This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.89 19:56:57.72 +33:43:08.1
69.91690 2.54206 galactic Cyg Second-epoch detections are separated by 1.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ZTF DR3 | 19:56:57.66 +33:43:07.4 (Gaia DR3) | 686110300122278 (VSX @ VizieR) | RR (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=0.111+/-0.046 (A)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:57.72 +33:43:08.1: 13.61 +/- 0.06 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:57.72 +33:43:08.1: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF DR3,2461186.6757,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF DR3 20260526.1757 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.33 19:56:18.94 +34:06:42.1
70.18358 2.86033 galactic Cyg Second-epoch detections are separated by 1.1" and 6.4 pix
The object was found in VSX 2" HAT 199-00851
Type: MISC
# Max. Min./Amp. JD0 Period
8.868 Ic 8.909 Ic
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:18.94 +34:06:42.1: 12.20 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:18.94 +34:06:42.1: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00851,2461186.6757,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00851 20260526.1757 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.85 19:56:24.76 +34:01:22.9
70.11804 2.79724 galactic Cyg Second-epoch detections are separated by 2.5" and 6.8 pix
The object was found in VSX22" ZTF J195623.43+340108.7
Type: RS
# Max. Min./Amp. JD0 Period
13.702 g Y 0.061 g 2458365.78010 2.330525000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:24.76 +34:01:22.9: 13.11 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:24.76 +34:01:22.9: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 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
ZTF J195623.43+340108.7,2461186.6757,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195623.43+340108.7 20260526.1757 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.35 19:55:32.12 +33:44:55.3
69.78868 2.81125 galactic Cyg Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J298.8771+33.7459 | 19:55:32.18 +33:44:55.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.355+/-0.028 (G)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:55:32.12 +33:44:55.3: 12.60 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:55:32.12 +33:44:55.3: 11.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.8771+33.7459,2461186.6757,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.8771+33.7459 20260526.1757 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.94 19:56:50.23 +33:51:17.5
70.01975 2.63478 galactic Cyg Second-epoch detections are separated by 3.3" 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 | ATO J299.1963+33.8565 | 19:56:50.56 +33:51:16.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.459+/-0.036 (G)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:50.23 +33:51:17.5: 13.14 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:50.23 +33:51:17.5: 12.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.1963+33.8565,2461186.6757,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.1963+33.8565 20260526.1757 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.76 19:56:46.48 +33:44:41.1
69.91877 2.58876 galactic Cyg Second-epoch detections are separated by 3.1" and 6.9 pix
The object was found in VSX21" ZTF J195645.67+334459.4
Type: BY
# Max. Min./Amp. JD0 Period
17.867 r Y 0.146 r 2458431.61760 29.625220800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:46.48 +33:44:41.1: 12.67 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:46.48 +33:44:41.1: 11.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 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
ZTF J195645.67+334459.4,2461186.6757,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195645.67+334459.4 20260526.1757 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.22 19:56:26.33 +33:53:30.5
70.00847 2.72464 galactic Cyg Second-epoch detections are separated by 2.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.0957+33.8908 | 19:56:26.32 +33:53:31.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1925AnHar.100....1C HD 226666 J-Ks=0.097+/-0.028 (A)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:26.33 +33:53:30.5: 12.43 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:26.33 +33:53:30.5: 11.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.0957+33.8908,2461186.6757,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.0957+33.8908 20260526.1757 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.75 19:58:28.44 +34:04:49.0
70.38921 2.46227 galactic Cyg Second-epoch detections are separated by 1.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.6116+34.0727 | 19:58:29.48 +34:04:03.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M 1925AnHar.100....1C HD 226880 J-Ks=0.682+/-0.027 (K)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:28.44 +34:04:49.0: 13.48 +/- 0.06 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:28.44 +34:04:49.0: 11.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.09 +/- 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
ATO J299.6116+34.0727,2461186.6757,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6116+34.0727 20260526.1757 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.06 19:56:31.72 +33:48:22.9
69.94498 2.66441 galactic Cyg Second-epoch detections are separated by 1.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.1233+33.8075 | 19:56:31.74 +33:48:22.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.658+/-0.028 (K)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:31.72 +33:48:22.9: 12.47 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:31.72 +33:48:22.9: 11.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.1233+33.8075,2461186.6757,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.1233+33.8075 20260526.1757 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 11.04 19:56:31.92 +33:48:53.1
69.95252 2.66817 galactic Cyg Second-epoch detections are separated by 4.9" and 7.0 pix
The object was found in VSX12" Gaia DR3 2034465367525257216
Type: ROT
# Max. Min./Amp. JD0 Period
13.940 G 13.980 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:31.92 +33:48:53.1: 13.30 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:31.92 +33:48:53.1: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034465367525257216,2461186.6757,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034465367525257216 20260526.1757 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.86 19:57:42.41 +33:57:22.6
70.20035 2.53331 galactic Cyg Second-epoch detections are separated by 1.1" and 6.5 pix
The object was found in VSX 9" Gaia DR3 2034490858112539648
Type: ROT
# Max. Min./Amp. JD0 Period
15.770 G 15.820 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:42.41 +33:57:22.6: 13.49 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:42.41 +33:57:22.6: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034490858112539648,2461186.6757,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034490858112539648 20260526.1757 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.80 19:58:56.67 +34:52:11.8
71.11405 2.79194 galactic Cyg Second-epoch detections are separated by 1.4" and 6.7 pix
The object was found in VSX 3" Gaia DR3 2059324569469845120
Type: L
# Max. Min./Amp. JD0 Period
17.880 G 18.330 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:56.67 +34:52:11.8: 12.41 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:56.67 +34:52:11.8: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2059324569469845120,2461186.6757,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2059324569469845120 20260526.1757 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.88 19:58:35.46 +34:30:30.3
70.76739 2.66513 galactic Cyg Second-epoch detections are separated by 1.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.6369+34.5133 | 19:58:35.44 +34:30:30.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A3 1953ApJ...118...77A LF 3a +34 12 J-Ks=0.160+/-0.028 (F)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:35.46 +34:30:30.3: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:35.46 +34:30:30.3: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6369+34.5133,2461186.6757,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6369+34.5133 20260526.1757 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.10 19:57:08.48 +34:11:39.8
70.34303 2.75712 galactic Cyg Second-epoch detections are separated by 0.3" 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 J299.2861+34.2024 | 19:57:08.51 +34:11:39.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.696+/-0.030 (K)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:08.48 +34:11:39.8: 12.04 +/- 0.01 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:08.48 +34:11:39.8: 11.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.2861+34.2024,2461186.6757,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.2861+34.2024 20260526.1757 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.06 19:56:20.56 +33:50:22.9
69.95349 2.71472 galactic Cyg Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2035216299588045952 | 19:56:20.50 +33:50:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1925AnHar.100....1C HD 226645 J-Ks=0.036+/-0.029 (A)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:20.56 +33:50:22.9: 12.25 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:20.56 +33:50:22.9: 11.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2035216299588045952,2461186.6757,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2035216299588045952 20260526.1757 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.77 19:56:48.79 +33:54:34.5
70.06399 2.66742 galactic Cyg Second-epoch detections are separated by 2.3" and 6.8 pix
The object was found in VSX17" ZTF J195649.57+335448.3
Type: EW
# Max. Min./Amp. JD0 Period
19.382 r Y 0.424 r 2458352.78000 0.411998400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:48.79 +33:54:34.5: 13.33 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:48.79 +33:54:34.5: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 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
ZTF J195649.57+335448.3,2461186.6757,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195649.57+335448.3 20260526.1757 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.76 19:56:55.55 +34:09:46.3
70.29289 2.77886 galactic Cyg Second-epoch detections are separated by 1.0" and 6.4 pix
The object was found in VSX25" V2218 Cyg
Type: M
# Max. Min./Amp. JD0 Period
13.289 r Y 4.712 r 2458541.07160 369.419225000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:55.55 +34:09:46.3: 12.89 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:55.55 +34:09:46.3: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2218 Cyg,2461186.6757,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2218 Cyg 20260526.1757 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.84 19:58:11.01 +34:33:39.6
70.76849 2.76416 galactic Cyg Second-epoch detections are separated by 2.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2059279626951303296 | 19:58:11.01 +34:33:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.483+/-0.029 (K)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:11.01 +34:33:39.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:11.01 +34:33:39.6: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2059279626951303296,2461186.6757,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2059279626951303296 20260526.1757 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 9.91 19:57:09.15 +33:56:11.4
70.12360 2.62123 galactic Cyg Second-epoch detections are separated by 1.4" and 6.7 pix
The object was found in VSX 5" Gaia DR3 2034491515288218752
Type: L
# Max. Min./Amp. JD0 Period
16.460 G 16.610 G M
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:09.15 +33:56:11.4: 12.29 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:09.15 +33:56:11.4: 10.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034491515288218752,2461186.6757,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034491515288218752 20260526.1757 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.75 19:58:27.43 +34:27:15.3
70.70673 2.66039 galactic Cyg Second-epoch detections are separated by 1.6" and 6.5 pix
The object was found in VSX 1" HAT 199-04857
Type: LPV
# Max. Min./Amp. JD0 Period
10.061 Ic 10.133 Ic
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:27.43 +34:27:15.3: 12.84 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:27.43 +34:27:15.3: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 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
HAT 199-04857,2461186.6757,10.75,0.05,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
HAT 199-04857 20260526.1757 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.82 19:57:59.37 +33:42:13.9
70.01527 2.35173 galactic Cyg Second-epoch detections are separated by 2.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.5008+33.7217 | 19:57:59.67 +33:42:54.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1925AnHar.100....1C HD 226828
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:59.37 +33:42:13.9: 13.80 +/- 0.08 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:59.37 +33:42:13.9: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5008+33.7217,2461186.6757,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5008+33.7217 20260526.1757 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.79 19:55:34.11 +33:59:11.3
69.99614 2.92809 galactic Cyg Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J298.8836+33.9933 | 19:55:34.13 +33:59:11.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.929+/-0.028 (M)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:55:34.11 +33:59:11.3: 12.75 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:55:34.11 +33:59:11.3: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.8836+33.9933,2461186.6757,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.8836+33.9933 20260526.1757 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 9.84 19:58:14.16 +34:11:07.6
70.45330 2.55915 galactic Cyg Second-epoch detections are separated by 0.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.5621+34.1931 | 19:58:14.20 +34:11:07.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.982+/-0.030 (M)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:14.16 +34:11:07.6: 11.99 +/- 0.01 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:14.16 +34:11:07.6: 10.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.98 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5621+34.1931,2461186.6757,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5621+34.1931 20260526.1757 9.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.58 19:58:05.76 +33:54:39.0
70.20360 2.44073 galactic Cyg Second-epoch detections are separated by 2.1" and 6.2 pix
The object was found in VSX 3" HAT 199-00777
Type: LPV
# Max. Min./Amp. JD0 Period
8.825 Ic 8.878 Ic
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:05.76 +33:54:39.0: 12.83 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:05.76 +33:54:39.0: 11.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 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
HAT 199-00777,2461186.6757,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00777 20260526.1757 10.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.73 19:57:41.27 +33:43:23.4
69.99906 2.41534 galactic Cyg Second-epoch detections are separated by 1.1" and 6.5 pix
The object was found in VSX 1" Gaia DR3 2034472273833498368
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.620 G 11.660 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:41.27 +33:43:23.4: 13.49 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:41.27 +33:43:23.4: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034472273833498368,2461186.6757,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034472273833498368 20260526.1757 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 11.02 19:57:14.92 +33:44:17.3
69.96433 2.50111 galactic Cyg Second-epoch detections are separated by 2.4" and 6.7 pix
The object was found in VSX23" Gaia DR3 2034460415385066880
Type:
# Max. Min./Amp. JD0 Period
18.140 G 18.990 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:14.92 +33:44:17.3: 13.64 +/- 0.07 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:14.92 +33:44:17.3: 12.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 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 2034460415385066880,2461186.6757,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034460415385066880 20260526.1757 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.80 19:58:36.77 +35:03:28.8
71.23913 2.94807 galactic Cyg Second-epoch detections are separated by 0.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.6677+35.0556 | 19:58:36.81 +35:03:28.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.745+/-0.025 (K)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:36.77 +35:03:28.8: 12.25 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:36.77 +35:03:28.8: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6677+35.0556,2461186.6757,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6677+35.0556 20260526.1757 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 11.13 19:57:40.05 +33:53:32.8
70.14154 2.50705 galactic Cyg Second-epoch detections are separated by 2.4" and 6.7 pix
The object was found in VSX 1" ASASSN-V J195740.15+335332.6
Type: SR
# Max. Min./Amp. JD0 Period
13.620 g Y 0.160 g 2458255.81200 350.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:40.05 +33:53:32.8: 13.74 +/- 0.07 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:40.05 +33:53:32.8: 12.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195740.15+335332.6,2461186.6757,11.13,0.05,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
ASASSN-V J195740.15+335332.6 20260526.1757 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 9.71 19:56:14.16 +33:43:46.0
69.84757 2.67661 galactic Cyg Second-epoch detections are separated by 1.2" and 6.7 pix
The object was found in VSX24" ZTF J195616.02+334353.3
Type: EA
# Max. Min./Amp. JD0 Period
17.342 r Y 0.684 r 2458257.96040 1.254355200000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:14.16 +33:43:46.0: 12.14 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:14.16 +33:43:46.0: 10.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.79 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195616.02+334353.3,2461186.6757,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195616.02+334353.3 20260526.1757 9.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 9.64 19:56:23.89 +33:47:43.2
69.92147 2.68189 galactic Cyg Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2035215848590218496 | 19:56:23.98 +33:47:42.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.050+/-0.031 (M)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:23.89 +33:47:43.2: 12.02 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:23.89 +33:47:43.2: 10.67 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.79 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2035215848590218496,2461186.6757,9.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2035215848590218496 20260526.1757 9.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.74 19:58:02.36 +33:45:28.1
70.06676 2.37100 galactic Cyg Second-epoch detections are separated by 2.4" and 6.5 pix
The object was found in VSX 1" Gaia DR3 2034473781322768768
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.430 G 11.460 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:02.36 +33:45:28.1: 13.83 +/- 0.08 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:02.36 +33:45:28.1: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034473781322768768,2461186.6757,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034473781322768768 20260526.1757 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.54 19:56:33.28 +33:44:05.2
69.88650 2.62270 galactic Cyg Second-epoch detections are separated by 1.1" and 6.6 pix
The object was found in VSX24" Gaia DR3 2034464096214863360
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.570 G 14.600 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:33.28 +33:44:05.2: 13.27 +/- 0.06 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:33.28 +33:44:05.2: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034464096214863360,2461186.6757,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034464096214863360 20260526.1757 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.73 19:57:32.49 +34:21:47.6
70.53046 2.77421 galactic Cyg Second-epoch detections are separated by 1.5" and 6.5 pix
The object was found in VSX 1" Gaia DR3 2035257217715215232
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.460 G 11.500 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:32.49 +34:21:47.6: 12.56 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:32.49 +34:21:47.6: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2035257217715215232,2461186.6757,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2035257217715215232 20260526.1757 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.63 19:58:13.37 +33:46:07.5
70.09601 2.34417 galactic Cyg Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2034473369005907456 | 19:58:13.38 +33:46:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.641+/-0.031 (K)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:13.37 +33:46:07.5: 13.56 +/- 0.06 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:13.37 +33:46:07.5: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034473369005907456,2461186.6757,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034473369005907456 20260526.1757 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.59 19:56:45.15 +33:56:36.1
70.08637 2.69570 galactic Cyg Second-epoch detections are separated by 2.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.1810+33.9385 | 19:56:45.15 +33:56:36.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.171+/-0.028 (F)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:45.15 +33:56:36.1: 12.88 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:45.15 +33:56:36.1: 11.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.1810+33.9385,2461186.6757,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.1810+33.9385 20260526.1757 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.90 19:57:28.89 +33:55:41.0
70.15188 2.55854 galactic Cyg Second-epoch detections are separated by 1.6" 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 | Gaia DR3 2034490381416640384 | 19:57:28.81 +33:55:40.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.281+/-0.035 (F)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:28.89 +33:55:41.0: 13.55 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:28.89 +33:55:41.0: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034490381416640384,2461186.6757,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034490381416640384 20260526.1757 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 9.21 19:56:27.66 +33:45:42.4
69.89951 2.65334 galactic Cyg Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ZTF J195629.37+334526.6 | 19:56:27.77 +33:45:41.5 (Gaia DR3) | SR (local) | 2458330.83480 (local) | Gaia3var=NOT_AVAILABLE J-Ks=1.327+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:27.66 +33:45:42.4: 11.57 +/- 0.01 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:27.66 +33:45:42.4: 10.32 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.43 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195629.37+334526.6,2461186.6757,9.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195629.37+334526.6 20260526.1757 9.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.56 19:58:23.41 +33:53:12.6
70.21497 2.37613 galactic Cyg Second-epoch detections are separated by 2.0" and 6.7 pix
The object was found in VSX 3" Gaia DR3 2034480485795844352
Type: E
# Max. Min./Amp. JD0 Period
16.690 G 16.830 G 0.228530000000 M
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:23.41 +33:53:12.6: 13.21 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:23.41 +33:53:12.6: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034480485795844352,2461186.6757,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034480485795844352 20260526.1757 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.56 19:58:00.94 +34:07:28.6
70.37755 2.56635 galactic Cyg Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.5111+34.1337 | 19:58:00.92 +34:07:29.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.067+/-0.031 (A)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:00.94 +34:07:28.6: 12.76 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:00.94 +34:07:28.6: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5111+34.1337,2461186.6757,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5111+34.1337 20260526.1757 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.43 19:56:26.91 +33:52:04.2
69.98898 2.71050 galactic Cyg Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2035216711904899328 | 19:56:26.86 +33:52:03.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.071+/-0.028 (A)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:26.91 +33:52:04.2: 12.77 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:26.91 +33:52:04.2: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2035216711904899328,2461186.6757,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2035216711904899328 20260526.1757 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 11.12 19:55:52.20 +33:56:55.0
69.99601 2.85501 galactic Cyg Second-epoch detections are separated by 2.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J298.9713+33.9562 | 19:55:52.28 +33:56:54.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.268+/-0.035 (F)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:55:52.20 +33:56:55.0: 13.16 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:55:52.20 +33:56:55.0: 12.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 J298.9713+33.9562,2461186.6757,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.9713+33.9562 20260526.1757 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.44 19:58:11.40 +34:18:42.2
70.55621 2.63310 galactic Cyg Second-epoch detections are separated by 1.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2059271758565171200 | 19:58:11.39 +34:18:41.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.579+/-0.025 (K)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:11.40 +34:18:42.2: 12.58 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:11.40 +34:18:42.2: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2059271758565171200,2461186.6757,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2059271758565171200 20260526.1757 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.37 19:58:02.24 +34:13:27.1
70.46497 2.61440 galactic Cyg Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2035251690120515840 | 19:58:02.30 +34:13:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=10.373+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:02.24 +34:13:27.1: 12.50 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:02.24 +34:13:27.1: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2035251690120515840,2461186.6757,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2035251690120515840 20260526.1757 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.39 19:57:29.27 +34:07:27.1
70.32028 2.65941 galactic Cyg Second-epoch detections are separated by 1.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.3770+34.1128 | 19:57:29.21 +34:07:26.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.268+/-0.028 (F)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:29.27 +34:07:27.1: 12.54 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:29.27 +34:07:27.1: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.3770+34.1128,2461186.6757,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.3770+34.1128 20260526.1757 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.32 19:57:15.53 +34:02:54.3
70.23080 2.66053 galactic Cyg Second-epoch detections are separated by 0.6" and 6.4 pix
The object was found in VSX 1" Gaia DR3 2035242962746431104
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.270 G 11.300 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:15.53 +34:02:54.3: 12.32 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:15.53 +34:02:54.3: 11.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2035242962746431104,2461186.6757,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2035242962746431104 20260526.1757 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1757 2461186.6757 10.90 19:58:20.83 +34:14:03.1
70.50693 2.56496 galactic Cyg Second-epoch detections are separated by 2.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.5985+34.2404 | 19:58:20.83 +34:14:03.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.723+/-0.027 (K)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:20.83 +34:14:03.1: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:20.83 +34:14:03.1: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5985+34.2404,2461186.6757,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5985+34.2404 20260526.1757 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.98596852 27.02.2026 11:39:37.680 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
First image: 2461098.98596852 27.02.2026 11:39:37.680 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
Last image: 2461186.67593835 26.05.2026 04:13:11.073 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.97
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: 5 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): 21534
Objects passed selection criteria: 21436
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 12890.5
Average stars matched: 12608.2 (97.8104 %)
Memory usage VmPeak: 130128 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 23:24:42 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: 2461098.98596852 27.02.2026 11:39:37.680 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
First image: 2461098.98596852 27.02.2026 11:39:37.680 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
Last image: 2461186.67593835 26.05.2026 04:13:11.073 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 242
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
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: 28 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): 187628
Objects passed selection criteria: 186969
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 111077
Average stars matched: 104085 (93.7051 %)
Memory usage VmPeak: 2029548 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 23:31:30 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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat to cache
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.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: 2461186.67544870
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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits exists and is non-empty
Saving wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits to local_wcs_cache/
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits' -> 'local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits'
wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits exists and is non-empty
Saving wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits to local_wcs_cache/
'wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits' -> 'local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits'
wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits exists and is non-empty
Saving wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits to local_wcs_cache/
'wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits' -> 'local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits'
wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits exists and is non-empty
Saving wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits to local_wcs_cache/
'wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits' -> 'local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits (1st reference image)
verification OK: wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
Image size: 941.0'x626.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 19:38:11.590 +38:00:12.09 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits (1st new image)
verification OK: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
Image size: 938.9'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:38:11.903 +38:00:00.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:38:11.590 +38:00:12.09
Second-epoch image center 19:38:11.903 +38:00:00.43
Angular distance between the image centers 0.0034 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits (2nd new image)
verification OK: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
Image size: 938.9'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:38:15.061 +37:59:53.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:38:11.590 +38:00:12.09
Second-epoch image center 19:38:15.061 +37:59:53.21
Angular distance between the image centers 0.0125 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 19:38:11.903 +38:00:00.43
Second-epoch second image center 19:38:15.061 +37:59:53.21
Angular distance between the image centers 0.01056 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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits &> /tmp/tmp.Tz3DoBsPjD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits &> /tmp/tmp.babD8UKt2M
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits &> /tmp/tmp.1ZvSHmt3ED
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits &> /tmp/tmp.msKuCHfMff
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat
The reference image (wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits) and catalog (wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat) found
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat' -> 'wcsmag.cat'
Read 37000 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.0052 to 305.3402 deg, Dec +32.3059 to +43.2769 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 284.0052 to 305.3402 deg, Dec 32.3059 to 43.2769 deg
Loaded 30016 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): 1833 out of 2063 total matches.
Matched with Tycho-2 2063 out of 37000 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.897500
a=0.000000 b=1.000000 c=22.897500
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.93
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.93
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 37000 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.0052 to 305.3402 deg, Dec +32.3059 to +43.2769 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 284.0052 to 305.3402 deg, Dec 32.3059 to 43.2769 deg
Loaded 30016 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): 1833 out of 2063 total matches.
Matched with Tycho-2 2063 out of 37000 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits:
Forced-photometry filter: calibrated wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits -> calib.txt_param_ref_wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits (aperture=6.5)
Read 30221 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.2602 to 305.6003 deg, Dec +31.9282 to +43.3427 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 284.2602 to 305.6003 deg, Dec 31.9282 to 43.3427 deg
Loaded 31531 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): 3431 out of 3757 total matches.
Matched with Tycho-2 3757 out of 30221 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits:
Forced-photometry filter: calibrated wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits -> calib.txt_param_ref_wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
2.1 pix Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
3.0 pix fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
3.0 pix fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
2.4 pix wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
2.1 pix wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
Limiting magnitude estimates:
14.9 mag. Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
14.8 mag. Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
11.3 mag. fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
11.5 mag. fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
All-image limiting magnitude estimate: 11.3 (SNR ) 8.9 (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.Tz3DoBsPjD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4223, passed=37000
Got 37000 stars (including 32754 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat
util/solve_plate_with_UCAC5 got 37000 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 829 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 800 matched stars entering correct_measured_positions(), 765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 798 matched stars entering correct_measured_positions(), 32645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 904 matched stars entering correct_measured_positions(), 32710 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.58"
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 34583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.60"
Excluding outliers - 903 stars left (next iteration limit 877)
WCS_QUALITY_DIAG: file=Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits N_match=903 sigma_overall_arcsec=5.188 sigma_q1_arcsec=3.202 sigma_q2_arcsec=3.014 sigma_q3_arcsec=3.371 sigma_q4_arcsec=3.082 n_q1=194 n_q2=334 n_q3=158 n_q4=217 worst_quadrant_to_overall_ratio=0.650
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits -region wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.babD8UKt2M (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.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-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3244, passed=30221
Got 30221 stars (including 26945 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat
util/solve_plate_with_UCAC5 got 30221 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 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 609 to 668 (Dec 31.9 to 43.3)
Done reading UCAC5 zone files...
Matched 753 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 716 matched stars entering correct_measured_positions(), 678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.03"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 715 matched stars entering correct_measured_positions(), 22395 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.26"
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 609 to 668 (Dec 31.9 to 43.3)
Done reading UCAC5 zone files...
Matched 783 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 751 matched stars entering correct_measured_positions(), 22419 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.21"
Accuracy estimation diagnostic: 750 matched stars entering correct_measured_positions(), 23583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.73"
Excluding outliers - 750 stars left (next iteration limit 786)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits N_match=750 sigma_overall_arcsec=3.492 sigma_q1_arcsec=3.079 sigma_q2_arcsec=2.663 sigma_q3_arcsec=10.589 sigma_q4_arcsec=4.096 n_q1=194 n_q2=281 n_q3=106 n_q4=169 worst_quadrant_to_overall_ratio=3.032
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits -region wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1ZvSHmt3ED (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=66, passed=1350
Got 1350 stars (including 1283 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat
util/solve_plate_with_UCAC5 got 1350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 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 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 1252 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
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 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 1251 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.10"
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 1250 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.14"
Excluding outliers - 918 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits N_match=918 sigma_overall_arcsec=1.091 sigma_q1_arcsec=0.893 sigma_q2_arcsec=1.367 sigma_q3_arcsec=0.705 sigma_q4_arcsec=1.195 n_q1=141 n_q2=486 n_q3=175 n_q4=116 worst_quadrant_to_overall_ratio=1.253
The image catalog is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.msKuCHfMff (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=68, passed=1325
Got 1325 stars (including 1254 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat
util/solve_plate_with_UCAC5 got 1325 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 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 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 1228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
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 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 1229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.10"
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 1230 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.17"
Excluding outliers - 916 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits N_match=916 sigma_overall_arcsec=1.076 sigma_q1_arcsec=0.812 sigma_q2_arcsec=1.419 sigma_q3_arcsec=0.753 sigma_q4_arcsec=1.033 n_q1=155 n_q2=470 n_q3=166 n_q4=125 worst_quadrant_to_overall_ratio=1.319
The image catalog is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits sigma_overall=5.188 worst_q_ratio=0.650
ref2=Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits sigma_overall=3.492 worst_q_ratio=3.032
new1=fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits sigma_overall=1.091 worst_q_ratio=1.253
new2=fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits sigma_overall=1.076 worst_q_ratio=1.319
reference average sigma_overall=4.34 worst_q_ratio=1.841
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281_astrometric_residuals.png (903 matched stars from wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065_astrometric_residuals.png (750 matched stars from wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090_astrometric_residuals.png (918 matched stars from wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091_astrometric_residuals.png (916 matched stars from wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits'
Saving fully-calibrated image wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits'
Preparing the HTML report for the field Cyg-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cyg-05-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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat to cache
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
Creating symlink local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits exists and is non-empty
wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits exists and is non-empty
wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits exists and is non-empty
wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits (1st reference image)
verification OK: wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
Image size: 941.0'x626.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 19:38:11.590 +38:00:12.09 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits (1st new image)
verification OK: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
Image size: 938.9'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:38:11.903 +38:00:00.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:38:11.590 +38:00:12.09
Second-epoch image center 19:38:11.903 +38:00:00.43
Angular distance between the image centers 0.0034 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits (2nd new image)
verification OK: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
Image size: 938.9'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:38:15.061 +37:59:53.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:38:11.590 +38:00:12.09
Second-epoch image center 19:38:15.061 +37:59:53.21
Angular distance between the image centers 0.0125 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 19:38:11.903 +38:00:00.43
Second-epoch second image center 19:38:15.061 +37:59:53.21
Angular distance between the image centers 0.01056 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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits &> /tmp/tmp.NGvpGy08Q7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits &> /tmp/tmp.c7FnHmt0g4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits &> /tmp/tmp.iCIEHVC2wL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits &> /tmp/tmp.JmU92V10VR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat
The reference image (wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits) and catalog (wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat) found
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat' -> 'wcsmag.cat'
Read 259664 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 283.9569 to 305.3402 deg, Dec +32.2935 to +43.2790 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 283.9569 to 305.3402 deg, Dec 32.2935 to 43.2790 deg
Loaded 30092 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): 1240 out of 2270 total matches.
Matched with Tycho-2 2270 out of 259664 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.742550
a=0.000000 b=1.000000 c=22.742550
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.11
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.11
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 259664 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 283.9569 to 305.3402 deg, Dec +32.2935 to +43.2790 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 283.9569 to 305.3402 deg, Dec 32.2935 to 43.2790 deg
Loaded 30092 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): 1240 out of 2270 total matches.
Matched with Tycho-2 2270 out of 259664 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits:
Forced-photometry filter: calibrated wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits -> calib.txt_param_ref_wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits (aperture=4.9)
Read 266283 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.2516 to 305.6124 deg, Dec +31.8798 to +43.3430 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 284.2516 to 305.6124 deg, Dec 31.8798 to 43.3430 deg
Loaded 31739 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): 2867 out of 4510 total matches.
Matched with Tycho-2 4510 out of 266283 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits:
Forced-photometry filter: calibrated wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits -> calib.txt_param_ref_wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 97 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
2.0 pix Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
2.4 pix fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
2.4 pix fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
2.3 pix wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
2.0 pix wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
Limiting magnitude estimates:
15.1 mag. Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
15.0 mag. Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
11.6 mag. fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
11.6 mag. fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
All-image limiting magnitude estimate: 11.6 (SNR ) 11.2 (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.NGvpGy08Q7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.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-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=51110, passed=259613
Got 259613 stars (including 208274 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat
util/solve_plate_with_UCAC5 got 259613 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 816 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 791 matched stars entering correct_measured_positions(), 754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 789 matched stars entering correct_measured_positions(), 235025 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 896 matched stars entering correct_measured_positions(), 235095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.63"
Accuracy estimation diagnostic: 896 matched stars entering correct_measured_positions(), 244751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.53"
Excluding outliers - 896 stars left (next iteration limit 867)
WCS_QUALITY_DIAG: file=Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits N_match=896 sigma_overall_arcsec=5.761 sigma_q1_arcsec=3.363 sigma_q2_arcsec=3.434 sigma_q3_arcsec=3.289 sigma_q4_arcsec=3.428 n_q1=197 n_q2=320 n_q3=160 n_q4=219 worst_quadrant_to_overall_ratio=0.596
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits -region wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.c7FnHmt0g4 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.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-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=44560, passed=266239
Got 266239 stars (including 221330 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat
util/solve_plate_with_UCAC5 got 266239 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 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 609 to 668 (Dec 31.9 to 43.3)
Done reading UCAC5 zone files...
Matched 748 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 713 matched stars entering correct_measured_positions(), 669 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 710 matched stars entering correct_measured_positions(), 206370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.86"
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 609 to 668 (Dec 31.9 to 43.3)
Done reading UCAC5 zone files...
Matched 782 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 746 matched stars entering correct_measured_positions(), 206397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.86"
Accuracy estimation diagnostic: 744 matched stars entering correct_measured_positions(), 215087 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.60"
Excluding outliers - 744 stars left (next iteration limit 781)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits N_match=744 sigma_overall_arcsec=3.161 sigma_q1_arcsec=2.867 sigma_q2_arcsec=2.162 sigma_q3_arcsec=8.685 sigma_q4_arcsec=4.052 n_q1=202 n_q2=299 n_q3=90 n_q4=153 worst_quadrant_to_overall_ratio=2.748
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits -region wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.iCIEHVC2wL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=459, passed=15047
Got 15047 stars (including 14563 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat
util/solve_plate_with_UCAC5 got 15047 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 13750 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 13750 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 13703 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Excluding outliers - 918 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits N_match=918 sigma_overall_arcsec=1.045 sigma_q1_arcsec=0.865 sigma_q2_arcsec=1.383 sigma_q3_arcsec=0.650 sigma_q4_arcsec=0.993 n_q1=157 n_q2=458 n_q3=175 n_q4=128 worst_quadrant_to_overall_ratio=1.324
The image catalog is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JmU92V10VR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=1, blended=450, passed=14663
Got 14663 stars (including 14190 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat
util/solve_plate_with_UCAC5 got 14663 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 13533 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 13529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 13534 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.03"
Excluding outliers - 916 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits N_match=916 sigma_overall_arcsec=1.056 sigma_q1_arcsec=0.838 sigma_q2_arcsec=1.343 sigma_q3_arcsec=0.759 sigma_q4_arcsec=0.993 n_q1=172 n_q2=437 n_q3=170 n_q4=137 worst_quadrant_to_overall_ratio=1.271
The image catalog is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits.cat.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-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-12-28_20.00sec_4.90C_LIGHT_0090.fits
Saving fully-calibrated image wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-05-Q2b1x1_231654_TTUQ2b1x1_1420824_OJ47U8sv/wcs_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091.fits
Preparing the HTML report for the field Cyg-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:56.25 +34:26:59.7: 12.22 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:06.63 +34:56:45.9: 12.71 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:28.79 +34:48:57.9: 11.52 +/- 0.01 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:08.15 +34:03:26.3: 13.90 +/- 0.08 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:25.64 +34:54:26.0: 12.72 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:38.17 +34:43:52.2: 12.48 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:18.94 +34:06:42.1: 12.20 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:57.72 +33:43:08.1: 13.61 +/- 0.06 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:06.63 +34:56:45.9: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:06.63 +34:56:45.9: ref_mag=12.71 +/- 0.02 new_mean_mag=11.0614 delta=1.64 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:28.79 +34:48:57.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:56.25 +34:26:59.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:25.64 +34:54:26.0: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Forced photometry filter KEPT candidate at 19:59:28.79 +34:48:57.9: ref_mag=11.52 +/- 0.01 new_mean_mag=9.7875 delta=1.73 (need > 0.90)
Forced photometry reference-image weighted average: 12.22 +/- 0.02
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry filter KEPT candidate at 19:58:56.25 +34:26:59.7: ref_mag=12.22 +/- 0.02 new_mean_mag=9.9705 delta=2.25 (need > 0.90)
Forced photometry filter KEPT candidate at 19:59:25.64 +34:54:26.0: ref_mag=12.72 +/- 0.02 new_mean_mag=11.0490 delta=1.67 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:08.15 +34:03:26.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:38.17 +34:43:52.2: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.90 +/- 0.08
Forced photometry filter KEPT candidate at 19:59:08.15 +34:03:26.3: ref_mag=13.90 +/- 0.08 new_mean_mag=10.8448 delta=3.05 (need > 0.90)
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:38.17 +34:43:52.2: ref_mag=12.48 +/- 0.02 new_mean_mag=10.5034 delta=1.98 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:18.94 +34:06:42.1: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Forced photometry filter KEPT candidate at 19:56:18.94 +34:06:42.1: ref_mag=11.46 +/- 0.01 new_mean_mag=10.3129 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:57.72 +33:43:08.1: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Forced photometry filter KEPT candidate at 19:56:57.72 +33:43:08.1: ref_mag=12.23 +/- 0.02 new_mean_mag=10.8871 delta=1.34 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:24.76 +34:01:22.9: 13.11 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:24.76 +34:01:22.9: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry filter KEPT candidate at 19:56:24.76 +34:01:22.9: ref_mag=12.16 +/- 0.01 new_mean_mag=10.8458 delta=1.31 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:51.31 +34:21:04.4: 12.56 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:11.92 +33:49:42.1: 14.28 +/- 0.10 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:55:32.12 +33:44:55.3: 12.60 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:46.48 +33:44:41.1: 12.67 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:50.23 +33:51:17.5: 13.14 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:26.33 +33:53:30.5: 12.43 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:51.31 +34:21:04.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:11.92 +33:49:42.1: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Forced photometry filter KEPT candidate at 19:58:51.31 +34:21:04.4: ref_mag=12.56 +/- 0.02 new_mean_mag=10.1912 delta=2.37 (need > 0.90)
Forced photometry reference-image weighted average: 14.28 +/- 0.10
Forced photometry filter KEPT candidate at 19:59:11.92 +33:49:42.1: ref_mag=14.28 +/- 0.10 new_mean_mag=10.8341 delta=3.45 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:55:32.12 +33:44:55.3: 11.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.01
Forced photometry filter KEPT candidate at 19:55:32.12 +33:44:55.3: ref_mag=11.36 +/- 0.01 new_mean_mag=10.2839 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:46.48 +33:44:41.1: 11.97 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:50.23 +33:51:17.5: 12.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry reference-image weighted average: 12.21 +/- 0.02
Forced photometry filter KEPT candidate at 19:56:46.48 +33:44:41.1: ref_mag=12.16 +/- 0.01 new_mean_mag=10.7414 delta=1.41 (need > 0.90)
Forced photometry filter KEPT candidate at 19:56:50.23 +33:51:17.5: ref_mag=12.21 +/- 0.02 new_mean_mag=10.9096 delta=1.30 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:26.33 +33:53:30.5: 11.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.01
Forced photometry filter KEPT candidate at 19:56:26.33 +33:53:30.5: ref_mag=11.36 +/- 0.01 new_mean_mag=10.1952 delta=1.16 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:28.44 +34:04:49.0: 13.48 +/- 0.06 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:28.44 +34:04:49.0: 11.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.02
Forced photometry filter KEPT candidate at 19:58:28.44 +34:04:49.0: ref_mag=12.09 +/- 0.02 new_mean_mag=10.7498 delta=1.34 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:31.92 +33:48:53.1: 13.30 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:31.72 +33:48:22.9: 12.47 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:31.92 +33:48:53.1: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Forced photometry filter KEPT candidate at 19:56:31.92 +33:48:53.1: ref_mag=12.49 +/- 0.02 new_mean_mag=11.0461 delta=1.44 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:31.72 +33:48:22.9: 11.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Forced photometry filter KEPT candidate at 19:56:31.72 +33:48:22.9: ref_mag=11.20 +/- 0.01 new_mean_mag=10.0583 delta=1.14 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:53.94 +34:27:52.9: 13.13 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:53.94 +34:27:52.9: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.13 +/- 0.04
Forced photometry filter KEPT candidate at 19:58:53.94 +34:27:52.9: ref_mag=13.13 +/- 0.04 new_mean_mag=10.8839 delta=2.24 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:59.93 +34:26:56.4: 12.80 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:59.93 +34:26:56.4: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Forced photometry filter KEPT candidate at 19:58:59.93 +34:26:56.4: ref_mag=12.80 +/- 0.03 new_mean_mag=10.8621 delta=1.94 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:25.66 +34:15:35.7: 13.24 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:42.41 +33:57:22.6: 13.49 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:25.66 +34:15:35.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:56.67 +34:52:11.8: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.04
Forced photometry filter KEPT candidate at 19:59:25.66 +34:15:35.7: ref_mag=13.24 +/- 0.04 new_mean_mag=10.7574 delta=2.48 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:42.41 +33:57:22.6: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter KEPT candidate at 19:57:42.41 +33:57:22.6: ref_mag=12.12 +/- 0.01 new_mean_mag=10.8663 delta=1.25 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:56.67 +34:52:11.8: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:56.67 +34:52:11.8: ref_mag=12.22 +/- 0.01 new_mean_mag=10.8053 delta=1.41 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:35.46 +34:30:30.3: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:35.46 +34:30:30.3: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:35.46 +34:30:30.3: ref_mag=12.18 +/- 0.01 new_mean_mag=10.8882 delta=1.30 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:25.66 +34:53:41.7: 12.66 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:25.66 +34:53:41.7: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:25.66 +34:53:41.7: ref_mag=12.66 +/- 0.02 new_mean_mag=10.7966 delta=1.86 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:08.48 +34:11:39.8: 12.04 +/- 0.01 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:08.48 +34:11:39.8: 11.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.01
Forced photometry filter KEPT candidate at 19:57:08.48 +34:11:39.8: ref_mag=11.21 +/- 0.01 new_mean_mag=10.0226 delta=1.19 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:20.56 +33:50:22.9: 12.25 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:48.79 +33:54:34.5: 13.33 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:20.56 +33:50:22.9: 11.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.01
Forced photometry filter KEPT candidate at 19:56:20.56 +33:50:22.9: ref_mag=11.15 +/- 0.01 new_mean_mag=10.0574 delta=1.10 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:48.79 +33:54:34.5: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter KEPT candidate at 19:56:48.79 +33:54:34.5: ref_mag=11.99 +/- 0.01 new_mean_mag=10.7672 delta=1.22 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:41.50 +34:14:16.5: 13.25 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:55.55 +34:09:46.3: 12.89 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:41.50 +34:14:16.5: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.25 +/- 0.04
Forced photometry filter KEPT candidate at 19:58:41.50 +34:14:16.5: ref_mag=13.25 +/- 0.04 new_mean_mag=10.8007 delta=2.45 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:55.55 +34:09:46.3: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry filter KEPT candidate at 19:56:55.55 +34:09:46.3: ref_mag=12.01 +/- 0.01 new_mean_mag=10.7410 delta=1.27 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:11.01 +34:33:39.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:09.15 +33:56:11.4: 12.29 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:11.01 +34:33:39.6: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:11.01 +34:33:39.6: ref_mag=12.11 +/- 0.01 new_mean_mag=10.8336 delta=1.28 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:09.15 +33:56:11.4: 10.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.01
Forced photometry filter KEPT candidate at 19:57:09.15 +33:56:11.4: ref_mag=11.08 +/- 0.01 new_mean_mag=9.9187 delta=1.16 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:42.40 +34:59:25.4: 12.72 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:42.40 +34:59:25.4: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:42.40 +34:59:25.4: ref_mag=12.72 +/- 0.02 new_mean_mag=10.7484 delta=1.98 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:27.43 +34:27:15.3: 12.84 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:27.43 +34:27:15.3: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:27.43 +34:27:15.3: ref_mag=11.99 +/- 0.01 new_mean_mag=10.7535 delta=1.23 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:13.20 +34:50:39.2: 12.58 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:59.37 +33:42:13.9: 13.80 +/- 0.08 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:13.20 +34:50:39.2: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:13.20 +34:50:39.2: ref_mag=12.58 +/- 0.02 new_mean_mag=10.7861 delta=1.80 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:59.37 +33:42:13.9: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Forced photometry filter KEPT candidate at 19:57:59.37 +33:42:13.9: ref_mag=11.89 +/- 0.01 new_mean_mag=10.8238 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:55:34.11 +33:59:11.3: 12.75 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:14.16 +34:11:07.6: 11.99 +/- 0.01 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:40.37 +34:05:53.0: 13.51 +/- 0.06 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:55:34.11 +33:59:11.3: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter KEPT candidate at 19:55:34.11 +33:59:11.3: ref_mag=11.98 +/- 0.01 new_mean_mag=10.7919 delta=1.19 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:14.16 +34:11:07.6: 10.84 +/- 0.01 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:40.37 +34:05:53.0: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 10.98 +/- 0.00
Forced photometry filter KEPT candidate at 19:58:14.16 +34:11:07.6: ref_mag=10.98 +/- 0.00 new_mean_mag=9.8265 delta=1.15 (need > 0.90)
Forced photometry reference-image weighted average: 13.51 +/- 0.06
Forced photometry filter KEPT candidate at 19:58:40.37 +34:05:53.0: ref_mag=13.51 +/- 0.06 new_mean_mag=10.7917 delta=2.71 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:05.76 +33:54:39.0: 12.83 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:41.27 +33:43:23.4: 13.49 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:05.76 +33:54:39.0: 11.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:05.76 +33:54:39.0: ref_mag=12.16 +/- 0.01 new_mean_mag=10.5780 delta=1.58 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:41.27 +33:43:23.4: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Forced photometry filter KEPT candidate at 19:57:41.27 +33:43:23.4: ref_mag=11.89 +/- 0.01 new_mean_mag=10.6666 delta=1.22 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:14.92 +33:44:17.3: 13.64 +/- 0.07 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:36.77 +35:03:28.8: 12.25 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:14.92 +33:44:17.3: 12.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.02
Forced photometry filter KEPT candidate at 19:57:14.92 +33:44:17.3: ref_mag=12.40 +/- 0.02 new_mean_mag=11.0196 delta=1.38 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:36.77 +35:03:28.8: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:36.77 +35:03:28.8: ref_mag=11.98 +/- 0.01 new_mean_mag=10.8046 delta=1.18 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:40.05 +33:53:32.8: 13.74 +/- 0.07 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:40.05 +33:53:32.8: 12.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Forced photometry filter KEPT candidate at 19:57:40.05 +33:53:32.8: ref_mag=12.38 +/- 0.02 new_mean_mag=11.1277 delta=1.25 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:14.16 +33:43:46.0: 12.14 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:14.16 +33:43:46.0: 10.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.79 +/- 0.00
Forced photometry filter KEPT candidate at 19:56:14.16 +33:43:46.0: ref_mag=10.79 +/- 0.00 new_mean_mag=9.7095 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:35.75 +35:03:15.6: 12.43 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:35.75 +35:03:15.6: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.43 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:35.75 +35:03:15.6: ref_mag=12.43 +/- 0.02 new_mean_mag=10.8479 delta=1.59 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:23.89 +33:47:43.2: 12.02 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:38.46 +34:10:15.3: 12.14 +/- 0.01 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:23.89 +33:47:43.2: 10.67 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.79 +/- 0.00
Forced photometry filter KEPT candidate at 19:56:23.89 +33:47:43.2: ref_mag=10.79 +/- 0.00 new_mean_mag=9.6467 delta=1.14 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:38.46 +34:10:15.3: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:38.46 +34:10:15.3: ref_mag=12.14 +/- 0.01 new_mean_mag=9.6791 delta=2.46 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:02.36 +33:45:28.1: 13.83 +/- 0.08 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:02.36 +33:45:28.1: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:02.36 +33:45:28.1: ref_mag=11.75 +/- 0.01 new_mean_mag=10.7410 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:33.28 +33:44:05.2: 13.27 +/- 0.06 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:33.28 +33:44:05.2: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Forced photometry filter KEPT candidate at 19:56:33.28 +33:44:05.2: ref_mag=11.79 +/- 0.01 new_mean_mag=10.5195 delta=1.27 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:59.56 +34:24:14.6: 13.09 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:59.56 +34:24:14.6: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Forced photometry filter KEPT candidate at 19:58:59.56 +34:24:14.6: ref_mag=13.09 +/- 0.03 new_mean_mag=10.7177 delta=2.37 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:32.49 +34:21:47.6: 12.56 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:32.49 +34:21:47.6: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter KEPT candidate at 19:57:32.49 +34:21:47.6: ref_mag=11.98 +/- 0.01 new_mean_mag=10.7378 delta=1.24 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:40.16 +35:12:46.1: 12.37 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:40.16 +35:12:46.1: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.37 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:40.16 +35:12:46.1: ref_mag=12.37 +/- 0.02 new_mean_mag=10.7780 delta=1.60 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:09.84 +35:03:22.3: 12.81 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:09.84 +35:03:22.3: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.81 +/- 0.03
Forced photometry filter KEPT candidate at 19:59:09.84 +35:03:22.3: ref_mag=12.81 +/- 0.03 new_mean_mag=11.1077 delta=1.70 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:54.25 +34:06:17.6: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:54.25 +34:06:17.6: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.29 +/- 0.04
Forced photometry filter KEPT candidate at 19:58:54.25 +34:06:17.6: ref_mag=13.29 +/- 0.04 new_mean_mag=10.6796 delta=2.61 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:13.37 +33:46:07.5: 13.56 +/- 0.06 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:05.64 +34:06:04.0: 13.48 +/- 0.06 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:13.37 +33:46:07.5: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:05.64 +34:06:04.0: 99.00 +/- 99.00 bad_region
Forced photometry filter KEPT candidate at 19:58:13.37 +33:46:07.5: ref_mag=11.66 +/- 0.01 new_mean_mag=10.5683 delta=1.10 (need > 0.90)
Forced photometry reference-image weighted average: 13.48 +/- 0.06
Forced photometry filter KEPT candidate at 19:59:05.64 +34:06:04.0: ref_mag=13.48 +/- 0.06 new_mean_mag=10.5624 delta=2.92 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:05.22 +34:07:27.1: 13.67 +/- 0.07 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:05.22 +34:07:27.1: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.67 +/- 0.07
Forced photometry filter KEPT candidate at 19:59:05.22 +34:07:27.1: ref_mag=13.67 +/- 0.07 new_mean_mag=10.9872 delta=2.69 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:44.97 +34:07:39.4: 13.37 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:44.97 +34:07:39.4: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.37 +/- 0.05
Forced photometry filter KEPT candidate at 19:58:44.97 +34:07:39.4: ref_mag=13.37 +/- 0.05 new_mean_mag=10.9486 delta=2.42 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:45.15 +33:56:36.1: 12.88 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:28.89 +33:55:41.0: 13.55 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:50.24 +34:17:51.7: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:45.15 +33:56:36.1: 11.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry filter KEPT candidate at 19:56:45.15 +33:56:36.1: ref_mag=11.81 +/- 0.01 new_mean_mag=10.5764 delta=1.23 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:28.89 +33:55:41.0: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.02
Forced photometry filter KEPT candidate at 19:57:28.89 +33:55:41.0: ref_mag=12.37 +/- 0.02 new_mean_mag=10.9059 delta=1.47 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:50.24 +34:17:51.7: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.07 +/- 0.04
Forced photometry filter KEPT candidate at 19:58:50.24 +34:17:51.7: ref_mag=13.07 +/- 0.04 new_mean_mag=10.5380 delta=2.53 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:27.66 +33:45:42.4: 11.57 +/- 0.01 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:06.71 +34:08:43.6: 13.88 +/- 0.09 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:23.41 +33:53:12.6: 13.21 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:27.66 +33:45:42.4: 10.32 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.43 +/- 0.00
Forced photometry filter KEPT candidate at 19:56:27.66 +33:45:42.4: ref_mag=10.43 +/- 0.00 new_mean_mag=9.2077 delta=1.22 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:06.71 +34:08:43.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:23.41 +33:53:12.6: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.09
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Forced photometry filter KEPT candidate at 19:59:06.71 +34:08:43.6: ref_mag=13.88 +/- 0.09 new_mean_mag=10.9503 delta=2.93 (need > 0.90)
Forced photometry filter KEPT candidate at 19:58:23.41 +33:53:12.6: ref_mag=11.64 +/- 0.01 new_mean_mag=10.5359 delta=1.10 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:00.94 +34:07:28.6: 12.76 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:16.79 +34:49:04.5: 12.80 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:00.94 +34:07:28.6: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:00.94 +34:07:28.6: ref_mag=11.73 +/- 0.01 new_mean_mag=10.5666 delta=1.16 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:16.79 +34:49:04.5: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:16.79 +34:49:04.5: ref_mag=12.80 +/- 0.02 new_mean_mag=11.0437 delta=1.76 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:26.59 +34:21:37.7: 13.80 +/- 0.07 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:56:26.91 +33:52:04.2: 12.77 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:26.59 +34:21:37.7: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.80 +/- 0.07
Forced photometry filter KEPT candidate at 19:59:26.59 +34:21:37.7: ref_mag=13.80 +/- 0.07 new_mean_mag=10.9863 delta=2.82 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:55:52.20 +33:56:55.0: 13.16 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:56:26.91 +33:52:04.2: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 0.01
Forced photometry filter KEPT candidate at 19:56:26.91 +33:52:04.2: ref_mag=11.65 +/- 0.01 new_mean_mag=10.4146 delta=1.24 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:55:52.20 +33:56:55.0: 12.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.02
Forced photometry filter KEPT candidate at 19:55:52.20 +33:56:55.0: ref_mag=12.30 +/- 0.02 new_mean_mag=11.0945 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:38.35 +33:48:22.0: 13.49 +/- 0.05 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:38.35 +33:48:22.0: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.49 +/- 0.05
Forced photometry filter KEPT candidate at 19:58:38.35 +33:48:22.0: ref_mag=13.49 +/- 0.05 new_mean_mag=10.5110 delta=2.98 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:11.40 +34:18:42.2: 12.58 +/- 0.03 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:11.40 +34:18:42.2: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:11.40 +34:18:42.2: ref_mag=11.55 +/- 0.01 new_mean_mag=10.4359 delta=1.11 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:02.24 +34:13:27.1: 12.50 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:02.24 +34:13:27.1: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:02.24 +34:13:27.1: ref_mag=11.60 +/- 0.01 new_mean_mag=10.3597 delta=1.24 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:29.27 +34:07:27.1: 12.54 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:29.27 +34:07:27.1: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Forced photometry filter KEPT candidate at 19:57:29.27 +34:07:27.1: ref_mag=11.59 +/- 0.01 new_mean_mag=10.3916 delta=1.20 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:57:15.53 +34:02:54.3: 12.32 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:57:15.53 +34:02:54.3: 11.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Forced photometry filter KEPT candidate at 19:57:15.53 +34:02:54.3: ref_mag=11.57 +/- 0.01 new_mean_mag=10.3314 delta=1.24 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:46.84 +35:02:05.2: 12.13 +/- 0.01 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:46.84 +35:02:05.2: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 19:59:46.84 +35:02:05.2: ref_mag=12.13 +/- 0.01 new_mean_mag=10.4534 delta=1.67 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:13.86 +33:44:11.5: 13.67 +/- 0.07 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:58:20.83 +34:14:03.1: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:13.86 +33:44:11.5: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.67 +/- 0.07
Forced photometry filter KEPT candidate at 19:59:13.86 +33:44:11.5: ref_mag=13.67 +/- 0.07 new_mean_mag=11.2678 delta=2.40 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:58:20.83 +34:14:03.1: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter KEPT candidate at 19:58:20.83 +34:14:03.1: ref_mag=12.20 +/- 0.01 new_mean_mag=10.8984 delta=1.30 (need > 0.90)
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits at 19:59:34.82 +35:09:50.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Cyg-05-Q2b1x1_2026-04-18_03-03-53_20.00sec_-4.90C_LIGHTs_0065.fits at 19:59:34.82 +35:09:50.3: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:34.82 +35:09:50.3: ref_mag=12.65 +/- 0.02 new_mean_mag=11.0428 delta=1.61 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out29095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out30373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out36862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out37621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out37942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out37943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out38413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out38414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out39003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out40133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out41246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out42053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out42795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out44376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out44599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out45537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out46772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out47013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out47472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out59477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out60788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out27588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62124.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 55s
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: 21s
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Considering the candidate 66681_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 66681_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:56:18.09 +35:05:01.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 58717_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 58717_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:25.64 +34:54:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 1.487 2059314703923324288 299.85633403337 +34.90716724442 11.5014 10.4456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 27588_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 27588_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 54375_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 54375_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:38.17 +34:43:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.51, MAG_FAINT_SEARCH_LIMIT=11.49)GAIADR2_OUTPUT=# 0.891 2059308008090549120 299.90885288581 +34.73135957472 11.3214 11.0979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56867_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 56867_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:28.79 +34:48:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.79, MAG_FAINT_SEARCH_LIMIT=10.77)GAIADR2_OUTPUT=# 0.316 2059313024612410496 299.86988555343 +34.81601905981 10.2915 9.5368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 47472_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 47472_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:56.25 +34:26:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.97, MAG_FAINT_SEARCH_LIMIT=10.95)GAIADR2_OUTPUT=# 0.755 2059279901823526528 299.73461523771 +34.44984778527 10.7589 10.3928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 36862_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 36862_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:08.15 +34:03:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 2.917 2058502547114700928 299.78478010218 +34.05686639444 11.1773 10.0955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 28452_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 28452_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:40.15 +33:43:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59477_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 59477_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:06.63 +34:56:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 0.352 2059327146465000320 299.77751176272 +34.94611446333 11.7968 11.3247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 37614_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 37614_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 35070_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 35070_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 28759_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 28759_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:57:21.11 +33:45:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39299_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 39299_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:16.18 +34:09:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28927_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 28927_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:16.60 +33:44:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27942_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 27942_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 31023_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 31023_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 28233_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 28233_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 31832_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 31832_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 44376_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 44376_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:51.31 +34:21:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.20, MAG_FAINT_SEARCH_LIMIT=11.18)GAIADR2_OUTPUT=# 0.727 2058522819361374720 299.71399790880 +34.35111358778 10.9219 10.3806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31041_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 31041_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:11.92 +33:49:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 0.895 2034477152916617728 299.79991052069 +33.82850529855 11.5122 10.7434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 28486_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 28486_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:56:50.99 +33:45:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37146_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 37146_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 29734_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 29734_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 29735_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 29735_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 47013_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 47013_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:53.94 +34:27:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 1.287 2059279966232128000 299.72503053610 +34.46496689733 11.7545 11.2064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 46772_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 46772_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:59.93 +34:26:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 0.461 2058529278992651904 299.74957948331 +34.44892829118 11.6759 11.0610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 42053_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 42053_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:25.66 +34:15:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 1.749 2058523540916128512 299.85750279701 +34.25995238485 11.3884 10.4296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33811_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 33811_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 57650_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 57650_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 47990_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 47990_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 58344_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 58344_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:25.66 +34:53:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 1.590 2059314635203847680 299.85646581984 +34.89467492012 11.7014 11.2475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 39687_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 39687_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 30479_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 30479_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 32207_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 32207_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 41246_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 41246_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:41.50 +34:14:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 0.552 2058519623905680000 299.67308392849 +34.23785033179 11.4849 10.7491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 38764_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 38764_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 49254_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 49254_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 33214_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 33214_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 60788_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 60788_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:42.40 +34:59:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.75, MAG_FAINT_SEARCH_LIMIT=11.73)GAIADR2_OUTPUT=# 0.703 2059320927352274048 299.92665085157 +34.99058374687 11.6425 11.2601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 46612_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 46612_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 27641_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 27641_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 57023_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 57023_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:13.20 +34:50:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 0.598 2059312612295603456 299.80494149633 +34.84438117140 11.6643 11.3799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33891_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 33891_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 40015_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 40015_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 37621_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 37621_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:40.37 +34:05:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 1.157 2058514813542097152 299.66859156430 +34.09810608222 11.4829 10.7652 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33335_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 33335_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 28231_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 28231_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 28023_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 28023_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 62124_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 62124_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 32159_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 32159_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 33381_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 33381_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:00.99 +33:55:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27782_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 27782_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 62552_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 62552_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:35.75 +35:03:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 2.363 2059333429980732416 299.89972724486 +35.05451996242 11.7771 11.4125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 29146_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 29146_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:57:27.01 +33:45:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29624_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 29624_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 40133_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 40133_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:38.46 +34:10:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.68, MAG_FAINT_SEARCH_LIMIT=10.66)GAIADR2_OUTPUT=# 1.165 2058516084852438656 299.66060183782 +34.17077538983 10.0637 9.1040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 28885_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 28885_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 27828_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 27828_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 45537_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 45537_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:59.56 +34:24:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 0.422 2058528866675718656 299.74829679219 +34.40410285654 11.5498 11.2903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 43998_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 43998_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 66737_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 66737_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:40.16 +35:12:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.78, MAG_FAINT_SEARCH_LIMIT=11.76)GAIADR2_OUTPUT=# 1.187 2059339722129277824 299.91743640211 +35.21312421955 11.4391 10.8683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 62362_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 62362_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:09.84 +35:03:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 0.517 2059336900314307456 299.79091200019 +35.05631868031 12.0600 11.6443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 37942_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 37942_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:54.25 +34:06:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.68, MAG_FAINT_SEARCH_LIMIT=11.66)GAIADR2_OUTPUT=# 2.596 2058514710462853376 299.72604973954 +34.10416776850 11.2764 10.5156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 29301_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 29301_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 37943_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 37943_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:05.64 +34:06:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.59, MAG_FAINT_SEARCH_LIMIT=11.57)GAIADR2_OUTPUT=# 0.414 2058503303028973312 299.77343735692 +34.10100862061 11.4103 10.9863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 38414_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 38414_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:05.22 +34:07:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.98, MAG_FAINT_SEARCH_LIMIT=11.96)GAIADR2_OUTPUT=# 2.026 2058515152817638656 299.77208377135 +34.12370413418 11.8663 11.0389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 38413_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 38413_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:44.97 +34:07:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 0.634 2058515706895295360 299.68724565105 +34.12747118633 11.3724 10.2996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33260_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 33260_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 33002_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 33002_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 42795_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 42795_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:50.24 +34:17:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 0.179 2058521509369223680 299.70938414674 +34.29766773095 11.4101 11.0659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 30045_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 30045_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:57:51.59 +33:45:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29093_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 29093_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 32370_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 32370_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 39003_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 39003_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:06.71 +34:08:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 2.648 2058515260218656000 299.77882764842 +34.14529200066 11.0629 9.8290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 38093_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 38093_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 56275_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 56275_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:16.79 +34:49:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 1.229 2059312333105656832 299.81966658174 +34.81767325381 11.6181 10.7250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 44599_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 44599_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:26.59 +34:21:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.98, MAG_FAINT_SEARCH_LIMIT=11.96)GAIADR2_OUTPUT=# 1.384 2058525190183660544 299.86125190068 +34.36041411123 11.8867 11.4513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31220_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 31220_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 33012_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 33012_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 50228_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 50228_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:57:43.44 +34:36:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30373_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 30373_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:38.35 +33:48:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.52, MAG_FAINT_SEARCH_LIMIT=11.50)GAIADR2_OUTPUT=# 0.659 2034476358303142912 299.65988768843 +33.80627582553 11.2194 10.7731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 43014_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 43014_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 40749_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 40749_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 37991_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 37991_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 36180_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 36180_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 62050_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 62050_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:46.84 +35:02:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 1.006 2059333193778879232 299.94482523798 +35.03477674275 11.2416 11.0678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.006#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 41041_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 41041_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 29095_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 29095_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:13.86 +33:44:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 1.239 2034428220314294272 299.80789944422 +33.73620669774 12.1469 11.1059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66262_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 66262_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:34.82 +35:09:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 0.086 2059339138013715328 299.89510212134 +35.16399059479 11.7918 11.2783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167449_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 167449_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:50:33.91 +38:43:23.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161330_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 161330_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:55:51.64 +38:29:11.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225711_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 225711_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:43:45.13 +41:46:22.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121289_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 121289_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:55.19 +37:02:33.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 207486_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 207486_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:57:13.91 +40:22:04.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151230_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 151230_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:16:22.50 +38:08:01.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177072_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 177072_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:13:45.81 +39:08:45.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93341_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091
The candidate 93341_fd_Cyg-05-Q2b1x1_2026-05-25_23-13-11_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:07:18.22 +36:06:00.6 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 79s
Prepared the HTML report for the field Cyg-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:56:57.72 +33:43:08.1
19:57:59.37 +33:42:13.9
19:56:14.16 +33:43:46.0
19:56:33.28 +33:44:05.2
19:55:32.12 +33:44:55.3
19:57:14.92 +33:44:17.3
19:57:41.27 +33:43:23.4
19:56:46.48 +33:44:41.1
19:58:02.36 +33:45:28.1
19:56:27.66 +33:45:42.4
19:58:13.37 +33:46:07.5
19:56:23.89 +33:47:43.2
19:56:31.72 +33:48:22.9
19:56:31.92 +33:48:53.1
19:56:20.56 +33:50:22.9
19:56:50.23 +33:51:17.5
19:56:26.91 +33:52:04.2
19:56:26.33 +33:53:30.5
19:57:40.05 +33:53:32.8
19:56:48.79 +33:54:34.5
19:58:23.41 +33:53:12.6
19:57:28.89 +33:55:41.0
19:55:52.20 +33:56:55.0
19:57:09.15 +33:56:11.4
19:56:45.15 +33:56:36.1
19:58:05.76 +33:54:39.0
19:57:42.41 +33:57:22.6
19:55:34.11 +33:59:11.3
19:56:24.76 +34:01:22.9
19:57:15.53 +34:02:54.3
19:58:28.44 +34:04:49.0
19:56:18.94 +34:06:42.1
19:57:29.27 +34:07:27.1
19:58:00.94 +34:07:28.6
19:56:55.55 +34:09:46.3
19:57:08.48 +34:11:39.8
19:58:14.16 +34:11:07.6
19:58:02.24 +34:13:27.1
19:58:20.83 +34:14:03.1
19:58:11.40 +34:18:42.2
19:57:32.49 +34:21:47.6
19:58:27.43 +34:27:15.3
19:58:35.46 +34:30:30.3
19:58:11.01 +34:33:39.6
19:58:56.67 +34:52:11.8
19:58:36.77 +35:03:28.8
########### Completed Cyg-05-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 ####
19:56:57.72 +33:43:08.1
19:56:18.94 +34:06:42.1
19:56:24.76 +34:01:22.9
19:55:32.12 +33:44:55.3
19:56:50.23 +33:51:17.5
19:56:46.48 +33:44:41.1
19:56:26.33 +33:53:30.5
19:58:28.44 +34:04:49.0
19:56:31.72 +33:48:22.9
19:56:31.92 +33:48:53.1
19:57:42.41 +33:57:22.6
19:58:56.67 +34:52:11.8
19:58:35.46 +34:30:30.3
19:57:08.48 +34:11:39.8
19:56:20.56 +33:50:22.9
19:56:48.79 +33:54:34.5
19:56:55.55 +34:09:46.3
19:58:11.01 +34:33:39.6
19:57:09.15 +33:56:11.4
19:58:27.43 +34:27:15.3
19:57:59.37 +33:42:13.9
19:55:34.11 +33:59:11.3
19:58:14.16 +34:11:07.6
19:58:05.76 +33:54:39.0
19:57:41.27 +33:43:23.4
19:57:14.92 +33:44:17.3
19:58:36.77 +35:03:28.8
19:57:40.05 +33:53:32.8
19:56:14.16 +33:43:46.0
19:56:23.89 +33:47:43.2
19:58:02.36 +33:45:28.1
19:56:33.28 +33:44:05.2
19:57:32.49 +34:21:47.6
19:58:13.37 +33:46:07.5
19:56:45.15 +33:56:36.1
19:57:28.89 +33:55:41.0
19:56:27.66 +33:45:42.4
19:58:23.41 +33:53:12.6
19:58:00.94 +34:07:28.6
19:56:26.91 +33:52:04.2
19:55:52.20 +33:56:55.0
19:58:11.40 +34:18:42.2
19:58:02.24 +34:13:27.1
19:57:29.27 +34:07:27.1
19:57:15.53 +34:02:54.3
19:58:20.83 +34:14:03.1
###################################################################################
19:56:57.72 +33:43:08.1 -- not an asteroid (will add it to exclusion list)
19:56:18.94 +34:06:42.1 -- not an asteroid (will add it to exclusion list)
19:56:24.76 +34:01:22.9 -- not an asteroid (will add it to exclusion list)
19:55:32.12 +33:44:55.3 -- not an asteroid (will add it to exclusion list)
19:56:50.23 +33:51:17.5 -- not an asteroid (will add it to exclusion list)
19:56:46.48 +33:44:41.1 -- not an asteroid (will add it to exclusion list)
19:56:26.33 +33:53:30.5 -- not an asteroid (will add it to exclusion list)
19:58:28.44 +34:04:49.0 -- not an asteroid (will add it to exclusion list)
19:56:31.72 +33:48:22.9 -- not an asteroid (will add it to exclusion list)
19:56:31.92 +33:48:53.1 -- not an asteroid (will add it to exclusion list)
19:57:42.41 +33:57:22.6 -- not an asteroid (will add it to exclusion list)
19:58:56.67 +34:52:11.8 -- not an asteroid (will add it to exclusion list)
19:58:35.46 +34:30:30.3 -- not an asteroid (will add it to exclusion list)
19:57:08.48 +34:11:39.8 -- not an asteroid (will add it to exclusion list)
19:56:20.56 +33:50:22.9 -- not an asteroid (will add it to exclusion list)
19:56:48.79 +33:54:34.5 -- not an asteroid (will add it to exclusion list)
19:56:55.55 +34:09:46.3 -- not an asteroid (will add it to exclusion list)
19:58:11.01 +34:33:39.6 -- not an asteroid (will add it to exclusion list)
19:57:09.15 +33:56:11.4 -- not an asteroid (will add it to exclusion list)
19:58:27.43 +34:27:15.3 -- not an asteroid (will add it to exclusion list)
19:57:59.37 +33:42:13.9 -- not an asteroid (will add it to exclusion list)
19:55:34.11 +33:59:11.3 -- not an asteroid (will add it to exclusion list)
19:58:14.16 +34:11:07.6 -- not an asteroid (will add it to exclusion list)
19:58:05.76 +33:54:39.0 -- not an asteroid (will add it to exclusion list)
19:57:41.27 +33:43:23.4 -- not an asteroid (will add it to exclusion list)
19:57:14.92 +33:44:17.3 -- not an asteroid (will add it to exclusion list)
19:58:36.77 +35:03:28.8 -- not an asteroid (will add it to exclusion list)
19:57:40.05 +33:53:32.8 -- not an asteroid (will add it to exclusion list)
19:56:14.16 +33:43:46.0 -- not an asteroid (will add it to exclusion list)
19:56:23.89 +33:47:43.2 -- not an asteroid (will add it to exclusion list)
19:58:02.36 +33:45:28.1 -- not an asteroid (will add it to exclusion list)
19:56:33.28 +33:44:05.2 -- not an asteroid (will add it to exclusion list)
19:57:32.49 +34:21:47.6 -- not an asteroid (will add it to exclusion list)
19:58:13.37 +33:46:07.5 -- not an asteroid (will add it to exclusion list)
19:56:45.15 +33:56:36.1 -- not an asteroid (will add it to exclusion list)
19:57:28.89 +33:55:41.0 -- not an asteroid (will add it to exclusion list)
19:56:27.66 +33:45:42.4 -- not an asteroid (will add it to exclusion list)
19:58:23.41 +33:53:12.6 -- not an asteroid (will add it to exclusion list)
19:58:00.94 +34:07:28.6 -- not an asteroid (will add it to exclusion list)
19:56:26.91 +33:52:04.2 -- not an asteroid (will add it to exclusion list)
19:55:52.20 +33:56:55.0 -- not an asteroid (will add it to exclusion list)
19:58:11.40 +34:18:42.2 -- not an asteroid (will add it to exclusion list)
19:58:02.24 +34:13:27.1 -- not an asteroid (will add it to exclusion list)
19:57:29.27 +34:07:27.1 -- not an asteroid (will add it to exclusion list)
19:57:15.53 +34:02:54.3 -- not an asteroid (will add it to exclusion list)
19:58:20.83 +34:14:03.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:55:32.12 +33:44:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:34.11 +33:59:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:52.20 +33:56:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:14.16 +33:43:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:18.94 +34:06:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:20.56 +33:50:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:23.89 +33:47:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:24.76 +34:01:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:26.33 +33:53:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:26.91 +33:52:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:27.66 +33:45:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:31.72 +33:48:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:31.92 +33:48:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:33.28 +33:44:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:45.15 +33:56:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:46.48 +33:44:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:48.79 +33:54:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:50.23 +33:51:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:55.55 +34:09:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:57.72 +33:43:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:08.48 +34:11:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:09.15 +33:56:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:14.92 +33:44:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:15.53 +34:02:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:28.89 +33:55:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:29.27 +34:07:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:32.49 +34:21:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:40.05 +33:53:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:41.27 +33:43:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:42.41 +33:57:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:59.37 +33:42:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:00.94 +34:07:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:02.24 +34:13:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:02.36 +33:45:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:05.76 +33:54:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:11.01 +34:33:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:11.40 +34:18:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:13.37 +33:46:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:14.16 +34:11:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:20.83 +34:14:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:23.41 +33:53:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:27.43 +34:27:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:28.44 +34:04:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:35.46 +34:30:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:36.77 +35:03:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:56.67 +34:52:11.8 -- 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)
19:55:32.12 +33:44:55.3 -- not a known variable star
19:55:34.11 +33:59:11.3 -- not a known variable star
19:55:52.20 +33:56:55.0 -- not a known variable star
19:56:14.16 +33:43:46.0 -- a known variable star
19:56:18.94 +34:06:42.1 -- a known variable star
19:56:20.56 +33:50:22.9 -- not a known variable star
19:56:23.89 +33:47:43.2 -- not a known variable star
19:56:24.76 +34:01:22.9 -- a known variable star
19:56:26.33 +33:53:30.5 -- not a known variable star
19:56:26.91 +33:52:04.2 -- not a known variable star
19:56:27.66 +33:45:42.4 -- not a known variable star
19:56:31.72 +33:48:22.9 -- not a known variable star
19:56:31.92 +33:48:53.1 -- a known variable star
19:56:33.28 +33:44:05.2 -- a known variable star
19:56:45.15 +33:56:36.1 -- not a known variable star
19:56:46.48 +33:44:41.1 -- a known variable star
19:56:48.79 +33:54:34.5 -- a known variable star
19:56:50.23 +33:51:17.5 -- not a known variable star
19:56:55.55 +34:09:46.3 -- a known variable star
19:56:57.72 +33:43:08.1 -- not a known variable star
19:57:08.48 +34:11:39.8 -- not a known variable star
19:57:09.15 +33:56:11.4 -- a known variable star
19:57:14.92 +33:44:17.3 -- a known variable star
19:57:15.53 +34:02:54.3 -- a known variable star
19:57:28.89 +33:55:41.0 -- not a known variable star
19:57:29.27 +34:07:27.1 -- not a known variable star
19:57:32.49 +34:21:47.6 -- a known variable star
19:57:40.05 +33:53:32.8 -- a known variable star
19:57:41.27 +33:43:23.4 -- a known variable star
19:57:42.41 +33:57:22.6 -- a known variable star
19:57:59.37 +33:42:13.9 -- not a known variable star
19:58:00.94 +34:07:28.6 -- not a known variable star
19:58:02.24 +34:13:27.1 -- not a known variable star
19:58:02.36 +33:45:28.1 -- a known variable star
19:58:05.76 +33:54:39.0 -- a known variable star
19:58:11.01 +34:33:39.6 -- not a known variable star
19:58:11.40 +34:18:42.2 -- not a known variable star
19:58:13.37 +33:46:07.5 -- not a known variable star
19:58:14.16 +34:11:07.6 -- not a known variable star
19:58:20.83 +34:14:03.1 -- not a known variable star
19:58:23.41 +33:53:12.6 -- a known variable star
19:58:27.43 +34:27:15.3 -- a known variable star
19:58:28.44 +34:04:49.0 -- not a known variable star
19:58:35.46 +34:30:30.3 -- not a known variable star
19:58:36.77 +35:03:28.8 -- not a known variable star
19:58:56.67 +34:52:11.8 -- a known variable star
Found 26 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
46 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 46 (excluding asteroids and hot pixels, 26 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461186.67544870 -observatory V36
05:07:08.25 +24:43:05.6 Mercury (-1.1mag)
06:35:51.72 +24:59:01.5 Venus (-3.9mag)
02:12:01.76 +12:33:44.7 Mars (1.3mag)
07:37:58.77 +21:56:26.6 Jupiter (-1.9mag)
00:45:17.86 +02:25:52.0 Saturn (0.9mag)
03:57:04.02 +20:16:18.5 Uranus (5.8mag)
00:15:13.68 +00:11:33.4 Neptune (7.8mag)
20:33:56.28 -23:00:03.6 Pluto (14.5mag)
12:19:34.36 -05:43:56.2 Moon (-11.2mag)
-rw-r--r-- 1 apache apache 363 May 25 23:24 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461186.67544870:
07:37:54.12 +21:56:38.2 Io (5.9mag)
07:38:09.46 +21:55:56.2 Europa (6.1mag)
07:37:51.47 +21:56:51.8 Ganymede (5.5mag)
07:37:37.11 +21:57:19.6 Callisto (6.7mag)
07:39:03.91 +21:32:47.2 Himalia (15.5mag)
07:37:58.66 +21:56:28.5 Thebe (16.5mag)
07:39:22.28 +21:54:02.9 Elara (17.5mag)
07:39:26.53 +22:15:12.1 Pasiphae (17.7mag)
07:45:05.90 +21:57:16.2 Carme (18.8mag)
00:45:19.95 +02:25:32.3 Titan (8.7mag)
00:45:13.84 +02:26:00.1 Rhea (10.0mag)
00:45:40.52 +02:25:58.7 Iapetus (11.4mag)
00:45:32.62 +02:25:54.7 Hyperion (14.7mag)
00:46:15.51 +02:29:39.0 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 25 23:24 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461186.67544870:
17:17:26.23 -33:19:53.9 JWST
16:01:28.43 +52:26:02.6 Chandra
08:15:46.04 -43:56:21.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 25 23:24 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461186.67544870 -observatory V36
13:20:47.36 -27:03:39.9 14.4mag D/1884 O1 (Barnard)
06:37:21.52 +30:40:20.2 15.7mag D/1886 K1 (Brooks)
15:26:18.13 +01:20:56.7 14.6mag D/1895 Q1 (Swift)
05:28:10.01 +24:38:53.7 17.2mag D/1918 W1 (Schorr)
09:31:19.21 +14:33:12.5 17.9mag P/2009 WX51 (Catalina)
18:51:01.27 -31:39:23.8 13.7mag P/2010 H2 (Vales)
05:40:52.62 -68:16:03.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:44:21.18 +31:48:29.7 17.4mag C/2017 K2 (PANSTARRS)
17:19:51.85 +14:32:54.6 17.7mag C/2021 G2 (ATLAS)
23:14:32.88 +31:02:48.2 17.2mag C/2022 E2 (ATLAS)
05:18:00.03 +26:51:28.2 16.4mag C/2022 N2 (PANSTARRS)
09:20:57.53 +31:29:36.9 16.5mag C/2022 QE78 (ATLAS)
08:44:00.90 +03:13:04.9 17.6mag C/2022 R6 (PANSTARRS)
18:36:21.96 +21:12:15.6 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:24:27.17 -11:02:16.4 17.5mag P/2023 B1 (PANSTARRS)
22:16:12.36 +65:39:43.6 17.7mag C/2023 H5 (Lemmon)
18:17:07.05 -05:32:07.5 13.7mag C/2023 R1 (PANSTARRS)
13:39:49.62 +85:48:07.2 17.9mag C/2023 X2 (Lemmon)
06:53:25.55 +63:55:41.8 17.6mag C/2024 A1 (ATLAS)
06:26:52.57 +26:28:50.8 13.1mag C/2024 E1 (Wierzchos)
15:47:53.33 +12:12:30.0 17.3mag C/2024 G6 (ATLAS)
20:19:48.07 +27:10:19.2 14.1mag C/2024 J3 (ATLAS)
04:04:58.54 -17:12:17.2 16.1mag C/2024 T5 (ATLAS)
05:53:39.21 +36:48:58.6 17.9mag C/2025 J1 (Borisov)
11:45:42.11 +53:20:13.6 16.9mag C/2025 L1 (ATLAS)
06:24:54.52 -10:11:16.2 12.6mag C/2025 R3 (PANSTARRS)
12:40:57.28 +04:36:58.7 17.2mag C/2025 Y1 (ATLAS)
01:36:18.18 +42:22:54.1 15.7mag C/2026 B2 (Sun-Gao)
11:10:26.58 -08:59:26.5 16.3mag A/2026 E1
19:59:39.44 -08:07:24.9 9.5mag 10P/Tempel
14:18:45.68 -02:35:19.3 17.6mag 24P/Schaumasse
10:59:43.11 -00:51:55.0 15.9mag 29P/Schwassmann-Wachmann
10:51:18.93 -02:34:28.4 17.8mag 43P/Wolf-Harrington
02:51:26.99 +23:50:06.5 17.6mag 47P/Ashbrook-Jackson
08:32:13.93 +27:22:12.5 16.9mag 63P/Wild
00:14:52.69 -07:19:22.0 15.7mag 65P/Gunn
06:01:37.33 +31:41:03.1 16.5mag 76P/West-Kohoutek-Ikemura
02:37:56.93 +15:23:21.6 13.9mag 78P/Gehrels
00:51:08.21 +01:49:05.2 15.3mag 88P/Howell
04:12:45.04 +28:56:37.7 15.1mag 93P/Lovas
02:07:23.92 +25:21:07.6 17.9mag 114P/Wiseman-Skiff
06:19:58.72 +33:19:28.0 15.7mag 123P/West-Hartley
09:27:56.80 +20:16:19.6 16.4mag 124P/Mrkos
03:37:35.53 +18:17:19.9 16.4mag 128P/Shoemaker-Holt
04:07:33.51 +18:20:52.5 17.7mag 131P/Mueller
04:58:40.24 +19:38:43.1 13.0mag 141P/Machholz
05:01:18.99 +16:22:52.2 12.9mag 141P-A/Machholz
03:46:28.97 +13:43:00.1 10.6mag 141P-D/Machholz
02:48:11.54 -26:39:16.9 17.3mag 161P/Hartley-IRAS
02:59:52.74 +18:13:46.8 14.9mag 162P/SidingSpring
19:34:44.82 -01:42:46.5 17.6mag 169P/NEAT
17:02:21.62 -09:21:34.4 16.2mag 235P/LINEAR
07:05:01.10 +35:51:53.3 17.3mag 240P/NEAT
23:58:32.17 -07:46:23.1 16.7mag 260P/McNaught
03:29:59.20 +29:55:17.0 17.7mag 295P/LINEAR
22:05:10.67 -27:30:54.0 17.7mag 320P/McNaught
15:21:44.98 +08:21:37.2 17.4mag 391P/Kowalski
07:57:12.88 +21:02:19.5 17.8mag 450P/LONEOS
06:38:44.83 +42:35:16.1 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 25 23:24 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
-rw-r--r-- 1 apache apache 5.6K May 25 23:24 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
-rw-r--r-- 1 apache apache 188K May 25 23:24 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:51:00.147 -40:59:30.34 AT 2026myv 2026-05-04.40 19.85
23:01:42.557 -37:41:28.08 AT 2026myu 2026-05-14.36 20.03
17:40:41.796 +55:46:35.59 AT 2026myt 2026-05-13.08 19.76
11:57:21.623 +08:17:50.60 AT 2026mys 2026-05-17.92 20.12
18:08:09.175 +24:46:16.68 AT 2026myr 2026-05-16.11 19.59
19:44:08.720 +05:58:44.85 AT 2026myq 2026-05-18.09 19.96
22:15:03.694 +37:18:03.97 SN 2026myp 2026-05-17.58 17.878
13:28:54.990 -05:49:13.50 AT 2026myo 2026-05-17.76 18.69
13:35:39.060 +60:25:07.59 AT 2026myn 2026-05-17.79 18.94
15:11:37.375 +27:04:22.10 AT 2026mym 2026-05-17.80 19.01
15:45:32.128 +08:10:41.12 AT 2026myl 2026-05-17.84 19.27
16:38:47.743 +40:50:56.52 AT 2026myk 2026-05-17.88 18.14
13:21:16.033 -33:01:10.62 AT 2026myj 2026-05-10.44 20.34
14:04:07.440 +19:21:36.43 AT 2026myi 2026-05-16.96 20.28
12:09:08.262 +13:15:11.92 AT 2026myh 2026-05-05.92 20.33
17:37:21.286 +36:24:32.57 AT 2026myg 2026-05-12.55 19.89
14:40:52.425 +10:22:25.10 AT 2026myf 2026-05-14.32 20.45
21:41:13.013 +64:08:54.76 AT 2026mye 2026-05-17.15 19.242
17:07:33.400 +35:38:40.42 AT 2026myd 2026-05-17.43 20.44
20:38:48.864 -58:53:21.28 AT 2026myc 2026-05-13.27 19.093
-rw-r--r-- 1 apache apache 30K May 25 23:24 tns_transients_list.txt
