This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f
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 09 13.4477 2461296.9477 12.38 22:01:35.33 +34:24:57.9
87.42282 -16.49395 galactic Peg Second-epoch detections are separated by 2.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:01:35.33 +34:24:57.9 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.032 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:01:35.33 +34:24:57.9: 13.35 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:01:35.33 +34:24:57.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461296.9477,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260913.4477 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.63 21:46:03.53 +37:01:48.6
86.66596 -12.46579 galactic Cyg Second-epoch detections are separated by 0.7" and 8.3 pix
The object was found in VSX 2" NSVS J2146034+370146
Type: SR
# Max. Min./Amp. JD0 Period
15.741 g Y 0.772 g 2458370.15740 204.083788500000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:46:03.53 +37:01:48.6: 14.16 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:46:03.53 +37:01:48.6: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 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
NSVS J2146034+370146,2461296.9477,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2146034+370146 20260913.4477 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.49 22:00:41.17 +34:31:04.8
87.33852 -16.29783 galactic Peg Second-epoch detections are separated by 3.6" and 8.8 pix
The object was found in VSX 0" Gaia DR3 1948016746780196864
Type: ROT
# Max. Min./Amp. JD0 Period
13.460 G 13.480 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:00:41.17 +34:31:04.8: 13.72 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:00:41.17 +34:31:04.8: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 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
Gaia DR3 1948016746780196864,2461296.9477,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948016746780196864 20260913.4477 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.51 21:39:53.49 +37:57:31.9
86.36563 -10.95836 galactic Cyg Second-epoch detections are separated by 1.7" and 8.1 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 1953494582430244864 | 21:39:56.02 +37:57:18.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.774+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:39:53.49 +37:57:31.9: 13.58 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:39:53.49 +37:57:31.9: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953494582430244864,2461296.9477,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953494582430244864 20260913.4477 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.38 21:58:28.30 +33:47:21.6
86.48806 -16.57254 galactic Peg Second-epoch detections are separated by 1.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:28.30 +33:47:21.6 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.029 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:58:28.30 +33:47:21.6: 13.50 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:58:28.30 +33:47:21.6: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461296.9477,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260913.4477 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.43 21:43:26.47 +39:54:00.6
88.20498 -9.97165 galactic Cyg Second-epoch detections are separated by 2.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.8607+39.9108 | 21:43:26.47 +39:54:00.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:43:26.47 +39:54:00.6: 13.42 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:43:26.47 +39:54:00.6: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.8607+39.9108,2461296.9477,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.8607+39.9108 20260913.4477 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.36 21:58:23.22 +33:51:16.4
86.51719 -16.51103 galactic Peg Second-epoch detections are separated by 3.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:23.22 +33:51:16.4 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:58:23.22 +33:51:16.4: 13.42 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:58:23.22 +33:51:16.4: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461296.9477,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260913.4477 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.43 21:40:35.26 +37:34:38.0
86.20809 -11.33344 galactic Cyg Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1589+37.5689 | 21:40:35.26 +37:34:38.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.158+/-0.032 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:40:35.26 +37:34:38.0: 13.43 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:40:35.26 +37:34:38.0: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1589+37.5689,2461296.9477,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1589+37.5689 20260913.4477 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.29 21:39:26.94 +37:59:19.1
86.32035 -10.87764 galactic Cyg Second-epoch detections are separated by 0.6" and 8.3 pix
The object was found in VSX 1" ASASSN-V J213926.90+375918.9
Type: L
# Max. Min./Amp. JD0 Period
13.520 V 13.780 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:39:26.94 +37:59:19.1: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:39:26.94 +37:59:19.1: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 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 J213926.90+375918.9,2461296.9477,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213926.90+375918.9 20260913.4477 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.39 21:56:32.82 +33:57:55.8
86.28476 -16.18194 galactic Peg Second-epoch detections are separated by 0.7" and 8.3 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 | 21:56:32.82 +33:57:55.8 (user input) | T | P | (position from user input) SpType: K7 1985ApJS...59..197B LTT 16409
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:56:32.82 +33:57:55.8: 13.42 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:56:32.82 +33:57:55.8: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461296.9477,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260913.4477 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.38 21:56:50.59 +33:55:50.8
86.31075 -16.24793 galactic Peg Second-epoch detections are separated by 2.7" and 8.3 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 1947928133014753664 | 21:56:48.84 +33:55:18.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.379+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:56:50.59 +33:55:50.8: 13.36 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:56:50.59 +33:55:50.8: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 1947928133014753664,2461296.9477,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947928133014753664 20260913.4477 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.31 21:54:17.91 +33:56:02.5
85.89223 -15.90605 galactic Peg Second-epoch detections are separated by 1.8" and 8.6 pix
The object was found in VSX25" Gaia DR3 1948104329753070848
Type: ROT
# Max. Min./Amp. JD0 Period
17.950 G 18.180 G 1.013390000000
ATTENTION: measured mag 12.31 is 5.6 mag brighter than the VSX record maximum brightness 17.95 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:54:17.91 +33:56:02.5: 13.35 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:54:17.91 +33:56:02.5: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 1948104329753070848,2461296.9477,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948104329753070848 20260913.4477 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.27 21:44:20.17 +39:44:12.1
88.22657 -10.20788 galactic Cyg Second-epoch detections are separated by 2.8" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:20.17 +39:44:12.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:44:20.17 +39:44:12.1: 13.34 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:44:20.17 +39:44:12.1: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461296.9477,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260913.4477 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.03 21:44:03.99 +39:45:06.3
88.19705 -10.16239 galactic Cyg Second-epoch detections are separated by 2.0" and 8.4 pix
The object was found in VSX 2" ASASSN-V J214404.17+394506.6
Type: SR
# Max. Min./Amp. JD0 Period
14.420 g Y 0.210 g 2458715.96600 43.900000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:44:03.99 +39:45:06.3: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:44:03.99 +39:45:06.3: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214404.17+394506.6,2461296.9477,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214404.17+394506.6 20260913.4477 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.35 21:57:21.74 +33:47:05.2
86.29983 -16.42911 galactic Peg Second-epoch detections are separated by 2.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:21.74 +33:47:05.2 (user input) | T | P | (position from user input) J-Ks=0.662+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:57:21.74 +33:47:05.2: 13.28 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:57:21.74 +33:47:05.2: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461296.9477,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260913.4477 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.11 22:00:04.84 +35:01:03.3
87.56483 -15.83119 galactic Peg Second-epoch detections are separated by 3.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:04.84 +35:01:03.3 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:00:04.84 +35:01:03.3: 13.22 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:00:04.84 +35:01:03.3: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461296.9477,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260913.4477 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 11.99 21:28:45.00 +40:30:20.4
86.53366 -7.62505 galactic Cyg Second-epoch detections are separated by 1.8" and 8.6 pix
The object was found in VSX 3" Gaia DR3 1966957174600987008
Type: L
# Max. Min./Amp. JD0 Period
11.770 G 11.910 G M
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:28:45.00 +40:30:20.4: 13.20 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:28:45.00 +40:30:20.4: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 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
Gaia DR3 1966957174600987008,2461296.9477,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966957174600987008 20260913.4477 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.21 21:42:51.70 +39:58:11.8
88.16728 -9.84583 galactic Cyg Second-epoch detections are separated by 1.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1954297913108215936 | 21:42:51.67 +39:58:11.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: M2 (LAMOST DR5) J-Ks=1.250+/-0.037 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:42:51.70 +39:58:11.8: 13.21 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:42:51.70 +39:58:11.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1954297913108215936,2461296.9477,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1954297913108215936 20260913.4477 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.12 21:30:48.90 +40:13:35.4
86.62503 -8.09882 galactic Cyg Second-epoch detections are separated by 1.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.7043+40.2271 | 21:30:49.02 +40:13:37.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M1 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:30:48.90 +40:13:35.4: 13.22 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:30:48.90 +40:13:35.4: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.7043+40.2271,2461296.9477,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.7043+40.2271 20260913.4477 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.26 21:42:24.67 +40:19:07.0
88.33617 -9.52761 galactic Cyg Second-epoch detections are separated by 3.6" and 8.8 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 | 21:42:24.67 +40:19:07.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.810+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:42:24.67 +40:19:07.0: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:42:24.67 +40:19:07.0: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461296.9477,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260913.4477 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.15 21:56:56.98 +33:44:11.6
86.19893 -16.41133 galactic Peg Second-epoch detections are separated by 1.2" and 8.1 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 | 21:56:56.98 +33:44:11.6 (user input) | T | P | (position from user input) J-Ks=0.746+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:56:56.98 +33:44:11.6: 13.18 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:56:56.98 +33:44:11.6: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461296.9477,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260913.4477 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.13 22:01:05.78 +34:25:18.6
87.34410 -16.42576 galactic Peg Second-epoch detections are separated by 1.9" and 8.2 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 | Large-amplitude variable Gaia DR2 1948012142572174592 | 22:01:05.78 +34:25:18.6 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.253+/-0.036 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:01:05.78 +34:25:18.6: 13.10 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:01:05.78 +34:25:18.6: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 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
Large-amplitude variable Gaia DR2 1948012142572174592,2461296.9477,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1948012142572174592 20260913.4477 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.07 22:01:13.52 +34:20:27.8
87.31282 -16.50535 galactic Peg Second-epoch detections are separated by 3.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.3106+34.3530 | 22:01:13.52 +34:20:27.8 (user input) | CBF (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.721+/-0.023 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:01:13.52 +34:20:27.8: 13.09 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:01:13.52 +34:20:27.8: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 J330.3106+34.3530,2461296.9477,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.3106+34.3530 20260913.4477 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 11.99 22:00:53.35 +34:51:56.5
87.59968 -16.05346 galactic Peg Second-epoch detections are separated by 1.2" and 8.4 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 | 22:00:53.35 +34:51:56.5 (user input) | T | P | (position from user input) J-Ks=0.690+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:00:53.35 +34:51:56.5: 13.06 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:00:53.35 +34:51:56.5: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461296.9477,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260913.4477 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.04 21:43:13.58 +39:43:47.6
88.05922 -10.07210 galactic Cyg Second-epoch detections are separated by 1.1" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.8113+39.7358 | 21:43:13.57 +39:43:46.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.171+/-0.032 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:43:13.58 +39:43:47.6: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:43:13.58 +39:43:47.6: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.8113+39.7358,2461296.9477,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.8113+39.7358 20260913.4477 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.07 21:32:21.62 +39:26:57.8
86.30112 -8.86645 galactic Cyg Second-epoch detections are separated by 1.3" and 8.5 pix
The object was found in VSX 1" ASASSN-V J213221.53+392658.6
Type: SR
# Max. Min./Amp. JD0 Period
14.170 g Y 0.280 g 2459377.90400 59.460000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:32:21.62 +39:26:57.8: 13.02 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:32:21.62 +39:26:57.8: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 J213221.53+392658.6,2461296.9477,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213221.53+392658.6 20260913.4477 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 12.06 21:58:37.05 +33:56:27.2
86.61294 -16.47481 galactic Peg Second-epoch detections are separated by 0.5" and 8.4 pix
The object was found in VSX15" Gaia DR3 1947972353997813376
Type: VAR
# Max. Min./Amp. JD0 Period
13.610 G 13.650 G 0.023918200000 A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:58:37.05 +33:56:27.2: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:58:37.05 +33:56:27.2: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 1947972353997813376,2461296.9477,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947972353997813376 20260913.4477 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 11.87 21:34:33.03 +41:49:56.0
88.25300 -7.41140 galactic Cyg Second-epoch detections are separated by 2.5" and 8.3 pix
The object was found in VSX 3" ASASSN-V J213432.98+414959.0
Type: SR
# Max. Min./Amp. JD0 Period
12.920 V 13.050 V 2458344.00000 308.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:34:33.03 +41:49:56.0: 12.80 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:34:33.03 +41:49:56.0: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 J213432.98+414959.0,2461296.9477,11.87,0.05,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
ASASSN-V J213432.98+414959.0 20260913.4477 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 09 13.4477 2461296.9477 11.90 21:59:27.66 +33:46:08.5
86.64038 -16.71876 galactic Peg Second-epoch detections are separated by 1.4" and 8.1 pix
The object was found in VSX 0" Gaia DR3 1947957819828599424
Type: ROT
# Max. Min./Amp. JD0 Period
12.560 G 12.590 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:59:27.66 +33:46:08.5: 12.80 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:59:27.66 +33:46:08.5: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 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 1947957819828599424,2461296.9477,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947957819828599424 20260913.4477 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 11.54 21:29:06.81 +40:44:11.5
86.74539 -7.50671 galactic Cyg Second-epoch detections are separated by 1.4" and 8.2 pix
The object was found in VSX 3" ASASSN-V J212906.70+404414.4
Type: L:
# Max. Min./Amp. JD0 Period
13.410 V 13.670 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:29:06.81 +40:44:11.5: 12.68 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:29:06.81 +40:44:11.5: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J212906.70+404414.4,2461296.9477,11.54,0.05,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
ASASSN-V J212906.70+404414.4 20260913.4477 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 09 13.4477 2461296.9477 11.61 21:59:35.58 +34:25:54.9
87.09979 -16.22270 galactic Peg Second-epoch detections are separated by 2.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.8984+34.4354 | 21:59:35.41 +34:25:53.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:59:35.58 +34:25:54.9: 12.48 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:59:35.58 +34:25:54.9: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 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
ATO J329.8984+34.4354,2461296.9477,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.8984+34.4354 20260913.4477 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 10.93 21:28:59.96 +41:13:10.8
87.06747 -7.14361 galactic Cyg Second-epoch detections are separated by 1.3" and 8.4 pix
The object was found in VSX 3" ASASSN-V J212859.78+411313.6
Type: L
# Max. Min./Amp. JD0 Period
12.710 V 13.500 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:28:59.96 +41:13:10.8: 11.98 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:28:59.96 +41:13:10.8: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J212859.78+411313.6,2461296.9477,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212859.78+411313.6 20260913.4477 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 13.4477 2461296.9477 10.89 21:46:05.42 +35:25:30.8
85.58173 -13.67430 galactic Cyg Second-epoch detections are separated by 1.0" and 8.5 pix
The object was found in VSX 4" NSVS J2146052+352528
Type: L:
# Max. Min./Amp. JD0 Period
9.634 R1 Y 0.413 R1 381.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:46:05.42 +35:25:30.8: 11.94 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:46:05.42 +35:25:30.8: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2146052+352528,2461296.9477,10.89,0.05,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
NSVS J2146052+352528 20260913.4477 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 09 13.4477 2461296.9477 10.97 21:43:57.06 +39:42:28.1
88.15064 -10.18076 galactic Cyg Second-epoch detections are separated by 1.1" and 8.3 pix
The object was found in VSX 1" ASASSN-V J214357.01+394228.6
Type: SR
# Max. Min./Amp. JD0 Period
12.180 V 12.650 V 2457285.70000 301.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:43:57.06 +39:42:28.1: 11.95 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:43:57.06 +39:42:28.1: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214357.01+394228.6,2461296.9477,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214357.01+394228.6 20260913.4477 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461235.92515677 14.07.2026 10:12:03.545 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
First image: 2461235.92515677 14.07.2026 10:12:03.545 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
Last image: 2461296.94800727 13.09.2026 10:44:57.828 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.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.: -7.37
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: 3 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 14891
Objects passed selection criteria: 14793
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 11995
Average stars matched: 9328.25 (77.7678 %)
Memory usage VmPeak: 247816 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 13 05:47:33 CDT 2026
Host name: tau
############################################################
ERROR: large change in astrometric-star counts between the two new images (q1: 213 -> 112, 47.418% > 20%; fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits vs fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits) - possible passing clouds or a bad plate solution; continuing processing
ERROR: large change in astrometric-star counts between the two new images (q4: 116 -> 149, 22.148% > 20%; fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits vs fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits) - possible passing clouds or a bad plate solution; continuing processing
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461235.92515677 14.07.2026 10:12:03.545 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
First image: 2461235.92515677 14.07.2026 10:12:03.545 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
Last image: 2461296.94800727 13.09.2026 10:44:57.828 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 123
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.00
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: 16 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 116979
Objects passed selection criteria: 116438
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 89928.2
Average stars matched: 73198.8 (81.3968 %)
Memory usage VmPeak: 627172 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 13 05:48:25 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.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_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.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: 2461296.94736677
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits exists and is non-empty
wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits (1st reference image)
verification OK: wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:04.814 +37:58:28.80 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits (1st new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
Image size: 937.6'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:48:50.230 +38:00:16.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:49:04.814 +37:58:28.80
Second-epoch image center 21:48:50.230 +38:00:16.51
Angular distance between the image centers 0.0565 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits (2nd new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
Image size: 937.7'x624.0' 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: 21:48:52.459 +37:59:35.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:49:04.814 +37:58:28.80
Second-epoch image center 21:48:52.459 +37:59:35.65
Angular distance between the image centers 0.0446 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 21:48:50.230 +38:00:16.51
Second-epoch second image center 21:48:52.459 +37:59:35.65
Angular distance between the image centers 0.01350 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits &> /tmp/tmp.TCmzwHfdEf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits &> /tmp/tmp.ISCe107C6D
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits &> /tmp/tmp.mMqGeZsrhS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits &> /tmp/tmp.k9K4rAjttw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.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_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits and wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits and wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat
Found non-empty wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits and wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat
The reference image (wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits) and catalog (wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat) found
'wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat' -> 'wcsmag.cat'
Read 29926 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.6609 to 337.8861 deg, Dec +32.4066 to +43.2386 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 316.6609 to 337.8861 deg, Dec 32.4066 to 43.2386 deg
Loaded 20755 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): 14769 out of 16083 total matches.
Matched with Tycho-2 16083 out of 29926 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.697200
a=0.000000 b=1.000000 c=22.697200
From vast_summary.log: estimated ref. image limiting mag.: -7.37
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29926 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.6609 to 337.8861 deg, Dec +32.4066 to +43.2386 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 316.6609 to 337.8861 deg, Dec 32.4066 to 43.2386 deg
Loaded 20755 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): 14769 out of 16083 total matches.
Matched with Tycho-2 16083 out of 29926 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits (aperture=6.2)
Read 31154 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.6168 to 337.8794 deg, Dec +32.4112 to +43.2590 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 316.6168 to 337.8794 deg, Dec 32.4112 to 43.2590 deg
Loaded 20833 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): 14708 out of 16188 total matches.
Matched with Tycho-2 16188 out of 31154 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits (aperture=6.1)
____ 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: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
2.2 pix Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
2.5 pix fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
2.6 pix fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
Limiting magnitude estimates:
15.3 mag. Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
15.4 mag. Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
12.5 mag. fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
12.4 mag. fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 10.3 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.TCmzwHfdEf (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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.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_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits' -> 'wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.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_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2765, bad_region=9311, passed=29926
Got 29926 stars (including 18740 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat
util/solve_plate_with_UCAC5 got 29926 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 4911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 22389 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 22389 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 22389 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4911 stars left (next iteration limit 5402)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits N_match=4911 sigma_overall_arcsec=0.478 sigma_q1_arcsec=0.408 sigma_q2_arcsec=0.540 sigma_q3_arcsec=0.493 sigma_q4_arcsec=0.460 n_q1=1608 n_q2=1102 n_q3=1317 n_q4=884 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits -region wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ISCe107C6D (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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.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_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits' -> 'wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.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_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3100, bad_region=5683, passed=31154
Got 31154 stars (including 22686 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat
util/solve_plate_with_UCAC5 got 31154 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 4916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 26640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 26640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 26640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4916 stars left (next iteration limit 5407)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits N_match=4916 sigma_overall_arcsec=0.482 sigma_q1_arcsec=0.442 sigma_q2_arcsec=0.441 sigma_q3_arcsec=0.536 sigma_q4_arcsec=0.490 n_q1=1629 n_q2=726 n_q3=1680 n_q4=881 worst_quadrant_to_overall_ratio=1.114
The image catalog is written to wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits -region wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.mMqGeZsrhS (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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.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_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=38, bad_region=93, passed=1233
Got 1233 stars (including 1104 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat
util/solve_plate_with_UCAC5 got 1233 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 613 to 667 (Dec 32.6 to 43.2)
Done reading UCAC5 zone files...
Matched 1083 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1077 matched stars entering correct_measured_positions(), 1054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1077 matched stars entering correct_measured_positions(), 1148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 613 to 667 (Dec 32.6 to 43.2)
Done reading UCAC5 zone files...
Matched 1084 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1075 matched stars entering correct_measured_positions(), 1149 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Accuracy estimation diagnostic: 1075 matched stars entering correct_measured_positions(), 1149 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 1075 stars left (next iteration limit 1184)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1075 robust_rms=6.569 arcsec worst_quadrant_rms=7.865 arcsec
SIP_REFIT: SIP order 3 trial: matched=1075 robust_rms=0.651 arcsec worst_quadrant_rms=0.703 arcsec
SIP_REFIT: SIP order 5 trial: matched=1075 robust_rms=0.605 arcsec worst_quadrant_rms=0.698 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=1075 robust_rms_before=0.839 arcsec robust_rms_before_corrected=0.771 arcsec robust_rms_after=0.651 arcsec worst_quadrant_rms_before=0.895 worst_quadrant_rms_after=0.703
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
Image size: 937.6'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:48:50.245 +38:00:16.36 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1233 stars ###
'wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/correct_sextractor_wcs_catalog_usingxy2sky2615748.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 0.839 -> 0.651 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.3 arcsec, 1075 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 613 to 667 (Dec 32.6 to 43.2)
Done reading UCAC5 zone files...
Matched 1031 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 1031 pairs (1075 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=1031 robust_rms=6.480 arcsec worst_quadrant_rms=7.734 arcsec
SIP_REFIT: SIP order 3 trial: matched=1031 robust_rms=0.635 arcsec worst_quadrant_rms=0.691 arcsec
SIP_REFIT: SIP order 5 trial: matched=1031 robust_rms=0.607 arcsec worst_quadrant_rms=0.672 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=1031 robust_rms_before=0.643 arcsec robust_rms_before_corrected=0.643 arcsec robust_rms_after=0.635 arcsec worst_quadrant_rms_before=0.690 worst_quadrant_rms_after=0.691
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.691 vs 0.690 arcsec) - keeping the current solution
SIP_REFIT: the second refit on the re-matched pairs was not applied - keeping the first refit solution
Accuracy estimation diagnostic: 1031 matched stars entering correct_measured_positions(), 1147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 1031 matched stars entering correct_measured_positions(), 1144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits N_match=1031 sigma_overall_arcsec=0.656 sigma_q1_arcsec=0.731 sigma_q2_arcsec=0.684 sigma_q3_arcsec=0.615 sigma_q4_arcsec=0.483 n_q1=213 n_q2=432 n_q3=270 n_q4=116 worst_quadrant_to_overall_ratio=1.114
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.k9K4rAjttw (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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.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_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=29, bad_region=76, passed=1182
Got 1182 stars (including 1082 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat
util/solve_plate_with_UCAC5 got 1182 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 667 (Dec 32.6 to 43.1)
Done reading UCAC5 zone files...
Matched 1062 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1053 matched stars entering correct_measured_positions(), 1022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1053 matched stars entering correct_measured_positions(), 1110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 667 (Dec 32.6 to 43.1)
Done reading UCAC5 zone files...
Matched 1063 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1053 matched stars entering correct_measured_positions(), 1110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 1053 matched stars entering correct_measured_positions(), 1110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 1053 stars left (next iteration limit 1158)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1053 robust_rms=5.660 arcsec worst_quadrant_rms=8.926 arcsec
SIP_REFIT: SIP order 3 trial: matched=1053 robust_rms=0.668 arcsec worst_quadrant_rms=0.803 arcsec
SIP_REFIT: SIP order 5 trial: matched=1053 robust_rms=0.626 arcsec worst_quadrant_rms=0.794 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=1053 robust_rms_before=0.839 arcsec robust_rms_before_corrected=0.725 arcsec robust_rms_after=0.668 arcsec worst_quadrant_rms_before=0.849 worst_quadrant_rms_after=0.803
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.849 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits N_match=1053 sigma_overall_arcsec=0.716 sigma_q1_arcsec=0.972 sigma_q2_arcsec=0.790 sigma_q3_arcsec=0.628 sigma_q4_arcsec=0.576 n_q1=112 n_q2=495 n_q3=297 n_q4=149 worst_quadrant_to_overall_ratio=1.358
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits'
Saving the final (post-refit) wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits'
Saving the final (post-refit) wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits'
Saving the final (post-refit) wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits sigma_overall=0.478 worst_q_ratio=1.130
ref2=Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits sigma_overall=0.482 worst_q_ratio=1.114
new1=fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits sigma_overall=0.656 worst_q_ratio=1.114
new2=fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits sigma_overall=0.716 worst_q_ratio=1.358
reference average sigma_overall=0.48 worst_q_ratio=1.122
warn-on-ratio threshold: 2.0x reference
###################################
ERROR: large change in astrometric-star counts between the two new images (q1: 213 -> 112, 47.418% > 20%; fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits vs fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits) - possible passing clouds or a bad plate solution; continuing processing
ERROR: large change in astrometric-star counts between the two new images (q4: 116 -> 149, 22.148% > 20%; fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits vs fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits) - possible passing clouds or a bad plate solution; continuing processing
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356_astrometric_residuals.png (4911 matched stars from wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898_astrometric_residuals.png (4916 matched stars from wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234_astrometric_residuals.png (1031 matched stars from wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235_astrometric_residuals.png (1053 matched stars from wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.64 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.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_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
Creating symlink local_wcs_cache/wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
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_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits exists and is non-empty
wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits (1st reference image)
verification OK: wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:04.814 +37:58:28.80 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits (1st new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
Image size: 937.6'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:48:50.245 +38:00:16.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:49:04.814 +37:58:28.80
Second-epoch image center 21:48:50.245 +38:00:16.36
Angular distance between the image centers 0.0564 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits (2nd new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
Image size: 937.7'x624.0' 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: 21:48:52.459 +37:59:35.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:49:04.814 +37:58:28.80
Second-epoch image center 21:48:52.459 +37:59:35.65
Angular distance between the image centers 0.0446 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 21:48:50.245 +38:00:16.36
Second-epoch second image center 21:48:52.459 +37:59:35.65
Angular distance between the image centers 0.01344 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits &> /tmp/tmp.ayNiXsFoD7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits &> /tmp/tmp.tD5DkSFLxk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits &> /tmp/tmp.ocnY0YLCnw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits &> /tmp/tmp.W5YwTb7hlN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.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_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits and wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits and wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat
Found non-empty wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits and wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat
The reference image (wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits) and catalog (wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat) found
'wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat' -> 'wcsmag.cat'
Read 207262 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.6493 to 337.9473 deg, Dec +32.3714 to +43.2400 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 316.6493 to 337.9473 deg, Dec 32.3714 to 43.2400 deg
Loaded 20889 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): 11570 out of 16460 total matches.
Matched with Tycho-2 16460 out of 207262 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.543900
a=0.000000 b=1.000000 c=22.543900
From vast_summary.log: estimated ref. image limiting mag.: -7.00
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.54
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.54
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 207262 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.6493 to 337.9473 deg, Dec +32.3714 to +43.2400 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 316.6493 to 337.9473 deg, Dec 32.3714 to 43.2400 deg
Loaded 20889 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): 11570 out of 16460 total matches.
Matched with Tycho-2 16460 out of 207262 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits (aperture=4.6)
Read 211259 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.5936 to 337.8847 deg, Dec +32.3867 to +43.2595 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 316.5936 to 337.8847 deg, Dec 32.3867 to 43.2595 deg
Loaded 20922 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): 11493 out of 16483 total matches.
Matched with Tycho-2 16483 out of 211259 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
2.1 pix Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
2.4 pix fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
2.5 pix fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
Limiting magnitude estimates:
15.5 mag. Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
15.5 mag. Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
12.8 mag. fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
13.0 mag. fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 12.4 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ayNiXsFoD7 (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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.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_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits' -> 'wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.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_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=64, blended=29591, bad_region=49553, passed=207198
Got 207198 stars (including 136079 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat
util/solve_plate_with_UCAC5 got 207198 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 4942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 4927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 169291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 4942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 169291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 169291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4927 stars left (next iteration limit 5419)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits N_match=4927 sigma_overall_arcsec=0.451 sigma_q1_arcsec=0.398 sigma_q2_arcsec=0.512 sigma_q3_arcsec=0.492 sigma_q4_arcsec=0.432 n_q1=1667 n_q2=1044 n_q3=1373 n_q4=843 worst_quadrant_to_overall_ratio=1.133
The image catalog is written to wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits -region wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.tD5DkSFLxk (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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.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_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits' -> 'wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.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_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=56, blended=30224, bad_region=29297, passed=211203
Got 211203 stars (including 154540 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat
util/solve_plate_with_UCAC5 got 211203 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4926 matched stars entering correct_measured_positions(), 4926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4926 matched stars entering correct_measured_positions(), 189374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4926 matched stars entering correct_measured_positions(), 189374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4926 matched stars entering correct_measured_positions(), 189374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4926 stars left (next iteration limit 5418)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits N_match=4926 sigma_overall_arcsec=0.465 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.423 sigma_q3_arcsec=0.542 sigma_q4_arcsec=0.461 n_q1=1610 n_q2=813 n_q3=1569 n_q4=934 worst_quadrant_to_overall_ratio=1.167
The image catalog is written to wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits -region wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ocnY0YLCnw (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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.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_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=491, bad_region=777, passed=12187
Got 12187 stars (including 10973 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat
util/solve_plate_with_UCAC5 got 12187 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.6 to 43.2)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 4876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 11649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.6 to 43.2)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 11649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 11649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Excluding outliers - 4880 stars left (next iteration limit 5369)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4880 robust_rms=6.599 arcsec worst_quadrant_rms=7.225 arcsec
SIP_REFIT: SIP order 3 trial: matched=4880 robust_rms=0.857 arcsec worst_quadrant_rms=1.022 arcsec
SIP_REFIT: SIP order 5 trial: matched=4880 robust_rms=0.839 arcsec worst_quadrant_rms=1.027 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4880 robust_rms_before=0.867 arcsec robust_rms_before_corrected=0.876 arcsec robust_rms_after=0.857 arcsec worst_quadrant_rms_before=1.043 worst_quadrant_rms_after=1.022
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.043 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits N_match=4880 sigma_overall_arcsec=0.848 sigma_q1_arcsec=0.904 sigma_q2_arcsec=1.014 sigma_q3_arcsec=0.719 sigma_q4_arcsec=0.711 n_q1=1109 n_q2=1828 n_q3=1355 n_q4=588 worst_quadrant_to_overall_ratio=1.196
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.W5YwTb7hlN (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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.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_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=478, bad_region=599, passed=11121
Got 11121 stars (including 10104 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat
util/solve_plate_with_UCAC5 got 11121 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.2)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 4851 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 10778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.2)
Done reading UCAC5 zone files...
Matched 4907 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 10778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 10778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
Excluding outliers - 4857 stars left (next iteration limit 5342)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4857 robust_rms=6.086 arcsec worst_quadrant_rms=7.710 arcsec
SIP_REFIT: SIP order 3 trial: matched=4857 robust_rms=0.898 arcsec worst_quadrant_rms=1.095 arcsec
SIP_REFIT: SIP order 5 trial: matched=4857 robust_rms=0.884 arcsec worst_quadrant_rms=1.095 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4857 robust_rms_before=1.062 arcsec robust_rms_before_corrected=0.931 arcsec robust_rms_after=0.898 arcsec worst_quadrant_rms_before=1.098 worst_quadrant_rms_after=1.095
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.098 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits N_match=4857 sigma_overall_arcsec=0.900 sigma_q1_arcsec=0.941 sigma_q2_arcsec=1.094 sigma_q3_arcsec=0.766 sigma_q4_arcsec=0.818 n_q1=612 n_q2=2033 n_q3=1489 n_q4=723 worst_quadrant_to_overall_ratio=1.216
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-02_20.00sec_-0.00C_LIGHT_0234.fits
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.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_2026-09-13_CI_Cyg-07-Q2b1x1_054538_TTUQ2b1x1_2604796_xkI1cy1f/wcs_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235.fits
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:46:03.53 +37:01:48.6: 14.16 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:58:28.30 +33:47:21.6: 13.50 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:40:35.26 +37:34:38.0: 13.43 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:39:53.49 +37:57:31.9: 13.58 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:01:35.33 +34:24:57.9: 13.35 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:43:26.47 +39:54:00.6: 13.42 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:00:41.17 +34:31:04.8: 13.72 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:58:23.22 +33:51:16.4: 13.42 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:39:26.94 +37:59:19.1: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:56:32.82 +33:57:55.8: 13.42 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:58:28.30 +33:47:21.6: 13.49 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:46:03.53 +37:01:48.6: 13.99 +/- 0.05 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:43:26.47 +39:54:00.6: 13.54 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:40:35.26 +37:34:38.0: 13.41 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:39:53.49 +37:57:31.9: 13.65 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:58:23.22 +33:51:16.4: 13.31 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:00:41.17 +34:31:04.8: 13.70 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:01:35.33 +34:24:57.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.04
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 21:58:28.30 +33:47:21.6: ref_mag=13.49 +/- 0.02 new_mean_mag=12.3747 delta=1.12 (need > 0.90)
Forced photometry filter KEPT candidate at 21:46:03.53 +37:01:48.6: ref_mag=14.06 +/- 0.04 new_mean_mag=12.6309 delta=1.42 (need > 0.90)
Forced photometry filter KEPT candidate at 21:58:23.22 +33:51:16.4: ref_mag=13.35 +/- 0.02 new_mean_mag=12.3331 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 22:00:41.17 +34:31:04.8: ref_mag=13.71 +/- 0.03 new_mean_mag=12.4942 delta=1.21 (need > 0.90)
Forced photometry filter KEPT candidate at 21:40:35.26 +37:34:38.0: ref_mag=13.42 +/- 0.02 new_mean_mag=12.4297 delta=0.99 (need > 0.90)
Forced photometry filter KEPT candidate at 21:39:53.49 +37:57:31.9: ref_mag=13.61 +/- 0.03 new_mean_mag=12.5055 delta=1.11 (need > 0.90)
Forced photometry filter KEPT candidate at 21:43:26.47 +39:54:00.6: ref_mag=13.47 +/- 0.02 new_mean_mag=12.4283 delta=1.04 (need > 0.90)
Forced photometry filter KEPT candidate at 22:01:35.33 +34:24:57.9: ref_mag=13.32 +/- 0.02 new_mean_mag=12.3721 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:56:32.82 +33:57:55.8: 13.38 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:39:26.94 +37:59:19.1: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 21:39:26.94 +37:59:19.1: ref_mag=13.36 +/- 0.02 new_mean_mag=12.2920 delta=1.07 (need > 0.90)
Forced photometry filter KEPT candidate at 21:56:32.82 +33:57:55.8: ref_mag=13.39 +/- 0.02 new_mean_mag=12.3945 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:56:50.59 +33:55:50.8: 13.36 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:54:17.91 +33:56:02.5: 13.35 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:56:50.59 +33:55:50.8: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 21:56:50.59 +33:55:50.8: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3762 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:54:17.91 +33:56:02.5: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry filter KEPT candidate at 21:54:17.91 +33:56:02.5: ref_mag=13.35 +/- 0.02 new_mean_mag=12.3126 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:44:20.17 +39:44:12.1: 13.34 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:44:20.17 +39:44:12.1: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 21:44:20.17 +39:44:12.1: ref_mag=13.33 +/- 0.02 new_mean_mag=12.2814 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:44:03.99 +39:45:06.3: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:44:03.99 +39:45:06.3: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 21:44:03.99 +39:45:06.3: ref_mag=13.26 +/- 0.02 new_mean_mag=12.0290 delta=1.23 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:57:21.74 +33:47:05.2: 13.28 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:57:21.74 +33:47:05.2: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 21:57:21.74 +33:47:05.2: ref_mag=13.23 +/- 0.02 new_mean_mag=12.2222 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:00:04.84 +35:01:03.3: 13.22 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:00:04.84 +35:01:03.3: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 22:00:04.84 +35:01:03.3: ref_mag=13.12 +/- 0.02 new_mean_mag=12.1230 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:28:45.00 +40:30:20.4: 13.20 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:28:45.00 +40:30:20.4: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 21:28:45.00 +40:30:20.4: ref_mag=13.24 +/- 0.02 new_mean_mag=11.9937 delta=1.25 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:42:51.70 +39:58:11.8: 13.21 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:42:51.70 +39:58:11.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 21:42:51.70 +39:58:11.8: ref_mag=13.26 +/- 0.02 new_mean_mag=12.2133 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:30:48.90 +40:13:35.4: 13.22 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:42:24.67 +40:19:07.0: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:56:56.98 +33:44:11.6: 13.18 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:01:05.78 +34:25:18.6: 13.10 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:30:48.90 +40:13:35.4: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 21:30:48.90 +40:13:35.4: ref_mag=13.26 +/- 0.02 new_mean_mag=12.1125 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:42:24.67 +40:19:07.0: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 21:42:24.67 +40:19:07.0: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1946 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:56:56.98 +33:44:11.6: 13.11 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:01:05.78 +34:25:18.6: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 21:56:56.98 +33:44:11.6: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1419 delta=1.00 (need > 0.90)
Forced photometry filter KEPT candidate at 22:01:05.78 +34:25:18.6: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1189 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:01:13.52 +34:20:27.8: 13.09 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:01:13.52 +34:20:27.8: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 22:01:13.52 +34:20:27.8: ref_mag=13.05 +/- 0.02 new_mean_mag=12.0535 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:59:26.67 +33:50:03.2: 13.08 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:59:26.67 +33:50:03.2: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter REJECTED candidate at 21:59:26.67 +33:50:03.2: ref_mag=12.99 +/- 0.01 new_mean_mag=12.1084 delta=0.88 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:00:53.35 +34:51:56.5: 13.06 +/- 0.03 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:00:53.35 +34:51:56.5: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 22:00:53.35 +34:51:56.5: ref_mag=13.03 +/- 0.02 new_mean_mag=11.9767 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:43:13.58 +39:43:47.6: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:43:13.58 +39:43:47.6: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 21:43:13.58 +39:43:47.6: ref_mag=13.04 +/- 0.02 new_mean_mag=12.0405 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:32:21.62 +39:26:57.8: 13.02 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:32:21.62 +39:26:57.8: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 21:32:21.62 +39:26:57.8: ref_mag=13.11 +/- 0.02 new_mean_mag=12.0567 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:58:37.05 +33:56:27.2: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:58:37.05 +33:56:27.2: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter KEPT candidate at 21:58:37.05 +33:56:27.2: ref_mag=12.97 +/- 0.02 new_mean_mag=12.0601 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:34:33.03 +41:49:56.0: 12.80 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:59:27.66 +33:46:08.5: 12.80 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:34:33.03 +41:49:56.0: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter KEPT candidate at 21:34:33.03 +41:49:56.0: ref_mag=12.85 +/- 0.02 new_mean_mag=11.8595 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:59:27.66 +33:46:08.5: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 21:59:27.66 +33:46:08.5: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8671 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:29:06.81 +40:44:11.5: 12.68 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:59:35.58 +34:25:54.9: 12.48 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 22:00:50.97 +34:24:00.0: 12.17 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:29:06.81 +40:44:11.5: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 21:29:06.81 +40:44:11.5: ref_mag=12.77 +/- 0.01 new_mean_mag=11.5336 delta=1.23 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:59:35.58 +34:25:54.9: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 21:59:35.58 +34:25:54.9: ref_mag=12.52 +/- 0.01 new_mean_mag=11.5978 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 22:00:50.97 +34:24:00.0: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter REJECTED candidate at 22:00:50.97 +34:24:00.0: ref_mag=12.17 +/- 0.01 new_mean_mag=11.2866 delta=0.88 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:28:59.96 +41:13:10.8: 11.98 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:46:05.42 +35:25:30.8: 11.94 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:28:59.96 +41:13:10.8: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter KEPT candidate at 21:28:59.96 +41:13:10.8: ref_mag=12.06 +/- 0.01 new_mean_mag=10.9325 delta=1.13 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-14_05-12-03_20.00sec_5.00C_LIGHT_0356.fits at 21:43:57.06 +39:42:28.1: 11.95 +/- 0.01 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:46:05.42 +35:25:30.8: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter KEPT candidate at 21:46:05.42 +35:25:30.8: ref_mag=11.92 +/- 0.01 new_mean_mag=10.8587 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-07-21_03-32-25_20.00sec_5.00C_LIGHT_0898.fits at 21:43:57.06 +39:42:28.1: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Forced photometry filter KEPT candidate at 21:43:57.06 +39:42:28.1: ref_mag=11.95 +/- 0.01 new_mean_mag=10.9724 delta=0.97 (need > 0.90)
Adding exclusion_list_local.txt__out110050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76684.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 29s
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: 14s
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Considering the candidate 284068_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
The candidate 284068_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235 did not pass the final checks
**** FOUND 22:01:54.14 +36:57:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284095_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
The candidate 284095_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235 did not pass the final checks
**** FOUND 21:32:50.37 +39:22:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177502_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 177502_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
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Considering the candidate 131104_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 131104_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
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Considering the candidate 179428_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 179428_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
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Considering the candidate 110815_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 110815_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
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Considering the candidate 167331_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 167331_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
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Considering the candidate 68107_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 68107_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
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Considering the candidate 168228_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 168228_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
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Considering the candidate 119058_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 119058_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
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Considering the candidate 110050_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 110050_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
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Considering the candidate 169789_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 169789_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
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Considering the candidate 169066_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 169066_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
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Considering the candidate 169456_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 169456_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71625_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 71625_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71309_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 71309_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166916_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 166916_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187876_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 187876_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54150_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 54150_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66640_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 66640_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59941_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 59941_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59551_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 59551_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166023_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 166023_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178332_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 178332_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176433_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 176433_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168248_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
The candidate 168248_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185658_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 185658_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71720_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 71720_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76684_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 76684_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60943_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
The candidate 60943_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235 did not pass the final checks
**** FOUND 21:45:41.31 +40:17:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169651_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 169651_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27263_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 27263_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167994_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 167994_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139611_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
The candidate 139611_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235 did not pass the final checks
**** FOUND 21:42:03.22 +36:37:54.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74275_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
The candidate 74275_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235 did not pass the final checks
**** FOUND 21:43:34.53 +39:38:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95810_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
The candidate 95810_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235 did not pass the final checks
**** FOUND 21:37:35.94 +38:38:22.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49397_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 49397_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178883_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 178883_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177709_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
The candidate 177709_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39848_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 39848_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194690_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 194690_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72754_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
Preparing report for the candidate 72754_fd_Cyg-07-Q2b1x1_2026-09-13_05-44-57_20.00sec_-0.00C_LIGHT_0235
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 45s
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 ####
21:39:26.94 +37:59:19.1
21:39:53.49 +37:57:31.9
21:40:35.26 +37:34:38.0
21:46:03.53 +37:01:48.6
21:56:56.98 +33:44:11.6
21:57:21.74 +33:47:05.2
21:58:28.30 +33:47:21.6
21:59:27.66 +33:46:08.5
21:58:23.22 +33:51:16.4
21:56:50.59 +33:55:50.8
21:54:17.91 +33:56:02.5
21:58:37.05 +33:56:27.2
21:56:32.82 +33:57:55.8
22:01:13.52 +34:20:27.8
22:01:35.33 +34:24:57.9
22:01:05.78 +34:25:18.6
21:59:35.58 +34:25:54.9
22:00:41.17 +34:31:04.8
22:00:53.35 +34:51:56.5
22:00:04.84 +35:01:03.3
21:46:05.42 +35:25:30.8
21:34:33.03 +41:49:56.0
21:28:59.96 +41:13:10.8
21:29:06.81 +40:44:11.5
21:28:45.00 +40:30:20.4
21:42:24.67 +40:19:07.0
21:30:48.90 +40:13:35.4
21:42:51.70 +39:58:11.8
21:43:26.47 +39:54:00.6
21:44:03.99 +39:45:06.3
21:44:20.17 +39:44:12.1
21:43:13.58 +39:43:47.6
21:43:57.06 +39:42:28.1
21:32:21.62 +39:26:57.8
########### 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 ####
22:01:35.33 +34:24:57.9
21:46:03.53 +37:01:48.6
22:00:41.17 +34:31:04.8
21:39:53.49 +37:57:31.9
21:58:28.30 +33:47:21.6
21:43:26.47 +39:54:00.6
21:58:23.22 +33:51:16.4
21:40:35.26 +37:34:38.0
21:39:26.94 +37:59:19.1
21:56:32.82 +33:57:55.8
21:56:50.59 +33:55:50.8
21:54:17.91 +33:56:02.5
21:44:20.17 +39:44:12.1
21:44:03.99 +39:45:06.3
21:57:21.74 +33:47:05.2
22:00:04.84 +35:01:03.3
21:28:45.00 +40:30:20.4
21:42:51.70 +39:58:11.8
21:30:48.90 +40:13:35.4
21:42:24.67 +40:19:07.0
21:56:56.98 +33:44:11.6
22:01:05.78 +34:25:18.6
22:01:13.52 +34:20:27.8
22:00:53.35 +34:51:56.5
21:43:13.58 +39:43:47.6
21:32:21.62 +39:26:57.8
21:58:37.05 +33:56:27.2
21:34:33.03 +41:49:56.0
21:59:27.66 +33:46:08.5
21:29:06.81 +40:44:11.5
21:59:35.58 +34:25:54.9
21:28:59.96 +41:13:10.8
21:46:05.42 +35:25:30.8
21:43:57.06 +39:42:28.1
###################################################################################
22:01:35.33 +34:24:57.9 -- not an asteroid (will add it to exclusion list)
21:46:03.53 +37:01:48.6 -- not an asteroid (will add it to exclusion list)
22:00:41.17 +34:31:04.8 -- not an asteroid (will add it to exclusion list)
21:39:53.49 +37:57:31.9 -- not an asteroid (will add it to exclusion list)
21:58:28.30 +33:47:21.6 -- not an asteroid (will add it to exclusion list)
21:43:26.47 +39:54:00.6 -- not an asteroid (will add it to exclusion list)
21:58:23.22 +33:51:16.4 -- not an asteroid (will add it to exclusion list)
21:40:35.26 +37:34:38.0 -- not an asteroid (will add it to exclusion list)
21:39:26.94 +37:59:19.1 -- not an asteroid (will add it to exclusion list)
21:56:32.82 +33:57:55.8 -- not an asteroid (will add it to exclusion list)
21:56:50.59 +33:55:50.8 -- not an asteroid (will add it to exclusion list)
21:54:17.91 +33:56:02.5 -- not an asteroid (will add it to exclusion list)
21:44:20.17 +39:44:12.1 -- not an asteroid (will add it to exclusion list)
21:44:03.99 +39:45:06.3 -- not an asteroid (will add it to exclusion list)
21:57:21.74 +33:47:05.2 -- not an asteroid (will add it to exclusion list)
22:00:04.84 +35:01:03.3 -- not an asteroid (will add it to exclusion list)
21:28:45.00 +40:30:20.4 -- not an asteroid (will add it to exclusion list)
21:42:51.70 +39:58:11.8 -- not an asteroid (will add it to exclusion list)
21:30:48.90 +40:13:35.4 -- not an asteroid (will add it to exclusion list)
21:42:24.67 +40:19:07.0 -- not an asteroid (will add it to exclusion list)
21:56:56.98 +33:44:11.6 -- not an asteroid (will add it to exclusion list)
22:01:05.78 +34:25:18.6 -- not an asteroid (will add it to exclusion list)
22:01:13.52 +34:20:27.8 -- not an asteroid (will add it to exclusion list)
22:00:53.35 +34:51:56.5 -- not an asteroid (will add it to exclusion list)
21:43:13.58 +39:43:47.6 -- not an asteroid (will add it to exclusion list)
21:32:21.62 +39:26:57.8 -- not an asteroid (will add it to exclusion list)
21:58:37.05 +33:56:27.2 -- not an asteroid (will add it to exclusion list)
21:34:33.03 +41:49:56.0 -- not an asteroid (will add it to exclusion list)
21:59:27.66 +33:46:08.5 -- not an asteroid (will add it to exclusion list)
21:29:06.81 +40:44:11.5 -- not an asteroid (will add it to exclusion list)
21:59:35.58 +34:25:54.9 -- not an asteroid (will add it to exclusion list)
21:28:59.96 +41:13:10.8 -- not an asteroid (will add it to exclusion list)
21:46:05.42 +35:25:30.8 -- not an asteroid (will add it to exclusion list)
21:43:57.06 +39:42:28.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:28:45.00 +40:30:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:59.96 +41:13:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:06.81 +40:44:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:48.90 +40:13:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:21.62 +39:26:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:33.03 +41:49:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:26.94 +37:59:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:53.49 +37:57:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:35.26 +37:34:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:24.67 +40:19:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:51.70 +39:58:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:13.58 +39:43:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:26.47 +39:54:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:57.06 +39:42:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:03.99 +39:45:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:20.17 +39:44:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:03.53 +37:01:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:05.42 +35:25:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:17.91 +33:56:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:32.82 +33:57:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:50.59 +33:55:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:56.98 +33:44:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:21.74 +33:47:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:23.22 +33:51:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:28.30 +33:47:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:37.05 +33:56:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:27.66 +33:46:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:35.58 +34:25:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:04.84 +35:01:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:41.17 +34:31:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:53.35 +34:51:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:05.78 +34:25:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:13.52 +34:20:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:35.33 +34:24:57.9 -- 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)
21:28:45.00 +40:30:20.4 -- a known variable star
21:28:59.96 +41:13:10.8 -- a known variable star
21:29:06.81 +40:44:11.5 -- a known variable star
21:30:48.90 +40:13:35.4 -- not a known variable star
21:32:21.62 +39:26:57.8 -- a known variable star
21:34:33.03 +41:49:56.0 -- a known variable star
21:39:26.94 +37:59:19.1 -- a known variable star
21:39:53.49 +37:57:31.9 -- not a known variable star
21:40:35.26 +37:34:38.0 -- not a known variable star
21:42:24.67 +40:19:07.0 -- not a known variable star
21:42:51.70 +39:58:11.8 -- not a known variable star
21:43:13.58 +39:43:47.6 -- not a known variable star
21:43:26.47 +39:54:00.6 -- not a known variable star
21:43:57.06 +39:42:28.1 -- a known variable star
21:44:03.99 +39:45:06.3 -- a known variable star
21:44:20.17 +39:44:12.1 -- not a known variable star
21:46:03.53 +37:01:48.6 -- a known variable star
21:46:05.42 +35:25:30.8 -- a known variable star
21:54:17.91 +33:56:02.5 -- a known variable star
21:56:32.82 +33:57:55.8 -- not a known variable star
21:56:50.59 +33:55:50.8 -- not a known variable star
21:56:56.98 +33:44:11.6 -- not a known variable star
21:57:21.74 +33:47:05.2 -- not a known variable star
21:58:23.22 +33:51:16.4 -- not a known variable star
21:58:28.30 +33:47:21.6 -- not a known variable star
21:58:37.05 +33:56:27.2 -- a known variable star
21:59:27.66 +33:46:08.5 -- a known variable star
21:59:35.58 +34:25:54.9 -- not a known variable star
22:00:04.84 +35:01:03.3 -- not a known variable star
22:00:41.17 +34:31:04.8 -- a known variable star
22:00:53.35 +34:51:56.5 -- not a known variable star
22:01:05.78 +34:25:18.6 -- not a known variable star
22:01:13.52 +34:20:27.8 -- not a known variable star
22:01:35.33 +34:24:57.9 -- not a known variable star
Found 20 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
34 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
21:28:45.00 +40:30:20.4
21:28:59.96 +41:13:10.8
21:29:06.81 +40:44:11.5
21:30:48.90 +40:13:35.4
21:32:21.62 +39:26:57.8
21:34:33.03 +41:49:56.0
21:39:26.94 +37:59:19.1
21:39:53.49 +37:57:31.9
21:40:35.26 +37:34:38.0
21:42:24.67 +40:19:07.0
21:42:51.70 +39:58:11.8
21:43:13.58 +39:43:47.6
21:43:26.47 +39:54:00.6
21:43:57.06 +39:42:28.1
21:44:03.99 +39:45:06.3
21:44:20.17 +39:44:12.1
21:46:03.53 +37:01:48.6
21:46:05.42 +35:25:30.8
21:54:17.91 +33:56:02.5
21:56:32.82 +33:57:55.8
21:56:50.59 +33:55:50.8
21:56:56.98 +33:44:11.6
21:57:21.74 +33:47:05.2
21:58:23.22 +33:51:16.4
21:58:28.30 +33:47:21.6
21:58:37.05 +33:56:27.2
21:59:27.66 +33:46:08.5
21:59:35.58 +34:25:54.9
22:00:04.84 +35:01:03.3
22:00:41.17 +34:31:04.8
22:00:53.35 +34:51:56.5
22:01:05.78 +34:25:18.6
22:01:13.52 +34:20:27.8
22:01:35.33 +34:24:57.9
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The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461296.94736677 -observatory V36
12:16:13.04 -01:17:33.8 Mercury (-0.5mag)
13:50:26.17 -16:42:43.5 Venus (-4.8mag)
07:30:25.64 +22:32:40.6 Mars (1.2mag)
09:14:02.68 +16:36:14.1 Jupiter (-1.8mag)
00:50:14.75 +02:28:13.4 Saturn (0.4mag)
04:13:41.82 +21:02:01.4 Uranus (5.7mag)
00:13:09.17 -00:07:13.0 Neptune (7.7mag)
20:25:11.72 -23:40:54.5 Pluto (14.5mag)
13:05:16.20 -11:26:46.0 Moon (-8.8mag)
-rw-r--r-- 1 apache apache 362 Sep 13 05:47 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461296.94736677:
09:14:00.61 +16:36:25.8 Io (6.0mag)
09:14:12.76 +16:35:24.1 Europa (6.2mag)
09:14:19.56 +16:34:48.8 Ganymede (5.6mag)
09:14:28.73 +16:34:05.1 Callisto (6.8mag)
09:12:03.09 +16:55:13.8 Himalia (15.7mag)
09:14:06.24 +16:35:57.7 Thebe (16.5mag)
09:11:35.59 +16:49:09.0 Elara (17.7mag)
09:17:46.46 +16:02:06.5 Pasiphae (17.9mag)
09:14:40.91 +16:55:42.8 Carme (18.9mag)
00:50:07.90 +02:27:44.9 Titan (8.3mag)
00:50:18.48 +02:27:55.4 Rhea (9.6mag)
00:50:12.43 +02:29:57.9 Iapetus (11.0mag)
00:50:19.16 +02:28:31.7 Hyperion (14.3mag)
00:48:55.31 +02:17:25.0 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 13 05:47 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461296.94736677:
22:54:29.07 +07:11:46.8 JWST
19:31:19.88 -08:34:02.6 Chandra
12:59:34.24 -62:20:41.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 13 05:47 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461296.94736677 -observatory V36
03:43:39.26 +19:36:11.3 17.3mag P/1996 R2 (Lagerkvist)
18:05:24.90 -34:05:40.5 14.4mag P/2010 H2 (Vales)
07:23:58.90 -70:39:00.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:16:17.22 +33:51:44.3 17.7mag C/2017 K2 (PANSTARRS)
22:08:41.60 +27:53:42.3 17.5mag C/2022 E2 (ATLAS)
07:14:41.89 +25:51:58.8 16.9mag C/2022 N2 (PANSTARRS)
10:55:08.84 +27:00:49.5 17.1mag C/2022 QE78 (ATLAS)
09:52:32.14 +05:11:54.6 18.0mag C/2022 R6 (PANSTARRS)
15:28:10.28 -16:11:14.9 14.9mag C/2023 R1 (PANSTARRS)
08:43:36.68 +33:17:18.2 15.9mag C/2024 E1 (Wierzchos)
15:07:30.60 +15:15:14.5 17.9mag C/2024 G6 (ATLAS)
18:30:11.89 +42:54:59.1 13.7mag C/2024 J3 (ATLAS)
20:18:02.09 +48:55:15.5 17.4mag C/2024 R4 (PANSTARRS)
05:38:40.56 -13:07:05.6 15.0mag C/2024 T5 (ATLAS)
07:13:31.11 +17:17:41.3 17.8mag C/2025 J1 (Borisov)
11:28:00.65 +18:17:02.8 16.7mag C/2025 V2 (Rankin)
13:24:47.84 -00:23:03.4 16.8mag C/2025 Y1 (ATLAS)
16:58:43.93 +72:57:28.4 16.0mag C/2026 A2 (Bok)
03:02:17.36 +45:53:49.4 17.5mag C/2026 B2 (Sun-Gao)
12:19:00.39 +11:47:08.9 17.6mag A/2026 E1
22:31:09.03 -35:14:26.3 13.6mag 10P/Tempel
01:29:04.62 +38:10:51.2 17.7mag 11P/Tempel-Swift-LINEAR
11:52:18.52 -05:56:07.5 16.3mag 29P/Schwassmann-Wachmann
12:20:57.36 -07:01:41.6 17.7mag 63P/Wild
06:50:58.70 +18:45:30.4 17.1mag 78P/Gehrels
03:17:00.81 +15:02:26.7 17.2mag 88P/Howell
05:58:56.99 +30:57:13.0 16.8mag 112P/Urata-Niijima
07:49:46.13 +23:10:24.2 15.8mag 114P/Wiseman-Skiff
10:41:32.52 +19:32:52.0 14.8mag 123P/West-Hartley
13:00:17.01 -23:27:20.4 17.5mag 124P/Mrkos
06:24:39.55 +20:26:17.0 15.9mag 128P/Shoemaker-Holt
02:03:27.89 -16:36:33.7 14.8mag 161P/Hartley-IRAS
09:10:08.99 +37:17:49.4 16.5mag 162P/Siding Spring
09:31:41.47 +10:22:05.0 13.4mag 169P/NEAT
03:28:53.39 +07:55:26.2 14.5mag 220P/McNaught
05:04:19.08 +38:11:09.8 15.3mag 260P/McNaught
08:48:07.04 +35:01:04.6 17.3mag 295P/LINEAR
15:29:22.85 -00:56:10.4 17.9mag 391P/Kowalski
09:33:02.77 +16:32:15.1 17.8mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.0K Sep 13 05:47 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
04:59:14.53 -83:27:58.80 ASASSN-26fd 2026-09-9.11 17.27
17:52:06.79 -23:43:20.70 ASASSN-26fc 2026-09-8.79 12.14
03:52:53.26 -14:19:28.70 SN 2026zfw 2026-09-8 17.78
01:53:26.46 +10:07:25.10 SN2026aacj 2026-09-7.17 16.27
20:04:34.47 +62:38:38.10 SN2026zji 2026-09-7.14 15.87
22:37:05.64 +34:24:35.00 SN2026aaiv 2026-09-7.25 13.48
22:24:21.29 -10:25:31.60 ASASSN-26fb 2026-09-5.3 13.93
00:44:54.28 +41:33:10.50 AT2026aabo 2026-09-3.29 15.02
00:52:12.40 -58:22:08.60 SN 2026zhl 2026-08-31.92 16.51
19:53:57.87 +61:00:19.70 ASASSN-26fa 2026-08-31.18 14.63
00:21:50.96 -09:29:16.30 AT2026zwp 2026-08-31.41 15.59
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
-rw-r--r-- 1 apache apache 5.7K Sep 13 05:47 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
00:42:12.76 +41:16:28.4 PNV J00421276+4116284 2026-09-10.9176 18.67Cmag
17:52:06.80 -23:43:20.7 TCP J17520680-2343207 2026-09-08.7896 12.6mag
-rw-r--r-- 1 apache apache 190K Sep 13 05:47 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:36:33.680 -54:17:06.96 AT 2026zht 2026-08-19.84 18.206
02:34:40.939 +11:29:01.73 AT 2026zhs 2026-08-16.18 20.38
00:06:27.710 -42:59:59.51 AT 2026zhr 2026-08-13.97 17.978
22:15:35.625 -80:38:43.32 AT 2026zhq 2026-08-20.04 18.351
17:58:22.424 -86:55:56.22 AT 2026zhp 2026-08-16.83 19.182
01:43:25.365 -80:23:54.49 AT 2026zho 2026-08-14.07 18.558
23:16:01.325 -41:57:55.14 AT 2026zhn 2026-08-20.17 18.943
23:07:30.879 -67:00:48.59 AT 2026zhm 2026-08-20.07 18.916
00:52:12.375 -58:22:08.73 SN 2026zhl 2026-08-20.13 17.801
00:39:52.355 +03:55:55.21 AT 2026zhk 2026-08-07.32 17.8794
23:48:06.315 +08:48:24.68 AT 2026zhj 2026-08-12.44 20.7977
03:11:32.085 -07:13:41.59 AT 2026zhi 2026-08-07.75 19.73
03:47:50.700 -13:23:38.20 AT 2026zhh 2026-08-07.76 20.24
03:34:14.398 -29:40:47.85 AT 2026zhg 2026-08-19.79 20.11
02:19:14.333 -35:57:34.60 AT 2026zhf 2026-08-06.74 19.89
03:22:56.866 -13:06:39.74 SN 2026zhe 2026-08-15.81 19.92
04:00:32.743 -08:48:10.25 AT 2026zhd 2026-08-18.80 19.31
02:16:11.122 -35:21:41.09 AT 2026zhc 2026-08-19.77 19.78
02:13:56.802 -25:48:46.13 AT 2026zhb 2026-08-18.76 19.66
03:52:53.306 -14:19:29.84 SN 2026zha 2026-08-18.78 18.94
-rw-r--r-- 1 apache apache 89K Sep 13 05:47 tns_transients_list.txt
