This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1
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 03.3828 2461163.8828 11.89 21:36:44.13 +39:54:01.8
87.23584 -9.11110 galactic Cyg Second-epoch detections are separated by 1.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:44.13 +39:54:01.8 (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 21:36:44.13 +39:54:01.8: 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 21:36:44.13 +39:54:01.8: 13.96 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.8828,11.89,0.05,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 20260503.3828 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 03.3828 2461163.8828 11.74 21:58:28.78 +40:10:16.7
90.62892 -11.61152 galactic Lac Second-epoch detections are separated by 1.7" and 6.4 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 | 21:58:28.78 +40:10:16.7 (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 21:58:28.78 +40:10:16.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:28.78 +40:10:16.7: 13.92 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.92 +/- 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+40.1726,2461163.8828,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.6214+40.1726 20260503.3828 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 03.3828 2461163.8828 11.70 21:40:34.76 +39:13:18.4
87.32852 -10.11167 galactic Cyg Second-epoch detections are separated by 1.6" and 6.4 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 | 21:40:34.76 +39:13:18.4 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.403+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:34.76 +39:13:18.4: 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 21:40:34.76 +39:13:18.4: 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
target,2461163.8828,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.3828 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 11.87 21:35:26.34 +41:08:46.5
87.90626 -8.02799 galactic Cyg Second-epoch detections are separated by 0.9" and 6.6 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 | 21:35:26.34 +41:08:46.5 (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 21:35:26.34 +41:08:46.5: 13.55 +/- 0.36 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:26.34 +41:08:46.5: 13.38 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.39 +/- 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+41.1463,2461163.8828,11.87,0.05,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
ATO J323.8637+41.1463 20260503.3828 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 03.3828 2461163.8828 11.63 21:39:48.79 +38:17:16.0
86.57916 -10.70451 galactic Cyg Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.9588+38.2866 | 21:39:48.79 +38:17:16.0 (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 21:39:48.79 +38:17:16.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:48.79 +38:17:16.0: 13.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.20 +/- 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+38.2866,2461163.8828,11.63,0.05,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 J324.9588+38.2866 20260503.3828 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 03.3828 2461163.8828 11.60 21:44:49.78 +36:36:01.4
86.18573 -12.62546 galactic Cyg Second-epoch detections are separated by 1.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:49.78 +36:36:01.4 (user input) | T | P | (position from user input) J-Ks=0.798+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:49.78 +36:36:01.4: 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 21:44:49.78 +36:36:01.4: 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
target,2461163.8828,11.60,0.05,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
target 20260503.3828 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 03.3828 2461163.8828 11.78 21:35:13.87 +36:45:19.3
84.84017 -11.21324 galactic Cyg Second-epoch detections are separated by 4.0" and 6.3 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 1951817552320582272 | 21:35:14.75 +36:45:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) 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 21:35:13.87 +36:45:19.3: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:13.87 +36:45:19.3: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 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 1951817552320582272,2461163.8828,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951817552320582272 20260503.3828 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 03.3828 2461163.8828 11.54 22:10:02.36 +38:52:02.6
91.63034 -14.00224 galactic Lac Second-epoch detections are separated by 2.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:10:02.36 +38:52:02.6 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:02.36 +38:52:02.6: 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 22:10:02.36 +38:52:02.6: 13.89 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461163.8828,11.54,0.05,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
target 20260503.3828 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 03.3828 2461163.8828 11.55 22:03:06.32 +40:42:36.4
91.67579 -11.72903 galactic Lac Second-epoch detections are separated by 2.8" and 6.4 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 | 22:03:06.32 +40:42:36.4 (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 22:03:06.32 +40:42:36.4: 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 22:03:06.32 +40:42:36.4: 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
target,2461163.8828,11.55,0.05,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 20260503.3828 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 03.3828 2461163.8828 11.49 21:26:09.33 +40:15:19.0
86.00037 -7.45973 galactic Cyg Second-epoch detections are separated by 3.4" and 7.2 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 | 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 21:26:09.33 +40:15:19.0: 11.69 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:09.33 +40:15:19.0: 13.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.70 +/- 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+401448.8,2461163.8828,11.49,0.05,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
ASASSN-V J212609.84+401448.8 20260503.3828 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 03.3828 2461163.8828 11.44 21:59:42.09 +38:13:15.1
89.57497 -13.28518 galactic Lac Second-epoch detections are separated by 0.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:42.09 +38:13:15.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:42.09 +38:13:15.1: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:42.09 +38:13:15.1: 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
target,2461163.8828,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.3828 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 03.3828 2461163.8828 11.49 22:01:04.22 +40:40:18.9
91.34044 -11.52318 galactic Lac Second-epoch detections are separated by 1.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.2723+40.6698 | 22:01:04.22 +40:40:18.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.559+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:04.22 +40:40:18.9: 13.57 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:04.22 +40:40:18.9: 13.87 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.2723+40.6698,2461163.8828,11.49,0.05,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
ATO J330.2723+40.6698 20260503.3828 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 03.3828 2461163.8828 11.45 21:34:27.13 +39:22:50.4
86.55135 -9.19338 galactic Cyg Second-epoch detections are separated by 2.6" and 6.9 pix
The object was found in VSX 3" Gaia DR3 1965875770554659200
Type: ROT
# Max. Min./Amp. JD0 Period
13.840 G 13.860 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 21:34:27.13 +39:22:50.4: 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 21:34:27.13 +39:22:50.4: 13.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.31 +/- 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 1965875770554659200,2461163.8828,11.45,0.05,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
Gaia DR3 1965875770554659200 20260503.3828 11.45CV 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 03.3828 2461163.8828 11.47 21:40:43.82 +37:22:58.5
86.09638 -11.49642 galactic Cyg Second-epoch detections are separated by 0.7" and 7.0 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 | 21:40:43.82 +37:22:58.5 (user input) | T | P | (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 21:40:43.82 +37:22:58.5: 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 21:40:43.82 +37:22:58.5: 13.70 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.8828,11.47,0.05,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
target 20260503.3828 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 03.3828 2461163.8828 11.41 21:57:39.32 +41:47:17.4
91.52941 -10.24889 galactic Lac Second-epoch detections are separated by 0.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.4174+41.7911 | 21:57:39.32 +41:47:17.4 (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 21:57:39.32 +41:47:17.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:39.32 +41:47:17.4: 13.43 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.4174+41.7911,2461163.8828,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.4174+41.7911 20260503.3828 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 11.46 22:01:22.43 +40:55:07.1
91.54128 -11.36373 galactic Lac Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.3389+40.9153 | 22:01:22.43 +40:55:07.1 (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 22:01:22.43 +40:55:07.1: 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 22:01:22.43 +40:55:07.1: 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
ATO J330.3389+40.9153,2461163.8828,11.46,0.05,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 J330.3389+40.9153 20260503.3828 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 03.3828 2461163.8828 11.59 21:30:08.33 +37:30:26.5
84.62137 -9.96850 galactic Cyg Second-epoch detections are separated by 3.3" and 6.6 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 J322.5413+37.5123 | 21:30:08.33 +37:30:26.5 (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 21:30:08.33 +37:30:26.5: 11.81 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:08.33 +37:30:26.5: 12.91 +/- 0.04 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 J322.5413+37.5123,2461163.8828,11.59,0.05,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 J322.5413+37.5123 20260503.3828 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 03.3828 2461163.8828 11.41 21:57:03.83 +40:57:15.8
90.91247 -10.83167 galactic Cyg Second-epoch detections are separated by 3.4" and 6.8 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 | 21:57:03.83 +40:57:15.8 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:03.83 +40:57:15.8: 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 21:57:03.83 +40:57:15.8: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.44 +/- 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,2461163.8828,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.3828 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 11.24 21:40:12.53 +37:22:51.1
86.01670 -11.42832 galactic Cyg Second-epoch detections are separated by 0.4" and 6.9 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 1952694649060067840 | 21:40:13.14 +37:22:20.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.354+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:12.53 +37:22:51.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:12.53 +37:22:51.1: 13.16 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952694649060067840,2461163.8828,11.24,0.05,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 1952694649060067840 20260503.3828 11.24CV 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 03.3828 2461163.8828 11.21 21:28:22.78 +38:27:06.0
85.03637 -9.04962 galactic Cyg Second-epoch detections are separated by 1.1" and 6.7 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 1964266905862674048 | 21:28:23.43 +38:27:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.394+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:22.78 +38:27:06.0: 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 21:28:22.78 +38:27:06.0: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 1964266905862674048,2461163.8828,11.21,0.05,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 1964266905862674048 20260503.3828 11.21CV 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 03.3828 2461163.8828 11.18 22:00:14.24 +41:40:32.2
91.84347 -10.63532 galactic Lac Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.0567+41.6700 | 22:00:14.24 +41:40:32.2 (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 22:00:14.24 +41:40:32.2: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:14.24 +41:40:32.2: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.99 +/- 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+41.6700,2461163.8828,11.18,0.05,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 J330.0567+41.6700 20260503.3828 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 03.3828 2461163.8828 11.21 21:40:56.40 +41:13:23.4
88.73341 -8.66625 galactic Cyg Second-epoch detections are separated by 0.7" and 6.5 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 J325.2343+41.2229 | 21:40:56.40 +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 21:40:56.40 +41:13:23.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:56.40 +41:13:23.4: 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
ATO J325.2343+41.2229,2461163.8828,11.21,0.05,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 J325.2343+41.2229 20260503.3828 11.21CV 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 03.3828 2461163.8828 11.11 21:48:47.13 +40:08:12.9
89.14875 -10.46190 galactic Cyg Second-epoch detections are separated by 1.4" and 6.3 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 J327.1964+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 21:48:47.13 +40:08:12.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:47.13 +40:08:12.9: 13.06 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.06 +/- 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+40.1375,2461163.8828,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.1964+40.1375 20260503.3828 11.11CV 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 03.3828 2461163.8828 11.12 21:26:23.51 +38:27:58.6
84.76551 -8.76670 galactic Cyg Second-epoch detections are separated by 2.0" and 6.6 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 | 21:26:23.51 +38:27:58.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.358+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:23.51 +38:27:58.6: 12.78 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:23.51 +38:27:58.6: 12.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.80 +/- 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,2461163.8828,11.12,0.05,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 20260503.3828 11.12CV 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 03.3828 2461163.8828 11.00 22:02:06.03 +36:06:25.6
88.60450 -15.23755 galactic Peg Second-epoch detections are separated by 3.6" and 6.7 pix
The object was found in VSX17" Gaia DR3 1948807192560317824
Type: ROT
# Max. Min./Amp. JD0 Period
14.030 G 14.060 G 8.170100000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:06.03 +36:06:25.6: 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 22:02:06.03 +36:06:25.6: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948807192560317824,2461163.8828,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948807192560317824 20260503.3828 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 11.08 21:41:05.77 +41:56:45.8
89.24098 -8.14539 galactic Cyg Second-epoch detections are separated by 2.0" and 6.4 pix
The object was found in VSX16" NSVS J2141045+415639
Type: L:
# Max. Min./Amp. JD0 Period
11.327 R1 Y 0.422 R1 54.000000000000
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 21:41:05.77 +41:56:45.8: 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 21:41:05.77 +41:56:45.8: 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
NSVS J2141045+415639,2461163.8828,11.08,0.05,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
NSVS J2141045+415639 20260503.3828 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 03.3828 2461163.8828 10.96 21:34:37.59 +34:15:56.2
82.99650 -12.93483 galactic Cyg Second-epoch detections are separated by 0.7" and 7.0 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 | 21:34:37.59 +34:15:56.2 (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 21:34:37.59 +34:15:56.2: 13.14 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:37.59 +34:15:56.2: 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
target,2461163.8828,10.96,0.05,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 20260503.3828 10.96CV 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 03.3828 2461163.8828 10.94 21:27:24.24 +33:39:57.3
81.47015 -12.31537 galactic Cyg Second-epoch detections are separated by 2.9" and 7.0 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 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 21:27:24.24 +33:39:57.3: 11.40 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:24.24 +33:39:57.3: 13.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 1854304305596960256,2461163.8828,10.94,0.05,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
Gaia DR3 1854304305596960256 20260503.3828 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 03.3828 2461163.8828 10.89 21:35:58.78 +38:02:59.5
85.85118 -10.36971 galactic Cyg Second-epoch detections are separated by 1.5" and 6.7 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 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 21:35:58.78 +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 21:35:58.78 +38:02:59.5: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952221343665700224,2461163.8828,10.89,0.05,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 1952221343665700224 20260503.3828 10.89CV 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 03.3828 2461163.8828 10.89 22:05:39.84 +34:53:38.7
88.41787 -16.63941 galactic Peg Second-epoch detections are separated by 0.6" and 7.0 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 22:05:39.84 +34:53:38.7: 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 22:05:39.84 +34:53:38.7: 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
Gaia DR3 1900468744392395008,2461163.8828,10.89,0.05,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 1900468744392395008 20260503.3828 10.89CV 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 03.3828 2461163.8828 10.95 21:51:51.67 +41:19:46.2
90.38091 -9.92242 galactic Cyg Second-epoch detections are separated by 1.0" and 6.3 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 | 21:51:51.67 +41:19:46.2 (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 21:51:51.67 +41:19:46.2: 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 21:51:51.67 +41:19:46.2: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 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,2461163.8828,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.3828 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 10.73 21:31:28.94 +38:53:29.7
85.78709 -9.15343 galactic Cyg Second-epoch detections are separated by 2.1" and 6.5 pix
The object was found in VSX 4" 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 21:31:28.94 +38:53:29.7: 13.11 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:28.94 +38:53:29.7: 12.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 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+385333.1,2461163.8828,10.73,0.05,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
ASASSN-V J213128.73+385333.1 20260503.3828 10.73CV 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 03.3828 2461163.8828 10.79 21:33:13.82 +37:12:42.8
84.86403 -10.60700 galactic Cyg Second-epoch detections are separated by 0.6" and 6.8 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 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 21:33:13.82 +37:12:42.8: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:13.82 +37:12:42.8: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 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 1952077135843691520,2461163.8828,10.79,0.05,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
Gaia DR3 1952077135843691520 20260503.3828 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 03.3828 2461163.8828 10.54 21:28:11.96 +34:45:26.5
82.37709 -11.65869 galactic Cyg Second-epoch detections are separated by 2.0" and 6.9 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 | 21:28:11.96 +34:45:26.5 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:11.96 +34:45:26.5: 10.91 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:11.96 +34:45:26.5: 12.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.88 +/- 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,2461163.8828,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.3828 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 10.48 21:28:09.28 +41:14:35.1
86.96865 -7.01652 galactic Cyg Second-epoch detections are separated by 1.0" and 6.5 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 J322.0200+41.2443 | 21:28:07.89 +41:14:23.4 (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 21:28:09.28 +41:14:35.1: 12.38 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:09.28 +41:14:35.1: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0200+41.2443,2461163.8828,10.48,0.05,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 J322.0200+41.2443 20260503.3828 10.48CV 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 03.3828 2461163.8828 10.70 21:35:21.82 +38:36:52.2
86.15240 -9.87425 galactic Cyg Second-epoch detections are separated by 1.4" and 6.7 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 1953795775599424384 | 21:35:22.92 +38:37:11.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.948+/-0.032 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:21.82 +38:36:52.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:21.82 +38:36:52.2: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 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 1953795775599424384,2461163.8828,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953795775599424384 20260503.3828 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 10.40 21:39:01.63 +41:05:55.9
88.37836 -8.51851 galactic Cyg Second-epoch detections are separated by 1.2" and 6.8 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 1966467720128308224 | 21:39:03.13 +41:06:06.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.631+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:01.63 +41:05:55.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:01.63 +41:05:55.9: 12.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.07 +/- 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 1966467720128308224,2461163.8828,10.40,0.05,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 1966467720128308224 20260503.3828 10.40CV 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 03.3828 2461163.8828 9.98 21:36:49.72 +39:45:20.1
87.14982 -9.22987 galactic Cyg Second-epoch detections are separated by 2.1" and 6.5 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 1965969366481229952 | 21:36:48.10 +39:45:16.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.284+/-0.035 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:49.72 +39:45:20.1: 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 21:36:49.72 +39:45:20.1: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1965969366481229952,2461163.8828,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1965969366481229952 20260503.3828 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 9.86 21:59:06.34 +34:00:16.5
86.73666 -16.48982 galactic Peg Second-epoch detections are separated by 0.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1947975824331378048 | 21:59:07.15 +34:00:38.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.727+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:06.34 +34:00:16.5: 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 21:59:06.34 +34:00:16.5: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 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 1947975824331378048,2461163.8828,9.86,0.05,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
Gaia DR3 1947975824331378048 20260503.3828 9.86CV 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 03.3828 2461163.8828 9.53 21:34:29.31 +39:23:38.5
86.56579 -9.18842 galactic Cyg Second-epoch detections are separated by 0.4" and 6.7 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 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 21:34:29.31 +39:23:38.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:29.31 +39:23:38.5: 11.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.24 +/- 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 1965875770554661504,2461163.8828,9.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1965875770554661504 20260503.3828 9.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 10.65 21:37:46.89 +36:44:33.7
85.21230 -11.57111 galactic Cyg Second-epoch detections are separated by 1.4" and 7.1 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 21:37:46.89 +36:44:33.7: 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 21:37:46.89 +36:44:33.7: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 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+364414.6,2461163.8828,10.65,0.05,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
ASASSN-V J213745.82+364414.6 20260503.3828 10.65CV 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 03.3828 2461163.8828 10.71 21:43:06.13 +37:12:25.7
86.33445 -11.94260 galactic Cyg Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:06.13 +37:12:25.7 (user input) | T | P | (position from user input) J-Ks=0.793+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:06.13 +37:12:25.7: 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 21:43:06.13 +37:12:25.7: 13.09 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 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,2461163.8828,10.71,0.05,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
target 20260503.3828 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 03.3828 2461163.8828 10.88 21:40:41.02 +36:19:20.0
85.36036 -12.27516 galactic Cyg Second-epoch detections are separated by 0.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1711+36.3226 | 21:40:38.96 +36:19:21.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:41.02 +36:19:20.0: 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 21:40:41.02 +36:19:20.0: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1711+36.3226,2461163.8828,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1711+36.3226 20260503.3828 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 10.83 22:02:13.91 +41:47:06.4
92.21108 -10.77669 galactic Lac Second-epoch detections are separated by 0.5" and 6.3 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 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 22:02:13.91 +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 22:02:13.91 +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+41.7805,2461163.8828,10.83,0.05,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 J330.5515+41.7805 20260503.3828 10.83CV 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 03.3828 2461163.8828 10.95 21:42:12.42 +38:54:23.2
87.35394 -10.55735 galactic Cyg Second-epoch detections are separated by 1.2" and 6.8 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 21:42:12.42 +38:54:23.2: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:12.42 +38:54:23.2: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 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+385425.2,2461163.8828,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214212.23+385425.2 20260503.3828 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 10.96 22:11:39.60 +42:09:38.3
93.87279 -11.52072 galactic Lac Second-epoch detections are separated by 1.6" and 6.1 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 1958339060720661248 | 22:11:41.43 +42:10:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.588+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:39.60 +42:09:38.3: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:39.60 +42:09:38.3: 13.42 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.42 +/- 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 1958339060720661248,2461163.8828,10.96,0.05,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 1958339060720661248 20260503.3828 10.96CV 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 03.3828 2461163.8828 11.06 21:49:58.87 +37:44:26.7
87.74548 -12.43782 galactic Cyg Second-epoch detections are separated by 1.7" and 6.8 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 J327.4891+37.7391 | 21:49:58.87 +37:44:26.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.408+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:58.87 +37:44:26.7: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:58.87 +37:44:26.7: 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 J327.4891+37.7391,2461163.8828,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.4891+37.7391 20260503.3828 11.06CV 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 03.3828 2461163.8828 11.12 22:02:15.09 +34:37:07.2
87.66600 -16.42128 galactic Peg Second-epoch detections are separated by 1.9" and 6.6 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 J330.5676+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 22:02:15.09 +34:37:07.2: 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 22:02:15.09 +34:37:07.2: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.5676+34.6142,2461163.8828,11.12,0.05,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 J330.5676+34.6142 20260503.3828 11.12CV 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 03.3828 2461163.8828 11.17 21:42:04.33 +40:56:44.4
88.70843 -9.01541 galactic Cyg Second-epoch detections are separated by 1.4" and 6.7 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 J325.5111+40.9358 | 21:42:04.42 +40:56:06.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 21:42:04.33 +40:56:44.4: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:04.33 +40:56:44.4: 13.38 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 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 J325.5111+40.9358,2461163.8828,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5111+40.9358 20260503.3828 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 11.22 22:02:42.16 +37:08:59.4
89.37071 -14.49361 galactic Lac Second-epoch detections are separated by 3.0" and 7.1 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 1954935045741178880 | 22:02:43.32 +37:08:15.0 (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 22:02:42.16 +37:08:59.4: 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 22:02:42.16 +37:08:59.4: 13.52 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.52 +/- 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 1954935045741178880,2461163.8828,11.22,0.05,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
Gaia DR3 1954935045741178880 20260503.3828 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 03.3828 2461163.8828 11.26 21:40:47.55 +37:32:56.8
86.21954 -11.38152 galactic Cyg Second-epoch detections are separated by 1.8" and 6.8 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 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 21:40:47.55 +37:32:56.8: 12.39 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:47.55 +37:32:56.8: 13.50 +/- 0.06 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
Gaia DR3 1953471527045546752,2461163.8828,11.26,0.05,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 1953471527045546752 20260503.3828 11.26CV 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 03.3828 2461163.8828 11.34 21:59:33.12 +37:57:30.3
89.38316 -13.47206 galactic Lac Second-epoch detections are separated by 3.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.8787+37.9479 | 21:59:33.12 +37:57:30.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.633+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:33.12 +37:57:30.3: 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 21:59:33.12 +37:57:30.3: 14.07 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.07 +/- 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 J329.8787+37.9479,2461163.8828,11.34,0.05,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
ATO J329.8787+37.9479 20260503.3828 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 03.3828 2461163.8828 11.20 21:44:26.46 +41:28:25.4
89.40001 -8.91222 galactic Cyg Second-epoch detections are separated by 0.2" and 6.6 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 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 21:44:26.46 +41:28:25.4: 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 21:44:26.46 +41:28:25.4: 13.33 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 1954551797221475456,2461163.8828,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1954551797221475456 20260503.3828 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 11.33 22:02:42.56 +41:44:09.0
92.25242 -10.87001 galactic Lac Second-epoch detections are separated by 2.5" and 6.7 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 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 22:02:42.56 +41:44:09.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:42.56 +41:44:09.0: 13.64 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959859277284333312,2461163.8828,11.33,0.05,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 1959859277284333312 20260503.3828 11.33CV 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 03.3828 2461163.8828 11.50 21:47:36.48 +40:21:16.9
89.11850 -10.15041 galactic Cyg Second-epoch detections are separated by 2.3" and 6.1 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 | 21:47:36.48 +40:21:16.9 (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 21:47:36.48 +40:21:16.9: 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 21:47:36.48 +40:21:16.9: 13.80 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.8828,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.3828 11.50CV 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 03.3828 2461163.8828 11.32 21:59:55.06 +41:57:02.5
91.96791 -10.38185 galactic Lac Second-epoch detections are separated by 0.5" and 6.5 pix
The object was found in VSX17" Gaia DR3 1959971393112412800
Type: ROT
# Max. Min./Amp. JD0 Period
14.590 G 14.640 G M
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 21:59:55.06 +41:57:02.5: 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 21:59:55.06 +41:57:02.5: 13.55 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.55 +/- 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 1959971393112412800,2461163.8828,11.32,0.05,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 1959971393112412800 20260503.3828 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 03.3828 2461163.8828 11.44 21:37:18.40 +40:36:04.6
87.79646 -8.66818 galactic Cyg Second-epoch detections are separated by 2.9" and 6.2 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 J324.3165+40.6074 | 21:37:15.79 +40:35:51.1 (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 21:37:18.40 +40:36:04.6: 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 21:37:18.40 +40:36:04.6: 13.55 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.55 +/- 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 J324.3165+40.6074,2461163.8828,11.44,0.05,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 J324.3165+40.6074 20260503.3828 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 03.3828 2461163.8828 11.47 21:39:00.47 +38:41:33.4
86.73756 -10.29896 galactic Cyg Second-epoch detections are separated by 4.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.7488+38.6969 | 21:38:58.77 +38:41:57.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.697+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:00.47 +38:41:33.4: 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 21:39:00.47 +38:41:33.4: 13.63 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.63 +/- 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 J324.7488+38.6969,2461163.8828,11.47,0.05,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
ATO J324.7488+38.6969 20260503.3828 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 03.3828 2461163.8828 11.46 21:59:27.59 +38:47:09.3
89.89814 -12.81358 galactic Lac Second-epoch detections are separated by 2.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:27.59 +38:47:09.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.774+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:27.59 +38:47:09.3: 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 21:59:27.59 +38:47:09.3: 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,2461163.8828,11.46,0.05,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 20260503.3828 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 03.3828 2461163.8828 11.50 21:48:57.89 +37:42:52.7
87.57172 -12.32709 galactic Cyg Second-epoch detections are separated by 1.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.2399+37.7077 | 21:48:57.59 +37:42:28.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:57.89 +37:42:52.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:57.89 +37:42:52.7: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.37 +/- 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+37.7077,2461163.8828,11.50,0.05,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
ATO J327.2399+37.7077 20260503.3828 11.50CV 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 03.3828 2461163.8828 11.52 21:48:12.53 +41:41:12.0
90.08187 -9.20957 galactic Cyg Second-epoch detections are separated by 1.3" and 6.6 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 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 21:48:12.53 +41:41:12.0: 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 21:48:12.53 +41:41:12.0: 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
Gaia DR3 1960503900338500992,2461163.8828,11.52,0.05,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 1960503900338500992 20260503.3828 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 03.3828 2461163.8828 11.69 21:33:26.67 +37:43:43.1
85.25708 -10.26143 galactic Cyg Second-epoch detections are separated by 1.0" and 6.9 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 1952201384956929536 | 21:33:25.97 +37:44:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.430+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:26.67 +37:43:43.1: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:26.67 +37:43:43.1: 13.62 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 1952201384956929536,2461163.8828,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952201384956929536 20260503.3828 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3828 2461163.8828 11.63 22:01:12.76 +38:02:20.6
89.69833 -13.61224 galactic Lac Second-epoch detections are separated by 3.7" and 6.2 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 J330.2927+38.0238 | 22:01:10.81 +38:01:52.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:12.76 +38:02:20.6: 12.81 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:12.76 +38:02:20.6: 13.54 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.2927+38.0238,2461163.8828,11.63,0.05,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 J330.2927+38.0238 20260503.3828 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 03.3828 2461163.8828 11.66 21:41:04.44 +37:19:15.5
86.10563 -11.58818 galactic Cyg Second-epoch detections are separated by 3.8" and 6.3 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 1952691251747209088 | 21:41:02.35 +37:19:26.6 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE J-Ks=0.731+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:04.44 +37:19:15.5: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:04.44 +37:19:15.5: 13.64 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952691251747209088,2461163.8828,11.66,0.05,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 1952691251747209088 20260503.3828 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 03.3828 2461163.8828 11.62 21:47:23.96 +34:53:12.0
85.42129 -14.25515 galactic Cyg Second-epoch detections are separated by 4.1" and 6.7 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 1947712555715677824 | 21:47:23.11 +34:53:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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 21:47:23.96 +34:53:12.0: 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 21:47:23.96 +34:53:12.0: 14.00 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 1947712555715677824,2461163.8828,11.62,0.05,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 1947712555715677824 20260503.3828 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 03.3828 2461163.8828 11.62 21:52:15.09 +36:58:29.9
87.59075 -13.31372 galactic Cyg Second-epoch detections are separated by 2.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:15.09 +36:58:29.9 (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 21:52:15.09 +36:58:29.9: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:15.09 +36:58:29.9: 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
target,2461163.8828,11.62,0.05,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 20260503.3828 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 03.3828 2461163.8828 11.83 21:46:53.96 +39:15:19.9
88.28495 -10.89544 galactic Cyg Second-epoch detections are separated by 3.5" and 7.2 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 | 21:46:53.96 +39:15:19.9 (user input) | T | P | (position from user input) J-Ks=0.595+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:53.96 +39:15:19.9: 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 21:46:53.96 +39:15:19.9: 14.35 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.8828,11.83,0.05,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 20260503.3828 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 03.3828 2461163.8828 11.89 21:56:00.45 +37:10:54.9
88.31908 -13.63368 galactic Cyg Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:00.45 +37:10:54.9 (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 21:56:00.45 +37:10:54.9: 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 21:56:00.45 +37:10:54.9: 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,2461163.8828,11.89,0.05,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 20260503.3828 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 03.3828 2461163.8828 11.91 21:38:19.80 +39:47:34.9
87.39109 -9.39699 galactic Cyg Second-epoch detections are separated by 2.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.5932+39.7857 | 21:38:19.80 +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 21:38:19.80 +39:47:34.9: 13.35 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:19.80 +39:47:34.9: 14.91 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.40 +/- 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+39.7857,2461163.8828,11.91,0.05,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
ATO J324.5932+39.7857 20260503.3828 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
## 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: 2461163.88306961 03.05.2026 09:11:27.214 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
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: 4 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): 15487
Objects passed selection criteria: 15468
Measurements per detected object (mean, median, min, max): 3.2 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 3.0 2 4
Average stars detected per image: 15106
Average stars matched: 13130.2 (86.9208 %)
Memory usage VmPeak: 124068 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 04:14:01 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: 2461163.88306961 03.05.2026 09:11:27.214 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 163
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: 64 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): 107121
Objects passed selection criteria: 106960
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 111688
Average stars matched: 100950 (90.386 %)
Memory usage VmPeak: 1923616 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 04:16:45 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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.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: 2461163.88244405
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_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.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_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits (1st new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
Image size: 937.8'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:07.178 +38:00:12.17 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 21:49:07.178 +38:00:12.17
Angular distance between the image centers 0.0448 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits (2nd new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
Image size: 937.8'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:04.311 +38:00:32.97 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 21:49:04.311 +38:00:32.97
Angular distance between the image centers 0.0343 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 21:49:07.178 +38:00:12.17
Second-epoch second image center 21:49:04.311 +38:00:32.97
Angular distance between the image centers 0.01104 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.pJN5zrabm6
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.qdXWdrq04V
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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits &> /tmp/tmp.tZsdY0coMi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits &> /tmp/tmp.AAj78aF3FB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
The reference image (wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits) and catalog (wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat) found
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Read 28429 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8517 to 337.9501 deg, Dec +32.2173 to +43.3775 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.8517 to 337.9501 deg, Dec 32.2173 to 43.3775 deg
Loaded 21151 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 23 out of 30 total matches.
Matched with Tycho-2 30 out of 28429 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.968900
a=0.000000 b=1.000000 c=22.968900
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 28429 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8517 to 337.9501 deg, Dec +32.2173 to +43.3775 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.8517 to 337.9501 deg, Dec 32.2173 to 43.3775 deg
Loaded 21151 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 23 out of 30 total matches.
Matched with Tycho-2 30 out of 28429 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits:
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits (aperture=6.2)
Read 21746 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.5217 to 337.7622 deg, Dec +32.2988 to +43.2789 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.5217 to 337.7622 deg, Dec 32.2988 to 43.2789 deg
Loaded 21125 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 13298 out of 14228 total matches.
Matched with Tycho-2 14228 out of 21746 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits:
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits (aperture=7.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 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_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
2.4 pix fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.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
14.3 mag. fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
14.3 mag. fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.5 (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.pJN5zrabm6 (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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/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)
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.qdXWdrq04V (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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/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! :)
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.tZsdY0coMi (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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.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_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1041, passed=13450
Got 13450 stars (including 12402 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat
util/solve_plate_with_UCAC5 got 13450 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 13279 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 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 13279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 13279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 967 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.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.AAj78aF3FB (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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.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_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1025, passed=13555
Got 13555 stars (including 12519 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat
util/solve_plate_with_UCAC5 got 13555 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 13433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 13435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 13435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 965 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits'
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.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_vSTL
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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Creating symlink local_wcs_cache/wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
Creating symlink local_wcs_cache/exclusion_list.txt
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
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
wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits exists and is non-empty
###################################
# 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_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits (1st new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
Image size: 937.8'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:07.178 +38:00:12.17 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 21:49:07.178 +38:00:12.17
Angular distance between the image centers 0.0448 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits (2nd new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
Image size: 937.8'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:04.311 +38:00:32.97 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 21:49:04.311 +38:00:32.97
Angular distance between the image centers 0.0343 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 21:49:07.178 +38:00:12.17
Second-epoch second image center 21:49:04.311 +38:00:32.97
Angular distance between the image centers 0.01104 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.GMwZRa9Z9q
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.sjAOp11Sv3
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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits &> /tmp/tmp.4qCpCylct2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits &> /tmp/tmp.awrGTXQKnt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
The reference image (wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits) and catalog (wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat) found
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Read 202105 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8070 to 338.0148 deg, Dec +32.1985 to +43.3825 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 316.8070 to 338.0148 deg, Dec 32.1985 to 43.3825 deg
Loaded 21303 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): 88 out of 119 total matches.
Matched with Tycho-2 119 out of 202105 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.387000
a=0.000000 b=1.000000 c=20.387000
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.98
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.98
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 202105 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8070 to 338.0148 deg, Dec +32.1985 to +43.3825 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 316.8070 to 338.0148 deg, Dec 32.1985 to 43.3825 deg
Loaded 21303 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): 88 out of 119 total matches.
Matched with Tycho-2 119 out of 202105 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=4.5)
Read 122789 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.5109 to 337.7859 deg, Dec +32.2804 to +43.2820 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 316.5109 to 337.7859 deg, Dec 32.2804 to 43.2820 deg
Loaded 21185 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): 12353 out of 15793 total matches.
Matched with Tycho-2 15793 out of 122789 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=5.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 139 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.8 pix Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
2.2 pix fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
2.3 pix fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
2.1 pix wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.8 pix wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Limiting magnitude estimates:
13.0 mag. Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
12.3 mag. Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
12.1 mag. fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
12.1 mag. fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
All-image limiting magnitude estimate: 12.1 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_vSTL
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.GMwZRa9Z9q (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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/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=65, blended=28738, passed=202040
Got 202040 stars (including 172959 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 202040 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 610 to 668 (Dec 32.2 to 43.4)
Done reading UCAC5 zone files...
Matched 409 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 372 matched stars entering correct_measured_positions(), 311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.16"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 369 matched stars entering correct_measured_positions(), 68006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.60"
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 610 to 668 (Dec 32.2 to 43.4)
Done reading UCAC5 zone files...
Matched 485 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 459 matched stars entering correct_measured_positions(), 68055 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.59"
Accuracy estimation diagnostic: 456 matched stars entering correct_measured_positions(), 86726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.74"
Excluding outliers - 456 stars left (next iteration limit 405)
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.sjAOp11Sv3 (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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/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=11, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=18258, passed=122767
Got 122767 stars (including 104392 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 122767 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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 120204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 120204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 120204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
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.4qCpCylct2 (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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.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_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=8859, passed=105236
Got 105236 stars (including 96248 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat
util/solve_plate_with_UCAC5 got 105236 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 103998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 103998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 103998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 962 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.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.awrGTXQKnt (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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.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_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.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_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=8868, passed=104472
Got 104472 stars (including 95451 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat
util/solve_plate_with_UCAC5 got 104472 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 103294 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 965 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(), 103294 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 103293 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 964 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-10-33_20.00sec_-4.90C_LIGHT_0347.fits
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cyg-07-Q2b1x1_041206_TTUQ2b1x1_1249055_rHJdGpY1/wcs_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348.fits
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:26.34 +41:08:46.5: 13.55 +/- 0.36 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:49.78 +36:36:01.4: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:48.79 +38:17:16.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:34.76 +39:13:18.4: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:02.36 +38:52:02.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:13.87 +36:45:19.3: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:44.13 +39:54:01.8: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:06.32 +40:42:36.4: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:28.78 +40:10:16.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:48.79 +38:17:16.0: 13.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.05
Forced photometry filter KEPT candidate at 21:39:48.79 +38:17:16.0: ref_mag=13.20 +/- 0.05 new_mean_mag=11.6175 delta=1.59 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:06.32 +40:42:36.4: 13.48 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:49.78 +36:36:01.4: 13.68 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:02.36 +38:52:02.6: 13.89 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.06
Forced photometry filter KEPT candidate at 22:03:06.32 +40:42:36.4: ref_mag=13.48 +/- 0.06 new_mean_mag=11.5520 delta=1.93 (need > 0.90)
Forced photometry reference-image weighted average: 13.68 +/- 0.07
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:26.34 +41:08:46.5: 13.38 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.09
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:09.33 +40:15:19.0: 11.69 +/- 0.07 detection
Forced photometry filter KEPT candidate at 21:44:49.78 +36:36:01.4: ref_mag=13.68 +/- 0.07 new_mean_mag=11.5894 delta=2.09 (need > 0.90)
Forced photometry filter KEPT candidate at 22:10:02.36 +38:52:02.6: ref_mag=13.89 +/- 0.09 new_mean_mag=11.5401 delta=2.35 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:34.76 +39:13:18.4: 13.54 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:28.78 +40:10:16.7: 13.92 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.06
Forced photometry filter KEPT candidate at 21:35:26.34 +41:08:46.5: ref_mag=13.39 +/- 0.06 new_mean_mag=11.8432 delta=1.55 (need > 0.90)
Forced photometry reference-image weighted average: 13.92 +/- 0.08
Forced photometry reference-image weighted average: 13.54 +/- 0.06
Forced photometry filter KEPT candidate at 21:58:28.78 +40:10:16.7: ref_mag=13.92 +/- 0.08 new_mean_mag=11.7198 delta=2.20 (need > 0.90)
Forced photometry filter KEPT candidate at 21:40:34.76 +39:13:18.4: ref_mag=13.54 +/- 0.06 new_mean_mag=11.6825 delta=1.86 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:13.87 +36:45:19.3: 13.19 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:44.13 +39:54:01.8: 13.96 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.04
Forced photometry reference-image weighted average: 13.96 +/- 0.09
Forced photometry filter KEPT candidate at 21:35:13.87 +36:45:19.3: ref_mag=13.19 +/- 0.04 new_mean_mag=11.7531 delta=1.44 (need > 0.90)
Forced photometry filter KEPT candidate at 21:36:44.13 +39:54:01.8: ref_mag=13.96 +/- 0.09 new_mean_mag=11.8949 delta=2.06 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:09.33 +40:15:19.0: 13.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.04
Forced photometry filter KEPT candidate at 21:26:09.33 +40:15:19.0: ref_mag=12.70 +/- 0.04 new_mean_mag=11.4937 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:42.09 +38:13:15.1: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:42.09 +38:13:15.1: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.06
Forced photometry filter KEPT candidate at 21:59:42.09 +38:13:15.1: ref_mag=13.67 +/- 0.06 new_mean_mag=11.4303 delta=2.24 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:04.22 +40:40:18.9: 13.57 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:04.22 +40:40:18.9: 13.87 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.09
Forced photometry filter KEPT candidate at 22:01:04.22 +40:40:18.9: ref_mag=13.85 +/- 0.09 new_mean_mag=11.4916 delta=2.36 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:27.13 +39:22:50.4: 12.76 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:43.82 +37:22:58.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:39.32 +41:47:17.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:27.13 +39:22:50.4: 13.36 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:22.43 +40:55:07.1: 13.61 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.31 +/- 0.05
Forced photometry filter KEPT candidate at 21:34:27.13 +39:22:50.4: ref_mag=13.31 +/- 0.05 new_mean_mag=11.4327 delta=1.87 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:08.33 +37:30:26.5: 11.81 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:43.82 +37:22:58.5: 13.70 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.07
Forced photometry filter KEPT candidate at 21:40:43.82 +37:22:58.5: ref_mag=13.70 +/- 0.07 new_mean_mag=11.4701 delta=2.23 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:39.32 +41:47:17.4: 13.43 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.06
Forced photometry filter KEPT candidate at 21:57:39.32 +41:47:17.4: ref_mag=13.43 +/- 0.06 new_mean_mag=11.4164 delta=2.01 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:22.43 +40:55:07.1: 13.62 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.06
Forced photometry filter KEPT candidate at 22:01:22.43 +40:55:07.1: ref_mag=13.62 +/- 0.06 new_mean_mag=11.4470 delta=2.17 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:08.33 +37:30:26.5: 12.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.03
Forced photometry filter KEPT candidate at 21:30:08.33 +37:30:26.5: ref_mag=12.71 +/- 0.03 new_mean_mag=11.5189 delta=1.19 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:03.83 +40:57:15.8: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:12.53 +37:22:51.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:03.83 +40:57:15.8: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.05
Forced photometry filter KEPT candidate at 21:57:03.83 +40:57:15.8: ref_mag=13.44 +/- 0.05 new_mean_mag=11.3799 delta=2.06 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:12.53 +37:22:51.1: 13.16 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
Forced photometry filter KEPT candidate at 21:40:12.53 +37:22:51.1: ref_mag=13.16 +/- 0.04 new_mean_mag=11.2421 delta=1.91 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:22.78 +38:27:06.0: 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 21:28:22.78 +38:27:06.0: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.04
Forced photometry filter KEPT candidate at 21:28:22.78 +38:27:06.0: ref_mag=12.90 +/- 0.04 new_mean_mag=11.2103 delta=1.69 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:14.24 +41:40:32.2: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:14.24 +41:40:32.2: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.04
Forced photometry filter KEPT candidate at 22:00:14.24 +41:40:32.2: ref_mag=12.99 +/- 0.04 new_mean_mag=11.1838 delta=1.81 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:56.40 +41:13:23.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:56.40 +41:13:23.4: 13.23 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.05
Forced photometry filter KEPT candidate at 21:40:56.40 +41:13:23.4: ref_mag=13.23 +/- 0.05 new_mean_mag=11.2030 delta=2.03 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:47.13 +40:08:12.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:47.13 +40:08:12.9: 13.06 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.04
Forced photometry filter KEPT candidate at 21:48:47.13 +40:08:12.9: ref_mag=13.06 +/- 0.04 new_mean_mag=11.1033 delta=1.96 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:23.51 +38:27:58.6: 12.78 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:23.51 +38:27:58.6: 12.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.04
Forced photometry filter KEPT candidate at 21:26:23.51 +38:27:58.6: ref_mag=12.80 +/- 0.04 new_mean_mag=11.1144 delta=1.69 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:06.03 +36:06:25.6: 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 22:02:06.03 +36:06:25.6: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.04
Forced photometry filter KEPT candidate at 22:02:06.03 +36:06:25.6: ref_mag=13.28 +/- 0.04 new_mean_mag=11.0043 delta=2.28 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:05.77 +41:56:45.8: 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 21:41:05.77 +41:56:45.8: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Forced photometry filter KEPT candidate at 21:41:05.77 +41:56:45.8: ref_mag=12.80 +/- 0.03 new_mean_mag=11.0759 delta=1.73 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:37.59 +34:15:56.2: 13.14 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:37.59 +34:15:56.2: 13.28 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.05
Forced photometry filter KEPT candidate at 21:34:37.59 +34:15:56.2: ref_mag=13.28 +/- 0.05 new_mean_mag=10.9520 delta=2.33 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:24.24 +33:39:57.3: 11.40 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:58.78 +38:02:59.5: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:39.84 +34:53:38.7: 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 21:27:24.24 +33:39:57.3: 13.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.04
Forced photometry filter KEPT candidate at 21:27:24.24 +33:39:57.3: ref_mag=12.39 +/- 0.04 new_mean_mag=10.9324 delta=1.45 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:58.78 +38:02:59.5: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Forced photometry filter KEPT candidate at 21:35:58.78 +38:02:59.5: ref_mag=12.85 +/- 0.03 new_mean_mag=10.8933 delta=1.96 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:39.84 +34:53:38.7: 13.23 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.05
Forced photometry filter KEPT candidate at 22:05:39.84 +34:53:38.7: ref_mag=13.23 +/- 0.05 new_mean_mag=10.8954 delta=2.34 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:51.67 +41:19:46.2: 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 21:51:51.67 +41:19:46.2: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Forced photometry filter KEPT candidate at 21:51:51.67 +41:19:46.2: ref_mag=12.92 +/- 0.03 new_mean_mag=10.9368 delta=1.98 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:28.94 +38:53:29.7: 13.11 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:28.94 +38:53:29.7: 12.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Forced photometry filter KEPT candidate at 21:31:28.94 +38:53:29.7: ref_mag=12.28 +/- 0.02 new_mean_mag=10.7217 delta=1.56 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:13.82 +37:12:42.8: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:13.82 +37:12:42.8: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.03
Forced photometry filter KEPT candidate at 21:33:13.82 +37:12:42.8: ref_mag=12.65 +/- 0.03 new_mean_mag=10.7756 delta=1.88 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:11.96 +34:45:26.5: 10.91 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:11.96 +34:45:26.5: 12.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.03
Forced photometry filter KEPT candidate at 21:28:11.96 +34:45:26.5: ref_mag=11.88 +/- 0.03 new_mean_mag=10.5430 delta=1.34 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:09.28 +41:14:35.1: 12.38 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:09.28 +41:14:35.1: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Forced photometry filter KEPT candidate at 21:28:09.28 +41:14:35.1: ref_mag=12.24 +/- 0.02 new_mean_mag=10.4593 delta=1.78 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:21.82 +38:36:52.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:21.82 +38:36:52.2: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Forced photometry filter KEPT candidate at 21:35:21.82 +38:36:52.2: ref_mag=12.56 +/- 0.02 new_mean_mag=10.6725 delta=1.88 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:01.63 +41:05:55.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:01.63 +41:05:55.9: 12.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.02
Forced photometry filter KEPT candidate at 21:39:01.63 +41:05:55.9: ref_mag=12.07 +/- 0.02 new_mean_mag=10.3888 delta=1.68 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:49.72 +39:45:20.1: 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 21:36:49.72 +39:45:20.1: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry filter KEPT candidate at 21:36:49.72 +39:45:20.1: ref_mag=11.81 +/- 0.01 new_mean_mag=9.9703 delta=1.84 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:06.34 +34:00:16.5: 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 21:59:06.34 +34:00:16.5: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry filter KEPT candidate at 21:59:06.34 +34:00:16.5: ref_mag=12.01 +/- 0.01 new_mean_mag=9.8575 delta=2.15 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:29.31 +39:23:38.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:29.31 +39:23:38.5: 11.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.01
Forced photometry filter KEPT candidate at 21:34:29.31 +39:23:38.5: ref_mag=11.24 +/- 0.01 new_mean_mag=9.5289 delta=1.71 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:46.89 +36:44:33.7: 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 21:37:46.89 +36:44:33.7: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.02
Forced photometry filter KEPT candidate at 21:37:46.89 +36:44:33.7: ref_mag=12.44 +/- 0.02 new_mean_mag=10.6189 delta=1.82 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:06.13 +37:12:25.7: 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 21:43:06.13 +37:12:25.7: 13.09 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.04
Forced photometry filter KEPT candidate at 21:43:06.13 +37:12:25.7: ref_mag=13.09 +/- 0.04 new_mean_mag=10.7123 delta=2.38 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:41.02 +36:19:20.0: 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 21:40:41.02 +36:19:20.0: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Forced photometry filter KEPT candidate at 21:40:41.02 +36:19:20.0: ref_mag=12.80 +/- 0.03 new_mean_mag=10.8667 delta=1.93 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:13.91 +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 22:02:13.91 +41:47:06.4: 12.81 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.03
Forced photometry filter KEPT candidate at 22:02:13.91 +41:47:06.4: ref_mag=12.81 +/- 0.03 new_mean_mag=10.8304 delta=1.98 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:12.42 +38:54:23.2: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:12.42 +38:54:23.2: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.04
Forced photometry filter KEPT candidate at 21:42:12.42 +38:54:23.2: ref_mag=13.14 +/- 0.04 new_mean_mag=10.9316 delta=2.21 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:39.60 +42:09:38.3: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:39.60 +42:09:38.3: 13.42 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.07
Forced photometry filter KEPT candidate at 22:11:39.60 +42:09:38.3: ref_mag=13.42 +/- 0.07 new_mean_mag=10.9513 delta=2.47 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:36.54 +37:49:17.9: 8.99 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:58.87 +37:44:26.7: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:58.87 +37:44:26.7: 13.30 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.05
Forced photometry filter KEPT candidate at 21:49:58.87 +37:44:26.7: ref_mag=13.30 +/- 0.05 new_mean_mag=11.0628 delta=2.24 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:36.54 +37:49:17.9: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 9.11 +/- 0.01
Forced photometry filter REJECTED candidate at 21:27:36.54 +37:49:17.9: ref_mag=9.11 +/- 0.01 new_mean_mag=11.0653 delta=-1.95 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:15.09 +34:37:07.2: 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 22:02:15.09 +34:37:07.2: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.05
Forced photometry filter KEPT candidate at 22:02:15.09 +34:37:07.2: ref_mag=13.40 +/- 0.05 new_mean_mag=11.1174 delta=2.28 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:04.33 +40:56:44.4: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:04.33 +40:56:44.4: 13.38 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
Forced photometry filter KEPT candidate at 21:42:04.33 +40:56:44.4: ref_mag=13.38 +/- 0.05 new_mean_mag=11.1674 delta=2.21 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:42.16 +37:08:59.4: 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 22:02:42.16 +37:08:59.4: 13.52 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.06
Forced photometry filter KEPT candidate at 22:02:42.16 +37:08:59.4: ref_mag=13.52 +/- 0.06 new_mean_mag=11.2193 delta=2.30 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:47.55 +37:32:56.8: 12.39 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:47.55 +37:32:56.8: 13.50 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.05
Forced photometry filter KEPT candidate at 21:40:47.55 +37:32:56.8: ref_mag=13.28 +/- 0.05 new_mean_mag=11.2564 delta=2.03 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:33.12 +37:57:30.3: 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 21:59:33.12 +37:57:30.3: 14.07 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.10
Forced photometry filter KEPT candidate at 21:59:33.12 +37:57:30.3: ref_mag=14.07 +/- 0.10 new_mean_mag=11.3155 delta=2.75 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:26.46 +41:28:25.4: 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 21:44:26.46 +41:28:25.4: 13.33 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.05
Forced photometry filter KEPT candidate at 21:44:26.46 +41:28:25.4: ref_mag=13.33 +/- 0.05 new_mean_mag=11.1931 delta=2.14 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:42.56 +41:44:09.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:42.56 +41:44:09.0: 13.64 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.07
Forced photometry filter KEPT candidate at 22:02:42.56 +41:44:09.0: ref_mag=13.64 +/- 0.07 new_mean_mag=11.3307 delta=2.31 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:36.48 +40:21:16.9: 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 21:47:36.48 +40:21:16.9: 13.80 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.08
Forced photometry filter KEPT candidate at 21:47:36.48 +40:21:16.9: ref_mag=13.80 +/- 0.08 new_mean_mag=11.5066 delta=2.29 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:55.06 +41:57:02.5: 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 21:59:55.06 +41:57:02.5: 13.55 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.07
Forced photometry filter KEPT candidate at 21:59:55.06 +41:57:02.5: ref_mag=13.55 +/- 0.07 new_mean_mag=11.3177 delta=2.24 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:18.40 +40:36:04.6: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:00.47 +38:41:33.4: 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 21:37:18.40 +40:36:04.6: 13.55 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.07
Forced photometry filter KEPT candidate at 21:37:18.40 +40:36:04.6: ref_mag=13.55 +/- 0.07 new_mean_mag=11.4403 delta=2.11 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:00.47 +38:41:33.4: 13.63 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.06
Forced photometry filter KEPT candidate at 21:39:00.47 +38:41:33.4: ref_mag=13.63 +/- 0.06 new_mean_mag=11.4755 delta=2.15 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:27.59 +38:47:09.3: 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 21:59:27.59 +38:47:09.3: 13.88 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.08
Forced photometry filter KEPT candidate at 21:59:27.59 +38:47:09.3: ref_mag=13.88 +/- 0.08 new_mean_mag=11.4671 delta=2.41 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:57.89 +37:42:52.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:57.89 +37:42:52.7: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.05
Forced photometry filter KEPT candidate at 21:48:57.89 +37:42:52.7: ref_mag=13.37 +/- 0.05 new_mean_mag=11.5013 delta=1.87 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:12.53 +41:41:12.0: 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 21:48:12.53 +41:41:12.0: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.05
Forced photometry filter KEPT candidate at 21:48:12.53 +41:41:12.0: ref_mag=13.27 +/- 0.05 new_mean_mag=11.5140 delta=1.76 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:26.67 +37:43:43.1: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:26.67 +37:43:43.1: 13.62 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.07
Forced photometry filter KEPT candidate at 21:33:26.67 +37:43:43.1: ref_mag=13.62 +/- 0.07 new_mean_mag=11.6895 delta=1.93 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:12.76 +38:02:20.6: 12.81 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:12.76 +38:02:20.6: 13.54 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.05
Forced photometry filter KEPT candidate at 22:01:12.76 +38:02:20.6: ref_mag=13.46 +/- 0.05 new_mean_mag=11.6360 delta=1.83 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:04.44 +37:19:15.5: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:04.44 +37:19:15.5: 13.64 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.07
Forced photometry filter KEPT candidate at 21:41:04.44 +37:19:15.5: ref_mag=13.64 +/- 0.07 new_mean_mag=11.6675 delta=1.98 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:23.96 +34:53:12.0: 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 21:47:23.96 +34:53:12.0: 14.00 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.09
Forced photometry filter KEPT candidate at 21:47:23.96 +34:53:12.0: ref_mag=14.00 +/- 0.09 new_mean_mag=11.6150 delta=2.38 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:15.09 +36:58:29.9: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:15.09 +36:58:29.9: 14.12 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.10
Forced photometry filter KEPT candidate at 21:52:15.09 +36:58:29.9: ref_mag=14.12 +/- 0.10 new_mean_mag=11.5823 delta=2.54 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:53.96 +39:15:19.9: 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 21:46:53.96 +39:15:19.9: 14.35 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.13
Forced photometry filter KEPT candidate at 21:46:53.96 +39:15:19.9: ref_mag=14.35 +/- 0.13 new_mean_mag=11.8177 delta=2.53 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:00.45 +37:10:54.9: 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 21:56:00.45 +37:10:54.9: 14.48 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.15
Forced photometry filter KEPT candidate at 21:56:00.45 +37:10:54.9: ref_mag=14.48 +/- 0.15 new_mean_mag=11.8925 delta=2.59 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:53.73 +40:06:52.6: 12.04 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:53.73 +40:06:52.6: 14.84 +/- 0.21 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.09
Forced photometry filter REJECTED candidate at 21:54:53.73 +40:06:52.6: ref_mag=12.49 +/- 0.09 new_mean_mag=12.1208 delta=0.37 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:19.80 +39:47:34.9: 13.35 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:19.80 +39:47:34.9: 14.91 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.18
Forced photometry filter KEPT candidate at 21:38:19.80 +39:47:34.9: ref_mag=14.40 +/- 0.18 new_mean_mag=11.8619 delta=2.54 (need > 0.90)
Adding exclusion_list_local.txt__out252929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253198.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254248.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 108s
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: 47s
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Considering the candidate 252929_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 252929_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 252933_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 252933_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 252953_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 252953_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 252958_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 252958_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 252965_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 252965_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 252979_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 252979_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 252987_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 252987_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 252996_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 252996_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:54:50.99 +40:08:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252999_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 252999_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253010_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253010_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253023_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253023_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253034_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253034_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253041_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253041_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253045_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253045_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253065_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253065_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253069_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253069_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253080_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253080_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253084_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253084_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253116_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253116_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253121_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253121_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253143_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253143_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:42:56.41 +37:35:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253151_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253151_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253161_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253161_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253169_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253169_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:29:06.80 +40:44:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253172_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253172_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253193_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253193_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253196_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253196_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253198_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253198_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253199_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253199_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:55:20.89 +40:52:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253209_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253209_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253213_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253213_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:58:28.18 +40:38:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253218_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253218_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253220_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253220_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253228_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253228_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253231_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253231_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253232_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253232_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:33:38.36 +37:37:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253239_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253239_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:41:19.40 +37:02:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253250_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253250_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253276_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253276_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 253278_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253278_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253279_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253279_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:05:08.23 +36:40:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253288_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253288_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253307_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253307_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:28:08.14 +36:39:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253311_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253311_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253313_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253313_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253314_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253314_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253322_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253322_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253359_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253359_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253360_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253360_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:31:39.28 +34:11:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253375_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253375_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253376_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253376_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:56:08.77 +41:50:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253385_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253385_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253398_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253398_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:01:07.94 +39:15:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253409_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253409_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:26:44.20 +37:33:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253420_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253420_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:31:50.40 +34:09:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253434_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253434_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:42:50.23 +37:29:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253436_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253436_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:47:14.37 +41:48:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253457_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253457_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:56:49.73 +42:13:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253463_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253463_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:11:47.79 +38:26:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253478_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253478_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253489_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253489_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:38:33.00 +37:54:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253490_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253490_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:29:32.65 +33:47:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253498_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253498_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:58:48.51 +41:41:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253523_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253523_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:36:19.75 +36:08:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253529_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253529_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:32:56.54 +34:26:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253530_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253530_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253534_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253534_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253535_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253535_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253536_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253536_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:39:05.43 +36:51:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253545_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253545_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253546_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253546_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:42:01.49 +37:34:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253547_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253547_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:07:05.51 +37:55:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253558_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253558_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253561_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253561_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:31:28.51 +35:34:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253564_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253564_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:32:54.44 +35:30:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253569_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253569_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:41:29.10 +37:46:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253572_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253572_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:50:04.41 +35:32:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253573_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253573_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:41:07.36 +41:16:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253583_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253583_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:57:40.55 +37:18:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253596_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253596_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:50:52.31 +39:37:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253598_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253598_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
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Considering the candidate 253603_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253603_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253604_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253604_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:42:06.24 +36:50:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253605_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253605_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:56:55.68 +36:07:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253608_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253608_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:08:10.01 +37:08:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253613_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253613_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:34:49.00 +41:16:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253616_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253616_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
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Considering the candidate 253621_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253621_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:01:53.30 +40:17:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253622_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253622_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:48:38.41 +41:48:07.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253624_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253624_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253642_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253642_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:36:22.22 +40:35:07.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253645_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253645_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:30:44.25 +41:40:26.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253649_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253649_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253650_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253650_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:58:07.78 +38:56:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253658_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253658_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253662_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253662_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:42:46.47 +37:59:50.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253670_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253670_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253675_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253675_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:52:09.06 +36:25:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253676_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253676_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253683_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253683_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:04:00.01 +39:46:40.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253684_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253684_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:57:06.75 +34:35:56.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253690_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253690_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:41:07.93 +34:22:02.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253693_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253693_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:42:22.95 +40:36:52.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253702_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253702_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:49:54.71 +34:54:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253715_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253715_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:01:13.37 +38:32:58.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253716_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253716_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:54:04.40 +37:39:39.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253718_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253718_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253733_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253733_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:01:01.59 +35:17:27.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253741_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253741_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:04:54.88 +37:38:39.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253746_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253746_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253752_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253752_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253776_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253776_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:02:40.33 +38:06:43.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253779_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253779_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:55:07.40 +37:29:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253784_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253784_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:43:32.10 +38:44:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253787_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253787_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:44:54.17 +33:55:44.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253788_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253788_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:00:54.61 +41:16:13.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253794_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253794_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253799_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253799_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253806_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253806_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:34:28.49 +39:24:31.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253815_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253815_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:27:59.90 +37:32:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253825_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253825_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253843_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253843_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:44:49.93 +36:56:54.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253846_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253846_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253881_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253881_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253901_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253901_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:49:54.48 +37:45:56.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253915_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253915_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253943_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253943_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:38:02.54 +39:00:05.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253947_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 253947_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 21:44:49.46 +35:31:37.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253957_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 253957_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254010_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 254010_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254017_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 254017_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254066_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 254066_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254163_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 254163_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254177_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 254177_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
**** FOUND 22:04:36.96 +38:54:15.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254181_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 254181_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254232_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 254232_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254248_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
Preparing report for the candidate 254248_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249278_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 249278_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
Rejecting candidate due to large distance (40.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 241290_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348
The candidate 241290_fd_Cyg-07-Q2b1x1_2026-05-03_04-11-27_20.00sec_-5.00C_LIGHT_0348 did not pass the final checks
Rejecting candidate due to large distance (40.5") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 160s
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 ####
21:36:44.13 +39:54:01.8
21:58:28.78 +40:10:16.7
21:40:34.76 +39:13:18.4
21:35:26.34 +41:08:46.5
21:39:48.79 +38:17:16.0
21:44:49.78 +36:36:01.4
21:35:13.87 +36:45:19.3
22:10:02.36 +38:52:02.6
22:03:06.32 +40:42:36.4
21:26:09.33 +40:15:19.0
21:59:42.09 +38:13:15.1
22:01:04.22 +40:40:18.9
21:34:27.13 +39:22:50.4
21:40:43.82 +37:22:58.5
21:57:39.32 +41:47:17.4
22:01:22.43 +40:55:07.1
21:30:08.33 +37:30:26.5
21:57:03.83 +40:57:15.8
21:40:12.53 +37:22:51.1
21:28:22.78 +38:27:06.0
22:00:14.24 +41:40:32.2
21:40:56.40 +41:13:23.4
21:48:47.13 +40:08:12.9
21:26:23.51 +38:27:58.6
22:02:06.03 +36:06:25.6
21:41:05.77 +41:56:45.8
21:34:37.59 +34:15:56.2
21:27:24.24 +33:39:57.3
21:35:58.78 +38:02:59.5
22:05:39.84 +34:53:38.7
21:51:51.67 +41:19:46.2
21:31:28.94 +38:53:29.7
21:33:13.82 +37:12:42.8
21:28:11.96 +34:45:26.5
21:28:09.28 +41:14:35.1
21:35:21.82 +38:36:52.2
21:39:01.63 +41:05:55.9
21:36:49.72 +39:45:20.1
21:59:06.34 +34:00:16.5
21:34:29.31 +39:23:38.5
21:37:46.89 +36:44:33.7
21:43:06.13 +37:12:25.7
21:40:41.02 +36:19:20.0
22:02:13.91 +41:47:06.4
21:42:12.42 +38:54:23.2
22:11:39.60 +42:09:38.3
21:49:58.87 +37:44:26.7
22:02:15.09 +34:37:07.2
21:42:04.33 +40:56:44.4
22:02:42.16 +37:08:59.4
21:40:47.55 +37:32:56.8
21:59:33.12 +37:57:30.3
21:44:26.46 +41:28:25.4
22:02:42.56 +41:44:09.0
21:47:36.48 +40:21:16.9
21:59:55.06 +41:57:02.5
21:37:18.40 +40:36:04.6
21:39:00.47 +38:41:33.4
21:59:27.59 +38:47:09.3
21:48:57.89 +37:42:52.7
21:48:12.53 +41:41:12.0
21:33:26.67 +37:43:43.1
22:01:12.76 +38:02:20.6
21:41:04.44 +37:19:15.5
21:47:23.96 +34:53:12.0
21:52:15.09 +36:58:29.9
21:46:53.96 +39:15:19.9
21:56:00.45 +37:10:54.9
21:38:19.80 +39:47:34.9
########### Completed Cyg-07-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:36:44.13 +39:54:01.8
21:58:28.78 +40:10:16.7
21:40:34.76 +39:13:18.4
21:35:26.34 +41:08:46.5
21:39:48.79 +38:17:16.0
21:44:49.78 +36:36:01.4
21:35:13.87 +36:45:19.3
22:10:02.36 +38:52:02.6
22:03:06.32 +40:42:36.4
21:26:09.33 +40:15:19.0
21:59:42.09 +38:13:15.1
22:01:04.22 +40:40:18.9
21:34:27.13 +39:22:50.4
21:40:43.82 +37:22:58.5
21:57:39.32 +41:47:17.4
22:01:22.43 +40:55:07.1
21:30:08.33 +37:30:26.5
21:57:03.83 +40:57:15.8
21:40:12.53 +37:22:51.1
21:28:22.78 +38:27:06.0
22:00:14.24 +41:40:32.2
21:40:56.40 +41:13:23.4
21:48:47.13 +40:08:12.9
21:26:23.51 +38:27:58.6
22:02:06.03 +36:06:25.6
21:41:05.77 +41:56:45.8
21:34:37.59 +34:15:56.2
21:27:24.24 +33:39:57.3
21:35:58.78 +38:02:59.5
22:05:39.84 +34:53:38.7
21:51:51.67 +41:19:46.2
21:31:28.94 +38:53:29.7
21:33:13.82 +37:12:42.8
21:28:11.96 +34:45:26.5
21:28:09.28 +41:14:35.1
21:35:21.82 +38:36:52.2
21:39:01.63 +41:05:55.9
21:36:49.72 +39:45:20.1
21:59:06.34 +34:00:16.5
21:34:29.31 +39:23:38.5
21:37:46.89 +36:44:33.7
21:43:06.13 +37:12:25.7
21:40:41.02 +36:19:20.0
22:02:13.91 +41:47:06.4
21:42:12.42 +38:54:23.2
22:11:39.60 +42:09:38.3
21:49:58.87 +37:44:26.7
22:02:15.09 +34:37:07.2
21:42:04.33 +40:56:44.4
22:02:42.16 +37:08:59.4
21:40:47.55 +37:32:56.8
21:59:33.12 +37:57:30.3
21:44:26.46 +41:28:25.4
22:02:42.56 +41:44:09.0
21:47:36.48 +40:21:16.9
21:59:55.06 +41:57:02.5
21:37:18.40 +40:36:04.6
21:39:00.47 +38:41:33.4
21:59:27.59 +38:47:09.3
21:48:57.89 +37:42:52.7
21:48:12.53 +41:41:12.0
21:33:26.67 +37:43:43.1
22:01:12.76 +38:02:20.6
21:41:04.44 +37:19:15.5
21:47:23.96 +34:53:12.0
21:52:15.09 +36:58:29.9
21:46:53.96 +39:15:19.9
21:56:00.45 +37:10:54.9
21:38:19.80 +39:47:34.9
###################################################################################
21:36:44.13 +39:54:01.8 -- not an asteroid (will add it to exclusion list)
21:58:28.78 +40:10:16.7 -- not an asteroid (will add it to exclusion list)
21:40:34.76 +39:13:18.4 -- not an asteroid (will add it to exclusion list)
21:35:26.34 +41:08:46.5 -- not an asteroid (will add it to exclusion list)
21:39:48.79 +38:17:16.0 -- not an asteroid (will add it to exclusion list)
21:44:49.78 +36:36:01.4 -- not an asteroid (will add it to exclusion list)
21:35:13.87 +36:45:19.3 -- not an asteroid (will add it to exclusion list)
22:10:02.36 +38:52:02.6 -- not an asteroid (will add it to exclusion list)
22:03:06.32 +40:42:36.4 -- not an asteroid (will add it to exclusion list)
21:26:09.33 +40:15:19.0 -- not an asteroid (will add it to exclusion list)
21:59:42.09 +38:13:15.1 -- not an asteroid (will add it to exclusion list)
22:01:04.22 +40:40:18.9 -- not an asteroid (will add it to exclusion list)
21:34:27.13 +39:22:50.4 -- not an asteroid (will add it to exclusion list)
21:40:43.82 +37:22:58.5 -- not an asteroid (will add it to exclusion list)
21:57:39.32 +41:47:17.4 -- not an asteroid (will add it to exclusion list)
22:01:22.43 +40:55:07.1 -- not an asteroid (will add it to exclusion list)
21:30:08.33 +37:30:26.5 -- not an asteroid (will add it to exclusion list)
21:57:03.83 +40:57:15.8 -- not an asteroid (will add it to exclusion list)
21:40:12.53 +37:22:51.1 -- not an asteroid (will add it to exclusion list)
21:28:22.78 +38:27:06.0 -- not an asteroid (will add it to exclusion list)
22:00:14.24 +41:40:32.2 -- not an asteroid (will add it to exclusion list)
21:40:56.40 +41:13:23.4 -- not an asteroid (will add it to exclusion list)
21:48:47.13 +40:08:12.9 -- not an asteroid (will add it to exclusion list)
21:26:23.51 +38:27:58.6 -- not an asteroid (will add it to exclusion list)
22:02:06.03 +36:06:25.6 -- not an asteroid (will add it to exclusion list)
21:41:05.77 +41:56:45.8 -- not an asteroid (will add it to exclusion list)
21:34:37.59 +34:15:56.2 -- not an asteroid (will add it to exclusion list)
21:27:24.24 +33:39:57.3 -- not an asteroid (will add it to exclusion list)
21:35:58.78 +38:02:59.5 -- not an asteroid (will add it to exclusion list)
22:05:39.84 +34:53:38.7 -- not an asteroid (will add it to exclusion list)
21:51:51.67 +41:19:46.2 -- not an asteroid (will add it to exclusion list)
21:31:28.94 +38:53:29.7 -- not an asteroid (will add it to exclusion list)
21:33:13.82 +37:12:42.8 -- not an asteroid (will add it to exclusion list)
21:28:11.96 +34:45:26.5 -- not an asteroid (will add it to exclusion list)
21:28:09.28 +41:14:35.1 -- not an asteroid (will add it to exclusion list)
21:35:21.82 +38:36:52.2 -- not an asteroid (will add it to exclusion list)
21:39:01.63 +41:05:55.9 -- not an asteroid (will add it to exclusion list)
21:36:49.72 +39:45:20.1 -- not an asteroid (will add it to exclusion list)
21:59:06.34 +34:00:16.5 -- not an asteroid (will add it to exclusion list)
21:34:29.31 +39:23:38.5 -- not an asteroid (will add it to exclusion list)
21:37:46.89 +36:44:33.7 -- not an asteroid (will add it to exclusion list)
21:43:06.13 +37:12:25.7 -- not an asteroid (will add it to exclusion list)
21:40:41.02 +36:19:20.0 -- not an asteroid (will add it to exclusion list)
22:02:13.91 +41:47:06.4 -- not an asteroid (will add it to exclusion list)
21:42:12.42 +38:54:23.2 -- not an asteroid (will add it to exclusion list)
22:11:39.60 +42:09:38.3 -- not an asteroid (will add it to exclusion list)
21:49:58.87 +37:44:26.7 -- not an asteroid (will add it to exclusion list)
22:02:15.09 +34:37:07.2 -- not an asteroid (will add it to exclusion list)
21:42:04.33 +40:56:44.4 -- not an asteroid (will add it to exclusion list)
22:02:42.16 +37:08:59.4 -- not an asteroid (will add it to exclusion list)
21:40:47.55 +37:32:56.8 -- not an asteroid (will add it to exclusion list)
21:59:33.12 +37:57:30.3 -- not an asteroid (will add it to exclusion list)
21:44:26.46 +41:28:25.4 -- not an asteroid (will add it to exclusion list)
22:02:42.56 +41:44:09.0 -- not an asteroid (will add it to exclusion list)
21:47:36.48 +40:21:16.9 -- not an asteroid (will add it to exclusion list)
21:59:55.06 +41:57:02.5 -- not an asteroid (will add it to exclusion list)
21:37:18.40 +40:36:04.6 -- not an asteroid (will add it to exclusion list)
21:39:00.47 +38:41:33.4 -- not an asteroid (will add it to exclusion list)
21:59:27.59 +38:47:09.3 -- not an asteroid (will add it to exclusion list)
21:48:57.89 +37:42:52.7 -- not an asteroid (will add it to exclusion list)
21:48:12.53 +41:41:12.0 -- not an asteroid (will add it to exclusion list)
21:33:26.67 +37:43:43.1 -- not an asteroid (will add it to exclusion list)
22:01:12.76 +38:02:20.6 -- not an asteroid (will add it to exclusion list)
21:41:04.44 +37:19:15.5 -- not an asteroid (will add it to exclusion list)
21:47:23.96 +34:53:12.0 -- not an asteroid (will add it to exclusion list)
21:52:15.09 +36:58:29.9 -- not an asteroid (will add it to exclusion list)
21:46:53.96 +39:15:19.9 -- not an asteroid (will add it to exclusion list)
21:56:00.45 +37:10:54.9 -- not an asteroid (will add it to exclusion list)
21:38:19.80 +39:47:34.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:26:09.33 +40:15:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:23.51 +38:27:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:24.24 +33:39:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:09.28 +41:14:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:11.96 +34:45:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:22.78 +38:27:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:08.33 +37:30:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:28.94 +38:53:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:13.82 +37:12:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:26.67 +37:43:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:27.13 +39:22:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:29.31 +39:23:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:37.59 +34:15:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:13.87 +36:45:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:21.82 +38:36:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:26.34 +41:08:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:58.78 +38:02:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:44.13 +39:54:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:49.72 +39:45:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:18.40 +40:36:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:46.89 +36:44:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:19.80 +39:47:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:00.47 +38:41:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:01.63 +41:05:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:48.79 +38:17:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:12.53 +37:22:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:34.76 +39:13:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:41.02 +36:19:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:43.82 +37:22:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:47.55 +37:32:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:56.40 +41:13:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:04.44 +37:19:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:05.77 +41:56:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:04.33 +40:56:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:12.42 +38:54:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:06.13 +37:12:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:26.46 +41:28:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:49.78 +36:36:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:53.96 +39:15:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:23.96 +34:53:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:36.48 +40:21:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:12.53 +41:41:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:47.13 +40:08:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:57.89 +37:42:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:58.87 +37:44:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:51.67 +41:19:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:15.09 +36:58:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:00.45 +37:10:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:03.83 +40:57:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:39.32 +41:47:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:28.78 +40:10:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:06.34 +34:00:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:27.59 +38:47:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:33.12 +37:57:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:42.09 +38:13:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:55.06 +41:57:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:14.24 +41:40:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:04.22 +40:40:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:12.76 +38:02:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:22.43 +40:55:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:06.03 +36:06:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:13.91 +41:47:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:15.09 +34:37:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.16 +37:08:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.56 +41:44:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:06.32 +40:42:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:39.84 +34:53:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:02.36 +38:52:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:39.60 +42:09:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
21:26:09.33 +40:15:19.0 -- not a known variable star
21:26:23.51 +38:27:58.6 -- not a known variable star
21:27:24.24 +33:39:57.3 -- not a known variable star
21:28:09.28 +41:14:35.1 -- not a known variable star
21:28:11.96 +34:45:26.5 -- not a known variable star
21:28:22.78 +38:27:06.0 -- not a known variable star
21:30:08.33 +37:30:26.5 -- not a known variable star
21:31:28.94 +38:53:29.7 -- a known variable star
21:33:13.82 +37:12:42.8 -- not a known variable star
21:33:26.67 +37:43:43.1 -- not a known variable star
21:34:27.13 +39:22:50.4 -- a known variable star
21:34:29.31 +39:23:38.5 -- not a known variable star
21:34:37.59 +34:15:56.2 -- not a known variable star
21:35:13.87 +36:45:19.3 -- not a known variable star
21:35:21.82 +38:36:52.2 -- not a known variable star
21:35:26.34 +41:08:46.5 -- not a known variable star
21:35:58.78 +38:02:59.5 -- not a known variable star
21:36:44.13 +39:54:01.8 -- not a known variable star
21:36:49.72 +39:45:20.1 -- not a known variable star
21:37:18.40 +40:36:04.6 -- not a known variable star
21:37:46.89 +36:44:33.7 -- a known variable star
21:38:19.80 +39:47:34.9 -- not a known variable star
21:39:00.47 +38:41:33.4 -- not a known variable star
21:39:01.63 +41:05:55.9 -- not a known variable star
21:39:48.79 +38:17:16.0 -- not a known variable star
21:40:12.53 +37:22:51.1 -- not a known variable star
21:40:34.76 +39:13:18.4 -- not a known variable star
21:40:41.02 +36:19:20.0 -- not a known variable star
21:40:43.82 +37:22:58.5 -- not a known variable star
21:40:47.55 +37:32:56.8 -- not a known variable star
21:40:56.40 +41:13:23.4 -- not a known variable star
21:41:04.44 +37:19:15.5 -- not a known variable star
21:41:05.77 +41:56:45.8 -- a known variable star
21:42:04.33 +40:56:44.4 -- not a known variable star
21:42:12.42 +38:54:23.2 -- a known variable star
21:43:06.13 +37:12:25.7 -- not a known variable star
21:44:26.46 +41:28:25.4 -- not a known variable star
21:44:49.78 +36:36:01.4 -- not a known variable star
21:46:53.96 +39:15:19.9 -- not a known variable star
21:47:23.96 +34:53:12.0 -- not a known variable star
21:47:36.48 +40:21:16.9 -- not a known variable star
21:48:12.53 +41:41:12.0 -- not a known variable star
21:48:47.13 +40:08:12.9 -- not a known variable star
21:48:57.89 +37:42:52.7 -- not a known variable star
21:49:58.87 +37:44:26.7 -- not a known variable star
21:51:51.67 +41:19:46.2 -- not a known variable star
21:52:15.09 +36:58:29.9 -- not a known variable star
21:56:00.45 +37:10:54.9 -- not a known variable star
21:57:03.83 +40:57:15.8 -- not a known variable star
21:57:39.32 +41:47:17.4 -- not a known variable star
21:58:28.78 +40:10:16.7 -- not a known variable star
21:59:06.34 +34:00:16.5 -- not a known variable star
21:59:27.59 +38:47:09.3 -- not a known variable star
21:59:33.12 +37:57:30.3 -- not a known variable star
21:59:42.09 +38:13:15.1 -- not a known variable star
21:59:55.06 +41:57:02.5 -- a known variable star
22:00:14.24 +41:40:32.2 -- not a known variable star
22:01:04.22 +40:40:18.9 -- not a known variable star
22:01:12.76 +38:02:20.6 -- not a known variable star
22:01:22.43 +40:55:07.1 -- not a known variable star
22:02:06.03 +36:06:25.6 -- a known variable star
22:02:13.91 +41:47:06.4 -- not a known variable star
22:02:15.09 +34:37:07.2 -- not a known variable star
22:02:42.16 +37:08:59.4 -- not a known variable star
22:02:42.56 +41:44:09.0 -- not a known variable star
22:03:06.32 +40:42:36.4 -- not a known variable star
22:05:39.84 +34:53:38.7 -- a known variable star
22:10:02.36 +38:52:02.6 -- not a known variable star
22:11:39.60 +42:09:38.3 -- not a known variable star
Found 61 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
69 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 69 (excluding asteroids and hot pixels, 61 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)2461163.88244405 -observatory V36
01:54:29.47 +09:58:46.4 Mercury (-1.0mag)
04:36:15.18 +23:03:06.9 Venus (-3.9mag)
01:07:05.77 +06:11:19.8 Mars (1.2mag)
07:22:00.88 +22:29:37.6 Jupiter (-2.0mag)
00:36:39.76 +01:34:55.9 Saturn (0.9mag)
03:51:34.87 +19:59:42.3 Uranus (5.8mag)
00:12:58.72 -00:02:02.3 Neptune (7.8mag)
20:34:13.13 -22:54:29.7 Pluto (14.5mag)
15:49:38.75 -25:59:45.7 Moon (-12.2mag)
-rw-r--r-- 1 apache apache 363 May 3 04:14 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461163.88244405:
07:21:54.13 +22:29:53.6 Io (5.9mag)
07:21:56.11 +22:29:51.3 Europa (6.0mag)
07:21:42.67 +22:30:19.7 Ganymede (5.4mag)
07:22:34.40 +22:28:19.8 Callisto (6.7mag)
07:24:27.90 +22:10:27.1 Himalia (15.4mag)
07:22:04.99 +22:29:28.3 Thebe (16.3mag)
07:24:54.87 +22:39:25.4 Elara (17.4mag)
07:22:03.74 +23:00:31.2 Pasiphae (17.5mag)
07:29:53.94 +22:29:02.9 Carme (18.6mag)
00:36:35.25 +01:35:24.5 Titan (8.7mag)
00:36:36.24 +01:35:08.3 Rhea (10.0mag)
00:36:13.78 +01:32:55.4 Iapetus (11.5mag)
00:36:55.05 +01:34:50.4 Hyperion (14.8mag)
00:38:01.38 +01:41:42.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 3 04:14 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461163.88244405:
16:38:22.51 -26:06:56.4 JWST
18:05:35.77 +33:21:52.3 Chandra
19:49:02.48 +13:58:03.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 3 04:14 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461163.88244405 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
06:43:58.24 +29:12:23.0 17.8mag P/2009 WX51 (Catalina)
18:55:53.53 -29:54:44.8 13.8mag P/2010 H2 (Vales)
05:20:22.02 -68:55:41.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:36:55.01 +31:34:28.0 17.3mag C/2017 K2 (PANSTARRS)
17:27:17.98 +12:29:56.4 17.7mag C/2021 G2 (ATLAS)
23:13:45.35 +29:59:07.2 17.1mag C/2022 E2 (ATLAS)
04:49:58.93 +26:28:00.1 16.2mag C/2022 N2 (PANSTARRS)
09:08:58.34 +31:57:28.8 16.4mag C/2022 QE78 (ATLAS)
08:35:07.68 +01:31:24.1 17.5mag C/2022 R6 (PANSTARRS)
18:48:00.74 +19:53:34.5 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:34:08.89 -11:16:13.6 17.5mag P/2023 B1 (PANSTARRS)
09:01:46.53 -09:19:11.7 17.8mag C/2023 F3 (ATLAS)
22:08:21.50 +64:01:55.1 17.6mag C/2023 H5 (Lemmon)
18:59:11.09 -04:12:09.6 13.9mag C/2023 R1 (PANSTARRS)
19:14:12.07 +88:08:37.4 17.9mag C/2023 X2 (Lemmon)
06:29:34.93 +63:32:49.6 17.3mag C/2024 A1 (ATLAS)
05:47:39.45 +22:52:16.8 12.1mag C/2024 E1 (Wierzchos)
16:06:42.53 +09:08:51.6 17.3mag C/2024 G6 (ATLAS)
20:23:35.00 +20:13:27.2 14.4mag C/2024 J3 (ATLAS)
03:42:33.92 -19:54:42.6 16.2mag C/2024 T5 (ATLAS)
05:32:12.98 +41:18:21.2 17.8mag C/2025 J1 (Borisov)
12:33:53.38 +52:10:29.1 16.0mag C/2025 L1 (ATLAS)
03:54:54.80 -29:13:10.5 18.0mag C/2025 Q3 (ATLAS)
04:26:55.30 -02:32:35.6 8.8mag C/2025 R3 (PANSTARRS)
12:47:06.71 +03:56:03.0 17.3mag C/2025 Y1 (ATLAS)
05:00:54.12 +01:38:23.7 16.8mag C/2026 A1 (MAPS)
00:45:31.39 +39:55:22.3 15.1mag C/2026 B2 (Sun-Gao)
19:16:31.45 -08:47:12.5 10.8mag 10P/Tempel
14:37:31.64 +01:00:20.4 15.6mag 24P/Schaumasse
10:59:33.92 -01:04:22.7 15.8mag 29P/Schwassmann-Wachmann
10:40:01.17 -03:01:34.5 17.3mag 43P/Wolf-Harrington
02:15:44.86 +20:21:43.8 17.4mag 47P/Ashbrook-Jackson
07:44:39.29 +33:06:04.4 16.9mag 63P/Wild
23:50:16.09 -09:28:49.7 15.7mag 65P/Gunn
04:51:56.92 +26:37:52.7 16.1mag 76P/West-Kohoutek-Ikemura
01:44:42.41 +11:32:20.6 14.1mag 78P/Gehrels
23:52:58.82 -04:18:05.4 14.9mag 88P/Howell
03:01:26.17 +24:53:10.8 15.0mag 93P/Lovas
05:29:34.24 +33:02:09.3 16.0mag 123P/West-Hartley
08:51:46.26 +30:24:36.3 16.3mag 124P/Mrkos
03:00:35.38 +16:12:56.4 16.4mag 128P/Shoemaker-Holt
03:21:56.90 +16:25:44.1 17.6mag 131P/Mueller
02:59:57.18 +17:56:57.9 10.8mag 141P/Machholz
03:05:43.14 +11:00:03.6 10.8mag 141P-A/Machholz
01:45:49.69 +06:50:05.6 11.0mag 141P-D/Machholz
01:51:37.84 +07:14:55.1 14.9mag 162P/SidingSpring
22:23:55.80 -07:25:35.9 18.0mag 218P/LINEAR
17:15:43.02 -11:47:56.4 16.1mag 235P/LINEAR
06:13:01.11 +35:39:08.2 17.0mag 240P/NEAT
07:48:43.40 -03:30:54.4 17.9mag 242P/Spahr
23:00:31.79 -15:52:32.6 17.4mag 260P/McNaught
02:35:25.32 +24:44:43.9 17.8mag 295P/LINEAR
15:34:25.31 +07:56:13.0 17.4mag 391P/Kowalski
07:42:28.29 +21:19:56.4 17.7mag 450P/LONEOS
06:02:15.18 +44:00:43.1 17.6mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K May 3 04:14 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
21:00:10.71 -32:17:03.90 2026-04-27.36 16.15
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
21:00:10.71 -32:17:03.90 2026-04-27.36 16.15
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 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
-rw-r--r-- 1 apache apache 5.8K May 3 04:14 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
-rw-r--r-- 1 apache apache 188K May 3 04:14 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:10:53.458 +45:56:52.48 SN 2026knu 2026-04-20.18 19.5784
13:23:31.702 -27:27:16.87 AT 2026knt 2026-04-21.45 19.6
14:59:13.174 -10:47:02.79 AT 2026kns 2026-04-09.59 20.1
14:45:20.668 -24:47:31.93 AT 2026knr 2026-03-24.65 20.36
11:45:24.981 +14:40:44.45 AT 2026knq 2026-04-13.92 20.18
04:52:30.865 -15:17:09.10 AT 2026knp 2026-04-20.71 18.098
17:25:02.776 +69:43:35.23 AT 2026kno 2026-04-23.10 19.208
15:15:42.943 -39:27:45.41 AT 2026knn 2026-04-14.63 19.62
21:02:34.025 +19:12:44.83 AT 2026knm 2026-04-22.60 18.74
14:38:36.298 -39:37:27.88 AT 2026knl 2026-04-21.52 20.1
13:24:43.943 +16:55:43.96 AT 2026knk 2026-04-20.96 20.03
13:55:11.417 +21:19:35.16 AT 2026knj 2026-04-20.98 19.3
16:21:58.180 +07:39:22.34 AT 2026kni 2026-04-22.11 19.97
18:25:00.619 +56:31:13.17 AT 2026knh 2026-04-14.18 19.89
11:52:14.846 +19:25:04.67 AT 2026kng 2026-04-12.92 20.24
17:52:14.690 -78:03:43.36 AT 2026kne 2026-04-23.29 18.712
19:46:54.481 -51:39:39.32 AT 2026knd 2026-04-20.32 17.94
21:24:26.061 +26:56:11.62 AT 2026knc 2026-04-23.59 17.66
11:18:30.556 -08:06:31.77 AT 2026knb 2026-04-22.86 19.129
14:56:59.281 +45:09:43.33 AT 2026kna 2026-04-23.01 19.329
-rw-r--r-- 1 apache apache 30K May 3 04:14 tns_transients_list.txt
