This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc
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 06 10.1709 2461201.6709 12.70 21:20:44.88 +54:21:22.7
95.27882 3.21448 galactic Cyg Second-epoch detections are separated by 4.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:20:44.88 +54:21:22.7 (user input) | T | P | (position from user input) J-Ks=0.976+/-0.025 (M)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:20:44.88 +54:21:22.7: 13.71 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:20:44.88 +54:21:22.7: 13.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461201.6709,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260610.1709 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.38 21:40:44.39 +55:43:50.7
98.31003 2.25742 galactic Cep Second-epoch detections are separated by 1.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1847+55.7315 | 21:40:44.39 +55:43:50.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:44.39 +55:43:50.7: 13.33 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:44.39 +55:43:50.7: 13.31 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1847+55.7315,2461201.6709,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1847+55.7315 20260610.1709 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 06 10.1709 2461201.6709 11.89 21:41:36.77 +56:01:48.4
98.59931 2.40252 galactic Cep Second-epoch detections are separated by 0.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4014+56.0264 | 21:41:36.77 +56:01:48.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.443+/-0.030 (G)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:36.77 +56:01:48.4: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:36.77 +56:01:48.4: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 J325.4014+56.0264,2461201.6709,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.4014+56.0264 20260610.1709 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.40 21:41:47.46 +56:20:41.8
98.82480 2.62385 galactic Cep Second-epoch detections are separated by 2.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2178089378792877696 | 21:41:47.63 +56:20:42.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.483+/-0.037 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:47.46 +56:20:41.8: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:47.46 +56:20:41.8: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 2178089378792877696,2461201.6709,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2178089378792877696 20260610.1709 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 11.96 21:41:33.31 +56:07:56.5
98.66041 2.48494 galactic Cep Second-epoch detections are separated by 0.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2175061117611542912 | 21:41:33.48 +56:07:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.633+/-0.044 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:33.31 +56:07:56.5: 12.90 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:33.31 +56:07:56.5: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 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 2175061117611542912,2461201.6709,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2175061117611542912 20260610.1709 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.15 21:39:07.47 +55:41:15.1
98.11051 2.37528 galactic Cep Second-epoch detections are separated by 1.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2174670486054033920 | 21:39:07.47 +55:41:15.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.359+/-0.032 (G)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:07.47 +55:41:15.1: 13.14 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:07.47 +55:41:15.1: 13.10 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 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
Large-amplitude variable Gaia DR2 2174670486054033920,2461201.6709,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2174670486054033920 20260610.1709 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 06 10.1709 2461201.6709 12.53 21:40:54.54 +56:04:30.6
98.55483 2.50106 galactic Cep Second-epoch detections are separated by 0.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:54.54 +56:04:30.6 (user input) | T | P | (position from user input) J-Ks=0.518+/-0.035 (K)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:54.54 +56:04:30.6: 13.48 +/- 0.06 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:54.54 +56:04:30.6: 13.44 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461201.6709,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260610.1709 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 11.74 21:14:14.26 +53:30:56.8
94.00619 3.31456 galactic Cyg Second-epoch detections are separated by 1.5" and 7.4 pix
The object was found in VSX 1" V3126 Cyg
Type: SRB
# Max. Min./Amp. JD0 Period
13.200 V 14.000 V 2458322.09900 110.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:14:14.26 +53:30:56.8: 12.62 +/- 0.02 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:14:14.26 +53:30:56.8: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 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
V3126 Cyg,2461201.6709,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V3126 Cyg 20260610.1709 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.38 21:35:35.27 +54:02:24.0
96.63148 1.48750 galactic Cyg Second-epoch detections are separated by 1.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2174430036605292928 | 21:35:35.36 +54:02:25.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.425+/-0.038 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:35.27 +54:02:24.0: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:35.27 +54:02:24.0: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 2174430036605292928,2461201.6709,12.38,0.05,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 2174430036605292928 20260610.1709 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 06 10.1709 2461201.6709 12.51 21:42:39.82 +57:33:16.8
99.70835 3.45999 galactic Cep Second-epoch detections are separated by 1.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:39.82 +57:33:16.8 (user input) | T | P | (position from user input) J-Ks=0.929+/-0.061 (M)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:42:39.82 +57:33:16.8: 13.46 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:42:39.82 +57:33:16.8: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461201.6709,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260610.1709 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 06 10.1709 2461201.6709 12.53 21:40:17.31 +56:40:55.6
98.89068 3.01411 galactic Cep Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.0720+56.6834 | 21:40:17.31 +56:40:55.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:17.31 +56:40:55.6: 13.43 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:17.31 +56:40:55.6: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.0720+56.6834,2461201.6709,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.0720+56.6834 20260610.1709 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.16 21:38:10.99 +55:19:31.2
97.77010 2.19292 galactic Cyg Second-epoch detections are separated by 3.2" and 6.9 pix
The object was found in VSX 2" ASASSN-V J213811.06+551932.9
Type: SR
# Max. Min./Amp. JD0 Period
13.890 V 14.000 V 2457859.00000 129.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:10.99 +55:19:31.2: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:10.99 +55:19:31.2: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 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
ASASSN-V J213811.06+551932.9,2461201.6709,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213811.06+551932.9 20260610.1709 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.34 21:40:07.98 +55:09:15.4
97.86500 1.88067 galactic Cyg Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.0125+55.1533 | 21:40:07.98 +55:09:15.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.778+/-0.031 (K)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:07.98 +55:09:15.4: 13.27 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:07.98 +55:09:15.4: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.0125+55.1533,2461201.6709,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.0125+55.1533 20260610.1709 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.96 21:07:17.70 +51:07:32.6
91.53159 2.46081 galactic Cyg Second-epoch detections are separated by 5.4" and 8.2 pix
The object was found in VSX 3" Gaia DR3 2169182445559497472
Type: YSO
# Max. Min./Amp. JD0 Period
13.080 G 13.120 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:07:17.70 +51:07:32.6: 14.00 +/- 0.08 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:07:17.70 +51:07:32.6: 14.09 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2169182445559497472,2461201.6709,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2169182445559497472 20260610.1709 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.13 21:41:12.65 +55:40:47.2
98.32647 2.17538 galactic Cep Second-epoch detections are separated by 0.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:12.65 +55:40:47.2 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.036 (G)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:12.65 +55:40:47.2: 13.09 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:12.65 +55:40:47.2: 13.08 +/- 0.04 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
target,2461201.6709,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260610.1709 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 06 10.1709 2461201.6709 12.54 21:33:39.04 +55:13:21.5
97.22215 2.54992 galactic Cyg Second-epoch detections are separated by 2.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.4129+55.2231 | 21:33:39.11 +55:13:23.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.551+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:33:39.04 +55:13:21.5: 13.42 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:33:39.04 +55:13:21.5: 13.60 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.4129+55.2231,2461201.6709,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.4129+55.2231 20260610.1709 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 11.93 21:40:13.06 +56:22:45.0
98.68310 2.79300 galactic Cep Second-epoch detections are separated by 1.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2178082064479579136 | 21:40:13.11 +56:22:47.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.947+/-0.032 (M)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:13.06 +56:22:45.0: 12.83 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:13.06 +56:22:45.0: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 2178082064479579136,2461201.6709,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2178082064479579136 20260610.1709 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.29 21:35:16.24 +54:10:19.6
96.68585 1.61657 galactic Cyg Second-epoch detections are separated by 0.8" and 6.8 pix
The object was found in VSX20" ZTF J213516.69+541000.2
Type: HADS:|EW
# Max. Min./Amp. JD0 Period
15.173 r Y 0.177 r 2458296.84420 0.176155600000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:16.24 +54:10:19.6: 13.22 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:16.24 +54:10:19.6: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 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
ZTF J213516.69+541000.2,2461201.6709,12.29,0.05,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
ZTF J213516.69+541000.2 20260610.1709 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 06 10.1709 2461201.6709 11.88 21:39:34.24 +55:56:34.3
98.32676 2.52510 galactic Cep Second-epoch detections are separated by 0.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2175051531244546816 | 21:39:34.33 +55:56:35.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.320+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:34.24 +55:56:34.3: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:34.24 +55:56:34.3: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.84 +/- 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 2175051531244546816,2461201.6709,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2175051531244546816 20260610.1709 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.53 21:37:45.34 +57:12:03.3
98.97669 3.63143 galactic Cep Second-epoch detections are separated by 1.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.4395+57.2012 | 21:37:45.49 +57:12:04.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.532+/-0.037 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:37:45.34 +57:12:03.3: 13.58 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:37:45.34 +57:12:03.3: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.4395+57.2012,2461201.6709,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.4395+57.2012 20260610.1709 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.46 21:40:46.98 +56:33:48.9
98.86362 2.88016 galactic Cep Second-epoch detections are separated by 1.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1852+56.5642 | 21:40:46.98 +56:33:48.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.722+/-0.033 (K)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:46.98 +56:33:48.9: 13.39 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:46.98 +56:33:48.9: 13.36 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1852+56.5642,2461201.6709,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1852+56.5642 20260610.1709 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.28 21:40:52.82 +56:29:35.7
98.82735 2.81839 galactic Cep Second-epoch detections are separated by 1.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:52.82 +56:29:35.7 (user input) | T | P | (position from user input) J-Ks=0.823+/-0.032 (M)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:52.82 +56:29:35.7: 13.39 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:52.82 +56:29:35.7: 13.31 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461201.6709,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260610.1709 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.27 21:39:37.31 +58:00:48.9
99.70532 4.07232 galactic Cep Second-epoch detections are separated by 0.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2178552758534378368 | 21:39:37.39 +58:00:50.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.266+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:37.31 +58:00:48.9: 13.21 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:37.31 +58:00:48.9: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 2178552758534378368,2461201.6709,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2178552758534378368 20260610.1709 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 06 10.1709 2461201.6709 12.22 21:40:56.82 +56:48:10.5
99.03841 3.04543 galactic Cep Second-epoch detections are separated by 1.5" and 7.0 pix
The object was found in VSX 1" ASASSN-V J214056.94+564811.5
Type: L
# Max. Min./Amp. JD0 Period
13.830 V 14.180 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:56.82 +56:48:10.5: 13.21 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:56.82 +56:48:10.5: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 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
ASASSN-V J214056.94+564811.5,2461201.6709,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214056.94+564811.5 20260610.1709 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.41 21:38:01.33 +54:32:13.7
97.22821 1.61980 galactic Cyg Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.5215+54.5459 | 21:38:01.33 +54:32:13.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.966+/-0.031 (M)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:01.33 +54:32:13.7: 13.36 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:01.33 +54:32:13.7: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.5215+54.5459,2461201.6709,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.5215+54.5459 20260610.1709 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.02 21:41:30.56 +55:57:24.7
98.54026 2.35676 galactic Cep Second-epoch detections are separated by 0.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3805+55.9615 | 21:41:30.63 +55:57:25.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.940+/-0.035 (M)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:30.56 +55:57:24.7: 12.95 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:30.56 +55:57:24.7: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 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 J325.3805+55.9615,2461201.6709,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3805+55.9615 20260610.1709 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.44 21:41:33.00 +57:11:40.5
99.35834 3.28648 galactic Cep Second-epoch detections are separated by 2.6" and 7.2 pix
The object was found in VSX21" ZTF J214134.67+571124.6
Type: EB:
# Max. Min./Amp. JD0 Period
18.456 r Y 0.407 r 2458433.61820 1.765768200000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:33.00 +57:11:40.5: 13.34 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:33.00 +57:11:40.5: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 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
ZTF J214134.67+571124.6,2461201.6709,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214134.67+571124.6 20260610.1709 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.41 21:38:15.43 +55:44:35.8
98.05614 2.49806 galactic Cep Second-epoch detections are separated by 0.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:38:15.43 +55:44:35.8 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.033 (G)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:15.43 +55:44:35.8: 13.31 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:15.43 +55:44:35.8: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461201.6709,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260610.1709 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 10.1709 2461201.6709 12.75 21:22:01.55 +54:44:15.4
95.68018 3.35294 galactic Cyg Second-epoch detections are separated by 1.4" and 7.2 pix
The object was found in ASASSN-V 3" ASASSN-V J212201.64+544417.8
Type: SR
MeanMag 14.79 m Amp. 0.13 m Period 27.7197053 d
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:22:01.55 +54:44:15.4: 13.75 +/- 0.06 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:22:01.55 +54:44:15.4: 13.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 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
VARIABLE_NAME,2461201.6709,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260610.1709 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461171.90353176 11.05.2026 09:40:55.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
First image: 2461171.90353176 11.05.2026 09:40:55.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Last image: 2461201.67120362 10.06.2026 04:06:21.993 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15777
Objects passed selection criteria: 15694
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 10759.8
Average stars matched: 10542.8 (97.9832 %)
Memory usage VmPeak: 122812 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 9 23:15:33 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461171.90353176 11.05.2026 09:40:55.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
First image: 2461171.90353176 11.05.2026 09:40:55.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Last image: 2461201.67120362 10.06.2026 04:06:21.993 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 106
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
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: 49 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 116595
Objects passed selection criteria: 116280
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 85954
Average stars matched: 82991.2 (96.5531 %)
Memory usage VmPeak: 1958056 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 9 23:20:24 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.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-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.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: 2461201.67062190
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits'
wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits (1st reference image)
verification OK: wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:10:39.370 +54:00:06.17 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-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits (1st new image)
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
Image size: 938.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:10:34.922 +54:00:01.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:10:39.370 +54:00:06.17
Second-epoch image center 21:10:34.922 +54:00:01.46
Angular distance between the image centers 0.0110 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits (2nd new image)
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
Image size: 938.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:10:38.499 +53:59:31.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:10:39.370 +54:00:06.17
Second-epoch image center 21:10:38.499 +53:59:31.41
Angular distance between the image centers 0.0099 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 21:10:34.922 +54:00:01.46
Second-epoch second image center 21:10:38.499 +53:59:31.41
Angular distance between the image centers 0.01210 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits &> /tmp/tmp.wQlxHKx5Hb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits &> /tmp/tmp.vokGPEAUM0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits &> /tmp/tmp.Ad2UcK3ffG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits &> /tmp/tmp.0HRprgNzSi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.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-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits and wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.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-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits and wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
Found non-empty wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits and wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
The reference image (wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits) and catalog (wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat) found
'wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat' -> 'wcsmag.cat'
Read 25074 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 302.6809 to 332.6436 deg, Dec +48.1331 to +59.2551 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 302.6809 to 332.6436 deg, Dec 48.1331 to 59.2551 deg
Loaded 20051 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): 12364 out of 13307 total matches.
Matched with Tycho-2 13307 out of 25074 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.604000
a=0.000000 b=1.000000 c=22.604000
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.86
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.86
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 25074 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 302.6809 to 332.6436 deg, Dec +48.1331 to +59.2551 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 302.6809 to 332.6436 deg, Dec 48.1331 to 59.2551 deg
Loaded 20051 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): 12364 out of 13307 total matches.
Matched with Tycho-2 13307 out of 25074 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits:
Forced-photometry filter: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits -> calib.txt_param_ref_wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits (aperture=6.5)
Read 23932 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 302.6813 to 332.6439 deg, Dec +48.1787 to +59.2616 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 302.6813 to 332.6439 deg, Dec 48.1787 to 59.2616 deg
Loaded 19971 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): 12294 out of 13147 total matches.
Matched with Tycho-2 13147 out of 23932 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits:
Forced-photometry filter: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits -> calib.txt_param_ref_wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.6 pix Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
2.6 pix Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
2.3 pix fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
2.3 pix fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
2.6 pix wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
2.6 pix wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
Limiting magnitude estimates:
14.9 mag. Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
14.8 mag. Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
13.2 mag. fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
13.3 mag. fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wQlxHKx5Hb (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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.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-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits' -> 'wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2300, passed=25074
Got 25074 stars (including 22754 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
util/solve_plate_with_UCAC5 got 25074 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 24212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 24212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 24212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits N_match=967 sigma_overall_arcsec=0.764 sigma_q1_arcsec=0.542 sigma_q2_arcsec=0.833 sigma_q3_arcsec=0.622 sigma_q4_arcsec=0.875 n_q1=190 n_q2=331 n_q3=174 n_q4=272 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits -region wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.vokGPEAUM0 (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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.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-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits' -> 'wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2110, passed=23932
Got 23932 stars (including 21798 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat
util/solve_plate_with_UCAC5 got 23932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 23180 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 23180 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 23180 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits N_match=967 sigma_overall_arcsec=0.770 sigma_q1_arcsec=0.579 sigma_q2_arcsec=0.827 sigma_q3_arcsec=0.679 sigma_q4_arcsec=0.930 n_q1=190 n_q2=327 n_q3=179 n_q4=271 worst_quadrant_to_overall_ratio=1.207
The image catalog is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits -region wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Ad2UcK3ffG (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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=278, passed=4836
Got 4836 stars (including 4549 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat
util/solve_plate_with_UCAC5 got 4836 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 4712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 4713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 4713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits N_match=964 sigma_overall_arcsec=0.608 sigma_q1_arcsec=0.628 sigma_q2_arcsec=0.481 sigma_q3_arcsec=0.617 sigma_q4_arcsec=0.647 n_q1=267 n_q2=141 n_q3=311 n_q4=245 worst_quadrant_to_overall_ratio=1.065
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0HRprgNzSi (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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=316, passed=5340
Got 5340 stars (including 5023 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat
util/solve_plate_with_UCAC5 got 5340 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5252 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5255 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5255 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits N_match=962 sigma_overall_arcsec=0.596 sigma_q1_arcsec=0.582 sigma_q2_arcsec=0.476 sigma_q3_arcsec=0.648 sigma_q4_arcsec=0.738 n_q1=282 n_q2=169 n_q3=314 n_q4=197 worst_quadrant_to_overall_ratio=1.238
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits sigma_overall=0.764 worst_q_ratio=1.146
ref2=Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits sigma_overall=0.770 worst_q_ratio=1.207
new1=fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits sigma_overall=0.608 worst_q_ratio=1.065
new2=fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits sigma_overall=0.596 worst_q_ratio=1.238
reference average sigma_overall=0.767 worst_q_ratio=1.1765
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484_astrometric_residuals.png (967 matched stars from wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.65 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485_astrometric_residuals.png (967 matched stars from wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.69 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025_astrometric_residuals.png (964 matched stars from wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026_astrometric_residuals.png (962 matched stars from wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.54 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits'
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:49:45.39 +50:08:23.3: 10.37 +/- 0.00 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:49:45.39 +50:08:23.3: 10.37 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.37 +/- 0.00
Forced photometry filter REJECTED candidate at 20:49:45.39 +50:08:23.3: ref_mag=10.37 +/- 0.00 new_mean_mag=10.5275 delta=-0.16 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30824_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 30824_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.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-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits exists and is non-empty
wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits (1st reference image)
verification OK: wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:10:39.370 +54:00:06.17 J2000 4789.000 3195.000
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The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
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# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits (1st new image)
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
Image size: 938.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:10:34.922 +54:00:01.46 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:10:39.370 +54:00:06.17
Second-epoch image center 21:10:34.922 +54:00:01.46
Angular distance between the image centers 0.0110 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
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# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits (2nd new image)
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
Image size: 938.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:10:38.499 +53:59:31.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:10:39.370 +54:00:06.17
Second-epoch image center 21:10:38.499 +53:59:31.41
Angular distance between the image centers 0.0099 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 21:10:34.922 +54:00:01.46
Second-epoch second image center 21:10:38.499 +53:59:31.41
Angular distance between the image centers 0.01210 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits &> /tmp/tmp.Stz2HB0WLQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits &> /tmp/tmp.gzB323GGvF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits &> /tmp/tmp.LscpXhZzsG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits &> /tmp/tmp.WN9QxoKmJb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.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-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits and wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.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-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits and wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
Found non-empty wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits and wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
The reference image (wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits) and catalog (wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat) found
'wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat' -> 'wcsmag.cat'
Read 166720 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 302.6238 to 332.6465 deg, Dec +48.1332 to +59.2664 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 302.6238 to 332.6465 deg, Dec 48.1332 to 59.2664 deg
Loaded 20101 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): 10299 out of 14062 total matches.
Matched with Tycho-2 14062 out of 166720 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.432000
a=0.000000 b=1.000000 c=22.432000
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 166720 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 302.6238 to 332.6465 deg, Dec +48.1332 to +59.2664 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 302.6238 to 332.6465 deg, Dec 48.1332 to 59.2664 deg
Loaded 20101 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): 10299 out of 14062 total matches.
Matched with Tycho-2 14062 out of 166720 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits:
Forced-photometry filter: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits -> calib.txt_param_ref_wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits (aperture=4.8)
Read 161710 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 302.6650 to 332.6591 deg, Dec +48.1415 to +59.2752 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 302.6650 to 332.6591 deg, Dec 48.1415 to 59.2752 deg
Loaded 20074 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): 10472 out of 14069 total matches.
Matched with Tycho-2 14069 out of 161710 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits:
Forced-photometry filter: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits -> calib.txt_param_ref_wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 71 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
2.4 pix Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
2.1 pix fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
2.2 pix fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
2.4 pix wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
2.4 pix wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
Limiting magnitude estimates:
15.0 mag. Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
15.0 mag. Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
13.4 mag. fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
13.5 mag. fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 13.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Stz2HB0WLQ (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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.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-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits' -> 'wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=23344, passed=166675
Got 166675 stars (including 143106 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
util/solve_plate_with_UCAC5 got 166675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 161984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 161982 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 161983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits N_match=972 sigma_overall_arcsec=0.709 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.746 sigma_q3_arcsec=0.588 sigma_q4_arcsec=0.812 n_q1=194 n_q2=311 n_q3=200 n_q4=267 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits -region wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.gzB323GGvF (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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.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-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits' -> 'wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=21772, passed=161655
Got 161655 stars (including 139686 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat
util/solve_plate_with_UCAC5 got 161655 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 156585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 156584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 156583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits N_match=969 sigma_overall_arcsec=0.738 sigma_q1_arcsec=0.515 sigma_q2_arcsec=0.771 sigma_q3_arcsec=0.660 sigma_q4_arcsec=0.812 n_q1=197 n_q2=314 n_q3=193 n_q4=265 worst_quadrant_to_overall_ratio=1.099
The image catalog is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits -region wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LscpXhZzsG (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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=2233, passed=45324
Got 45324 stars (including 43003 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat
util/solve_plate_with_UCAC5 got 45324 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 44337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 44338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 44338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits N_match=961 sigma_overall_arcsec=0.586 sigma_q1_arcsec=0.638 sigma_q2_arcsec=0.498 sigma_q3_arcsec=0.633 sigma_q4_arcsec=0.613 n_q1=271 n_q2=143 n_q3=304 n_q4=243 worst_quadrant_to_overall_ratio=1.089
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WN9QxoKmJb (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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=2543, passed=47916
Got 47916 stars (including 45299 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat
util/solve_plate_with_UCAC5 got 47916 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 47140 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 47140 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 47140 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits N_match=965 sigma_overall_arcsec=0.598 sigma_q1_arcsec=0.610 sigma_q2_arcsec=0.464 sigma_q3_arcsec=0.650 sigma_q4_arcsec=0.682 n_q1=294 n_q2=172 n_q3=300 n_q4=199 worst_quadrant_to_overall_ratio=1.140
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
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-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-05-31_20.00sec_4.90C_LIGHT_0025.fits
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.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_2026-06-09_CI_Cyg-02-Q2b1x1_231106_TTUQ2b1x1_2244493_P88MzZnc/wcs_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026.fits
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:26:25.07 +53:01:53.9: 13.18 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:48:13.11 +54:17:13.5: 12.47 +/- 0.02 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:26:50.02 +55:45:28.1: 11.47 +/- 0.01 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:28:02.88 +51:35:41.8: 13.35 +/- 0.06 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:29:33.81 +54:58:34.2: 12.96 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:19:08.10 +57:30:01.5: 12.02 +/- 0.01 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:40:26.80 +55:05:48.3: 12.29 +/- 0.02 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:26:37.01 +52:23:03.2: 12.39 +/- 0.02 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:49:25.42 +50:46:35.1: 12.13 +/- 0.02 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:28:02.88 +51:35:41.8: 13.25 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:26:50.02 +55:45:28.1: 11.43 +/- 0.01 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:48:13.11 +54:17:13.5: 12.44 +/- 0.02 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:25:24.47 +55:25:10.7: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.04
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:29:33.81 +54:58:34.2: 12.90 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 20:28:02.88 +51:35:41.8: ref_mag=13.29 +/- 0.04 new_mean_mag=13.1659 delta=0.13 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:26:25.07 +53:01:53.9: 13.03 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 20:26:50.02 +55:45:28.1: ref_mag=11.45 +/- 0.01 new_mean_mag=11.4028 delta=0.04 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:40:26.80 +55:05:48.3: 12.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 20:48:13.11 +54:17:13.5: ref_mag=12.45 +/- 0.01 new_mean_mag=12.9822 delta=-0.53 (need > 0.90)
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:19:08.10 +57:30:01.5: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Forced photometry reference-image weighted average: 12.31 +/- 0.02
Forced photometry filter REJECTED candidate at 20:29:33.81 +54:58:34.2: ref_mag=12.93 +/- 0.02 new_mean_mag=12.7960 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 20:26:25.07 +53:01:53.9: ref_mag=13.11 +/- 0.03 new_mean_mag=13.0826 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 20:40:26.80 +55:05:48.3: ref_mag=12.31 +/- 0.02 new_mean_mag=12.2932 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry filter REJECTED candidate at 21:19:08.10 +57:30:01.5: ref_mag=12.01 +/- 0.01 new_mean_mag=12.4809 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:49:25.42 +50:46:35.1: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:26:37.01 +52:23:03.2: 12.38 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 20:49:25.42 +50:46:35.1: ref_mag=12.15 +/- 0.01 new_mean_mag=12.1231 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Forced photometry filter REJECTED candidate at 20:26:37.01 +52:23:03.2: ref_mag=12.38 +/- 0.02 new_mean_mag=12.3322 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:25:24.47 +55:25:10.7: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter REJECTED candidate at 20:25:24.47 +55:25:10.7: ref_mag=12.87 +/- 0.02 new_mean_mag=12.4912 delta=0.38 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:32:14.01 +54:10:28.8: 12.73 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:31:28.47 +52:34:12.3: 12.82 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:20:30.53 +56:32:41.6: 13.08 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:54:22.63 +53:44:50.3: 12.43 +/- 0.02 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:32:14.01 +54:10:28.8: 12.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry filter REJECTED candidate at 20:32:14.01 +54:10:28.8: ref_mag=12.72 +/- 0.02 new_mean_mag=12.5191 delta=0.20 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:31:28.47 +52:34:12.3: 12.76 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.03
Forced photometry filter REJECTED candidate at 20:31:28.47 +52:34:12.3: ref_mag=12.79 +/- 0.03 new_mean_mag=12.7490 delta=0.04 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:20:30.53 +56:32:41.6: 13.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.03
Forced photometry filter REJECTED candidate at 20:20:30.53 +56:32:41.6: ref_mag=13.05 +/- 0.03 new_mean_mag=12.7311 delta=0.32 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:54:22.63 +53:44:50.3: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.02
Forced photometry filter REJECTED candidate at 20:54:22.63 +53:44:50.3: ref_mag=12.44 +/- 0.02 new_mean_mag=12.5172 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:31:28.92 +56:34:18.2: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:26:33.75 +52:45:15.2: 12.29 +/- 0.02 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:25:21.85 +57:12:36.0: 13.22 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:26:41.75 +57:35:31.0: 13.60 +/- 0.06 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:31:00.87 +54:15:54.8: 13.34 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:31:28.92 +56:34:18.2: 12.95 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:25:21.85 +57:12:36.0: 13.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry reference-image weighted average: 13.25 +/- 0.04
Forced photometry filter REJECTED candidate at 20:25:21.85 +57:12:36.0: ref_mag=13.25 +/- 0.04 new_mean_mag=13.0259 delta=0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 20:31:28.92 +56:34:18.2: ref_mag=12.94 +/- 0.02 new_mean_mag=12.6915 delta=0.25 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:26:33.75 +52:45:15.2: 12.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter REJECTED candidate at 21:26:33.75 +52:45:15.2: ref_mag=12.29 +/- 0.01 new_mean_mag=12.3671 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:26:41.75 +57:35:31.0: 13.59 +/- 0.06 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:31:00.87 +54:15:54.8: 13.32 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter REJECTED candidate at 20:31:00.87 +54:15:54.8: ref_mag=13.33 +/- 0.03 new_mean_mag=13.0158 delta=0.32 (need > 0.90)
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Forced photometry filter REJECTED candidate at 20:26:41.75 +57:35:31.0: ref_mag=13.60 +/- 0.04 new_mean_mag=13.4748 delta=0.12 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:20:44.88 +54:21:22.7: 13.71 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:44.39 +55:43:50.7: 13.33 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:36.77 +56:01:48.4: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:47.46 +56:20:41.8: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:33.31 +56:07:56.5: 12.90 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:20:44.88 +54:21:22.7: 13.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter KEPT candidate at 21:20:44.88 +54:21:22.7: ref_mag=13.74 +/- 0.04 new_mean_mag=12.6625 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:44.39 +55:43:50.7: 13.31 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:36.77 +56:01:48.4: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.04
Forced photometry filter KEPT candidate at 21:40:44.39 +55:43:50.7: ref_mag=13.32 +/- 0.04 new_mean_mag=12.3797 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry filter KEPT candidate at 21:41:36.77 +56:01:48.4: ref_mag=12.88 +/- 0.02 new_mean_mag=11.8887 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:47.46 +56:20:41.8: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Forced photometry filter KEPT candidate at 21:41:47.46 +56:20:41.8: ref_mag=13.28 +/- 0.03 new_mean_mag=12.3623 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:33.31 +56:07:56.5: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 21:41:33.31 +56:07:56.5: ref_mag=12.91 +/- 0.02 new_mean_mag=11.9535 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:54.54 +56:04:30.6: 13.48 +/- 0.06 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:07.47 +55:41:15.1: 13.14 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:14:14.26 +53:30:56.8: 12.62 +/- 0.02 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:42:09.75 +54:11:31.4: 13.18 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:07.47 +55:41:15.1: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:42:09.75 +54:11:31.4: 13.29 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter KEPT candidate at 21:39:07.47 +55:41:15.1: ref_mag=13.12 +/- 0.03 new_mean_mag=12.1450 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:54.54 +56:04:30.6: 13.44 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Forced photometry filter REJECTED candidate at 20:42:09.75 +54:11:31.4: ref_mag=13.22 +/- 0.03 new_mean_mag=13.0532 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Forced photometry filter KEPT candidate at 21:40:54.54 +56:04:30.6: ref_mag=13.46 +/- 0.04 new_mean_mag=12.5289 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:14:14.26 +53:30:56.8: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 21:14:14.26 +53:30:56.8: ref_mag=12.62 +/- 0.01 new_mean_mag=11.6965 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:35.27 +54:02:24.0: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:35.27 +54:02:24.0: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry filter KEPT candidate at 21:35:35.27 +54:02:24.0: ref_mag=13.30 +/- 0.03 new_mean_mag=12.3527 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:42:39.82 +57:33:16.8: 13.46 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:42:39.82 +57:33:16.8: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 21:42:39.82 +57:33:16.8: ref_mag=13.36 +/- 0.03 new_mean_mag=12.4473 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:17.31 +56:40:55.6: 13.43 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:17.31 +56:40:55.6: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter KEPT candidate at 21:40:17.31 +56:40:55.6: ref_mag=13.44 +/- 0.03 new_mean_mag=12.5287 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:10.99 +55:19:31.2: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:10.99 +55:19:31.2: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Forced photometry filter KEPT candidate at 21:38:10.99 +55:19:31.2: ref_mag=13.10 +/- 0.03 new_mean_mag=12.1539 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:07.98 +55:09:15.4: 13.27 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:07.98 +55:09:15.4: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Forced photometry filter KEPT candidate at 21:40:07.98 +55:09:15.4: ref_mag=13.24 +/- 0.03 new_mean_mag=12.3213 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:07:17.70 +51:07:32.6: 14.00 +/- 0.08 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:12.65 +55:40:47.2: 13.09 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:33:39.04 +55:13:21.5: 13.42 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:07:17.70 +51:07:32.6: 14.09 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.06
Forced photometry filter KEPT candidate at 21:07:17.70 +51:07:32.6: ref_mag=14.04 +/- 0.06 new_mean_mag=12.9230 delta=1.11 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:12.65 +55:40:47.2: 13.08 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 21:41:12.65 +55:40:47.2: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1176 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:13.06 +56:22:45.0: 12.83 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:33:39.04 +55:13:21.5: 13.60 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Forced photometry filter KEPT candidate at 21:33:39.04 +55:13:21.5: ref_mag=13.48 +/- 0.04 new_mean_mag=12.5053 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:16.24 +54:10:19.6: 13.22 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:13.06 +56:22:45.0: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 21:40:13.06 +56:22:45.0: ref_mag=12.87 +/- 0.02 new_mean_mag=11.9215 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:34.24 +55:56:34.3: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:16.24 +54:10:19.6: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Forced photometry filter KEPT candidate at 21:35:16.24 +54:10:19.6: ref_mag=13.25 +/- 0.03 new_mean_mag=12.3083 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:34.24 +55:56:34.3: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter KEPT candidate at 21:39:34.24 +55:56:34.3: ref_mag=12.84 +/- 0.02 new_mean_mag=11.8784 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:37:45.34 +57:12:03.3: 13.58 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:46.98 +56:33:48.9: 13.39 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:37:45.34 +57:12:03.3: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:46.98 +56:33:48.9: 13.36 +/- 0.05 detection
Forced photometry filter KEPT candidate at 21:37:45.34 +57:12:03.3: ref_mag=13.56 +/- 0.04 new_mean_mag=12.5244 delta=1.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 21:40:46.98 +56:33:48.9: ref_mag=13.38 +/- 0.03 new_mean_mag=12.4538 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:52.82 +56:29:35.7: 13.39 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:52.82 +56:29:35.7: 13.31 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 21:40:52.82 +56:29:35.7: ref_mag=13.35 +/- 0.03 new_mean_mag=12.2801 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:37.31 +58:00:48.9: 13.21 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:37.31 +58:00:48.9: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry filter KEPT candidate at 21:39:37.31 +58:00:48.9: ref_mag=13.20 +/- 0.03 new_mean_mag=12.2593 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:56.82 +56:48:10.5: 13.21 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:56.82 +56:48:10.5: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Forced photometry filter KEPT candidate at 21:40:56.82 +56:48:10.5: ref_mag=13.21 +/- 0.03 new_mean_mag=12.2011 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:01.33 +54:32:13.7: 13.36 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:01.33 +54:32:13.7: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 21:38:01.33 +54:32:13.7: ref_mag=13.36 +/- 0.03 new_mean_mag=12.4128 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:30.56 +55:57:24.7: 12.95 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:30.56 +55:57:24.7: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 21:41:30.56 +55:57:24.7: ref_mag=12.94 +/- 0.02 new_mean_mag=12.0120 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:33.00 +57:11:40.5: 13.34 +/- 0.05 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:33.00 +57:11:40.5: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 21:41:33.00 +57:11:40.5: ref_mag=13.36 +/- 0.03 new_mean_mag=12.3804 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:15.43 +55:44:35.8: 13.31 +/- 0.04 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:22:01.55 +54:44:15.4: 13.75 +/- 0.06 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:15.43 +55:44:35.8: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry filter KEPT candidate at 21:38:15.43 +55:44:35.8: ref_mag=13.30 +/- 0.03 new_mean_mag=12.3971 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:22:01.55 +54:44:15.4: 13.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter KEPT candidate at 21:22:01.55 +54:44:15.4: ref_mag=13.76 +/- 0.04 new_mean_mag=12.7325 delta=1.02 (need > 0.90)
Adding exclusion_list_local.txt__out103578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97984.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 50s
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: 13s
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Considering the candidate 187512_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187512_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187517_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187517_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187524_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187524_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187532_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187532_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 20:44:09.35 +55:04:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187533_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187533_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187538_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187538_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187552_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187552_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187641_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187641_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:39:06.82 +56:56:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187696_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187696_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 20:31:30.47 +49:11:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187736_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187736_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187738_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187738_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187750_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187750_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187764_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187764_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187779_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187779_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 20:24:21.75 +54:03:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187821_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187821_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:01:54.83 +57:06:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187838_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187838_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 20:31:17.12 +49:11:35.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 187840_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187840_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187842_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187842_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 20:46:17.58 +53:01:15.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 187843_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187843_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 187849_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187849_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:19:34.60 +53:02:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187859_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187859_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 20:26:20.02 +56:39:26.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 187865_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187865_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187885_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187885_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187889_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187889_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
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Considering the candidate 187901_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187901_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:17:49.87 +52:29:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187927_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187927_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:34:48.75 +54:40:21.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187933_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187933_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:30:27.48 +52:56:37.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187936_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187936_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:18:56.23 +50:04:39.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187986_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 187986_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 20:27:03.45 +53:51:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188000_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 188000_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:39:32.47 +55:21:52.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188011_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 188011_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:27:07.38 +55:34:17.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188012_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 188012_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188114_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 188114_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188123_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 188123_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188138_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 188138_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 20:54:07.06 +57:10:00.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188227_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 188227_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188228_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 188228_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97984_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 97984_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143153_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 143153_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138420_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 138420_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133974_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 133974_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137084_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 137084_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143921_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 143921_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137960_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 137960_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84501_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 84501_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104599_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 104599_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:32:48.33 +54:40:12.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181446_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 181446_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99461_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 99461_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:34:28.27 +54:19:37.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94987_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 94987_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165653_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 165653_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129973_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 129973_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149918_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 149918_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114476_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 114476_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42567_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 42567_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143881_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 143881_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114160_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 114160_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133981_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 133981_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96779_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 96779_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140465_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 140465_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123784_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 123784_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131466_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 131466_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137073_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 137073_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:38:54.18 +56:09:27.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132491_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 132491_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160531_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 160531_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128290_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 128290_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103578_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 103578_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139443_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 139443_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123245_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 123245_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143289_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 143289_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126834_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
The candidate 126834_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026 did not pass the final checks
**** FOUND 21:42:03.54 +56:54:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104495_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
Preparing report for the candidate 104495_fd_Cyg-02-Q2b1x1_2026-06-09_23-06-21_20.00sec_5.00C_LIGHT_0026
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 66s
Prepared the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:38:01.33 +54:32:13.7
21:22:01.55 +54:44:15.4
21:33:39.04 +55:13:21.5
21:40:07.98 +55:09:15.4
21:41:33.00 +57:11:40.5
21:37:45.34 +57:12:03.3
21:40:56.82 +56:48:10.5
21:40:17.31 +56:40:55.6
21:40:46.98 +56:33:48.9
21:40:52.82 +56:29:35.7
21:41:47.46 +56:20:41.8
21:40:13.06 +56:22:45.0
21:41:33.31 +56:07:56.5
21:40:54.54 +56:04:30.6
21:41:36.77 +56:01:48.4
21:41:30.56 +55:57:24.7
21:39:34.24 +55:56:34.3
21:40:44.39 +55:43:50.7
21:38:15.43 +55:44:35.8
21:41:12.65 +55:40:47.2
21:39:07.47 +55:41:15.1
21:38:10.99 +55:19:31.2
21:39:37.31 +58:00:48.9
21:42:39.82 +57:33:16.8
21:07:17.70 +51:07:32.6
21:14:14.26 +53:30:56.8
21:35:35.27 +54:02:24.0
21:35:16.24 +54:10:19.6
21:20:44.88 +54:21:22.7
########### Completed Cyg-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:20:44.88 +54:21:22.7
21:40:44.39 +55:43:50.7
21:41:36.77 +56:01:48.4
21:41:47.46 +56:20:41.8
21:41:33.31 +56:07:56.5
21:39:07.47 +55:41:15.1
21:40:54.54 +56:04:30.6
21:14:14.26 +53:30:56.8
21:35:35.27 +54:02:24.0
21:42:39.82 +57:33:16.8
21:40:17.31 +56:40:55.6
21:38:10.99 +55:19:31.2
21:40:07.98 +55:09:15.4
21:07:17.70 +51:07:32.6
21:41:12.65 +55:40:47.2
21:33:39.04 +55:13:21.5
21:40:13.06 +56:22:45.0
21:35:16.24 +54:10:19.6
21:39:34.24 +55:56:34.3
21:37:45.34 +57:12:03.3
21:40:46.98 +56:33:48.9
21:40:52.82 +56:29:35.7
21:39:37.31 +58:00:48.9
21:40:56.82 +56:48:10.5
21:38:01.33 +54:32:13.7
21:41:30.56 +55:57:24.7
21:41:33.00 +57:11:40.5
21:38:15.43 +55:44:35.8
21:22:01.55 +54:44:15.4
###################################################################################
21:20:44.88 +54:21:22.7 -- not an asteroid (will add it to exclusion list)
21:40:44.39 +55:43:50.7 -- not an asteroid (will add it to exclusion list)
21:41:36.77 +56:01:48.4 -- not an asteroid (will add it to exclusion list)
21:41:47.46 +56:20:41.8 -- not an asteroid (will add it to exclusion list)
21:41:33.31 +56:07:56.5 -- not an asteroid (will add it to exclusion list)
21:39:07.47 +55:41:15.1 -- not an asteroid (will add it to exclusion list)
21:40:54.54 +56:04:30.6 -- not an asteroid (will add it to exclusion list)
21:14:14.26 +53:30:56.8 -- not an asteroid (will add it to exclusion list)
21:35:35.27 +54:02:24.0 -- not an asteroid (will add it to exclusion list)
21:42:39.82 +57:33:16.8 -- not an asteroid (will add it to exclusion list)
21:40:17.31 +56:40:55.6 -- not an asteroid (will add it to exclusion list)
21:38:10.99 +55:19:31.2 -- not an asteroid (will add it to exclusion list)
21:40:07.98 +55:09:15.4 -- not an asteroid (will add it to exclusion list)
21:07:17.70 +51:07:32.6 -- not an asteroid (will add it to exclusion list)
21:41:12.65 +55:40:47.2 -- not an asteroid (will add it to exclusion list)
21:33:39.04 +55:13:21.5 -- not an asteroid (will add it to exclusion list)
21:40:13.06 +56:22:45.0 -- not an asteroid (will add it to exclusion list)
21:35:16.24 +54:10:19.6 -- not an asteroid (will add it to exclusion list)
21:39:34.24 +55:56:34.3 -- not an asteroid (will add it to exclusion list)
21:37:45.34 +57:12:03.3 -- not an asteroid (will add it to exclusion list)
21:40:46.98 +56:33:48.9 -- not an asteroid (will add it to exclusion list)
21:40:52.82 +56:29:35.7 -- not an asteroid (will add it to exclusion list)
21:39:37.31 +58:00:48.9 -- not an asteroid (will add it to exclusion list)
21:40:56.82 +56:48:10.5 -- not an asteroid (will add it to exclusion list)
21:38:01.33 +54:32:13.7 -- not an asteroid (will add it to exclusion list)
21:41:30.56 +55:57:24.7 -- not an asteroid (will add it to exclusion list)
21:41:33.00 +57:11:40.5 -- not an asteroid (will add it to exclusion list)
21:38:15.43 +55:44:35.8 -- not an asteroid (will add it to exclusion list)
21:22:01.55 +54:44:15.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:07:17.70 +51:07:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:14.26 +53:30:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:44.88 +54:21:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:01.55 +54:44:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:39.04 +55:13:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:16.24 +54:10:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:35.27 +54:02:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:45.34 +57:12:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:01.33 +54:32:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:10.99 +55:19:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:15.43 +55:44:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:07.47 +55:41:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:34.24 +55:56:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:37.31 +58:00:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:07.98 +55:09:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:13.06 +56:22:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:17.31 +56:40:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:44.39 +55:43:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:46.98 +56:33:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:52.82 +56:29:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:54.54 +56:04:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:56.82 +56:48:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:12.65 +55:40:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:30.56 +55:57:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:33.00 +57:11:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:33.31 +56:07:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:36.77 +56:01:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:47.46 +56:20:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:39.82 +57:33:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
21:07:17.70 +51:07:32.6 -- a known variable star
21:14:14.26 +53:30:56.8 -- a known variable star
21:20:44.88 +54:21:22.7 -- not a known variable star
21:22:01.55 +54:44:15.4 -- a known variable star
21:33:39.04 +55:13:21.5 -- not a known variable star
21:35:16.24 +54:10:19.6 -- a known variable star
21:35:35.27 +54:02:24.0 -- not a known variable star
21:37:45.34 +57:12:03.3 -- not a known variable star
21:38:01.33 +54:32:13.7 -- not a known variable star
21:38:10.99 +55:19:31.2 -- a known variable star
21:38:15.43 +55:44:35.8 -- not a known variable star
21:39:07.47 +55:41:15.1 -- not a known variable star
21:39:34.24 +55:56:34.3 -- not a known variable star
21:39:37.31 +58:00:48.9 -- not a known variable star
21:40:07.98 +55:09:15.4 -- not a known variable star
21:40:13.06 +56:22:45.0 -- not a known variable star
21:40:17.31 +56:40:55.6 -- not a known variable star
21:40:44.39 +55:43:50.7 -- not a known variable star
21:40:46.98 +56:33:48.9 -- not a known variable star
21:40:52.82 +56:29:35.7 -- not a known variable star
21:40:54.54 +56:04:30.6 -- not a known variable star
21:40:56.82 +56:48:10.5 -- a known variable star
21:41:12.65 +55:40:47.2 -- not a known variable star
21:41:30.56 +55:57:24.7 -- not a known variable star
21:41:33.00 +57:11:40.5 -- a known variable star
21:41:33.31 +56:07:56.5 -- not a known variable star
21:41:36.77 +56:01:48.4 -- not a known variable star
21:41:47.46 +56:20:41.8 -- not a known variable star
21:42:39.82 +57:33:16.8 -- not a known variable star
Found 22 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
29 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 ####
21:07:17.70 +51:07:32.6
21:14:14.26 +53:30:56.8
21:20:44.88 +54:21:22.7
21:22:01.55 +54:44:15.4
21:33:39.04 +55:13:21.5
21:35:16.24 +54:10:19.6
21:35:35.27 +54:02:24.0
21:37:45.34 +57:12:03.3
21:38:01.33 +54:32:13.7
21:38:10.99 +55:19:31.2
21:38:15.43 +55:44:35.8
21:39:07.47 +55:41:15.1
21:39:34.24 +55:56:34.3
21:39:37.31 +58:00:48.9
21:40:07.98 +55:09:15.4
21:40:13.06 +56:22:45.0
21:40:17.31 +56:40:55.6
21:40:44.39 +55:43:50.7
21:40:46.98 +56:33:48.9
21:40:52.82 +56:29:35.7
21:40:54.54 +56:04:30.6
21:40:56.82 +56:48:10.5
21:41:12.65 +55:40:47.2
21:41:30.56 +55:57:24.7
21:41:33.00 +57:11:40.5
21:41:33.31 +56:07:56.5
21:41:36.77 +56:01:48.4
21:41:47.46 +56:20:41.8
21:42:39.82 +57:33:16.8
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461201.67062190 -observatory V36
06:55:08.31 +24:36:18.2 Mercury (0.2mag)
07:52:46.25 +22:58:26.9 Venus (-4.0mag)
02:55:21.73 +16:09:18.6 Mars (1.3mag)
07:50:05.48 +21:27:16.2 Jupiter (-1.9mag)
00:49:55.71 +02:51:41.4 Saturn (0.9mag)
04:00:40.56 +20:26:48.6 Uranus (5.8mag)
00:16:15.28 +00:17:25.6 Neptune (7.8mag)
20:33:14.66 -23:05:17.7 Pluto (14.5mag)
00:35:43.17 +06:29:09.8 Moon (-9.8mag)
-rw-r--r-- 1 apache apache 361 Jun 9 23:15 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461201.67062190:
07:50:11.12 +21:27:00.8 Io (6.0mag)
07:50:03.58 +21:27:20.7 Europa (6.2mag)
07:50:07.75 +21:27:14.8 Ganymede (5.6mag)
07:50:02.90 +21:27:17.5 Callisto (6.7mag)
07:50:15.68 +21:03:43.3 Himalia (15.6mag)
07:50:09.77 +21:27:03.0 Thebe (16.5mag)
07:50:11.83 +21:18:17.8 Elara (17.5mag)
07:52:22.26 +21:37:53.2 Pasiphae (17.7mag)
07:56:35.32 +21:29:07.7 Carme (18.9mag)
00:49:53.03 +02:51:22.3 Titan (8.6mag)
00:49:58.44 +02:51:32.4 Rhea (9.9mag)
00:50:26.64 +02:54:01.4 Iapetus (11.3mag)
00:49:59.14 +02:51:11.3 Hyperion (14.6mag)
00:50:35.55 +02:53:20.8 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 9 23:15 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461201.67062190:
17:27:25.59 -35:24:02.6 JWST
19:49:36.11 +02:01:24.0 Chandra
18:37:09.99 -23:05:36.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 9 23:15 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461201.67062190 -observatory V36
18:42:07.86 -32:47:47.7 13.6mag P/2010 H2 (Vales)
05:55:25.17 -68:02:41.0 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:49:47.27 +31:59:38.2 17.5mag C/2017 K2 (PANSTARRS)
17:13:56.42 +15:26:51.6 17.8mag C/2021 G2 (ATLAS)
21:30:48.92 -48:21:09.4 16.7mag P/2021 N1 (ZTF)
23:12:10.67 +31:39:58.2 17.2mag C/2022 E2 (ATLAS)
05:36:27.87 +26:59:10.7 16.5mag C/2022 N2 (PANSTARRS)
09:31:09.53 +31:00:46.8 16.6mag C/2022 QE78 (ATLAS)
08:51:36.76 +04:01:30.4 17.7mag C/2022 R6 (PANSTARRS)
18:26:55.82 +21:38:13.5 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:18:40.47 -11:00:45.4 17.6mag P/2023 B1 (PANSTARRS)
22:13:44.03 +66:38:51.9 17.7mag C/2023 H5 (Lemmon)
17:41:29.71 -06:53:01.5 13.7mag C/2023 R1 (PANSTARRS)
13:17:14.94 +82:32:29.5 17.9mag C/2023 X2 (Lemmon)
07:13:10.61 +64:22:35.6 17.7mag C/2024 A1 (ATLAS)
06:50:15.70 +28:00:31.3 13.7mag C/2024 E1 (Wierzchos)
15:35:45.01 +13:41:45.4 17.4mag C/2024 G6 (ATLAS)
20:11:42.19 +31:43:16.9 14.0mag C/2024 J3 (ATLAS)
04:20:00.46 -15:46:47.0 16.0mag C/2024 T5 (ATLAS)
06:07:45.20 +34:08:55.0 17.9mag C/2025 J1 (Borisov)
11:34:02.04 +52:38:04.9 17.5mag C/2025 L1 (ATLAS)
06:47:18.62 -10:57:37.4 14.3mag C/2025 R3 (PANSTARRS)
09:25:47.87 +23:18:45.0 17.9mag C/2025 V2 (Rankin)
12:39:40.33 +04:40:56.2 17.2mag C/2025 Y1 (ATLAS)
18:09:38.39 +75:33:09.4 17.9mag C/2026 A2 (Bok)
02:04:04.36 +43:33:16.4 16.1mag C/2026 B2 (Sun-Gao)
11:11:44.75 -03:02:53.4 16.5mag A/2026 E1
20:27:14.32 -08:43:16.3 8.6mag 10P/Tempel
11:02:28.92 -00:59:51.6 16.0mag 29P/Schwassmann-Wachmann
03:14:46.68 +25:54:32.4 17.7mag 47P/Ashbrook-Jackson
09:04:11.75 +23:12:09.9 16.9mag 63P/Wild
00:28:36.48 -06:14:33.4 15.7mag 65P/Gunn
06:49:51.15 +33:37:13.7 16.9mag 76P/West-Kohoutek-Ikemura
03:13:57.70 +17:27:55.9 13.8mag 78P/Gehrels
01:25:01.52 +05:16:30.7 15.6mag 88P/Howell
05:01:00.31 +30:26:38.9 15.3mag 93P/Lovas
02:48:33.95 +27:56:18.2 17.6mag 114P/Wiseman-Skiff
06:55:16.03 +32:57:46.2 15.6mag 123P/West-Hartley
09:53:37.38 +13:47:31.0 16.5mag 124P/Mrkos
04:02:17.83 +19:22:50.6 16.3mag 128P/Shoemaker-Holt
04:37:29.59 +19:10:20.4 17.7mag 131P/Mueller
06:06:43.38 +18:25:43.8 14.9mag 141P/Machholz
06:09:27.80 +17:46:03.8 14.8mag 141P-A/Machholz
05:03:59.52 +16:25:53.0 11.8mag 141P-D/Machholz
02:59:03.88 -24:25:41.0 16.8mag 161P/Hartley-IRAS
03:48:03.82 +24:35:38.1 14.9mag 162P/SidingSpring
19:36:25.04 +02:19:11.6 16.8mag 169P/NEAT
00:23:39.13 +02:50:59.8 17.9mag 220P/McNaught
16:50:41.25 -08:23:03.3 16.4mag 235P/LINEAR
07:39:07.34 +35:24:23.6 17.6mag 240P/NEAT
00:37:32.55 -01:37:32.7 16.3mag 260P/McNaught
04:09:36.80 +32:50:09.5 17.5mag 295P/LINEAR
00:04:29.95 -07:14:19.3 17.6mag 320P/McNaught
15:14:21.93 +08:01:43.0 17.4mag 391P/Kowalski
08:08:43.05 +20:41:44.3 17.9mag 450P/LONEOS
07:03:11.77 +41:33:19.8 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 9 23:15 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
-rw-r--r-- 1 apache apache 5.6K Jun 9 23:15 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
-rw-r--r-- 1 apache apache 189K Jun 9 23:15 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:23:26.878 -06:31:24.83 AT 2026obw 2026-04-21.32 20.79
09:08:05.365 +06:07:17.93 AT 2026obv 2026-04-19.27 20.87
14:54:41.741 +00:55:10.94 AT 2026obu 2026-05-21.33 21.1
12:03:02.150 -22:17:26.93 AT 2026obt 2026-05-17.30 20.99
23:11:22.861 -04:36:21.86 AT 2026obs 2026-05-20.59 21.32
07:02:52.735 +46:23:45.20 AT 2026obr 2026-01-19.40 22.44
12:14:13.586 +31:56:42.56 AT 2026obq 2026-04-21.42 21.1
14:28:24.646 -28:44:51.08 AT 2026obp 2026-02-26.57 20.77
00:42:53.928 +32:34:56.39 AT 2026obo 2026-06-02.19 18.19
20:47:03.272 -14:56:15.37 AT 2026obn 2026-05-29.20 19.74
12:24:13.754 +16:36:40.39 AT 2026obm 2026-06-01.18 20.1102
09:14:15.863 +00:13:04.61 AT 2026obl 2026-01-27.47 21.36
00:13:44.023 +42:21:15.72 AT 2026obk 2026-06-02.20 19.05
00:30:43.223 +42:00:32.99 AT 2026obj 2026-06-02.43 20.7792
01:06:40.547 +57:42:52.94 AT 2026obi 2026-06-02.43 20.5301
00:59:15.693 +47:14:15.65 AT 2026obh 2026-06-02.42 20.5376
00:58:21.823 +39:08:48.29 AT 2026obg 2026-06-02.43 19.2173
02:23:14.293 -15:08:54.46 SN 2026obf 2026-06-02.40 16.903
00:15:06.071 +10:42:05.91 AT 2026obe 2026-05-31.47 19.1659
00:56:14.195 +38:06:56.20 AT 2026obd 2026-06-02.43 19.7885
-rw-r--r-- 1 apache apache 30K Jun 9 23:15 tns_transients_list.txt
