This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG
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 28.3851 2461188.8851 12.37 21:51:06.25 +37:29:04.1
87.74916 -12.77713 galactic Cyg Second-epoch detections are separated by 2.0" 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 | 21:51:06.25 +37:29:04.1 (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 21:51:06.25 +37:29:04.1: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:06.25 +37:29:04.1: 13.88 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.88 +/- 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,2461188.8851,12.37,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.06 21:48:41.00 +41:58:38.6
90.34035 -9.04464 galactic Cyg Second-epoch detections are separated by 4.9" 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 | 21:48:41.00 +41:58:38.6 (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 21:48:41.00 +41:58:38.6: 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 21:48:41.00 +41:58:38.6: 13.91 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.91 +/- 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,2461188.8851,12.06,0.05,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
target 20260528.3851 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 28.3851 2461188.8851 12.14 21:49:17.84 +40:40:26.6
89.57712 -10.11496 galactic Cyg 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 | target | 21:49:17.84 +40:40:26.6 (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 21:49:17.84 +40:40:26.6: 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 21:49:17.84 +40:40:26.6: 14.24 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.24 +/- 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,2461188.8851,12.14,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.29 21:59:58.68 +41:37:47.8
91.77602 -10.64148 galactic Lac Second-epoch detections are separated by 2.5" 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 | 21:59:58.68 +41:37:47.8 (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 21:59:58.68 +41:37:47.8: 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 21:59:58.68 +41:37:47.8: 14.43 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.43 +/- 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,2461188.8851,12.29,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.18 22:06:54.83 +41:38:24.1
92.83183 -11.41970 galactic Lac 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 | target | 22:06:54.83 +41:38:24.1 (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 22:06:54.83 +41:38:24.1: 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 22:06:54.83 +41:38:24.1: 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,2461188.8851,12.18,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.15 21:43:24.75 +37:27:40.3
86.55428 -11.79406 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 J325.8421+37.4582 | 21:43:24.75 +37:27:40.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.764+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:24.75 +37:27:40.3: 13.19 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:24.75 +37:27:40.3: 13.84 +/- 0.08 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 J325.8421+37.4582,2461188.8851,12.15,0.05,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 J325.8421+37.4582 20260528.3851 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 28.3851 2461188.8851 12.23 21:34:08.01 +36:35:12.1
84.55899 -11.18471 galactic Cyg Second-epoch detections are separated by 0.9" 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 | 21:34:08.01 +36:35:12.1 (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 21:34:08.01 +36:35:12.1: 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 21:34:08.01 +36:35:12.1: 14.17 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.17 +/- 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,2461188.8851,12.23,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.11 21:27:51.06 +36:06:23.5
83.29314 -10.64994 galactic Cyg Second-epoch detections are separated by 3.5" 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 | 21:27:51.06 +36:06:23.5 (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 21:27:51.06 +36:06:23.5: 12.33 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:51.06 +36:06:23.5: 14.02 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.32 +/- 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,2461188.8851,12.11,0.05,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
target 20260528.3851 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 28.3851 2461188.8851 12.12 21:57:31.17 +38:48:28.2
89.60965 -12.56022 galactic Cyg Second-epoch detections are separated by 2.7" 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 | 21:57:31.17 +38:48:28.2 (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 21:57:31.17 +38:48:28.2: 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 21:57:31.17 +38:48:28.2: 14.57 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.57 +/- 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 J329.3824+38.7999,2461188.8851,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 12.28 21:45:42.22 +41:54:53.3
89.87245 -8.73288 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 | ATO J326.4313+41.9264 | 21:45:42.22 +41:54:53.3 (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 21:45:42.22 +41:54:53.3: 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 21:45:42.22 +41:54:53.3: 14.35 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.35 +/- 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 J326.4313+41.9264,2461188.8851,12.28,0.05,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 J326.4313+41.9264 20260528.3851 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 28.3851 2461188.8851 12.36 21:58:37.93 +35:47:10.9
87.82942 -15.04819 galactic Peg 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 | 21:58:37.93 +35:47:10.9 (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 21:58:37.93 +35:47:10.9: 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 21:58:37.93 +35:47:10.9: 14.82 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.82 +/- 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,2461188.8851,12.36,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.12 21:45:02.91 +36:40:06.0
86.26557 -12.60369 galactic Cyg Second-epoch detections are separated by 2.0" 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 | 21:45:02.91 +36:40:06.0 (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 21:45:02.91 +36:40:06.0: 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 21:45:02.91 +36:40:06.0: 13.80 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.80 +/- 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,2461188.8851,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.93 21:47:07.79 +38:39:18.7
87.91957 -11.37905 galactic Cyg Second-epoch detections are separated by 2.9" 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 | 21:47:07.79 +38:39:18.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.258+/-0.042 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:07.79 +38:39:18.7: 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 21:47:07.79 +38:39:18.7: 13.93 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461188.8851,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 12.19 21:47:04.59 +40:58:26.8
89.44952 -9.61422 galactic Cyg Second-epoch detections are separated by 1.1" and 2.5 pix
The object was found in VSX 3" Gaia DR3 1954467547142058624
Type: ROT
# Max. Min./Amp. JD0 Period
14.520 G 14.570 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 21:47:04.59 +40:58:26.8: 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 21:47:04.59 +40:58:26.8: 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
Gaia DR3 1954467547142058624,2461188.8851,12.19,0.05,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 1954467547142058624 20260528.3851 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 28.3851 2461188.8851 11.94 21:53:53.81 +41:17:50.0
90.65996 -10.19012 galactic Cyg Second-epoch detections are separated by 1.6" 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 | 21:53:53.81 +41:17:50.0 (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 21:53:53.81 +41:17:50.0: 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 21:53:53.81 +41:17:50.0: 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,2461188.8851,11.94,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.95 21:34:19.66 +37:09:36.8
84.98930 -10.79484 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 | 21:34:19.66 +37:09:36.8 (user input) | T | P | (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 21:34:19.66 +37:09:36.8: 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 21:34:19.66 +37:09:36.8: 14.06 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461188.8851,11.95,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.04 21:50:15.92 +34:58:33.6
85.93908 -14.57381 galactic Peg Second-epoch detections are separated by 3.6" 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 | Gaia DR3 1949015859252113664 | 21:50:15.15 +34:58:57.7 (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 21:50:15.92 +34:58:33.6: 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 21:50:15.92 +34:58:33.6: 14.60 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.60 +/- 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 1949015859252113664,2461188.8851,12.04,0.05,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
Gaia DR3 1949015859252113664 20260528.3851 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 28.3851 2461188.8851 12.12 21:29:02.89 +40:09:05.6
86.32674 -7.91931 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 | 21:29:02.89 +40:09:05.6 (user input) | T | P | (position from user input) J-Ks=0.881+/-0.032 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:02.89 +40:09:05.6: 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 21:29:02.89 +40:09:05.6: 13.95 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.95 +/- 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,2461188.8851,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 12.12 21:36:44.06 +39:54:02.6
87.23583 -9.11078 galactic Cyg 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 | 21:36:44.06 +39:54:02.6 (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 21:36:44.06 +39:54:02.6: 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 21:36:44.06 +39:54:02.6: 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
target,2461188.8851,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.96 21:44:38.60 +38:02:23.9
87.13208 -11.52209 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 | 21:44:38.60 +38:02:23.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.665+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:38.60 +38:02:23.9: 12.84 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:38.60 +38:02:23.9: 14.03 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461188.8851,11.96,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.19 21:36:54.42 +37:55:38.0
85.90248 -10.58391 galactic Cyg 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 | 21:36:54.42 +37:55:38.0 (user input) | T | P | (position from user input) J-Ks=0.360+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:54.42 +37:55:38.0: 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 21:36:54.42 +37:55:38.0: 14.03 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461188.8851,12.19,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.85 21:39:53.77 +37:58:52.8
86.38172 -10.94234 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 | 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 21:39:53.77 +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 21:39:53.77 +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 1953496811513244032,2461188.8851,11.85,0.05,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 1953496811513244032 20260528.3851 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 28.3851 2461188.8851 11.90 21:40:07.72 +34:33:18.6
84.04963 -13.50103 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 | 21:40:07.72 +34:33:18.6 (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 21:40:07.72 +34:33:18.6: 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 21:40:07.72 +34:33:18.6: 14.43 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.43 +/- 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,2461188.8851,11.90,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.09 21:27:29.88 +38:47:35.3
85.15319 -8.68501 galactic Cyg Second-epoch detections are separated by 0.8" and 2.4 pix
The object was found in VSX18" Gaia DR3 1964465367711968768
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
18.730 G 18.990 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 21:27:29.88 +38:47:35.3: 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 21:27:29.88 +38:47:35.3: 14.27 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.27 +/- 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 1964465367711968768,2461188.8851,12.09,0.05,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 1964465367711968768 20260528.3851 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 28.3851 2461188.8851 11.80 21:27:35.74 +41:34:26.3
87.12462 -6.70588 galactic Cyg 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 J321.9055+41.5650 | 21:27:35.74 +41:34:26.3 (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 21:27:35.74 +41:34:26.3: 12.41 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:35.74 +41:34:26.3: 13.74 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.38 +/- 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 J321.9055+41.5650,2461188.8851,11.80,0.05,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
ATO J321.9055+41.5650 20260528.3851 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 28.3851 2461188.8851 11.91 21:31:28.79 +39:48:09.4
86.42272 -8.49354 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 | target | 21:31:28.79 +39:48:09.4 (user input) | T | P | (position from user input) J-Ks=0.705+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:28.79 +39:48:09.4: 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 21:31:28.79 +39:48:09.4: 13.98 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.98 +/- 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,2461188.8851,11.91,0.05,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
target 20260528.3851 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 28.3851 2461188.8851 11.95 21:35:26.39 +41:08:48.9
87.90683 -8.02760 galactic Cyg 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 | ATO J323.8637+41.1463 | 21:35:26.39 +41:08:48.9 (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 21:35:26.39 +41:08:48.9: 13.47 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:26.39 +41:08:48.9: 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 J323.8637+41.1463,2461188.8851,11.95,0.05,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
ATO J323.8637+41.1463 20260528.3851 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 28.3851 2461188.8851 11.76 21:42:09.02 +41:33:18.7
89.12799 -8.56839 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 J325.5362+41.5566 | 21:42:09.02 +41:33:18.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.469+/-0.049 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:09.02 +41:33:18.7: 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 21:42:09.02 +41:33:18.7: 13.48 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 J325.5362+41.5566,2461188.8851,11.76,0.05,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
ATO J325.5362+41.5566 20260528.3851 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 28.3851 2461188.8851 12.02 22:02:59.35 +41:26:45.6
92.11508 -11.13186 galactic Lac Second-epoch detections are separated by 3.7" 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 J330.7640+41.4473 | 22:03:03.37 +41:26:50.4 (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 22:02:59.35 +41:26:45.6: 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 22:02:59.35 +41:26:45.6: 14.32 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.32 +/- 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 J330.7640+41.4473,2461188.8851,12.02,0.05,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
ATO J330.7640+41.4473 20260528.3851 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 28.3851 2461188.8851 11.90 21:40:14.01 +36:18:19.9
85.28030 -12.22636 galactic Cyg Second-epoch detections are separated by 0.9" 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 | 21:40:14.01 +36:18:19.9 (user input) | T | P | (position from user input) J-Ks=0.736+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:14.01 +36:18:19.9: 12.72 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:14.01 +36:18:19.9: 14.14 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461188.8851,11.90,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.87 21:29:00.27 +38:59:29.9
85.50575 -8.74734 galactic Cyg Second-epoch detections are separated by 4.2" 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 | Large-amplitude variable Gaia DR2 1964564358128327936 | 21:29:00.27 +38:59:29.9 (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=0.358+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:00.27 +38:59:29.9: 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 21:29:00.27 +38:59:29.9: 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
Large-amplitude variable Gaia DR2 1964564358128327936,2461188.8851,11.87,0.05,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
Large-amplitude variable Gaia DR2 1964564358128327936 20260528.3851 11.87CV 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 28.3851 2461188.8851 12.05 21:37:48.52 +41:23:34.6
88.40622 -8.14678 galactic Cyg Second-epoch detections are separated by 1.1" 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 | 21:37:48.52 +41:23:34.6 (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 21:37:48.52 +41:23:34.6: 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 21:37:48.52 +41:23:34.6: 14.12 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.12 +/- 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,2461188.8851,12.05,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.77 21:42:06.53 +39:57:24.1
88.04878 -9.76010 galactic Cyg Second-epoch detections are separated by 1.8" 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 J325.5321+39.9657 | 21:42:06.53 +39:57:24.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.867+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:06.53 +39:57:24.1: 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 21:42:06.53 +39:57:24.1: 13.84 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.84 +/- 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 J325.5321+39.9657,2461188.8851,11.77,0.05,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 J325.5321+39.9657 20260528.3851 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 28.3851 2461188.8851 11.82 21:58:28.64 +40:10:15.9
90.62842 -11.61141 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 | ATO J329.6214+40.1726 | 21:58:28.64 +40:10:15.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.423+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:28.64 +40:10:15.9: 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 21:58:28.64 +40:10:15.9: 13.91 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 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 J329.6214+40.1726,2461188.8851,11.82,0.05,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
ATO J329.6214+40.1726 20260528.3851 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 28.3851 2461188.8851 11.71 21:41:28.44 +41:30:42.9
89.00312 -8.51695 galactic Cyg Second-epoch detections are separated by 1.4" 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 J325.3764+41.5141 | 21:41:28.44 +41:30:42.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.429+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:28.44 +41:30:42.9: 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 21:41:28.44 +41:30:42.9: 13.45 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.45 +/- 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 J325.3764+41.5141,2461188.8851,11.71,0.05,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 J325.3764+41.5141 20260528.3851 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 28.3851 2461188.8851 11.80 21:59:26.27 +37:53:39.1
89.32386 -13.50819 galactic Lac 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 | ATO J329.8779+37.8989 | 21:59:28.15 +37:53:59.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.894+/-0.030 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:26.27 +37:53:39.1: 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 21:59:26.27 +37:53:39.1: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 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 J329.8779+37.8989,2461188.8851,11.80,0.05,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
ATO J329.8779+37.8989 20260528.3851 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 28.3851 2461188.8851 11.83 21:48:31.19 +41:08:42.6
89.77212 -9.66041 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 | ATO J327.1211+41.1406 | 21:48:31.19 +41:08:42.6 (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 21:48:31.19 +41:08:42.6: 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 21:48:31.19 +41:08:42.6: 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
ATO J327.1211+41.1406,2461188.8851,11.83,0.05,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 J327.1211+41.1406 20260528.3851 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 28.3851 2461188.8851 11.99 21:44:03.08 +37:47:35.5
86.87600 -11.62978 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 | 21:44:03.08 +37:47:35.5 (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 21:44:03.08 +37:47:35.5: 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 21:44:03.08 +37:47:35.5: 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
target,2461188.8851,11.99,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.89 21:55:39.52 +36:53:21.5
88.07238 -13.81544 galactic Cyg 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 | 21:55:39.52 +36:53:21.5 (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 21:55:39.52 +36:53:21.5: 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 21:55:39.52 +36:53:21.5: 13.87 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.87 +/- 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,2461188.8851,11.89,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.99 21:39:43.16 +34:48:30.4
84.16274 -13.25789 galactic Cyg Second-epoch detections are separated by 0.9" 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 | 21:39:43.16 +34:48:30.4 (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 21:39:43.16 +34:48:30.4: 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 21:39:43.16 +34:48:30.4: 13.98 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.98 +/- 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,2461188.8851,11.99,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.87 22:05:37.35 +38:57:39.8
90.98055 -13.41196 galactic Lac Second-epoch detections are separated by 1.4" 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 | 22:05:37.35 +38:57:39.8 (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 22:05:37.35 +38:57:39.8: 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 22:05:37.35 +38:57:39.8: 13.71 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.71 +/- 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,2461188.8851,11.87,0.05,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
target 20260528.3851 11.87CV 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 28.3851 2461188.8851 11.77 21:49:03.69 +39:29:38.5
88.76619 -10.98614 galactic Cyg Second-epoch detections are separated by 2.9" 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 J327.2650+39.4941 | 21:49:03.69 +39:29:38.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.562+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:03.69 +39:29:38.5: 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 21:49:03.69 +39:29:38.5: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 J327.2650+39.4941,2461188.8851,11.77,0.05,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 J327.2650+39.4941 20260528.3851 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 28.3851 2461188.8851 11.61 21:38:23.51 +40:06:13.9
87.61194 -9.17506 galactic Cyg Second-epoch detections are separated by 2.8" 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 1966007123531818496 | 21:38:26.69 +40:06:12.2 (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 21:38:23.51 +40:06:13.9: 13.12 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:23.51 +40:06:13.9: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 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 1966007123531818496,2461188.8851,11.61,0.05,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
Gaia DR3 1966007123531818496 20260528.3851 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 28.3851 2461188.8851 11.77 21:31:19.30 +37:55:42.1
85.08889 -9.82764 galactic Cyg Second-epoch detections are separated by 2.2" 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 J322.8187+37.9342 | 21:31:19.30 +37:55:42.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.383+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:19.30 +37:55:42.1: 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 21:31:19.30 +37:55:42.1: 13.28 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 J322.8187+37.9342,2461188.8851,11.77,0.05,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 J322.8187+37.9342 20260528.3851 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 28.3851 2461188.8851 11.81 21:28:06.25 +33:41:27.5
81.59371 -12.40068 galactic Cyg Second-epoch detections are separated by 8.0" 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 | ATO J322.0376+33.6940 | 21:28:06.25 +33:41:27.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.486+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:06.25 +33:41:27.5: 12.00 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:06.25 +33:41:27.5: 13.87 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 J322.0376+33.6940,2461188.8851,11.81,0.05,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
ATO J322.0376+33.6940 20260528.3851 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 28.3851 2461188.8851 11.83 22:05:10.51 +37:28:20.7
89.97617 -14.54061 galactic Lac Second-epoch detections are separated by 2.0" 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 | 22:05:10.51 +37:28:20.7 (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 22:05:10.51 +37:28:20.7: 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 22:05:10.51 +37:28:20.7: 14.01 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.01 +/- 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,2461188.8851,11.83,0.05,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
target 20260528.3851 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 28.3851 2461188.8851 11.64 21:58:00.61 +37:39:31.2
88.94596 -13.51511 galactic Lac 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 | 21:58:00.61 +37:39:31.2 (user input) | T | P | (position from user input) J-Ks=0.272+/-0.035 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:00.61 +37:39:31.2: 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 21:58:00.61 +37:39:31.2: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.27 +/- 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
target,2461188.8851,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.46 21:30:54.99 +34:30:59.3
82.61140 -12.22247 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 | ATO J322.7144+34.5154 | 21:30:54.99 +34:30:59.3 (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 21:30:54.99 +34:30:59.3: 13.11 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:54.99 +34:30:59.3: 13.34 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.33 +/- 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+34.5154,2461188.8851,11.46,0.05,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 J322.7144+34.5154 20260528.3851 11.46CV 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 28.3851 2461188.8851 11.65 21:28:22.13 +41:32:01.6
87.20119 -6.83533 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 | ATO J322.0893+41.5337 | 21:28:22.13 +41:32:01.6 (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 21:28:22.13 +41:32:01.6: 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 21:28:22.13 +41:32:01.6: 13.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 J322.0893+41.5337,2461188.8851,11.65,0.05,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
ATO J322.0893+41.5337 20260528.3851 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 28.3851 2461188.8851 11.59 21:30:40.26 +41:59:21.8
87.83081 -6.80301 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 J322.6613+41.9895 | 21:30:40.26 +41:59:21.8 (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 21:30:40.26 +41:59:21.8: 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 21:30:40.26 +41:59:21.8: 13.61 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.61 +/- 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 J322.6613+41.9895,2461188.8851,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.6613+41.9895 20260528.3851 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.68 21:37:14.43 +35:50:17.4
84.50135 -12.15931 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 | ATO J324.3126+35.8461 | 21:37:13.72 +35:50:39.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.495+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:14.43 +35:50:17.4: 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 21:37:14.43 +35:50:17.4: 13.48 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 J324.3126+35.8461,2461188.8851,11.68,0.05,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
ATO J324.3126+35.8461 20260528.3851 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 28.3851 2461188.8851 11.62 22:03:59.35 +40:08:11.4
91.45539 -12.28657 galactic Lac Second-epoch detections are separated by 1.4" and 2.7 pix
The object was found in VSX 7" Gaia DR3 1956613381520278656
Type: ROT
# Max. Min./Amp. JD0 Period
14.510 G 14.540 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 22:03:59.35 +40:08:11.4: 13.32 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:59.35 +40:08:11.4: 13.51 +/- 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 1956613381520278656,2461188.8851,11.62,0.05,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 1956613381520278656 20260528.3851 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 28.3851 2461188.8851 11.64 21:51:46.23 +37:08:04.9
87.62120 -13.12976 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 | 21:51:46.23 +37:08:04.9 (user input) | T | P | (position from user input) J-Ks=0.645+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:46.23 +37:08:04.9: 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 21:51:46.23 +37:08:04.9: 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
target,2461188.8851,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.60 21:56:13.21 +35:31:23.9
87.26454 -14.94080 galactic Peg Second-epoch detections are separated by 1.1" and 2.3 pix
The object was found in VSX 1" Gaia DR3 1948367662787539968
Type: ROT
# Max. Min./Amp. JD0 Period
13.670 G 13.700 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 21:56:13.21 +35:31:23.9: 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 21:56:13.21 +35:31:23.9: 13.71 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 1948367662787539968,2461188.8851,11.60,0.05,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 1948367662787539968 20260528.3851 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 28.3851 2461188.8851 11.55 21:33:10.12 +41:39:57.2
87.94849 -7.35754 galactic Cyg 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 | 21:33:10.12 +41:39:57.2 (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 21:33:10.12 +41:39:57.2: 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 21:33:10.12 +41:39:57.2: 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
target,2461188.8851,11.55,0.05,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 20260528.3851 11.55CV 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 28.3851 2461188.8851 11.76 21:56:28.96 +37:56:46.4
88.89138 -13.10170 galactic Cyg Second-epoch detections are separated by 1.0" 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 | ATO J329.1061+37.9513 | 21:56:28.96 +37:56:46.4 (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 21:56:28.96 +37:56:46.4: 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 21:56:28.96 +37:56:46.4: 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
ATO J329.1061+37.9513,2461188.8851,11.76,0.05,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
ATO J329.1061+37.9513 20260528.3851 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 28.3851 2461188.8851 11.49 21:44:23.93 +37:43:55.7
86.88722 -11.72101 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 | Gaia DR3 1952764815946037760 | 21:44:23.62 +37:43:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:23.93 +37:43:55.7: 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 21:44:23.93 +37:43:55.7: 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
Gaia DR3 1952764815946037760,2461188.8851,11.49,0.05,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 1952764815946037760 20260528.3851 11.49CV 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 28.3851 2461188.8851 11.47 21:48:12.44 +41:41:11.1
90.08149 -9.20958 galactic Cyg Second-epoch detections are separated by 1.9" 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 1960503900338500992 | 21:48:14.24 +41:40:60.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.489+/-0.045 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:12.44 +41:41:11.1: 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 21:48:12.44 +41:41:11.1: 13.30 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 1960503900338500992,2461188.8851,11.47,0.05,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
Gaia DR3 1960503900338500992 20260528.3851 11.47CV 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 28.3851 2461188.8851 11.48 21:38:50.77 +35:08:49.5
84.26420 -12.88788 galactic Cyg Second-epoch detections are separated by 1.5" and 2.3 pix
The object was found in VSX22" NSVS J2138513+350911
Type: L:
# Max. Min./Amp. JD0 Period
10.605 R1 Y 0.457 R1 404.000000000000
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 21:38:50.77 +35:08:49.5: 13.33 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:50.77 +35:08:49.5: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.27 +/- 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
NSVS J2138513+350911,2461188.8851,11.48,0.05,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
NSVS J2138513+350911 20260528.3851 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 28.3851 2461188.8851 11.51 21:27:26.96 +35:34:46.7
82.85683 -10.96706 galactic Cyg Second-epoch detections are separated by 1.1" 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 | Gaia DR3 1951510513699055872 | 21:27:25.33 +35:35:12.3 (Gaia DR3) | T | P | 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 21:27:26.96 +35:34:46.7: 12.74 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:26.96 +35:34:46.7: 13.43 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 1951510513699055872,2461188.8851,11.51,0.05,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
Gaia DR3 1951510513699055872 20260528.3851 11.51CV 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 28.3851 2461188.8851 11.54 21:43:17.68 +38:29:47.6
87.23814 -11.00467 galactic Cyg Second-epoch detections are separated by 1.1" 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 J325.8236+38.4970 | 21:43:17.68 +38:29:47.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.680+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:17.68 +38:29:47.6: 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 21:43:17.68 +38:29:47.6: 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 J325.8236+38.4970,2461188.8851,11.54,0.05,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 J325.8236+38.4970 20260528.3851 11.54CV 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 28.3851 2461188.8851 11.64 21:30:43.77 +34:28:20.2
82.55160 -12.22713 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 | ATO J322.6902+34.4735 | 21:30:43.77 +34:28:20.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.384+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:43.77 +34:28:20.2: 12.56 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:43.77 +34:28:20.2: 13.76 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.50 +/- 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 J322.6902+34.4735,2461188.8851,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.6902+34.4735 20260528.3851 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.40 21:40:43.71 +37:22:58.9
86.09618 -11.49610 galactic Cyg Second-epoch detections are separated by 0.1" 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 J325.1759+37.3947 | 21:40:43.71 +37:22:58.9 (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 21:40:43.71 +37:22:58.9: 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 21:40:43.71 +37:22:58.9: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 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+37.3947,2461188.8851,11.40,0.05,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 J325.1759+37.3947 20260528.3851 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 28.3851 2461188.8851 11.62 21:33:57.71 +41:11:31.3
87.73191 -7.80538 galactic Cyg Second-epoch detections are separated by 3.4" and 2.0 pix
The object was found in VSX19" Gaia DR3 1966352340127500160
Type: ROT
# Max. Min./Amp. JD0 Period
15.970 G 16.040 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 21:33:57.71 +41:11:31.3: 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 21:33:57.71 +41:11:31.3: 13.48 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 1966352340127500160,2461188.8851,11.62,0.05,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 1966352340127500160 20260528.3851 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 28.3851 2461188.8851 11.57 21:39:48.72 +38:17:17.1
86.57920 -10.70413 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 | ATO J324.9588+38.2866 | 21:39:48.72 +38:17:17.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.759+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:48.72 +38:17:17.1: 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 21:39:48.72 +38:17:17.1: 13.28 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 J324.9588+38.2866,2461188.8851,11.57,0.05,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
ATO J324.9588+38.2866 20260528.3851 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 28.3851 2461188.8851 11.40 21:26:09.20 +40:15:19.5
86.00017 -7.45934 galactic Cyg 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 | ASASSN-V J212609.84+401448.8 | 21:26:10.64 +40:15:05.6 (Gaia DR3) | ROT: (local) | d (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.374+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:09.20 +40:15:19.5: 11.61 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:09.20 +40:15:19.5: 13.23 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.64 +/- 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
ASASSN-V J212609.84+401448.8,2461188.8851,11.40,0.05,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
ASASSN-V J212609.84+401448.8 20260528.3851 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 28.3851 2461188.8851 11.44 21:43:35.25 +37:12:37.5
86.41040 -12.00448 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 | ATO J325.8963+37.2123 | 21:43:35.25 +37:12:37.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.459+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:35.25 +37:12:37.5: 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 21:43:35.25 +37:12:37.5: 13.46 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.46 +/- 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 J325.8963+37.2123,2461188.8851,11.44,0.05,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
ATO J325.8963+37.2123 20260528.3851 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 28.3851 2461188.8851 11.29 21:32:48.36 +39:29:40.1
86.39572 -8.89280 galactic Cyg 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 | ATO J323.2117+39.4959 | 21:32:48.36 +39:29:40.1 (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 21:32:48.36 +39:29:40.1: 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 21:32:48.36 +39:29:40.1: 13.30 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 J323.2117+39.4959,2461188.8851,11.29,0.05,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
ATO J323.2117+39.4959 20260528.3851 11.29CV 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 28.3851 2461188.8851 11.39 22:06:48.50 +39:07:17.3
91.26883 -13.42316 galactic Lac Second-epoch detections are separated by 0.9" 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 J331.6984+39.1280 | 22:06:48.50 +39:07:17.3 (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 22:06:48.50 +39:07:17.3: 12.94 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:48.50 +39:07:17.3: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 J331.6984+39.1280,2461188.8851,11.39,0.05,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 J331.6984+39.1280 20260528.3851 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 28.3851 2461188.8851 11.38 21:29:37.11 +34:43:56.6
82.57101 -11.88134 galactic Cyg Second-epoch detections are separated by 5.2" and 2.8 pix
The object was found in VSX21" Gaia DR3 1951221548299261696
Type: ROT
# Max. Min./Amp. JD0 Period
14.470 G 14.500 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 21:29:37.11 +34:43:56.6: 11.73 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:37.11 +34:43:56.6: 13.77 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.66 +/- 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
Gaia DR3 1951221548299261696,2461188.8851,11.38,0.05,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
Gaia DR3 1951221548299261696 20260528.3851 11.38CV 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 28.3851 2461188.8851 11.34 21:34:13.43 +42:00:56.8
88.33390 -7.23548 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 | Gaia DR3 1967513939802011776 | 21:34:15.18 +42:01:10.0 (Gaia DR3) | DSCT/GDOR (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 21:34:13.43 +42:00:56.8: 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 21:34:13.43 +42:00:56.8: 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 1967513939802011776,2461188.8851,11.34,0.05,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 1967513939802011776 20260528.3851 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 28.3851 2461188.8851 11.32 22:01:22.36 +40:55:07.0
91.54109 -11.36361 galactic Lac Second-epoch detections are separated by 1.1" 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 J330.3389+40.9153 | 22:01:22.36 +40:55:07.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:22.36 +40:55:07.0: 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 22:01:22.36 +40:55:07.0: 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 J330.3389+40.9153,2461188.8851,11.32,0.05,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 J330.3389+40.9153 20260528.3851 11.32CV 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 28.3851 2461188.8851 11.23 21:40:56.27 +41:13:23.4
88.73310 -8.66598 galactic Cyg Second-epoch detections are separated by 1.6" 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 | ATO J325.2343+41.2229 | 21:40:56.27 +41:13:23.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.331+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:56.27 +41:13:23.4: 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 21:40:56.27 +41:13:23.4: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.15 +/- 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
ATO J325.2343+41.2229,2461188.8851,11.23,0.05,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 J325.2343+41.2229 20260528.3851 11.23CV 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 28.3851 2461188.8851 11.39 22:06:21.81 +39:23:02.5
91.36075 -13.16173 galactic Lac 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 | Gaia DR3 1956329054685443328 | 22:06:20.16 +39:22:54.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:21.81 +39:23:02.5: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:21.81 +39:23:02.5: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 1956329054685443328,2461188.8851,11.39,0.05,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
Gaia DR3 1956329054685443328 20260528.3851 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 28.3851 2461188.8851 11.23 21:58:41.91 +39:00:24.6
89.92051 -12.54850 galactic Lac Second-epoch detections are separated by 1.7" 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 1956095030507751168 | 21:58:40.43 +39:00:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.336+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:41.91 +39:00:24.6: 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 21:58:41.91 +39:00:24.6: 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 1956095030507751168,2461188.8851,11.23,0.05,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 1956095030507751168 20260528.3851 11.23CV 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 28.3851 2461188.8851 11.04 21:35:58.63 +38:02:59.5
85.85082 -10.36938 galactic Cyg Second-epoch detections are separated by 2.3" 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 | Gaia DR3 1952221343665700224 | 21:36:00.25 +38:03:13.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.808+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:58.63 +38:02:59.5: 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 21:35:58.63 +38:02:59.5: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 1952221343665700224,2461188.8851,11.04,0.05,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
Gaia DR3 1952221343665700224 20260528.3851 11.04CV 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 28.3851 2461188.8851 11.14 21:48:47.08 +40:08:12.8
89.14861 -10.46182 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 | ATO J327.1964+40.1375 | 21:48:43.45 +40:08:21.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-0.035 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:47.08 +40:08:12.8: 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 21:48:47.08 +40:08:12.8: 13.05 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.05 +/- 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
ATO J327.1964+40.1375,2461188.8851,11.14,0.05,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 J327.1964+40.1375 20260528.3851 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 28.3851 2461188.8851 11.19 21:26:50.66 +37:00:11.1
83.78769 -9.87028 galactic Cyg Second-epoch detections are separated by 1.0" and 2.5 pix
The object was found in VSX 5" 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 21:26:50.66 +37:00:11.1: 12.51 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:50.66 +37:00:11.1: 13.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 1963749143269434240,2461188.8851,11.19,0.05,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 1963749143269434240 20260528.3851 11.19CV 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 28.3851 2461188.8851 11.18 21:28:20.33 +39:05:27.1
85.48186 -8.58611 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 J322.0694+39.0850 | 21:28:19.24 +39:05:14.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.600+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:20.33 +39:05:27.1: 13.08 +/- 0.26 detection
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 +39:05:27.1: 12.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.71 +/- 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 J322.0694+39.0850,2461188.8851,11.18,0.05,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
ATO J322.0694+39.0850 20260528.3851 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 28.3851 2461188.8851 11.08 21:34:37.64 +34:15:57.0
82.99678 -12.93479 galactic Cyg Second-epoch detections are separated by 1.7" 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 | 21:34:37.64 +34:15:57.0 (user input) | T | P | (position from user input) J-Ks=0.500+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:37.64 +34:15:57.0: 13.11 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:37.64 +34:15:57.0: 13.23 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.23 +/- 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
target,2461188.8851,11.08,0.05,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 20260528.3851 11.08CV 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 28.3851 2461188.8851 11.04 22:11:02.22 +38:11:05.6
91.37458 -14.66743 galactic Lac Second-epoch detections are separated by 2.2" 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 1955415905978584576 | 22:11:03.83 +38:11:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.358+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:02.22 +38:11:05.6: 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 22:11:02.22 +38:11:05.6: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 1955415905978584576,2461188.8851,11.04,0.05,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
Gaia DR3 1955415905978584576 20260528.3851 11.04CV 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 28.3851 2461188.8851 11.27 22:03:31.27 +39:03:21.3
90.70703 -13.08830 galactic Lac 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 J330.8768+39.0496 | 22:03:30.11 +39:03:10.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.248+/-0.035 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:31.27 +39:03:21.3: 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 22:03:31.27 +39:03:21.3: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 J330.8768+39.0496,2461188.8851,11.27,0.05,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
ATO J330.8768+39.0496 20260528.3851 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 28.3851 2461188.8851 11.23 22:10:31.99 +41:45:05.3
93.45493 -11.72996 galactic Lac Second-epoch detections are separated by 2.4" and 2.1 pix
The object was found in VSX 2" Gaia DR3 1958278935478930816
Type: ROT
# Max. Min./Amp. JD0 Period
13.370 G 13.410 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 22:10:31.99 +41:45:05.3: 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 22:10:31.99 +41:45:05.3: 13.31 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.31 +/- 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 1958278935478930816,2461188.8851,11.23,0.05,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 1958278935478930816 20260528.3851 11.23CV 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 28.3851 2461188.8851 11.02 22:00:14.34 +41:40:32.5
91.84377 -10.63544 galactic Lac 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 | ATO J330.0567+41.6700 | 22:00:14.34 +41:40:32.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:14.34 +41:40:32.5: 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 22:00:14.34 +41:40:32.5: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.01 +/- 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
ATO J330.0567+41.6700,2461188.8851,11.02,0.05,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
ATO J330.0567+41.6700 20260528.3851 11.02CV 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 28.3851 2461188.8851 11.14 22:02:11.36 +35:32:41.1
88.25635 -15.68920 galactic Peg Second-epoch detections are separated by 1.5" 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 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 22:02:11.36 +35:32:41.1: 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 22:02:11.36 +35:32:41.1: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.43 +/- 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 1948505887717109376,2461188.8851,11.14,0.05,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
Gaia DR3 1948505887717109376 20260528.3851 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 28.3851 2461188.8851 10.99 21:27:24.11 +33:39:56.7
81.46970 -12.31517 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 | Gaia DR3 1854304305596960256 | 21:27:21.99 +33:40:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.297+/-0.028 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:24.11 +33:39:56.7: 11.36 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:24.11 +33:39:56.7: 13.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.34 +/- 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 1854304305596960256,2461188.8851,10.99,0.05,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 1854304305596960256 20260528.3851 10.99CV 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 28.3851 2461188.8851 10.94 21:40:40.97 +36:19:19.9
85.36022 -12.27506 galactic Cyg Second-epoch detections are separated by 1.1" 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 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 21:40:40.97 +36:19:19.9: 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 21:40:40.97 +36:19:19.9: 12.76 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.76 +/- 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+36.3226,2461188.8851,10.94,0.05,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 20260528.3851 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 28.3851 2461188.8851 10.78 21:31:28.70 +38:53:30.8
85.78673 -9.15268 galactic Cyg Second-epoch detections are separated by 2.4" and 2.3 pix
The object was found in VSX 2" ASASSN-V J213128.73+385333.1
Type: L
# Max. Min./Amp. JD0 Period
12.380 V 12.510 V
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 21:31:28.70 +38:53:30.8: 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 21:31:28.70 +38:53:30.8: 12.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.26 +/- 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
ASASSN-V J213128.73+385333.1,2461188.8851,10.78,0.05,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
ASASSN-V J213128.73+385333.1 20260528.3851 10.78CV 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 28.3851 2461188.8851 10.90 22:05:39.85 +34:53:38.1
88.41780 -16.63956 galactic Peg Second-epoch detections are separated by 0.5" and 2.5 pix
The object was found in VSX20" 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 22:05:39.85 +34:53:38.1: 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 22:05:39.85 +34:53:38.1: 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 1900468744392395008,2461188.8851,10.90,0.05,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 1900468744392395008 20260528.3851 10.90CV 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 28.3851 2461188.8851 10.79 21:51:51.69 +41:19:45.6
90.38085 -9.92259 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 | 21:51:51.69 +41:19:45.6 (user input) | T | P | (position from user input) J-Ks=0.798+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:51.69 +41:19:45.6: 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 21:51:51.69 +41:19:45.6: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 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,2461188.8851,10.79,0.05,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 20260528.3851 10.79CV 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 28.3851 2461188.8851 10.79 21:59:20.89 +36:56:48.2
88.69925 -14.23642 galactic Lac 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 | 21:59:20.89 +36:56:48.2 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:20.89 +36:56:48.2: 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 21:59:20.89 +36:56:48.2: 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
target,2461188.8851,10.79,0.05,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 20260528.3851 10.79CV 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 28.3851 2461188.8851 10.66 21:33:13.71 +37:12:42.7
84.86374 -10.60677 galactic Cyg Second-epoch detections are separated by 0.9" 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 21:33:13.71 +37:12:42.7: 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 21:33:13.71 +37:12:42.7: 12.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.69 +/- 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 1952077135843691520,2461188.8851,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 10.62 22:06:01.44 +39:10:16.5
91.17502 -13.29173 galactic Lac Second-epoch detections are separated by 1.9" 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 | 22:06:01.44 +39:10:16.5 (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 22:06:01.44 +39:10:16.5: 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 22:06:01.44 +39:10:16.5: 12.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.83 +/- 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,2461188.8851,10.62,0.05,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
target 20260528.3851 10.62CV 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 28.3851 2461188.8851 10.69 21:46:25.62 +39:38:17.9
88.46939 -10.54616 galactic Cyg Second-epoch detections are separated by 1.4" 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 | Gaia DR3 1954064507410070656 | 21:46:27.00 +39:38:12.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.830+/-0.032 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:25.62 +39:38:17.9: 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 21:46:25.62 +39:38:17.9: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 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 1954064507410070656,2461188.8851,10.69,0.05,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 1954064507410070656 20260528.3851 10.69CV 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 28.3851 2461188.8851 10.66 21:37:46.88 +36:44:33.3
85.21220 -11.57117 galactic Cyg Second-epoch detections are separated by 1.0" and 2.3 pix
The object was found in VSX23" ASASSN-V J213745.82+364414.6
Type: L
# Max. Min./Amp. JD0 Period
11.610 V 11.730 V
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 21:37:46.88 +36:44:33.3: 13.30 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:46.88 +36:44:33.3: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 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
ASASSN-V J213745.82+364414.6,2461188.8851,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J213745.82+364414.6 20260528.3851 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 10.63 21:28:11.90 +34:45:20.1
82.37567 -11.65980 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 | Gaia DR3 1951212820925260928 | 21:28:12.04 +34:44:37.9 (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 21:28:11.90 +34:45:20.1: 10.79 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:11.90 +34:45:20.1: 12.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.65 +/- 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 1951212820925260928,2461188.8851,10.63,0.05,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
Gaia DR3 1951212820925260928 20260528.3851 10.63CV 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 28.3851 2461188.8851 10.71 21:27:20.09 +35:46:48.3
82.98382 -10.80842 galactic Cyg Second-epoch detections are separated by 2.7" 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 1951517935397882496 | 21:27:20.07 +35:47:12.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.482+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:20.09 +35:46:48.3: 11.25 +/- 0.05 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:20.09 +35:46:48.3: 12.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.21 +/- 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 1951517935397882496,2461188.8851,10.71,0.05,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
Gaia DR3 1951517935397882496 20260528.3851 10.71CV 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 28.3851 2461188.8851 10.46 21:30:31.96 +35:46:44.6
83.45438 -11.26376 galactic Cyg Second-epoch detections are separated by 0.9" 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 | 21:30:31.96 +35:46:44.6 (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 21:30:31.96 +35:46:44.6: 12.67 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:31.96 +35:46:44.6: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 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,2461188.8851,10.46,0.05,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 20260528.3851 10.46CV 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 28.3851 2461188.8851 10.46 21:59:33.49 +41:27:38.5
91.60687 -10.72626 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 1959925282343117056 | 21:59:31.92 +41:27:29.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.384+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:33.49 +41:27:38.5: 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 21:59:33.49 +41:27:38.5: 12.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.06 +/- 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 1959925282343117056,2461188.8851,10.46,0.05,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
Gaia DR3 1959925282343117056 20260528.3851 10.46CV 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 28.3851 2461188.8851 10.18 21:28:41.97 +34:20:03.0
82.14733 -12.03169 galactic Cyg Second-epoch detections are separated by 0.9" and 2.5 pix
The object was found in VSX22" ASASSN-V J212841.40+341941.9
Type: SR
# Max. Min./Amp. JD0 Period
12.670 g Y 0.180 g 2459377.90500 104.000000000000
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 21:28:41.97 +34:20:03.0: 10.19 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:41.97 +34:20:03.0: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.20 +/- 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
ASASSN-V J212841.40+341941.9,2461188.8851,10.18,0.05,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
ASASSN-V J212841.40+341941.9 20260528.3851 10.18CV 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 28.3851 2461188.8851 10.25 22:01:26.27 +38:07:01.0
89.78374 -13.57849 galactic Lac Second-epoch detections are separated by 0.9" 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 | 22:01:26.27 +38:07:01.0 (user input) | T | P | (position from user input) J-Ks=0.633+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:26.27 +38:07:01.0: 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 22:01:26.27 +38:07:01.0: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 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,2461188.8851,10.25,0.05,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 20260528.3851 10.25CV 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 28.3851 2461188.8851 10.07 21:41:57.33 +40:22:13.9
88.30520 -9.43117 galactic Cyg Second-epoch detections are separated by 0.4" 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 | Gaia DR3 1954390886263865600 | 21:41:58.76 +40:22:22.1 (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 21:41:57.33 +40:22:13.9: 11.34 +/- 0.05 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:57.33 +40:22:13.9: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 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 1954390886263865600,2461188.8851,10.07,0.05,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
Gaia DR3 1954390886263865600 20260528.3851 10.07CV 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 28.3851 2461188.8851 9.91 21:29:15.48 +38:35:05.1
85.25505 -9.07392 galactic Cyg Second-epoch detections are separated by 2.0" 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 | Gaia DR3 1964351503842249472 | 21:29:16.83 +38:35:14.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.255+/-0.031 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:15.48 +38:35:05.1: 12.99 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:15.48 +38:35:05.1: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 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 1964351503842249472,2461188.8851,9.91,0.05,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 1964351503842249472 20260528.3851 9.91CV 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 28.3851 2461188.8851 10.02 21:57:16.71 +37:31:04.8
88.73905 -13.53316 galactic Cyg 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 | Gaia DR3 1949929308597009664 | 21:57:18.11 +37:31:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6V 2000ApJ...541..841A GSC 3185-1968
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:16.71 +37:31:04.8: 13.45 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:16.71 +37:31:04.8: 12.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.00 +/- 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 1949929308597009664,2461188.8851,10.02,0.05,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 1949929308597009664 20260528.3851 10.02CV 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 28.3851 2461188.8851 9.68 21:29:30.58 +37:27:31.5
84.49605 -9.91650 galactic Cyg Second-epoch detections are separated by 1.6" 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 1952133971151570816 | 21:29:30.77 +37:27:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.266+/-0.034 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:30.58 +37:27:31.5: 12.27 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:30.58 +37:27:31.5: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 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 1952133971151570816,2461188.8851,9.68,0.05,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
Gaia DR3 1952133971151570816 20260528.3851 9.68CV 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 28.3851 2461188.8851 9.68 22:01:18.65 +41:30:27.0
91.89967 -10.89125 galactic Lac Second-epoch detections are separated by 0.6" 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 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 22:01:18.65 +41:30:27.0: 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 22:01:18.65 +41:30:27.0: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 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 1959759393525967360,2461188.8851,9.68,0.05,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
Gaia DR3 1959759393525967360 20260528.3851 9.68CV 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 28.3851 2461188.8851 9.77 21:59:06.38 +34:00:17.5
86.73695 -16.48969 galactic Peg 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 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 21:59:06.38 +34:00:17.5: 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 21:59:06.38 +34:00:17.5: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 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 1947975824331378048,2461188.8851,9.77,0.05,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 1947975824331378048 20260528.3851 9.77CV 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 28.3851 2461188.8851 9.48 21:34:29.33 +39:23:37.9
86.56572 -9.18858 galactic Cyg Second-epoch detections are separated by 1.4" 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 | Gaia DR3 1965875770554661504 | 21:34:28.39 +39:23:25.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.762+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:29.33 +39:23:37.9: 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 21:34:29.33 +39:23:37.9: 11.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 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 1965875770554661504,2461188.8851,9.48,0.05,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
Gaia DR3 1965875770554661504 20260528.3851 9.48CV 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 28.3851 2461188.8851 9.40 21:31:14.96 +38:46:29.2
85.67212 -9.20655 galactic Cyg Second-epoch detections are separated by 1.7" and 2.2 pix
The object was found in VSX 3" V2072 Cyg
Type: M
# Max. Min./Amp. JD0 Period
10.400 V 17.900 V 2451388.00000 317.100000000000
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 21:31:14.96 +38:46:29.2: 12.67 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:14.96 +38:46:29.2: 12.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.86 +/- 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
V2072 Cyg,2461188.8851,9.40,0.05,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
V2072 Cyg 20260528.3851 9.40CV 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 28.3851 2461188.8851 10.04 21:42:51.25 +37:54:04.8
86.76900 -11.39196 galactic Cyg Second-epoch detections are separated by 1.8" 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 J325.7134+37.9017 | 21:42:51.22 +37:54:06.3 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.234+/-0.039 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:51.25 +37:54:04.8: 13.35 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:51.25 +37:54:04.8: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 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 J325.7134+37.9017,2461188.8851,10.04,0.05,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
ATO J325.7134+37.9017 20260528.3851 10.04CV 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 28.3851 2461188.8851 10.55 21:44:42.92 +35:29:06.6
85.40736 -13.44352 galactic Cyg Second-epoch detections are separated by 1.9" and 2.5 pix
The object was found in VSX 1" ASASSN-V J214442.97+352907.2
Type: SR
# Max. Min./Amp. JD0 Period
14.180 g Y 0.300 g 2458641.96400 41.070000000000
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 21:44:42.92 +35:29:06.6: 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 21:44:42.92 +35:29:06.6: 12.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.34 +/- 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
ASASSN-V J214442.97+352907.2,2461188.8851,10.55,0.05,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
ASASSN-V J214442.97+352907.2 20260528.3851 10.55CV 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 28.3851 2461188.8851 10.44 22:09:13.48 +39:15:45.4
91.74139 -13.59044 galactic Lac 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 | Gaia DR3 1956289747146754688 | 22:09:11.61 +39:15:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.504+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:13.48 +39:15:45.4: 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 22:09:13.48 +39:15:45.4: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 1956289747146754688,2461188.8851,10.44,0.05,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 1956289747146754688 20260528.3851 10.44CV 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 28.3851 2461188.8851 10.80 22:02:13.90 +41:47:06.4
92.21105 -10.77667 galactic Lac 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 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 22:02:13.90 +41:47:06.4: 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 22:02:13.90 +41:47:06.4: 12.81 +/- 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 J330.5515+41.7805,2461188.8851,10.80,0.05,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 J330.5515+41.7805 20260528.3851 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 28.3851 2461188.8851 10.92 21:44:09.46 +37:55:02.4
86.97602 -11.55071 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 | 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 21:44:09.46 +37:55:02.4: 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 21:44:09.46 +37:55:02.4: 12.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.74 +/- 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+37.9120,2461188.8851,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 10.90 21:42:12.45 +38:54:23.1
87.35399 -10.55743 galactic Cyg Second-epoch detections are separated by 1.5" and 2.4 pix
The object was found in VSX 3" ZTF J214212.23+385425.2
Type: RS:
# Max. Min./Amp. JD0 Period
13.756 r Y 0.081 r 2458607.86350 0.150071000000
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 21:42:12.45 +38:54:23.1: 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 21:42:12.45 +38:54:23.1: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.15 +/- 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
ZTF J214212.23+385425.2,2461188.8851,10.90,0.05,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
ZTF J214212.23+385425.2 20260528.3851 10.90CV 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 28.3851 2461188.8851 11.05 21:44:26.49 +41:28:25.9
89.40018 -8.91218 galactic Cyg Second-epoch detections are separated by 1.0" 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 | Gaia DR3 1954551797221475456 | 21:44:29.47 +41:28:29.3 (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 21:44:26.49 +41:28:25.9: 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 21:44:26.49 +41:28:25.9: 13.32 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 1954551797221475456,2461188.8851,11.05,0.05,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
Gaia DR3 1954551797221475456 20260528.3851 11.05CV 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 28.3851 2461188.8851 11.22 22:02:14.79 +34:37:06.2
87.66498 -16.42085 galactic Peg Second-epoch detections are separated by 3.1" 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 J330.5676+34.6142 | 22:02:16.63 +34:36:26.3 (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 22:02:14.79 +34:37:06.2: 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 22:02:14.79 +34:37:06.2: 13.46 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.46 +/- 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+34.6142,2461188.8851,11.22,0.05,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
ATO J330.5676+34.6142 20260528.3851 11.22CV 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 28.3851 2461188.8851 11.35 21:43:31.53 +35:02:27.4
84.91634 -13.61210 galactic Cyg Second-epoch detections are separated by 2.3" 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 | Gaia DR3 1947764099624781184 | 21:43:29.81 +35:02:12.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.443+/-0.065 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:31.53 +35:02:27.4: 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 21:43:31.53 +35:02:27.4: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 1947764099624781184,2461188.8851,11.35,0.05,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
Gaia DR3 1947764099624781184 20260528.3851 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 28.3851 2461188.8851 11.35 21:53:19.48 +36:06:08.2
87.18201 -14.12019 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 | ATO J328.3318+36.1032 | 21:53:19.48 +36:06:08.2 (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 21:53:19.48 +36:06:08.2: 13.21 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:19.48 +36:06:08.2: 13.73 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 J328.3318+36.1032,2461188.8851,11.35,0.05,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 J328.3318+36.1032 20260528.3851 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 28.3851 2461188.8851 11.35 21:44:06.73 +37:26:46.3
86.65017 -11.89750 galactic Cyg 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 | Gaia DR3 1952751759248047232 | 21:44:07.88 +37:27:17.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:06.73 +37:26:46.3: 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 21:44:06.73 +37:26:46.3: 13.61 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.61 +/- 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 1952751759248047232,2461188.8851,11.35,0.05,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
Gaia DR3 1952751759248047232 20260528.3851 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 28.3851 2461188.8851 11.46 22:06:31.80 +34:33:31.3
88.34942 -17.01338 galactic Peg Second-epoch detections are separated by 1.8" 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 | 22:06:31.80 +34:33:31.3 (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 22:06:31.80 +34:33:31.3: 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 22:06:31.80 +34:33:31.3: 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
target,2461188.8851,11.46,0.05,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 20260528.3851 11.46CV 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 28.3851 2461188.8851 11.32 22:02:42.44 +41:44:09.0
92.25211 -10.86978 galactic Lac Second-epoch detections are separated by 0.8" 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 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 22:02:42.44 +41:44:09.0: 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 22:02:42.44 +41:44:09.0: 13.59 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 1959859277284333312,2461188.8851,11.32,0.05,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
Gaia DR3 1959859277284333312 20260528.3851 11.32CV 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 28.3851 2461188.8851 11.48 21:29:41.53 +38:48:30.5
85.47420 -8.97201 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 J322.4223+38.8106 | 21:29:40.43 +38:49:03.5 (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 21:29:41.53 +38:48:30.5: 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 21:29:41.53 +38:48:30.5: 13.82 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.82 +/- 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 J322.4223+38.8106,2461188.8851,11.48,0.05,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 J322.4223+38.8106 20260528.3851 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 28.3851 2461188.8851 11.47 21:57:42.00 +40:41:31.7
90.84151 -11.11168 galactic Lac 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 | Gaia DR3 1959523479562430976 | 21:57:44.16 +40:41:26.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.409+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:42.00 +40:41:31.7: 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 21:57:42.00 +40:41:31.7: 12.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 1959523479562430976,2461188.8851,11.47,0.05,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
Gaia DR3 1959523479562430976 20260528.3851 11.47CV 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 28.3851 2461188.8851 11.48 22:05:01.98 +41:27:43.6
92.43577 -11.35091 galactic Lac Second-epoch detections are separated by 3.9" 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 J331.2733+41.4646 | 22:05:01.98 +41:27:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.327+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:01.98 +41:27:43.6: 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 22:05:01.98 +41:27:43.6: 14.01 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.01 +/- 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 J331.2733+41.4646,2461188.8851,11.48,0.05,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 J331.2733+41.4646 20260528.3851 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 28.3851 2461188.8851 11.52 22:04:59.74 +39:57:17.2
91.49930 -12.54789 galactic Lac Second-epoch detections are separated by 0.5" and 2.5 pix
The object was found in VSX 2" Gaia DR3 1956561223437486208
Type: ROT
# Max. Min./Amp. JD0 Period
13.720 G 13.750 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 22:04:59.74 +39:57:17.2: 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 22:04:59.74 +39:57:17.2: 13.54 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 1956561223437486208,2461188.8851,11.52,0.05,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
Gaia DR3 1956561223437486208 20260528.3851 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 28.3851 2461188.8851 11.54 22:09:46.14 +41:39:55.4
93.28542 -11.71570 galactic Lac Second-epoch detections are separated by 0.1" 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 1958254196465679360 | 22:09:49.52 +41:39:34.9 (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 22:09:46.14 +41:39:55.4: 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 22:09:46.14 +41:39:55.4: 13.79 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.79 +/- 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 1958254196465679360,2461188.8851,11.54,0.05,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 1958254196465679360 20260528.3851 11.54CV 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 28.3851 2461188.8851 11.55 22:02:04.69 +37:45:26.0
89.65701 -13.93931 galactic Lac Second-epoch detections are separated by 1.1" 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 | 22:02:04.69 +37:45:26.0 (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 22:02:04.69 +37:45:26.0: 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 22:02:04.69 +37:45:26.0: 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,2461188.8851,11.55,0.05,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 20260528.3851 11.55CV 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 28.3851 2461188.8851 11.43 21:39:00.59 +38:41:33.2
86.73782 -10.29926 galactic Cyg Second-epoch detections are separated by 1.4" 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 J324.7488+38.6969 | 21:38:58.77 +38:41:57.6 (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 21:39:00.59 +38:41:33.2: 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 21:39:00.59 +38:41:33.2: 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 J324.7488+38.6969,2461188.8851,11.43,0.05,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 J324.7488+38.6969 20260528.3851 11.43CV 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 28.3851 2461188.8851 11.49 21:47:33.59 +37:22:54.8
87.13334 -12.39718 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 | 21:47:33.59 +37:22:54.8 (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 21:47:33.59 +37:22:54.8: 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 21:47:33.59 +37:22:54.8: 13.84 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461188.8851,11.49,0.05,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 20260528.3851 11.49CV 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 28.3851 2461188.8851 11.53 21:49:41.22 +37:43:27.7
87.68927 -12.41255 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 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 21:49:41.22 +37:43:27.7: 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 21:49:41.22 +37:43:27.7: 13.83 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 J327.4213+37.7226,2461188.8851,11.53,0.05,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 J327.4213+37.7226 20260528.3851 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 28.3851 2461188.8851 11.46 21:40:47.54 +37:32:55.6
86.21928 -11.38175 galactic Cyg Second-epoch detections are separated by 1.1" 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 | Gaia DR3 1953471527045546752 | 21:40:46.82 +37:33:21.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=0.770+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:47.54 +37:32:55.6: 12.59 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:47.54 +37:32:55.6: 13.56 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 1953471527045546752,2461188.8851,11.46,0.05,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
Gaia DR3 1953471527045546752 20260528.3851 11.46CV 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 28.3851 2461188.8851 11.56 21:47:48.83 +38:11:35.7
87.71494 -11.81627 galactic Cyg Second-epoch detections are separated by 4.9" and 1.8 pix
The object was found in VSX 9" Gaia DR3 1953161975863304576
Type: RS
# Max. Min./Amp. JD0 Period
17.500 G 17.720 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 21:47:48.83 +38:11:35.7: 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 21:47:48.83 +38:11:35.7: 14.06 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 1953161975863304576,2461188.8851,11.56,0.05,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
Gaia DR3 1953161975863304576 20260528.3851 11.56CV 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 28.3851 2461188.8851 11.63 21:27:14.50 +36:18:38.9
83.35038 -10.41827 galactic Cyg Second-epoch detections are separated by 1.7" 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 J321.7938+36.3044 | 21:27:13.08 +36:18:13.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE 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 21:27:14.50 +36:18:38.9: 12.13 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:14.50 +36:18:38.9: 13.78 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 J321.7938+36.3044,2461188.8851,11.63,0.05,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 J321.7938+36.3044 20260528.3851 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 28.3851 2461188.8851 11.57 21:32:00.66 +39:23:57.8
86.21676 -8.85631 galactic Cyg Second-epoch detections are separated by 0.7" and 2.4 pix
The object was found in VSX21" ZTF J213202.41+392353.1
Type: RS
# Max. Min./Amp. JD0 Period
16.910 r Y 0.103 r 2458456.64000 0.223017700000
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 21:32:00.66 +39:23:57.8: 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 21:32:00.66 +39:23:57.8: 13.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.21 +/- 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
ZTF J213202.41+392353.1,2461188.8851,11.57,0.05,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
ZTF J213202.41+392353.1 20260528.3851 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 28.3851 2461188.8851 11.62 22:11:12.57 +37:18:40.2
90.86625 -15.39098 galactic Lac 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 | target | 22:11:12.57 +37:18:40.2 (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 22:11:12.57 +37:18:40.2: 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 22:11:12.57 +37:18:40.2: 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,2461188.8851,11.62,0.05,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
target 20260528.3851 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 28.3851 2461188.8851 11.73 21:41:04.24 +37:16:07.0
86.06927 -11.62657 galactic Cyg Second-epoch detections are separated by 2.0" 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 J325.2513+37.2756 | 21:41:03.22 +37:16:37.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.411+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:04.24 +37:16:07.0: 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 21:41:04.24 +37:16:07.0: 13.58 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.58 +/- 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 J325.2513+37.2756,2461188.8851,11.73,0.05,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 J325.2513+37.2756 20260528.3851 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 28.3851 2461188.8851 11.62 21:58:43.13 +42:11:57.6
91.94594 -10.04892 galactic Lac Second-epoch detections are separated by 3.7" 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 | ATO J329.6664+42.1926 | 21:58:43.13 +42:11:57.6 (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 21:58:43.13 +42:11:57.6: 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 21:58:43.13 +42:11:57.6: 13.97 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.97 +/- 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 J329.6664+42.1926,2461188.8851,11.62,0.05,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
ATO J329.6664+42.1926 20260528.3851 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 28.3851 2461188.8851 11.52 21:27:37.80 +38:16:28.5
84.80461 -9.07354 galactic Cyg Second-epoch detections are separated by 5.1" 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 | Gaia DR3 1964258114074497920 | 21:27:39.42 +38:15:47.8 (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 21:27:37.80 +38:16:28.5: 11.62 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:37.80 +38:16:28.5: 13.69 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.53 +/- 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 1964258114074497920,2461188.8851,11.52,0.05,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
Gaia DR3 1964258114074497920 20260528.3851 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 28.3851 2461188.8851 11.59 21:30:29.32 +34:39:51.4
82.65273 -12.05523 galactic Cyg 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 J322.6185+34.6631 | 21:30:29.32 +34:39:51.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.336+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:29.32 +34:39:51.4: 12.88 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:29.32 +34:39:51.4: 14.10 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 J322.6185+34.6631,2461188.8851,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.6185+34.6631 20260528.3851 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.60 21:58:18.35 +39:25:59.2
90.13202 -12.16796 galactic Lac Second-epoch detections are separated by 3.7" 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 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 21:58:18.35 +39:25:59.2: 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 21:58:18.35 +39:25:59.2: 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 J329.5793+39.4473,2461188.8851,11.60,0.05,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 J329.5793+39.4473 20260528.3851 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 28.3851 2461188.8851 11.74 22:09:48.54 +36:44:29.8
90.28072 -15.68129 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 | Gaia DR3 1954723114873206912 | 22:09:51.21 +36:44:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.432+/-0.031 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:48.54 +36:44:29.8: 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 22:09:48.54 +36:44:29.8: 13.29 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 1954723114873206912,2461188.8851,11.74,0.05,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
Gaia DR3 1954723114873206912 20260528.3851 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 28.3851 2461188.8851 11.82 22:01:12.18 +35:17:05.4
87.92473 -15.76695 galactic Peg 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 | target | 22:01:12.18 +35:17:05.4 (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 22:01:12.18 +35:17:05.4: 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 22:01:12.18 +35:17:05.4: 14.18 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.18 +/- 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,2461188.8851,11.82,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.56 21:48:57.93 +37:42:53.0
87.57187 -12.32711 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 | 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 21:48:57.93 +37:42:53.0: 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 21:48:57.93 +37:42:53.0: 13.39 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 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+37.7077,2461188.8851,11.56,0.05,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
ATO J327.2399+37.7077 20260528.3851 11.56CV 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 28.3851 2461188.8851 11.59 21:57:06.51 +36:41:43.9
88.17693 -14.14937 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 | Gaia DR3 1949610901203299200 | 21:57:05.46 +36:42:13.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.331+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:06.51 +36:41:43.9: 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 21:57:06.51 +36:41:43.9: 13.62 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 1949610901203299200,2461188.8851,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1949610901203299200 20260528.3851 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.62 22:05:42.72 +35:53:00.3
89.05817 -15.86415 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 J331.4278+35.8836 | 22:05:42.72 +35:53:00.3 (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 22:05:42.72 +35:53:00.3: 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 22:05:42.72 +35:53:00.3: 14.46 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.46 +/- 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+35.8836,2461188.8851,11.62,0.05,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
ATO J331.4278+35.8836 20260528.3851 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 28.3851 2461188.8851 11.68 21:56:29.34 +36:52:33.7
88.19582 -13.93113 galactic Cyg Second-epoch detections are separated by 1.7" 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 J329.1195+36.8762 | 21:56:29.34 +36:52:33.7 (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 21:56:29.34 +36:52:33.7: 12.21 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:29.34 +36:52:33.7: 14.26 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.91 +/- 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+36.8762,2461188.8851,11.68,0.05,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
ATO J329.1195+36.8762 20260528.3851 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 28.3851 2461188.8851 11.77 21:44:34.11 +41:24:31.9
89.37519 -8.97685 galactic Cyg Second-epoch detections are separated by 4.5" 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 1954548155089222912 | 21:44:31.60 +41:24:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.774+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:34.11 +41:24:31.9: 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 21:44:34.11 +41:24:31.9: 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
Gaia DR3 1954548155089222912,2461188.8851,11.77,0.05,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 1954548155089222912 20260528.3851 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 28.3851 2461188.8851 11.73 21:35:24.00 +36:47:15.8
84.88788 -11.21282 galactic Cyg Second-epoch detections are separated by 2.6" 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 1951911453183188096 | 21:35:26.01 +36:47:10.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.737+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:24.00 +36:47:15.8: 12.10 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:24.00 +36:47:15.8: 13.84 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.09 +/- 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 1951911453183188096,2461188.8851,11.73,0.05,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
Gaia DR3 1951911453183188096 20260528.3851 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 28.3851 2461188.8851 11.90 21:58:25.00 +35:15:16.4
87.44596 -15.43271 galactic Peg Second-epoch detections are separated by 4.5" 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 J329.6007+35.2560 | 21:58:22.74 +35:15:40.3 (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 21:58:25.00 +35:15:16.4: 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 21:58:25.00 +35:15:16.4: 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
ATO J329.6007+35.2560,2461188.8851,11.90,0.05,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
ATO J329.6007+35.2560 20260528.3851 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 28.3851 2461188.8851 11.49 21:41:07.37 +34:51:42.7
84.41772 -13.41358 galactic Cyg Second-epoch detections are separated by 8.2" and 3.8 pix
The object was found in VSX21" Gaia DR3 1950661140965705344
Type: ROT
# Max. Min./Amp. JD0 Period
16.890 G 16.970 G 1.857020000000 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 21:41:07.37 +34:51:42.7: 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 21:41:07.37 +34:51:42.7: 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
Gaia DR3 1950661140965705344,2461188.8851,11.49,0.05,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 1950661140965705344 20260528.3851 11.49CV 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 28.3851 2461188.8851 11.80 21:29:55.36 +37:14:39.4
84.40411 -10.12754 galactic Cyg Second-epoch detections are separated by 5.7" 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 | ATO J322.4632+37.2562 | 21:29:53.76 +37:15:13.4 (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 21:29:55.36 +37:14:39.4: 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 21:29:55.36 +37:14:39.4: 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
ATO J322.4632+37.2562,2461188.8851,11.80,0.05,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
ATO J322.4632+37.2562 20260528.3851 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 28.3851 2461188.8851 11.86 22:09:11.53 +36:46:04.1
90.19440 -15.58620 galactic Lac Second-epoch detections are separated by 1.4" 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 J332.2936+36.7689 | 22:09:11.53 +36:46:04.1 (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 22:09:11.53 +36:46:04.1: 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 22:09:11.53 +36:46:04.1: 14.73 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.73 +/- 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 J332.2936+36.7689,2461188.8851,11.86,0.05,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
ATO J332.2936+36.7689 20260528.3851 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 28.3851 2461188.8851 11.78 21:27:00.72 +33:45:01.6
81.47254 -12.19796 galactic Cyg Second-epoch detections are separated by 1.1" 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 J321.7555+33.7505 | 21:27:00.72 +33:45:01.6 (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 21:27:00.72 +33:45:01.6: 12.67 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:00.72 +33:45:01.6: 14.51 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.69 +/- 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+33.7505,2461188.8851,11.78,0.05,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 J321.7555+33.7505 20260528.3851 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 28.3851 2461188.8851 11.89 21:49:23.24 +36:27:43.6
86.79997 -13.33193 galactic Peg Second-epoch detections are separated by 2.7" 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 | 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 21:49:23.24 +36:27:43.6: 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 21:49:23.24 +36:27:43.6: 13.96 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 1949440133303961728,2461188.8851,11.89,0.05,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
Gaia DR3 1949440133303961728 20260528.3851 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 28.3851 2461188.8851 11.66 21:41:49.97 +40:05:14.3
88.09673 -9.62737 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 | Gaia DR3 1954313615516288128 | 21:41:48.93 +40:05:47.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.441+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:49.97 +40:05:14.3: 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 21:41:49.97 +40:05:14.3: 13.71 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 1954313615516288128,2461188.8851,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1954313615516288128 20260528.3851 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.84 21:36:03.27 +36:35:42.2
84.85100 -11.44310 galactic Cyg Second-epoch detections are separated by 2.5" 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 | Gaia DR3 1951893826638656768 | 21:36:01.03 +36:35:12.7 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE 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 21:36:03.27 +36:35:42.2: 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 21:36:03.27 +36:35:42.2: 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
Gaia DR3 1951893826638656768,2461188.8851,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1951893826638656768 20260528.3851 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.79 21:38:38.24 +33:58:29.0
83.41088 -13.71655 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 | target | 21:38:38.24 +33:58:29.0 (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 21:38:38.24 +33:58:29.0: 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 21:38:38.24 +33:58:29.0: 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
target,2461188.8851,11.79,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.79 22:01:20.08 +41:45:31.1
92.05983 -10.69544 galactic Lac Second-epoch detections are separated by 0.4" and 2.5 pix
The object was found in VSX21" Gaia DR3 1959956068669176064
Type: ROT
# Max. Min./Amp. JD0 Period
16.640 G 16.700 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 22:01:20.08 +41:45:31.1: 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 22:01:20.08 +41:45:31.1: 14.00 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 1959956068669176064,2461188.8851,11.79,0.05,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 1959956068669176064 20260528.3851 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 28.3851 2461188.8851 11.84 22:04:54.62 +35:49:30.4
88.88764 -15.81056 galactic Peg Second-epoch detections are separated by 4.7" 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 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 22:04:54.62 +35:49:30.4: 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 22:04:54.62 +35:49:30.4: 14.12 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.12 +/- 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 J331.2245+35.8493,2461188.8851,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.93 21:55:49.60 +34:16:12.6
86.36889 -15.85253 galactic Peg 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 | 21:55:49.60 +34:16:12.6 (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 21:55:49.60 +34:16:12.6: 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 21:55:49.60 +34:16:12.6: 14.87 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.87 +/- 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,2461188.8851,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.89 21:47:12.11 +36:46:39.0
86.67176 -12.80641 galactic Cyg Second-epoch detections are separated by 1.9" 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 1952472135393923456 | 21:47:13.44 +36:46:19.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:12.11 +36:46:39.0: 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 21:47:12.11 +36:46:39.0: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 1952472135393923456,2461188.8851,11.89,0.05,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
Gaia DR3 1952472135393923456 20260528.3851 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 28.3851 2461188.8851 11.81 22:10:20.09 +38:44:18.8
91.59926 -14.14009 galactic Lac Second-epoch detections are separated by 1.7" and 2.6 pix
The object was found in VSX 2" 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 22:10:20.09 +38:44:18.8: 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 22:10:20.09 +38:44:18.8: 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
Gaia DR3 1955512632942240128,2461188.8851,11.81,0.05,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
Gaia DR3 1955512632942240128 20260528.3851 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 28.3851 2461188.8851 11.87 21:56:34.42 +37:00:24.9
88.29474 -13.84059 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 | 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 21:56:34.42 +37:00:24.9: 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 21:56:34.42 +37:00:24.9: 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
Gaia DR3 1949631375305780480,2461188.8851,11.87,0.05,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
Gaia DR3 1949631375305780480 20260528.3851 11.87CV 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 28.3851 2461188.8851 11.82 21:32:24.43 +37:16:08.5
84.78350 -10.45261 galactic Cyg Second-epoch detections are separated by 1.8" 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 | 21:32:24.43 +37:16:08.5 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.577+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:24.43 +37:16:08.5: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:24.43 +37:16:08.5: 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,2461188.8851,11.82,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.82 21:40:15.48 +37:50:19.6
86.33794 -11.09586 galactic Cyg Second-epoch detections are separated by 1.4" 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 J325.0657+37.8384 | 21:40:15.48 +37:50:19.6 (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 21:40:15.48 +37:50:19.6: 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 21:40:15.48 +37:50:19.6: 13.67 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.67 +/- 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+37.8384,2461188.8851,11.82,0.05,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
ATO J325.0657+37.8384 20260528.3851 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 28.3851 2461188.8851 11.74 21:33:14.76 +33:54:31.4
82.53124 -12.99394 galactic Cyg Second-epoch detections are separated by 3.4" 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 | ASASSN-V J213311.49+335442.1 | 21:33:11.49 +33:54:42.1 (Gaia DR3) | SRS (local) | 22.560000000000 (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 21:33:14.76 +33:54:31.4: 12.34 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:14.76 +33:54:31.4: 13.96 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.40 +/- 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
ASASSN-V J213311.49+335442.1,2461188.8851,11.74,0.05,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
ASASSN-V J213311.49+335442.1 20260528.3851 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 28.3851 2461188.8851 12.10 21:50:58.66 +36:44:36.3
87.23715 -13.32577 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 | target | 21:50:58.66 +36:44:36.3 (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 21:50:58.66 +36:44:36.3: 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 21:50:58.66 +36:44:36.3: 14.39 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.39 +/- 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,2461188.8851,12.10,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.06 21:50:34.35 +37:11:01.0
87.46680 -12.93808 galactic Cyg 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 | target | 21:50:34.35 +37:11:01.0 (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 21:50:34.35 +37:11:01.0: 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 21:50:34.35 +37:11:01.0: 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
target,2461188.8851,12.06,0.05,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
target 20260528.3851 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 28.3851 2461188.8851 12.10 21:48:46.56 +35:26:19.9
86.01460 -14.02478 galactic Cyg Second-epoch detections are separated by 1.8" 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 | 21:48:46.56 +35:26:19.9 (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 21:48:46.56 +35:26:19.9: 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 21:48:46.56 +35:26:19.9: 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
target,2461188.8851,12.10,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.18 22:06:12.26 +39:36:02.7
91.46973 -12.97031 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 | 22:06:12.26 +39:36:02.7 (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 22:06:12.26 +39:36:02.7: 13.41 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:12.26 +39:36:02.7: 14.77 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.36 +/- 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,2461188.8851,12.18,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.95 21:56:00.51 +37:10:54.8
88.31922 -13.63383 galactic Cyg Second-epoch detections are separated by 1.8" 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 | 21:56:00.51 +37:10:54.8 (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 21:56:00.51 +37:10:54.8: 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 21:56:00.51 +37:10:54.8: 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
target,2461188.8851,11.95,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.84 21:55:18.34 +37:03:14.0
88.12419 -13.64361 galactic Cyg 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 | Gaia DR3 1949822557189904512 | 21:55:19.37 +37:03:58.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.277+/-0.042 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:18.34 +37:03:14.0: 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 21:55:18.34 +37:03:14.0: 14.24 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.24 +/- 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 1949822557189904512,2461188.8851,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1949822557189904512 20260528.3851 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 12.24 22:08:34.54 +37:33:21.7
90.58341 -14.88228 galactic Lac Second-epoch detections are separated by 2.5" 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 | 22:08:34.54 +37:33:21.7 (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 22:08:34.54 +37:33:21.7: 13.38 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:34.54 +37:33:21.7: 15.45 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.38 +/- 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,2461188.8851,12.24,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.93 21:27:12.31 +39:44:01.9
85.77705 -7.97287 galactic Cyg Second-epoch detections are separated by 3.9" 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 | 21:27:12.31 +39:44:01.9 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:12.31 +39:44:01.9: 12.74 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:12.31 +39:44:01.9: 14.38 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461188.8851,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260528.3851 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 12.09 21:50:07.60 +42:10:52.3
90.68075 -9.06070 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 | 21:50:07.60 +42:10:52.3 (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 21:50:07.60 +42:10:52.3: 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 21:50:07.60 +42:10:52.3: 14.65 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.65 +/- 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 J327.5325+42.1739,2461188.8851,12.09,0.05,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 J327.5325+42.1739 20260528.3851 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 28.3851 2461188.8851 12.04 21:58:36.20 +41:09:22.1
91.27161 -10.85450 galactic Lac Second-epoch detections are separated by 1.0" 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 | 21:58:36.20 +41:09:22.1 (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 21:58:36.20 +41:09:22.1: 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 21:58:36.20 +41:09:22.1: 14.78 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.78 +/- 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,2461188.8851,12.04,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.10 21:39:06.43 +37:40:28.2
86.05386 -11.06417 galactic Cyg Second-epoch detections are separated by 5.0" 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 | 21:39:06.43 +37:40:28.2 (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 21:39:06.43 +37:40:28.2: 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 21:39:06.43 +37:40:28.2: 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
target,2461188.8851,12.10,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.04 21:27:03.54 +35:21:30.8
82.64061 -11.06780 galactic Cyg Second-epoch detections are separated by 3.1" 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 | Gaia DR3 1951313838558088064 | 21:27:06.42 +35:21:15.8 (Gaia DR3) | T | P | 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 21:27:03.54 +35:21:30.8: 12.23 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:03.54 +35:21:30.8: 14.08 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 1951313838558088064,2461188.8851,12.04,0.05,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
Gaia DR3 1951313838558088064 20260528.3851 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 28.3851 2461188.8851 12.06 21:48:57.08 +34:21:29.2
85.30921 -14.86306 galactic Cyg Second-epoch detections are separated by 2.3" and 2.2 pix
The object was found in VSX 4" 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 21:48:57.08 +34:21:29.2: 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 21:48:57.08 +34:21:29.2: 14.91 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.91 +/- 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
ASASSN-V J214856.87+342131.6,2461188.8851,12.06,0.05,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
ASASSN-V J214856.87+342131.6 20260528.3851 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 28.3851 2461188.8851 12.07 21:55:06.39 +37:00:04.1
88.05808 -13.65896 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 | TYC 2731-1513-1 | 21:55:04.45 +36:59:49.7 (Gaia DR3) | EA (local) | 2.020654000000 (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:06.39 +37:00:04.1: 13.12 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:06.39 +37:00:04.1: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 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
TYC 2731-1513-1,2461188.8851,12.07,0.05,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
TYC 2731-1513-1 20260528.3851 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 28.3851 2461188.8851 12.20 22:00:12.79 +35:06:22.8
87.64473 -15.77923 galactic Peg 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 | 22:00:12.79 +35:06:22.8 (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 22:00:12.79 +35:06:22.8: 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 22:00:12.79 +35:06:22.8: 14.91 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.91 +/- 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,2461188.8851,12.20,0.05,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
target 20260528.3851 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 28.3851 2461188.8851 12.03 21:44:51.82 +36:12:11.9
85.92079 -12.92706 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 | ATO J326.2141+36.2023 | 21:44:51.82 +36:12:11.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G6 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:51.82 +36:12:11.9: 12.72 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:51.82 +36:12:11.9: 14.44 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 J326.2141+36.2023,2461188.8851,12.03,0.05,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
ATO J326.2141+36.2023 20260528.3851 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 28.3851 2461188.8851 12.08 21:31:26.58 +33:46:05.0
82.15524 -12.83378 galactic Cyg Second-epoch detections are separated by 2.9" 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 | 21:31:26.58 +33:46:05.0 (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 21:31:26.58 +33:46:05.0: 13.09 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:26.58 +33:46:05.0: 14.60 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.12 +/- 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,2461188.8851,12.08,0.05,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 20260528.3851 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 28.3851 2461188.8851 11.99 22:02:35.28 +41:45:10.0
92.24463 -10.84279 galactic Lac Second-epoch detections are separated by 1.8" 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 | 22:02:35.28 +41:45:10.0 (user input) | T | P | (position from user input) J-Ks=0.740+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:35.28 +41:45:10.0: 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 22:02:35.28 +41:45:10.0: 14.56 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.56 +/- 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,2461188.8851,11.99,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.12 21:43:22.57 +35:03:28.2
84.90462 -13.57909 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 1947764443222176128 | 21:43:21.05 +35:04:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.328+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:22.57 +35:03:28.2: 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 21:43:22.57 +35:03:28.2: 14.45 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.45 +/- 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 1947764443222176128,2461188.8851,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1947764443222176128 20260528.3851 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 11.96 21:31:50.19 +41:32:47.9
87.68318 -7.27396 galactic Cyg Second-epoch detections are separated by 3.3" 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 | Gaia DR3 1967127736343468288 | 21:31:53.89 +41:32:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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 21:31:50.19 +41:32:47.9: 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 21:31:50.19 +41:32:47.9: 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 1967127736343468288,2461188.8851,11.96,0.05,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
Gaia DR3 1967127736343468288 20260528.3851 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 28.3851 2461188.8851 12.19 21:49:28.11 +38:12:24.9
87.97624 -12.01752 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 | ATO J327.3641+38.2092 | 21:49:27.26 +38:11:52.7 (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 21:49:28.11 +38:12:24.9: 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 21:49:28.11 +38:12:24.9: 13.98 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.98 +/- 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 J327.3641+38.2092,2461188.8851,12.19,0.05,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 J327.3641+38.2092 20260528.3851 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 28.3851 2461188.8851 12.17 21:31:00.37 +36:55:32.7
84.33678 -10.50670 galactic Cyg Second-epoch detections are separated by 3.7" 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 J322.7455+36.9184 | 21:30:57.77 +36:54:58.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE 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 21:31:00.37 +36:55:32.7: 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 21:31:00.37 +36:55:32.7: 14.58 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.58 +/- 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 J322.7455+36.9184,2461188.8851,12.17,0.05,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
ATO J322.7455+36.9184 20260528.3851 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 28.3851 2461188.8851 12.29 21:50:53.87 +40:31:54.1
89.72043 -10.41938 galactic Cyg Second-epoch detections are separated by 1.8" and 2.2 pix
The object was found in VSX 1" Gaia DR3 1960199129457344512
Type: ROT
# Max. Min./Amp. JD0 Period
14.550 G 14.590 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 21:50:53.87 +40:31:54.1: 13.23 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:53.87 +40:31:54.1: 14.69 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.18 +/- 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 1960199129457344512,2461188.8851,12.29,0.05,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 1960199129457344512 20260528.3851 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 28.3851 2461188.8851 12.11 21:55:08.90 +41:19:55.0
90.86751 -10.31143 galactic Cyg Second-epoch detections are separated by 4.0" and 2.1 pix
The object was found in VSX22" Gaia DR3 1959615666741532928
Type: RS
# Max. Min./Amp. JD0 Period
15.440 G 15.510 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 21:55:08.90 +41:19:55.0: 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 21:55:08.90 +41:19:55.0: 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
Gaia DR3 1959615666741532928,2461188.8851,12.11,0.05,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
Gaia DR3 1959615666741532928 20260528.3851 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 28.3851 2461188.8851 12.24 21:47:51.33 +40:21:48.7
89.16075 -10.17432 galactic Cyg Second-epoch detections are separated by 1.7" 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 1954247369938340736 | 21:47:54.59 +40:21:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.521+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:51.33 +40:21:48.7: 13.43 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:51.33 +40:21:48.7: 14.51 +/- 0.15 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
Gaia DR3 1954247369938340736,2461188.8851,12.24,0.05,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 1954247369938340736 20260528.3851 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 28.3851 2461188.8851 12.33 22:04:51.59 +36:57:55.6
89.60451 -14.90358 galactic Lac Second-epoch detections are separated by 2.1" and 2.2 pix
The object was found in VSX 4" Gaia DR3 1954873507448471680
Type: RS
# Max. Min./Amp. JD0 Period
15.100 G 15.210 G 0.369502000000 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 22:04:51.59 +36:57:55.6: 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 22:04:51.59 +36:57:55.6: 15.27 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.27 +/- 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 1954873507448471680,2461188.8851,12.33,0.05,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
Gaia DR3 1954873507448471680 20260528.3851 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 28.3851 2461188.8851 12.23 21:36:58.18 +37:51:35.4
85.86512 -10.64176 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 | ATO J324.2508+37.8632 | 21:36:58.18 +37:51:35.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) 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 21:36:58.18 +37:51:35.4: 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 21:36:58.18 +37:51:35.4: 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 J324.2508+37.8632,2461188.8851,12.23,0.05,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 J324.2508+37.8632 20260528.3851 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 28.3851 2461188.8851 12.07 21:26:51.51 +34:03:07.6
81.66814 -11.96252 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 | 21:26:51.51 +34:03:07.6 (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 21:26:51.51 +34:03:07.6: 13.19 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:51.51 +34:03:07.6: 14.70 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.22 +/- 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,2461188.8851,12.07,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.18 21:44:25.94 +38:03:28.6
87.11240 -11.48114 galactic Cyg Second-epoch detections are separated by 1.4" 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 1952820238205138560 | 21:44:26.49 +38:04:04.0 (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 21:44:25.94 +38:03:28.6: 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 21:44:25.94 +38:03:28.6: 14.72 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.72 +/- 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 1952820238205138560,2461188.8851,12.18,0.05,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
Gaia DR3 1952820238205138560 20260528.3851 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 28.3851 2461188.8851 12.26 21:31:55.98 +35:27:42.5
83.43745 -11.68962 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 J322.9931+35.4609 | 21:31:55.98 +35:27:42.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.464+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:55.98 +35:27:42.5: 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 21:31:55.98 +35:27:42.5: 14.83 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.83 +/- 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 J322.9931+35.4609,2461188.8851,12.26,0.05,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 J322.9931+35.4609 20260528.3851 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 28.3851 2461188.8851 12.29 21:29:23.73 +35:04:44.7
82.78603 -11.60212 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 | target | 21:29:23.73 +35:04:44.7 (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 21:29:23.73 +35:04:44.7: 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 21:29:23.73 +35:04:44.7: 14.80 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.80 +/- 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,2461188.8851,12.29,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.14 21:39:31.89 +40:39:06.1
88.14711 -8.91449 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 | ATO J324.8818+40.6426 | 21:39:31.89 +40:39:06.1 (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 21:39:31.89 +40:39:06.1: 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 21:39:31.89 +40:39:06.1: 14.33 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.33 +/- 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 J324.8818+40.6426,2461188.8851,12.14,0.05,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 J324.8818+40.6426 20260528.3851 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 28.3851 2461188.8851 12.40 21:55:36.71 +38:47:53.5
89.30782 -12.33360 galactic Cyg Second-epoch detections are separated by 3.9" 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 | 21:55:36.71 +38:47:53.5 (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 21:55:36.71 +38:47:53.5: 12.97 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:36.71 +38:47:53.5: 15.38 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.46 +/- 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,2461188.8851,12.40,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.05 21:50:52.87 +41:13:07.7
90.16532 -9.88990 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 1960301040442818816 | 21:50:51.45 +41:13:50.7 (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 21:50:52.87 +41:13:07.7: 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 21:50:52.87 +41:13:07.7: 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
Gaia DR3 1960301040442818816,2461188.8851,12.05,0.05,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
Gaia DR3 1960301040442818816 20260528.3851 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 28.3851 2461188.8851 12.19 22:06:00.60 +35:37:20.3
88.94162 -16.10763 galactic Lac 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 | Gaia DR3 1948554236166909952 | 22:06:01.15 +35:37:50.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.385+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:00.60 +35:37:20.3: 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 22:06:00.60 +35:37:20.3: 14.00 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 1948554236166909952,2461188.8851,12.19,0.05,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 1948554236166909952 20260528.3851 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 28.3851 2461188.8851 12.21 21:38:51.07 +37:54:38.7
86.17825 -10.85570 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 | 21:38:51.07 +37:54:38.7 (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 21:38:51.07 +37:54:38.7: 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 21:38:51.07 +37:54:38.7: 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
target,2461188.8851,12.21,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.24 21:28:15.72 +34:43:42.3
82.36561 -11.68830 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 | 21:28:15.72 +34:43:42.3 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:15.72 +34:43:42.3: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:15.72 +34:43:42.3: 14.51 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.51 +/- 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,2461188.8851,12.24,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.30 21:28:08.23 +36:20:36.7
83.50425 -10.52174 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 | 21:28:08.23 +36:20:36.7 (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 21:28:08.23 +36:20:36.7: 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 21:28:08.23 +36:20:36.7: 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+36.3316,2461188.8851,12.30,0.05,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 J322.0319+36.3316 20260528.3851 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 28.3851 2461188.8851 12.21 21:35:18.86 +33:54:53.5
82.85340 -13.28680 galactic Cyg Second-epoch detections are separated by 1.1" and 2.6 pix
The object was found in VSX 5" Gaia DR3 1950269920985407104
Type: ROT
# Max. Min./Amp. JD0 Period
14.620 G 14.680 G 6.481300000000 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 21:35:18.86 +33:54:53.5: 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 21:35:18.86 +33:54:53.5: 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
Gaia DR3 1950269920985407104,2461188.8851,12.21,0.05,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 1950269920985407104 20260528.3851 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 28.3851 2461188.8851 12.15 22:08:10.72 +39:02:00.5
91.43323 -13.65321 galactic Lac Second-epoch detections are separated by 2.1" and 2.3 pix
The object was found in VSX 3" Gaia DR3 1956261950116724096
Type: ROT
# Max. Min./Amp. JD0 Period
14.220 G 14.260 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 22:08:10.72 +39:02:00.5: 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 22:08:10.72 +39:02:00.5: 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
Gaia DR3 1956261950116724096,2461188.8851,12.15,0.05,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 1956261950116724096 20260528.3851 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 28.3851 2461188.8851 12.16 21:31:29.47 +33:55:37.8
82.27662 -12.72699 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 | 21:31:29.47 +33:55:37.8 (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 21:31:29.47 +33:55:37.8: 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 21:31:29.47 +33:55:37.8: 14.60 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.24 +/- 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,2461188.8851,12.16,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.13 21:29:53.00 +36:05:31.8
83.58114 -10.94778 galactic Cyg Second-epoch detections are separated by 1.9" 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 J322.4726+36.0925 | 21:29:53.00 +36:05:31.8 (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 21:29:53.00 +36:05:31.8: 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 21:29:53.00 +36:05:31.8: 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 J322.4726+36.0925,2461188.8851,12.13,0.05,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 J322.4726+36.0925 20260528.3851 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 28.3851 2461188.8851 12.36 21:47:18.26 +36:55:52.2
86.79111 -12.70402 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 | target | 21:47:18.26 +36:55:52.2 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:18.26 +36:55:52.2: 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 21:47:18.26 +36:55:52.2: 14.80 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.80 +/- 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,2461188.8851,12.36,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.33 21:32:35.94 +35:36:10.5
83.63708 -11.68208 galactic Cyg Second-epoch detections are separated by 5.2" and 1.6 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 J323.1465+35.6027 | 21:32:35.94 +35:36:10.5 (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 21:32:35.94 +35:36:10.5: 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 21:32:35.94 +35:36:10.5: 14.74 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.74 +/- 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 J323.1465+35.6027,2461188.8851,12.33,0.05,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 J323.1465+35.6027 20260528.3851 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 28.3851 2461188.8851 12.44 21:48:18.39 +36:18:17.3
86.52513 -13.30867 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 | ATO J327.0885+36.3012 | 21:48:21.25 +36:18:04.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.474+/-0.041 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:18.39 +36:18:17.3: 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 21:48:18.39 +36:18:17.3: 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
ATO J327.0885+36.3012,2461188.8851,12.44,0.05,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 J327.0885+36.3012 20260528.3851 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 28.3851 2461188.8851 12.35 21:58:49.44 +40:28:41.5
90.87609 -11.41195 galactic Lac 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 | target | 21:58:49.44 +40:28:41.5 (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 21:58:49.44 +40:28:41.5: 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 21:58:49.44 +40:28:41.5: 15.00 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.00 +/- 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,2461188.8851,12.35,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.40 21:51:11.88 +37:00:39.9
87.44969 -13.15032 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 | Gaia DR3 1949490156780126336 | 21:51:09.14 +37:01:09.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.426+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:11.88 +37:00:39.9: 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 21:51:11.88 +37:00:39.9: 14.71 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.71 +/- 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 1949490156780126336,2461188.8851,12.40,0.05,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 1949490156780126336 20260528.3851 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 28.3851 2461188.8851 12.34 21:51:49.80 +37:26:00.3
87.82821 -12.90909 galactic Cyg Second-epoch detections are separated by 2.7" and 2.1 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 21:51:49.80 +37:26:00.3: 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 21:51:49.80 +37:26:00.3: 14.96 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.96 +/- 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+372556.3,2461188.8851,12.34,0.05,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
STSP J215151.42+372556.3 20260528.3851 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 28.3851 2461188.8851 12.35 21:37:52.96 +35:41:21.3
84.49497 -12.35707 galactic Cyg Second-epoch detections are separated by 3.6" 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 | 21:37:52.96 +35:41:21.3 (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 21:37:52.96 +35:41:21.3: 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 21:37:52.96 +35:41:21.3: 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,2461188.8851,12.35,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.31 21:46:21.03 +36:51:38.6
86.59640 -12.63162 galactic Cyg Second-epoch detections are separated by 4.0" 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 1952522025734029696 | 21:46:23.20 +36:51:55.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.588+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:21.03 +36:51:38.6: 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 21:46:21.03 +36:51:38.6: 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
Gaia DR3 1952522025734029696,2461188.8851,12.31,0.05,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 1952522025734029696 20260528.3851 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 28.3851 2461188.8851 12.29 21:51:39.07 +36:55:27.1
87.46292 -13.27513 galactic Cyg 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 J327.8989+36.9256 | 21:51:39.07 +36:55:27.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:39.07 +36:55:27.1: 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 21:51:39.07 +36:55:27.1: 15.57 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.57 +/- 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
ATO J327.8989+36.9256,2461188.8851,12.29,0.05,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
ATO J327.8989+36.9256 20260528.3851 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 28.3851 2461188.8851 12.26 21:28:28.56 +35:45:20.7
83.13400 -10.98849 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 | 21:28:28.56 +35:45:20.7 (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 21:28:28.56 +35:45:20.7: 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 21:28:28.56 +35:45:20.7: 14.38 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.38 +/- 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,2461188.8851,12.26,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.35 21:43:25.59 +36:45:52.5
86.08227 -12.31579 galactic Cyg Second-epoch detections are separated by 3.2" 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 | 21:43:25.59 +36:45:52.5 (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 21:43:25.59 +36:45:52.5: 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 21:43:25.59 +36:45:52.5: 14.97 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.97 +/- 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,2461188.8851,12.35,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.42 22:00:27.70 +40:13:15.7
90.96373 -11.80707 galactic Lac Second-epoch detections are separated by 2.0" 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 | 22:00:27.70 +40:13:15.7 (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 22:00:27.70 +40:13:15.7: 13.53 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:27.70 +40:13:15.7: 15.45 +/- 0.36 detection
Forced photometry reference-image weighted average: 14.36 +/- 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,2461188.8851,12.42,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.20 21:43:05.89 +37:32:43.1
86.56390 -11.68979 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 | 21:43:05.89 +37:32:43.1 (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 21:43:05.89 +37:32:43.1: 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 21:43:05.89 +37:32:43.1: 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,2461188.8851,12.20,0.05,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
target 20260528.3851 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 28.3851 2461188.8851 12.41 21:45:44.91 +38:12:59.8
87.41770 -11.53266 galactic Cyg Second-epoch detections are separated by 2.9" 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 | 21:45:44.91 +38:12:59.8 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:44.91 +38:12:59.8: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:44.91 +38:12:59.8: 15.07 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.07 +/- 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,2461188.8851,12.41,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.24 21:46:36.83 +37:07:17.3
86.81286 -12.47001 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 | Gaia DR3 1952535116796630656 | 21:46:38.74 +37:07:55.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:36.83 +37:07:17.3: 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 21:46:36.83 +37:07:17.3: 14.90 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.90 +/- 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 1952535116796630656,2461188.8851,12.24,0.05,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 1952535116796630656 20260528.3851 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 28.3851 2461188.8851 12.35 21:41:31.67 +37:12:07.8
86.09272 -11.73687 galactic Cyg 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 | 21:41:31.67 +37:12:07.8 (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 21:41:31.67 +37:12:07.8: 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 21:41:31.67 +37:12:07.8: 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,2461188.8851,12.35,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.34 21:45:18.28 +34:36:16.9
84.89618 -14.18065 galactic Cyg 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 | target | 21:45:18.28 +34:36:16.9 (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 21:45:18.28 +34:36:16.9: 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 21:45:18.28 +34:36:16.9: 15.10 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.10 +/- 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,2461188.8851,12.34,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.24 21:34:30.37 +33:45:39.6
82.61951 -13.28189 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 21:34:30.37 +33:45:39.6 (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 21:34:30.37 +33:45:39.6: 13.25 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:30.37 +33:45:39.6: 15.07 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.21 +/- 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,2461188.8851,12.24,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.21 21:53:38.94 +34:51:15.5
86.40290 -15.11691 galactic Peg Second-epoch detections are separated by 1.4" 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 J328.4121+34.8419 | 21:53:38.94 +34:51:15.5 (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 21:53:38.94 +34:51:15.5: 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 21:53:38.94 +34:51:15.5: 15.21 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.21 +/- 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
ATO J328.4121+34.8419,2461188.8851,12.21,0.05,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 J328.4121+34.8419 20260528.3851 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 28.3851 2461188.8851 12.36 21:45:08.10 +34:06:59.6
84.53318 -14.52100 galactic Cyg Second-epoch detections are separated by 1.4" 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 | target | 21:45:08.10 +34:06:59.6 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:08.10 +34:06:59.6: 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 21:45:08.10 +34:06:59.6: 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,2461188.8851,12.36,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.18 21:29:56.04 +35:08:35.1
82.91203 -11.63359 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 | ATO J322.4990+35.1416 | 21:29:56.04 +35:08:35.1 (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 21:29:56.04 +35:08:35.1: 12.76 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:56.04 +35:08:35.1: 14.80 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.64 +/- 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+35.1416,2461188.8851,12.18,0.05,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 J322.4990+35.1416 20260528.3851 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 28.3851 2461188.8851 12.45 21:46:56.43 +37:17:27.2
86.97709 -12.38511 galactic Cyg Second-epoch detections are separated by 2.7" 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 | 21:46:56.43 +37:17:27.2 (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 21:46:56.43 +37:17:27.2: 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 21:46:56.43 +37:17:27.2: 15.27 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.27 +/- 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,2461188.8851,12.45,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.41 22:08:40.10 +38:50:06.8
91.38971 -13.86904 galactic Lac Second-epoch detections are separated by 2.5" and 2.1 pix
The object was found in VSX 1" 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 +38:50:06.8: 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 22:08:40.10 +38:50:06.8: 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
Gaia DR3 1955508063096780544,2461188.8851,12.41,0.05,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
Gaia DR3 1955508063096780544 20260528.3851 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 28.3851 2461188.8851 12.34 21:40:38.86 +39:10:23.2
87.30546 -10.15670 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 | 21:40:38.86 +39:10:23.2 (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 21:40:38.86 +39:10:23.2: 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 21:40:38.86 +39:10:23.2: 15.34 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.34 +/- 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,2461188.8851,12.34,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.22 22:02:22.46 +41:34:46.0
92.10486 -10.95592 galactic Lac Second-epoch detections are separated by 1.4" 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 | 22:02:22.46 +41:34:46.0 (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 22:02:22.46 +41:34:46.0: 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 22:02:22.46 +41:34:46.0: 14.74 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.74 +/- 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,2461188.8851,12.22,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.47 21:46:43.25 +34:59:48.9
85.38892 -14.08050 galactic Cyg Second-epoch detections are separated by 4.6" 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 | 21:46:43.25 +34:59:48.9 (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 21:46:43.25 +34:59:48.9: 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 21:46:43.25 +34:59:48.9: 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,2461188.8851,12.47,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.26 21:43:09.86 +39:56:52.1
88.19654 -9.90081 galactic Cyg Second-epoch detections are separated by 2.4" and 2.5 pix
The object was found in VSX15" Gaia DR3 1954296951040334464
Type: ROT
# Max. Min./Amp. JD0 Period
15.750 G 15.780 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 21:43:09.86 +39:56:52.1: 13.30 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:09.86 +39:56:52.1: 14.43 +/- 0.13 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
Gaia DR3 1954296951040334464,2461188.8851,12.26,0.05,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 1954296951040334464 20260528.3851 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 28.3851 2461188.8851 12.16 21:38:19.68 +39:47:34.9
87.39080 -9.39674 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 | ATO J324.5932+39.7857 | 21:38:19.68 +39:47:34.9 (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 21:38:19.68 +39:47:34.9: 13.34 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:19.68 +39:47:34.9: 14.89 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.38 +/- 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 J324.5932+39.7857,2461188.8851,12.16,0.05,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
ATO J324.5932+39.7857 20260528.3851 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 28.3851 2461188.8851 12.30 21:35:24.48 +35:59:57.1
84.33744 -11.78801 galactic Cyg 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 | 21:35:24.48 +35:59:57.1 (user input) | T | P | (position from user input) 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 21:35:24.48 +35:59:57.1: 13.02 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:24.48 +35:59:57.1: 15.21 +/- 0.30 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461188.8851,12.30,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.30 21:39:41.36 +36:54:57.7
85.61895 -11.70207 galactic Cyg Second-epoch detections are separated by 2.3" 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 J324.9160+36.9228 | 21:39:39.86 +36:55:22.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.666+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:41.36 +36:54:57.7: 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 21:39:41.36 +36:54:57.7: 14.37 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.37 +/- 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 J324.9160+36.9228,2461188.8851,12.30,0.05,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 J324.9160+36.9228 20260528.3851 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 28.3851 2461188.8851 12.37 21:45:58.80 +39:55:46.0
88.59703 -10.26980 galactic Cyg Second-epoch detections are separated by 0.7" and 2.4 pix
The object was found in VSX 2" 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 21:45:58.80 +39:55:46.0: 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 21:45:58.80 +39:55:46.0: 14.72 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.72 +/- 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 1954120926101711872,2461188.8851,12.37,0.05,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 1954120926101711872 20260528.3851 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 28.3851 2461188.8851 12.31 21:50:17.51 +42:04:58.0
90.64069 -9.15588 galactic Cyg Second-epoch detections are separated by 0.8" and 2.4 pix
The object was found in VSX19" 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 21:50:17.51 +42:04:58.0: 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 21:50:17.51 +42:04:58.0: 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 1960632160939763456,2461188.8851,12.31,0.05,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 1960632160939763456 20260528.3851 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 28.3851 2461188.8851 12.28 21:45:18.10 +37:39:33.6
86.97494 -11.89371 galactic Cyg 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 | Gaia DR3 1952759833784056192 | 21:45:16.89 +37:39:00.0 (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 21:45:18.10 +37:39:33.6: 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 21:45:18.10 +37:39:33.6: 14.39 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.39 +/- 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 1952759833784056192,2461188.8851,12.28,0.05,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 1952759833784056192 20260528.3851 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 28.3851 2461188.8851 12.35 22:02:43.02 +36:12:43.0
88.77306 -15.23251 galactic Peg Second-epoch detections are separated by 1.1" 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 | target | 22:02:43.02 +36:12:43.0 (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 22:02:43.02 +36:12:43.0: 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 22:02:43.02 +36:12:43.0: 15.32 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.32 +/- 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,2461188.8851,12.35,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.32 21:30:03.94 +35:14:05.6
82.99723 -11.58682 galactic Cyg Second-epoch detections are separated by 1.8" and 2.8 pix
The object was found in VSX 4" ASASSN-V J213004.08+351408.6
Type: ROT
# Max. Min./Amp. JD0 Period
15.280 g Y 0.260 g 2459531.72200 18.580000000000
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 21:30:03.94 +35:14:05.6: 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 21:30:03.94 +35:14:05.6: 15.10 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.10 +/- 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
ASASSN-V J213004.08+351408.6,2461188.8851,12.32,0.05,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
ASASSN-V J213004.08+351408.6 20260528.3851 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 28.3851 2461188.8851 12.36 21:40:19.77 +35:37:23.1
84.82306 -12.74289 galactic Cyg Second-epoch detections are separated by 1.7" 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 21:40:19.77 +35:37:23.1: 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 21:40:19.77 +35:37:23.1: 15.18 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.18 +/- 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 1950852765226527104,2461188.8851,12.36,0.05,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 1950852765226527104 20260528.3851 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 28.3851 2461188.8851 12.30 21:46:14.54 +37:25:06.3
86.95593 -12.19779 galactic Cyg Second-epoch detections are separated by 2.4" 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 | Gaia DR3 1952554912304902528 | 21:46:16.92 +37:24:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:14.54 +37:25:06.3: 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 21:46:14.54 +37:25:06.3: 14.38 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.38 +/- 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 1952554912304902528,2461188.8851,12.30,0.05,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 1952554912304902528 20260528.3851 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 28.3851 2461188.8851 12.53 21:49:25.02 +42:02:02.4
90.48286 -9.08908 galactic Cyg Second-epoch detections are separated by 2.7" 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 | 21:49:25.02 +42:02:02.4 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:25.02 +42:02:02.4: 12.84 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:25.02 +42:02:02.4: 15.04 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461188.8851,12.53,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.31 21:42:07.94 +34:27:43.3
84.29781 -13.84875 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 | 21:42:07.94 +34:27:43.3 (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 21:42:07.94 +34:27:43.3: 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 21:42:07.94 +34:27:43.3: 15.03 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.03 +/- 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,2461188.8851,12.31,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.18 21:54:32.76 +35:25:31.2
86.92865 -14.79801 galactic Peg Second-epoch detections are separated by 1.8" 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 | 21:54:32.76 +35:25:31.2 (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 21:54:32.76 +35:25:31.2: 13.14 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:32.76 +35:25:31.2: 14.99 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461188.8851,12.18,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.41 22:09:41.40 +37:45:14.5
90.88885 -14.85582 galactic Lac 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 | target | 22:09:41.40 +37:45:14.5 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.031 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:41.40 +37:45:14.5: 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 22:09:41.40 +37:45:14.5: 15.33 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.33 +/- 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
target,2461188.8851,12.41,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.26 21:40:55.58 +35:54:46.6
85.11511 -12.61065 galactic Cyg Second-epoch detections are separated by 2.4" 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 | ATO J325.2405+35.9163 | 21:40:55.58 +35:54:46.6 (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 21:40:55.58 +35:54:46.6: 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 21:40:55.58 +35:54:46.6: 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
ATO J325.2405+35.9163,2461188.8851,12.26,0.05,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 J325.2405+35.9163 20260528.3851 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 28.3851 2461188.8851 12.53 21:59:43.47 +35:08:50.8
87.59090 -15.68442 galactic Peg 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 | 21:59:43.47 +35:08:50.8 (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 21:59:43.47 +35:08:50.8: 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 21:59:43.47 +35:08:50.8: 14.80 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.80 +/- 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,2461188.8851,12.53,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.46 21:51:42.10 +40:48:55.3
90.02406 -10.29902 galactic Cyg Second-epoch detections are separated by 1.8" 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 | 21:51:42.10 +40:48:55.3 (user input) | T | P | (position from user input) J-Ks=0.844+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:42.10 +40:48:55.3: 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 21:51:42.10 +40:48:55.3: 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,2461188.8851,12.46,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.46 21:50:22.21 +36:49:01.4
87.19112 -13.19082 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 | target | 21:50:22.21 +36:49:01.4 (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 21:50:22.21 +36:49:01.4: 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 21:50:22.21 +36:49:01.4: 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,2461188.8851,12.46,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.30 21:43:28.74 +37:46:46.7
86.78046 -11.56488 galactic Cyg Second-epoch detections are separated by 1.8" and 2.3 pix
The object was found in VSX17" Gaia DR3 1952809964643278080
Type: RS
# Max. Min./Amp. JD0 Period
16.190 G 16.250 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 21:43:28.74 +37:46:46.7: 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 21:43:28.74 +37:46:46.7: 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
Gaia DR3 1952809964643278080,2461188.8851,12.30,0.05,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 1952809964643278080 20260528.3851 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 28.3851 2461188.8851 12.36 21:38:40.51 +35:56:34.2
84.79205 -12.28041 galactic Cyg Second-epoch detections are separated by 2.7" 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 | 21:38:40.51 +35:56:34.2 (user input) | T | P | (position from user input) J-Ks=0.741+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:40.51 +35:56:34.2: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:40.51 +35:56:34.2: 15.23 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.23 +/- 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,2461188.8851,12.36,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.52 21:43:52.41 +39:31:29.7
88.01656 -10.30828 galactic Cyg Second-epoch detections are separated by 0.9" 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 | 21:43:52.41 +39:31:29.7 (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 21:43:52.41 +39:31:29.7: 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 21:43:52.41 +39:31:29.7: 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,2461188.8851,12.52,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.45 22:03:45.54 +37:16:44.0
89.62396 -14.52142 galactic Lac Second-epoch detections are separated by 1.0" 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 | 22:03:45.54 +37:16:44.0 (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 22:03:45.54 +37:16:44.0: 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 22:03:45.54 +37:16:44.0: 15.44 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.44 +/- 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
target,2461188.8851,12.45,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.34 21:45:01.30 +42:15:59.8
90.00789 -8.38383 galactic Cyg Second-epoch detections are separated by 1.4" 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 | 21:45:01.30 +42:15:59.8 (user input) | T | P | (position from user input) J-Ks=0.858+/-0.027 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:01.30 +42:15:59.8: 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 21:45:01.30 +42:15:59.8: 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,2461188.8851,12.34,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.49 21:45:06.45 +36:34:12.2
86.20792 -12.68514 galactic Cyg Second-epoch detections are separated by 3.7" 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 | 21:45:06.45 +36:34:12.2 (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 21:45:06.45 +36:34:12.2: 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 21:45:06.45 +36:34:12.2: 14.96 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.96 +/- 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,2461188.8851,12.49,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.38 21:45:42.14 +34:31:02.7
84.89924 -14.30028 galactic Cyg 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 | 21:45:42.14 +34:31:02.7 (user input) | T | P | (position from user input) J-Ks=0.381+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:42.14 +34:31:02.7: 13.26 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:42.14 +34:31:02.7: 14.93 +/- 0.23 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,2461188.8851,12.38,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.48 22:05:29.70 +37:47:39.1
90.23045 -14.32402 galactic Lac 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 | 22:05:29.70 +37:47:39.1 (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 22:05:29.70 +37:47:39.1: 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 22:05:29.70 +37:47:39.1: 15.43 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.43 +/- 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,2461188.8851,12.48,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.44 21:46:29.51 +35:05:33.5
85.41805 -13.97773 galactic Cyg Second-epoch detections are separated by 2.7" 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 | 21:46:29.51 +35:05:33.5 (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 21:46:29.51 +35:05:33.5: 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 21:46:29.51 +35:05:33.5: 14.94 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.94 +/- 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,2461188.8851,12.44,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.45 21:40:28.52 +37:56:37.5
86.44214 -11.04687 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 | 21:40:28.52 +37:56:37.5 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.099 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:28.52 +37:56:37.5: 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 21:40:28.52 +37:56:37.5: 14.88 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.88 +/- 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,2461188.8851,12.45,0.05,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 20260528.3851 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 28.3851 2461188.8851 12.42 21:50:53.20 +41:33:16.5
90.38422 -9.63259 galactic Cyg Second-epoch detections are separated by 2.0" 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 | Gaia DR3 1960326157411639424 | 21:50:53.84 +41:32:45.8 (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 21:50:53.20 +41:33:16.5: 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 21:50:53.20 +41:33:16.5: 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
Gaia DR3 1960326157411639424,2461188.8851,12.42,0.05,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
Gaia DR3 1960326157411639424 20260528.3851 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 28.3851 2461188.8851 12.50 21:44:02.25 +38:00:17.7
87.01712 -11.46941 galactic Cyg Second-epoch detections are separated by 2.3" and 2.1 pix
The object was found in VSX 3" Gaia DR3 1952819791528683648
Type: ROT
# Max. Min./Amp. JD0 Period
14.690 G 14.710 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 21:44:02.25 +38:00:17.7: 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 21:44:02.25 +38:00:17.7: 15.52 +/- 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
Gaia DR3 1952819791528683648,2461188.8851,12.50,0.05,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
Gaia DR3 1952819791528683648 20260528.3851 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 28.3851 2461188.8851 12.36 21:46:33.32 +36:26:40.4
86.34673 -12.97163 galactic Cyg Second-epoch detections are separated by 1.1" 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 | 21:46:33.32 +36:26:40.4 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:33.32 +36:26:40.4: 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 21:46:33.32 +36:26:40.4: 14.89 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.89 +/- 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,2461188.8851,12.36,0.05,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 20260528.3851 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 28.3851 2461188.8851 10.12 21:18:30.91 +41:07:55.5
85.59728 -5.81484 galactic Cyg Second-epoch detections are separated by 1.2" and 2.4 pix
The object was found in VSX 4" V0531 Cyg
Type: M
# Max. Min./Amp. JD0 Period
13.900 pg < 16.500 pg 2428045.00000 257.000000000000
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 21:18:30.91 +41:07:55.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:30.91 +41:07:55.5: 13.94 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.94 +/- 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
V0531 Cyg,2461188.8851,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0531 Cyg 20260528.3851 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.3851 2461188.8851 9.95 21:26:52.38 +41:39:00.4
87.08049 -6.55715 galactic Cyg Second-epoch detections are separated by 0.9" and 2.3 pix
The object was found in VSX 3" V0607 Cyg
Type: M
# Max. Min./Amp. JD0 Period
13.300 pg < 16.300 pg 2433510.00000 130.500000000000
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 21:26:52.38 +41:39:00.4: 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 21:26:52.38 +41:39:00.4: 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
V0607 Cyg,2461188.8851,9.95,0.05,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
V0607 Cyg 20260528.3851 9.95CV 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
## 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: 2461188.88532861 28.05.2026 09:14:42.392 /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
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: 9 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): 17139
Objects passed selection criteria: 17126
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: 16796.2
Average stars matched: 14799 (88.109 %)
Memory usage VmPeak: 124316 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 28 05:35:45 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: 2461188.88532861 28.05.2026 09:14:42.392 /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 477
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: 158 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): 128890
Objects passed selection criteria: 128636
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: 125300
Average stars matched: 113382 (90.4886 %)
Memory usage VmPeak: 1959784 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 28 05:40:59 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_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.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_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.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: 2461188.88489380
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
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_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.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_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits (1st new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
Image size: 937.4'x624.2' 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: 21:49:04.778 +37:59:47.42 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 21:49:04.778 +37:59:47.42
Angular distance between the image centers 0.0456 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits (2nd new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
Image size: 937.4'x624.2' 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: 21:49:05.750 +37:59:55.75 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 21:49:05.750 +37:59:55.75
Angular distance between the image centers 0.0454 deg.
###################################
###################################
# 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 21:49:04.778 +37:59:47.42
Second-epoch second image center 21:49:05.750 +37:59:55.75
Angular distance between the image centers 0.00394 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.raJOuSVCP6
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.gzgc4risy2
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_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits &> /tmp/tmp.V8calkuGMy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits &> /tmp/tmp.03zCwNaahy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.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
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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 3 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
2.4 pix fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
2.4 pix fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.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
14.7 mag. fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
14.7 mag. fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.7 (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.raJOuSVCP6 (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_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/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.gzgc4risy2 (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_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/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.V8calkuGMy (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_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.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_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.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_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1345, passed=18014
Got 18014 stars (including 16651 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits.cat
util/solve_plate_with_UCAC5 got 18014 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 17776 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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 17775 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 17775 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits N_match=964 sigma_overall_arcsec=0.583 sigma_q1_arcsec=0.457 sigma_q2_arcsec=0.789 sigma_q3_arcsec=0.491 sigma_q4_arcsec=0.829 n_q1=230 n_q2=226 n_q3=268 n_q4=240 worst_quadrant_to_overall_ratio=1.423
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.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.03zCwNaahy (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_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.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_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.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_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1350, passed=17930
Got 17930 stars (including 16557 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits.cat
util/solve_plate_with_UCAC5 got 17930 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 961 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(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 17663 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 961 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(), 17661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 17661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits N_match=960 sigma_overall_arcsec=0.644 sigma_q1_arcsec=0.492 sigma_q2_arcsec=0.756 sigma_q3_arcsec=0.578 sigma_q4_arcsec=0.778 n_q1=231 n_q2=224 n_q3=264 n_q4=241 worst_quadrant_to_overall_ratio=1.209
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits sigma_overall=5.245 worst_q_ratio=6.408
ref2=Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits sigma_overall=0.836 worst_q_ratio=1.625
new1=fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits sigma_overall=0.583 worst_q_ratio=1.423
new2=fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits sigma_overall=0.644 worst_q_ratio=1.209
reference average sigma_overall=3.0405 worst_q_ratio=4.0165
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041_astrometric_residuals.png (452 matched stars from wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728_astrometric_residuals.png (958 matched stars from wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311_astrometric_residuals.png (964 matched stars from wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312_astrometric_residuals.png (960 matched stars from wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-04_20.00sec_4.90C_LIGHT_0311.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-28_CI_Cyg-07-Q2b1x1_052904_TTUQ2b1x1_1628165_TvcwVpSG/wcs_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312.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 22:01:51.14 +39:18:53.3: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:14.94 +38:46:27.9: 14.43 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:03.43 +33:51:36.1: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:14.94 +38:46:27.9: 12.66 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:03.43 +33:51:36.1: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.03
Forced photometry filter KEPT candidate at 21:31:14.94 +38:46:27.9: ref_mag=12.77 +/- 0.03 new_mean_mag=11.6457 delta=1.12 (need > 0.90)
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Forced photometry filter REJECTED candidate at 21:47:03.43 +33:51:36.1: ref_mag=11.70 +/- 0.01 new_mean_mag=12.1133 delta=-0.42 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:51.14 +39:18:53.3: 10.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.71 +/- 0.01
Forced photometry filter REJECTED candidate at 22:01:51.14 +39:18:53.3: ref_mag=10.71 +/- 0.01 new_mean_mag=11.1315 delta=-0.42 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out37925.dat to exclusion_list_gaiadr2.txt
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_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 37882_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 37925_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 37925_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:31:14.94 +38:46:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 4.273 1964379403950450560 322.81239217790 +38.77559847284 12.1472 10.2801 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 37954_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 37954_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 252928_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 252928_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 252955_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 252955_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 252956_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 252956_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 252957_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 252957_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 252959_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 252959_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 252971_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 252971_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 252985_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 252985_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 252989_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 252989_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 252990_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 252990_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 252991_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 252991_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 252992_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 252992_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 252999_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 252999_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253009_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253009_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253020_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253020_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253025_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253025_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253041_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253041_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253042_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253042_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253047_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253047_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253049_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253049_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253061_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253061_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253065_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253065_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253069_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253069_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253071_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253071_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253074_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253074_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253075_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253075_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253088_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253088_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253090_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253090_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253105_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253105_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253112_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253112_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253116_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253116_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253125_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253125_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253145_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253145_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253167_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253167_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253172_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253172_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253186_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253186_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253215_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253215_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253221_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253221_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253233_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253233_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253237_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253237_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253243_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253243_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253248_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253248_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253251_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253251_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253253_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253253_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:47:14.99 +42:04:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253256_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253256_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253277_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253277_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253279_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253279_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253285_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253285_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253295_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253295_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253315_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253315_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253343_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253343_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253346_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253346_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253351_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253351_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253360_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253360_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253363_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253363_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253367_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253367_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253375_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253375_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253380_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253380_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253394_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253394_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253406_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253406_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253414_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253414_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253421_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253421_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253423_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253423_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253429_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253429_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253433_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253433_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253439_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253439_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253447_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253447_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253454_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253454_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253456_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253456_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:54:31.65 +34:37:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253460_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253460_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253468_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253468_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:54:51.07 +40:08:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253469_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253469_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:01:57.42 +35:42:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253483_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253483_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253491_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253491_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253506_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253506_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253516_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253516_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253520_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253520_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253524_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253524_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253526_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253526_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253535_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253535_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:42:55.23 +37:35:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253540_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253540_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:58:37.23 +33:56:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253548_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253548_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253559_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253559_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253598_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253598_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253602_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253602_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253604_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253604_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253615_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253615_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:10:36.40 +41:28:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253619_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253619_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253623_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253623_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253631_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253631_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253640_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253640_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253645_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253645_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253648_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253648_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253649_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253649_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253653_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253653_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253656_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253656_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:55:20.82 +40:52:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253658_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253658_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253673_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253673_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:58:28.05 +40:38:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253676_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253676_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 253681_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253681_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:41:19.36 +37:02:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253682_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253682_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253687_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253687_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253697_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253697_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253707_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253707_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253711_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253711_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:05:08.06 +36:40:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253714_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253714_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253717_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253717_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:41:05.66 +41:56:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253720_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253720_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253723_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253723_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253724_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253724_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253733_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253733_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253740_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253740_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253745_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253745_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:27:58.51 +34:36:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253747_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253747_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253760_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253760_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253770_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253770_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253787_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253787_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:31:39.28 +34:11:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253791_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253791_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253795_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253795_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253801_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253801_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253809_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253809_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253810_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253810_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253816_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253816_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:56:08.71 +41:50:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253822_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253822_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253826_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253826_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253828_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253828_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253831_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253831_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253849_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253849_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:01:07.92 +39:15:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253888_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253888_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253898_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253898_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:12:26.50 +40:55:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253925_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253925_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:31:50.35 +34:09:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253941_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253941_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:40:50.66 +37:16:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253943_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 253943_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 253947_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253947_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:08:28.90 +40:57:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253948_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253948_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 253960_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253960_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:47:14.33 +41:48:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253965_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253965_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:42:50.27 +37:29:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253973_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253973_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:11:47.76 +38:26:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253975_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253975_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 253982_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253982_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 253984_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253984_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:56:49.70 +42:13:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253987_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 253987_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:38:33.06 +37:54:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254018_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254018_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254023_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254023_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254048_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254048_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:56:37.89 +37:20:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254062_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254062_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 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 254068_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254068_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:58:48.38 +41:41:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254072_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254072_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:39:05.41 +36:51:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254077_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254077_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254088_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254088_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:42:45.52 +36:52:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254100_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254100_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 254120_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254120_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:42:32.95 +34:14:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254123_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254123_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:31:28.37 +35:34:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254126_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254126_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:32:54.32 +35:30:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254145_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254145_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254152_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254152_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:08:10.07 +37:08:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254166_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254166_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254171_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254171_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:57:06.66 +34:35:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254179_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254179_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:57:40.50 +37:18:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254191_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254191_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:01:55.17 +35:25:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254195_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254195_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:10:04.77 +41:24:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254198_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254198_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:58:07.69 +38:56:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254205_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254205_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254208_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254208_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 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 254209_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254209_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:42:06.21 +36:50:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254242_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254242_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:10:39.64 +41:12:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254263_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254263_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254264_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254264_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:04:54.84 +37:38:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254277_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254277_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254279_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254279_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:49:54.65 +34:54:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254280_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254280_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:59:59.43 +37:35:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254284_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254284_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:06:46.55 +39:39:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254292_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254292_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 254295_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254295_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:00:54.49 +41:16:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254297_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254297_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:50:52.30 +39:37:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254298_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254298_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:05:43.99 +41:00:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254314_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254314_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:09:21.11 +33:46:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254332_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254332_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:05:15.49 +37:31:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254335_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254335_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254340_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254340_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:03:59.98 +39:46:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254343_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254343_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:50:27.42 +35:49:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254345_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254345_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:47:01.47 +35:15:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254350_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254350_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254354_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254354_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254361_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254361_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254364_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254364_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:02:40.26 +38:06:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254365_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254365_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:55:27.22 +42:00:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254366_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254366_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:01:53.19 +40:17:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254367_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254367_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:42:46.48 +37:59:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254376_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254376_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:02:27.83 +42:04:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254379_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254379_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 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 254383_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254383_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:54:04.29 +37:39:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254404_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254404_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:59:27.43 +38:47:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254414_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254414_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:51:54.89 +33:54:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254420_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254420_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:38:02.64 +39:00:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254424_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254424_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:48:38.05 +41:48:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254425_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254425_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:55:07.32 +37:29:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254427_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254427_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254429_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254429_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:44:49.74 +36:56:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254449_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254449_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254454_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254454_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254455_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254455_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254460_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254460_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254466_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254466_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254467_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254467_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254476_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254476_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 254482_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254482_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:05:11.30 +39:28:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254483_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254483_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254495_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254495_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:34:28.37 +39:24:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254500_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254500_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:48:22.39 +38:39:15.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254504_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254504_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254505_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254505_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:42:16.99 +37:34:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254515_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254515_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254517_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254517_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:09:23.73 +40:29:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254525_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254525_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:55:01.56 +42:15:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254526_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254526_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:07:03.97 +38:06:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254537_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254537_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:58:13.54 +38:26:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254543_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254543_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254549_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254549_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:57:23.11 +40:56:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254552_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254552_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:31:28.76 +34:33:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254555_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254555_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254559_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254559_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254564_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254564_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254566_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254566_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 254576_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254576_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:59:00.14 +41:56:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254589_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254589_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:58:15.44 +41:40:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254598_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254598_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254600_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254600_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254618_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254618_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:50:11.57 +35:33:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254625_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254625_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254627_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254627_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:43:32.02 +38:44:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254633_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254633_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:49:46.99 +41:07:49.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254640_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254640_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:44:49.51 +35:31:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254644_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254644_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:52:06.36 +38:25:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254651_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254651_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254655_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254655_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 254660_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254660_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:56:57.62 +35:29:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254666_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254666_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:09:15.65 +39:15:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254671_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254671_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:02:25.81 +38:25:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254678_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254678_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254684_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254684_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254686_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254686_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254690_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254690_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254702_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254702_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254710_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254710_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:04:36.94 +38:54:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254716_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254716_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:49:54.33 +37:45:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254729_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254729_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254731_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254731_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:06:29.77 +39:42:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254748_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254748_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254754_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254754_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254785_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254785_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:39:03.07 +40:22:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254794_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254794_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 254813_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254813_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 254834_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254834_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:49:18.14 +39:21:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254850_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254850_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254866_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254866_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254870_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254870_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254909_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254909_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254913_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254913_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254918_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254918_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254936_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254936_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 254939_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254939_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:00:00.09 +38:42:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254971_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254971_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254977_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254977_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254986_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 254986_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 254992_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 254992_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:53:08.53 +40:33:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255000_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255000_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255023_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255023_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255032_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255032_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255036_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 255036_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 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 255062_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255062_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255072_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255072_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255094_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255094_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255108_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255108_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255243_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255243_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255260_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255260_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255264_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255264_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255269_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255269_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255348_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255348_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255384_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255384_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255389_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 255389_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 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 255393_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255393_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255437_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255437_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255443_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255443_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255475_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 255475_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:27:09.53 +36:53:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255499_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 255499_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 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 255584_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255584_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255590_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255590_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255611_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255611_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255639_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 255639_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:41:51.03 +35:55:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255641_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 255641_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 21:46:28.81 +39:28:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255668_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255668_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255687_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255687_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255706_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255706_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255726_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255726_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255753_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255753_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255767_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255767_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255813_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255813_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255827_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255827_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255882_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255882_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255894_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255894_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255901_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255901_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255906_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255906_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255915_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255915_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255940_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 255940_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 255989_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 255989_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 256065_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 256065_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 256092_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256092_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256130_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256130_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256137_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256137_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256144_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256144_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256164_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256164_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256167_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256167_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256170_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256170_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256190_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256190_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256205_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256205_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256212_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256212_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256238_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256238_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256273_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256273_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256286_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256286_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256307_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256307_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256321_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256321_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256325_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 256325_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 256351_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256351_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256374_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256374_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256387_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256387_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256399_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256399_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256403_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256403_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256404_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256404_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256406_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256406_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256409_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256409_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256454_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256454_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256461_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256461_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256464_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256464_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256465_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256465_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256484_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256484_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256504_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256504_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256516_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256516_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256517_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256517_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256521_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256521_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256522_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256522_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256524_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256524_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256527_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256527_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256531_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256531_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256540_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256540_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256543_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256543_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256563_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256563_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256572_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256572_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256574_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256574_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256583_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256583_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256597_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256597_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256599_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256599_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256604_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256604_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256610_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256610_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256615_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256615_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256645_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256645_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256661_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256661_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256665_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256665_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256681_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 256681_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 256684_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256684_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256686_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256686_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256698_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256698_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256699_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256699_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256712_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256712_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256717_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256717_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256722_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256722_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256747_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 256747_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 256753_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256753_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256754_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256754_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256759_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256759_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256760_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 256760_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 256819_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256819_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256851_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256851_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256852_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256852_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256855_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256855_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256869_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256869_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256878_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256878_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256916_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 256916_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 256918_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256918_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256921_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 256921_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 256928_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 256928_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 256929_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256929_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256931_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256931_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256933_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256933_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256959_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256959_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256966_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256966_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256970_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256970_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 256988_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 256988_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
**** FOUND 22:00:32.81 +39:39:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256990_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 256990_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 257004_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 257004_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 257018_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
The candidate 257018_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312 did not pass the final checks
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Considering the candidate 257023_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 257023_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 257030_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 257030_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 243136_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 243136_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
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Considering the candidate 33331_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
Preparing report for the candidate 33331_fd_Cyg-07-Q2b1x1_2026-05-28_04-14-42_20.00sec_5.00C_LIGHT_0312
make_report_in_HTML.sh Phase 2 (HTML assembly): 18s
make_report_in_HTML.sh TOTAL: 624s
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 ####
21:18:30.91 +41:07:55.5
21:51:06.25 +37:29:04.1
21:48:41.00 +41:58:38.6
21:49:17.84 +40:40:26.6
21:59:58.68 +41:37:47.8
22:06:54.83 +41:38:24.1
21:43:24.75 +37:27:40.3
21:34:08.01 +36:35:12.1
21:27:51.06 +36:06:23.5
21:57:31.17 +38:48:28.2
21:45:42.22 +41:54:53.3
21:58:37.93 +35:47:10.9
21:45:02.91 +36:40:06.0
21:47:07.79 +38:39:18.7
21:47:04.59 +40:58:26.8
21:53:53.81 +41:17:50.0
21:34:19.66 +37:09:36.8
21:50:15.92 +34:58:33.6
21:29:02.89 +40:09:05.6
21:36:44.06 +39:54:02.6
21:44:38.60 +38:02:23.9
21:36:54.42 +37:55:38.0
21:39:53.77 +37:58:52.8
21:40:07.72 +34:33:18.6
21:27:29.88 +38:47:35.3
21:27:35.74 +41:34:26.3
21:31:28.79 +39:48:09.4
21:35:26.39 +41:08:48.9
21:42:09.02 +41:33:18.7
22:02:59.35 +41:26:45.6
21:40:14.01 +36:18:19.9
21:29:00.27 +38:59:29.9
21:37:48.52 +41:23:34.6
21:42:06.53 +39:57:24.1
21:58:28.64 +40:10:15.9
21:41:28.44 +41:30:42.9
21:59:26.27 +37:53:39.1
21:48:31.19 +41:08:42.6
21:44:03.08 +37:47:35.5
21:55:39.52 +36:53:21.5
21:39:43.16 +34:48:30.4
22:05:37.35 +38:57:39.8
21:49:03.69 +39:29:38.5
21:38:23.51 +40:06:13.9
21:31:19.30 +37:55:42.1
21:28:06.25 +33:41:27.5
22:05:10.51 +37:28:20.7
21:58:00.61 +37:39:31.2
21:30:54.99 +34:30:59.3
21:28:22.13 +41:32:01.6
21:30:40.26 +41:59:21.8
21:37:14.43 +35:50:17.4
22:03:59.35 +40:08:11.4
21:51:46.23 +37:08:04.9
21:56:13.21 +35:31:23.9
21:33:10.12 +41:39:57.2
21:56:28.96 +37:56:46.4
21:44:23.93 +37:43:55.7
21:48:12.44 +41:41:11.1
21:38:50.77 +35:08:49.5
21:27:26.96 +35:34:46.7
21:43:17.68 +38:29:47.6
21:30:43.77 +34:28:20.2
21:40:43.71 +37:22:58.9
21:33:57.71 +41:11:31.3
21:39:48.72 +38:17:17.1
21:26:09.20 +40:15:19.5
21:43:35.25 +37:12:37.5
21:32:48.36 +39:29:40.1
22:06:48.50 +39:07:17.3
21:29:37.11 +34:43:56.6
21:34:13.43 +42:00:56.8
22:01:22.36 +40:55:07.0
21:40:56.27 +41:13:23.4
22:06:21.81 +39:23:02.5
21:58:41.91 +39:00:24.6
21:35:58.63 +38:02:59.5
21:48:47.08 +40:08:12.8
21:26:50.66 +37:00:11.1
21:28:20.33 +39:05:27.1
21:34:37.64 +34:15:57.0
22:11:02.22 +38:11:05.6
22:03:31.27 +39:03:21.3
22:10:31.99 +41:45:05.3
22:00:14.34 +41:40:32.5
22:02:11.36 +35:32:41.1
21:27:24.11 +33:39:56.7
21:40:40.97 +36:19:19.9
21:31:28.70 +38:53:30.8
22:05:39.85 +34:53:38.1
21:51:51.69 +41:19:45.6
21:59:20.89 +36:56:48.2
21:33:13.71 +37:12:42.7
22:06:01.44 +39:10:16.5
21:46:25.62 +39:38:17.9
21:37:46.88 +36:44:33.3
21:28:11.90 +34:45:20.1
21:27:20.09 +35:46:48.3
21:30:31.96 +35:46:44.6
21:59:33.49 +41:27:38.5
21:28:41.97 +34:20:03.0
22:01:26.27 +38:07:01.0
21:41:57.33 +40:22:13.9
21:29:15.48 +38:35:05.1
21:57:16.71 +37:31:04.8
21:29:30.58 +37:27:31.5
22:01:18.65 +41:30:27.0
21:59:06.38 +34:00:17.5
21:34:29.33 +39:23:37.9
21:31:14.96 +38:46:29.2
21:42:51.25 +37:54:04.8
21:44:42.92 +35:29:06.6
22:09:13.48 +39:15:45.4
22:02:13.90 +41:47:06.4
21:44:09.46 +37:55:02.4
21:42:12.45 +38:54:23.1
21:44:26.49 +41:28:25.9
22:02:14.79 +34:37:06.2
21:43:31.53 +35:02:27.4
21:53:19.48 +36:06:08.2
21:44:06.73 +37:26:46.3
22:06:31.80 +34:33:31.3
22:02:42.44 +41:44:09.0
21:29:41.53 +38:48:30.5
21:57:42.00 +40:41:31.7
22:05:01.98 +41:27:43.6
22:04:59.74 +39:57:17.2
22:09:46.14 +41:39:55.4
22:02:04.69 +37:45:26.0
21:39:00.59 +38:41:33.2
21:47:33.59 +37:22:54.8
21:49:41.22 +37:43:27.7
21:40:47.54 +37:32:55.6
21:47:48.83 +38:11:35.7
21:27:14.50 +36:18:38.9
21:32:00.66 +39:23:57.8
22:11:12.57 +37:18:40.2
21:41:04.24 +37:16:07.0
21:58:43.13 +42:11:57.6
21:27:37.80 +38:16:28.5
21:30:29.32 +34:39:51.4
21:58:18.35 +39:25:59.2
22:09:48.54 +36:44:29.8
22:01:12.18 +35:17:05.4
21:48:57.93 +37:42:53.0
21:57:06.51 +36:41:43.9
22:05:42.72 +35:53:00.3
21:56:29.34 +36:52:33.7
21:44:34.11 +41:24:31.9
21:35:24.00 +36:47:15.8
21:58:25.00 +35:15:16.4
21:41:07.37 +34:51:42.7
21:29:55.36 +37:14:39.4
22:09:11.53 +36:46:04.1
21:27:00.72 +33:45:01.6
21:49:23.24 +36:27:43.6
21:41:49.97 +40:05:14.3
21:36:03.27 +36:35:42.2
21:38:38.24 +33:58:29.0
22:01:20.08 +41:45:31.1
22:04:54.62 +35:49:30.4
21:55:49.60 +34:16:12.6
21:47:12.11 +36:46:39.0
22:10:20.09 +38:44:18.8
21:56:34.42 +37:00:24.9
21:32:24.43 +37:16:08.5
21:40:15.48 +37:50:19.6
21:33:14.76 +33:54:31.4
21:50:58.66 +36:44:36.3
21:50:34.35 +37:11:01.0
21:48:46.56 +35:26:19.9
22:06:12.26 +39:36:02.7
21:56:00.51 +37:10:54.8
21:55:18.34 +37:03:14.0
22:08:34.54 +37:33:21.7
21:27:12.31 +39:44:01.9
21:50:07.60 +42:10:52.3
21:58:36.20 +41:09:22.1
21:39:06.43 +37:40:28.2
21:27:03.54 +35:21:30.8
21:48:57.08 +34:21:29.2
21:55:06.39 +37:00:04.1
22:00:12.79 +35:06:22.8
21:44:51.82 +36:12:11.9
21:31:26.58 +33:46:05.0
22:02:35.28 +41:45:10.0
21:43:22.57 +35:03:28.2
21:31:50.19 +41:32:47.9
21:49:28.11 +38:12:24.9
21:31:00.37 +36:55:32.7
21:50:53.87 +40:31:54.1
21:55:08.90 +41:19:55.0
21:47:51.33 +40:21:48.7
22:04:51.59 +36:57:55.6
21:36:58.18 +37:51:35.4
21:26:51.51 +34:03:07.6
21:44:25.94 +38:03:28.6
21:31:55.98 +35:27:42.5
21:29:23.73 +35:04:44.7
21:39:31.89 +40:39:06.1
21:55:36.71 +38:47:53.5
21:50:52.87 +41:13:07.7
22:06:00.60 +35:37:20.3
21:38:51.07 +37:54:38.7
21:28:15.72 +34:43:42.3
21:28:08.23 +36:20:36.7
21:35:18.86 +33:54:53.5
22:08:10.72 +39:02:00.5
21:31:29.47 +33:55:37.8
21:29:53.00 +36:05:31.8
21:47:18.26 +36:55:52.2
21:32:35.94 +35:36:10.5
21:48:18.39 +36:18:17.3
21:58:49.44 +40:28:41.5
21:51:11.88 +37:00:39.9
21:51:49.80 +37:26:00.3
21:37:52.96 +35:41:21.3
21:46:21.03 +36:51:38.6
21:51:39.07 +36:55:27.1
21:28:28.56 +35:45:20.7
21:43:25.59 +36:45:52.5
22:00:27.70 +40:13:15.7
21:43:05.89 +37:32:43.1
21:45:44.91 +38:12:59.8
21:46:36.83 +37:07:17.3
21:41:31.67 +37:12:07.8
21:45:18.28 +34:36:16.9
21:34:30.37 +33:45:39.6
21:53:38.94 +34:51:15.5
21:45:08.10 +34:06:59.6
21:29:56.04 +35:08:35.1
21:46:56.43 +37:17:27.2
22:08:40.10 +38:50:06.8
21:40:38.86 +39:10:23.2
22:02:22.46 +41:34:46.0
21:46:43.25 +34:59:48.9
21:43:09.86 +39:56:52.1
21:38:19.68 +39:47:34.9
21:35:24.48 +35:59:57.1
21:39:41.36 +36:54:57.7
21:45:58.80 +39:55:46.0
21:50:17.51 +42:04:58.0
21:45:18.10 +37:39:33.6
22:02:43.02 +36:12:43.0
21:30:03.94 +35:14:05.6
21:40:19.77 +35:37:23.1
21:46:14.54 +37:25:06.3
21:49:25.02 +42:02:02.4
21:42:07.94 +34:27:43.3
21:54:32.76 +35:25:31.2
22:09:41.40 +37:45:14.5
21:40:55.58 +35:54:46.6
21:59:43.47 +35:08:50.8
21:51:42.10 +40:48:55.3
21:50:22.21 +36:49:01.4
21:43:28.74 +37:46:46.7
21:38:40.51 +35:56:34.2
21:43:52.41 +39:31:29.7
22:03:45.54 +37:16:44.0
21:45:01.30 +42:15:59.8
21:45:06.45 +36:34:12.2
21:45:42.14 +34:31:02.7
22:05:29.70 +37:47:39.1
21:46:29.51 +35:05:33.5
21:40:28.52 +37:56:37.5
21:50:53.20 +41:33:16.5
21:44:02.25 +38:00:17.7
21:46:33.32 +36:26:40.4
21:26:52.38 +41:39:00.4
########### 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 ####
21:51:06.25 +37:29:04.1
21:48:41.00 +41:58:38.6
21:49:17.84 +40:40:26.6
21:59:58.68 +41:37:47.8
22:06:54.83 +41:38:24.1
21:43:24.75 +37:27:40.3
21:34:08.01 +36:35:12.1
21:27:51.06 +36:06:23.5
21:57:31.17 +38:48:28.2
21:45:42.22 +41:54:53.3
21:58:37.93 +35:47:10.9
21:45:02.91 +36:40:06.0
21:47:07.79 +38:39:18.7
21:47:04.59 +40:58:26.8
21:53:53.81 +41:17:50.0
21:34:19.66 +37:09:36.8
21:50:15.92 +34:58:33.6
21:29:02.89 +40:09:05.6
21:36:44.06 +39:54:02.6
21:44:38.60 +38:02:23.9
21:36:54.42 +37:55:38.0
21:39:53.77 +37:58:52.8
21:40:07.72 +34:33:18.6
21:27:29.88 +38:47:35.3
21:27:35.74 +41:34:26.3
21:31:28.79 +39:48:09.4
21:35:26.39 +41:08:48.9
21:42:09.02 +41:33:18.7
22:02:59.35 +41:26:45.6
21:40:14.01 +36:18:19.9
21:29:00.27 +38:59:29.9
21:37:48.52 +41:23:34.6
21:42:06.53 +39:57:24.1
21:58:28.64 +40:10:15.9
21:41:28.44 +41:30:42.9
21:59:26.27 +37:53:39.1
21:48:31.19 +41:08:42.6
21:44:03.08 +37:47:35.5
21:55:39.52 +36:53:21.5
21:39:43.16 +34:48:30.4
22:05:37.35 +38:57:39.8
21:49:03.69 +39:29:38.5
21:38:23.51 +40:06:13.9
21:31:19.30 +37:55:42.1
21:28:06.25 +33:41:27.5
22:05:10.51 +37:28:20.7
21:58:00.61 +37:39:31.2
21:30:54.99 +34:30:59.3
21:28:22.13 +41:32:01.6
21:30:40.26 +41:59:21.8
21:37:14.43 +35:50:17.4
22:03:59.35 +40:08:11.4
21:51:46.23 +37:08:04.9
21:56:13.21 +35:31:23.9
21:33:10.12 +41:39:57.2
21:56:28.96 +37:56:46.4
21:44:23.93 +37:43:55.7
21:48:12.44 +41:41:11.1
21:38:50.77 +35:08:49.5
21:27:26.96 +35:34:46.7
21:43:17.68 +38:29:47.6
21:30:43.77 +34:28:20.2
21:40:43.71 +37:22:58.9
21:33:57.71 +41:11:31.3
21:39:48.72 +38:17:17.1
21:26:09.20 +40:15:19.5
21:43:35.25 +37:12:37.5
21:32:48.36 +39:29:40.1
22:06:48.50 +39:07:17.3
21:29:37.11 +34:43:56.6
21:34:13.43 +42:00:56.8
22:01:22.36 +40:55:07.0
21:40:56.27 +41:13:23.4
22:06:21.81 +39:23:02.5
21:58:41.91 +39:00:24.6
21:35:58.63 +38:02:59.5
21:48:47.08 +40:08:12.8
21:26:50.66 +37:00:11.1
21:28:20.33 +39:05:27.1
21:34:37.64 +34:15:57.0
22:11:02.22 +38:11:05.6
22:03:31.27 +39:03:21.3
22:10:31.99 +41:45:05.3
22:00:14.34 +41:40:32.5
22:02:11.36 +35:32:41.1
21:27:24.11 +33:39:56.7
21:40:40.97 +36:19:19.9
21:31:28.70 +38:53:30.8
22:05:39.85 +34:53:38.1
21:51:51.69 +41:19:45.6
21:59:20.89 +36:56:48.2
21:33:13.71 +37:12:42.7
22:06:01.44 +39:10:16.5
21:46:25.62 +39:38:17.9
21:37:46.88 +36:44:33.3
21:28:11.90 +34:45:20.1
21:27:20.09 +35:46:48.3
21:30:31.96 +35:46:44.6
21:59:33.49 +41:27:38.5
21:28:41.97 +34:20:03.0
22:01:26.27 +38:07:01.0
21:41:57.33 +40:22:13.9
21:29:15.48 +38:35:05.1
21:57:16.71 +37:31:04.8
21:29:30.58 +37:27:31.5
22:01:18.65 +41:30:27.0
21:59:06.38 +34:00:17.5
21:34:29.33 +39:23:37.9
21:31:14.96 +38:46:29.2
21:42:51.25 +37:54:04.8
21:44:42.92 +35:29:06.6
22:09:13.48 +39:15:45.4
22:02:13.90 +41:47:06.4
21:44:09.46 +37:55:02.4
21:42:12.45 +38:54:23.1
21:44:26.49 +41:28:25.9
22:02:14.79 +34:37:06.2
21:43:31.53 +35:02:27.4
21:53:19.48 +36:06:08.2
21:44:06.73 +37:26:46.3
22:06:31.80 +34:33:31.3
22:02:42.44 +41:44:09.0
21:29:41.53 +38:48:30.5
21:57:42.00 +40:41:31.7
22:05:01.98 +41:27:43.6
22:04:59.74 +39:57:17.2
22:09:46.14 +41:39:55.4
22:02:04.69 +37:45:26.0
21:39:00.59 +38:41:33.2
21:47:33.59 +37:22:54.8
21:49:41.22 +37:43:27.7
21:40:47.54 +37:32:55.6
21:47:48.83 +38:11:35.7
21:27:14.50 +36:18:38.9
21:32:00.66 +39:23:57.8
22:11:12.57 +37:18:40.2
21:41:04.24 +37:16:07.0
21:58:43.13 +42:11:57.6
21:27:37.80 +38:16:28.5
21:30:29.32 +34:39:51.4
21:58:18.35 +39:25:59.2
22:09:48.54 +36:44:29.8
22:01:12.18 +35:17:05.4
21:48:57.93 +37:42:53.0
21:57:06.51 +36:41:43.9
22:05:42.72 +35:53:00.3
21:56:29.34 +36:52:33.7
21:44:34.11 +41:24:31.9
21:35:24.00 +36:47:15.8
21:58:25.00 +35:15:16.4
21:41:07.37 +34:51:42.7
21:29:55.36 +37:14:39.4
22:09:11.53 +36:46:04.1
21:27:00.72 +33:45:01.6
21:49:23.24 +36:27:43.6
21:41:49.97 +40:05:14.3
21:36:03.27 +36:35:42.2
21:38:38.24 +33:58:29.0
22:01:20.08 +41:45:31.1
22:04:54.62 +35:49:30.4
21:55:49.60 +34:16:12.6
21:47:12.11 +36:46:39.0
22:10:20.09 +38:44:18.8
21:56:34.42 +37:00:24.9
21:32:24.43 +37:16:08.5
21:40:15.48 +37:50:19.6
21:33:14.76 +33:54:31.4
21:50:58.66 +36:44:36.3
21:50:34.35 +37:11:01.0
21:48:46.56 +35:26:19.9
22:06:12.26 +39:36:02.7
21:56:00.51 +37:10:54.8
21:55:18.34 +37:03:14.0
22:08:34.54 +37:33:21.7
21:27:12.31 +39:44:01.9
21:50:07.60 +42:10:52.3
21:58:36.20 +41:09:22.1
21:39:06.43 +37:40:28.2
21:27:03.54 +35:21:30.8
21:48:57.08 +34:21:29.2
21:55:06.39 +37:00:04.1
22:00:12.79 +35:06:22.8
21:44:51.82 +36:12:11.9
21:31:26.58 +33:46:05.0
22:02:35.28 +41:45:10.0
21:43:22.57 +35:03:28.2
21:31:50.19 +41:32:47.9
21:49:28.11 +38:12:24.9
21:31:00.37 +36:55:32.7
21:50:53.87 +40:31:54.1
21:55:08.90 +41:19:55.0
21:47:51.33 +40:21:48.7
22:04:51.59 +36:57:55.6
21:36:58.18 +37:51:35.4
21:26:51.51 +34:03:07.6
21:44:25.94 +38:03:28.6
21:31:55.98 +35:27:42.5
21:29:23.73 +35:04:44.7
21:39:31.89 +40:39:06.1
21:55:36.71 +38:47:53.5
21:50:52.87 +41:13:07.7
22:06:00.60 +35:37:20.3
21:38:51.07 +37:54:38.7
21:28:15.72 +34:43:42.3
21:28:08.23 +36:20:36.7
21:35:18.86 +33:54:53.5
22:08:10.72 +39:02:00.5
21:31:29.47 +33:55:37.8
21:29:53.00 +36:05:31.8
21:47:18.26 +36:55:52.2
21:32:35.94 +35:36:10.5
21:48:18.39 +36:18:17.3
21:58:49.44 +40:28:41.5
21:51:11.88 +37:00:39.9
21:51:49.80 +37:26:00.3
21:37:52.96 +35:41:21.3
21:46:21.03 +36:51:38.6
21:51:39.07 +36:55:27.1
21:28:28.56 +35:45:20.7
21:43:25.59 +36:45:52.5
22:00:27.70 +40:13:15.7
21:43:05.89 +37:32:43.1
21:45:44.91 +38:12:59.8
21:46:36.83 +37:07:17.3
21:41:31.67 +37:12:07.8
21:45:18.28 +34:36:16.9
21:34:30.37 +33:45:39.6
21:53:38.94 +34:51:15.5
21:45:08.10 +34:06:59.6
21:29:56.04 +35:08:35.1
21:46:56.43 +37:17:27.2
22:08:40.10 +38:50:06.8
21:40:38.86 +39:10:23.2
22:02:22.46 +41:34:46.0
21:46:43.25 +34:59:48.9
21:43:09.86 +39:56:52.1
21:38:19.68 +39:47:34.9
21:35:24.48 +35:59:57.1
21:39:41.36 +36:54:57.7
21:45:58.80 +39:55:46.0
21:50:17.51 +42:04:58.0
21:45:18.10 +37:39:33.6
22:02:43.02 +36:12:43.0
21:30:03.94 +35:14:05.6
21:40:19.77 +35:37:23.1
21:46:14.54 +37:25:06.3
21:49:25.02 +42:02:02.4
21:42:07.94 +34:27:43.3
21:54:32.76 +35:25:31.2
22:09:41.40 +37:45:14.5
21:40:55.58 +35:54:46.6
21:59:43.47 +35:08:50.8
21:51:42.10 +40:48:55.3
21:50:22.21 +36:49:01.4
21:43:28.74 +37:46:46.7
21:38:40.51 +35:56:34.2
21:43:52.41 +39:31:29.7
22:03:45.54 +37:16:44.0
21:45:01.30 +42:15:59.8
21:45:06.45 +36:34:12.2
21:45:42.14 +34:31:02.7
22:05:29.70 +37:47:39.1
21:46:29.51 +35:05:33.5
21:40:28.52 +37:56:37.5
21:50:53.20 +41:33:16.5
21:44:02.25 +38:00:17.7
21:46:33.32 +36:26:40.4
21:18:30.91 +41:07:55.5
21:26:52.38 +41:39:00.4
###################################################################################
21:51:06.25 +37:29:04.1 -- not an asteroid (will add it to exclusion list)
21:48:41.00 +41:58:38.6 -- not an asteroid (will add it to exclusion list)
21:49:17.84 +40:40:26.6 -- not an asteroid (will add it to exclusion list)
21:59:58.68 +41:37:47.8 -- not an asteroid (will add it to exclusion list)
22:06:54.83 +41:38:24.1 -- not an asteroid (will add it to exclusion list)
21:43:24.75 +37:27:40.3 -- not an asteroid (will add it to exclusion list)
21:34:08.01 +36:35:12.1 -- not an asteroid (will add it to exclusion list)
21:27:51.06 +36:06:23.5 -- not an asteroid (will add it to exclusion list)
21:57:31.17 +38:48:28.2 -- not an asteroid (will add it to exclusion list)
21:45:42.22 +41:54:53.3 -- not an asteroid (will add it to exclusion list)
21:58:37.93 +35:47:10.9 -- not an asteroid (will add it to exclusion list)
21:45:02.91 +36:40:06.0 -- not an asteroid (will add it to exclusion list)
21:47:07.79 +38:39:18.7 -- not an asteroid (will add it to exclusion list)
21:47:04.59 +40:58:26.8 -- not an asteroid (will add it to exclusion list)
21:53:53.81 +41:17:50.0 -- not an asteroid (will add it to exclusion list)
21:34:19.66 +37:09:36.8 -- not an asteroid (will add it to exclusion list)
21:50:15.92 +34:58:33.6 -- not an asteroid (will add it to exclusion list)
21:29:02.89 +40:09:05.6 -- not an asteroid (will add it to exclusion list)
21:36:44.06 +39:54:02.6 -- not an asteroid (will add it to exclusion list)
21:44:38.60 +38:02:23.9 -- not an asteroid (will add it to exclusion list)
21:36:54.42 +37:55:38.0 -- not an asteroid (will add it to exclusion list)
21:39:53.77 +37:58:52.8 -- not an asteroid (will add it to exclusion list)
21:40:07.72 +34:33:18.6 -- not an asteroid (will add it to exclusion list)
21:27:29.88 +38:47:35.3 -- not an asteroid (will add it to exclusion list)
21:27:35.74 +41:34:26.3 -- not an asteroid (will add it to exclusion list)
21:31:28.79 +39:48:09.4 -- not an asteroid (will add it to exclusion list)
21:35:26.39 +41:08:48.9 -- not an asteroid (will add it to exclusion list)
21:42:09.02 +41:33:18.7 -- not an asteroid (will add it to exclusion list)
22:02:59.35 +41:26:45.6 -- not an asteroid (will add it to exclusion list)
21:40:14.01 +36:18:19.9 -- not an asteroid (will add it to exclusion list)
21:29:00.27 +38:59:29.9 -- not an asteroid (will add it to exclusion list)
21:37:48.52 +41:23:34.6 -- not an asteroid (will add it to exclusion list)
21:42:06.53 +39:57:24.1 -- not an asteroid (will add it to exclusion list)
21:58:28.64 +40:10:15.9 -- not an asteroid (will add it to exclusion list)
21:41:28.44 +41:30:42.9 -- not an asteroid (will add it to exclusion list)
21:59:26.27 +37:53:39.1 -- not an asteroid (will add it to exclusion list)
21:48:31.19 +41:08:42.6 -- not an asteroid (will add it to exclusion list)
21:44:03.08 +37:47:35.5 -- not an asteroid (will add it to exclusion list)
21:55:39.52 +36:53:21.5 -- not an asteroid (will add it to exclusion list)
21:39:43.16 +34:48:30.4 -- not an asteroid (will add it to exclusion list)
22:05:37.35 +38:57:39.8 -- not an asteroid (will add it to exclusion list)
21:49:03.69 +39:29:38.5 -- not an asteroid (will add it to exclusion list)
21:38:23.51 +40:06:13.9 -- not an asteroid (will add it to exclusion list)
21:31:19.30 +37:55:42.1 -- not an asteroid (will add it to exclusion list)
21:28:06.25 +33:41:27.5 -- not an asteroid (will add it to exclusion list)
22:05:10.51 +37:28:20.7 -- not an asteroid (will add it to exclusion list)
21:58:00.61 +37:39:31.2 -- not an asteroid (will add it to exclusion list)
21:30:54.99 +34:30:59.3 -- not an asteroid (will add it to exclusion list)
21:28:22.13 +41:32:01.6 -- not an asteroid (will add it to exclusion list)
21:30:40.26 +41:59:21.8 -- not an asteroid (will add it to exclusion list)
21:37:14.43 +35:50:17.4 -- not an asteroid (will add it to exclusion list)
22:03:59.35 +40:08:11.4 -- not an asteroid (will add it to exclusion list)
21:51:46.23 +37:08:04.9 -- not an asteroid (will add it to exclusion list)
21:56:13.21 +35:31:23.9 -- not an asteroid (will add it to exclusion list)
21:33:10.12 +41:39:57.2 -- not an asteroid (will add it to exclusion list)
21:56:28.96 +37:56:46.4 -- not an asteroid (will add it to exclusion list)
21:44:23.93 +37:43:55.7 -- not an asteroid (will add it to exclusion list)
21:48:12.44 +41:41:11.1 -- not an asteroid (will add it to exclusion list)
21:38:50.77 +35:08:49.5 -- not an asteroid (will add it to exclusion list)
21:27:26.96 +35:34:46.7 -- not an asteroid (will add it to exclusion list)
21:43:17.68 +38:29:47.6 -- not an asteroid (will add it to exclusion list)
21:30:43.77 +34:28:20.2 -- not an asteroid (will add it to exclusion list)
21:40:43.71 +37:22:58.9 -- not an asteroid (will add it to exclusion list)
21:33:57.71 +41:11:31.3 -- not an asteroid (will add it to exclusion list)
21:39:48.72 +38:17:17.1 -- not an asteroid (will add it to exclusion list)
21:26:09.20 +40:15:19.5 -- not an asteroid (will add it to exclusion list)
21:43:35.25 +37:12:37.5 -- not an asteroid (will add it to exclusion list)
21:32:48.36 +39:29:40.1 -- not an asteroid (will add it to exclusion list)
22:06:48.50 +39:07:17.3 -- not an asteroid (will add it to exclusion list)
21:29:37.11 +34:43:56.6 -- not an asteroid (will add it to exclusion list)
21:34:13.43 +42:00:56.8 -- not an asteroid (will add it to exclusion list)
22:01:22.36 +40:55:07.0 -- not an asteroid (will add it to exclusion list)
21:40:56.27 +41:13:23.4 -- not an asteroid (will add it to exclusion list)
22:06:21.81 +39:23:02.5 -- not an asteroid (will add it to exclusion list)
21:58:41.91 +39:00:24.6 -- not an asteroid (will add it to exclusion list)
21:35:58.63 +38:02:59.5 -- not an asteroid (will add it to exclusion list)
21:48:47.08 +40:08:12.8 -- not an asteroid (will add it to exclusion list)
21:26:50.66 +37:00:11.1 -- not an asteroid (will add it to exclusion list)
21:28:20.33 +39:05:27.1 -- not an asteroid (will add it to exclusion list)
21:34:37.64 +34:15:57.0 -- not an asteroid (will add it to exclusion list)
22:11:02.22 +38:11:05.6 -- not an asteroid (will add it to exclusion list)
22:03:31.27 +39:03:21.3 -- not an asteroid (will add it to exclusion list)
22:10:31.99 +41:45:05.3 -- not an asteroid (will add it to exclusion list)
22:00:14.34 +41:40:32.5 -- not an asteroid (will add it to exclusion list)
22:02:11.36 +35:32:41.1 -- not an asteroid (will add it to exclusion list)
21:27:24.11 +33:39:56.7 -- not an asteroid (will add it to exclusion list)
21:40:40.97 +36:19:19.9 -- not an asteroid (will add it to exclusion list)
21:31:28.70 +38:53:30.8 -- not an asteroid (will add it to exclusion list)
22:05:39.85 +34:53:38.1 -- not an asteroid (will add it to exclusion list)
21:51:51.69 +41:19:45.6 -- not an asteroid (will add it to exclusion list)
21:59:20.89 +36:56:48.2 -- not an asteroid (will add it to exclusion list)
21:33:13.71 +37:12:42.7 -- not an asteroid (will add it to exclusion list)
22:06:01.44 +39:10:16.5 -- not an asteroid (will add it to exclusion list)
21:46:25.62 +39:38:17.9 -- not an asteroid (will add it to exclusion list)
21:37:46.88 +36:44:33.3 -- not an asteroid (will add it to exclusion list)
21:28:11.90 +34:45:20.1 -- not an asteroid (will add it to exclusion list)
21:27:20.09 +35:46:48.3 -- not an asteroid (will add it to exclusion list)
21:30:31.96 +35:46:44.6 -- not an asteroid (will add it to exclusion list)
21:59:33.49 +41:27:38.5 -- not an asteroid (will add it to exclusion list)
21:28:41.97 +34:20:03.0 -- not an asteroid (will add it to exclusion list)
22:01:26.27 +38:07:01.0 -- not an asteroid (will add it to exclusion list)
21:41:57.33 +40:22:13.9 -- not an asteroid (will add it to exclusion list)
21:29:15.48 +38:35:05.1 -- not an asteroid (will add it to exclusion list)
21:57:16.71 +37:31:04.8 -- not an asteroid (will add it to exclusion list)
21:29:30.58 +37:27:31.5 -- not an asteroid (will add it to exclusion list)
22:01:18.65 +41:30:27.0 -- not an asteroid (will add it to exclusion list)
21:59:06.38 +34:00:17.5 -- not an asteroid (will add it to exclusion list)
21:34:29.33 +39:23:37.9 -- not an asteroid (will add it to exclusion list)
21:31:14.96 +38:46:29.2 -- not an asteroid (will add it to exclusion list)
21:42:51.25 +37:54:04.8 -- not an asteroid (will add it to exclusion list)
21:44:42.92 +35:29:06.6 -- not an asteroid (will add it to exclusion list)
22:09:13.48 +39:15:45.4 -- not an asteroid (will add it to exclusion list)
22:02:13.90 +41:47:06.4 -- not an asteroid (will add it to exclusion list)
21:44:09.46 +37:55:02.4 -- not an asteroid (will add it to exclusion list)
21:42:12.45 +38:54:23.1 -- not an asteroid (will add it to exclusion list)
21:44:26.49 +41:28:25.9 -- not an asteroid (will add it to exclusion list)
22:02:14.79 +34:37:06.2 -- not an asteroid (will add it to exclusion list)
21:43:31.53 +35:02:27.4 -- not an asteroid (will add it to exclusion list)
21:53:19.48 +36:06:08.2 -- not an asteroid (will add it to exclusion list)
21:44:06.73 +37:26:46.3 -- not an asteroid (will add it to exclusion list)
22:06:31.80 +34:33:31.3 -- not an asteroid (will add it to exclusion list)
22:02:42.44 +41:44:09.0 -- not an asteroid (will add it to exclusion list)
21:29:41.53 +38:48:30.5 -- not an asteroid (will add it to exclusion list)
21:57:42.00 +40:41:31.7 -- not an asteroid (will add it to exclusion list)
22:05:01.98 +41:27:43.6 -- not an asteroid (will add it to exclusion list)
22:04:59.74 +39:57:17.2 -- not an asteroid (will add it to exclusion list)
22:09:46.14 +41:39:55.4 -- not an asteroid (will add it to exclusion list)
22:02:04.69 +37:45:26.0 -- not an asteroid (will add it to exclusion list)
21:39:00.59 +38:41:33.2 -- not an asteroid (will add it to exclusion list)
21:47:33.59 +37:22:54.8 -- not an asteroid (will add it to exclusion list)
21:49:41.22 +37:43:27.7 -- not an asteroid (will add it to exclusion list)
21:40:47.54 +37:32:55.6 -- not an asteroid (will add it to exclusion list)
21:47:48.83 +38:11:35.7 -- not an asteroid (will add it to exclusion list)
21:27:14.50 +36:18:38.9 -- not an asteroid (will add it to exclusion list)
21:32:00.66 +39:23:57.8 -- not an asteroid (will add it to exclusion list)
22:11:12.57 +37:18:40.2 -- not an asteroid (will add it to exclusion list)
21:41:04.24 +37:16:07.0 -- not an asteroid (will add it to exclusion list)
21:58:43.13 +42:11:57.6 -- not an asteroid (will add it to exclusion list)
21:27:37.80 +38:16:28.5 -- not an asteroid (will add it to exclusion list)
21:30:29.32 +34:39:51.4 -- not an asteroid (will add it to exclusion list)
21:58:18.35 +39:25:59.2 -- not an asteroid (will add it to exclusion list)
22:09:48.54 +36:44:29.8 -- not an asteroid (will add it to exclusion list)
22:01:12.18 +35:17:05.4 -- not an asteroid (will add it to exclusion list)
21:48:57.93 +37:42:53.0 -- not an asteroid (will add it to exclusion list)
21:57:06.51 +36:41:43.9 -- not an asteroid (will add it to exclusion list)
22:05:42.72 +35:53:00.3 -- not an asteroid (will add it to exclusion list)
21:56:29.34 +36:52:33.7 -- not an asteroid (will add it to exclusion list)
21:44:34.11 +41:24:31.9 -- not an asteroid (will add it to exclusion list)
21:35:24.00 +36:47:15.8 -- not an asteroid (will add it to exclusion list)
21:58:25.00 +35:15:16.4 -- not an asteroid (will add it to exclusion list)
21:41:07.37 +34:51:42.7 -- not an asteroid (will add it to exclusion list)
21:29:55.36 +37:14:39.4 -- not an asteroid (will add it to exclusion list)
22:09:11.53 +36:46:04.1 -- not an asteroid (will add it to exclusion list)
21:27:00.72 +33:45:01.6 -- not an asteroid (will add it to exclusion list)
21:49:23.24 +36:27:43.6 -- not an asteroid (will add it to exclusion list)
21:41:49.97 +40:05:14.3 -- not an asteroid (will add it to exclusion list)
21:36:03.27 +36:35:42.2 -- not an asteroid (will add it to exclusion list)
21:38:38.24 +33:58:29.0 -- not an asteroid (will add it to exclusion list)
22:01:20.08 +41:45:31.1 -- not an asteroid (will add it to exclusion list)
22:04:54.62 +35:49:30.4 -- not an asteroid (will add it to exclusion list)
21:55:49.60 +34:16:12.6 -- not an asteroid (will add it to exclusion list)
21:47:12.11 +36:46:39.0 -- not an asteroid (will add it to exclusion list)
22:10:20.09 +38:44:18.8 -- not an asteroid (will add it to exclusion list)
21:56:34.42 +37:00:24.9 -- not an asteroid (will add it to exclusion list)
21:32:24.43 +37:16:08.5 -- not an asteroid (will add it to exclusion list)
21:40:15.48 +37:50:19.6 -- not an asteroid (will add it to exclusion list)
21:33:14.76 +33:54:31.4 -- not an asteroid (will add it to exclusion list)
21:50:58.66 +36:44:36.3 -- not an asteroid (will add it to exclusion list)
21:50:34.35 +37:11:01.0 -- not an asteroid (will add it to exclusion list)
21:48:46.56 +35:26:19.9 -- not an asteroid (will add it to exclusion list)
22:06:12.26 +39:36:02.7 -- not an asteroid (will add it to exclusion list)
21:56:00.51 +37:10:54.8 -- not an asteroid (will add it to exclusion list)
21:55:18.34 +37:03:14.0 -- not an asteroid (will add it to exclusion list)
22:08:34.54 +37:33:21.7 -- not an asteroid (will add it to exclusion list)
21:27:12.31 +39:44:01.9 -- not an asteroid (will add it to exclusion list)
21:50:07.60 +42:10:52.3 -- not an asteroid (will add it to exclusion list)
21:58:36.20 +41:09:22.1 -- not an asteroid (will add it to exclusion list)
21:39:06.43 +37:40:28.2 -- not an asteroid (will add it to exclusion list)
21:27:03.54 +35:21:30.8 -- not an asteroid (will add it to exclusion list)
21:48:57.08 +34:21:29.2 -- not an asteroid (will add it to exclusion list)
21:55:06.39 +37:00:04.1 -- not an asteroid (will add it to exclusion list)
22:00:12.79 +35:06:22.8 -- not an asteroid (will add it to exclusion list)
21:44:51.82 +36:12:11.9 -- not an asteroid (will add it to exclusion list)
21:31:26.58 +33:46:05.0 -- not an asteroid (will add it to exclusion list)
22:02:35.28 +41:45:10.0 -- not an asteroid (will add it to exclusion list)
21:43:22.57 +35:03:28.2 -- not an asteroid (will add it to exclusion list)
21:31:50.19 +41:32:47.9 -- not an asteroid (will add it to exclusion list)
21:49:28.11 +38:12:24.9 -- not an asteroid (will add it to exclusion list)
21:31:00.37 +36:55:32.7 -- not an asteroid (will add it to exclusion list)
21:50:53.87 +40:31:54.1 -- not an asteroid (will add it to exclusion list)
21:55:08.90 +41:19:55.0 -- not an asteroid (will add it to exclusion list)
21:47:51.33 +40:21:48.7 -- not an asteroid (will add it to exclusion list)
22:04:51.59 +36:57:55.6 -- not an asteroid (will add it to exclusion list)
21:36:58.18 +37:51:35.4 -- not an asteroid (will add it to exclusion list)
21:26:51.51 +34:03:07.6 -- not an asteroid (will add it to exclusion list)
21:44:25.94 +38:03:28.6 -- not an asteroid (will add it to exclusion list)
21:31:55.98 +35:27:42.5 -- not an asteroid (will add it to exclusion list)
21:29:23.73 +35:04:44.7 -- not an asteroid (will add it to exclusion list)
21:39:31.89 +40:39:06.1 -- not an asteroid (will add it to exclusion list)
21:55:36.71 +38:47:53.5 -- not an asteroid (will add it to exclusion list)
21:50:52.87 +41:13:07.7 -- not an asteroid (will add it to exclusion list)
22:06:00.60 +35:37:20.3 -- not an asteroid (will add it to exclusion list)
21:38:51.07 +37:54:38.7 -- not an asteroid (will add it to exclusion list)
21:28:15.72 +34:43:42.3 -- not an asteroid (will add it to exclusion list)
21:28:08.23 +36:20:36.7 -- not an asteroid (will add it to exclusion list)
21:35:18.86 +33:54:53.5 -- not an asteroid (will add it to exclusion list)
22:08:10.72 +39:02:00.5 -- not an asteroid (will add it to exclusion list)
21:31:29.47 +33:55:37.8 -- not an asteroid (will add it to exclusion list)
21:29:53.00 +36:05:31.8 -- not an asteroid (will add it to exclusion list)
21:47:18.26 +36:55:52.2 -- not an asteroid (will add it to exclusion list)
21:32:35.94 +35:36:10.5 -- not an asteroid (will add it to exclusion list)
21:48:18.39 +36:18:17.3 -- not an asteroid (will add it to exclusion list)
21:58:49.44 +40:28:41.5 -- not an asteroid (will add it to exclusion list)
21:51:11.88 +37:00:39.9 -- not an asteroid (will add it to exclusion list)
21:51:49.80 +37:26:00.3 -- not an asteroid (will add it to exclusion list)
21:37:52.96 +35:41:21.3 -- not an asteroid (will add it to exclusion list)
21:46:21.03 +36:51:38.6 -- not an asteroid (will add it to exclusion list)
21:51:39.07 +36:55:27.1 -- not an asteroid (will add it to exclusion list)
21:28:28.56 +35:45:20.7 -- not an asteroid (will add it to exclusion list)
21:43:25.59 +36:45:52.5 -- not an asteroid (will add it to exclusion list)
22:00:27.70 +40:13:15.7 -- not an asteroid (will add it to exclusion list)
21:43:05.89 +37:32:43.1 -- not an asteroid (will add it to exclusion list)
21:45:44.91 +38:12:59.8 -- not an asteroid (will add it to exclusion list)
21:46:36.83 +37:07:17.3 -- not an asteroid (will add it to exclusion list)
21:41:31.67 +37:12:07.8 -- not an asteroid (will add it to exclusion list)
21:45:18.28 +34:36:16.9 -- not an asteroid (will add it to exclusion list)
21:34:30.37 +33:45:39.6 -- not an asteroid (will add it to exclusion list)
21:53:38.94 +34:51:15.5 -- not an asteroid (will add it to exclusion list)
21:45:08.10 +34:06:59.6 -- not an asteroid (will add it to exclusion list)
21:29:56.04 +35:08:35.1 -- not an asteroid (will add it to exclusion list)
21:46:56.43 +37:17:27.2 -- not an asteroid (will add it to exclusion list)
22:08:40.10 +38:50:06.8 -- not an asteroid (will add it to exclusion list)
21:40:38.86 +39:10:23.2 -- not an asteroid (will add it to exclusion list)
22:02:22.46 +41:34:46.0 -- not an asteroid (will add it to exclusion list)
21:46:43.25 +34:59:48.9 -- not an asteroid (will add it to exclusion list)
21:43:09.86 +39:56:52.1 -- not an asteroid (will add it to exclusion list)
21:38:19.68 +39:47:34.9 -- not an asteroid (will add it to exclusion list)
21:35:24.48 +35:59:57.1 -- not an asteroid (will add it to exclusion list)
21:39:41.36 +36:54:57.7 -- not an asteroid (will add it to exclusion list)
21:45:58.80 +39:55:46.0 -- not an asteroid (will add it to exclusion list)
21:50:17.51 +42:04:58.0 -- not an asteroid (will add it to exclusion list)
21:45:18.10 +37:39:33.6 -- not an asteroid (will add it to exclusion list)
22:02:43.02 +36:12:43.0 -- not an asteroid (will add it to exclusion list)
21:30:03.94 +35:14:05.6 -- not an asteroid (will add it to exclusion list)
21:40:19.77 +35:37:23.1 -- not an asteroid (will add it to exclusion list)
21:46:14.54 +37:25:06.3 -- not an asteroid (will add it to exclusion list)
21:49:25.02 +42:02:02.4 -- not an asteroid (will add it to exclusion list)
21:42:07.94 +34:27:43.3 -- not an asteroid (will add it to exclusion list)
21:54:32.76 +35:25:31.2 -- not an asteroid (will add it to exclusion list)
22:09:41.40 +37:45:14.5 -- not an asteroid (will add it to exclusion list)
21:40:55.58 +35:54:46.6 -- not an asteroid (will add it to exclusion list)
21:59:43.47 +35:08:50.8 -- not an asteroid (will add it to exclusion list)
21:51:42.10 +40:48:55.3 -- not an asteroid (will add it to exclusion list)
21:50:22.21 +36:49:01.4 -- not an asteroid (will add it to exclusion list)
21:43:28.74 +37:46:46.7 -- not an asteroid (will add it to exclusion list)
21:38:40.51 +35:56:34.2 -- not an asteroid (will add it to exclusion list)
21:43:52.41 +39:31:29.7 -- not an asteroid (will add it to exclusion list)
22:03:45.54 +37:16:44.0 -- not an asteroid (will add it to exclusion list)
21:45:01.30 +42:15:59.8 -- not an asteroid (will add it to exclusion list)
21:45:06.45 +36:34:12.2 -- not an asteroid (will add it to exclusion list)
21:45:42.14 +34:31:02.7 -- not an asteroid (will add it to exclusion list)
22:05:29.70 +37:47:39.1 -- not an asteroid (will add it to exclusion list)
21:46:29.51 +35:05:33.5 -- not an asteroid (will add it to exclusion list)
21:40:28.52 +37:56:37.5 -- not an asteroid (will add it to exclusion list)
21:50:53.20 +41:33:16.5 -- not an asteroid (will add it to exclusion list)
21:44:02.25 +38:00:17.7 -- not an asteroid (will add it to exclusion list)
21:46:33.32 +36:26:40.4 -- not an asteroid (will add it to exclusion list)
21:18:30.91 +41:07:55.5 -- not an asteroid (will add it to exclusion list)
21:26:52.38 +41:39:00.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:18:30.91 +41:07:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:09.20 +40:15:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:50.66 +37:00:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:51.51 +34:03:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:52.38 +41:39:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:00.72 +33:45:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:03.54 +35:21:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:12.31 +39:44:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:14.50 +36:18:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:20.09 +35:46:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:24.11 +33:39:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:26.96 +35:34:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:29.88 +38:47:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:35.74 +41:34:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:37.80 +38:16:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:51.06 +36:06:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:06.25 +33:41:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:08.23 +36:20:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:11.90 +34:45:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:15.72 +34:43:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:20.33 +39:05:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:22.13 +41:32:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:28.56 +35:45:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:41.97 +34:20:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:00.27 +38:59:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:02.89 +40:09:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:15.48 +38:35:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:23.73 +35:04:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:30.58 +37:27:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:37.11 +34:43:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:41.53 +38:48:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:53.00 +36:05:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:55.36 +37:14:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:56.04 +35:08:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:03.94 +35:14:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:29.32 +34:39:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:31.96 +35:46:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:40.26 +41:59:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:43.77 +34:28:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:54.99 +34:30:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:00.37 +36:55:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:14.96 +38:46:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:19.30 +37:55:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:26.58 +33:46:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:28.70 +38:53:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:28.79 +39:48:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:29.47 +33:55:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:50.19 +41:32:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:55.98 +35:27:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:00.66 +39:23:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:24.43 +37:16:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:35.94 +35:36:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:48.36 +39:29:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:10.12 +41:39:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:13.71 +37:12:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:14.76 +33:54:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:57.71 +41:11:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:08.01 +36:35:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:13.43 +42:00:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:19.66 +37:09:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:29.33 +39:23:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:30.37 +33:45:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:37.64 +34:15:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:18.86 +33:54:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:24.00 +36:47:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:24.48 +35:59:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:26.39 +41:08:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:58.63 +38:02:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:03.27 +36:35:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:44.06 +39:54:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:54.42 +37:55:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:58.18 +37:51:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:14.43 +35:50:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:46.88 +36:44:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:48.52 +41:23:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:52.96 +35:41:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:19.68 +39:47:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:23.51 +40:06:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:38.24 +33:58:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:40.51 +35:56:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:50.77 +35:08:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:51.07 +37:54:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:00.59 +38:41:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:06.43 +37:40:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:31.89 +40:39:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:41.36 +36:54:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:43.16 +34:48:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:48.72 +38:17:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:53.77 +37:58:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:07.72 +34:33:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:14.01 +36:18:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:15.48 +37:50:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:19.77 +35:37:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:28.52 +37:56:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:38.86 +39:10:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:40.97 +36:19:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:43.71 +37:22:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:47.54 +37:32:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:55.58 +35:54:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:56.27 +41:13:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:04.24 +37:16:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:07.37 +34:51:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:28.44 +41:30:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:31.67 +37:12:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:49.97 +40:05:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:57.33 +40:22:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:06.53 +39:57:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:07.94 +34:27:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:09.02 +41:33:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:12.45 +38:54:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:51.25 +37:54:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:05.89 +37:32:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:09.86 +39:56:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:17.68 +38:29:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:22.57 +35:03:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:24.75 +37:27:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:25.59 +36:45:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:28.74 +37:46:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:31.53 +35:02:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:35.25 +37:12:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:52.41 +39:31:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:02.25 +38:00:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:03.08 +37:47:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:06.73 +37:26:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:09.46 +37:55:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:23.93 +37:43:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:25.94 +38:03:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:26.49 +41:28:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:34.11 +41:24:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:38.60 +38:02:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:42.92 +35:29:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:51.82 +36:12:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:01.30 +42:15:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:02.91 +36:40:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:06.45 +36:34:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:08.10 +34:06:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:18.10 +37:39:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:18.28 +34:36:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:42.14 +34:31:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:42.22 +41:54:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:44.91 +38:12:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:58.80 +39:55:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:14.54 +37:25:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:21.03 +36:51:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:25.62 +39:38:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:29.51 +35:05:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:33.32 +36:26:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:36.83 +37:07:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:43.25 +34:59:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:56.43 +37:17:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:04.59 +40:58:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:07.79 +38:39:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:12.11 +36:46:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:18.26 +36:55:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:33.59 +37:22:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:48.83 +38:11:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:51.33 +40:21:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:12.44 +41:41:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:18.39 +36:18:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:31.19 +41:08:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:41.00 +41:58:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:46.56 +35:26:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:47.08 +40:08:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:57.08 +34:21:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:57.93 +37:42:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:03.69 +39:29:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:17.84 +40:40:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:23.24 +36:27:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:25.02 +42:02:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:28.11 +38:12:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:41.22 +37:43:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:07.60 +42:10:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:15.92 +34:58:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:17.51 +42:04:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:22.21 +36:49:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:34.35 +37:11:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:52.87 +41:13:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:53.20 +41:33:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:53.87 +40:31:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:58.66 +36:44:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:06.25 +37:29:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:11.88 +37:00:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:39.07 +36:55:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:42.10 +40:48:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:46.23 +37:08:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:49.80 +37:26:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:51.69 +41:19:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:19.48 +36:06:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:38.94 +34:51:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:53.81 +41:17:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:32.76 +35:25:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:06.39 +37:00:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:08.90 +41:19:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:18.34 +37:03:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:36.71 +38:47:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:39.52 +36:53:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:49.60 +34:16:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:00.51 +37:10:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:13.21 +35:31:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:28.96 +37:56:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:29.34 +36:52:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:34.42 +37:00:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:06.51 +36:41:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:16.71 +37:31:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:31.17 +38:48:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:42.00 +40:41:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:00.61 +37:39:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:18.35 +39:25:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:25.00 +35:15:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:28.64 +40:10:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:36.20 +41:09:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:37.93 +35:47:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:41.91 +39:00:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:43.13 +42:11:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:49.44 +40:28:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:06.38 +34:00:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:20.89 +36:56:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:26.27 +37:53:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:33.49 +41:27:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:43.47 +35:08:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:58.68 +41:37:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:12.79 +35:06:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:14.34 +41:40:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:27.70 +40:13:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:12.18 +35:17:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:18.65 +41:30:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:20.08 +41:45:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:22.36 +40:55:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:26.27 +38:07:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:04.69 +37:45:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:11.36 +35:32:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:13.90 +41:47:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:14.79 +34:37:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:22.46 +41:34:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:35.28 +41:45:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.44 +41:44:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:43.02 +36:12:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:59.35 +41:26:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:31.27 +39:03:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:45.54 +37:16:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:59.35 +40:08:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:51.59 +36:57:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:54.62 +35:49:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:59.74 +39:57:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:01.98 +41:27:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:10.51 +37:28:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:29.70 +37:47:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:37.35 +38:57:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:39.85 +34:53:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:42.72 +35:53:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:00.60 +35:37:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:01.44 +39:10:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:12.26 +39:36:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:21.81 +39:23:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:31.80 +34:33:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:48.50 +39:07:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:54.83 +41:38:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:10.72 +39:02:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:34.54 +37:33:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:40.10 +38:50:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:11.53 +36:46:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:13.48 +39:15:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:41.40 +37:45:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:46.14 +41:39:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:48.54 +36:44:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:20.09 +38:44:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:31.99 +41:45:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:02.22 +38:11:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:12.57 +37:18:40.2 -- 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)
21:18:30.91 +41:07:55.5 -- a known variable star
21:26:09.20 +40:15:19.5 -- not a known variable star
21:26:50.66 +37:00:11.1 -- a known variable star
21:26:51.51 +34:03:07.6 -- not a known variable star
21:26:52.38 +41:39:00.4 -- a known variable star
21:27:00.72 +33:45:01.6 -- not a known variable star
21:27:03.54 +35:21:30.8 -- not a known variable star
21:27:12.31 +39:44:01.9 -- not a known variable star
21:27:14.50 +36:18:38.9 -- not a known variable star
21:27:20.09 +35:46:48.3 -- not a known variable star
21:27:24.11 +33:39:56.7 -- not a known variable star
21:27:26.96 +35:34:46.7 -- not a known variable star
21:27:29.88 +38:47:35.3 -- a known variable star
21:27:35.74 +41:34:26.3 -- not a known variable star
21:27:37.80 +38:16:28.5 -- not a known variable star
21:27:51.06 +36:06:23.5 -- not a known variable star
21:28:06.25 +33:41:27.5 -- not a known variable star
21:28:08.23 +36:20:36.7 -- not a known variable star
21:28:11.90 +34:45:20.1 -- not a known variable star
21:28:15.72 +34:43:42.3 -- not a known variable star
21:28:20.33 +39:05:27.1 -- not a known variable star
21:28:22.13 +41:32:01.6 -- not a known variable star
21:28:28.56 +35:45:20.7 -- not a known variable star
21:28:41.97 +34:20:03.0 -- a known variable star
21:29:00.27 +38:59:29.9 -- not a known variable star
21:29:02.89 +40:09:05.6 -- not a known variable star
21:29:15.48 +38:35:05.1 -- not a known variable star
21:29:23.73 +35:04:44.7 -- not a known variable star
21:29:30.58 +37:27:31.5 -- not a known variable star
21:29:37.11 +34:43:56.6 -- a known variable star
21:29:41.53 +38:48:30.5 -- not a known variable star
21:29:53.00 +36:05:31.8 -- not a known variable star
21:29:55.36 +37:14:39.4 -- not a known variable star
21:29:56.04 +35:08:35.1 -- not a known variable star
21:30:03.94 +35:14:05.6 -- a known variable star
21:30:29.32 +34:39:51.4 -- not a known variable star
21:30:31.96 +35:46:44.6 -- not a known variable star
21:30:40.26 +41:59:21.8 -- not a known variable star
21:30:43.77 +34:28:20.2 -- not a known variable star
21:30:54.99 +34:30:59.3 -- not a known variable star
21:31:00.37 +36:55:32.7 -- not a known variable star
21:31:14.96 +38:46:29.2 -- a known variable star
21:31:19.30 +37:55:42.1 -- not a known variable star
21:31:26.58 +33:46:05.0 -- not a known variable star
21:31:28.70 +38:53:30.8 -- a known variable star
21:31:28.79 +39:48:09.4 -- not a known variable star
21:31:29.47 +33:55:37.8 -- not a known variable star
21:31:50.19 +41:32:47.9 -- not a known variable star
21:31:55.98 +35:27:42.5 -- not a known variable star
21:32:00.66 +39:23:57.8 -- a known variable star
21:32:24.43 +37:16:08.5 -- not a known variable star
21:32:35.94 +35:36:10.5 -- not a known variable star
21:32:48.36 +39:29:40.1 -- not a known variable star
21:33:10.12 +41:39:57.2 -- not a known variable star
21:33:13.71 +37:12:42.7 -- not a known variable star
21:33:14.76 +33:54:31.4 -- not a known variable star
21:33:57.71 +41:11:31.3 -- a known variable star
21:34:08.01 +36:35:12.1 -- not a known variable star
21:34:13.43 +42:00:56.8 -- not a known variable star
21:34:19.66 +37:09:36.8 -- not a known variable star
21:34:29.33 +39:23:37.9 -- not a known variable star
21:34:30.37 +33:45:39.6 -- not a known variable star
21:34:37.64 +34:15:57.0 -- not a known variable star
21:35:18.86 +33:54:53.5 -- a known variable star
21:35:24.00 +36:47:15.8 -- not a known variable star
21:35:24.48 +35:59:57.1 -- not a known variable star
21:35:26.39 +41:08:48.9 -- not a known variable star
21:35:58.63 +38:02:59.5 -- not a known variable star
21:36:03.27 +36:35:42.2 -- not a known variable star
21:36:44.06 +39:54:02.6 -- not a known variable star
21:36:54.42 +37:55:38.0 -- not a known variable star
21:36:58.18 +37:51:35.4 -- not a known variable star
21:37:14.43 +35:50:17.4 -- not a known variable star
21:37:46.88 +36:44:33.3 -- a known variable star
21:37:48.52 +41:23:34.6 -- not a known variable star
21:37:52.96 +35:41:21.3 -- not a known variable star
21:38:19.68 +39:47:34.9 -- not a known variable star
21:38:23.51 +40:06:13.9 -- not a known variable star
21:38:38.24 +33:58:29.0 -- not a known variable star
21:38:40.51 +35:56:34.2 -- not a known variable star
21:38:50.77 +35:08:49.5 -- a known variable star
21:38:51.07 +37:54:38.7 -- not a known variable star
21:39:00.59 +38:41:33.2 -- not a known variable star
21:39:06.43 +37:40:28.2 -- not a known variable star
21:39:31.89 +40:39:06.1 -- not a known variable star
21:39:41.36 +36:54:57.7 -- not a known variable star
21:39:43.16 +34:48:30.4 -- not a known variable star
21:39:48.72 +38:17:17.1 -- not a known variable star
21:39:53.77 +37:58:52.8 -- not a known variable star
21:40:07.72 +34:33:18.6 -- not a known variable star
21:40:14.01 +36:18:19.9 -- not a known variable star
21:40:15.48 +37:50:19.6 -- not a known variable star
21:40:19.77 +35:37:23.1 -- a known variable star
21:40:28.52 +37:56:37.5 -- not a known variable star
21:40:38.86 +39:10:23.2 -- not a known variable star
21:40:40.97 +36:19:19.9 -- not a known variable star
21:40:43.71 +37:22:58.9 -- not a known variable star
21:40:47.54 +37:32:55.6 -- not a known variable star
21:40:55.58 +35:54:46.6 -- not a known variable star
21:40:56.27 +41:13:23.4 -- not a known variable star
21:41:04.24 +37:16:07.0 -- not a known variable star
21:41:07.37 +34:51:42.7 -- a known variable star
21:41:28.44 +41:30:42.9 -- not a known variable star
21:41:31.67 +37:12:07.8 -- not a known variable star
21:41:49.97 +40:05:14.3 -- not a known variable star
21:41:57.33 +40:22:13.9 -- not a known variable star
21:42:06.53 +39:57:24.1 -- not a known variable star
21:42:07.94 +34:27:43.3 -- not a known variable star
21:42:09.02 +41:33:18.7 -- not a known variable star
21:42:12.45 +38:54:23.1 -- a known variable star
21:42:51.25 +37:54:04.8 -- not a known variable star
21:43:05.89 +37:32:43.1 -- not a known variable star
21:43:09.86 +39:56:52.1 -- a known variable star
21:43:17.68 +38:29:47.6 -- not a known variable star
21:43:22.57 +35:03:28.2 -- not a known variable star
21:43:24.75 +37:27:40.3 -- not a known variable star
21:43:25.59 +36:45:52.5 -- not a known variable star
21:43:28.74 +37:46:46.7 -- a known variable star
21:43:31.53 +35:02:27.4 -- not a known variable star
21:43:35.25 +37:12:37.5 -- not a known variable star
21:43:52.41 +39:31:29.7 -- not a known variable star
21:44:02.25 +38:00:17.7 -- a known variable star
21:44:03.08 +37:47:35.5 -- not a known variable star
21:44:06.73 +37:26:46.3 -- not a known variable star
21:44:09.46 +37:55:02.4 -- not a known variable star
21:44:23.93 +37:43:55.7 -- not a known variable star
21:44:25.94 +38:03:28.6 -- not a known variable star
21:44:26.49 +41:28:25.9 -- not a known variable star
21:44:34.11 +41:24:31.9 -- not a known variable star
21:44:38.60 +38:02:23.9 -- not a known variable star
21:44:42.92 +35:29:06.6 -- a known variable star
21:44:51.82 +36:12:11.9 -- not a known variable star
21:45:01.30 +42:15:59.8 -- not a known variable star
21:45:02.91 +36:40:06.0 -- not a known variable star
21:45:06.45 +36:34:12.2 -- not a known variable star
21:45:08.10 +34:06:59.6 -- not a known variable star
21:45:18.10 +37:39:33.6 -- not a known variable star
21:45:18.28 +34:36:16.9 -- not a known variable star
21:45:42.14 +34:31:02.7 -- not a known variable star
21:45:42.22 +41:54:53.3 -- not a known variable star
21:45:44.91 +38:12:59.8 -- not a known variable star
21:45:58.80 +39:55:46.0 -- a known variable star
21:46:14.54 +37:25:06.3 -- not a known variable star
21:46:21.03 +36:51:38.6 -- not a known variable star
21:46:25.62 +39:38:17.9 -- not a known variable star
21:46:29.51 +35:05:33.5 -- not a known variable star
21:46:33.32 +36:26:40.4 -- not a known variable star
21:46:36.83 +37:07:17.3 -- not a known variable star
21:46:43.25 +34:59:48.9 -- not a known variable star
21:46:56.43 +37:17:27.2 -- not a known variable star
21:47:04.59 +40:58:26.8 -- a known variable star
21:47:07.79 +38:39:18.7 -- not a known variable star
21:47:12.11 +36:46:39.0 -- not a known variable star
21:47:18.26 +36:55:52.2 -- not a known variable star
21:47:33.59 +37:22:54.8 -- not a known variable star
21:47:48.83 +38:11:35.7 -- a known variable star
21:47:51.33 +40:21:48.7 -- not a known variable star
21:48:12.44 +41:41:11.1 -- not a known variable star
21:48:18.39 +36:18:17.3 -- not a known variable star
21:48:31.19 +41:08:42.6 -- not a known variable star
21:48:41.00 +41:58:38.6 -- not a known variable star
21:48:46.56 +35:26:19.9 -- not a known variable star
21:48:47.08 +40:08:12.8 -- not a known variable star
21:48:57.08 +34:21:29.2 -- a known variable star
21:48:57.93 +37:42:53.0 -- not a known variable star
21:49:03.69 +39:29:38.5 -- not a known variable star
21:49:17.84 +40:40:26.6 -- not a known variable star
21:49:23.24 +36:27:43.6 -- not a known variable star
21:49:25.02 +42:02:02.4 -- not a known variable star
21:49:28.11 +38:12:24.9 -- not a known variable star
21:49:41.22 +37:43:27.7 -- not a known variable star
21:50:07.60 +42:10:52.3 -- not a known variable star
21:50:15.92 +34:58:33.6 -- not a known variable star
21:50:17.51 +42:04:58.0 -- a known variable star
21:50:22.21 +36:49:01.4 -- not a known variable star
21:50:34.35 +37:11:01.0 -- not a known variable star
21:50:52.87 +41:13:07.7 -- not a known variable star
21:50:53.20 +41:33:16.5 -- not a known variable star
21:50:53.87 +40:31:54.1 -- a known variable star
21:50:58.66 +36:44:36.3 -- not a known variable star
21:51:06.25 +37:29:04.1 -- not a known variable star
21:51:11.88 +37:00:39.9 -- not a known variable star
21:51:39.07 +36:55:27.1 -- not a known variable star
21:51:42.10 +40:48:55.3 -- not a known variable star
21:51:46.23 +37:08:04.9 -- not a known variable star
21:51:49.80 +37:26:00.3 -- a known variable star
21:51:51.69 +41:19:45.6 -- not a known variable star
21:53:19.48 +36:06:08.2 -- not a known variable star
21:53:38.94 +34:51:15.5 -- not a known variable star
21:53:53.81 +41:17:50.0 -- not a known variable star
21:54:32.76 +35:25:31.2 -- not a known variable star
21:55:06.39 +37:00:04.1 -- not a known variable star
21:55:08.90 +41:19:55.0 -- a known variable star
21:55:18.34 +37:03:14.0 -- not a known variable star
21:55:36.71 +38:47:53.5 -- not a known variable star
21:55:39.52 +36:53:21.5 -- not a known variable star
21:55:49.60 +34:16:12.6 -- not a known variable star
21:56:00.51 +37:10:54.8 -- not a known variable star
21:56:13.21 +35:31:23.9 -- a known variable star
21:56:28.96 +37:56:46.4 -- not a known variable star
21:56:29.34 +36:52:33.7 -- not a known variable star
21:56:34.42 +37:00:24.9 -- not a known variable star
21:57:06.51 +36:41:43.9 -- not a known variable star
21:57:16.71 +37:31:04.8 -- not a known variable star
21:57:31.17 +38:48:28.2 -- not a known variable star
21:57:42.00 +40:41:31.7 -- not a known variable star
21:58:00.61 +37:39:31.2 -- not a known variable star
21:58:18.35 +39:25:59.2 -- not a known variable star
21:58:25.00 +35:15:16.4 -- not a known variable star
21:58:28.64 +40:10:15.9 -- not a known variable star
21:58:36.20 +41:09:22.1 -- not a known variable star
21:58:37.93 +35:47:10.9 -- not a known variable star
21:58:41.91 +39:00:24.6 -- not a known variable star
21:58:43.13 +42:11:57.6 -- not a known variable star
21:58:49.44 +40:28:41.5 -- not a known variable star
21:59:06.38 +34:00:17.5 -- not a known variable star
21:59:20.89 +36:56:48.2 -- not a known variable star
21:59:26.27 +37:53:39.1 -- not a known variable star
21:59:33.49 +41:27:38.5 -- not a known variable star
21:59:43.47 +35:08:50.8 -- not a known variable star
21:59:58.68 +41:37:47.8 -- not a known variable star
22:00:12.79 +35:06:22.8 -- not a known variable star
22:00:14.34 +41:40:32.5 -- not a known variable star
22:00:27.70 +40:13:15.7 -- not a known variable star
22:01:12.18 +35:17:05.4 -- not a known variable star
22:01:18.65 +41:30:27.0 -- not a known variable star
22:01:20.08 +41:45:31.1 -- a known variable star
22:01:22.36 +40:55:07.0 -- not a known variable star
22:01:26.27 +38:07:01.0 -- not a known variable star
22:02:04.69 +37:45:26.0 -- not a known variable star
22:02:11.36 +35:32:41.1 -- not a known variable star
22:02:13.90 +41:47:06.4 -- not a known variable star
22:02:14.79 +34:37:06.2 -- not a known variable star
22:02:22.46 +41:34:46.0 -- not a known variable star
22:02:35.28 +41:45:10.0 -- not a known variable star
22:02:42.44 +41:44:09.0 -- not a known variable star
22:02:43.02 +36:12:43.0 -- not a known variable star
22:02:59.35 +41:26:45.6 -- not a known variable star
22:03:31.27 +39:03:21.3 -- not a known variable star
22:03:45.54 +37:16:44.0 -- not a known variable star
22:03:59.35 +40:08:11.4 -- a known variable star
22:04:51.59 +36:57:55.6 -- a known variable star
22:04:54.62 +35:49:30.4 -- not a known variable star
22:04:59.74 +39:57:17.2 -- a known variable star
22:05:01.98 +41:27:43.6 -- not a known variable star
22:05:10.51 +37:28:20.7 -- not a known variable star
22:05:29.70 +37:47:39.1 -- not a known variable star
22:05:37.35 +38:57:39.8 -- not a known variable star
22:05:39.85 +34:53:38.1 -- a known variable star
22:05:42.72 +35:53:00.3 -- not a known variable star
22:06:00.60 +35:37:20.3 -- not a known variable star
22:06:01.44 +39:10:16.5 -- not a known variable star
22:06:12.26 +39:36:02.7 -- not a known variable star
22:06:21.81 +39:23:02.5 -- not a known variable star
22:06:31.80 +34:33:31.3 -- not a known variable star
22:06:48.50 +39:07:17.3 -- not a known variable star
22:06:54.83 +41:38:24.1 -- not a known variable star
22:08:10.72 +39:02:00.5 -- a known variable star
22:08:34.54 +37:33:21.7 -- not a known variable star
22:08:40.10 +38:50:06.8 -- a known variable star
22:09:11.53 +36:46:04.1 -- not a known variable star
22:09:13.48 +39:15:45.4 -- not a known variable star
22:09:41.40 +37:45:14.5 -- not a known variable star
22:09:46.14 +41:39:55.4 -- not a known variable star
22:09:48.54 +36:44:29.8 -- not a known variable star
22:10:20.09 +38:44:18.8 -- a known variable star
22:10:31.99 +41:45:05.3 -- a known variable star
22:11:02.22 +38:11:05.6 -- not a known variable star
22:11:12.57 +37:18:40.2 -- not a known variable star
Found 230 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
269 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 269 (excluding asteroids and hot pixels, 230 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)2461188.88489380 -observatory V36
05:25:49.11 +25:12:39.3 Mercury (-0.9mag)
06:47:24.66 +24:50:46.6 Venus (-3.9mag)
02:18:22.89 +13:07:34.6 Mars (1.3mag)
07:39:41.93 +21:52:30.2 Jupiter (-1.9mag)
00:46:02.41 +02:30:05.6 Saturn (0.9mag)
03:57:36.29 +20:17:53.4 Uranus (5.8mag)
00:15:24.26 +00:12:35.2 Neptune (7.8mag)
20:33:51.59 -23:00:46.0 Pluto (14.5mag)
13:57:18.13 -17:24:41.6 Moon (-11.8mag)
-rw-r--r-- 1 apache apache 363 May 28 05:35 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461188.88489380:
07:39:38.71 +21:52:41.0 Io (6.0mag)
07:39:39.67 +21:52:38.9 Europa (6.1mag)
07:40:00.38 +21:51:39.9 Ganymede (5.5mag)
07:39:12.29 +21:53:51.5 Callisto (6.7mag)
07:40:38.93 +21:28:42.4 Himalia (15.5mag)
07:39:46.56 +21:52:16.8 Thebe (16.5mag)
07:40:54.61 +21:48:59.8 Elara (17.5mag)
07:41:17.33 +22:10:04.1 Pasiphae (17.7mag)
07:46:43.94 +21:53:28.1 Carme (18.8mag)
00:46:12.62 +02:29:50.2 Titan (8.7mag)
00:46:07.98 +02:30:05.0 Rhea (10.0mag)
00:46:28.79 +02:30:36.7 Iapetus (11.4mag)
00:46:12.26 +02:30:25.0 Hyperion (14.7mag)
00:46:57.51 +02:33:34.2 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 28 05:35 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461188.88489380:
17:18:26.84 -33:48:05.9 JWST
11:11:37.69 +48:15:56.9 Chandra
09:23:37.83 -53:35:21.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 28 05:35 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461188.88489380 -observatory V36
13:19:01.32 -26:49:54.1 14.4mag D/1884 O1 (Barnard)
06:41:15.31 +30:36:41.8 15.7mag D/1886 K1 (Brooks)
15:24:16.34 +01:25:52.7 14.6mag D/1895 Q1 (Swift)
05:31:43.47 +24:43:28.0 17.2mag D/1918 W1 (Schorr)
09:46:37.51 +12:31:16.3 17.9mag P/2009 WX51 (Catalina)
18:49:57.50 -31:49:50.5 13.7mag P/2010 H2 (Vales)
05:42:58.88 -68:13:25.5 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:45:08.23 +31:50:02.4 17.5mag C/2017 K2 (PANSTARRS)
17:19:00.84 +14:42:19.6 17.7mag C/2021 G2 (ATLAS)
19:47:59.56 -51:35:55.7 17.9mag P/2021 N1 (ZTF)
23:14:21.19 +31:08:42.2 17.2mag C/2022 E2 (ATLAS)
05:20:43.91 +26:53:00.3 16.4mag C/2022 N2 (PANSTARRS)
09:22:21.69 +31:25:48.0 16.6mag C/2022 QE78 (ATLAS)
08:45:03.54 +03:21:06.4 17.6mag C/2022 R6 (PANSTARRS)
18:35:02.36 +21:17:31.3 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:23:32.51 -11:01:35.7 17.5mag P/2023 B1 (PANSTARRS)
22:16:14.60 +65:49:01.4 17.7mag C/2023 H5 (Lemmon)
18:12:09.23 -05:42:47.9 13.7mag C/2023 R1 (PANSTARRS)
13:33:06.87 +85:21:02.9 17.9mag C/2023 X2 (Lemmon)
06:56:09.46 +63:59:04.9 17.6mag C/2024 A1 (ATLAS)
06:30:25.78 +26:44:18.1 13.2mag C/2024 E1 (Wierzchos)
15:46:02.84 +12:27:22.2 17.3mag C/2024 G6 (ATLAS)
20:18:54.27 +27:51:09.7 14.1mag C/2024 J3 (ATLAS)
04:07:11.26 -16:58:36.7 16.1mag C/2024 T5 (ATLAS)
05:55:44.81 +36:24:44.2 17.9mag C/2025 J1 (Borisov)
11:43:10.25 +53:15:57.6 17.0mag C/2025 L1 (ATLAS)
06:29:04.62 -10:19:52.8 12.9mag C/2025 R3 (PANSTARRS)
12:40:36.83 +04:38:43.3 17.2mag C/2025 Y1 (ATLAS)
01:40:40.49 +42:34:23.0 15.8mag C/2026 B2 (Sun-Gao)
11:10:19.36 -08:00:09.1 16.3mag A/2026 E1
20:03:45.49 -08:08:29.9 9.3mag 10P/Tempel
14:17:51.11 -02:57:09.5 17.8mag 24P/Schaumasse
10:59:59.92 -00:52:16.7 15.9mag 29P/Schwassmann-Wachmann
10:52:48.65 -02:35:12.3 17.8mag 43P/Wolf-Harrington
02:54:54.28 +24:09:06.1 17.6mag 47P/Ashbrook-Jackson
08:36:56.02 +26:46:29.9 16.9mag 63P/Wild
00:17:02.23 -07:08:42.8 15.7mag 65P/Gunn
06:08:39.12 +32:02:25.1 16.6mag 76P/West-Kohoutek-Ikemura
02:43:12.97 +15:43:16.6 13.9mag 78P/Gehrels
00:56:20.94 +02:21:32.3 15.3mag 88P/Howell
04:19:50.33 +29:13:35.4 15.2mag 93P/Lovas
02:13:15.61 +25:45:41.1 17.9mag 114P/Wiseman-Skiff
06:25:05.76 +33:18:02.4 15.7mag 123P/West-Hartley
09:31:39.59 +19:18:26.8 16.4mag 124P/Mrkos
03:41:13.47 +18:27:51.7 16.4mag 128P/Shoemaker-Holt
04:11:59.09 +18:29:31.3 17.7mag 131P/Mueller
05:09:18.09 +19:33:36.8 13.3mag 141P/Machholz
05:11:51.13 +16:41:23.0 13.2mag 141P-A/Machholz
03:58:11.01 +14:13:28.0 10.7mag 141P-D/Machholz
02:49:50.38 -26:18:09.9 17.2mag 161P/Hartley-IRAS
03:06:48.16 +19:13:20.3 14.9mag 162P/SidingSpring
19:35:25.03 -01:10:40.6 17.4mag 169P/NEAT
23:48:56.77 +00:15:27.8 18.0mag 220P/McNaught
17:00:38.54 -09:10:37.9 16.3mag 235P/LINEAR
07:10:04.33 +35:49:30.8 17.4mag 240P/NEAT
00:04:14.01 -06:54:21.0 16.7mag 260P/McNaught
03:35:38.58 +30:22:50.1 17.6mag 295P/LINEAR
22:26:42.03 -24:36:25.0 17.6mag 320P/McNaught
15:20:33.97 +08:20:31.5 17.4mag 391P/Kowalski
07:58:50.03 +20:59:43.3 17.8mag 450P/LONEOS
06:42:20.68 +42:26:27.2 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 3.0K May 28 05:35 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
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 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
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
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
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
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
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
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
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 2026-04-9.14 13.64
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 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
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
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
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
-rw-r--r-- 1 apache apache 5.6K May 28 05:35 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
-rw-r--r-- 1 apache apache 188K May 28 05:35 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:20:11.486 +09:24:13.02 AT 2026nbc 2026-04-24.43 21.0629
10:03:54.706 +03:13:12.09 AT 2026nbb 2026-05-18.00 23.44
15:12:52.836 +15:19:04.18 SN 2026nba 2026-05-10.29 21.0132
13:32:20.126 +01:34:12.61 SN 2026naz 2026-05-13.26 20.8156
14:56:58.087 +36:57:10.58 AT 2026nay 2026-05-19.27 19.6866
11:46:04.206 +13:54:30.53 AT 2026nax 2026-05-07.19 20.6018
12:09:12.149 +41:27:00.14 AT 2026naw 2026-05-11.29 20.6337
06:25:45.633 -48:14:58.83 AT 2026nav 2026-05-04.02 18.255
06:58:22.644 -55:50:37.36 AT 2026nau 2026-05-18.96 18.984
08:46:46.014 +33:52:05.28 AT 2026nat 2026-05-17.28 19.023
10:01:59.220 +03:28:24.29 AT 2026nas 2026-05-16.99 23.35
08:33:18.216 +19:20:44.80 AT 2026nar 2026-05-18.88 19.333
12:51:56.463 +16:16:53.32 SN 2026naq 2026-05-19.19 19.6515
08:02:36.297 +15:58:21.39 AT 2026nap 2026-05-15.16 19.132
12:35:48.509 -01:02:49.40 AT 2026nao 2026-05-16.27 20.0531
11:46:27.658 +23:07:49.57 AT 2026nan 2026-05-08.18 20.1914
11:15:28.304 -01:08:27.49 AT 2026nam 2026-05-16.20 20.4814
02:05:49.697 -30:29:09.67 AT 2026nal 2026-05-18.43 15.4
12:23:18.242 +28:09:07.23 SN 2026nak 2026-05-18.88 19.67
13:47:06.036 +18:15:15.14 AT 2026naj 2026-05-17.91 19.77
-rw-r--r-- 1 apache apache 30K May 28 05:35 tns_transients_list.txt
