This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.39 12:35:56.84 +34:37:38.8
145.86263 81.79931 galactic CVn Second-epoch detections are separated by 1.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:56.84 +34:37:38.8 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.402+/-0.034 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:56.84 +34:37:38.8: 13.58 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:56.84 +34:37:38.8: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.53 12:44:07.66 +34:23:07.2
134.68368 82.57539 galactic CVn Second-epoch detections are separated by 1.9" and 8.2 pix
The object was found in VSX 2" Gaia DR3 1515244159719187712
Type: ROT
# Max. Min./Amp. JD0 Period
13.360 G 13.380 G K
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:44:07.66 +34:23:07.2: 13.62 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:44:07.66 +34:23:07.2: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1515244159719187712,2461290.6252,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1515244159719187712 20260907.1252 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.91 12:40:51.61 +35:04:47.6
138.15637 81.73333 galactic CVn Second-epoch detections are separated by 0.8" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:40:51.61 +35:04:47.6 (user input) | T | P | (position from user input) SpType: F8 1960UppAn...4i...1M [M60b] +35 285 J-Ks=0.472+/-0.029 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:51.61 +35:04:47.6: 12.77 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:51.61 +35:04:47.6: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 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
target,2461290.6252,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.10 12:32:57.33 +37:21:20.1
142.64286 79.05558 galactic CVn Second-epoch detections are separated by 0.1" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:57.33 +37:21:20.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.350+/-0.036 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:57.33 +37:21:20.1: 13.02 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:57.33 +37:21:20.1: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.04 12:39:51.16 +34:18:56.4
141.31282 82.39467 galactic CVn Second-epoch detections are separated by 1.8" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:39:51.16 +34:18:56.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.370+/-0.031 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:51.16 +34:18:56.4: 13.02 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:51.16 +34:18:56.4: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.16 12:32:33.84 +34:57:15.2
149.06359 81.19464 galactic CVn Second-epoch detections are separated by 2.4" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:33.84 +34:57:15.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.334+/-0.028 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:33.84 +34:57:15.2: 13.19 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:33.84 +34:57:15.2: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.15 12:31:28.78 +38:11:55.7
142.39837 78.16466 galactic CVn Second-epoch detections are separated by 0.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:31:28.78 +38:11:55.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.397+/-0.033 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:31:28.78 +38:11:55.7: 13.20 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:31:28.78 +38:11:55.7: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.31 12:44:29.46 +34:30:28.0
133.92097 82.47168 galactic CVn Second-epoch detections are separated by 0.7" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:44:29.46 +34:30:28.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.394+/-0.030 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:44:29.46 +34:30:28.0: 13.26 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:44:29.46 +34:30:28.0: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.23 12:39:01.38 +35:03:59.9
140.65638 81.62998 galactic CVn Second-epoch detections are separated by 1.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:39:01.38 +35:03:59.9 (user input) | T | P | (position from user input) J-Ks=0.683+/-0.035 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:01.38 +35:03:59.9: 13.33 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:01.38 +35:03:59.9: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.20 12:45:15.75 +34:42:52.8
132.44491 82.29919 galactic CVn Second-epoch detections are separated by 6.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:45:15.75 +34:42:52.8 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:45:15.75 +34:42:52.8: 13.32 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:45:15.75 +34:42:52.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.44 12:41:12.93 +33:22:57.0
141.73998 83.36836 galactic CVn Second-epoch detections are separated by 0.7" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:41:12.93 +33:22:57.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.366+/-0.032 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:41:12.93 +33:22:57.0: 13.37 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:41:12.93 +33:22:57.0: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.34 12:33:56.36 +36:19:51.1
143.82310 80.07697 galactic CVn Second-epoch detections are separated by 2.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:33:56.36 +36:19:51.1 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.408+/-0.031 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:56.36 +36:19:51.1: 13.38 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:56.36 +36:19:51.1: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.38 12:29:30.00 +38:16:30.4
143.98115 77.94194 galactic CVn Second-epoch detections are separated by 2.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:29:30.00 +38:16:30.4 (user input) | T | P | (position from user input) J-Ks=0.498+/-0.036 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:30.00 +38:16:30.4: 13.40 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:30.00 +38:16:30.4: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.46 12:39:26.88 +33:44:01.3
143.55581 82.90801 galactic CVn Second-epoch detections are separated by 1.3" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:39:26.88 +33:44:01.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.298+/-0.032 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:26.88 +33:44:01.3: 13.50 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:26.88 +33:44:01.3: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.51 12:34:18.56 +35:26:32.1
145.60232 80.91908 galactic CVn Second-epoch detections are separated by 1.6" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:18.56 +35:26:32.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.333+/-0.029 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:18.56 +35:26:32.1: 13.51 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:18.56 +35:26:32.1: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.39 12:32:31.39 +36:22:20.8
145.22590 79.92301 galactic CVn Second-epoch detections are separated by 1.7" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:31.39 +36:22:20.8 (user input) | T | P | (position from user input) J-Ks=0.399+/-0.033 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:31.39 +36:22:20.8: 13.47 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:31.39 +36:22:20.8: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.33 12:29:43.15 +36:16:16.7
148.34759 79.76111 galactic CVn Second-epoch detections are separated by 3.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:29:43.15 +36:16:16.7 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:43.15 +36:16:16.7: 13.49 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:43.15 +36:16:16.7: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.39 12:38:12.38 +34:18:09.8
143.72616 82.28390 galactic CVn Second-epoch detections are separated by 1.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:38:12.38 +34:18:09.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.392+/-0.033 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:12.38 +34:18:09.8: 13.45 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:12.38 +34:18:09.8: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.40 12:35:05.83 +34:36:50.2
147.00539 81.73605 galactic CVn Second-epoch detections are separated by 0.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:05.83 +34:36:50.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.378+/-0.030 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:05.83 +34:36:50.2: 13.43 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:05.83 +34:36:50.2: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.25 12:33:13.82 +35:46:32.4
145.95460 80.52406 galactic CVn Second-epoch detections are separated by 3.0" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:33:13.82 +35:46:32.4 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.766+/-0.027 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:13.82 +35:46:32.4: 13.42 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:13.82 +35:46:32.4: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.37 12:41:59.87 +33:41:18.3
139.58195 83.13202 galactic CVn Second-epoch detections are separated by 0.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:41:59.87 +33:41:18.3 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.417+/-0.032 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:41:59.87 +33:41:18.3: 13.42 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:41:59.87 +33:41:18.3: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.25 12:39:56.27 +35:09:01.7
139.25618 81.61011 galactic CVn Second-epoch detections are separated by 0.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J189.9838+35.1538 | 12:39:56.27 +35:09:01.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.456+/-0.028 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:56.27 +35:09:01.7: 13.41 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:56.27 +35:09:01.7: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J189.9838+35.1538,2461290.6252,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J189.9838+35.1538 20260907.1252 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.38 12:32:19.80 +34:34:46.4
150.56177 81.49777 galactic CVn Second-epoch detections are separated by 1.0" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:19.80 +34:34:46.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.489+/-0.028 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:19.80 +34:34:46.4: 13.40 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:19.80 +34:34:46.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.47 12:31:38.50 +35:27:29.4
148.59417 80.66174 galactic CVn Second-epoch detections are separated by 2.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:31:38.50 +35:27:29.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:31:38.50 +35:27:29.4: 13.40 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:31:38.50 +35:27:29.4: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.36 12:41:10.62 +35:19:01.8
137.27638 81.52338 galactic CVn Second-epoch detections are separated by 1.7" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:41:10.62 +35:19:01.8 (user input) | T | P | (position from user input) J-Ks=0.321+/-0.027 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:41:10.62 +35:19:01.8: 13.38 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:41:10.62 +35:19:01.8: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.29 12:44:34.61 +33:11:32.1
136.25055 83.75761 galactic CVn Second-epoch detections are separated by 0.7" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:44:34.61 +33:11:32.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.311+/-0.030 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:44:34.61 +33:11:32.1: 13.39 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:44:34.61 +33:11:32.1: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.35 12:38:12.12 +33:51:27.4
145.07135 82.69284 galactic CVn Second-epoch detections are separated by 1.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:38:12.12 +33:51:27.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.528+/-0.033 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:12.12 +33:51:27.4: 13.37 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:12.12 +33:51:27.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.35 12:32:16.98 +36:39:57.6
144.78468 79.63599 galactic CVn Second-epoch detections are separated by 2.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:16.98 +36:39:57.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.415+/-0.032 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:16.98 +36:39:57.6: 13.39 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:16.98 +36:39:57.6: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.34 12:45:45.98 +33:43:15.9
133.08469 83.29501 galactic CVn Second-epoch detections are separated by 1.4" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:45:45.98 +33:43:15.9 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.400+/-0.028 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:45:45.98 +33:43:15.9: 13.38 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:45:45.98 +33:43:15.9: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.22 12:32:15.54 +36:51:37.1
144.37001 79.45678 galactic CVn Second-epoch detections are separated by 1.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:15.54 +36:51:37.1 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.034 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:15.54 +36:51:37.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:15.54 +36:51:37.1: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.21 12:35:24.99 +34:18:44.7
147.53814 82.03538 galactic CVn Second-epoch detections are separated by 2.3" and 8.4 pix
The object was found in VSX 0" Gaia DR3 1517951260425812736
Type: ROT
# Max. Min./Amp. JD0 Period
12.910 G 12.940 G K
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:24.99 +34:18:44.7: 13.36 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:24.99 +34:18:44.7: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1517951260425812736,2461290.6252,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1517951260425812736 20260907.1252 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.19 12:40:05.47 +34:07:16.4
141.46520 82.59427 galactic CVn Second-epoch detections are separated by 1.9" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:40:05.47 +34:07:16.4 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.639+/-0.028 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:05.47 +34:07:16.4: 13.35 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:05.47 +34:07:16.4: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.38 12:32:56.67 +35:49:39.1
146.13592 80.45229 galactic CVn Second-epoch detections are separated by 0.5" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:56.67 +35:49:39.1 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.536+/-0.029 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:56.67 +35:49:39.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:56.67 +35:49:39.1: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.40 12:39:48.21 +36:01:59.2
137.73563 80.75827 galactic CVn Second-epoch detections are separated by 1.1" and 8.1 pix
The object was found in VSX 1" Gaia DR3 1518711881954190080
Type: ROT
# Max. Min./Amp. JD0 Period
12.750 G 12.780 G M
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:48.21 +36:01:59.2: 13.32 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:48.21 +36:01:59.2: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1518711881954190080,2461290.6252,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1518711881954190080 20260907.1252 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.22 12:42:15.28 +34:20:30.1
137.65541 82.52223 galactic CVn Second-epoch detections are separated by 1.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:42:15.28 +34:20:30.1 (user input) | T | P | (position from user input) J-Ks=0.583+/-0.031 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:42:15.28 +34:20:30.1: 13.33 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:42:15.28 +34:20:30.1: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 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
target,2461290.6252,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.36 12:44:55.56 +33:09:48.2
135.65966 83.80314 galactic CVn Second-epoch detections are separated by 1.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:44:55.56 +33:09:48.2 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.293+/-0.029 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:44:55.56 +33:09:48.2: 13.29 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:44:55.56 +33:09:48.2: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 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
target,2461290.6252,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.31 12:34:44.15 +35:35:45.6
144.70394 80.81497 galactic CVn Second-epoch detections are separated by 0.8" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:44.15 +35:35:45.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.371+/-0.028 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:44.15 +35:35:45.6: 13.32 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:44.15 +35:35:45.6: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.40 12:31:06.92 +37:27:58.9
144.16802 78.81043 galactic CVn Second-epoch detections are separated by 1.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:31:06.92 +37:27:58.9 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.627+/-0.034 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:31:06.92 +37:27:58.9: 13.34 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:31:06.92 +37:27:58.9: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.28 12:28:16.38 +36:32:47.4
149.02668 79.37994 galactic CVn Second-epoch detections are separated by 1.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:16.38 +36:32:47.4 (user input) | T | P | (position from user input) J-Ks=0.382+/-0.030 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:16.38 +36:32:47.4: 13.31 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:16.38 +36:32:47.4: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.34 12:32:16.65 +35:08:34.1
148.81577 81.00091 galactic CVn Second-epoch detections are separated by 1.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:16.65 +35:08:34.1 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.376+/-0.028 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:16.65 +35:08:34.1: 13.28 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:16.65 +35:08:34.1: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.36 12:34:40.98 +36:10:11.3
143.38132 80.28371 galactic CVn Second-epoch detections are separated by 2.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:40.98 +36:10:11.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.354+/-0.030 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:40.98 +36:10:11.3: 13.28 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:40.98 +36:10:11.3: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.30 12:38:42.36 +33:22:33.9
145.89774 83.17508 galactic CVn Second-epoch detections are separated by 2.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:38:42.36 +33:22:33.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.268+/-0.033 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:42.36 +33:22:33.9: 13.26 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:42.36 +33:22:33.9: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.34 12:39:49.33 +34:48:58.7
140.14438 81.92003 galactic CVn Second-epoch detections are separated by 4.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:39:49.33 +34:48:58.7 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.567+/-0.028 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:49.33 +34:48:58.7: 13.24 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:49.33 +34:48:58.7: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.23 12:30:21.40 +36:09:38.8
147.99909 79.91913 galactic CVn Second-epoch detections are separated by 0.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:30:21.40 +36:09:38.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.289+/-0.033 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:21.40 +36:09:38.8: 13.23 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:21.40 +36:09:38.8: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.13 12:38:23.40 +35:30:56.4
140.47977 81.16349 galactic CVn Second-epoch detections are separated by 3.0" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:38:23.40 +35:30:56.4 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.486+/-0.033 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:23.40 +35:30:56.4: 13.22 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:23.40 +35:30:56.4: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 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
target,2461290.6252,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.26 12:34:03.07 +37:19:24.1
141.63387 79.16574 galactic CVn Second-epoch detections are separated by 1.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:03.07 +37:19:24.1 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.273+/-0.033 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:03.07 +37:19:24.1: 13.22 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:03.07 +37:19:24.1: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 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
target,2461290.6252,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.19 12:33:04.18 +35:11:19.6
147.76106 81.03572 galactic CVn Second-epoch detections are separated by 2.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:33:04.18 +35:11:19.6 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.418+/-0.030 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:04.18 +35:11:19.6: 13.20 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:04.18 +35:11:19.6: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.18 12:33:10.89 +35:55:23.1
145.62936 80.38650 galactic CVn Second-epoch detections are separated by 1.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:33:10.89 +35:55:23.1 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.479+/-0.028 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:10.89 +35:55:23.1: 13.20 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:10.89 +35:55:23.1: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.19 12:35:22.55 +34:54:08.0
145.79793 81.50066 galactic CVn Second-epoch detections are separated by 0.9" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:22.55 +34:54:08.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.355+/-0.027 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:22.55 +34:54:08.0: 13.20 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:22.55 +34:54:08.0: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.19 12:37:32.27 +35:53:42.3
140.71484 80.74814 galactic CVn Second-epoch detections are separated by 2.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:37:32.27 +35:53:42.3 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.434+/-0.028 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:37:32.27 +35:53:42.3: 13.19 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:37:32.27 +35:53:42.3: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.27 12:32:06.51 +34:48:00.7
150.09149 81.28376 galactic CVn Second-epoch detections are separated by 0.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:06.51 +34:48:00.7 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.320+/-0.030 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:06.51 +34:48:00.7: 13.18 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:06.51 +34:48:00.7: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.24 12:35:32.33 +36:41:18.7
141.34534 79.86465 galactic CVn Second-epoch detections are separated by 1.7" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:32.33 +36:41:18.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.369+/-0.035 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:32.33 +36:41:18.7: 13.18 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:32.33 +36:41:18.7: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.18 12:28:53.25 +37:36:47.3
145.88745 78.49087 galactic CVn Second-epoch detections are separated by 1.5" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:53.25 +37:36:47.3 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.500+/-0.026 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:53.25 +37:36:47.3: 13.16 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:53.25 +37:36:47.3: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.18 12:42:54.61 +34:00:10.7
137.34946 82.88500 galactic CVn Second-epoch detections are separated by 1.2" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:42:54.61 +34:00:10.7 (user input) | T | P | (position from user input) J-Ks=0.501+/-0.035 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:42:54.61 +34:00:10.7: 13.15 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:42:54.61 +34:00:10.7: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.16 12:36:18.49 +34:19:26.1
146.30189 82.10570 galactic CVn Second-epoch detections are separated by 1.2" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:36:18.49 +34:19:26.1 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.320+/-0.035 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:36:18.49 +34:19:26.1: 13.14 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:36:18.49 +34:19:26.1: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.24 12:42:45.87 +34:46:39.6
136.04781 82.12849 galactic CVn Second-epoch detections are separated by 1.0" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:42:45.87 +34:46:39.6 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.033 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:42:45.87 +34:46:39.6: 13.14 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:42:45.87 +34:46:39.6: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.22 12:48:24.99 +33:18:11.1
128.77879 83.79083 galactic CVn Second-epoch detections are separated by 0.8" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:48:24.99 +33:18:11.1 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.391+/-0.027 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:48:24.99 +33:18:11.1: 13.15 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:48:24.99 +33:18:11.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.18 12:40:08.24 +35:08:15.6
139.01618 81.63469 galactic CVn Second-epoch detections are separated by 1.4" and 8.2 pix
The object was found in VSX 1" Gaia DR3 1518343442479826560
Type: ROT
# Max. Min./Amp. JD0 Period
12.930 G 12.950 G G
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:08.24 +35:08:15.6: 13.15 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:08.24 +35:08:15.6: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 1518343442479826560,2461290.6252,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1518343442479826560 20260907.1252 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.12 12:43:02.18 +35:01:01.3
135.24626 81.90936 galactic CVn Second-epoch detections are separated by 2.1" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:43:02.18 +35:01:01.3 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.033 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:43:02.18 +35:01:01.3: 13.13 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:43:02.18 +35:01:01.3: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.20 12:28:16.86 +37:55:02.6
145.76147 78.16486 galactic CVn Second-epoch detections are separated by 1.3" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:16.86 +37:55:02.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.341+/-0.030 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:16.86 +37:55:02.6: 13.15 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:16.86 +37:55:02.6: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.13 12:29:43.68 +36:25:44.7
147.92392 79.62272 galactic CVn Second-epoch detections are separated by 1.6" and 8.1 pix
The object was found in VSX 2" Gaia DR3 1519310875273176704
Type: ROT
# Max. Min./Amp. JD0 Period
12.720 G 12.740 G K
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:43.68 +36:25:44.7: 13.15 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:43.68 +36:25:44.7: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 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 1519310875273176704,2461290.6252,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1519310875273176704 20260907.1252 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.15 12:38:28.87 +33:50:01.9
144.72763 82.73783 galactic CVn Second-epoch detections are separated by 0.9" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:38:28.87 +33:50:01.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.455+/-0.032 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:28.87 +33:50:01.9: 13.13 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:28.87 +33:50:01.9: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.12 12:28:23.00 +37:53:28.7
145.72853 78.19714 galactic CVn Second-epoch detections are separated by 2.7" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:23.00 +37:53:28.7 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.271+/-0.028 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:23.00 +37:53:28.7: 13.12 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:23.00 +37:53:28.7: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.18 12:40:01.14 +33:15:12.0
144.16870 83.39749 galactic CVn Second-epoch detections are separated by 1.0" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:40:01.14 +33:15:12.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.386+/-0.028 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:01.14 +33:15:12.0: 13.11 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:01.14 +33:15:12.0: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.12 12:49:39.45 +33:05:29.8
126.51618 84.02424 galactic CVn Second-epoch detections are separated by 2.9" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:49:39.45 +33:05:29.8 (user input) | T | P | (position from user input) SpType: F5 1960UppAn...4i...1M [M60b] +33 449 J-Ks=0.309+/-0.033 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:49:39.45 +33:05:29.8: 13.10 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:49:39.45 +33:05:29.8: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.12 12:28:38.09 +38:10:00.4
144.93763 77.96983 galactic CVn Second-epoch detections are separated by 2.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:38.09 +38:10:00.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.351+/-0.030 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:38.09 +38:10:00.4: 13.14 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:38.09 +38:10:00.4: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.11 12:34:05.36 +36:28:00.0
143.35703 79.96369 galactic CVn Second-epoch detections are separated by 2.0" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:05.36 +36:28:00.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.345+/-0.031 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:05.36 +36:28:00.0: 13.09 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:05.36 +36:28:00.0: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.13 12:35:25.21 +36:33:38.7
141.73089 79.97574 galactic CVn Second-epoch detections are separated by 1.1" and 7.8 pix
The object was found in VSX 1" ZTF J123525.27+363338.7
Type: EW
# Max. Min./Amp. JD0 Period
12.721 r Y 0.130 r 2458282.69500 0.263949600000
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:25.21 +36:33:38.7: 13.12 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:25.21 +36:33:38.7: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 J123525.27+363338.7,2461290.6252,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J123525.27+363338.7 20260907.1252 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.14 12:36:29.75 +34:45:16.5
144.77956 81.72996 galactic CVn Second-epoch detections are separated by 2.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:36:29.75 +34:45:16.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.319+/-0.025 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:36:29.75 +34:45:16.5: 13.09 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:36:29.75 +34:45:16.5: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.11 12:36:08.72 +35:38:57.9
142.91504 80.87756 galactic CVn Second-epoch detections are separated by 0.6" and 8.1 pix
The object was found in VSX 2" Gaia DR3 1518639245467180032
Type: ROT
# Max. Min./Amp. JD0 Period
12.820 G 12.850 G K
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:36:08.72 +35:38:57.9: 13.09 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:36:08.72 +35:38:57.9: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 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 1518639245467180032,2461290.6252,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1518639245467180032 20260907.1252 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.10 12:30:41.09 +35:22:14.9
149.90487 80.64379 galactic CVn Second-epoch detections are separated by 1.9" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:30:41.09 +35:22:14.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.357+/-0.029 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:41.09 +35:22:14.9: 13.07 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:41.09 +35:22:14.9: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.11 12:30:37.78 +36:10:11.0
147.69631 79.93680 galactic CVn Second-epoch detections are separated by 2.0" and 8.1 pix
The object was found in VSX 3" HAT-185-0001064
Type: VAR
# Max. Min./Amp. JD0 Period
13.248 V 29.889854000000
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:37.78 +36:10:11.0: 13.09 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:37.78 +36:10:11.0: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT-185-0001064,2461290.6252,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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-185-0001064 20260907.1252 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.11 12:45:23.26 +33:15:36.1
134.59301 83.73067 galactic CVn Second-epoch detections are separated by 0.6" and 8.0 pix
The object was found in VSX 1" Gaia DR3 1514926950614889344
Type: E
# Max. Min./Amp. JD0 Period
12.950 G 13.020 G 2.163930000000 F
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:45:23.26 +33:15:36.1: 13.08 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:45:23.26 +33:15:36.1: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1514926950614889344,2461290.6252,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1514926950614889344 20260907.1252 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.07 12:45:34.48 +33:24:06.5
133.97741 83.60023 galactic CVn Second-epoch detections are separated by 1.7" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:45:34.48 +33:24:06.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.555+/-0.027 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:45:34.48 +33:24:06.5: 13.05 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:45:34.48 +33:24:06.5: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.12 12:38:39.24 +34:26:58.9
142.68582 82.18209 galactic CVn Second-epoch detections are separated by 0.8" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:38:39.24 +34:26:58.9 (user input) | T | P | (position from user input) J-Ks=0.603+/-0.031 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:39.24 +34:26:58.9: 13.06 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:39.24 +34:26:58.9: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.96 12:28:47.34 +36:20:38.3
149.07057 79.60736 galactic CVn Second-epoch detections are separated by 0.6" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:47.34 +36:20:38.3 (user input) | T | P | (position from user input) J-Ks=0.704+/-0.025 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:47.34 +36:20:38.3: 13.05 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:47.34 +36:20:38.3: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.81 12:35:55.96 +37:12:24.6
139.95764 79.40365 galactic CVn Second-epoch detections are separated by 0.7" and 7.9 pix
The object was found in VSX 1" SV CVn
Type: RRAB
# Max. Min./Amp. JD0 Period
12.200 V 13.000 V 2439952.76000 0.668062000000 A0
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:55.96 +37:12:24.6: 13.04 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:55.96 +37:12:24.6: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 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
SV CVn,2461290.6252,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SV CVn 20260907.1252 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.04 12:35:29.02 +35:48:01.3
143.33445 80.68702 galactic CVn Second-epoch detections are separated by 0.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:29.02 +35:48:01.3 (user input) | T | P | (position from user input) SpType: F2 1960UppAn...4i...1M [M60b] +36 268 J-Ks=0.294+/-0.028 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:29.02 +35:48:01.3: 13.03 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:29.02 +35:48:01.3: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.04 12:30:38.10 +36:08:45.0
147.75411 79.95848 galactic CVn Second-epoch detections are separated by 2.6" and 7.7 pix
The object was found in VSX 0" Gaia DR3 1519113100619048192
Type: ROT
# Max. Min./Amp. JD0 Period
12.780 G 12.810 G G
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:38.10 +36:08:45.0: 13.03 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:38.10 +36:08:45.0: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1519113100619048192,2461290.6252,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1519113100619048192 20260907.1252 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.11 12:27:47.53 +38:01:36.7
145.94754 78.02417 galactic CVn Second-epoch detections are separated by 2.0" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:27:47.53 +38:01:36.7 (user input) | T | P | (position from user input) SpType: G5V 1960UppAn...4i...1M [M60b] +38 95 J-Ks=0.241+/-0.029 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:27:47.53 +38:01:36.7: 13.03 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:27:47.53 +38:01:36.7: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.10 12:37:52.54 +33:15:28.8
147.64716 83.20699 galactic CVn Second-epoch detections are separated by 0.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:37:52.54 +33:15:28.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.573+/-0.025 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:37:52.54 +33:15:28.8: 13.03 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:37:52.54 +33:15:28.8: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.07 12:45:34.45 +33:06:52.7
134.52863 83.88104 galactic CVn Second-epoch detections are separated by 0.7" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:45:34.45 +33:06:52.7 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:45:34.45 +33:06:52.7: 13.02 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:45:34.45 +33:06:52.7: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.06 12:28:16.22 +37:17:58.8
147.15315 78.71609 galactic CVn Second-epoch detections are separated by 0.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1531787888411280896 | 12:28:16.22 +37:17:58.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G3 (LAMOST DR5) J-Ks=0.355+/-0.030 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:16.22 +37:17:58.8: 13.02 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:16.22 +37:17:58.8: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1531787888411280896,2461290.6252,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1531787888411280896 20260907.1252 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.02 12:28:59.72 +36:14:52.3
149.12902 79.71155 galactic CVn Second-epoch detections are separated by 1.5" and 8.3 pix
The object was found in VSX 1" Gaia DR3 1519302281043213824
Type: ROT
# Max. Min./Amp. JD0 Period
12.650 G 12.670 G K
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:59.72 +36:14:52.3: 12.96 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:59.72 +36:14:52.3: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 1519302281043213824,2461290.6252,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1519302281043213824 20260907.1252 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.98 12:43:32.79 +34:25:12.7
135.52229 82.51418 galactic CVn Second-epoch detections are separated by 1.0" and 7.8 pix
The object was found in VSX 2" Gaia DR3 1515246496181373568
Type: ROT
# Max. Min./Amp. JD0 Period
12.660 G 12.670 G K
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:43:32.79 +34:25:12.7: 12.96 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:43:32.79 +34:25:12.7: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1515246496181373568,2461290.6252,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1515246496181373568 20260907.1252 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.96 12:32:59.33 +35:44:32.1
146.31085 80.53303 galactic CVn Second-epoch detections are separated by 1.2" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:59.33 +35:44:32.1 (user input) | T | P | (position from user input) SpType: G8V 1960UppAn...4i...1M [M60b] +36 236 J-Ks=0.358+/-0.029 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:59.33 +35:44:32.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:59.33 +35:44:32.1: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.03 12:42:30.95 +34:13:49.0
137.48827 82.64412 galactic CVn Second-epoch detections are separated by 1.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:42:30.95 +34:13:49.0 (user input) | T | P | (position from user input) J-Ks=0.515+/-0.033 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:42:30.95 +34:13:49.0: 12.90 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:42:30.95 +34:13:49.0: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.94 12:37:56.53 +34:13:33.3
144.32452 82.33355 galactic CVn Second-epoch detections are separated by 0.8" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:37:56.53 +34:13:33.3 (user input) | T | P | (position from user input) SpType: G0V 1960UppAn...4i...1M [M60b] +34 306 J-Ks=0.283+/-0.030 (F)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:37:56.53 +34:13:33.3: 12.88 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:37:56.53 +34:13:33.3: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.70 12:40:33.37 +34:22:55.5
140.11278 82.37975 galactic CVn Second-epoch detections are separated by 1.6" and 8.1 pix
The object was found in VSX 0" DQ CVn
Type: EW
# Max. Min./Amp. JD0 Period
12.120 w 12.590 w 2453094.61680 0.491421000000 G8V
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:33.37 +34:22:55.5: 12.87 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:33.37 +34:22:55.5: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DQ CVn,2461290.6252,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DQ CVn 20260907.1252 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.92 12:40:21.74 +33:04:30.8
144.18917 83.58953 galactic CVn Second-epoch detections are separated by 0.8" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:40:21.74 +33:04:30.8 (user input) | T | P | (position from user input) J-Ks=0.562+/-0.025 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:21.74 +33:04:30.8: 12.89 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:21.74 +33:04:30.8: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.91 12:29:01.79 +37:35:16.3
145.81571 78.52594 galactic CVn Second-epoch detections are separated by 0.8" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:29:01.79 +37:35:16.3 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.027 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:01.79 +37:35:16.3: 12.87 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:01.79 +37:35:16.3: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.91 12:46:57.15 +33:05:15.7
131.90005 83.96226 galactic CVn Second-epoch detections are separated by 0.7" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J191.7339+33.0876 | 12:46:57.15 +33:05:15.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.441+/-0.025 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:46:57.15 +33:05:15.7: 12.85 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:46:57.15 +33:05:15.7: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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 J191.7339+33.0876,2461290.6252,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J191.7339+33.0876 20260907.1252 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.90 12:32:35.75 +37:15:31.7
143.18737 79.11766 galactic CVn Second-epoch detections are separated by 0.3" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:35.75 +37:15:31.7 (user input) | T | P | (position from user input) SpType: F8 1960UppAn...4i...1M [M60b] +37 251 J-Ks=0.405+/-0.032 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:35.75 +37:15:31.7: 12.85 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:35.75 +37:15:31.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.89 12:33:50.70 +35:33:48.9
145.81765 80.76915 galactic CVn Second-epoch detections are separated by 2.3" and 7.7 pix
The object was found in VSX 1" Gaia DR3 1518274070167976192
Type: ROT
# Max. Min./Amp. JD0 Period
12.590 G 12.620 G G
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:50.70 +35:33:48.9: 12.82 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:50.70 +35:33:48.9: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1518274070167976192,2461290.6252,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1518274070167976192 20260907.1252 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.40 12:29:36.38 +36:22:02.2
148.20563 79.66579 galactic CVn Second-epoch detections are separated by 1.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1519304759239746688 | 12:29:36.32 +36:22:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0V 1960UppAn...4i...1M [M60b] +36 198 J-Ks=0.441+/-0.035 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:36.38 +36:22:02.2: 12.43 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:36.38 +36:22:02.2: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 1519304759239746688,2461290.6252,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1519304759239746688 20260907.1252 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.34 13:38:59.94 +41:09:43.8
91.09967 72.89673 galactic CVn Second-epoch detections are separated by 4.8" 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 1500217443541286144 | 13:39:00.08 +41:09:42.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.445+/-0.030 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 13:38:59.94 +41:09:43.8: 12.35 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 13:38:59.94 +41:09:43.8: 12.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 1500217443541286144,2461290.6252,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1500217443541286144 20260907.1252 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 11.34 12:28:32.31 +36:50:55.3
147.99882 79.14021 galactic CVn Second-epoch detections are separated by 1.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1519381828132869376 | 12:28:32.29 +36:50:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8V 1960UppAn...4i...1M [M60b] +37 210 J-Ks=0.565+/-0.028 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:32.31 +36:50:55.3: 12.29 +/- 0.01 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:32.31 +36:50:55.3: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 1519381828132869376,2461290.6252,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1519381828132869376 20260907.1252 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.59 12:33:36.48 +35:02:57.8
147.53675 81.20994 galactic CVn Second-epoch detections are separated by 3.3" and 7.7 pix
The object was found in VSX 1" Gaia DR3 1518242149971043328
Type: ROT
# Max. Min./Amp. JD0 Period
13.430 G 13.460 G K
The object was not found in astcheck.
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:36.48 +35:02:57.8: 13.81 +/- 0.06 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:36.48 +35:02:57.8: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1518242149971043328,2461290.6252,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1518242149971043328 20260907.1252 12.59CV 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 09 07.1252 2461290.6252 12.62 12:28:56.96 +36:30:58.8
148.45735 79.47189 galactic CVn Second-epoch detections are separated by 1.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:56.96 +36:30:58.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:56.96 +36:30:58.8: 13.83 +/- 0.06 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:56.96 +36:30:58.8: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.40 12:30:00.08 +36:03:14.3
148.65065 79.97936 galactic CVn Second-epoch detections are separated by 1.0" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:30:00.08 +36:03:14.3 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.035 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:00.08 +36:03:14.3: 13.80 +/- 0.06 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:00.08 +36:03:14.3: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.59 12:28:33.87 +37:36:02.8
146.20230 78.47376 galactic CVn Second-epoch detections are separated by 0.8" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:33.87 +37:36:02.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.387+/-0.030 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:33.87 +37:36:02.8: 13.78 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:33.87 +37:36:02.8: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.59CV 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 09 07.1252 2461290.6252 12.45 12:28:17.80 +36:28:25.1
149.19783 79.44584 galactic CVn Second-epoch detections are separated by 1.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:17.80 +36:28:25.1 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.032 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:17.80 +36:28:25.1: 13.75 +/- 0.06 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:17.80 +36:28:25.1: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.58 12:30:35.26 +36:12:10.0
147.65210 79.90356 galactic CVn Second-epoch detections are separated by 1.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:30:35.26 +36:12:10.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.343+/-0.036 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:35.26 +36:12:10.0: 13.72 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:35.26 +36:12:10.0: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.58CV 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 09 07.1252 2461290.6252 12.56 12:36:23.61 +36:47:13.7
140.24145 79.83026 galactic CVn Second-epoch detections are separated by 2.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:36:23.61 +36:47:13.7 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.377+/-0.033 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:36:23.61 +36:47:13.7: 13.71 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:36:23.61 +36:47:13.7: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.56CV 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 09 07.1252 2461290.6252 12.49 12:38:57.16 +33:51:30.6
143.93776 82.75343 galactic CVn Second-epoch detections are separated by 0.9" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:38:57.16 +33:51:30.6 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.437+/-0.034 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:57.16 +33:51:30.6: 13.68 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:57.16 +33:51:30.6: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.57 12:31:06.85 +36:13:53.0
147.03787 79.92651 galactic CVn Second-epoch detections are separated by 1.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:31:06.85 +36:13:53.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:31:06.85 +36:13:53.0: 13.67 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:31:06.85 +36:13:53.0: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.42 12:34:49.36 +34:23:24.2
148.06839 81.91061 galactic CVn Second-epoch detections are separated by 2.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:49.36 +34:23:24.2 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.547+/-0.028 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:49.36 +34:23:24.2: 13.64 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:49.36 +34:23:24.2: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.51 12:29:09.47 +35:48:09.2
150.22513 80.11471 galactic CVn Second-epoch detections are separated by 2.6" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:29:09.47 +35:48:09.2 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.469+/-0.033 (K)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:09.47 +35:48:09.2: 13.61 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:09.47 +35:48:09.2: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.44 12:40:10.19 +35:28:50.8
138.28978 81.30886 galactic CVn Second-epoch detections are separated by 1.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:40:10.19 +35:28:50.8 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.029 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:10.19 +35:28:50.8: 13.63 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:10.19 +35:28:50.8: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.50 12:33:42.26 +34:38:50.9
148.65798 81.57570 galactic CVn Second-epoch detections are separated by 1.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:33:42.26 +34:38:50.9 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:42.26 +34:38:50.9: 13.59 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:42.26 +34:38:50.9: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.48 12:36:30.53 +34:33:08.4
145.34190 81.91574 galactic CVn Second-epoch detections are separated by 0.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:36:30.53 +34:33:08.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.354+/-0.026 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:36:30.53 +34:33:08.4: 13.57 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:36:30.53 +34:33:08.4: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.43 12:28:44.43 +37:13:11.4
146.91290 78.82984 galactic CVn Second-epoch detections are separated by 2.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:44.43 +37:13:11.4 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.349+/-0.029 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:44.43 +37:13:11.4: 13.56 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:44.43 +37:13:11.4: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.48 12:41:48.91 +34:05:26.7
138.89136 82.73692 galactic CVn Second-epoch detections are separated by 1.0" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:41:48.91 +34:05:26.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.401+/-0.039 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:41:48.91 +34:05:26.7: 13.56 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:41:48.91 +34:05:26.7: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1252 2461290.6252 12.45 12:31:30.25 +36:54:35.0
145.00688 79.34951 galactic CVn Second-epoch detections are separated by 2.6" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:31:30.25 +36:54:35.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.357+/-0.033 (G)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:31:30.25 +36:54:35.0: 13.54 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:31:30.25 +36:54:35.0: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6252,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1252 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461178.74973063 18.05.2026 05:59:26.726 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
First image: 2461178.74973063 18.05.2026 05:59:26.726 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
Last image: 2461290.62554344 07.09.2026 03:00:36.953 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 5075
Objects passed selection criteria: 5037
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 2996.25
Average stars matched: 2927.5 (97.7055 %)
Memory usage VmPeak: 237944 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 7 00:09:18 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: 2461178.74973063 18.05.2026 05:59:26.726 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
First image: 2461178.74973063 18.05.2026 05:59:26.726 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
Last image: 2461290.62554344 07.09.2026 03:00:36.953 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 153
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.10
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: 10 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 23134
Objects passed selection criteria: 23044
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 15169
Average stars matched: 14474 (95.4183 %)
Memory usage VmPeak: 247776 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 7 00:10:19 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
SExtractor catalog cache: saved CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.cat to cache
SExtractor catalog cache: saved CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.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/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.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: 2461290.62484846
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_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits exists and is non-empty
wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits exists and is non-empty
wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits exists and is non-empty
wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits (1st reference image)
verification OK: wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
Image size: 937.2'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:05:27.532 +38:00:11.66 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits (1st new image)
verification OK: wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
Image size: 942.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:05:25.865 +38:01:51.99 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:05:27.532 +38:00:11.66
Second-epoch image center 13:05:25.865 +38:01:51.99
Angular distance between the image centers 0.0284 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits (2nd new image)
verification OK: wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
Image size: 942.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:05:28.299 +38:01:17.08 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:05:27.532 +38:00:11.66
Second-epoch image center 13:05:28.299 +38:01:17.08
Angular distance between the image centers 0.0183 deg.
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# 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 13:05:25.865 +38:01:51.99
Second-epoch second image center 13:05:28.299 +38:01:17.08
Angular distance between the image centers 0.01256 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits &> /tmp/tmp.Ju1mua28D3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits &> /tmp/tmp.dnI3PGlqPQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits &> /tmp/tmp.OsLG5VX57E
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits &> /tmp/tmp.SIRPkaOgQV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
Calibrating the magnitude scale
Found non-empty wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.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_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits and wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits and wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat
Found non-empty wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits and wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat
The reference image (wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits) and catalog (wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat) found
'wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat' -> 'wcsmag.cat'
Read 5327 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.7883 to 206.9331 deg, Dec +32.4372 to +43.2598 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 185.7883 to 206.9331 deg, Dec 32.4372 to 43.2598 deg
Loaded 4174 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): 3152 out of 3224 total matches.
Matched with Tycho-2 3224 out of 5327 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.569750
a=0.000000 b=1.000000 c=22.569750
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5327 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.7883 to 206.9331 deg, Dec +32.4372 to +43.2598 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 185.7883 to 206.9331 deg, Dec 32.4372 to 43.2598 deg
Loaded 4174 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): 3152 out of 3224 total matches.
Matched with Tycho-2 3224 out of 5327 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
Forced-photometry filter: calibrated wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits -> calib.txt_param_ref_wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits (aperture=6.5)
Read 5334 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.7738 to 206.9331 deg, Dec +32.4372 to +43.2371 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 185.7738 to 206.9331 deg, Dec 32.4372 to 43.2371 deg
Loaded 4175 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): 3147 out of 3225 total matches.
Matched with Tycho-2 3225 out of 5334 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
Forced-photometry filter: calibrated wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits -> calib.txt_param_ref_wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
2.3 pix CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
2.3 pix fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
2.3 pix fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
Limiting magnitude estimates:
15.2 mag. CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
15.3 mag. CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
12.5 mag. fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
12.4 mag. fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 10.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.Ju1mua28D3 (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/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.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_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits' -> 'wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
WCS_IMAGE_NAME=wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
WCS-calibrated image found: wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
Checking if the catalog wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat corresponding to the image wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits alredy exist and is non-empty...
Catalog wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat corresponding to the image wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
WCS catalog name: wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=282, bad_region=0, passed=5327
Got 5327 stars (including 5041 good ones) from the SExtractor catalog wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat
util/solve_plate_with_UCAC5 got 5327 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 4853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 5327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 5327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 5327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4853 stars left (next iteration limit 5338)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits N_match=4853 sigma_overall_arcsec=0.332 sigma_q1_arcsec=0.261 sigma_q2_arcsec=0.403 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.396 n_q1=1187 n_q2=1273 n_q3=1179 n_q4=1214 worst_quadrant_to_overall_ratio=1.214
The image catalog is written to wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits -region wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.dnI3PGlqPQ (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/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.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_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits' -> 'wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
WCS_IMAGE_NAME=wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
WCS-calibrated image found: wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
Checking if the catalog wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat corresponding to the image wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits alredy exist and is non-empty...
Catalog wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat corresponding to the image wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
WCS catalog name: wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=279, bad_region=0, passed=5334
Got 5334 stars (including 5050 good ones) from the SExtractor catalog wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat
util/solve_plate_with_UCAC5 got 5334 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 4862 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 4855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 5334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 4862 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 5334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 5334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4855 stars left (next iteration limit 5340)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits N_match=4855 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.290 sigma_q2_arcsec=0.426 sigma_q3_arcsec=0.331 sigma_q4_arcsec=0.389 n_q1=1176 n_q2=1274 n_q3=1179 n_q4=1226 worst_quadrant_to_overall_ratio=1.220
The image catalog is written to wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits -region wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.OsLG5VX57E (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
WCS_IMAGE_NAME=wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
WCS-calibrated image found: wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
Checking if the catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat corresponding to the image wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat corresponding to the image wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
WCS catalog name: wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=44, bad_region=0, passed=662
Got 662 stars (including 615 good ones) from the SExtractor catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 662 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.4'
Seting catalog search parameters based on the expected field of view 942.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013089 (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 0.010471 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 669 (Dec 32.3 to 43.4)
Done reading UCAC5 zone files...
Matched 593 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 592 matched stars entering correct_measured_positions(), 502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 592 matched stars entering correct_measured_positions(), 558 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 669 (Dec 32.3 to 43.4)
Done reading UCAC5 zone files...
Matched 593 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 592 matched stars entering correct_measured_positions(), 555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 592 matched stars entering correct_measured_positions(), 555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 592 stars left (next iteration limit 651)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=592 robust_rms=5.468 arcsec worst_quadrant_rms=56.827 arcsec
SIP_REFIT: SIP order 3 trial: matched=592 robust_rms=0.638 arcsec worst_quadrant_rms=0.819 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=592 robust_rms_before=0.957 arcsec robust_rms_before_corrected=0.503 arcsec robust_rms_after=0.638 arcsec worst_quadrant_rms_before=0.555 worst_quadrant_rms_after=0.819
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.555 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits N_match=592 sigma_overall_arcsec=0.522 sigma_q1_arcsec=0.536 sigma_q2_arcsec=0.599 sigma_q3_arcsec=0.435 sigma_q4_arcsec=0.490 n_q1=94 n_q2=131 n_q3=70 n_q4=297 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits -region wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.SIRPkaOgQV (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
WCS_IMAGE_NAME=wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
WCS-calibrated image found: wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
Checking if the catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat corresponding to the image wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat corresponding to the image wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
WCS catalog name: wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=50, bad_region=0, passed=725
Got 725 stars (including 674 good ones) from the SExtractor catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat
util/solve_plate_with_UCAC5 got 725 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (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 0.010472 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 669 (Dec 32.3 to 43.4)
Done reading UCAC5 zone files...
Matched 653 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 651 matched stars entering correct_measured_positions(), 564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 651 matched stars entering correct_measured_positions(), 626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 669 (Dec 32.3 to 43.4)
Done reading UCAC5 zone files...
Matched 653 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 651 matched stars entering correct_measured_positions(), 629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 651 matched stars entering correct_measured_positions(), 629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 651 stars left (next iteration limit 716)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=651 robust_rms=5.685 arcsec worst_quadrant_rms=48.326 arcsec
SIP_REFIT: SIP order 3 trial: matched=651 robust_rms=0.658 arcsec worst_quadrant_rms=0.836 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=651 robust_rms_before=0.995 arcsec robust_rms_before_corrected=0.521 arcsec robust_rms_after=0.658 arcsec worst_quadrant_rms_before=0.580 worst_quadrant_rms_after=0.836
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.580 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits N_match=651 sigma_overall_arcsec=0.558 sigma_q1_arcsec=0.559 sigma_q2_arcsec=0.585 sigma_q3_arcsec=0.460 sigma_q4_arcsec=0.542 n_q1=112 n_q2=142 n_q3=84 n_q4=313 worst_quadrant_to_overall_ratio=1.049
The image catalog is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits -region wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits to local_wcs_cache/
'wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits' -> 'local_wcs_cache/wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits'
Saving the final (post-refit) wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits to local_wcs_cache/
'wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits' -> 'local_wcs_cache/wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits'
Saving the final (post-refit) wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits to local_wcs_cache/
'wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits' -> 'local_wcs_cache/wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits'
Saving the final (post-refit) wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits to local_wcs_cache/
'wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits' -> 'local_wcs_cache/wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits sigma_overall=0.332 worst_q_ratio=1.214
ref2=CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits sigma_overall=0.349 worst_q_ratio=1.220
new1=fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits sigma_overall=0.522 worst_q_ratio=1.149
new2=fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits sigma_overall=0.558 worst_q_ratio=1.049
reference average sigma_overall=0.3405 worst_q_ratio=1.217
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576_astrometric_residuals.png (4853 matched stars from wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577_astrometric_residuals.png (4855 matched stars from wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070_astrometric_residuals.png (592 matched stars from wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071_astrometric_residuals.png (651 matched stars from wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits'
Saving fully-calibrated image wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits'
Preparing the HTML report for the field CVn-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field CVn-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
SExtractor catalog cache: saved CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.cat to cache
SExtractor catalog cache: saved CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
Creating symlink local_wcs_cache/wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
Creating symlink local_wcs_cache/wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
Creating symlink local_wcs_cache/wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits exists and is non-empty
wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits exists and is non-empty
wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits exists and is non-empty
wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits (1st reference image)
verification OK: wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
Image size: 937.2'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:05:27.532 +38:00:11.66 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits (1st new image)
verification OK: wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
Image size: 942.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:05:25.865 +38:01:51.99 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:05:27.532 +38:00:11.66
Second-epoch image center 13:05:25.865 +38:01:51.99
Angular distance between the image centers 0.0284 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits (2nd new image)
verification OK: wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
Image size: 942.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:05:28.299 +38:01:17.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:05:27.532 +38:00:11.66
Second-epoch image center 13:05:28.299 +38:01:17.08
Angular distance between the image centers 0.0183 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 13:05:25.865 +38:01:51.99
Second-epoch second image center 13:05:28.299 +38:01:17.08
Angular distance between the image centers 0.01256 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits &> /tmp/tmp.5WPkn1Et4W
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits &> /tmp/tmp.BlBYzr1EuW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits &> /tmp/tmp.grqr0IApzD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits &> /tmp/tmp.kSQ8pm5H4t
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
Calibrating the magnitude scale
Found non-empty wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.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_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits and wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits and wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat
Found non-empty wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits and wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat
The reference image (wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits) and catalog (wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat) found
'wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat' -> 'wcsmag.cat'
Read 24753 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.7834 to 207.0346 deg, Dec +32.4158 to +43.2598 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 185.7834 to 207.0346 deg, Dec 32.4158 to 43.2598 deg
Loaded 4212 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): 3071 out of 3252 total matches.
Matched with Tycho-2 3252 out of 24753 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.470800
a=0.000000 b=1.000000 c=22.470800
From vast_summary.log: estimated ref. image limiting mag.: -7.10
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 24753 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.7834 to 207.0346 deg, Dec +32.4158 to +43.2598 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 185.7834 to 207.0346 deg, Dec 32.4158 to 43.2598 deg
Loaded 4212 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): 3071 out of 3252 total matches.
Matched with Tycho-2 3252 out of 24753 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
Forced-photometry filter: calibrated wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits -> calib.txt_param_ref_wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits (aperture=5.2)
Read 25058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.7738 to 206.9742 deg, Dec +32.4156 to +43.2593 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 185.7738 to 206.9742 deg, Dec 32.4156 to 43.2593 deg
Loaded 4197 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): 3077 out of 3256 total matches.
Matched with Tycho-2 3256 out of 25058 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
Forced-photometry filter: calibrated wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits -> calib.txt_param_ref_wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits (aperture=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 142 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
2.2 pix CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
2.1 pix fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
2.1 pix fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
Limiting magnitude estimates:
15.4 mag. CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
15.4 mag. CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
12.4 mag. fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
12.6 mag. fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 12.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5WPkn1Et4W (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/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.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_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits' -> 'wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
WCS_IMAGE_NAME=wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
WCS-calibrated image found: wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
Checking if the catalog wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat corresponding to the image wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits alredy exist and is non-empty...
Catalog wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat corresponding to the image wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits
WCS catalog name: wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=952, bad_region=0, passed=24744
Got 24744 stars (including 23759 good ones) from the SExtractor catalog wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat
util/solve_plate_with_UCAC5 got 24744 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 4844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 24744 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 24744 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 24744 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4844 stars left (next iteration limit 5328)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits N_match=4844 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.256 sigma_q2_arcsec=0.390 sigma_q3_arcsec=0.297 sigma_q4_arcsec=0.382 n_q1=1207 n_q2=1230 n_q3=1218 n_q4=1189 worst_quadrant_to_overall_ratio=1.195
The image catalog is written to wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits -region wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.BlBYzr1EuW (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/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.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_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits' -> 'wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
WCS_IMAGE_NAME=wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
WCS-calibrated image found: wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
Checking if the catalog wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat corresponding to the image wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits alredy exist and is non-empty...
Catalog wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat corresponding to the image wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits
WCS catalog name: wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=935, bad_region=0, passed=25050
Got 25050 stars (including 24081 good ones) from the SExtractor catalog wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat
util/solve_plate_with_UCAC5 got 25050 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4854 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 4848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 25050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4855 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 25050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 25050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4849 stars left (next iteration limit 5332)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits N_match=4849 sigma_overall_arcsec=0.345 sigma_q1_arcsec=0.291 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.335 sigma_q4_arcsec=0.385 n_q1=1212 n_q2=1236 n_q3=1214 n_q4=1187 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits -region wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.grqr0IApzD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
WCS_IMAGE_NAME=wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
WCS-calibrated image found: wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
Checking if the catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat corresponding to the image wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat corresponding to the image wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
WCS catalog name: wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=391, bad_region=3, passed=5601
Got 5601 stars (including 5192 good ones) from the SExtractor catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 5601 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.4'
Seting catalog search parameters based on the expected field of view 942.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013089 (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 0.010471 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4726 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4719 matched stars entering correct_measured_positions(), 4719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4719 matched stars entering correct_measured_positions(), 5601 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4727 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4720 matched stars entering correct_measured_positions(), 5601 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Accuracy estimation diagnostic: 4720 matched stars entering correct_measured_positions(), 5601 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 4720 stars left (next iteration limit 5190)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4720 robust_rms=6.305 arcsec worst_quadrant_rms=24.624 arcsec
SIP_REFIT: SIP order 3 trial: matched=4720 robust_rms=0.978 arcsec worst_quadrant_rms=1.039 arcsec
SIP_REFIT: SIP order 5 trial: matched=4720 robust_rms=0.845 arcsec worst_quadrant_rms=0.865 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4720 robust_rms_before=1.270 arcsec robust_rms_before_corrected=0.827 arcsec robust_rms_after=0.845 arcsec worst_quadrant_rms_before=0.838 worst_quadrant_rms_after=0.865
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.838 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits N_match=4720 sigma_overall_arcsec=0.788 sigma_q1_arcsec=0.802 sigma_q2_arcsec=0.822 sigma_q3_arcsec=0.797 sigma_q4_arcsec=0.761 n_q1=975 n_q2=1224 n_q3=599 n_q4=1922 worst_quadrant_to_overall_ratio=1.043
The image catalog is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits -region wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.kSQ8pm5H4t (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
WCS_IMAGE_NAME=wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
WCS-calibrated image found: wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
Checking if the catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat corresponding to the image wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat corresponding to the image wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
WCS catalog name: wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=229, bad_region=4, passed=5773
Got 5773 stars (including 5528 good ones) from the SExtractor catalog wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat
util/solve_plate_with_UCAC5 got 5773 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (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 0.010472 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4713 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4705 matched stars entering correct_measured_positions(), 4704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4705 matched stars entering correct_measured_positions(), 5772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4714 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4706 matched stars entering correct_measured_positions(), 5773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Accuracy estimation diagnostic: 4706 matched stars entering correct_measured_positions(), 5773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 4706 stars left (next iteration limit 5175)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4706 robust_rms=6.600 arcsec worst_quadrant_rms=26.240 arcsec
SIP_REFIT: SIP order 3 trial: matched=4706 robust_rms=0.949 arcsec worst_quadrant_rms=0.988 arcsec
SIP_REFIT: SIP order 5 trial: matched=4706 robust_rms=0.829 arcsec worst_quadrant_rms=0.858 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4706 robust_rms_before=1.270 arcsec robust_rms_before_corrected=0.814 arcsec robust_rms_after=0.829 arcsec worst_quadrant_rms_before=0.857 worst_quadrant_rms_after=0.858
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.857 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits N_match=4706 sigma_overall_arcsec=0.773 sigma_q1_arcsec=0.742 sigma_q2_arcsec=0.784 sigma_q3_arcsec=0.827 sigma_q4_arcsec=0.756 n_q1=963 n_q2=1216 n_q3=647 n_q4=1880 worst_quadrant_to_overall_ratio=1.070
The image catalog is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits -region wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/wcs_fd_CVn-02-Q1b1x1_2026-09-06_21-59-36_20.00sec_-0.00C_LIGHTs_0070.fits
Saving fully-calibrated image wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_CVn-02-Q1b1x1_220246_TTUQ1b1x1_4106687_3ftb39RF/wcs_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071.fits
Preparing the HTML report for the field CVn-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:03.33 +36:56:06.4: 13.14 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:51:47.65 +36:23:05.9: 12.46 +/- 0.01 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:56.84 +34:37:38.8: 13.58 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:51.61 +35:04:47.6: 12.77 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:44:07.66 +34:23:07.2: 13.62 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:51.16 +34:18:56.4: 13.02 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:31:28.78 +38:11:55.7: 13.20 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:57.33 +37:21:20.1: 13.02 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:33.84 +34:57:15.2: 13.19 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:44:29.46 +34:30:28.0: 13.26 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:51:47.65 +36:23:05.9: 12.46 +/- 0.01 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:56.84 +34:37:38.8: 13.59 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:03.33 +36:56:06.4: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter REJECTED candidate at 12:30:03.33 +36:56:06.4: ref_mag=13.16 +/- 0.02 new_mean_mag=12.3261 delta=0.84 (need > 0.90)
Forced photometry filter REJECTED candidate at 12:51:47.65 +36:23:05.9: ref_mag=12.46 +/- 0.01 new_mean_mag=12.3235 delta=0.14 (need > 0.90)
Forced photometry filter KEPT candidate at 12:35:56.84 +34:37:38.8: ref_mag=13.59 +/- 0.03 new_mean_mag=12.3935 delta=1.19 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:51.61 +35:04:47.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:51.16 +34:18:56.4: 13.06 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:44:07.66 +34:23:07.2: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 12:40:51.61 +35:04:47.6: ref_mag=12.81 +/- 0.01 new_mean_mag=11.9090 delta=0.90 (need > 0.90)
Forced photometry filter KEPT candidate at 12:39:51.16 +34:18:56.4: ref_mag=13.04 +/- 0.02 new_mean_mag=12.0360 delta=1.00 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:31:28.78 +38:11:55.7: 13.26 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:57.33 +37:21:20.1: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 12:44:07.66 +34:23:07.2: ref_mag=13.62 +/- 0.03 new_mean_mag=12.5103 delta=1.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 12:31:28.78 +38:11:55.7: ref_mag=13.23 +/- 0.02 new_mean_mag=12.1552 delta=1.07 (need > 0.90)
Forced photometry filter KEPT candidate at 12:32:57.33 +37:21:20.1: ref_mag=13.02 +/- 0.02 new_mean_mag=12.0927 delta=0.92 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:33.84 +34:57:15.2: 13.10 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:44:29.46 +34:30:28.0: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 12:32:33.84 +34:57:15.2: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1669 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 12:44:29.46 +34:30:28.0: ref_mag=13.22 +/- 0.02 new_mean_mag=12.3114 delta=0.91 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:01.38 +35:03:59.9: 13.33 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:45:15.75 +34:42:52.8: 13.32 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:01.38 +35:03:59.9: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 12:39:01.38 +35:03:59.9: ref_mag=13.34 +/- 0.02 new_mean_mag=12.2257 delta=1.11 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:45:15.75 +34:42:52.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 12:45:15.75 +34:42:52.8: ref_mag=13.34 +/- 0.02 new_mean_mag=12.1098 delta=1.23 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:41:12.93 +33:22:57.0: 13.37 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:41:12.93 +33:22:57.0: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 12:41:12.93 +33:22:57.0: ref_mag=13.38 +/- 0.03 new_mean_mag=12.4331 delta=0.94 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:56.36 +36:19:51.1: 13.38 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:30.00 +38:16:30.4: 13.40 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:56.36 +36:19:51.1: 13.40 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:30.00 +38:16:30.4: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter KEPT candidate at 12:33:56.36 +36:19:51.1: ref_mag=13.39 +/- 0.03 new_mean_mag=12.3032 delta=1.09 (need > 0.90)
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter KEPT candidate at 12:29:30.00 +38:16:30.4: ref_mag=13.40 +/- 0.03 new_mean_mag=12.3568 delta=1.05 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:26.88 +33:44:01.3: 13.50 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:18.56 +35:26:32.1: 13.51 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:26.88 +33:44:01.3: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter KEPT candidate at 12:39:26.88 +33:44:01.3: ref_mag=13.44 +/- 0.03 new_mean_mag=12.4542 delta=0.98 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:31.39 +36:22:20.8: 13.47 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:18.56 +35:26:32.1: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:18.56 +35:26:32.1: ref_mag=13.50 +/- 0.03 new_mean_mag=12.5101 delta=0.99 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:43.15 +36:16:16.7: 13.49 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:12.38 +34:18:09.8: 13.45 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:31.39 +36:22:20.8: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 12:32:31.39 +36:22:20.8: ref_mag=13.45 +/- 0.03 new_mean_mag=12.3760 delta=1.07 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:43.15 +36:16:16.7: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter KEPT candidate at 12:29:43.15 +36:16:16.7: ref_mag=13.56 +/- 0.03 new_mean_mag=12.3446 delta=1.22 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:05.83 +34:36:50.2: 13.43 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:12.38 +34:18:09.8: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry filter KEPT candidate at 12:38:12.38 +34:18:09.8: ref_mag=13.47 +/- 0.03 new_mean_mag=12.3852 delta=1.09 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:05.83 +34:36:50.2: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 12:35:05.83 +34:36:50.2: ref_mag=13.45 +/- 0.03 new_mean_mag=12.3956 delta=1.05 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:13.82 +35:46:32.4: 13.42 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:13.82 +35:46:32.4: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter KEPT candidate at 12:33:13.82 +35:46:32.4: ref_mag=13.43 +/- 0.03 new_mean_mag=12.2245 delta=1.21 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:41:59.87 +33:41:18.3: 13.42 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:41:59.87 +33:41:18.3: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter KEPT candidate at 12:41:59.87 +33:41:18.3: ref_mag=13.40 +/- 0.03 new_mean_mag=12.3361 delta=1.06 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:56.27 +35:09:01.7: 13.41 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:56.27 +35:09:01.7: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter KEPT candidate at 12:39:56.27 +35:09:01.7: ref_mag=13.39 +/- 0.03 new_mean_mag=12.2700 delta=1.12 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:19.80 +34:34:46.4: 13.40 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:19.80 +34:34:46.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Forced photometry filter KEPT candidate at 12:32:19.80 +34:34:46.4: ref_mag=13.34 +/- 0.03 new_mean_mag=12.3813 delta=0.96 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:31:38.50 +35:27:29.4: 13.40 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:41:10.62 +35:19:01.8: 13.38 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:44:34.61 +33:11:32.1: 13.39 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:31:38.50 +35:27:29.4: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter KEPT candidate at 12:31:38.50 +35:27:29.4: ref_mag=13.42 +/- 0.03 new_mean_mag=12.4720 delta=0.95 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:41:10.62 +35:19:01.8: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 12:41:10.62 +35:19:01.8: ref_mag=13.34 +/- 0.02 new_mean_mag=12.3561 delta=0.98 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:44:34.61 +33:11:32.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:12.12 +33:51:27.4: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Forced photometry filter KEPT candidate at 12:44:34.61 +33:11:32.1: ref_mag=13.37 +/- 0.03 new_mean_mag=12.2913 delta=1.08 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:16.98 +36:39:57.6: 13.39 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:12.12 +33:51:27.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter KEPT candidate at 12:38:12.12 +33:51:27.4: ref_mag=13.33 +/- 0.03 new_mean_mag=12.3415 delta=0.99 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:16.98 +36:39:57.6: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter KEPT candidate at 12:32:16.98 +36:39:57.6: ref_mag=13.41 +/- 0.03 new_mean_mag=12.2898 delta=1.12 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:45:45.98 +33:43:15.9: 13.38 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:45:45.98 +33:43:15.9: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 12:45:45.98 +33:43:15.9: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3403 delta=1.03 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:15.54 +36:51:37.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:24.99 +34:18:44.7: 13.36 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:15.54 +36:51:37.1: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 12:32:15.54 +36:51:37.1: ref_mag=13.34 +/- 0.02 new_mean_mag=12.2206 delta=1.12 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:24.99 +34:18:44.7: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry filter KEPT candidate at 12:35:24.99 +34:18:44.7: ref_mag=13.31 +/- 0.03 new_mean_mag=12.2065 delta=1.11 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:05.47 +34:07:16.4: 13.35 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:05.47 +34:07:16.4: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry filter KEPT candidate at 12:40:05.47 +34:07:16.4: ref_mag=13.32 +/- 0.03 new_mean_mag=12.1666 delta=1.15 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:56.67 +35:49:39.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:56.67 +35:49:39.1: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Forced photometry filter KEPT candidate at 12:32:56.67 +35:49:39.1: ref_mag=13.37 +/- 0.03 new_mean_mag=12.3885 delta=0.98 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:48.21 +36:01:59.2: 13.32 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:44:55.56 +33:09:48.2: 13.29 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:42:15.28 +34:20:30.1: 13.33 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:44.15 +35:35:45.6: 13.32 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:48.21 +36:01:59.2: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry filter KEPT candidate at 12:39:48.21 +36:01:59.2: ref_mag=13.35 +/- 0.02 new_mean_mag=12.3751 delta=0.98 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:44:55.56 +33:09:48.2: 13.30 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:42:15.28 +34:20:30.1: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 12:44:55.56 +33:09:48.2: ref_mag=13.30 +/- 0.02 new_mean_mag=12.3347 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 12:42:15.28 +34:20:30.1: ref_mag=13.30 +/- 0.02 new_mean_mag=12.2322 delta=1.07 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:44.15 +35:35:45.6: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 12:34:44.15 +35:35:45.6: ref_mag=13.27 +/- 0.02 new_mean_mag=12.2676 delta=1.00 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:31:06.92 +37:27:58.9: 13.34 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:16.38 +36:32:47.4: 13.31 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:31:06.92 +37:27:58.9: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 12:31:06.92 +37:27:58.9: ref_mag=13.38 +/- 0.03 new_mean_mag=12.3879 delta=0.99 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:16.38 +36:32:47.4: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry filter KEPT candidate at 12:28:16.38 +36:32:47.4: ref_mag=13.32 +/- 0.03 new_mean_mag=12.2834 delta=1.04 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:16.65 +35:08:34.1: 13.28 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:16.65 +35:08:34.1: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 12:32:16.65 +35:08:34.1: ref_mag=13.27 +/- 0.02 new_mean_mag=12.3304 delta=0.94 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:40.98 +36:10:11.3: 13.28 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:40.98 +36:10:11.3: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 12:34:40.98 +36:10:11.3: ref_mag=13.33 +/- 0.02 new_mean_mag=12.3363 delta=0.99 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:42.36 +33:22:33.9: 13.26 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:42.36 +33:22:33.9: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 12:38:42.36 +33:22:33.9: ref_mag=13.29 +/- 0.02 new_mean_mag=12.3062 delta=0.98 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:39:49.33 +34:48:58.7: 13.24 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:39:49.33 +34:48:58.7: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 12:39:49.33 +34:48:58.7: ref_mag=13.28 +/- 0.02 new_mean_mag=12.3389 delta=0.94 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:21.40 +36:09:38.8: 13.23 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:21.40 +36:09:38.8: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 12:30:21.40 +36:09:38.8: ref_mag=13.19 +/- 0.02 new_mean_mag=12.2312 delta=0.96 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:23.40 +35:30:56.4: 13.22 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:03.07 +37:19:24.1: 13.22 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:23.40 +35:30:56.4: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 12:38:23.40 +35:30:56.4: ref_mag=13.21 +/- 0.02 new_mean_mag=12.1286 delta=1.08 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:04.18 +35:11:19.6: 13.20 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:03.07 +37:19:24.1: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 12:34:03.07 +37:19:24.1: ref_mag=13.21 +/- 0.02 new_mean_mag=12.2688 delta=0.94 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:04.18 +35:11:19.6: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 12:33:04.18 +35:11:19.6: ref_mag=13.24 +/- 0.02 new_mean_mag=12.1783 delta=1.06 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:10.89 +35:55:23.1: 13.20 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:22.55 +34:54:08.0: 13.20 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:37:32.27 +35:53:42.3: 13.19 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:06.51 +34:48:00.7: 13.18 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:22.55 +34:54:08.0: 13.20 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:10.89 +35:55:23.1: 13.16 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:37:32.27 +35:53:42.3: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 12:35:22.55 +34:54:08.0: ref_mag=13.20 +/- 0.02 new_mean_mag=12.1536 delta=1.04 (need > 0.90)
Forced photometry filter KEPT candidate at 12:33:10.89 +35:55:23.1: ref_mag=13.18 +/- 0.02 new_mean_mag=12.1784 delta=1.00 (need > 0.90)
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 12:37:32.27 +35:53:42.3: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1942 delta=0.99 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:06.51 +34:48:00.7: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 12:32:06.51 +34:48:00.7: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2731 delta=0.95 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:32.33 +36:41:18.7: 13.18 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:32.33 +36:41:18.7: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 12:35:32.33 +36:41:18.7: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2475 delta=0.97 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:53.25 +37:36:47.3: 13.16 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:53.25 +37:36:47.3: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 12:28:53.25 +37:36:47.3: ref_mag=13.18 +/- 0.02 new_mean_mag=12.1793 delta=1.00 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:42:54.61 +34:00:10.7: 13.15 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:36:18.49 +34:19:26.1: 13.14 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:42:45.87 +34:46:39.6: 13.14 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:42:54.61 +34:00:10.7: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 12:42:54.61 +34:00:10.7: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1507 delta=0.99 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:36:18.49 +34:19:26.1: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 12:36:18.49 +34:19:26.1: ref_mag=13.12 +/- 0.02 new_mean_mag=12.1655 delta=0.95 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:42:45.87 +34:46:39.6: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 12:42:45.87 +34:46:39.6: ref_mag=13.14 +/- 0.02 new_mean_mag=12.2345 delta=0.91 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:48:24.99 +33:18:11.1: 13.15 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:48:24.99 +33:18:11.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 12:48:24.99 +33:18:11.1: ref_mag=13.18 +/- 0.02 new_mean_mag=12.2116 delta=0.97 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:08.24 +35:08:15.6: 13.15 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:43:02.18 +35:01:01.3: 13.13 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:16.86 +37:55:02.6: 13.15 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:43.68 +36:25:44.7: 13.15 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:08.24 +35:08:15.6: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 12:40:08.24 +35:08:15.6: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1818 delta=0.98 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:43:02.18 +35:01:01.3: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 12:43:02.18 +35:01:01.3: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1109 delta=0.98 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:16.86 +37:55:02.6: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 12:28:16.86 +37:55:02.6: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1985 delta=0.96 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:43.68 +36:25:44.7: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 12:29:43.68 +36:25:44.7: ref_mag=13.08 +/- 0.02 new_mean_mag=12.1313 delta=0.95 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:28.87 +33:50:01.9: 13.13 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:23.00 +37:53:28.7: 13.12 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:28.87 +33:50:01.9: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 12:38:28.87 +33:50:01.9: ref_mag=13.11 +/- 0.02 new_mean_mag=12.1507 delta=0.96 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:23.00 +37:53:28.7: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 12:28:23.00 +37:53:28.7: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1125 delta=1.02 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:01.14 +33:15:12.0: 13.11 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:01.14 +33:15:12.0: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 12:40:01.14 +33:15:12.0: ref_mag=13.10 +/- 0.02 new_mean_mag=12.1732 delta=0.92 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:49:39.45 +33:05:29.8: 13.10 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:49:39.45 +33:05:29.8: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 12:49:39.45 +33:05:29.8: ref_mag=13.06 +/- 0.02 new_mean_mag=12.1233 delta=0.93 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:05.36 +36:28:00.0: 13.09 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:38.09 +38:10:00.4: 13.14 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:25.21 +36:33:38.7: 13.12 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:05.36 +36:28:00.0: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 12:34:05.36 +36:28:00.0: ref_mag=13.08 +/- 0.02 new_mean_mag=12.0638 delta=1.02 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:38.09 +38:10:00.4: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 12:28:38.09 +38:10:00.4: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1137 delta=0.98 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:25.21 +36:33:38.7: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 12:35:25.21 +36:33:38.7: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1173 delta=1.01 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:36:29.75 +34:45:16.5: 13.09 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:36:29.75 +34:45:16.5: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 12:36:29.75 +34:45:16.5: ref_mag=13.12 +/- 0.02 new_mean_mag=12.1444 delta=0.98 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:36:08.72 +35:38:57.9: 13.09 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:41.09 +35:22:14.9: 13.07 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:37.78 +36:10:11.0: 13.09 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:36:08.72 +35:38:57.9: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:41.09 +35:22:14.9: 13.02 +/- 0.03 detection
Forced photometry filter KEPT candidate at 12:36:08.72 +35:38:57.9: ref_mag=13.08 +/- 0.02 new_mean_mag=12.1181 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 12:30:41.09 +35:22:14.9: ref_mag=13.04 +/- 0.02 new_mean_mag=12.0929 delta=0.95 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:37.78 +36:10:11.0: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 12:30:37.78 +36:10:11.0: ref_mag=13.11 +/- 0.02 new_mean_mag=12.0979 delta=1.01 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:45:23.26 +33:15:36.1: 13.08 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:45:34.48 +33:24:06.5: 13.05 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:45:23.26 +33:15:36.1: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 12:45:23.26 +33:15:36.1: ref_mag=13.09 +/- 0.02 new_mean_mag=12.0959 delta=1.00 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:45:34.48 +33:24:06.5: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 12:45:34.48 +33:24:06.5: ref_mag=13.04 +/- 0.02 new_mean_mag=12.0596 delta=0.98 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:39.24 +34:26:58.9: 13.06 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:47.34 +36:20:38.3: 13.05 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:55.96 +37:12:24.6: 13.04 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:39.24 +34:26:58.9: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:47.34 +36:20:38.3: 12.94 +/- 0.02 detection
Forced photometry filter KEPT candidate at 12:38:39.24 +34:26:58.9: ref_mag=13.07 +/- 0.02 new_mean_mag=12.0887 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 12:28:47.34 +36:20:38.3: ref_mag=12.99 +/- 0.02 new_mean_mag=11.9594 delta=1.03 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:55.96 +37:12:24.6: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 12:35:55.96 +37:12:24.6: ref_mag=13.01 +/- 0.02 new_mean_mag=11.8030 delta=1.21 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:35:29.02 +35:48:01.3: 13.03 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:38.10 +36:08:45.0: 13.03 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:35:29.02 +35:48:01.3: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 12:35:29.02 +35:48:01.3: ref_mag=13.04 +/- 0.02 new_mean_mag=12.0457 delta=0.99 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:38.10 +36:08:45.0: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 12:30:38.10 +36:08:45.0: ref_mag=13.03 +/- 0.02 new_mean_mag=12.0589 delta=0.97 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:27:47.53 +38:01:36.7: 13.03 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:27:47.53 +38:01:36.7: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 12:27:47.53 +38:01:36.7: ref_mag=13.05 +/- 0.02 new_mean_mag=12.1039 delta=0.94 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:37:52.54 +33:15:28.8: 13.03 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:37:52.54 +33:15:28.8: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 12:37:52.54 +33:15:28.8: ref_mag=13.05 +/- 0.02 new_mean_mag=12.1002 delta=0.95 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:45:34.45 +33:06:52.7: 13.02 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:16.22 +37:17:58.8: 13.02 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:45:34.45 +33:06:52.7: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 12:45:34.45 +33:06:52.7: ref_mag=13.00 +/- 0.02 new_mean_mag=12.0483 delta=0.95 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:16.22 +37:17:58.8: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 12:28:16.22 +37:17:58.8: ref_mag=13.06 +/- 0.02 new_mean_mag=12.0636 delta=1.00 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:59.72 +36:14:52.3: 12.96 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:59.72 +36:14:52.3: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 12:28:59.72 +36:14:52.3: ref_mag=12.95 +/- 0.02 new_mean_mag=12.0109 delta=0.94 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:43:32.79 +34:25:12.7: 12.96 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:43:32.79 +34:25:12.7: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 12:43:32.79 +34:25:12.7: ref_mag=12.94 +/- 0.02 new_mean_mag=11.9838 delta=0.96 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:59.33 +35:44:32.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:59.33 +35:44:32.1: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry filter KEPT candidate at 12:32:59.33 +35:44:32.1: ref_mag=12.89 +/- 0.02 new_mean_mag=11.9594 delta=0.93 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:42:30.95 +34:13:49.0: 12.90 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:37:56.53 +34:13:33.3: 12.88 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:42:30.95 +34:13:49.0: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter KEPT candidate at 12:42:30.95 +34:13:49.0: ref_mag=12.97 +/- 0.02 new_mean_mag=12.0294 delta=0.94 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:37:56.53 +34:13:33.3: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 12:37:56.53 +34:13:33.3: ref_mag=12.87 +/- 0.02 new_mean_mag=11.9414 delta=0.93 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:33.37 +34:22:55.5: 12.87 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:21.74 +33:04:30.8: 12.89 +/- 0.03 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:33.37 +34:22:55.5: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter KEPT candidate at 12:40:33.37 +34:22:55.5: ref_mag=12.85 +/- 0.02 new_mean_mag=11.6873 delta=1.16 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:21.74 +33:04:30.8: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 12:40:21.74 +33:04:30.8: ref_mag=12.87 +/- 0.02 new_mean_mag=11.9198 delta=0.95 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:01.79 +37:35:16.3: 12.87 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:01.79 +37:35:16.3: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry filter KEPT candidate at 12:29:01.79 +37:35:16.3: ref_mag=12.88 +/- 0.02 new_mean_mag=11.9114 delta=0.96 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:46:57.15 +33:05:15.7: 12.85 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:46:57.15 +33:05:15.7: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry filter KEPT candidate at 12:46:57.15 +33:05:15.7: ref_mag=12.83 +/- 0.02 new_mean_mag=11.9108 delta=0.92 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:32:35.75 +37:15:31.7: 12.85 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:32:35.75 +37:15:31.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter KEPT candidate at 12:32:35.75 +37:15:31.7: ref_mag=12.84 +/- 0.02 new_mean_mag=11.9077 delta=0.93 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:50.70 +35:33:48.9: 12.82 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:50.70 +35:33:48.9: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter KEPT candidate at 12:33:50.70 +35:33:48.9: ref_mag=12.84 +/- 0.02 new_mean_mag=11.8916 delta=0.95 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:36.38 +36:22:02.2: 12.43 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 13:38:59.94 +41:09:43.8: 12.35 +/- 0.02 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:32.31 +36:50:55.3: 12.29 +/- 0.01 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 13:38:59.94 +41:09:43.8: 12.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:36.38 +36:22:02.2: 12.35 +/- 0.01 detection
Forced photometry filter KEPT candidate at 13:38:59.94 +41:09:43.8: ref_mag=12.35 +/- 0.01 new_mean_mag=11.3167 delta=1.03 (need > 0.90)
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 12:29:36.38 +36:22:02.2: ref_mag=12.39 +/- 0.01 new_mean_mag=11.3947 delta=0.99 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:32.31 +36:50:55.3: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter KEPT candidate at 12:28:32.31 +36:50:55.3: ref_mag=12.30 +/- 0.01 new_mean_mag=11.3383 delta=0.96 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:36.48 +35:02:57.8: 13.81 +/- 0.06 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:36.48 +35:02:57.8: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry filter KEPT candidate at 12:33:36.48 +35:02:57.8: ref_mag=13.81 +/- 0.04 new_mean_mag=12.5879 delta=1.22 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:56.96 +36:30:58.8: 13.83 +/- 0.06 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:00.08 +36:03:14.3: 13.80 +/- 0.06 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:56.96 +36:30:58.8: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Forced photometry filter KEPT candidate at 12:28:56.96 +36:30:58.8: ref_mag=13.87 +/- 0.04 new_mean_mag=12.6254 delta=1.24 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:00.08 +36:03:14.3: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry filter KEPT candidate at 12:30:00.08 +36:03:14.3: ref_mag=13.78 +/- 0.04 new_mean_mag=12.3814 delta=1.39 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:33.87 +37:36:02.8: 13.78 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:17.80 +36:28:25.1: 13.75 +/- 0.06 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:33.87 +37:36:02.8: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Forced photometry filter KEPT candidate at 12:28:33.87 +37:36:02.8: ref_mag=13.82 +/- 0.04 new_mean_mag=12.5570 delta=1.26 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:17.80 +36:28:25.1: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter KEPT candidate at 12:28:17.80 +36:28:25.1: ref_mag=13.74 +/- 0.04 new_mean_mag=12.4376 delta=1.30 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:30:35.26 +36:12:10.0: 13.72 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:36:23.61 +36:47:13.7: 13.71 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:30:35.26 +36:12:10.0: 13.74 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:36:23.61 +36:47:13.7: 13.66 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:38:57.16 +33:51:30.6: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 12:36:23.61 +36:47:13.7: ref_mag=13.68 +/- 0.03 new_mean_mag=12.5657 delta=1.12 (need > 0.90)
Forced photometry filter KEPT candidate at 12:30:35.26 +36:12:10.0: ref_mag=13.73 +/- 0.04 new_mean_mag=12.5646 delta=1.17 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:38:57.16 +33:51:30.6: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Forced photometry filter KEPT candidate at 12:38:57.16 +33:51:30.6: ref_mag=13.72 +/- 0.04 new_mean_mag=12.4914 delta=1.23 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:31:06.85 +36:13:53.0: 13.67 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:31:06.85 +36:13:53.0: 13.70 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:34:49.36 +34:23:24.2: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Forced photometry filter KEPT candidate at 12:31:06.85 +36:13:53.0: ref_mag=13.69 +/- 0.03 new_mean_mag=12.5714 delta=1.11 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:34:49.36 +34:23:24.2: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:49.36 +34:23:24.2: ref_mag=13.63 +/- 0.03 new_mean_mag=12.4294 delta=1.21 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:29:09.47 +35:48:09.2: 13.61 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:29:09.47 +35:48:09.2: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry filter KEPT candidate at 12:29:09.47 +35:48:09.2: ref_mag=13.63 +/- 0.03 new_mean_mag=12.5191 delta=1.11 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:40:10.19 +35:28:50.8: 13.63 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:40:10.19 +35:28:50.8: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Forced photometry filter KEPT candidate at 12:40:10.19 +35:28:50.8: ref_mag=13.61 +/- 0.03 new_mean_mag=12.4295 delta=1.18 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:33:42.26 +34:38:50.9: 13.59 +/- 0.05 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:33:42.26 +34:38:50.9: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Forced photometry filter KEPT candidate at 12:33:42.26 +34:38:50.9: ref_mag=13.61 +/- 0.03 new_mean_mag=12.5017 delta=1.10 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:36:30.53 +34:33:08.4: 13.57 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:36:30.53 +34:33:08.4: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Forced photometry filter KEPT candidate at 12:36:30.53 +34:33:08.4: ref_mag=13.52 +/- 0.03 new_mean_mag=12.4751 delta=1.05 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:28:44.43 +37:13:11.4: 13.56 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:41:48.91 +34:05:26.7: 13.56 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_00-59-26_20.00sec_4.90C_LIGHT_1576.fits at 12:31:30.25 +36:54:35.0: 13.54 +/- 0.04 detection
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:28:44.43 +37:13:11.4: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter KEPT candidate at 12:28:44.43 +37:13:11.4: ref_mag=13.43 +/- 0.03 new_mean_mag=12.4183 delta=1.01 (need > 0.90)
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:41:48.91 +34:05:26.7: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Forced photometry on wcs_CVn-02-Q1b1x1_2026-05-18_01-00-14_20.00sec_5.00C_LIGHT_1577.fits at 12:31:30.25 +36:54:35.0: 13.54 +/- 0.04 detection
Forced photometry filter KEPT candidate at 12:41:48.91 +34:05:26.7: ref_mag=13.53 +/- 0.03 new_mean_mag=12.4496 delta=1.08 (need > 0.90)
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Forced photometry filter KEPT candidate at 12:31:30.25 +36:54:35.0: ref_mag=13.54 +/- 0.03 new_mean_mag=12.4302 delta=1.11 (need > 0.90)
Adding exclusion_list_local.txt__out04011.dat to exclusion_list_local.txt
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make_report_in_HTML.sh Phase 1 (network queries): 124s
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: 96s
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Considering the candidate 31896_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 31896_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
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Considering the candidate 31897_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 31897_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
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Considering the candidate 31898_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 31898_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:30:06.32 +34:15:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31900_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 31900_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:27:12.26 +40:26:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31903_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 31903_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:32:01.98 +34:05:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31904_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 31904_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:30:26.09 +36:07:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32277_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 32277_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:40:13.03 +34:11:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32372_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 32372_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 13:10:44.08 +34:19:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20705_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 20705_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
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Considering the candidate 20883_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20883_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 19982_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 19982_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21746_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21746_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 13553_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 13553_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 19998_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 19998_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21730_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21730_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 11378_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 11378_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20281_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20281_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21761_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21761_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20792_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20792_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16829_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16829_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 18116_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 18116_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 11083_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 11083_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 19736_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 19736_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:30:03.58 +34:03:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18529_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 18529_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 22770_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 22770_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 13619_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 13619_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:27:02.12 +37:13:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17124_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17124_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 17045_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17045_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20017_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20017_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20854_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20854_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 24255_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 24255_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:27:56.93 +36:01:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21709_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 21709_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:30:51.52 +35:17:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23589_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 23589_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 18367_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 18367_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21935_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21935_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20807_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20807_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21760_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 21760_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:29:14.41 +34:54:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22530_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 22530_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:31:39.54 +35:15:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22941_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 22941_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 22349_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 22349_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16336_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16336_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 18231_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 18231_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 17851_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17851_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 18461_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 18461_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 14974_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 14974_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:27:09.16 +36:40:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14766_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 14766_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20125_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20125_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 22102_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 22102_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:31:14.06 +35:06:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19580_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 19580_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 23707_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 23707_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 09841_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 09841_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:26:46.32 +38:42:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23957_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 23957_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 19964_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 19964_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16278_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16278_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20875_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20875_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 13222_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 13222_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 17735_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17735_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 23261_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 23261_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:28:24.03 +35:35:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21852_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21852_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 22014_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 22014_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:29:53.75 +35:00:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24365_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 24365_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16875_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16875_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21184_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21184_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 24430_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 24430_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 22819_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 22819_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 13686_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 13686_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 22253_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 22253_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 23903_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 23903_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21494_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21494_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 23654_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 23654_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21296_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21296_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 17711_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17711_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 12752_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 12752_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 23922_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 23922_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:28:23.14 +35:51:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19121_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 19121_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20168_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20168_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21003_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21003_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16499_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16499_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21959_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21959_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21623_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21623_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 11959_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 11959_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 17288_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17288_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 18792_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 18792_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 12008_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 12008_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16568_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16568_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16038_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16038_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 11339_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 11339_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 17322_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17322_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 17473_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17473_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21208_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21208_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20848_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20848_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21243_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21243_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 24545_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 24545_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16461_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16461_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16781_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16781_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20389_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20389_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 17170_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17170_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 14045_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 14045_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 23532_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 23532_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 24428_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 24428_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 11643_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 11643_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16636_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16636_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16170_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16170_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 13481_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 13481_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 18192_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 18192_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 14745_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 14745_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:27:07.42 +36:46:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20035_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20035_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 22428_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 22428_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:31:38.21 +35:11:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23521_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 23521_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 19720_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 19720_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 19820_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 19820_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20171_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20171_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16202_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16202_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 12809_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 12809_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 16069_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 16069_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 13779_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 13779_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 21113_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21113_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20485_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 20485_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:36:18.53 +34:27:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19651_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 19651_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:28:18.86 +35:56:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17306_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17306_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 04011_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 04011_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 14634_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 14634_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 02308_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 02308_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 13:39:57.97 +41:52:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21945_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 21945_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 17664_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17664_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 19403_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 19403_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 12783_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 12783_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 17558_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 17558_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 18503_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 18503_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 15105_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 15105_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 18905_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 18905_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 18500_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 18500_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 20159_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20159_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 22978_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 22978_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:30:12.13 +35:25:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20536_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20536_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
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Considering the candidate 22701_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 22701_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20929_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20929_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20687_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 20687_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13712_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 13712_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19315_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 19315_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13560_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
The candidate 13560_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071 did not pass the final checks
**** FOUND 12:27:04.41 +37:15:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14639_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
Preparing report for the candidate 14639_fd_CVn-02-Q1b1x1_2026-09-06_22-00-36_20.00sec_-0.00C_LIGHTs_0071
make_report_in_HTML.sh Phase 2 (HTML assembly): 20s
make_report_in_HTML.sh TOTAL: 240s
Prepared the HTML report for the field CVn-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:38:59.94 +41:09:43.8
12:29:30.00 +38:16:30.4
12:28:38.09 +38:10:00.4
12:31:28.78 +38:11:55.7
12:27:47.53 +38:01:36.7
12:28:16.86 +37:55:02.6
12:28:23.00 +37:53:28.7
12:28:53.25 +37:36:47.3
12:28:33.87 +37:36:02.8
12:29:01.79 +37:35:16.3
12:31:06.92 +37:27:58.9
12:28:16.22 +37:17:58.8
12:32:57.33 +37:21:20.1
12:34:03.07 +37:19:24.1
12:28:44.43 +37:13:11.4
12:32:35.75 +37:15:31.7
12:35:55.96 +37:12:24.6
12:28:32.31 +36:50:55.3
12:31:30.25 +36:54:35.0
12:32:15.54 +36:51:37.1
12:36:23.61 +36:47:13.7
12:49:39.45 +33:05:29.8
12:46:57.15 +33:05:15.7
12:45:34.45 +33:06:52.7
12:40:21.74 +33:04:30.8
12:44:55.56 +33:09:48.2
12:44:34.61 +33:11:32.1
12:45:23.26 +33:15:36.1
12:48:24.99 +33:18:11.1
12:40:01.14 +33:15:12.0
12:37:52.54 +33:15:28.8
12:45:34.48 +33:24:06.5
12:41:12.93 +33:22:57.0
12:38:42.36 +33:22:33.9
12:29:43.15 +36:16:16.7
12:32:31.39 +36:22:20.8
12:28:47.34 +36:20:38.3
12:29:43.68 +36:25:44.7
12:29:36.38 +36:22:02.2
12:34:05.36 +36:28:00.0
12:35:25.21 +36:33:38.7
12:28:17.80 +36:28:25.1
12:28:56.96 +36:30:58.8
12:35:32.33 +36:41:18.7
12:28:16.38 +36:32:47.4
12:32:16.98 +36:39:57.6
12:33:56.36 +36:19:51.1
12:28:59.72 +36:14:52.3
12:38:12.12 +33:51:27.4
12:41:59.87 +33:41:18.3
12:45:45.98 +33:43:15.9
12:31:06.85 +36:13:53.0
12:30:35.26 +36:12:10.0
12:39:26.88 +33:44:01.3
12:38:28.87 +33:50:01.9
12:38:57.16 +33:51:30.6
12:42:54.61 +34:00:10.7
12:41:48.91 +34:05:26.7
12:30:00.08 +36:03:14.3
12:40:05.47 +34:07:16.4
12:42:30.95 +34:13:49.0
12:37:56.53 +34:13:33.3
12:42:15.28 +34:20:30.1
12:44:07.66 +34:23:07.2
12:39:51.16 +34:18:56.4
12:38:12.38 +34:18:09.8
12:43:32.79 +34:25:12.7
12:35:24.99 +34:18:44.7
12:34:49.36 +34:23:24.2
12:36:18.49 +34:19:26.1
12:40:33.37 +34:22:55.5
12:44:29.46 +34:30:28.0
12:38:39.24 +34:26:58.9
12:29:09.47 +35:48:09.2
12:36:30.53 +34:33:08.4
12:45:15.75 +34:42:52.8
12:32:19.80 +34:34:46.4
12:36:08.72 +35:38:57.9
12:35:05.83 +34:36:50.2
12:34:44.15 +35:35:45.6
12:35:56.84 +34:37:38.8
12:33:42.26 +34:38:50.9
12:42:45.87 +34:46:39.6
12:33:50.70 +35:33:48.9
12:39:49.33 +34:48:58.7
12:36:29.75 +34:45:16.5
12:30:41.09 +35:22:14.9
12:32:06.51 +34:48:00.7
12:35:22.55 +34:54:08.0
12:43:02.18 +35:01:01.3
12:32:33.84 +34:57:15.2
12:40:51.61 +35:04:47.6
12:39:01.38 +35:03:59.9
12:32:16.65 +35:08:34.1
12:39:56.27 +35:09:01.7
12:33:36.48 +35:02:57.8
12:40:08.24 +35:08:15.6
12:33:04.18 +35:11:19.6
12:41:10.62 +35:19:01.8
12:40:10.19 +35:28:50.8
12:34:18.56 +35:26:32.1
12:38:23.40 +35:30:56.4
12:31:38.50 +35:27:29.4
12:32:59.33 +35:44:32.1
12:35:29.02 +35:48:01.3
12:33:13.82 +35:46:32.4
12:37:32.27 +35:53:42.3
12:32:56.67 +35:49:39.1
12:33:10.89 +35:55:23.1
12:39:48.21 +36:01:59.2
12:34:40.98 +36:10:11.3
12:30:38.10 +36:08:45.0
12:30:21.40 +36:09:38.8
12:30:37.78 +36:10:11.0
########### Completed CVn-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
12:35:56.84 +34:37:38.8
12:44:07.66 +34:23:07.2
12:40:51.61 +35:04:47.6
12:32:57.33 +37:21:20.1
12:39:51.16 +34:18:56.4
12:32:33.84 +34:57:15.2
12:31:28.78 +38:11:55.7
12:44:29.46 +34:30:28.0
12:39:01.38 +35:03:59.9
12:45:15.75 +34:42:52.8
12:41:12.93 +33:22:57.0
12:33:56.36 +36:19:51.1
12:29:30.00 +38:16:30.4
12:39:26.88 +33:44:01.3
12:34:18.56 +35:26:32.1
12:32:31.39 +36:22:20.8
12:29:43.15 +36:16:16.7
12:38:12.38 +34:18:09.8
12:35:05.83 +34:36:50.2
12:33:13.82 +35:46:32.4
12:41:59.87 +33:41:18.3
12:39:56.27 +35:09:01.7
12:32:19.80 +34:34:46.4
12:31:38.50 +35:27:29.4
12:41:10.62 +35:19:01.8
12:44:34.61 +33:11:32.1
12:38:12.12 +33:51:27.4
12:32:16.98 +36:39:57.6
12:45:45.98 +33:43:15.9
12:32:15.54 +36:51:37.1
12:35:24.99 +34:18:44.7
12:40:05.47 +34:07:16.4
12:32:56.67 +35:49:39.1
12:39:48.21 +36:01:59.2
12:42:15.28 +34:20:30.1
12:44:55.56 +33:09:48.2
12:34:44.15 +35:35:45.6
12:31:06.92 +37:27:58.9
12:28:16.38 +36:32:47.4
12:32:16.65 +35:08:34.1
12:34:40.98 +36:10:11.3
12:38:42.36 +33:22:33.9
12:39:49.33 +34:48:58.7
12:30:21.40 +36:09:38.8
12:38:23.40 +35:30:56.4
12:34:03.07 +37:19:24.1
12:33:04.18 +35:11:19.6
12:33:10.89 +35:55:23.1
12:35:22.55 +34:54:08.0
12:37:32.27 +35:53:42.3
12:32:06.51 +34:48:00.7
12:35:32.33 +36:41:18.7
12:28:53.25 +37:36:47.3
12:42:54.61 +34:00:10.7
12:36:18.49 +34:19:26.1
12:42:45.87 +34:46:39.6
12:48:24.99 +33:18:11.1
12:40:08.24 +35:08:15.6
12:43:02.18 +35:01:01.3
12:28:16.86 +37:55:02.6
12:29:43.68 +36:25:44.7
12:38:28.87 +33:50:01.9
12:28:23.00 +37:53:28.7
12:40:01.14 +33:15:12.0
12:49:39.45 +33:05:29.8
12:28:38.09 +38:10:00.4
12:34:05.36 +36:28:00.0
12:35:25.21 +36:33:38.7
12:36:29.75 +34:45:16.5
12:36:08.72 +35:38:57.9
12:30:41.09 +35:22:14.9
12:30:37.78 +36:10:11.0
12:45:23.26 +33:15:36.1
12:45:34.48 +33:24:06.5
12:38:39.24 +34:26:58.9
12:28:47.34 +36:20:38.3
12:35:55.96 +37:12:24.6
12:35:29.02 +35:48:01.3
12:30:38.10 +36:08:45.0
12:27:47.53 +38:01:36.7
12:37:52.54 +33:15:28.8
12:45:34.45 +33:06:52.7
12:28:16.22 +37:17:58.8
12:28:59.72 +36:14:52.3
12:43:32.79 +34:25:12.7
12:32:59.33 +35:44:32.1
12:42:30.95 +34:13:49.0
12:37:56.53 +34:13:33.3
12:40:33.37 +34:22:55.5
12:40:21.74 +33:04:30.8
12:29:01.79 +37:35:16.3
12:46:57.15 +33:05:15.7
12:32:35.75 +37:15:31.7
12:33:50.70 +35:33:48.9
12:29:36.38 +36:22:02.2
13:38:59.94 +41:09:43.8
12:28:32.31 +36:50:55.3
12:33:36.48 +35:02:57.8
12:28:56.96 +36:30:58.8
12:30:00.08 +36:03:14.3
12:28:33.87 +37:36:02.8
12:28:17.80 +36:28:25.1
12:30:35.26 +36:12:10.0
12:36:23.61 +36:47:13.7
12:38:57.16 +33:51:30.6
12:31:06.85 +36:13:53.0
12:34:49.36 +34:23:24.2
12:29:09.47 +35:48:09.2
12:40:10.19 +35:28:50.8
12:33:42.26 +34:38:50.9
12:36:30.53 +34:33:08.4
12:28:44.43 +37:13:11.4
12:41:48.91 +34:05:26.7
12:31:30.25 +36:54:35.0
###################################################################################
12:35:56.84 +34:37:38.8 -- not an asteroid (will add it to exclusion list)
12:44:07.66 +34:23:07.2 -- not an asteroid (will add it to exclusion list)
12:40:51.61 +35:04:47.6 -- not an asteroid (will add it to exclusion list)
12:32:57.33 +37:21:20.1 -- not an asteroid (will add it to exclusion list)
12:39:51.16 +34:18:56.4 -- not an asteroid (will add it to exclusion list)
12:32:33.84 +34:57:15.2 -- not an asteroid (will add it to exclusion list)
12:31:28.78 +38:11:55.7 -- not an asteroid (will add it to exclusion list)
12:44:29.46 +34:30:28.0 -- not an asteroid (will add it to exclusion list)
12:39:01.38 +35:03:59.9 -- not an asteroid (will add it to exclusion list)
12:45:15.75 +34:42:52.8 -- not an asteroid (will add it to exclusion list)
12:41:12.93 +33:22:57.0 -- not an asteroid (will add it to exclusion list)
12:33:56.36 +36:19:51.1 -- not an asteroid (will add it to exclusion list)
12:29:30.00 +38:16:30.4 -- not an asteroid (will add it to exclusion list)
12:39:26.88 +33:44:01.3 -- not an asteroid (will add it to exclusion list)
12:34:18.56 +35:26:32.1 -- not an asteroid (will add it to exclusion list)
12:32:31.39 +36:22:20.8 -- not an asteroid (will add it to exclusion list)
12:29:43.15 +36:16:16.7 -- not an asteroid (will add it to exclusion list)
12:38:12.38 +34:18:09.8 -- not an asteroid (will add it to exclusion list)
12:35:05.83 +34:36:50.2 -- not an asteroid (will add it to exclusion list)
12:33:13.82 +35:46:32.4 -- not an asteroid (will add it to exclusion list)
12:41:59.87 +33:41:18.3 -- not an asteroid (will add it to exclusion list)
12:39:56.27 +35:09:01.7 -- not an asteroid (will add it to exclusion list)
12:32:19.80 +34:34:46.4 -- not an asteroid (will add it to exclusion list)
12:31:38.50 +35:27:29.4 -- not an asteroid (will add it to exclusion list)
12:41:10.62 +35:19:01.8 -- not an asteroid (will add it to exclusion list)
12:44:34.61 +33:11:32.1 -- not an asteroid (will add it to exclusion list)
12:38:12.12 +33:51:27.4 -- not an asteroid (will add it to exclusion list)
12:32:16.98 +36:39:57.6 -- not an asteroid (will add it to exclusion list)
12:45:45.98 +33:43:15.9 -- not an asteroid (will add it to exclusion list)
12:32:15.54 +36:51:37.1 -- not an asteroid (will add it to exclusion list)
12:35:24.99 +34:18:44.7 -- not an asteroid (will add it to exclusion list)
12:40:05.47 +34:07:16.4 -- not an asteroid (will add it to exclusion list)
12:32:56.67 +35:49:39.1 -- not an asteroid (will add it to exclusion list)
12:39:48.21 +36:01:59.2 -- not an asteroid (will add it to exclusion list)
12:42:15.28 +34:20:30.1 -- not an asteroid (will add it to exclusion list)
12:44:55.56 +33:09:48.2 -- not an asteroid (will add it to exclusion list)
12:34:44.15 +35:35:45.6 -- not an asteroid (will add it to exclusion list)
12:31:06.92 +37:27:58.9 -- not an asteroid (will add it to exclusion list)
12:28:16.38 +36:32:47.4 -- not an asteroid (will add it to exclusion list)
12:32:16.65 +35:08:34.1 -- not an asteroid (will add it to exclusion list)
12:34:40.98 +36:10:11.3 -- not an asteroid (will add it to exclusion list)
12:38:42.36 +33:22:33.9 -- not an asteroid (will add it to exclusion list)
12:39:49.33 +34:48:58.7 -- not an asteroid (will add it to exclusion list)
12:30:21.40 +36:09:38.8 -- not an asteroid (will add it to exclusion list)
12:38:23.40 +35:30:56.4 -- not an asteroid (will add it to exclusion list)
12:34:03.07 +37:19:24.1 -- not an asteroid (will add it to exclusion list)
12:33:04.18 +35:11:19.6 -- not an asteroid (will add it to exclusion list)
12:33:10.89 +35:55:23.1 -- not an asteroid (will add it to exclusion list)
12:35:22.55 +34:54:08.0 -- not an asteroid (will add it to exclusion list)
12:37:32.27 +35:53:42.3 -- not an asteroid (will add it to exclusion list)
12:32:06.51 +34:48:00.7 -- not an asteroid (will add it to exclusion list)
12:35:32.33 +36:41:18.7 -- not an asteroid (will add it to exclusion list)
12:28:53.25 +37:36:47.3 -- not an asteroid (will add it to exclusion list)
12:42:54.61 +34:00:10.7 -- not an asteroid (will add it to exclusion list)
12:36:18.49 +34:19:26.1 -- not an asteroid (will add it to exclusion list)
12:42:45.87 +34:46:39.6 -- not an asteroid (will add it to exclusion list)
12:48:24.99 +33:18:11.1 -- not an asteroid (will add it to exclusion list)
12:40:08.24 +35:08:15.6 -- not an asteroid (will add it to exclusion list)
12:43:02.18 +35:01:01.3 -- not an asteroid (will add it to exclusion list)
12:28:16.86 +37:55:02.6 -- not an asteroid (will add it to exclusion list)
12:29:43.68 +36:25:44.7 -- not an asteroid (will add it to exclusion list)
12:38:28.87 +33:50:01.9 -- not an asteroid (will add it to exclusion list)
12:28:23.00 +37:53:28.7 -- not an asteroid (will add it to exclusion list)
12:40:01.14 +33:15:12.0 -- not an asteroid (will add it to exclusion list)
12:49:39.45 +33:05:29.8 -- not an asteroid (will add it to exclusion list)
12:28:38.09 +38:10:00.4 -- not an asteroid (will add it to exclusion list)
12:34:05.36 +36:28:00.0 -- not an asteroid (will add it to exclusion list)
12:35:25.21 +36:33:38.7 -- not an asteroid (will add it to exclusion list)
12:36:29.75 +34:45:16.5 -- not an asteroid (will add it to exclusion list)
12:36:08.72 +35:38:57.9 -- not an asteroid (will add it to exclusion list)
12:30:41.09 +35:22:14.9 -- not an asteroid (will add it to exclusion list)
12:30:37.78 +36:10:11.0 -- not an asteroid (will add it to exclusion list)
12:45:23.26 +33:15:36.1 -- not an asteroid (will add it to exclusion list)
12:45:34.48 +33:24:06.5 -- not an asteroid (will add it to exclusion list)
12:38:39.24 +34:26:58.9 -- not an asteroid (will add it to exclusion list)
12:28:47.34 +36:20:38.3 -- not an asteroid (will add it to exclusion list)
12:35:55.96 +37:12:24.6 -- not an asteroid (will add it to exclusion list)
12:35:29.02 +35:48:01.3 -- not an asteroid (will add it to exclusion list)
12:30:38.10 +36:08:45.0 -- not an asteroid (will add it to exclusion list)
12:27:47.53 +38:01:36.7 -- not an asteroid (will add it to exclusion list)
12:37:52.54 +33:15:28.8 -- not an asteroid (will add it to exclusion list)
12:45:34.45 +33:06:52.7 -- not an asteroid (will add it to exclusion list)
12:28:16.22 +37:17:58.8 -- not an asteroid (will add it to exclusion list)
12:28:59.72 +36:14:52.3 -- not an asteroid (will add it to exclusion list)
12:43:32.79 +34:25:12.7 -- not an asteroid (will add it to exclusion list)
12:32:59.33 +35:44:32.1 -- not an asteroid (will add it to exclusion list)
12:42:30.95 +34:13:49.0 -- not an asteroid (will add it to exclusion list)
12:37:56.53 +34:13:33.3 -- not an asteroid (will add it to exclusion list)
12:40:33.37 +34:22:55.5 -- not an asteroid (will add it to exclusion list)
12:40:21.74 +33:04:30.8 -- not an asteroid (will add it to exclusion list)
12:29:01.79 +37:35:16.3 -- not an asteroid (will add it to exclusion list)
12:46:57.15 +33:05:15.7 -- not an asteroid (will add it to exclusion list)
12:32:35.75 +37:15:31.7 -- not an asteroid (will add it to exclusion list)
12:33:50.70 +35:33:48.9 -- not an asteroid (will add it to exclusion list)
12:29:36.38 +36:22:02.2 -- not an asteroid (will add it to exclusion list)
13:38:59.94 +41:09:43.8 -- not an asteroid (will add it to exclusion list)
12:28:32.31 +36:50:55.3 -- not an asteroid (will add it to exclusion list)
12:33:36.48 +35:02:57.8 -- not an asteroid (will add it to exclusion list)
12:28:56.96 +36:30:58.8 -- not an asteroid (will add it to exclusion list)
12:30:00.08 +36:03:14.3 -- not an asteroid (will add it to exclusion list)
12:28:33.87 +37:36:02.8 -- not an asteroid (will add it to exclusion list)
12:28:17.80 +36:28:25.1 -- not an asteroid (will add it to exclusion list)
12:30:35.26 +36:12:10.0 -- not an asteroid (will add it to exclusion list)
12:36:23.61 +36:47:13.7 -- not an asteroid (will add it to exclusion list)
12:38:57.16 +33:51:30.6 -- not an asteroid (will add it to exclusion list)
12:31:06.85 +36:13:53.0 -- not an asteroid (will add it to exclusion list)
12:34:49.36 +34:23:24.2 -- not an asteroid (will add it to exclusion list)
12:29:09.47 +35:48:09.2 -- not an asteroid (will add it to exclusion list)
12:40:10.19 +35:28:50.8 -- not an asteroid (will add it to exclusion list)
12:33:42.26 +34:38:50.9 -- not an asteroid (will add it to exclusion list)
12:36:30.53 +34:33:08.4 -- not an asteroid (will add it to exclusion list)
12:28:44.43 +37:13:11.4 -- not an asteroid (will add it to exclusion list)
12:41:48.91 +34:05:26.7 -- not an asteroid (will add it to exclusion list)
12:31:30.25 +36:54:35.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
12:27:47.53 +38:01:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:16.22 +37:17:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:16.38 +36:32:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:16.86 +37:55:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:17.80 +36:28:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:23.00 +37:53:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:32.31 +36:50:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:33.87 +37:36:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:38.09 +38:10:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:44.43 +37:13:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:47.34 +36:20:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:53.25 +37:36:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:56.96 +36:30:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:59.72 +36:14:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:29:01.79 +37:35:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:29:09.47 +35:48:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:29:30.00 +38:16:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:29:36.38 +36:22:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:29:43.15 +36:16:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:29:43.68 +36:25:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:30:00.08 +36:03:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:30:21.40 +36:09:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:30:35.26 +36:12:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:30:37.78 +36:10:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:30:38.10 +36:08:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:30:41.09 +35:22:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:31:06.85 +36:13:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:31:06.92 +37:27:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:31:28.78 +38:11:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:31:30.25 +36:54:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:31:38.50 +35:27:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:06.51 +34:48:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:15.54 +36:51:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:16.65 +35:08:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:16.98 +36:39:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:19.80 +34:34:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:31.39 +36:22:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:33.84 +34:57:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:35.75 +37:15:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:56.67 +35:49:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:57.33 +37:21:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:59.33 +35:44:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:04.18 +35:11:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:10.89 +35:55:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:13.82 +35:46:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:36.48 +35:02:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:42.26 +34:38:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:50.70 +35:33:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:56.36 +36:19:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:03.07 +37:19:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:05.36 +36:28:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:18.56 +35:26:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:40.98 +36:10:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:44.15 +35:35:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:49.36 +34:23:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:05.83 +34:36:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:22.55 +34:54:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:24.99 +34:18:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:25.21 +36:33:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:29.02 +35:48:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:32.33 +36:41:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:55.96 +37:12:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:56.84 +34:37:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:08.72 +35:38:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:18.49 +34:19:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:23.61 +36:47:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:29.75 +34:45:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:30.53 +34:33:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:37:32.27 +35:53:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:37:52.54 +33:15:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:37:56.53 +34:13:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:12.12 +33:51:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:12.38 +34:18:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:23.40 +35:30:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:28.87 +33:50:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:39.24 +34:26:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:42.36 +33:22:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:57.16 +33:51:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:39:01.38 +35:03:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:39:26.88 +33:44:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:39:48.21 +36:01:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:39:49.33 +34:48:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:39:51.16 +34:18:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:39:56.27 +35:09:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:01.14 +33:15:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:05.47 +34:07:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:08.24 +35:08:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:10.19 +35:28:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:21.74 +33:04:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:33.37 +34:22:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:51.61 +35:04:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:10.62 +35:19:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:12.93 +33:22:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:48.91 +34:05:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:59.87 +33:41:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:15.28 +34:20:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:30.95 +34:13:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:45.87 +34:46:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:54.61 +34:00:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:43:02.18 +35:01:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:43:32.79 +34:25:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:07.66 +34:23:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:29.46 +34:30:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:34.61 +33:11:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:55.56 +33:09:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:15.75 +34:42:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:23.26 +33:15:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:34.45 +33:06:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:34.48 +33:24:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:45.98 +33:43:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:57.15 +33:05:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:24.99 +33:18:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:39.45 +33:05:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:38:59.94 +41:09:43.8 -- 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)
12:27:47.53 +38:01:36.7 -- not a known variable star
12:28:16.22 +37:17:58.8 -- not a known variable star
12:28:16.38 +36:32:47.4 -- not a known variable star
12:28:16.86 +37:55:02.6 -- not a known variable star
12:28:17.80 +36:28:25.1 -- not a known variable star
12:28:23.00 +37:53:28.7 -- not a known variable star
12:28:32.31 +36:50:55.3 -- not a known variable star
12:28:33.87 +37:36:02.8 -- not a known variable star
12:28:38.09 +38:10:00.4 -- not a known variable star
12:28:44.43 +37:13:11.4 -- not a known variable star
12:28:47.34 +36:20:38.3 -- not a known variable star
12:28:53.25 +37:36:47.3 -- not a known variable star
12:28:56.96 +36:30:58.8 -- not a known variable star
12:28:59.72 +36:14:52.3 -- a known variable star
12:29:01.79 +37:35:16.3 -- not a known variable star
12:29:09.47 +35:48:09.2 -- not a known variable star
12:29:30.00 +38:16:30.4 -- not a known variable star
12:29:36.38 +36:22:02.2 -- not a known variable star
12:29:43.15 +36:16:16.7 -- not a known variable star
12:29:43.68 +36:25:44.7 -- a known variable star
12:30:00.08 +36:03:14.3 -- not a known variable star
12:30:21.40 +36:09:38.8 -- not a known variable star
12:30:35.26 +36:12:10.0 -- not a known variable star
12:30:37.78 +36:10:11.0 -- a known variable star
12:30:38.10 +36:08:45.0 -- a known variable star
12:30:41.09 +35:22:14.9 -- not a known variable star
12:31:06.85 +36:13:53.0 -- not a known variable star
12:31:06.92 +37:27:58.9 -- not a known variable star
12:31:28.78 +38:11:55.7 -- not a known variable star
12:31:30.25 +36:54:35.0 -- not a known variable star
12:31:38.50 +35:27:29.4 -- not a known variable star
12:32:06.51 +34:48:00.7 -- not a known variable star
12:32:15.54 +36:51:37.1 -- not a known variable star
12:32:16.65 +35:08:34.1 -- not a known variable star
12:32:16.98 +36:39:57.6 -- not a known variable star
12:32:19.80 +34:34:46.4 -- not a known variable star
12:32:31.39 +36:22:20.8 -- not a known variable star
12:32:33.84 +34:57:15.2 -- not a known variable star
12:32:35.75 +37:15:31.7 -- not a known variable star
12:32:56.67 +35:49:39.1 -- not a known variable star
12:32:57.33 +37:21:20.1 -- not a known variable star
12:32:59.33 +35:44:32.1 -- not a known variable star
12:33:04.18 +35:11:19.6 -- not a known variable star
12:33:10.89 +35:55:23.1 -- not a known variable star
12:33:13.82 +35:46:32.4 -- not a known variable star
12:33:36.48 +35:02:57.8 -- a known variable star
12:33:42.26 +34:38:50.9 -- not a known variable star
12:33:50.70 +35:33:48.9 -- a known variable star
12:33:56.36 +36:19:51.1 -- not a known variable star
12:34:03.07 +37:19:24.1 -- not a known variable star
12:34:05.36 +36:28:00.0 -- not a known variable star
12:34:18.56 +35:26:32.1 -- not a known variable star
12:34:40.98 +36:10:11.3 -- not a known variable star
12:34:44.15 +35:35:45.6 -- not a known variable star
12:34:49.36 +34:23:24.2 -- not a known variable star
12:35:05.83 +34:36:50.2 -- not a known variable star
12:35:22.55 +34:54:08.0 -- not a known variable star
12:35:24.99 +34:18:44.7 -- a known variable star
12:35:25.21 +36:33:38.7 -- a known variable star
12:35:29.02 +35:48:01.3 -- not a known variable star
12:35:32.33 +36:41:18.7 -- not a known variable star
12:35:55.96 +37:12:24.6 -- a known variable star
12:35:56.84 +34:37:38.8 -- not a known variable star
12:36:08.72 +35:38:57.9 -- a known variable star
12:36:18.49 +34:19:26.1 -- not a known variable star
12:36:23.61 +36:47:13.7 -- not a known variable star
12:36:29.75 +34:45:16.5 -- not a known variable star
12:36:30.53 +34:33:08.4 -- not a known variable star
12:37:32.27 +35:53:42.3 -- not a known variable star
12:37:52.54 +33:15:28.8 -- not a known variable star
12:37:56.53 +34:13:33.3 -- not a known variable star
12:38:12.12 +33:51:27.4 -- not a known variable star
12:38:12.38 +34:18:09.8 -- not a known variable star
12:38:23.40 +35:30:56.4 -- not a known variable star
12:38:28.87 +33:50:01.9 -- not a known variable star
12:38:39.24 +34:26:58.9 -- not a known variable star
12:38:42.36 +33:22:33.9 -- not a known variable star
12:38:57.16 +33:51:30.6 -- not a known variable star
12:39:01.38 +35:03:59.9 -- not a known variable star
12:39:26.88 +33:44:01.3 -- not a known variable star
12:39:48.21 +36:01:59.2 -- a known variable star
12:39:49.33 +34:48:58.7 -- not a known variable star
12:39:51.16 +34:18:56.4 -- not a known variable star
12:39:56.27 +35:09:01.7 -- not a known variable star
12:40:01.14 +33:15:12.0 -- not a known variable star
12:40:05.47 +34:07:16.4 -- not a known variable star
12:40:08.24 +35:08:15.6 -- a known variable star
12:40:10.19 +35:28:50.8 -- not a known variable star
12:40:21.74 +33:04:30.8 -- not a known variable star
12:40:33.37 +34:22:55.5 -- a known variable star
12:40:51.61 +35:04:47.6 -- not a known variable star
12:41:10.62 +35:19:01.8 -- not a known variable star
12:41:12.93 +33:22:57.0 -- not a known variable star
12:41:48.91 +34:05:26.7 -- not a known variable star
12:41:59.87 +33:41:18.3 -- not a known variable star
12:42:15.28 +34:20:30.1 -- not a known variable star
12:42:30.95 +34:13:49.0 -- not a known variable star
12:42:45.87 +34:46:39.6 -- not a known variable star
12:42:54.61 +34:00:10.7 -- not a known variable star
12:43:02.18 +35:01:01.3 -- not a known variable star
12:43:32.79 +34:25:12.7 -- a known variable star
12:44:07.66 +34:23:07.2 -- a known variable star
12:44:29.46 +34:30:28.0 -- not a known variable star
12:44:34.61 +33:11:32.1 -- not a known variable star
12:44:55.56 +33:09:48.2 -- not a known variable star
12:45:15.75 +34:42:52.8 -- not a known variable star
12:45:23.26 +33:15:36.1 -- a known variable star
12:45:34.45 +33:06:52.7 -- not a known variable star
12:45:34.48 +33:24:06.5 -- not a known variable star
12:45:45.98 +33:43:15.9 -- not a known variable star
12:46:57.15 +33:05:15.7 -- not a known variable star
12:48:24.99 +33:18:11.1 -- not a known variable star
12:49:39.45 +33:05:29.8 -- not a known variable star
13:38:59.94 +41:09:43.8 -- not a known variable star
Found 98 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
114 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 114 (excluding asteroids and hot pixels, 98 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)2461290.62484846 -observatory V36
11:37:48.98 +03:35:37.4 Mercury (-0.9mag)
13:35:37.93 -14:27:17.6 Venus (-4.7mag)
07:13:31.40 +22:59:31.8 Mars (1.2mag)
09:08:54.48 +16:58:08.7 Jupiter (-1.8mag)
00:51:46.38 +02:38:54.6 Saturn (0.4mag)
04:13:41.14 +21:01:59.0 Uranus (5.7mag)
00:13:45.78 -00:03:07.0 Neptune (7.7mag)
20:25:36.32 -23:39:34.6 Pluto (14.5mag)
07:34:13.54 +24:07:24.0 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 362 Sep 7 00:09 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461290.62484846:
09:09:00.89 +16:57:37.5 Io (6.2mag)
09:08:53.01 +16:58:17.1 Europa (6.3mag)
09:09:05.80 +16:57:11.7 Ganymede (5.7mag)
09:08:29.34 +17:00:12.5 Callisto (6.9mag)
09:06:40.38 +17:14:36.3 Himalia (15.7mag)
09:08:55.38 +16:58:04.7 Thebe (16.6mag)
09:06:17.73 +17:08:35.6 Elara (17.7mag)
09:12:48.36 +16:25:46.3 Pasiphae (17.9mag)
09:10:00.28 +17:15:52.5 Carme (19.0mag)
00:51:43.21 +02:39:17.9 Titan (8.3mag)
00:51:39.65 +02:38:50.9 Rhea (9.6mag)
00:52:02.06 +02:41:26.3 Iapetus (11.0mag)
00:52:00.22 +02:38:20.3 Hyperion (14.3mag)
00:50:33.34 +02:28:39.8 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 7 00:09 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461290.62484846:
22:03:58.05 +00:49:33.9 JWST
17:29:04.25 +38:53:33.4 Chandra
09:18:44.23 -52:18:54.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 7 00:09 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461290.62484846 -observatory V36
03:40:19.30 +19:19:55.5 17.4mag P/1996 R2 (Lagerkvist)
18:02:51.07 -34:12:53.0 14.3mag P/2010 H2 (Vales)
07:19:20.38 -70:17:31.1 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:40.37 +33:41:44.9 17.7mag C/2017 K2 (PANSTARRS)
04:51:10.09 +45:27:03.1 15.8mag P/2021 N1 (ZTF)
04:51:10.09 +45:27:03.1 15.8mag P/2021 N1 (ZTF)
04:51:10.09 +45:27:03.1 15.8mag P/2021 N1 (ZTF)
04:51:10.09 +45:27:03.1 15.8mag P/2021 N1 (ZTF)
04:51:10.09 +45:27:03.1 15.8mag P/2021 N1 (ZTF)
22:13:37.43 +28:41:28.8 17.4mag C/2022 E2 (ATLAS)
07:10:03.65 +25:58:55.1 16.9mag C/2022 N2 (PANSTARRS)
10:49:20.28 +27:13:56.3 17.1mag C/2022 QE78 (ATLAS)
09:48:33.61 +05:14:02.4 18.0mag C/2022 R6 (PANSTARRS)
15:29:34.85 -15:38:03.4 14.8mag C/2023 R1 (PANSTARRS)
08:38:14.41 +32:52:54.0 15.8mag C/2024 E1 (Wierzchos)
15:06:34.34 +15:19:30.3 17.9mag C/2024 G6 (ATLAS)
18:33:43.13 +43:10:54.1 13.7mag C/2024 J3 (ATLAS)
20:26:24.42 +49:18:39.0 17.4mag C/2024 R4 (PANSTARRS)
05:35:30.93 -13:01:26.9 15.1mag C/2024 T5 (ATLAS)
07:11:34.21 +18:34:39.9 17.8mag C/2025 J1 (Borisov)
11:17:42.17 +18:46:57.3 16.8mag C/2025 V2 (Rankin)
13:19:28.95 +00:07:48.6 16.8mag C/2025 Y1 (ATLAS)
16:40:56.28 +74:03:48.2 16.1mag C/2026 A2 (Bok)
03:05:52.81 +46:08:24.2 17.4mag C/2026 B2 (Sun-Gao)
12:13:06.67 +11:16:08.1 17.5mag A/2026 E1
22:25:52.73 -35:01:43.4 13.4mag 10P/Tempel
01:19:13.52 +36:59:43.7 17.9mag 11P/Tempel-Swift-LINEAR
11:48:03.32 -05:27:19.1 16.3mag 29P/Schwassmann-Wachmann
12:08:13.31 -05:02:25.3 17.6mag 63P/Wild
00:44:45.88 -07:03:30.6 15.4mag 65P/Gunn
06:38:59.82 +19:15:54.2 17.1mag 78P/Gehrels
03:17:16.26 +14:59:45.4 16.7mag 88P/Howell
05:37:38.88 +28:33:53.2 17.5mag 112P/Urata-Niijima
07:31:17.28 +24:51:36.9 17.9mag 114P/Wiseman-Skiff
10:27:30.41 +20:54:15.3 14.8mag 123P/West-Hartley
12:46:13.12 -21:16:43.9 17.4mag 124P/Mrkos
06:17:12.44 +20:38:39.7 15.9mag 128P/Shoemaker-Holt
02:32:52.77 -17:37:53.7 15.2mag 161P/Hartley-IRAS
09:37:53.88 +13:51:02.0 12.1mag 169P/NEAT
03:24:17.81 +08:29:20.1 14.5mag 220P/McNaught
04:47:36.35 +36:15:57.7 15.2mag 260P/McNaught
08:31:24.79 +35:43:09.3 17.3mag 295P/LINEAR
15:25:07.37 -00:13:47.1 17.9mag 391P/Kowalski
09:27:38.17 +16:51:32.9 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.2K Sep 7 00:09 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
-rw-r--r-- 1 apache apache 190K Sep 7 00:09 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
00:34:06.502 +12:42:13.91 AT 2026ypz 2026-08-08.10 20
21:30:05.008 +02:38:33.95 AT 2026ypy 2026-08-06.53 20.21
21:00:04.179 -04:29:11.16 AT 2026ypx 2026-08-10.99 20.06
02:37:12.256 +15:20:39.63 AT 2026ypw 2026-08-12.19 20.13
20:30:21.422 +77:41:45.40 AT 2026ypv 2026-08-02.23 20.4969
13:32:08.201 +00:21:43.54 AT 2026ypu 2026-08-05.16 19.6868
14:07:14.862 +00:31:05.95 AT 2026ypt 2026-08-08.16 20.0684
17:39:38.555 +44:15:43.22 AT 2026yps 2026-07-22.33 20.9161
23:51:42.078 +03:04:27.33 AT 2026ypr 2026-08-12.07 20.05
02:34:15.880 +40:31:56.36 AT 2026ypq 2026-08-11.58 18.82
15:38:07.902 +06:01:37.84 AT 2026ypp 2026-08-11.26 20.34
15:24:17.953 +11:26:31.29 AT 2026ypo 2026-08-11.26 20.8
14:21:16.003 +25:15:33.98 AT 2026ypn 2026-08-11.26 18.72
16:23:56.085 +09:36:23.21 AT 2026ypm 2026-08-11.28 20.97
20:54:11.595 +10:54:51.15 SN 2026ypl 2026-08-09.34 20.4
00:40:25.122 +24:26:45.82 AT 2026ypk 2026-08-07.45 20.4501
17:05:06.872 +77:16:36.60 AT 2026ypj 2026-08-11.31 18.807
20:49:46.878 -06:36:38.40 AT 2026ypi 2026-08-09.29 20.4359
00:12:21.150 -17:28:55.44 AT 2026yph 2026-08-08.42 20.4034
00:48:58.972 +17:28:17.78 AT 2026ypg 2026-08-05.48 20.2336
-rw-r--r-- 1 apache apache 88K Sep 7 00:09 tns_transients_list.txt
