16:45.8
21:26:12.88 +41:49:13.0
21:40:12.45 +37:22:52.0
21:40:43.80 +37:23:00.4
21:57:14.44 +42:01:04.2
21:30:55.05 +34:30:59.6
22:02:05.96 +36:06:27.4
21:26:50.52 +37:00:11.8
22:02:11.35 +35:32:42.6
22:05:39.86 +34:53:39.2
21:59:59.27 +36:08:34.1
21:59:20.92 +36:56:49.6
21:44:09.56 +37:55:03.4
21:28:09.20 +41:14:36.6
21:33:13.75 +37:12:43.5
21:30:32.04 +35:46:44.8
22:06:01.48 +39:10:17.5
21:28:11.90 +34:45:26.3
21:59:06.37 +34:00:18.2
22:01:18.73 +41:30:28.0
22:01:14.46 +38:33:47.2
22:04:54.79 +40:37:24.8
22:02:13.89 +41:47:07.9
21:40:41.03 +36:19:20.7
22:02:14.84 +34:37:08.9
22:02:42.09 +37:09:00.8
22:00:24.20 +35:58:54.0
22:02:42.59 +41:44:10.6
22:06:31.88 +34:33:33.2
21:47:33.64 +37:22:56.1
21:58:18.40 +39:26:01.3
22:02:04.56 +37:45:27.6
22:07:43.40 +37:37:06.9
21:48:57.90 +37:42:53.1
21:51:57.54 +37:11:56.1
21:49:41.28 +37:43:30.9
22:10:20.04 +38:44:22.5
22:04:54.72 +35:49:32.8
22:09:33.60 +41:54:58.6
21:29:32.26 +33:48:21.6
21:38:38.20 +33:58:31.1
22:05:42.75 +35:53:01.4
22:11:12.63 +37:18:42.5
21:59:28.80 +37:59:47.4
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21:59:01.83 +36:26:59.1
22:06:38.32 +41:43:55.3
21:58:43.07 +42:11:58.0
21:56:29.21 +36:52:35.9
22:00:26.18 +37:37:17.9
21:57:23.01 +41:48:54.3
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21:56:00.49 +37:10:56.8
21:36:48.58 +38:51:42.1
21:27:10.32 +36:53:17.9
21:50:34.31 +37:11:03.4
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21:49:23.30 +36:27:43.5
21:48:46.74 +35:26:23.2
22:01:12.15 +35:17:06.7
21:50:58.71 +36:44:36.8
21:39:40.89 +34:24:59.7
21:50:58.46 +39:25:04.2
21:57:10.69 +42:10:42.9
21:54:38.63 +36:53:54.3
21:46:54.19 +39:15:20.8
21:46:14.75 +37:25:08.7
21:29:56.13 +35:08:34.3
21:42:07.42 +39:04:10.8
22:06:12.38 +39:36:05.5
21:51:11.60 +37:00:46.2
21:56:34.45 +37:00:27.0
21:48:07.30 +36:02:35.7
21:57:57.47 +34:05:54.2
22:04:30.42 +41:26:44.9
21:42:33.76 +41:45:51.2
21:50:44.43 +36:27:35.9
21:35:27.29 +35:03:48.3
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21:48:57.14 +34:21:32.4
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21:50:31.56 +38:39:10.8
21:27:00.73 +33:45:03.0
21:27:07.35 +35:14:57.5
21:55:36.26 +35:51:33.8
21:42:31.24 +35:51:14.2
21:31:26.82 +33:46:07.4
21:35:34.11 +34:35:52.7
21:42:10.93 +39:16:11.0
21:28:43.61 +35:11:03.8
21:28:15.22 +35:43:26.1
21:27:17.53 +34:59:18.0
21:58:19.49 +37:12:23.5
21:58:15.44 +33:46:39.2
21:58:36.19 +41:09:24.0
21:31:29.58 +33:55:40.3
22:02:22.56 +41:34:47.3
21:33:06.86 +34:09:51.6
21:37:58.70 +36:42:06.9
21:30:18.12 +34:13:06.9
21:51:16.57 +41:52:19.3
22:03:08.32 +41:49:51.3
22:07:22.82 +40:35:20.9
21:49:05.09 +37:22:34.0
22:00:11.35 +39:37:39.9
21:52:15.38 +41:18:17.8
21:26:47.03 +37:17:35.4
21:35:46.59 +36:12:51.7
22:00:10.35 +38:33:14.2
21:55:49.63 +34:16:14.3
21:36:08.46 +35:55:08.9
21:27:06.44 +33:44:11.4
21:57:33.35 +41:16:30.9
21:43:05.94 +37:32:43.6
21:53:14.90 +36:41:34.9
21:29:18.02 +33:38:42.9
21:45:58.86 +39:55:48.1
21:30:09.31 +35:59:14.0
21:33:16.35 +41:46:52.0
22:06:09.36 +39:56:12.9
21:49:33.44 +39:24:22.7
22:09:09.62 +38:13:27.4
21:44:26.00 +38:03:30.2
21:55:15.58 +37:52:02.2
22:07:19.28 +35:59:01.1
21:59:53.99 +34:16:51.1
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21:50:35.53 +37:36:20.2
21:42:09.63 +36:32:21.6
22:07:10.81 +38:37:35.0
21:54:17.27 +36:52:14.7
22:09:48.87 +37:29:08.6
21:35:30.92 +33:55:27.4
21:40:12.88 +34:16:56.2
21:52:15.51 +41:52:18.1
21:47:59.25 +38:52:24.5
21:36:58.81 +34:31:60.0
21:58:49.50 +40:28:43.6
21:26:55.40 +38:03:54.9
21:41:28.54 +34:59:55.2
21:43:18.88 +42:12:56.5
21:38:19.66 +39:47:36.5
21:35:04.40 +35:48:31.4
21:36:20.55 +34:21:42.7
22:08:34.53 +37:33:23.8
21:32:07.92 +37:19:43.0
22:00:30.51 +41:08:38.3
21:32:41.23 +35:18:26.0
21:32:35.87 +35:36:11.1
22:05:26.20 +37:35:45.0
21:57:52.74 +34:06:47.3
22:05:26.98 +41:32:29.9
21:29:44.30 +35:02:50.1
21:52:19.85 +34:09:35.2
21:56:45.73 +40:47:17.4
21:58:48.24 +40:45:29.0
22:08:35.89 +37:44:55.1
21:43:45.89 +35:25:54.1
21:57:39.52 +41:25:20.8
21:43:07.95 +37:05:02.1
22:04:46.12 +42:08:02.3
21:44:35.13 +34:15:55.6
21:51:49.79 +37:26:02.0
21:41:03.69 +37:41:57.4
21:55:34.88 +36:37:37.0
21:56:14.98 +41:22:12.1
21:36:23.98 +37:34:32.5
21:26:51.55 +34:03:09.1
21:59:43.45 +35:08:54.3
21:54:32.73 +35:25:33.6
21:35:30.25 +38:08:37.0
21:27:08.93 +35:52:28.6
22:08:40.10 +38:50:08.0
22:08:30.73 +37:04:05.1
21:29:09.49 +34:06:49.0
21:58:43.76 +39:44:50.6
21:40:43.39 +37:37:29.1
22:00:33.04 +35:15:46.4
21:49:47.22 +34:12:11.0
21:43:00.40 +34:57:39.2
22:02:22.22 +33:59:02.7
21:53:00.60 +35:46:14.9
21:52:58.87 +39:47:12.8
21:31:04.27 +36:50:21.3
21:29:56.56 +36:19:12.5
21:47:28.68 +39:11:54.5
22:11:53.83 +39:29:36.8
22:00:55.83 +36:53:37.8
21:59:13.18 +42:19:04.5
21:43:08.73 +40:49:38.0
22:04:41.19 +40:20:52.3
22:11:52.79 +40:52:48.9
21:56:01.47 +35:45:22.2
21:50:07.58 +42:10:53.8
21:44:30.95 +38:50:13.2
21:51:39.60 +42:01:59.1
21:49:56.15 +36:30:34.0
21:59:29.65 +36:02:35.0
21:37:37.21 +37:57:03.9
22:08:05.83 +41:53:32.3
21:52:57.02 +41:56:24.6
21:55:40.14 +42:12:52.4
21:39:26.15 +34:58:47.9
21:40:55.08 +37:27:31.1
22:00:48.39 +36:27:05.0
21:44:34.94 +33:59:27.3
21:54:18.94 +34:21:39.2
22:11:11.50 +41:48:09.4
21:59:19.84 +39:44:23.1
21:29:38.93 +36:14:26.8
21:52:13.78 +34:04:19.5
21:45:59.71 +34:32:51.9
22:01:32.44 +34:05:01.2
21:48:31.76 +39:16:35.8
22:11:40.95 +38:00:40.6
21:28:56.61 +38:33:57.6
21:49:46.32 +40:24:29.2
21:56:21.42 +38:37:25.6
21:48:59.09 +35:21:20.3
21:50:11.78 +38:02:34.9
21:58:18.04 +34:23:37.9
22:03:45.00 +39:44:32.7
21:43:25.64 +36:45:53.6
22:10:04.13 +38:55:16.1
21:28:31.39 +33:41:58.1
22:05:41.20 +41:02:04.2
21:54:13.78 +42:03:15.5
21:37:31.25 +35:02:48.5
22:11:18.84 +39:15:07.6
21:44:37.79 +36:48:09.8
21:50:41.89 +37:37:59.7
22:05:03.22 +41:23:49.0
21:50:23.40 +37:34:17.7
21:58:27.10 +41:39:27.4
21:31:39.41 +36:46:29.7
22:10:13.66 +36:21:54.4
21:42:21.27 +38:13:08.4
21:52:45.52 +42:15:34.6
21:48:54.48 +37:26:43.2
21:45:57.25 +39:56:07.7
22:10:15.72 +41:34:00.8
21:50:24.73 +34:50:30.8
21:47:39.91 +41:28:28.4
21:58:30.14 +36:23:05.3
21:58:01.30 +38:57:27.6
21:59:57.43 +36:55:02.7
21:47:31.96 +35:11:22.3
21:55:53.83 +37:45:14.8
22:06:03.46 +41:22:06.3
22:02:54.61 +40:29:58.1
22:01:31.62 +37:57:47.2
22:04:28.27 +41:44:47.9
21:47:07.93 +39:07:42.5
21:43:18.36 +39:30:22.8
22:03:45.74 +37:39:38.7
22:09:32.18 +42:04:31.1
21:36:40.42 +34:18:58.2
21:31:04.35 +38:40:11.5
21:39:12.74 +36:17:19.8
21:59:59.28 +38:04:07.7
21:45:15.69 +35:22:23.0
21:58:32.55 +37:54:59.4
21:51:40.80 +35:15:18.4
21:49:29.14 +36:55:04.6
21:58:40.75 +35:20:14.8
22:02:16.99 +35:25:29.1
21:39:30.92 +37:21:42.5
21:45:18.26 +34:36:19.2
21:44:17.40 +36:34:05.3
21:28:45.69 +39:40:27.0
21:56:54.99 +41:26:11.6
21:50:02.20 +37:36:18.4
21:51:40.04 +38:49:50.4
21:52:00.27 +36:48:32.6
21:50:09.92 +40:20:09.6
21:28:08.21 +36:20:37.8
21:37:52.89 +35:41:21.5
21:58:05.47 +36:02:57.0
21:55:36.85 +38:47:54.9
21:51:39.69 +34:33:54.7
21:51:54.16 +39:30:23.0
21:55:20.73 +34:39:48.1
21:51:45.90 +37:59:55.3
21:56:38.98 +41:55:31.3
21:38:12.01 +37:42:55.4
21:56:48.74 +40:07:52.5
21:41:24.09 +39:05:05.1
21:28:20.33 +36:35:54.5
22:05:36.58 +41:17:42.1
21:48:39.20 +37:49:36.7
21:43:12.83 +35:46:27.1
21:59:29.20 +39:40:34.1
22:00:32.74 +41:01:59.0
21:46:56.51 +37:17:28.1
21:44:35.61 +34:37:03.7
21:30:41.20 +35:07:20.1
21:53:17.71 +39:27:53.4
21:55:29.46 +39:55:36.7
21:45:05.81 +37:10:31.4
21:37:04.93 +35:55:02.5
21:53:44.10 +39:01:58.7
21:40:19.76 +35:37:23.6
21:54:41.38 +41:37:13.6
21:33:09.40 +37:05:57.4
21:38:56.80 +37:31:13.6
21:34:40.41 +37:53:56.9
########### Completed Cyg-07-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:59:12.69 +42:08:23.3
21:56:43.44 +37:32:19.1
21:41:34.32 +34:36:23.6
21:42:11.57 +36:19:08.9
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21:37:06.39 +33:54:16.9
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21:48:57.03 +38:28:35.1
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21:32:45.94 +37:06:19.5
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21:55:29.67 +36:36:05.8
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21:36:58.24 +37:51:38.0
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21:43:44.26 +34:49:10.4
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21:53:31.13 +33:46:50.1
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21:26:12.88 +41:49:13.0
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21:40:43.80 +37:23:00.4
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22:05:39.86 +34:53:39.2
21:59:59.27 +36:08:34.1
21:59:20.92 +36:56:49.6
21:44:09.56 +37:55:03.4
21:28:09.20 +41:14:36.6
21:33:13.75 +37:12:43.5
21:30:32.04 +35:46:44.8
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21:28:11.90 +34:45:26.3
21:59:06.37 +34:00:18.2
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21:40:41.03 +36:19:20.7
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21:33:16.35 +41:46:52.0
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21:38:19.66 +39:47:36.5
21:35:04.40 +35:48:31.4
21:36:20.55 +34:21:42.7
22:08:34.53 +37:33:23.8
21:32:07.92 +37:19:43.0
22:00:30.51 +41:08:38.3
21:32:41.23 +35:18:26.0
21:32:35.87 +35:36:11.1
22:05:26.20 +37:35:45.0
21:57:52.74 +34:06:47.3
22:05:26.98 +41:32:29.9
21:29:44.30 +35:02:50.1
21:52:19.85 +34:09:35.2
21:56:45.73 +40:47:17.4
21:58:48.24 +40:45:29.0
22:08:35.89 +37:44:55.1
21:43:45.89 +35:25:54.1
21:57:39.52 +41:25:20.8
21:43:07.95 +37:05:02.1
22:04:46.12 +42:08:02.3
21:44:35.13 +34:15:55.6
21:51:49.79 +37:26:02.0
21:41:03.69 +37:41:57.4
21:55:34.88 +36:37:37.0
21:56:14.98 +41:22:12.1
21:36:23.98 +37:34:32.5
21:26:51.55 +34:03:09.1
21:59:43.45 +35:08:54.3
21:54:32.73 +35:25:33.6
21:35:30.25 +38:08:37.0
21:27:08.93 +35:52:28.6
22:08:40.10 +38:50:08.0
22:08:30.73 +37:04:05.1
21:29:09.49 +34:06:49.0
21:58:43.76 +39:44:50.6
21:40:43.39 +37:37:29.1
22:00:33.04 +35:15:46.4
21:49:47.22 +34:12:11.0
21:43:00.40 +34:57:39.2
22:02:22.22 +33:59:02.7
21:53:00.60 +35:46:14.9
21:52:58.87 +39:47:12.8
21:31:04.27 +36:50:21.3
21:29:56.56 +36:19:12.5
21:47:28.68 +39:11:54.5
22:11:53.83 +39:29:36.8
22:00:55.83 +36:53:37.8
21:59:13.18 +42:19:04.5
21:43:08.73 +40:49:38.0
22:04:41.19 +40:20:52.3
22:11:52.79 +40:52:48.9
21:56:01.47 +35:45:22.2
21:50:07.58 +42:10:53.8
21:44:30.95 +38:50:13.2
21:51:39.60 +42:01:59.1
21:49:56.15 +36:30:34.0
21:59:29.65 +36:02:35.0
21:37:37.21 +37:57:03.9
22:08:05.83 +41:53:32.3
21:52:57.02 +41:56:24.6
21:55:40.14 +42:12:52.4
21:39:26.15 +34:58:47.9
21:40:55.08 +37:27:31.1
22:00:48.39 +36:27:05.0
21:44:34.94 +33:59:27.3
21:54:18.94 +34:21:39.2
22:11:11.50 +41:48:09.4
21:59:19.84 +39:44:23.1
21:29:38.93 +36:14:26.8
21:52:13.78 +34:04:19.5
21:45:59.71 +34:32:51.9
22:01:32.44 +34:05:01.2
21:48:31.76 +39:16:35.8
22:11:40.95 +38:00:40.6
21:28:56.61 +38:33:57.6
21:49:46.32 +40:24:29.2
21:56:21.42 +38:37:25.6
21:48:59.09 +35:21:20.3
21:50:11.78 +38:02:34.9
21:58:18.04 +34:23:37.9
22:03:45.00 +39:44:32.7
21:43:25.64 +36:45:53.6
22:10:04.13 +38:55:16.1
21:28:31.39 +33:41:58.1
22:05:41.20 +41:02:04.2
21:54:13.78 +42:03:15.5
21:37:31.25 +35:02:48.5
22:11:18.84 +39:15:07.6
21:44:37.79 +36:48:09.8
21:50:41.89 +37:37:59.7
22:05:03.22 +41:23:49.0
21:50:23.40 +37:34:17.7
21:58:27.10 +41:39:27.4
21:31:39.41 +36:46:29.7
22:10:13.66 +36:21:54.4
21:42:21.27 +38:13:08.4
21:52:45.52 +42:15:34.6
21:48:54.48 +37:26:43.2
21:45:57.25 +39:56:07.7
22:10:15.72 +41:34:00.8
21:50:24.73 +34:50:30.8
21:47:39.91 +41:28:28.4
21:58:30.14 +36:23:05.3
21:58:01.30 +38:57:27.6
21:59:57.43 +36:55:02.7
21:47:31.96 +35:11:22.3
21:55:53.83 +37:45:14.8
22:06:03.46 +41:22:06.3
22:02:54.61 +40:29:58.1
22:01:31.62 +37:57:47.2
22:04:28.27 +41:44:47.9
21:47:07.93 +39:07:42.5
21:43:18.36 +39:30:22.8
22:03:45.74 +37:39:38.7
22:09:32.18 +42:04:31.1
21:36:40.42 +34:18:58.2
21:31:04.35 +38:40:11.5
21:39:12.74 +36:17:19.8
21:59:59.28 +38:04:07.7
21:45:15.69 +35:22:23.0
21:58:32.55 +37:54:59.4
21:51:40.80 +35:15:18.4
21:49:29.14 +36:55:04.6
21:58:40.75 +35:20:14.8
22:02:16.99 +35:25:29.1
21:39:30.92 +37:21:42.5
21:45:18.26 +34:36:19.2
21:44:17.40 +36:34:05.3
21:28:45.69 +39:40:27.0
21:56:54.99 +41:26:11.6
21:50:02.20 +37:36:18.4
21:51:40.04 +38:49:50.4
21:52:00.27 +36:48:32.6
21:50:09.92 +40:20:09.6
21:28:08.21 +36:20:37.8
21:37:52.89 +35:41:21.5
21:58:05.47 +36:02:57.0
21:55:36.85 +38:47:54.9
21:51:39.69 +34:33:54.7
21:51:54.16 +39:30:23.0
21:55:20.73 +34:39:48.1
21:51:45.90 +37:59:55.3
21:56:38.98 +41:55:31.3
21:38:12.01 +37:42:55.4
21:56:48.74 +40:07:52.5
21:41:24.09 +39:05:05.1
21:28:20.33 +36:35:54.5
22:05:36.58 +41:17:42.1
21:48:39.20 +37:49:36.7
21:43:12.83 +35:46:27.1
21:59:29.20 +39:40:34.1
22:00:32.74 +41:01:59.0
21:46:56.51 +37:17:28.1
21:44:35.61 +34:37:03.7
21:30:41.20 +35:07:20.1
21:53:17.71 +39:27:53.4
21:55:29.46 +39:55:36.7
21:45:05.81 +37:10:31.4
21:37:04.93 +35:55:02.5
21:53:44.10 +39:01:58.7
21:40:19.76 +35:37:23.6
21:54:41.38 +41:37:13.6
21:33:09.40 +37:05:57.4
21:38:56.80 +37:31:13.6
21:34:40.41 +37:53:56.9
###################################################################################
21:59:12.69 +42:08:23.3 -- not an asteroid (will add it to exclusion list)
21:56:43.44 +37:32:19.1 -- not an asteroid (will add it to exclusion list)
21:41:34.32 +34:36:23.6 -- not an asteroid (will add it to exclusion list)
21:42:11.57 +36:19:08.9 -- not an asteroid (will add it to exclusion list)
22:02:54.20 +40:44:54.5 -- not an asteroid (will add it to exclusion list)
21:48:53.93 +36:09:36.7 -- not an asteroid (will add it to exclusion list)
21:37:06.39 +33:54:16.9 -- not an asteroid (will add it to exclusion list)
21:38:16.22 +34:33:06.6 -- not an asteroid (will add it to exclusion list)
21:48:57.03 +38:28:35.1 -- not an asteroid (will add it to exclusion list)
21:50:40.99 +39:31:45.3 -- not an asteroid (will add it to exclusion list)
21:32:45.94 +37:06:19.5 -- not an asteroid (will add it to exclusion list)
22:10:18.73 +41:32:58.6 -- not an asteroid (will add it to exclusion list)
21:59:20.80 +39:40:39.1 -- not an asteroid (will add it to exclusion list)
21:55:29.67 +36:36:05.8 -- not an asteroid (will add it to exclusion list)
21:56:43.41 +41:51:09.7 -- not an asteroid (will add it to exclusion list)
21:40:11.20 +37:48:07.1 -- not an asteroid (will add it to exclusion list)
22:03:12.09 +37:15:34.4 -- not an asteroid (will add it to exclusion list)
21:54:14.01 +35:39:31.5 -- not an asteroid (will add it to exclusion list)
21:55:25.02 +39:42:15.4 -- not an asteroid (will add it to exclusion list)
21:35:34.81 +41:02:12.4 -- not an asteroid (will add it to exclusion list)
21:40:22.44 +39:00:37.6 -- not an asteroid (will add it to exclusion list)
22:01:48.31 +39:56:08.6 -- not an asteroid (will add it to exclusion list)
21:50:17.67 +42:04:59.5 -- not an asteroid (will add it to exclusion list)
21:31:25.66 +35:04:07.5 -- not an asteroid (will add it to exclusion list)
21:48:34.08 +42:19:14.2 -- not an asteroid (will add it to exclusion list)
21:29:26.32 +37:55:02.9 -- not an asteroid (will add it to exclusion list)
21:51:41.33 +39:11:41.9 -- not an asteroid (will add it to exclusion list)
22:06:06.12 +38:12:56.7 -- not an asteroid (will add it to exclusion list)
21:51:41.89 +34:07:05.8 -- not an asteroid (will add it to exclusion list)
22:02:38.66 +37:44:29.0 -- not an asteroid (will add it to exclusion list)
21:36:58.24 +37:51:38.0 -- not an asteroid (will add it to exclusion list)
22:06:54.87 +41:38:25.6 -- not an asteroid (will add it to exclusion list)
22:02:56.21 +40:46:06.2 -- not an asteroid (will add it to exclusion list)
21:43:44.26 +34:49:10.4 -- not an asteroid (will add it to exclusion list)
22:07:48.88 +34:48:04.2 -- not an asteroid (will add it to exclusion list)
22:08:33.12 +35:58:49.2 -- not an asteroid (will add it to exclusion list)
22:10:57.06 +37:02:42.5 -- not an asteroid (will add it to exclusion list)
21:50:25.14 +38:28:30.2 -- not an asteroid (will add it to exclusion list)
22:09:56.44 +39:05:40.5 -- not an asteroid (will add it to exclusion list)
21:44:37.46 +38:02:18.1 -- not an asteroid (will add it to exclusion list)
21:57:31.30 +38:48:29.4 -- not an asteroid (will add it to exclusion list)
22:02:38.78 +37:13:44.8 -- not an asteroid (will add it to exclusion list)
22:09:04.27 +36:22:36.8 -- not an asteroid (will add it to exclusion list)
22:09:49.48 +37:06:45.4 -- not an asteroid (will add it to exclusion list)
21:40:15.55 +37:50:21.5 -- not an asteroid (will add it to exclusion list)
21:45:03.10 +36:40:08.6 -- not an asteroid (will add it to exclusion list)
22:07:19.75 +40:15:15.6 -- not an asteroid (will add it to exclusion list)
21:52:04.60 +34:41:09.5 -- not an asteroid (will add it to exclusion list)
21:55:46.12 +35:47:06.6 -- not an asteroid (will add it to exclusion list)
22:05:32.42 +38:58:34.1 -- not an asteroid (will add it to exclusion list)
21:48:31.26 +41:08:43.0 -- not an asteroid (will add it to exclusion list)
21:53:31.13 +33:46:50.1 -- not an asteroid (will add it to exclusion list)
21:58:49.48 +40:53:49.1 -- not an asteroid (will add it to exclusion list)
21:42:14.31 +37:22:59.4 -- not an asteroid (will add it to exclusion list)
21:53:53.60 +41:17:52.3 -- not an asteroid (will add it to exclusion list)
21:43:02.43 +34:00:50.1 -- not an asteroid (will add it to exclusion list)
22:00:24.41 +39:57:07.7 -- not an asteroid (will add it to exclusion list)
21:56:29.02 +37:56:47.0 -- not an asteroid (will add it to exclusion list)
21:55:57.26 +40:10:25.0 -- not an asteroid (will add it to exclusion list)
21:29:16.58 +34:43:05.5 -- not an asteroid (will add it to exclusion list)
21:44:03.16 +37:47:35.8 -- not an asteroid (will add it to exclusion list)
21:39:53.76 +37:58:52.8 -- not an asteroid (will add it to exclusion list)
21:53:17.50 +41:45:59.3 -- not an asteroid (will add it to exclusion list)
21:55:39.50 +36:53:22.5 -- not an asteroid (will add it to exclusion list)
22:10:45.32 +40:14:53.9 -- not an asteroid (will add it to exclusion list)
22:09:47.58 +36:16:45.8 -- not an asteroid (will add it to exclusion list)
21:26:12.88 +41:49:13.0 -- not an asteroid (will add it to exclusion list)
21:40:12.45 +37:22:52.0 -- not an asteroid (will add it to exclusion list)
21:40:43.80 +37:23:00.4 -- not an asteroid (will add it to exclusion list)
21:57:14.44 +42:01:04.2 -- not an asteroid (will add it to exclusion list)
21:30:55.05 +34:30:59.6 -- not an asteroid (will add it to exclusion list)
22:02:05.96 +36:06:27.4 -- not an asteroid (will add it to exclusion list)
21:26:50.52 +37:00:11.8 -- not an asteroid (will add it to exclusion list)
22:02:11.35 +35:32:42.6 -- not an asteroid (will add it to exclusion list)
22:05:39.86 +34:53:39.2 -- not an asteroid (will add it to exclusion list)
21:59:59.27 +36:08:34.1 -- not an asteroid (will add it to exclusion list)
21:59:20.92 +36:56:49.6 -- not an asteroid (will add it to exclusion list)
21:44:09.56 +37:55:03.4 -- not an asteroid (will add it to exclusion list)
21:28:09.20 +41:14:36.6 -- not an asteroid (will add it to exclusion list)
21:33:13.75 +37:12:43.5 -- not an asteroid (will add it to exclusion list)
21:30:32.04 +35:46:44.8 -- not an asteroid (will add it to exclusion list)
22:06:01.48 +39:10:17.5 -- not an asteroid (will add it to exclusion list)
21:28:11.90 +34:45:26.3 -- not an asteroid (will add it to exclusion list)
21:59:06.37 +34:00:18.2 -- not an asteroid (will add it to exclusion list)
22:01:18.73 +41:30:28.0 -- not an asteroid (will add it to exclusion list)
22:01:14.46 +38:33:47.2 -- not an asteroid (will add it to exclusion list)
22:04:54.79 +40:37:24.8 -- not an asteroid (will add it to exclusion list)
22:02:13.89 +41:47:07.9 -- not an asteroid (will add it to exclusion list)
21:40:41.03 +36:19:20.7 -- not an asteroid (will add it to exclusion list)
22:02:14.84 +34:37:08.9 -- not an asteroid (will add it to exclusion list)
22:02:42.09 +37:09:00.8 -- not an asteroid (will add it to exclusion list)
22:00:24.20 +35:58:54.0 -- not an asteroid (will add it to exclusion list)
22:02:42.59 +41:44:10.6 -- not an asteroid (will add it to exclusion list)
22:06:31.88 +34:33:33.2 -- not an asteroid (will add it to exclusion list)
21:47:33.64 +37:22:56.1 -- not an asteroid (will add it to exclusion list)
21:58:18.40 +39:26:01.3 -- not an asteroid (will add it to exclusion list)
22:02:04.56 +37:45:27.6 -- not an asteroid (will add it to exclusion list)
22:07:43.40 +37:37:06.9 -- not an asteroid (will add it to exclusion list)
21:48:57.90 +37:42:53.1 -- not an asteroid (will add it to exclusion list)
21:51:57.54 +37:11:56.1 -- not an asteroid (will add it to exclusion list)
21:49:41.28 +37:43:30.9 -- not an asteroid (will add it to exclusion list)
22:10:20.04 +38:44:22.5 -- not an asteroid (will add it to exclusion list)
22:04:54.72 +35:49:32.8 -- not an asteroid (will add it to exclusion list)
22:09:33.60 +41:54:58.6 -- not an asteroid (will add it to exclusion list)
21:29:32.26 +33:48:21.6 -- not an asteroid (will add it to exclusion list)
21:38:38.20 +33:58:31.1 -- not an asteroid (will add it to exclusion list)
22:05:42.75 +35:53:01.4 -- not an asteroid (will add it to exclusion list)
22:11:12.63 +37:18:42.5 -- not an asteroid (will add it to exclusion list)
21:59:28.80 +37:59:47.4 -- not an asteroid (will add it to exclusion list)
22:06:23.67 +41:39:57.7 -- not an asteroid (will add it to exclusion list)
22:09:11.52 +36:46:06.6 -- not an asteroid (will add it to exclusion list)
21:59:01.83 +36:26:59.1 -- not an asteroid (will add it to exclusion list)
22:06:38.32 +41:43:55.3 -- not an asteroid (will add it to exclusion list)
21:58:43.07 +42:11:58.0 -- not an asteroid (will add it to exclusion list)
21:56:29.21 +36:52:35.9 -- not an asteroid (will add it to exclusion list)
22:00:26.18 +37:37:17.9 -- not an asteroid (will add it to exclusion list)
21:57:23.01 +41:48:54.3 -- not an asteroid (will add it to exclusion list)
22:01:04.06 +41:04:57.6 -- not an asteroid (will add it to exclusion list)
21:56:00.49 +37:10:56.8 -- not an asteroid (will add it to exclusion list)
21:36:48.58 +38:51:42.1 -- not an asteroid (will add it to exclusion list)
21:27:10.32 +36:53:17.9 -- not an asteroid (will add it to exclusion list)
21:50:34.31 +37:11:03.4 -- not an asteroid (will add it to exclusion list)
22:02:19.99 +34:02:56.0 -- not an asteroid (will add it to exclusion list)
22:05:11.32 +41:31:54.9 -- not an asteroid (will add it to exclusion list)
21:49:23.30 +36:27:43.5 -- not an asteroid (will add it to exclusion list)
21:48:46.74 +35:26:23.2 -- not an asteroid (will add it to exclusion list)
22:01:12.15 +35:17:06.7 -- not an asteroid (will add it to exclusion list)
21:50:58.71 +36:44:36.8 -- not an asteroid (will add it to exclusion list)
21:39:40.89 +34:24:59.7 -- not an asteroid (will add it to exclusion list)
21:50:58.46 +39:25:04.2 -- not an asteroid (will add it to exclusion list)
21:57:10.69 +42:10:42.9 -- not an asteroid (will add it to exclusion list)
21:54:38.63 +36:53:54.3 -- not an asteroid (will add it to exclusion list)
21:46:54.19 +39:15:20.8 -- not an asteroid (will add it to exclusion list)
21:46:14.75 +37:25:08.7 -- not an asteroid (will add it to exclusion list)
21:29:56.13 +35:08:34.3 -- not an asteroid (will add it to exclusion list)
21:42:07.42 +39:04:10.8 -- not an asteroid (will add it to exclusion list)
22:06:12.38 +39:36:05.5 -- not an asteroid (will add it to exclusion list)
21:51:11.60 +37:00:46.2 -- not an asteroid (will add it to exclusion list)
21:56:34.45 +37:00:27.0 -- not an asteroid (will add it to exclusion list)
21:48:07.30 +36:02:35.7 -- not an asteroid (will add it to exclusion list)
21:57:57.47 +34:05:54.2 -- not an asteroid (will add it to exclusion list)
22:04:30.42 +41:26:44.9 -- not an asteroid (will add it to exclusion list)
21:42:33.76 +41:45:51.2 -- not an asteroid (will add it to exclusion list)
21:50:44.43 +36:27:35.9 -- not an asteroid (will add it to exclusion list)
21:35:27.29 +35:03:48.3 -- not an asteroid (will add it to exclusion list)
22:06:29.23 +39:32:47.9 -- not an asteroid (will add it to exclusion list)
21:48:57.14 +34:21:32.4 -- not an asteroid (will add it to exclusion list)
22:08:10.51 +39:02:03.1 -- not an asteroid (will add it to exclusion list)
21:50:31.56 +38:39:10.8 -- not an asteroid (will add it to exclusion list)
21:27:00.73 +33:45:03.0 -- not an asteroid (will add it to exclusion list)
21:27:07.35 +35:14:57.5 -- not an asteroid (will add it to exclusion list)
21:55:36.26 +35:51:33.8 -- not an asteroid (will add it to exclusion list)
21:42:31.24 +35:51:14.2 -- not an asteroid (will add it to exclusion list)
21:31:26.82 +33:46:07.4 -- not an asteroid (will add it to exclusion list)
21:35:34.11 +34:35:52.7 -- not an asteroid (will add it to exclusion list)
21:42:10.93 +39:16:11.0 -- not an asteroid (will add it to exclusion list)
21:28:43.61 +35:11:03.8 -- not an asteroid (will add it to exclusion list)
21:28:15.22 +35:43:26.1 -- not an asteroid (will add it to exclusion list)
21:27:17.53 +34:59:18.0 -- not an asteroid (will add it to exclusion list)
21:58:19.49 +37:12:23.5 -- not an asteroid (will add it to exclusion list)
21:58:15.44 +33:46:39.2 -- not an asteroid (will add it to exclusion list)
21:58:36.19 +41:09:24.0 -- not an asteroid (will add it to exclusion list)
21:31:29.58 +33:55:40.3 -- not an asteroid (will add it to exclusion list)
22:02:22.56 +41:34:47.3 -- not an asteroid (will add it to exclusion list)
21:33:06.86 +34:09:51.6 -- not an asteroid (will add it to exclusion list)
21:37:58.70 +36:42:06.9 -- not an asteroid (will add it to exclusion list)
21:30:18.12 +34:13:06.9 -- not an asteroid (will add it to exclusion list)
21:51:16.57 +41:52:19.3 -- not an asteroid (will add it to exclusion list)
22:03:08.32 +41:49:51.3 -- not an asteroid (will add it to exclusion list)
22:07:22.82 +40:35:20.9 -- not an asteroid (will add it to exclusion list)
21:49:05.09 +37:22:34.0 -- not an asteroid (will add it to exclusion list)
22:00:11.35 +39:37:39.9 -- not an asteroid (will add it to exclusion list)
21:52:15.38 +41:18:17.8 -- not an asteroid (will add it to exclusion list)
21:26:47.03 +37:17:35.4 -- not an asteroid (will add it to exclusion list)
21:35:46.59 +36:12:51.7 -- not an asteroid (will add it to exclusion list)
22:00:10.35 +38:33:14.2 -- not an asteroid (will add it to exclusion list)
21:55:49.63 +34:16:14.3 -- not an asteroid (will add it to exclusion list)
21:36:08.46 +35:55:08.9 -- not an asteroid (will add it to exclusion list)
21:27:06.44 +33:44:11.4 -- not an asteroid (will add it to exclusion list)
21:57:33.35 +41:16:30.9 -- not an asteroid (will add it to exclusion list)
21:43:05.94 +37:32:43.6 -- not an asteroid (will add it to exclusion list)
21:53:14.90 +36:41:34.9 -- not an asteroid (will add it to exclusion list)
21:29:18.02 +33:38:42.9 -- not an asteroid (will add it to exclusion list)
21:45:58.86 +39:55:48.1 -- not an asteroid (will add it to exclusion list)
21:30:09.31 +35:59:14.0 -- not an asteroid (will add it to exclusion list)
21:33:16.35 +41:46:52.0 -- not an asteroid (will add it to exclusion list)
22:06:09.36 +39:56:12.9 -- not an asteroid (will add it to exclusion list)
21:49:33.44 +39:24:22.7 -- not an asteroid (will add it to exclusion list)
22:09:09.62 +38:13:27.4 -- not an asteroid (will add it to exclusion list)
21:44:26.00 +38:03:30.2 -- not an asteroid (will add it to exclusion list)
21:55:15.58 +37:52:02.2 -- not an asteroid (will add it to exclusion list)
22:07:19.28 +35:59:01.1 -- not an asteroid (will add it to exclusion list)
21:59:53.99 +34:16:51.1 -- not an asteroid (will add it to exclusion list)
22:10:22.57 +40:43:10.2 -- not an asteroid (will add it to exclusion list)
21:50:35.53 +37:36:20.2 -- not an asteroid (will add it to exclusion list)
21:42:09.63 +36:32:21.6 -- not an asteroid (will add it to exclusion list)
22:07:10.81 +38:37:35.0 -- not an asteroid (will add it to exclusion list)
21:54:17.27 +36:52:14.7 -- not an asteroid (will add it to exclusion list)
22:09:48.87 +37:29:08.6 -- not an asteroid (will add it to exclusion list)
21:35:30.92 +33:55:27.4 -- not an asteroid (will add it to exclusion list)
21:40:12.88 +34:16:56.2 -- not an asteroid (will add it to exclusion list)
21:52:15.51 +41:52:18.1 -- not an asteroid (will add it to exclusion list)
21:47:59.25 +38:52:24.5 -- not an asteroid (will add it to exclusion list)
21:36:58.81 +34:31:60.0 -- not an asteroid (will add it to exclusion list)
21:58:49.50 +40:28:43.6 -- not an asteroid (will add it to exclusion list)
21:26:55.40 +38:03:54.9 -- not an asteroid (will add it to exclusion list)
21:41:28.54 +34:59:55.2 -- not an asteroid (will add it to exclusion list)
21:43:18.88 +42:12:56.5 -- not an asteroid (will add it to exclusion list)
21:38:19.66 +39:47:36.5 -- not an asteroid (will add it to exclusion list)
21:35:04.40 +35:48:31.4 -- not an asteroid (will add it to exclusion list)
21:36:20.55 +34:21:42.7 -- not an asteroid (will add it to exclusion list)
22:08:34.53 +37:33:23.8 -- not an asteroid (will add it to exclusion list)
21:32:07.92 +37:19:43.0 -- not an asteroid (will add it to exclusion list)
22:00:30.51 +41:08:38.3 -- not an asteroid (will add it to exclusion list)
21:32:41.23 +35:18:26.0 -- not an asteroid (will add it to exclusion list)
21:32:35.87 +35:36:11.1 -- not an asteroid (will add it to exclusion list)
22:05:26.20 +37:35:45.0 -- not an asteroid (will add it to exclusion list)
21:57:52.74 +34:06:47.3 -- not an asteroid (will add it to exclusion list)
22:05:26.98 +41:32:29.9 -- not an asteroid (will add it to exclusion list)
21:29:44.30 +35:02:50.1 -- not an asteroid (will add it to exclusion list)
21:52:19.85 +34:09:35.2 -- not an asteroid (will add it to exclusion list)
21:56:45.73 +40:47:17.4 -- not an asteroid (will add it to exclusion list)
21:58:48.24 +40:45:29.0 -- not an asteroid (will add it to exclusion list)
22:08:35.89 +37:44:55.1 -- not an asteroid (will add it to exclusion list)
21:43:45.89 +35:25:54.1 -- not an asteroid (will add it to exclusion list)
21:57:39.52 +41:25:20.8 -- not an asteroid (will add it to exclusion list)
21:43:07.95 +37:05:02.1 -- not an asteroid (will add it to exclusion list)
22:04:46.12 +42:08:02.3 -- not an asteroid (will add it to exclusion list)
21:44:35.13 +34:15:55.6 -- not an asteroid (will add it to exclusion list)
21:51:49.79 +37:26:02.0 -- not an asteroid (will add it to exclusion list)
21:41:03.69 +37:41:57.4 -- not an asteroid (will add it to exclusion list)
21:55:34.88 +36:37:37.0 -- not an asteroid (will add it to exclusion list)
21:56:14.98 +41:22:12.1 -- not an asteroid (will add it to exclusion list)
21:36:23.98 +37:34:32.5 -- not an asteroid (will add it to exclusion list)
21:26:51.55 +34:03:09.1 -- not an asteroid (will add it to exclusion list)
21:59:43.45 +35:08:54.3 -- not an asteroid (will add it to exclusion list)
21:54:32.73 +35:25:33.6 -- not an asteroid (will add it to exclusion list)
21:35:30.25 +38:08:37.0 -- not an asteroid (will add it to exclusion list)
21:27:08.93 +35:52:28.6 -- not an asteroid (will add it to exclusion list)
22:08:40.10 +38:50:08.0 -- not an asteroid (will add it to exclusion list)
22:08:30.73 +37:04:05.1 -- not an asteroid (will add it to exclusion list)
21:29:09.49 +34:06:49.0 -- not an asteroid (will add it to exclusion list)
21:58:43.76 +39:44:50.6 -- not an asteroid (will add it to exclusion list)
21:40:43.39 +37:37:29.1 -- not an asteroid (will add it to exclusion list)
22:00:33.04 +35:15:46.4 -- not an asteroid (will add it to exclusion list)
21:49:47.22 +34:12:11.0 -- not an asteroid (will add it to exclusion list)
21:43:00.40 +34:57:39.2 -- not an asteroid (will add it to exclusion list)
22:02:22.22 +33:59:02.7 -- not an asteroid (will add it to exclusion list)
21:53:00.60 +35:46:14.9 -- not an asteroid (will add it to exclusion list)
21:52:58.87 +39:47:12.8 -- not an asteroid (will add it to exclusion list)
21:31:04.27 +36:50:21.3 -- not an asteroid (will add it to exclusion list)
21:29:56.56 +36:19:12.5 -- not an asteroid (will add it to exclusion list)
21:47:28.68 +39:11:54.5 -- not an asteroid (will add it to exclusion list)
22:11:53.83 +39:29:36.8 -- not an asteroid (will add it to exclusion list)
22:00:55.83 +36:53:37.8 -- not an asteroid (will add it to exclusion list)
21:59:13.18 +42:19:04.5 -- not an asteroid (will add it to exclusion list)
21:43:08.73 +40:49:38.0 -- not an asteroid (will add it to exclusion list)
22:04:41.19 +40:20:52.3 -- not an asteroid (will add it to exclusion list)
22:11:52.79 +40:52:48.9 -- not an asteroid (will add it to exclusion list)
21:56:01.47 +35:45:22.2 -- not an asteroid (will add it to exclusion list)
21:50:07.58 +42:10:53.8 -- not an asteroid (will add it to exclusion list)
21:44:30.95 +38:50:13.2 -- not an asteroid (will add it to exclusion list)
21:51:39.60 +42:01:59.1 -- not an asteroid (will add it to exclusion list)
21:49:56.15 +36:30:34.0 -- not an asteroid (will add it to exclusion list)
21:59:29.65 +36:02:35.0 -- not an asteroid (will add it to exclusion list)
21:37:37.21 +37:57:03.9 -- not an asteroid (will add it to exclusion list)
22:08:05.83 +41:53:32.3 -- not an asteroid (will add it to exclusion list)
21:52:57.02 +41:56:24.6 -- not an asteroid (will add it to exclusion list)
21:55:40.14 +42:12:52.4 -- not an asteroid (will add it to exclusion list)
21:39:26.15 +34:58:47.9 -- not an asteroid (will add it to exclusion list)
21:40:55.08 +37:27:31.1 -- not an asteroid (will add it to exclusion list)
22:00:48.39 +36:27:05.0 -- not an asteroid (will add it to exclusion list)
21:44:34.94 +33:59:27.3 -- not an asteroid (will add it to exclusion list)
21:54:18.94 +34:21:39.2 -- not an asteroid (will add it to exclusion list)
22:11:11.50 +41:48:09.4 -- not an asteroid (will add it to exclusion list)
21:59:19.84 +39:44:23.1 -- not an asteroid (will add it to exclusion list)
21:29:38.93 +36:14:26.8 -- not an asteroid (will add it to exclusion list)
21:52:13.78 +34:04:19.5 -- not an asteroid (will add it to exclusion list)
21:45:59.71 +34:32:51.9 -- not an asteroid (will add it to exclusion list)
22:01:32.44 +34:05:01.2 -- not an asteroid (will add it to exclusion list)
21:48:31.76 +39:16:35.8 -- not an asteroid (will add it to exclusion list)
22:11:40.95 +38:00:40.6 -- not an asteroid (will add it to exclusion list)
21:28:56.61 +38:33:57.6 -- not an asteroid (will add it to exclusion list)
21:49:46.32 +40:24:29.2 -- not an asteroid (will add it to exclusion list)
21:56:21.42 +38:37:25.6 -- not an asteroid (will add it to exclusion list)
21:48:59.09 +35:21:20.3 -- not an asteroid (will add it to exclusion list)
21:50:11.78 +38:02:34.9 -- not an asteroid (will add it to exclusion list)
21:58:18.04 +34:23:37.9 -- not an asteroid (will add it to exclusion list)
22:03:45.00 +39:44:32.7 -- not an asteroid (will add it to exclusion list)
21:43:25.64 +36:45:53.6 -- not an asteroid (will add it to exclusion list)
22:10:04.13 +38:55:16.1 -- not an asteroid (will add it to exclusion list)
21:28:31.39 +33:41:58.1 -- not an asteroid (will add it to exclusion list)
22:05:41.20 +41:02:04.2 -- not an asteroid (will add it to exclusion list)
21:54:13.78 +42:03:15.5 -- not an asteroid (will add it to exclusion list)
21:37:31.25 +35:02:48.5 -- not an asteroid (will add it to exclusion list)
22:11:18.84 +39:15:07.6 -- not an asteroid (will add it to exclusion list)
21:44:37.79 +36:48:09.8 -- not an asteroid (will add it to exclusion list)
21:50:41.89 +37:37:59.7 -- not an asteroid (will add it to exclusion list)
22:05:03.22 +41:23:49.0 -- not an asteroid (will add it to exclusion list)
21:50:23.40 +37:34:17.7 -- not an asteroid (will add it to exclusion list)
21:58:27.10 +41:39:27.4 -- not an asteroid (will add it to exclusion list)
21:31:39.41 +36:46:29.7 -- not an asteroid (will add it to exclusion list)
22:10:13.66 +36:21:54.4 -- not an asteroid (will add it to exclusion list)
21:42:21.27 +38:13:08.4 -- not an asteroid (will add it to exclusion list)
21:52:45.52 +42:15:34.6 -- not an asteroid (will add it to exclusion list)
21:48:54.48 +37:26:43.2 -- not an asteroid (will add it to exclusion list)
21:45:57.25 +39:56:07.7 -- not an asteroid (will add it to exclusion list)
22:10:15.72 +41:34:00.8 -- not an asteroid (will add it to exclusion list)
21:50:24.73 +34:50:30.8 -- not an asteroid (will add it to exclusion list)
21:47:39.91 +41:28:28.4 -- not an asteroid (will add it to exclusion list)
21:58:30.14 +36:23:05.3 -- not an asteroid (will add it to exclusion list)
21:58:01.30 +38:57:27.6 -- not an asteroid (will add it to exclusion list)
21:59:57.43 +36:55:02.7 -- not an asteroid (will add it to exclusion list)
21:47:31.96 +35:11:22.3 -- not an asteroid (will add it to exclusion list)
21:55:53.83 +37:45:14.8 -- not an asteroid (will add it to exclusion list)
22:06:03.46 +41:22:06.3 -- not an asteroid (will add it to exclusion list)
22:02:54.61 +40:29:58.1 -- not an asteroid (will add it to exclusion list)
22:01:31.62 +37:57:47.2 -- not an asteroid (will add it to exclusion list)
22:04:28.27 +41:44:47.9 -- not an asteroid (will add it to exclusion list)
21:47:07.93 +39:07:42.5 -- not an asteroid (will add it to exclusion list)
21:43:18.36 +39:30:22.8 -- not an asteroid (will add it to exclusion list)
22:03:45.74 +37:39:38.7 -- not an asteroid (will add it to exclusion list)
22:09:32.18 +42:04:31.1 -- not an asteroid (will add it to exclusion list)
21:36:40.42 +34:18:58.2 -- not an asteroid (will add it to exclusion list)
21:31:04.35 +38:40:11.5 -- not an asteroid (will add it to exclusion list)
21:39:12.74 +36:17:19.8 -- not an asteroid (will add it to exclusion list)
21:59:59.28 +38:04:07.7 -- not an asteroid (will add it to exclusion list)
21:45:15.69 +35:22:23.0 -- not an asteroid (will add it to exclusion list)
21:58:32.55 +37:54:59.4 -- not an asteroid (will add it to exclusion list)
21:51:40.80 +35:15:18.4 -- not an asteroid (will add it to exclusion list)
21:49:29.14 +36:55:04.6 -- not an asteroid (will add it to exclusion list)
21:58:40.75 +35:20:14.8 -- not an asteroid (will add it to exclusion list)
22:02:16.99 +35:25:29.1 -- not an asteroid (will add it to exclusion list)
21:39:30.92 +37:21:42.5 -- not an asteroid (will add it to exclusion list)
21:45:18.26 +34:36:19.2 -- not an asteroid (will add it to exclusion list)
21:44:17.40 +36:34:05.3 -- not an asteroid (will add it to exclusion list)
21:28:45.69 +39:40:27.0 -- not an asteroid (will add it to exclusion list)
21:56:54.99 +41:26:11.6 -- not an asteroid (will add it to exclusion list)
21:50:02.20 +37:36:18.4 -- not an asteroid (will add it to exclusion list)
21:51:40.04 +38:49:50.4 -- not an asteroid (will add it to exclusion list)
21:52:00.27 +36:48:32.6 -- not an asteroid (will add it to exclusion list)
21:50:09.92 +40:20:09.6 -- not an asteroid (will add it to exclusion list)
21:28:08.21 +36:20:37.8 -- not an asteroid (will add it to exclusion list)
21:37:52.89 +35:41:21.5 -- not an asteroid (will add it to exclusion list)
21:58:05.47 +36:02:57.0 -- not an asteroid (will add it to exclusion list)
21:55:36.85 +38:47:54.9 -- not an asteroid (will add it to exclusion list)
21:51:39.69 +34:33:54.7 -- not an asteroid (will add it to exclusion list)
21:51:54.16 +39:30:23.0 -- not an asteroid (will add it to exclusion list)
21:55:20.73 +34:39:48.1 -- not an asteroid (will add it to exclusion list)
21:51:45.90 +37:59:55.3 -- not an asteroid (will add it to exclusion list)
21:56:38.98 +41:55:31.3 -- not an asteroid (will add it to exclusion list)
21:38:12.01 +37:42:55.4 -- not an asteroid (will add it to exclusion list)
21:56:48.74 +40:07:52.5 -- not an asteroid (will add it to exclusion list)
21:41:24.09 +39:05:05.1 -- not an asteroid (will add it to exclusion list)
21:28:20.33 +36:35:54.5 -- not an asteroid (will add it to exclusion list)
22:05:36.58 +41:17:42.1 -- not an asteroid (will add it to exclusion list)
21:48:39.20 +37:49:36.7 -- not an asteroid (will add it to exclusion list)
21:43:12.83 +35:46:27.1 -- not an asteroid (will add it to exclusion list)
21:59:29.20 +39:40:34.1 -- not an asteroid (will add it to exclusion list)
22:00:32.74 +41:01:59.0 -- not an asteroid (will add it to exclusion list)
21:46:56.51 +37:17:28.1 -- not an asteroid (will add it to exclusion list)
21:44:35.61 +34:37:03.7 -- not an asteroid (will add it to exclusion list)
21:30:41.20 +35:07:20.1 -- not an asteroid (will add it to exclusion list)
21:53:17.71 +39:27:53.4 -- not an asteroid (will add it to exclusion list)
21:55:29.46 +39:55:36.7 -- not an asteroid (will add it to exclusion list)
21:45:05.81 +37:10:31.4 -- not an asteroid (will add it to exclusion list)
21:37:04.93 +35:55:02.5 -- not an asteroid (will add it to exclusion list)
21:53:44.10 +39:01:58.7 -- not an asteroid (will add it to exclusion list)
21:40:19.76 +35:37:23.6 -- not an asteroid (will add it to exclusion list)
21:54:41.38 +41:37:13.6 -- not an asteroid (will add it to exclusion list)
21:33:09.40 +37:05:57.4 -- not an asteroid (will add it to exclusion list)
21:38:56.80 +37:31:13.6 -- not an asteroid (will add it to exclusion list)
21:34:40.41 +37:53:56.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:26:12.88 +41:49:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:47.03 +37:17:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:50.52 +37:00:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:51.55 +34:03:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:55.40 +38:03:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:00.73 +33:45:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:06.44 +33:44:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:07.35 +35:14:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:08.93 +35:52:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:10.32 +36:53:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:17.53 +34:59:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:08.21 +36:20:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:09.20 +41:14:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:11.90 +34:45:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:15.22 +35:43:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:20.33 +36:35:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:31.39 +33:41:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:43.61 +35:11:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:45.69 +39:40:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:56.61 +38:33:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:09.49 +34:06:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:16.58 +34:43:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:18.02 +33:38:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:26.32 +37:55:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:32.26 +33:48:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:38.93 +36:14:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:44.30 +35:02:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:56.13 +35:08:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:56.56 +36:19:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:09.31 +35:59:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:18.12 +34:13:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:32.04 +35:46:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:41.20 +35:07:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:55.05 +34:30:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:04.27 +36:50:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:04.35 +38:40:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:25.66 +35:04:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:26.82 +33:46:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:29.58 +33:55:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:39.41 +36:46:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:07.92 +37:19:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:35.87 +35:36:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:41.23 +35:18:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:45.94 +37:06:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:06.86 +34:09:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:09.40 +37:05:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:13.75 +37:12:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:16.35 +41:46:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:40.41 +37:53:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:04.40 +35:48:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:27.29 +35:03:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:30.25 +38:08:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:30.92 +33:55:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:34.11 +34:35:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:34.81 +41:02:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:46.59 +36:12:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:08.46 +35:55:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:20.55 +34:21:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:23.98 +37:34:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:40.42 +34:18:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:48.58 +38:51:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:58.24 +37:51:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:58.81 +34:31:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:04.93 +35:55:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:06.39 +33:54:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:31.25 +35:02:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:37.21 +37:57:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:52.89 +35:41:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:58.70 +36:42:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:12.01 +37:42:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:16.22 +34:33:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:19.66 +39:47:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:38.20 +33:58:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:56.80 +37:31:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:12.74 +36:17:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:26.15 +34:58:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:30.92 +37:21:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:40.89 +34:24:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:53.76 +37:58:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:11.20 +37:48:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:12.45 +37:22:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:12.88 +34:16:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:15.55 +37:50:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:19.76 +35:37:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:22.44 +39:00:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:41.03 +36:19:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:43.39 +37:37:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:43.80 +37:23:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:55.08 +37:27:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:03.69 +37:41:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:24.09 +39:05:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:28.54 +34:59:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:34.32 +34:36:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:07.42 +39:04:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:09.63 +36:32:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:10.93 +39:16:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:11.57 +36:19:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:14.31 +37:22:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:21.27 +38:13:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:31.24 +35:51:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:33.76 +41:45:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:00.40 +34:57:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:02.43 +34:00:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:05.94 +37:32:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:07.95 +37:05:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:08.73 +40:49:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:12.83 +35:46:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:18.36 +39:30:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:18.88 +42:12:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:25.64 +36:45:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:44.26 +34:49:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:45.89 +35:25:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:03.16 +37:47:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:09.56 +37:55:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:17.40 +36:34:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:26.00 +38:03:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:30.95 +38:50:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:34.94 +33:59:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:35.13 +34:15:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:35.61 +34:37:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:37.46 +38:02:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:37.79 +36:48:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:03.10 +36:40:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:05.81 +37:10:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:15.69 +35:22:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:18.26 +34:36:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:57.25 +39:56:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:58.86 +39:55:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:59.71 +34:32:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:14.75 +37:25:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:54.19 +39:15:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:56.51 +37:17:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:07.93 +39:07:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:28.68 +39:11:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:31.96 +35:11:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:33.64 +37:22:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:39.91 +41:28:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:59.25 +38:52:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:07.30 +36:02:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:31.26 +41:08:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:31.76 +39:16:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:34.08 +42:19:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:39.20 +37:49:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:46.74 +35:26:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:53.93 +36:09:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:54.48 +37:26:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:57.03 +38:28:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:57.14 +34:21:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:57.90 +37:42:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:59.09 +35:21:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:05.09 +37:22:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:23.30 +36:27:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:29.14 +36:55:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:33.44 +39:24:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:41.28 +37:43:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:46.32 +40:24:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:47.22 +34:12:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:56.15 +36:30:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:02.20 +37:36:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:07.58 +42:10:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:09.92 +40:20:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:11.78 +38:02:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:17.67 +42:04:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:23.40 +37:34:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:24.73 +34:50:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:25.14 +38:28:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:31.56 +38:39:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:34.31 +37:11:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:35.53 +37:36:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:40.99 +39:31:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:41.89 +37:37:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:44.43 +36:27:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:58.46 +39:25:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:58.71 +36:44:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:11.60 +37:00:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:16.57 +41:52:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:39.60 +42:01:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:39.69 +34:33:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:40.04 +38:49:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:40.80 +35:15:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:41.33 +39:11:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:41.89 +34:07:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:45.90 +37:59:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:49.79 +37:26:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:54.16 +39:30:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:57.54 +37:11:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:00.27 +36:48:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:04.60 +34:41:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:13.78 +34:04:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:15.38 +41:18:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:15.51 +41:52:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:19.85 +34:09:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:45.52 +42:15:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:57.02 +41:56:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:58.87 +39:47:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:00.60 +35:46:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:14.90 +36:41:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:17.50 +41:45:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:17.71 +39:27:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:31.13 +33:46:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:44.10 +39:01:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:53.60 +41:17:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:13.78 +42:03:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:14.01 +35:39:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:17.27 +36:52:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:18.94 +34:21:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:32.73 +35:25:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:38.63 +36:53:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:41.38 +41:37:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:15.58 +37:52:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:20.73 +34:39:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:25.02 +39:42:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:29.46 +39:55:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:29.67 +36:36:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:34.88 +36:37:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:36.26 +35:51:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:36.85 +38:47:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:39.50 +36:53:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:40.14 +42:12:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:46.12 +35:47:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:49.63 +34:16:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:53.83 +37:45:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:57.26 +40:10:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:00.49 +37:10:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:01.47 +35:45:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:14.98 +41:22:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:21.42 +38:37:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:29.02 +37:56:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:29.21 +36:52:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:34.45 +37:00:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:38.98 +41:55:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:43.41 +41:51:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:43.44 +37:32:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:45.73 +40:47:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:48.74 +40:07:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:54.99 +41:26:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:10.69 +42:10:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:14.44 +42:01:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:23.01 +41:48:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:31.30 +38:48:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:33.35 +41:16:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:39.52 +41:25:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:52.74 +34:06:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:57.47 +34:05:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:01.30 +38:57:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:05.47 +36:02:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:15.44 +33:46:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:18.04 +34:23:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:18.40 +39:26:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:19.49 +37:12:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:27.10 +41:39:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:30.14 +36:23:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:32.55 +37:54:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:36.19 +41:09:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:40.75 +35:20:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:43.07 +42:11:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:43.76 +39:44:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:48.24 +40:45:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:49.48 +40:53:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:49.50 +40:28:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:01.83 +36:26:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:06.37 +34:00:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:12.69 +42:08:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:13.18 +42:19:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:19.84 +39:44:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:20.80 +39:40:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:20.92 +36:56:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:28.80 +37:59:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:29.20 +39:40:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:29.65 +36:02:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:43.45 +35:08:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:53.99 +34:16:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:57.43 +36:55:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:59.27 +36:08:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:59.28 +38:04:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:10.35 +38:33:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:11.35 +39:37:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:24.20 +35:58:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:24.41 +39:57:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:26.18 +37:37:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:30.51 +41:08:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:32.74 +41:01:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:33.04 +35:15:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:48.39 +36:27:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:55.83 +36:53:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:04.06 +41:04:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:12.15 +35:17:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:14.46 +38:33:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:18.73 +41:30:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:31.62 +37:57:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:32.44 +34:05:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:48.31 +39:56:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:04.56 +37:45:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:05.96 +36:06:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:11.35 +35:32:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:13.89 +41:47:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:14.84 +34:37:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:16.99 +35:25:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:19.99 +34:02:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:22.22 +33:59:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:22.56 +41:34:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:38.66 +37:44:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:38.78 +37:13:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.09 +37:09:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.59 +41:44:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:54.20 +40:44:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:54.61 +40:29:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:56.21 +40:46:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:08.32 +41:49:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:12.09 +37:15:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:45.00 +39:44:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:45.74 +37:39:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:28.27 +41:44:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:30.42 +41:26:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:41.19 +40:20:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:46.12 +42:08:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:54.72 +35:49:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:54.79 +40:37:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:03.22 +41:23:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:11.32 +41:31:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:26.20 +37:35:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:26.98 +41:32:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:32.42 +38:58:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:36.58 +41:17:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:39.86 +34:53:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:41.20 +41:02:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:42.75 +35:53:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:01.48 +39:10:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:03.46 +41:22:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:06.12 +38:12:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:09.36 +39:56:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:12.38 +39:36:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:23.67 +41:39:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:29.23 +39:32:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:31.88 +34:33:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:38.32 +41:43:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:54.87 +41:38:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:10.81 +38:37:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:19.28 +35:59:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:19.75 +40:15:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:22.82 +40:35:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:43.40 +37:37:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:48.88 +34:48:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:05.83 +41:53:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:10.51 +39:02:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:30.73 +37:04:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:33.12 +35:58:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:34.53 +37:33:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:35.89 +37:44:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:40.10 +38:50:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:04.27 +36:22:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:09.62 +38:13:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:11.52 +36:46:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:32.18 +42:04:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:33.60 +41:54:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:47.58 +36:16:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:48.87 +37:29:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:49.48 +37:06:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:56.44 +39:05:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:04.13 +38:55:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:13.66 +36:21:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:15.72 +41:34:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:18.73 +41:32:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:20.04 +38:44:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:22.57 +40:43:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:45.32 +40:14:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:57.06 +37:02:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:11.50 +41:48:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:12.63 +37:18:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:18.84 +39:15:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:40.95 +38:00:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:52.79 +40:52:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:53.83 +39:29:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
21:26:12.88 +41:49:13.0 -- not a known variable star
21:26:47.03 +37:17:35.4 -- a known variable star
21:26:50.52 +37:00:11.8 -- a known variable star
21:26:51.55 +34:03:09.1 -- a known variable star
21:26:55.40 +38:03:54.9 -- not a known variable star
21:27:00.73 +33:45:03.0 -- not a known variable star
21:27:06.44 +33:44:11.4 -- a known variable star
21:27:07.35 +35:14:57.5 -- not a known variable star
21:27:08.93 +35:52:28.6 -- a known variable star
21:27:10.32 +36:53:17.9 -- not a known variable star
21:27:17.53 +34:59:18.0 -- a known variable star
21:28:08.21 +36:20:37.8 -- not a known variable star
21:28:09.20 +41:14:36.6 -- not a known variable star
21:28:11.90 +34:45:26.3 -- not a known variable star
21:28:15.22 +35:43:26.1 -- not a known variable star
21:28:20.33 +36:35:54.5 -- not a known variable star
21:28:31.39 +33:41:58.1 -- not a known variable star
21:28:43.61 +35:11:03.8 -- a known variable star
21:28:45.69 +39:40:27.0 -- not a known variable star
21:28:56.61 +38:33:57.6 -- not a known variable star
21:29:09.49 +34:06:49.0 -- not a known variable star
21:29:16.58 +34:43:05.5 -- not a known variable star
21:29:18.02 +33:38:42.9 -- not a known variable star
21:29:26.32 +37:55:02.9 -- not a known variable star
21:29:32.26 +33:48:21.6 -- not a known variable star
21:29:38.93 +36:14:26.8 -- not a known variable star
21:29:44.30 +35:02:50.1 -- not a known variable star
21:29:56.13 +35:08:34.3 -- not a known variable star
21:29:56.56 +36:19:12.5 -- not a known variable star
21:30:09.31 +35:59:14.0 -- not a known variable star
21:30:18.12 +34:13:06.9 -- not a known variable star
21:30:32.04 +35:46:44.8 -- not a known variable star
21:30:41.20 +35:07:20.1 -- not a known variable star
21:30:55.05 +34:30:59.6 -- not a known variable star
21:31:04.27 +36:50:21.3 -- not a known variable star
21:31:04.35 +38:40:11.5 -- not a known variable star
21:31:25.66 +35:04:07.5 -- not a known variable star
21:31:26.82 +33:46:07.4 -- not a known variable star
21:31:29.58 +33:55:40.3 -- not a known variable star
21:31:39.41 +36:46:29.7 -- not a known variable star
21:32:07.92 +37:19:43.0 -- not a known variable star
21:32:35.87 +35:36:11.1 -- not a known variable star
21:32:41.23 +35:18:26.0 -- not a known variable star
21:32:45.94 +37:06:19.5 -- not a known variable star
21:33:06.86 +34:09:51.6 -- not a known variable star
21:33:09.40 +37:05:57.4 -- not a known variable star
21:33:13.75 +37:12:43.5 -- not a known variable star
21:33:16.35 +41:46:52.0 -- not a known variable star
21:34:40.41 +37:53:56.9 -- not a known variable star
21:35:04.40 +35:48:31.4 -- a known variable star
21:35:27.29 +35:03:48.3 -- not a known variable star
21:35:30.25 +38:08:37.0 -- not a known variable star
21:35:30.92 +33:55:27.4 -- a known variable star
21:35:34.11 +34:35:52.7 -- not a known variable star
21:35:34.81 +41:02:12.4 -- not a known variable star
21:35:46.59 +36:12:51.7 -- not a known variable star
21:36:08.46 +35:55:08.9 -- not a known variable star
21:36:20.55 +34:21:42.7 -- a known variable star
21:36:23.98 +37:34:32.5 -- not a known variable star
21:36:40.42 +34:18:58.2 -- not a known variable star
21:36:48.58 +38:51:42.1 -- not a known variable star
21:36:58.24 +37:51:38.0 -- not a known variable star
21:36:58.81 +34:31:60.0 -- not a known variable star
21:37:04.93 +35:55:02.5 -- not a known variable star
21:37:06.39 +33:54:16.9 -- a known variable star
21:37:31.25 +35:02:48.5 -- not a known variable star
21:37:37.21 +37:57:03.9 -- not a known variable star
21:37:52.89 +35:41:21.5 -- not a known variable star
21:37:58.70 +36:42:06.9 -- not a known variable star
21:38:12.01 +37:42:55.4 -- not a known variable star
21:38:16.22 +34:33:06.6 -- not a known variable star
21:38:19.66 +39:47:36.5 -- not a known variable star
21:38:38.20 +33:58:31.1 -- not a known variable star
21:38:56.80 +37:31:13.6 -- not a known variable star
21:39:12.74 +36:17:19.8 -- not a known variable star
21:39:26.15 +34:58:47.9 -- not a known variable star
21:39:30.92 +37:21:42.5 -- not a known variable star
21:39:40.89 +34:24:59.7 -- not a known variable star
21:39:53.76 +37:58:52.8 -- not a known variable star
21:40:11.20 +37:48:07.1 -- not a known variable star
21:40:12.45 +37:22:52.0 -- not a known variable star
21:40:12.88 +34:16:56.2 -- not a known variable star
21:40:15.55 +37:50:21.5 -- not a known variable star
21:40:19.76 +35:37:23.6 -- a known variable star
21:40:22.44 +39:00:37.6 -- not a known variable star
21:40:41.03 +36:19:20.7 -- not a known variable star
21:40:43.39 +37:37:29.1 -- not a known variable star
21:40:43.80 +37:23:00.4 -- not a known variable star
21:40:55.08 +37:27:31.1 -- not a known variable star
21:41:03.69 +37:41:57.4 -- not a known variable star
21:41:24.09 +39:05:05.1 -- not a known variable star
21:41:28.54 +34:59:55.2 -- not a known variable star
21:41:34.32 +34:36:23.6 -- not a known variable star
21:42:07.42 +39:04:10.8 -- not a known variable star
21:42:09.63 +36:32:21.6 -- not a known variable star
21:42:10.93 +39:16:11.0 -- not a known variable star
21:42:11.57 +36:19:08.9 -- a known variable star
21:42:14.31 +37:22:59.4 -- not a known variable star
21:42:21.27 +38:13:08.4 -- not a known variable star
21:42:31.24 +35:51:14.2 -- not a known variable star
21:42:33.76 +41:45:51.2 -- not a known variable star
21:43:00.40 +34:57:39.2 -- not a known variable star
21:43:02.43 +34:00:50.1 -- not a known variable star
21:43:05.94 +37:32:43.6 -- not a known variable star
21:43:07.95 +37:05:02.1 -- a known variable star
21:43:08.73 +40:49:38.0 -- not a known variable star
21:43:12.83 +35:46:27.1 -- not a known variable star
21:43:18.36 +39:30:22.8 -- not a known variable star
21:43:18.88 +42:12:56.5 -- not a known variable star
21:43:25.64 +36:45:53.6 -- not a known variable star
21:43:44.26 +34:49:10.4 -- not a known variable star
21:43:45.89 +35:25:54.1 -- not a known variable star
21:44:03.16 +37:47:35.8 -- not a known variable star
21:44:09.56 +37:55:03.4 -- not a known variable star
21:44:17.40 +36:34:05.3 -- a known variable star
21:44:26.00 +38:03:30.2 -- not a known variable star
21:44:30.95 +38:50:13.2 -- not a known variable star
21:44:34.94 +33:59:27.3 -- not a known variable star
21:44:35.13 +34:15:55.6 -- not a known variable star
21:44:35.61 +34:37:03.7 -- not a known variable star
21:44:37.46 +38:02:18.1 -- not a known variable star
21:44:37.79 +36:48:09.8 -- not a known variable star
21:45:03.10 +36:40:08.6 -- not a known variable star
21:45:05.81 +37:10:31.4 -- not a known variable star
21:45:15.69 +35:22:23.0 -- not a known variable star
21:45:18.26 +34:36:19.2 -- not a known variable star
21:45:57.25 +39:56:07.7 -- not a known variable star
21:45:58.86 +39:55:48.1 -- a known variable star
21:45:59.71 +34:32:51.9 -- not a known variable star
21:46:14.75 +37:25:08.7 -- not a known variable star
21:46:54.19 +39:15:20.8 -- not a known variable star
21:46:56.51 +37:17:28.1 -- not a known variable star
21:47:07.93 +39:07:42.5 -- a known variable star
21:47:28.68 +39:11:54.5 -- not a known variable star
21:47:31.96 +35:11:22.3 -- not a known variable star
21:47:33.64 +37:22:56.1 -- not a known variable star
21:47:39.91 +41:28:28.4 -- not a known variable star
21:47:59.25 +38:52:24.5 -- not a known variable star
21:48:07.30 +36:02:35.7 -- not a known variable star
21:48:31.26 +41:08:43.0 -- not a known variable star
21:48:31.76 +39:16:35.8 -- not a known variable star
21:48:34.08 +42:19:14.2 -- not a known variable star
21:48:39.20 +37:49:36.7 -- not a known variable star
21:48:46.74 +35:26:23.2 -- not a known variable star
21:48:53.93 +36:09:36.7 -- not a known variable star
21:48:54.48 +37:26:43.2 -- not a known variable star
21:48:57.03 +38:28:35.1 -- not a known variable star
21:48:57.14 +34:21:32.4 -- a known variable star
21:48:57.90 +37:42:53.1 -- not a known variable star
21:48:59.09 +35:21:20.3 -- not a known variable star
21:49:05.09 +37:22:34.0 -- not a known variable star
21:49:23.30 +36:27:43.5 -- not a known variable star
21:49:29.14 +36:55:04.6 -- not a known variable star
21:49:33.44 +39:24:22.7 -- not a known variable star
21:49:41.28 +37:43:30.9 -- not a known variable star
21:49:46.32 +40:24:29.2 -- not a known variable star
21:49:47.22 +34:12:11.0 -- not a known variable star
21:49:56.15 +36:30:34.0 -- not a known variable star
21:50:02.20 +37:36:18.4 -- not a known variable star
21:50:07.58 +42:10:53.8 -- not a known variable star
21:50:09.92 +40:20:09.6 -- not a known variable star
21:50:11.78 +38:02:34.9 -- not a known variable star
21:50:17.67 +42:04:59.5 -- a known variable star
21:50:23.40 +37:34:17.7 -- not a known variable star
21:50:24.73 +34:50:30.8 -- not a known variable star
21:50:25.14 +38:28:30.2 -- not a known variable star
21:50:31.56 +38:39:10.8 -- not a known variable star
21:50:34.31 +37:11:03.4 -- not a known variable star
21:50:35.53 +37:36:20.2 -- not a known variable star
21:50:40.99 +39:31:45.3 -- not a known variable star
21:50:41.89 +37:37:59.7 -- not a known variable star
21:50:44.43 +36:27:35.9 -- not a known variable star
21:50:58.46 +39:25:04.2 -- not a known variable star
21:50:58.71 +36:44:36.8 -- not a known variable star
21:51:11.60 +37:00:46.2 -- not a known variable star
21:51:16.57 +41:52:19.3 -- not a known variable star
21:51:39.60 +42:01:59.1 -- not a known variable star
21:51:39.69 +34:33:54.7 -- not a known variable star
21:51:40.04 +38:49:50.4 -- not a known variable star
21:51:40.80 +35:15:18.4 -- not a known variable star
21:51:41.33 +39:11:41.9 -- a known variable star
21:51:41.89 +34:07:05.8 -- not a known variable star
21:51:45.90 +37:59:55.3 -- not a known variable star
21:51:49.79 +37:26:02.0 -- a known variable star
21:51:54.16 +39:30:23.0 -- not a known variable star
21:51:57.54 +37:11:56.1 -- not a known variable star
21:52:00.27 +36:48:32.6 -- not a known variable star
21:52:04.60 +34:41:09.5 -- not a known variable star
21:52:13.78 +34:04:19.5 -- not a known variable star
21:52:15.38 +41:18:17.8 -- not a known variable star
21:52:15.51 +41:52:18.1 -- not a known variable star
21:52:19.85 +34:09:35.2 -- not a known variable star
21:52:45.52 +42:15:34.6 -- not a known variable star
21:52:57.02 +41:56:24.6 -- not a known variable star
21:52:58.87 +39:47:12.8 -- not a known variable star
21:53:00.60 +35:46:14.9 -- not a known variable star
21:53:14.90 +36:41:34.9 -- not a known variable star
21:53:17.50 +41:45:59.3 -- a known variable star
21:53:17.71 +39:27:53.4 -- not a known variable star
21:53:31.13 +33:46:50.1 -- a known variable star
21:53:44.10 +39:01:58.7 -- not a known variable star
21:53:53.60 +41:17:52.3 -- not a known variable star
21:54:13.78 +42:03:15.5 -- not a known variable star
21:54:14.01 +35:39:31.5 -- not a known variable star
21:54:17.27 +36:52:14.7 -- not a known variable star
21:54:18.94 +34:21:39.2 -- not a known variable star
21:54:32.73 +35:25:33.6 -- not a known variable star
21:54:38.63 +36:53:54.3 -- a known variable star
21:54:41.38 +41:37:13.6 -- not a known variable star
21:55:15.58 +37:52:02.2 -- not a known variable star
21:55:20.73 +34:39:48.1 -- not a known variable star
21:55:25.02 +39:42:15.4 -- not a known variable star
21:55:29.46 +39:55:36.7 -- not a known variable star
21:55:29.67 +36:36:05.8 -- not a known variable star
21:55:34.88 +36:37:37.0 -- not a known variable star
21:55:36.26 +35:51:33.8 -- not a known variable star
21:55:36.85 +38:47:54.9 -- not a known variable star
21:55:39.50 +36:53:22.5 -- not a known variable star
21:55:40.14 +42:12:52.4 -- a known variable star
21:55:46.12 +35:47:06.6 -- not a known variable star
21:55:49.63 +34:16:14.3 -- not a known variable star
21:55:53.83 +37:45:14.8 -- not a known variable star
21:55:57.26 +40:10:25.0 -- not a known variable star
21:56:00.49 +37:10:56.8 -- not a known variable star
21:56:01.47 +35:45:22.2 -- not a known variable star
21:56:14.98 +41:22:12.1 -- not a known variable star
21:56:21.42 +38:37:25.6 -- not a known variable star
21:56:29.02 +37:56:47.0 -- not a known variable star
21:56:29.21 +36:52:35.9 -- not a known variable star
21:56:34.45 +37:00:27.0 -- not a known variable star
21:56:38.98 +41:55:31.3 -- a known variable star
21:56:43.41 +41:51:09.7 -- not a known variable star
21:56:43.44 +37:32:19.1 -- not a known variable star
21:56:45.73 +40:47:17.4 -- not a known variable star
21:56:48.74 +40:07:52.5 -- not a known variable star
21:56:54.99 +41:26:11.6 -- not a known variable star
21:57:10.69 +42:10:42.9 -- not a known variable star
21:57:14.44 +42:01:04.2 -- not a known variable star
21:57:23.01 +41:48:54.3 -- not a known variable star
21:57:31.30 +38:48:29.4 -- not a known variable star
21:57:33.35 +41:16:30.9 -- not a known variable star
21:57:39.52 +41:25:20.8 -- not a known variable star
21:57:52.74 +34:06:47.3 -- not a known variable star
21:57:57.47 +34:05:54.2 -- not a known variable star
21:58:01.30 +38:57:27.6 -- not a known variable star
21:58:05.47 +36:02:57.0 -- not a known variable star
21:58:15.44 +33:46:39.2 -- not a known variable star
21:58:18.04 +34:23:37.9 -- not a known variable star
21:58:18.40 +39:26:01.3 -- not a known variable star
21:58:19.49 +37:12:23.5 -- not a known variable star
21:58:27.10 +41:39:27.4 -- not a known variable star
21:58:30.14 +36:23:05.3 -- not a known variable star
21:58:32.55 +37:54:59.4 -- not a known variable star
21:58:36.19 +41:09:24.0 -- not a known variable star
21:58:40.75 +35:20:14.8 -- not a known variable star
21:58:43.07 +42:11:58.0 -- not a known variable star
21:58:43.76 +39:44:50.6 -- not a known variable star
21:58:48.24 +40:45:29.0 -- not a known variable star
21:58:49.48 +40:53:49.1 -- not a known variable star
21:58:49.50 +40:28:43.6 -- not a known variable star
21:59:01.83 +36:26:59.1 -- not a known variable star
21:59:06.37 +34:00:18.2 -- not a known variable star
21:59:12.69 +42:08:23.3 -- not a known variable star
21:59:13.18 +42:19:04.5 -- not a known variable star
21:59:19.84 +39:44:23.1 -- not a known variable star
21:59:20.80 +39:40:39.1 -- not a known variable star
21:59:20.92 +36:56:49.6 -- not a known variable star
21:59:28.80 +37:59:47.4 -- not a known variable star
21:59:29.20 +39:40:34.1 -- not a known variable star
21:59:29.65 +36:02:35.0 -- not a known variable star
21:59:43.45 +35:08:54.3 -- not a known variable star
21:59:53.99 +34:16:51.1 -- not a known variable star
21:59:57.43 +36:55:02.7 -- not a known variable star
21:59:59.27 +36:08:34.1 -- not a known variable star
21:59:59.28 +38:04:07.7 -- not a known variable star
22:00:10.35 +38:33:14.2 -- not a known variable star
22:00:11.35 +39:37:39.9 -- not a known variable star
22:00:24.20 +35:58:54.0 -- not a known variable star
22:00:24.41 +39:57:07.7 -- a known variable star
22:00:26.18 +37:37:17.9 -- not a known variable star
22:00:30.51 +41:08:38.3 -- a known variable star
22:00:32.74 +41:01:59.0 -- a known variable star
22:00:33.04 +35:15:46.4 -- not a known variable star
22:00:48.39 +36:27:05.0 -- not a known variable star
22:00:55.83 +36:53:37.8 -- not a known variable star
22:01:04.06 +41:04:57.6 -- a known variable star
22:01:12.15 +35:17:06.7 -- not a known variable star
22:01:14.46 +38:33:47.2 -- not a known variable star
22:01:18.73 +41:30:28.0 -- not a known variable star
22:01:31.62 +37:57:47.2 -- not a known variable star
22:01:32.44 +34:05:01.2 -- not a known variable star
22:01:48.31 +39:56:08.6 -- not a known variable star
22:02:04.56 +37:45:27.6 -- not a known variable star
22:02:05.96 +36:06:27.4 -- a known variable star
22:02:11.35 +35:32:42.6 -- not a known variable star
22:02:13.89 +41:47:07.9 -- not a known variable star
22:02:14.84 +34:37:08.9 -- not a known variable star
22:02:16.99 +35:25:29.1 -- not a known variable star
22:02:19.99 +34:02:56.0 -- not a known variable star
22:02:22.22 +33:59:02.7 -- not a known variable star
22:02:22.56 +41:34:47.3 -- not a known variable star
22:02:38.66 +37:44:29.0 -- not a known variable star
22:02:38.78 +37:13:44.8 -- not a known variable star
22:02:42.09 +37:09:00.8 -- not a known variable star
22:02:42.59 +41:44:10.6 -- not a known variable star
22:02:54.20 +40:44:54.5 -- not a known variable star
22:02:54.61 +40:29:58.1 -- not a known variable star
22:02:56.21 +40:46:06.2 -- not a known variable star
22:03:08.32 +41:49:51.3 -- not a known variable star
22:03:12.09 +37:15:34.4 -- not a known variable star
22:03:45.00 +39:44:32.7 -- not a known variable star
22:03:45.74 +37:39:38.7 -- not a known variable star
22:04:28.27 +41:44:47.9 -- not a known variable star
22:04:30.42 +41:26:44.9 -- not a known variable star
22:04:41.19 +40:20:52.3 -- a known variable star
22:04:46.12 +42:08:02.3 -- not a known variable star
22:04:54.72 +35:49:32.8 -- not a known variable star
22:04:54.79 +40:37:24.8 -- a known variable star
22:05:03.22 +41:23:49.0 -- not a known variable star
22:05:11.32 +41:31:54.9 -- not a known variable star
22:05:26.20 +37:35:45.0 -- not a known variable star
22:05:26.98 +41:32:29.9 -- not a known variable star
22:05:32.42 +38:58:34.1 -- a known variable star
22:05:36.58 +41:17:42.1 -- not a known variable star
22:05:39.86 +34:53:39.2 -- a known variable star
22:05:41.20 +41:02:04.2 -- not a known variable star
22:05:42.75 +35:53:01.4 -- not a known variable star
22:06:01.48 +39:10:17.5 -- not a known variable star
22:06:03.46 +41:22:06.3 -- not a known variable star
22:06:06.12 +38:12:56.7 -- not a known variable star
22:06:09.36 +39:56:12.9 -- not a known variable star
22:06:12.38 +39:36:05.5 -- not a known variable star
22:06:23.67 +41:39:57.7 -- not a known variable star
22:06:29.23 +39:32:47.9 -- not a known variable star
22:06:31.88 +34:33:33.2 -- not a known variable star
22:06:38.32 +41:43:55.3 -- not a known variable star
22:06:54.87 +41:38:25.6 -- not a known variable star
22:07:10.81 +38:37:35.0 -- not a known variable star
22:07:19.28 +35:59:01.1 -- not a known variable star
22:07:19.75 +40:15:15.6 -- a known variable star
22:07:22.82 +40:35:20.9 -- not a known variable star
22:07:43.40 +37:37:06.9 -- not a known variable star
22:07:48.88 +34:48:04.2 -- not a known variable star
22:08:05.83 +41:53:32.3 -- a known variable star
22:08:10.51 +39:02:03.1 -- a known variable star
22:08:30.73 +37:04:05.1 -- not a known variable star
22:08:33.12 +35:58:49.2 -- not a known variable star
22:08:34.53 +37:33:23.8 -- not a known variable star
22:08:35.89 +37:44:55.1 -- not a known variable star
22:08:40.10 +38:50:08.0 -- a known variable star
22:09:04.27 +36:22:36.8 -- not a known variable star
22:09:09.62 +38:13:27.4 -- not a known variable star
22:09:11.52 +36:46:06.6 -- not a known variable star
22:09:32.18 +42:04:31.1 -- not a known variable star
22:09:33.60 +41:54:58.6 -- not a known variable star
22:09:47.58 +36:16:45.8 -- not a known variable star
22:09:48.87 +37:29:08.6 -- not a known variable star
22:09:49.48 +37:06:45.4 -- not a known variable star
22:09:56.44 +39:05:40.5 -- not a known variable star
22:10:04.13 +38:55:16.1 -- not a known variable star
22:10:13.66 +36:21:54.4 -- not a known variable star
22:10:15.72 +41:34:00.8 -- not a known variable star
22:10:18.73 +41:32:58.6 -- not a known variable star
22:10:20.04 +38:44:22.5 -- a known variable star
22:10:22.57 +40:43:10.2 -- not a known variable star
22:10:45.32 +40:14:53.9 -- not a known variable star
22:10:57.06 +37:02:42.5 -- not a known variable star
22:11:11.50 +41:48:09.4 -- not a known variable star
22:11:12.63 +37:18:42.5 -- not a known variable star
22:11:18.84 +39:15:07.6 -- not a known variable star
22:11:40.95 +38:00:40.6 -- not a known variable star
22:11:52.79 +40:52:48.9 -- not a known variable star
22:11:53.83 +39:29:36.8 -- a known variable star
Found 332 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
373 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 373 (excluding asteroids and hot pixels, 332 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461172.85766941 -observatory V36
03:04:44.67 +17:06:50.3 Mercury (-2.1mag)
05:23:06.96 +24:31:53.8 Venus (-3.9mag)
01:32:33.92 +08:48:20.5 Mars (1.2mag)
07:27:52.46 +22:18:09.3 Jupiter (-2.0mag)
00:40:15.39 +01:56:27.7 Saturn (0.9mag)
03:53:42.79 +20:06:15.0 Uranus (5.8mag)
00:13:57.14 +00:03:55.3 Neptune (7.8mag)
20:34:13.62 -22:56:17.7 Pluto (14.5mag)
23:27:30.38 -02:54:09.1 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 May 12 04:31 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461172.85766941:
07:27:47.22 +22:18:23.5 Io (5.9mag)
07:27:57.10 +22:17:55.5 Europa (6.1mag)
07:27:52.98 +22:18:14.4 Ganymede (5.5mag)
07:27:23.49 +22:19:22.5 Callisto (6.7mag)
07:29:48.11 +21:56:34.3 Himalia (15.5mag)
07:27:53.95 +22:18:04.0 Thebe (16.4mag)
07:30:16.09 +22:23:10.3 Elara (17.4mag)
07:28:29.97 +22:44:18.2 Pasiphae (17.6mag)
07:35:28.97 +22:18:08.8 Carme (18.7mag)
00:40:25.59 +01:56:14.9 Titan (8.7mag)
00:40:11.85 +01:56:40.3 Rhea (10.0mag)
00:40:05.79 +01:54:34.7 Iapetus (11.4mag)
00:40:05.82 +01:56:50.7 Hyperion (14.7mag)
00:41:28.07 +02:02:06.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 12 04:32 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461172.85766941:
16:59:28.36 -29:37:12.6 JWST
06:04:34.15 -28:48:59.6 Chandra
08:57:56.68 -50:54:26.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 12 04:31 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461172.85766941 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
07:49:29.59 +25:15:37.0 17.7mag P/2009 WX51 (Catalina)
18:55:20.43 -30:34:34.1 13.7mag P/2010 H2 (Vales)
05:28:08.87 -68:37:26.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:39:40.57 +31:39:33.8 17.4mag C/2017 K2 (PANSTARRS)
17:24:43.85 +13:23:29.5 17.7mag C/2021 G2 (ATLAS)
23:14:38.77 +30:24:20.4 17.2mag C/2022 E2 (ATLAS)
05:00:57.23 +26:38:49.0 16.3mag C/2022 N2 (PANSTARRS)
09:13:06.79 +31:49:13.7 16.4mag C/2022 QE78 (ATLAS)
08:38:11.31 +02:15:35.7 17.5mag C/2022 R6 (PANSTARRS)
18:43:55.59 +20:29:22.5 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:30:20.86 -11:09:29.4 17.5mag P/2023 B1 (PANSTARRS)
09:00:15.95 -08:10:48.7 17.9mag C/2023 F3 (ATLAS)
22:13:00.32 +64:40:07.6 17.6mag C/2023 H5 (Lemmon)
18:44:45.88 -04:37:06.4 13.8mag C/2023 R1 (PANSTARRS)
15:49:23.35 +88:04:12.7 17.9mag C/2023 X2 (Lemmon)
06:37:57.58 +63:39:07.2 17.4mag C/2024 A1 (ATLAS)
06:03:43.19 +24:31:57.3 12.5mag C/2024 E1 (Wierzchos)
15:59:26.82 +10:27:05.9 17.3mag C/2024 G6 (ATLAS)
20:23:13.06 +22:55:22.2 14.3mag C/2024 J3 (ATLAS)
03:51:16.55 -18:46:11.9 16.2mag C/2024 T5 (ATLAS)
05:40:35.10 +39:27:26.1 17.8mag C/2025 J1 (Borisov)
12:09:38.69 +53:12:35.7 16.4mag C/2025 L1 (ATLAS)
05:41:13.28 -08:05:17.1 10.5mag C/2025 R3 (PANSTARRS)
12:44:09.62 +04:16:59.9 17.3mag C/2025 Y1 (ATLAS)
05:28:53.21 +01:20:31.0 17.9mag C/2026 A1 (MAPS)
01:06:46.15 +41:00:35.7 15.4mag C/2026 B2 (Sun-Gao)
19:33:40.07 -08:23:21.3 10.3mag 10P/Tempel
14:28:08.58 -00:21:14.7 16.4mag 24P/Schaumasse
10:59:01.23 -00:56:02.0 15.8mag 29P/Schwassmann-Wachmann
10:43:29.32 -02:43:08.4 17.5mag 43P/Wolf-Harrington
02:29:48.26 +21:46:23.5 17.5mag 47P/Ashbrook-Jackson
08:03:06.84 +30:55:55.2 16.9mag 63P/Wild
00:00:26.26 -08:33:53.8 15.7mag 65P/Gunn
05:18:40.93 +28:54:42.4 16.2mag 76P/West-Kohoutek-Ikemura
02:05:25.40 +13:08:17.2 14.0mag 78P/Gehrels
00:16:51.21 -01:47:12.4 15.0mag 88P/Howell
03:29:01.92 +26:43:05.5 15.1mag 93P/Lovas
05:48:50.88 +33:15:27.5 15.9mag 123P/West-Hartley
09:05:28.18 +26:22:36.1 16.3mag 124P/Mrkos
03:15:02.40 +17:05:07.9 16.4mag 128P/Shoemaker-Holt
03:39:52.56 +17:16:30.7 17.6mag 131P/Mueller
03:48:14.67 +19:13:27.9 11.5mag 141P/Machholz
03:52:23.24 +13:34:44.1 11.4mag 141P-A/Machholz
02:32:49.31 +09:49:42.6 10.5mag 141P-D/Machholz
02:37:43.92 -29:02:52.4 17.7mag 161P/Hartley-IRAS
02:17:52.99 +11:41:56.9 14.9mag 162P/SidingSpring
17:11:44.52 -10:44:38.3 16.1mag 235P/LINEAR
06:33:24.22 +35:52:25.0 17.2mag 240P/NEAT
07:55:05.84 -02:50:23.6 18.0mag 242P/Spahr
23:23:14.04 -12:52:24.3 17.1mag 260P/McNaught
02:56:05.89 +26:51:52.5 17.8mag 295P/LINEAR
15:29:28.05 +08:13:53.9 17.4mag 391P/Kowalski
07:47:48.72 +21:15:01.3 17.8mag 450P/LONEOS
06:16:26.68 +43:28:05.7 17.7mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K May 12 04:31 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
12:59:50.45 -10:58:38.80 2026-05-9.06 17.5
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
12:59:50.45 -10:58:38.80 2026-05-9.06 17.5
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
-rw-r--r-- 1 apache apache 5.8K May 12 04:31 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
-rw-r--r-- 1 apache apache 188K May 12 04:31 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:59:36.274 +47:45:03.39 AT 2026lny 2026-04-29.38 19.5987
11:06:29.182 +44:51:04.29 AT 2026lnx 2026-05-06.32 18.654
12:25:50.354 +05:38:12.16 AT 2026lnw 2026-05-02.22 19.7726
16:59:22.419 +01:38:47.05 AT 2026lnv 2026-05-07.34 19.2961
10:41:49.538 -18:22:59.53 AT 2026lnu 2026-05-05.37 19.94
15:55:05.718 +01:53:48.70 AT 2026lnt 2026-05-07.33 18.2083
13:29:49.691 -05:45:05.96 SN 2026lns 2026-05-07.21 19.2662
15:08:03.565 +59:43:20.93 AT 2026lnr 2026-05-07.24 19.8187
13:19:56.192 +04:42:46.60 AT 2026lnq 2026-05-07.23 19.7266
13:42:37.932 +03:25:31.87 AT 2026lnp 2026-05-07.23 19.3378
13:05:48.294 -23:51:09.88 AT 2026lno 2026-05-07.23 19.2731
13:28:10.220 -24:58:07.02 AT 2026lnn 2026-05-07.23 19.1862
13:01:10.346 -26:29:29.03 AT 2026lnm 2026-05-07.21 19.8458
13:06:44.896 +73:12:18.55 AT 2026lnl 2026-05-07.22 18.8585
16:53:20.972 +24:45:10.02 AT 2026lnk 2026-04-29.39 20.1096
15:20:12.330 +05:17:27.37 AT 2026lnj 2026-04-23.40 20.1549
17:43:07.678 +22:57:21.39 AT 2026lni 2026-04-23.41 20.7995
16:52:47.004 +68:05:03.93 AT 2026lnh 2026-05-06.48 18.813
11:50:05.757 +07:28:43.49 AT 2026lng 2026-05-07.19 19.3993
10:13:11.650 +10:44:10.92 AT 2026lnf 2026-05-07.20 19.5524
-rw-r--r-- 1 apache apache 30K May 12 04:31 tns_transients_list.txt
