This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs
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 10 11.3564 2461324.8564 12.12 07:05:58.00 -14:01:10.6
227.05522 -3.19656 galactic CMa Second-epoch detections are separated by 1.9" and 7.5 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 | 07:05:58.00 -14:01:10.6 (user input) | T | P | (position from user input) J-Ks=0.847+/-0.033 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:58.00 -14:01:10.6: 13.22 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:58.00 -14:01:10.6: 13.32 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.26 +/- 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,2461324.8564,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.3564 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 10 11.3564 2461324.8564 12.20 07:05:04.89 -14:04:33.8
227.00739 -3.41333 galactic CMa Second-epoch detections are separated by 1.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.2703-14.0759 | 07:05:04.89 -14:04:33.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.812+/-0.033 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:04.89 -14:04:33.8: 13.31 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:04.89 -14:04:33.8: 13.28 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.2703-14.0759,2461324.8564,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.2703-14.0759 20261011.3564 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 10 11.3564 2461324.8564 12.22 07:09:42.94 -13:25:52.4
226.94972 -2.11764 galactic CMa Second-epoch detections are separated by 2.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.4261-13.4407 | 07:09:42.28 -13:26:26.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.296+/-0.036 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:42.94 -13:25:52.4: 13.28 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:42.94 -13:25:52.4: 13.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4261-13.4407,2461324.8564,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4261-13.4407 20261011.3564 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 10 11.3564 2461324.8564 12.12 07:05:43.87 -13:54:15.5
226.92635 -3.19473 galactic CMa Second-epoch detections are separated by 2.4" and 7.4 pix
The object was found in VSX20" Gaia DR3 3044523611135893248
Type: ROT
# Max. Min./Amp. JD0 Period
18.320 G 18.460 G
ATTENTION: measured mag 12.12 is 6.2 mag brighter than the VSX record maximum brightness 18.32 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:43.87 -13:54:15.5: 13.40 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:43.87 -13:54:15.5: 13.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 3044523611135893248,2461324.8564,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044523611135893248 20261011.3564 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 10 11.3564 2461324.8564 12.29 07:05:51.49 -13:40:57.7
226.74302 -3.06607 galactic CMa Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.4646-13.6828 | 07:05:51.49 -13:40:57.7 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.927+/-0.029 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:51.49 -13:40:57.7: 13.48 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:51.49 -13:40:57.7: 13.58 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4646-13.6828,2461324.8564,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4646-13.6828 20261011.3564 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 10 11.3564 2461324.8564 10.93 07:05:42.40 -13:56:55.1
226.96313 -3.22026 galactic CMa Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.4265-13.9485 | 07:05:42.36 -13:56:54.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.206+/-0.033 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:42.40 -13:56:55.1: 11.77 +/- 0.01 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:42.40 -13:56:55.1: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4265-13.9485,2461324.8564,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4265-13.9485 20261011.3564 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 12.21 07:09:10.99 -13:53:31.6
227.29975 -2.44449 galactic CMa Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2965-13.8922 | 07:09:10.99 -13:53:31.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:10.99 -13:53:31.6: 13.47 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:10.99 -13:53:31.6: 13.40 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2965-13.8922,2461324.8564,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2965-13.8922 20261011.3564 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 10 11.3564 2461324.8564 11.11 07:05:29.73 -14:01:32.5
227.00838 -3.30101 galactic CMa Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.3851-14.0203 | 07:05:32.44 -14:01:13.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M1.5II-III 2010MacCon.unpub..M UCAC2 26624105 J-Ks=0.181+/-0.033 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:29.73 -14:01:32.5: 12.00 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:29.73 -14:01:32.5: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3851-14.0203,2461324.8564,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3851-14.0203 20261011.3564 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.19 07:04:28.87 -14:03:21.3
226.92296 -3.53374 galactic CMa Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.1204-14.0559 | 07:04:28.92 -14:03:21.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.697+/-0.031 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:28.87 -14:03:21.3: 12.02 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:28.87 -14:03:21.3: 12.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1204-14.0559,2461324.8564,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1204-14.0559 20261011.3564 11.19CV 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 10 11.3564 2461324.8564 11.14 07:09:32.38 -14:01:26.9
227.45690 -2.42837 galactic CMa Second-epoch detections are separated by 0.6" and 7.3 pix
The object was found in VSX 1" Gaia DR3 3044471422996310272
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.970 G 12.030 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:32.38 -14:01:26.9: 12.09 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:32.38 -14:01:26.9: 12.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.09 +/- 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 3044471422996310272,2461324.8564,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044471422996310272 20261011.3564 11.14CV 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 10 11.3564 2461324.8564 11.22 07:06:00.79 -14:03:10.6
227.09008 -3.20175 galactic CMa Second-epoch detections are separated by 1.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.5032-14.0530 | 07:06:00.79 -14:03:10.9 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1971PW&SO...1a...1S LS 161 J-Ks=0.120+/-0.032 (A)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:00.79 -14:03:10.6: 12.14 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:00.79 -14:03:10.6: 12.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.5032-14.0530,2461324.8564,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5032-14.0530 20261011.3564 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.31 07:05:35.89 -13:42:00.8
226.72974 -3.13025 galactic CMa Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.3995-13.7000 | 07:05:35.89 -13:42:00.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.412+/-0.035 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:35.89 -13:42:00.8: 12.15 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:35.89 -13:42:00.8: 12.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3995-13.7000,2461324.8564,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3995-13.7000 20261011.3564 11.31CV 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 10 11.3564 2461324.8564 11.29 07:09:39.63 -14:03:02.4
227.49397 -2.41455 galactic CMa Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.4152-14.0506 | 07:09:39.66 -14:03:02.3 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.669+/-0.040 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:39.63 -14:03:02.4: 12.26 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:39.63 -14:03:02.4: 12.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4152-14.0506,2461324.8564,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4152-14.0506 20261011.3564 11.29CV 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 10 11.3564 2461324.8564 11.57 07:08:15.62 -14:01:49.0
227.31971 -2.70682 galactic CMa Second-epoch detections are separated by 0.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.0648-14.0303 | 07:08:15.57 -14:01:49.4 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.363+/-0.030 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:15.62 -14:01:49.0: 12.47 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:15.62 -14:01:49.0: 12.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0648-14.0303,2461324.8564,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0648-14.0303 20261011.3564 11.57CV 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 10 11.3564 2461324.8564 11.49 07:08:57.25 -14:09:08.1
227.50549 -2.61334 galactic CMa Second-epoch detections are separated by 1.4" and 7.1 pix
The object was found in VSX 0" Gaia DR3 3044468566836340352
Type: ROT
# Max. Min./Amp. JD0 Period
12.370 G 12.410 G G
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:57.25 -14:09:08.1: 12.49 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:57.25 -14:09:08.1: 12.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.52 +/- 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 3044468566836340352,2461324.8564,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044468566836340352 20261011.3564 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.73 07:04:06.93 -14:07:11.7
226.93961 -3.64183 galactic CMa Second-epoch detections are separated by 1.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.0289-14.1199 | 07:04:06.94 -14:07:11.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.664+/-0.031 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:06.93 -14:07:11.7: 12.57 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:06.93 -14:07:11.7: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.57 +/- 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 J106.0289-14.1199,2461324.8564,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0289-14.1199 20261011.3564 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.59 07:06:06.86 -13:52:57.1
226.94949 -3.10206 galactic CMa Second-epoch detections are separated by 1.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.5285-13.8826 | 07:06:06.86 -13:52:57.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.290+/-0.035 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:06.86 -13:52:57.1: 12.51 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:06.86 -13:52:57.1: 12.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 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 J106.5285-13.8826,2461324.8564,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5285-13.8826 20261011.3564 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.64 07:06:30.73 -13:26:20.8
226.59889 -2.81333 galactic CMa Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.6280-13.4390 | 07:06:30.74 -13:26:20.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.916+/-0.033 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:30.73 -13:26:20.8: 12.63 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:30.73 -13:26:20.8: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.64 +/- 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 J106.6280-13.4390,2461324.8564,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6280-13.4390 20261011.3564 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.77 07:07:15.75 -13:41:05.7
226.90127 -2.76376 galactic CMa Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.8158-13.6850 | 07:07:15.81 -13:41:06.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.733+/-0.033 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:15.75 -13:41:05.7: 12.66 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:15.75 -13:41:05.7: 12.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.69 +/- 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
ATO J106.8158-13.6850,2461324.8564,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.8158-13.6850 20261011.3564 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.82 07:07:59.71 -13:22:12.9
226.70307 -2.46122 galactic CMa Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.9986-13.3703 | 07:07:59.71 -13:22:12.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.334+/-0.032 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:59.71 -13:22:12.9: 12.70 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:59.71 -13:22:12.9: 12.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 J106.9986-13.3703,2461324.8564,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.9986-13.3703 20261011.3564 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.81 07:09:05.02 -14:03:20.5
227.43407 -2.54109 galactic CMa Second-epoch detections are separated by 0.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2707-14.0556 | 07:09:05.02 -14:03:20.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.299+/-0.035 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:05.02 -14:03:20.5: 12.78 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:05.02 -14:03:20.5: 12.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.75 +/- 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 J107.2707-14.0556,2461324.8564,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2707-14.0556 20261011.3564 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 10 11.3564 2461324.8564 11.84 07:09:45.43 -13:38:19.2
227.13867 -2.20416 galactic CMa Second-epoch detections are separated by 0.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.4392-13.6387 | 07:09:45.43 -13:38:19.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.350+/-0.038 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:45.43 -13:38:19.2: 12.80 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:45.43 -13:38:19.2: 12.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 J107.4392-13.6387,2461324.8564,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4392-13.6387 20261011.3564 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.91 07:09:04.23 -13:49:41.3
227.23030 -2.43938 galactic CMa Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2677-13.8283 | 07:09:04.23 -13:49:41.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.814+/-0.033 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:04.23 -13:49:41.3: 12.83 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:04.23 -13:49:41.3: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 J107.2677-13.8283,2461324.8564,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2677-13.8283 20261011.3564 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 10 11.3564 2461324.8564 11.88 07:09:11.26 -14:08:16.7
227.51882 -2.55650 galactic CMa Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2972-14.1380 | 07:09:11.26 -14:08:16.7 (user input) | MSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.832+/-0.033 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:11.26 -14:08:16.7: 12.94 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:11.26 -14:08:16.7: 13.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 J107.2972-14.1380,2461324.8564,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2972-14.1380 20261011.3564 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.94 07:09:19.63 -14:04:46.4
227.48245 -2.49961 galactic CMa Second-epoch detections are separated by 0.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3318-14.0794 | 07:09:19.63 -14:04:46.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.268+/-0.033 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:19.63 -14:04:46.4: 12.99 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:19.63 -14:04:46.4: 13.04 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 J107.3318-14.0794,2461324.8564,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3318-14.0794 20261011.3564 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 10 11.3564 2461324.8564 12.05 07:05:58.60 -13:42:04.5
226.77272 -3.04894 galactic CMa Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.4942-13.7011 | 07:05:58.60 -13:42:04.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.747+/-0.032 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:58.60 -13:42:04.5: 13.10 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:58.60 -13:42:04.5: 13.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4942-13.7011,2461324.8564,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4942-13.7011 20261011.3564 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 12.03 07:08:43.37 -13:38:04.2
227.01933 -2.42540 galactic CMa Second-epoch detections are separated by 0.4" and 7.3 pix
The object was found in VSX 2" GDS_J0708434-133804
Type: VAR
# Max. Min./Amp. JD0 Period
12.670 r Y 0.200 r
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:43.37 -13:38:04.2: 13.13 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:43.37 -13:38:04.2: 13.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.12 +/- 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
GDS_J0708434-133804,2461324.8564,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0708434-133804 20261011.3564 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 10 11.3564 2461324.8564 11.99 07:06:48.83 -13:36:32.5
226.78375 -2.82591 galactic CMa Second-epoch detections are separated by 1.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.6957-13.6194 | 07:06:46.98 -13:37:10.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.853+/-0.031 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:48.83 -13:36:32.5: 13.16 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:48.83 -13:36:32.5: 13.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.6957-13.6194,2461324.8564,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6957-13.6194 20261011.3564 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 12.12 07:07:55.10 -12:57:33.2
226.32899 -2.28918 galactic CMa Second-epoch detections are separated by 0.6" and 7.3 pix
The object was found in VSX 6" Gaia DR3 3044869205683784576
Type: E
# Max. Min./Amp. JD0 Period
18.960 G 19.580 G 1.355760000000
ATTENTION: measured mag 12.12 is 6.8 mag brighter than the VSX record maximum brightness 18.96 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:55.10 -12:57:33.2: 13.17 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:55.10 -12:57:33.2: 13.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3044869205683784576,2461324.8564,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044869205683784576 20261011.3564 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 10 11.3564 2461324.8564 12.06 07:09:29.40 -14:02:13.5
227.46286 -2.44502 galactic CMa Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3725-14.0370 | 07:09:29.40 -14:02:13.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.809+/-0.034 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:29.40 -14:02:13.5: 13.14 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:29.40 -14:02:13.5: 13.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3725-14.0370,2461324.8564,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3725-14.0370 20261011.3564 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 10 11.3564 2461324.8564 12.14 07:09:26.92 -13:38:23.1
227.10512 -2.27121 galactic CMa Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3624-13.6398 | 07:09:26.92 -13:38:23.1 (user input) | MSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.223+/-0.038 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:26.92 -13:38:23.1: 13.19 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:26.92 -13:38:23.1: 13.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3624-13.6398,2461324.8564,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3624-13.6398 20261011.3564 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 10 11.3564 2461324.8564 12.04 07:09:13.88 -13:56:14.0
227.34523 -2.45484 galactic CMa Second-epoch detections are separated by 1.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3080-13.9371 | 07:09:13.88 -13:56:14.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.305+/-0.034 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:13.88 -13:56:14.0: 13.11 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:13.88 -13:56:14.0: 13.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3080-13.9371,2461324.8564,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3080-13.9371 20261011.3564 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 10 11.3564 2461324.8564 12.08 07:05:01.06 -14:09:59.8
227.08107 -3.46839 galactic CMa Second-epoch detections are separated by 2.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.2534-14.1660 | 07:05:01.06 -14:09:59.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:01.06 -14:09:59.8: 13.12 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:01.06 -14:09:59.8: 13.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.2534-14.1660,2461324.8564,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.2534-14.1660 20261011.3564 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 12.12 07:06:04.59 -13:42:22.7
226.78832 -3.02969 galactic CMa Second-epoch detections are separated by 1.6" and 7.4 pix
The object was found in VSX 2" Gaia DR3 3044535229031056512
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.140 G 13.170 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:04.59 -13:42:22.7: 13.10 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:04.59 -13:42:22.7: 13.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3044535229031056512,2461324.8564,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044535229031056512 20261011.3564 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 10 11.3564 2461324.8564 11.98 07:05:45.96 -13:58:36.5
226.99481 -3.22032 galactic CMa Second-epoch detections are separated by 0.7" and 7.4 pix
The object was found in VSX15" Gaia DR3 3044509974623574272
Type: ROT
# Max. Min./Amp. JD0 Period
17.150 G 17.200 G K
ATTENTION: measured mag 11.98 is 5.2 mag brighter than the VSX record maximum brightness 17.15 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:45.96 -13:58:36.5: 13.08 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:45.96 -13:58:36.5: 13.18 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 3044509974623574272,2461324.8564,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044509974623574272 20261011.3564 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 10 11.3564 2461324.8564 11.99 07:05:24.98 -14:02:52.4
227.01939 -3.32823 galactic CMa Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.3541-14.0478 | 07:05:24.98 -14:02:52.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.175+/-0.037 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:24.98 -14:02:52.4: 13.05 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:24.98 -14:02:52.4: 13.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3541-14.0478,2461324.8564,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3541-14.0478 20261011.3564 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 12.07 07:07:53.83 -14:04:32.8
227.31976 -2.80596 galactic CMa Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.9741-14.0754 | 07:07:53.83 -14:04:32.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.691+/-0.033 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:53.83 -14:04:32.8: 13.02 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:53.83 -14:04:32.8: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 J106.9741-14.0754,2461324.8564,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.9741-14.0754 20261011.3564 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 10 11.3564 2461324.8564 11.95 07:09:05.91 -13:53:47.2
227.29415 -2.46473 galactic CMa Second-epoch detections are separated by 0.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2745-13.8968 | 07:09:05.91 -13:53:47.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.904+/-0.033 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:05.91 -13:53:47.2: 13.05 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:05.91 -13:53:47.2: 13.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.03 +/- 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 J107.2745-13.8968,2461324.8564,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2745-13.8968 20261011.3564 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.96 07:08:28.85 -14:06:43.6
227.41706 -2.69686 galactic CMa Second-epoch detections are separated by 1.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.1198-14.1120 | 07:08:28.85 -14:06:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.559+/-0.033 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:28.85 -14:06:43.6: 12.98 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:28.85 -14:06:43.6: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 J107.1198-14.1120,2461324.8564,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1198-14.1120 20261011.3564 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 10 11.3564 2461324.8564 11.94 07:06:22.60 -13:25:31.0
226.57148 -2.83630 galactic CMa Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.6056-13.4318 | 07:06:25.34 -13:25:54.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.333+/-0.032 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:22.60 -13:25:31.0: 12.97 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:22.60 -13:25:31.0: 13.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 J106.6056-13.4318,2461324.8564,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6056-13.4318 20261011.3564 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 10 11.3564 2461324.8564 11.98 07:08:05.83 -13:25:34.5
226.76427 -2.46488 galactic CMa Second-epoch detections are separated by 1.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.0247-13.4240 | 07:08:05.83 -13:25:34.5 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.114+/-0.032 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:05.83 -13:25:34.5: 12.98 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:05.83 -13:25:34.5: 12.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 J107.0247-13.4240,2461324.8564,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0247-13.4240 20261011.3564 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 10 11.3564 2461324.8564 11.93 07:09:10.29 -13:41:36.4
227.12185 -2.35569 galactic CMa Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2929-13.6935 | 07:09:10.29 -13:41:36.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.233+/-0.038 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:10.29 -13:41:36.4: 12.96 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:10.29 -13:41:36.4: 12.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.94 +/- 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 J107.2929-13.6935,2461324.8564,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2929-13.6935 20261011.3564 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.92 07:09:23.71 -14:07:36.1
227.53194 -2.50664 galactic CMa Second-epoch detections are separated by 1.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3487-14.1271 | 07:09:23.71 -14:07:36.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.173+/-0.033 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:23.71 -14:07:36.1: 12.98 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:23.71 -14:07:36.1: 12.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3487-14.1271,2461324.8564,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3487-14.1271 20261011.3564 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 10 11.3564 2461324.8564 11.97 07:08:28.88 -14:00:34.6
227.32595 -2.64971 galactic CMa Second-epoch detections are separated by 1.2" and 7.3 pix
The object was found in VSX 1" Gaia DR3 3044474274854599424
Type: ROT
# Max. Min./Amp. JD0 Period
12.790 G 12.820 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:28.88 -14:00:34.6: 12.96 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:28.88 -14:00:34.6: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 3044474274854599424,2461324.8564,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044474274854599424 20261011.3564 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 12.04 07:06:45.43 -13:04:15.4
226.29855 -2.59176 galactic CMa Second-epoch detections are separated by 1.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.6894-13.0706 | 07:06:45.43 -13:04:15.4 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.171+/-0.037 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:45.43 -13:04:15.4: 12.94 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:45.43 -13:04:15.4: 12.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 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 J106.6894-13.0706,2461324.8564,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6894-13.0706 20261011.3564 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 10 11.3564 2461324.8564 11.86 07:06:49.70 -13:27:28.7
226.65091 -2.75362 galactic CMa Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.7075-13.4578 | 07:06:48.37 -13:26:55.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.920+/-0.033 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:49.70 -13:27:28.7: 12.92 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:49.70 -13:27:28.7: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 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 J106.7075-13.4578,2461324.8564,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.7075-13.4578 20261011.3564 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.87 07:05:44.04 -13:47:21.9
226.82430 -3.14165 galactic CMa Second-epoch detections are separated by 1.9" and 7.3 pix
The object was found in VSX24" Gaia DR3 3044525672720508416
Type: E
# Max. Min./Amp. JD0 Period
16.700 G 16.780 G 0.467180000000 A
ATTENTION: measured mag 11.87 is 4.8 mag brighter than the VSX record maximum brightness 16.70 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:44.04 -13:47:21.9: 12.89 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:44.04 -13:47:21.9: 12.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 3044525672720508416,2461324.8564,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044525672720508416 20261011.3564 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.96 07:09:25.12 -13:58:59.6
227.40703 -2.43562 galactic CMa Second-epoch detections are separated by 3.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3652-13.9813 | 07:09:27.65 -13:58:52.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.799+/-0.033 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:25.12 -13:58:59.6: 12.89 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:25.12 -13:58:59.6: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3652-13.9813,2461324.8564,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3652-13.9813 20261011.3564 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 10 11.3564 2461324.8564 11.80 07:06:12.23 -13:44:14.7
226.83019 -3.01641 galactic CMa Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.5510-13.7374 | 07:06:12.25 -13:44:14.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.791+/-0.030 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:12.23 -13:44:14.7: 12.88 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:12.23 -13:44:14.7: 12.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.5510-13.7374,2461324.8564,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5510-13.7374 20261011.3564 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.90 07:09:18.69 -13:59:28.4
227.40218 -2.46239 galactic CMa Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3279-13.9912 | 07:09:18.69 -13:59:28.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.259+/-0.034 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:18.69 -13:59:28.4: 12.82 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:18.69 -13:59:28.4: 12.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 J107.3279-13.9912,2461324.8564,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3279-13.9912 20261011.3564 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 10 11.3564 2461324.8564 11.86 07:09:42.73 -13:36:41.8
227.10959 -2.20142 galactic CMa Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was found in ASASSN-V 2" ASASSN-V J070942.62-133641.4
Type: SR
MeanMag 13.19 m Amp. 0.1 m Period 212.2040441 d
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:42.73 -13:36:41.8: 12.85 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:42.73 -13:36:41.8: 12.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.87 +/- 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
VARIABLE_NAME,2461324.8564,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.3564 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.98 07:07:45.89 -13:28:55.8
226.77689 -2.56233 galactic CMa Second-epoch detections are separated by 1.2" 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 | ATO J106.9415-13.4820 | 07:07:45.97 -13:28:55.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.161+/-0.033 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:45.89 -13:28:55.8: 12.87 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:45.89 -13:28:55.8: 12.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.89 +/- 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 J106.9415-13.4820,2461324.8564,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.9415-13.4820 20261011.3564 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 10 11.3564 2461324.8564 11.83 07:05:58.17 -13:50:32.2
226.89755 -3.11494 galactic CMa Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.4924-13.8420 | 07:05:58.17 -13:50:32.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.213+/-0.032 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:58.17 -13:50:32.2: 12.82 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:58.17 -13:50:32.2: 12.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 J106.4924-13.8420,2461324.8564,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4924-13.8420 20261011.3564 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.84 07:08:27.43 -14:08:48.0
227.44516 -2.71781 galactic CMa Second-epoch detections are separated by 0.2" and 7.3 pix
The object was found in VSX 8" ZTF J070827.19-140840.3
Type: EW
# Max. Min./Amp. JD0 Period
15.634 g Y 0.594 g 2458481.77760 0.455879600000
ATTENTION: measured mag 11.84 is 3.2 mag brighter than the VSX record maximum brightness 15.04 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:27.43 -14:08:48.0: 12.77 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:27.43 -14:08:48.0: 12.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J070827.19-140840.3,2461324.8564,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J070827.19-140840.3 20261011.3564 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.85 07:04:30.77 -13:56:57.3
226.83134 -3.47831 galactic CMa Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.1281-13.9495 | 07:04:30.77 -13:56:57.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.243+/-0.033 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:30.77 -13:56:57.3: 12.76 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:30.77 -13:56:57.3: 12.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.76 +/- 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 J106.1281-13.9495,2461324.8564,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1281-13.9495 20261011.3564 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.87 07:06:02.84 -13:24:57.4
226.52649 -2.90324 galactic CMa Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.5118-13.4158 | 07:06:02.84 -13:24:57.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.245+/-0.030 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:02.84 -13:24:57.4: 12.76 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:02.84 -13:24:57.4: 12.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 J106.5118-13.4158,2461324.8564,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5118-13.4158 20261011.3564 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.85 07:07:32.28 -13:13:35.8
226.52425 -2.49416 galactic CMa Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.8847-13.2264 | 07:07:32.33 -13:13:35.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.768+/-0.030 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:32.28 -13:13:35.8: 12.77 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:32.28 -13:13:35.8: 12.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.72 +/- 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 J106.8847-13.2264,2461324.8564,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.8847-13.2264 20261011.3564 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.72 07:09:25.25 -13:58:31.3
227.40028 -2.43154 galactic CMa Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3652-13.9813 | 07:09:27.65 -13:58:52.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.459+/-0.037 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:25.25 -13:58:31.3: 12.74 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:25.25 -13:58:31.3: 12.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.73 +/- 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 J107.3652-13.9813,2461324.8564,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3652-13.9813 20261011.3564 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.69 07:06:03.29 -13:48:18.0
226.87382 -3.07948 galactic CMa Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.5136-13.8050 | 07:06:03.28 -13:48:18.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.703+/-0.031 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:03.29 -13:48:18.0: 12.74 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:03.29 -13:48:18.0: 12.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 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 J106.5136-13.8050,2461324.8564,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5136-13.8050 20261011.3564 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.84 07:09:27.09 -13:29:22.5
226.97200 -2.20152 galactic CMa Second-epoch detections are separated by 0.8" 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 | 07:09:27.09 -13:29:22.5 (user input) | T | P | (position from user input) J-Ks=0.299+/-0.032 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:27.09 -13:29:22.5: 12.74 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:27.09 -13:29:22.5: 12.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.76 +/- 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,2461324.8564,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261011.3564 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.68 07:08:53.33 -14:04:30.4
227.42962 -2.59198 galactic CMa Second-epoch detections are separated by 2.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2141-14.0744 | 07:08:51.40 -14:04:27.8 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.787+/-0.033 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:53.33 -14:04:30.4: 12.68 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:53.33 -14:04:30.4: 12.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 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 J107.2141-14.0744,2461324.8564,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2141-14.0744 20261011.3564 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.88 07:06:45.65 -13:03:00.9
226.28054 -2.58148 galactic CMa Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.6900-13.0500 | 07:06:45.65 -13:03:00.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.827+/-0.033 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:45.65 -13:03:00.9: 12.74 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:45.65 -13:03:00.9: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 J106.6900-13.0500,2461324.8564,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6900-13.0500 20261011.3564 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.86 07:08:00.75 -13:20:33.2
226.68038 -2.44477 galactic CMa Second-epoch detections are separated by 1.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.0034-13.3426 | 07:08:00.75 -13:20:33.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.113+/-0.033 (A)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:00.75 -13:20:33.2: 12.72 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:00.75 -13:20:33.2: 12.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.73 +/- 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 J107.0034-13.3426,2461324.8564,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0034-13.3426 20261011.3564 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.82 07:08:49.57 -13:55:21.4
227.28702 -2.53545 galactic CMa Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2065-13.9226 | 07:08:49.57 -13:55:21.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.358+/-0.034 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:49.57 -13:55:21.4: 12.67 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:49.57 -13:55:21.4: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.67 +/- 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 J107.2065-13.9226,2461324.8564,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2065-13.9226 20261011.3564 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.70 07:09:42.39 -13:32:26.3
227.04590 -2.16998 galactic CMa Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.4268-13.5405 | 07:09:42.43 -13:32:25.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.141+/-0.035 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:42.39 -13:32:26.3: 12.66 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:42.39 -13:32:26.3: 12.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.64 +/- 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 J107.4268-13.5405,2461324.8564,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4268-13.5405 20261011.3564 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 10 11.3564 2461324.8564 11.67 07:06:50.67 -13:30:13.3
226.69341 -2.77106 galactic CMa Second-epoch detections are separated by 1.2" and 7.3 pix
The object was found in VSX 0" Gaia DR3 3044563541456445568
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.590 G 12.610 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:50.67 -13:30:13.3: 12.65 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:50.67 -13:30:13.3: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 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 3044563541456445568,2461324.8564,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044563541456445568 20261011.3564 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.61 07:05:35.18 -13:47:41.1
226.81265 -3.17598 galactic CMa Second-epoch detections are separated by 1.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.3969-13.7946 | 07:05:35.26 -13:47:40.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.850+/-0.032 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:35.18 -13:47:41.1: 12.64 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:35.18 -13:47:41.1: 12.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 J106.3969-13.7946,2461324.8564,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3969-13.7946 20261011.3564 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.77 07:08:34.04 -14:03:41.5
227.38170 -2.65501 galactic CMa Second-epoch detections are separated by 0.1" and 7.2 pix
The object was found in VSX 6" Gaia DR3 3044473037904018816
Type: ROT
# Max. Min./Amp. JD0 Period
15.690 G 15.730 G 3.895930000000 K
ATTENTION: measured mag 11.77 is 3.9 mag brighter than the VSX record maximum brightness 15.69 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:34.04 -14:03:41.5: 12.65 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:34.04 -14:03:41.5: 12.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 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 3044473037904018816,2461324.8564,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044473037904018816 20261011.3564 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.66 07:06:14.63 -13:36:34.3
226.72075 -2.94929 galactic CMa Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.5610-13.6096 | 07:06:14.66 -13:36:34.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.024+/-0.030 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:14.63 -13:36:34.3: 12.64 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:14.63 -13:36:34.3: 12.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 J106.5610-13.6096,2461324.8564,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5610-13.6096 20261011.3564 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.69 07:06:06.37 -13:52:36.9
226.94359 -3.10126 galactic CMa Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.5263-13.8769 | 07:06:06.37 -13:52:36.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.177+/-0.033 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:06.37 -13:52:36.9: 12.57 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:06.37 -13:52:36.9: 12.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.5263-13.8769,2461324.8564,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5263-13.8769 20261011.3564 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.65 07:06:57.92 -13:31:14.6
226.72203 -2.75274 galactic CMa Second-epoch detections are separated by 1.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.7427-13.5210 | 07:06:57.92 -13:31:14.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.839+/-0.038 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:57.92 -13:31:14.6: 12.59 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:57.92 -13:31:14.6: 12.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.60 +/- 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 J106.7427-13.5210,2461324.8564,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.7427-13.5210 20261011.3564 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.53 07:08:54.20 -14:02:58.9
227.40863 -2.57719 galactic CMa Second-epoch detections are separated by 1.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2256-14.0495 | 07:08:54.17 -14:02:58.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.461+/-0.033 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:54.20 -14:02:58.9: 12.56 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:54.20 -14:02:58.9: 12.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 J107.2256-14.0495,2461324.8564,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2256-14.0495 20261011.3564 11.53CV 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 10 11.3564 2461324.8564 11.54 07:08:50.37 -14:06:20.4
227.45129 -2.61664 galactic CMa Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2098-14.1057 | 07:08:50.37 -14:06:20.4 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.247+/-0.033 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:50.37 -14:06:20.4: 12.56 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:50.37 -14:06:20.4: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.57 +/- 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 J107.2098-14.1057,2461324.8564,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2098-14.1057 20261011.3564 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.56 07:04:35.38 -14:05:07.6
226.96131 -3.52377 galactic CMa Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.1473-14.0854 | 07:04:35.35 -14:05:07.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.214+/-0.033 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:35.38 -14:05:07.6: 12.50 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:35.38 -14:05:07.6: 12.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1473-14.0854,2461324.8564,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1473-14.0854 20261011.3564 11.56CV 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 10 11.3564 2461324.8564 11.57 07:04:50.50 -14:04:19.2
226.97722 -3.46325 galactic CMa Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.2104-14.0687 | 07:04:50.50 -14:04:19.2 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.793+/-0.035 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:50.50 -14:04:19.2: 12.53 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:50.50 -14:04:19.2: 12.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.53 +/- 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 J106.2104-14.0687,2461324.8564,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.2104-14.0687 20261011.3564 11.57CV 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 10 11.3564 2461324.8564 11.59 07:06:45.17 -13:48:33.7
226.95531 -2.93077 galactic CMa Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.6880-13.8093 | 07:06:45.14 -13:48:33.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.375+/-0.033 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:45.17 -13:48:33.7: 12.50 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:45.17 -13:48:33.7: 12.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 J106.6880-13.8093,2461324.8564,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6880-13.8093 20261011.3564 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.38 07:09:49.44 -13:54:04.2
227.37938 -2.31055 galactic CMa Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.4558-13.9011 | 07:09:49.40 -13:54:04.3 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.210+/-0.036 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:49.44 -13:54:04.2: 12.43 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:49.44 -13:54:04.2: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4558-13.9011,2461324.8564,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4558-13.9011 20261011.3564 11.38CV 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 10 11.3564 2461324.8564 11.54 07:05:13.56 -13:43:57.1
226.71720 -3.22542 galactic CMa Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3044717571863652352 | 07:05:13.55 -13:43:57.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.335+/-0.032 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:13.56 -13:43:57.1: 12.42 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:13.56 -13:43:57.1: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 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 3044717571863652352,2461324.8564,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044717571863652352 20261011.3564 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.32 07:09:47.45 -14:00:56.7
227.47749 -2.37042 galactic CMa Second-epoch detections are separated by 0.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.4478-14.0158 | 07:09:47.49 -14:00:57.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.905+/-0.037 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:47.45 -14:00:56.7: 12.45 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:47.45 -14:00:56.7: 12.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.41 +/- 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 J107.4478-14.0158,2461324.8564,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4478-14.0158 20261011.3564 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.38 07:05:55.37 -13:46:41.3
226.83523 -3.09571 galactic CMa Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.4808-13.7780 | 07:05:55.40 -13:46:40.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.753+/-0.034 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:55.37 -13:46:41.3: 12.43 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:55.37 -13:46:41.3: 12.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.41 +/- 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 J106.4808-13.7780,2461324.8564,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4808-13.7780 20261011.3564 11.38CV 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 10 11.3564 2461324.8564 11.49 07:06:13.84 -13:16:37.8
226.42335 -2.80011 galactic CMa Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.5577-13.2770 | 07:06:13.85 -13:16:37.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.333+/-0.032 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:13.84 -13:16:37.8: 12.39 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:13.84 -13:16:37.8: 12.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.35 +/- 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
ATO J106.5577-13.2770,2461324.8564,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5577-13.2770 20261011.3564 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.41 07:08:51.43 -14:04:29.1
227.42576 -2.59864 galactic CMa Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2141-14.0744 | 07:08:51.40 -14:04:27.8 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.962+/-0.035 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:51.43 -14:04:29.1: 12.38 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:51.43 -14:04:29.1: 12.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2141-14.0744,2461324.8564,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2141-14.0744 20261011.3564 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.38 07:06:36.98 -13:26:37.9
226.61473 -2.79298 galactic CMa Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX 1" ASASSN-V J070637.06-132638.3
Type: SRS
# Max. Min./Amp. JD0 Period
13.670 g Y 0.150 g 2458736.63600 28.387000000000
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:36.98 -13:26:37.9: 12.38 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:36.98 -13:26:37.9: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070637.06-132638.3,2461324.8564,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J070637.06-132638.3 20261011.3564 11.38CV 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 10 11.3564 2461324.8564 11.49 07:05:53.49 -13:35:56.4
226.67218 -3.02062 galactic CMa Second-epoch detections are separated by 0.1" and 7.3 pix
The object was found in VSX 0" GDS_J0705534-133556
Type: VAR
# Max. Min./Amp. JD0 Period
12.340 r Y 0.280 r
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:53.49 -13:35:56.4: 12.36 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:53.49 -13:35:56.4: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0705534-133556,2461324.8564,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0705534-133556 20261011.3564 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.43 07:04:53.68 -13:59:44.8
226.91512 -3.41706 galactic CMa Second-epoch detections are separated by 0.8" and 7.1 pix
The object was found in VSX 0" Gaia DR3 2948445330167400704
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.280 G 12.340 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:53.68 -13:59:44.8: 12.36 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:53.68 -13:59:44.8: 12.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2948445330167400704,2461324.8564,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2948445330167400704 20261011.3564 11.43CV 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 10 11.3564 2461324.8564 11.39 07:04:45.64 -14:02:58.8
226.94833 -3.47056 galactic CMa Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.1901-14.0497 | 07:04:45.64 -14:02:59.1 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.785+/-0.033 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:45.64 -14:02:58.8: 12.34 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:45.64 -14:02:58.8: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 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
ATO J106.1901-14.0497,2461324.8564,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1901-14.0497 20261011.3564 11.39CV 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 10 11.3564 2461324.8564 11.35 07:05:22.65 -13:58:34.7
226.95128 -3.30394 galactic CMa Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.3444-13.9763 | 07:05:22.66 -13:58:34.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.020+/-0.035 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:22.65 -13:58:34.7: 12.33 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:22.65 -13:58:34.7: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 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
ATO J106.3444-13.9763,2461324.8564,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3444-13.9763 20261011.3564 11.35CV 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 10 11.3564 2461324.8564 11.37 07:08:21.67 -14:08:18.5
227.42718 -2.73473 galactic CMa Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.0902-14.1384 | 07:08:21.65 -14:08:18.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.342+/-0.033 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:21.67 -14:08:18.5: 12.26 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:21.67 -14:08:18.5: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 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 J107.0902-14.1384,2461324.8564,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0902-14.1384 20261011.3564 11.37CV 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 10 11.3564 2461324.8564 11.28 07:09:40.01 -14:00:48.2
227.46154 -2.39604 galactic CMa Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.4165-14.0134 | 07:09:39.98 -14:00:48.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.318+/-0.040 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:40.01 -14:00:48.2: 12.23 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:40.01 -14:00:48.2: 12.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.25 +/- 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 J107.4165-14.0134,2461324.8564,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4165-14.0134 20261011.3564 11.28CV 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 10 11.3564 2461324.8564 11.29 07:09:01.71 -14:05:04.7
227.45366 -2.56627 galactic CMa Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2572-14.0847 | 07:09:01.73 -14:05:05.1 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.369+/-0.033 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:01.71 -14:05:04.7: 12.18 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:01.71 -14:05:04.7: 12.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2572-14.0847,2461324.8564,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2572-14.0847 20261011.3564 11.29CV 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 10 11.3564 2461324.8564 11.18 07:09:44.01 -13:46:09.9
227.25219 -2.26944 galactic CMa Second-epoch detections are separated by 0.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.4335-13.7690 | 07:09:44.04 -13:46:08.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.707+/-0.040 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:44.01 -13:46:09.9: 12.17 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:44.01 -13:46:09.9: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 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 J107.4335-13.7690,2461324.8564,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4335-13.7690 20261011.3564 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.22 07:08:48.57 -14:04:34.5
227.42179 -2.60959 galactic CMa Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2141-14.0744 | 07:08:51.40 -14:04:27.8 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.265+/-0.033 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:48.57 -14:04:34.5: 12.15 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:48.57 -14:04:34.5: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 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 J107.2141-14.0744,2461324.8564,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2141-14.0744 20261011.3564 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.16 07:09:16.09 -14:05:31.0
227.48688 -2.51801 galactic CMa Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3170-14.0919 | 07:09:16.10 -14:05:30.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.585+/-0.032 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:16.09 -14:05:31.0: 12.13 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:16.09 -14:05:31.0: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 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
ATO J107.3170-14.0919,2461324.8564,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3170-14.0919 20261011.3564 11.16CV 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 10 11.3564 2461324.8564 11.29 07:06:49.56 -13:22:51.3
226.58207 -2.71884 galactic CMa Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.7064-13.3809 | 07:06:49.54 -13:22:51.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.182+/-0.035 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:49.56 -13:22:51.3: 12.12 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:49.56 -13:22:51.3: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.7064-13.3809,2461324.8564,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.7064-13.3809 20261011.3564 11.29CV 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 10 11.3564 2461324.8564 11.18 07:06:47.41 -13:38:15.2
226.80651 -2.84408 galactic CMa Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.6976-13.6376 | 07:06:47.44 -13:38:15.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.889+/-0.031 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:47.41 -13:38:15.2: 12.09 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:47.41 -13:38:15.2: 12.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.6976-13.6376,2461324.8564,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6976-13.6376 20261011.3564 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.22 07:05:42.65 -13:36:28.3
226.65998 -3.06371 galactic CMa Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.4278-13.6077 | 07:05:42.68 -13:36:27.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.622+/-0.033 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:42.65 -13:36:28.3: 12.10 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:42.65 -13:36:28.3: 12.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4278-13.6077,2461324.8564,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4278-13.6077 20261011.3564 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.05 07:09:44.76 -13:54:06.4
227.37120 -2.32764 galactic CMa Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.4364-13.9018 | 07:09:44.74 -13:54:06.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.295+/-0.036 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:44.76 -13:54:06.4: 12.08 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:44.76 -13:54:06.4: 12.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4364-13.9018,2461324.8564,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4364-13.9018 20261011.3564 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.16 07:04:21.81 -14:06:20.0
226.95422 -3.58175 galactic CMa Second-epoch detections are separated by 1.3" and 7.5 pix
The object was found in VSX18" Gaia DR3 2948437152548347776
Type: L
# Max. Min./Amp. JD0 Period
12.680 G 12.830 G M
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:21.81 -14:06:20.0: 12.09 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:21.81 -14:06:20.0: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.04 +/- 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 2948437152548347776,2461324.8564,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2948437152548347776 20261011.3564 11.16CV 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 10 11.3564 2461324.8564 11.08 07:09:15.06 -14:00:32.8
227.41133 -2.48364 galactic CMa Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3127-14.0091 | 07:09:15.07 -14:00:33.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.255+/-0.035 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:15.06 -14:00:32.8: 12.02 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:15.06 -14:00:32.8: 12.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3127-14.0091,2461324.8564,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3127-14.0091 20261011.3564 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 11.10 07:07:05.03 -13:31:34.4
226.74013 -2.72966 galactic CMa Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.7709-13.5262 | 07:07:05.02 -13:31:34.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.143+/-0.032 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:05.03 -13:31:34.4: 11.99 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:05.03 -13:31:34.4: 11.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.7709-13.5262,2461324.8564,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.7709-13.5262 20261011.3564 11.10CV 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 10 11.3564 2461324.8564 11.02 07:09:30.48 -13:53:31.0
227.33587 -2.37440 galactic CMa Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3771-13.8919 | 07:09:30.51 -13:53:30.9 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.747+/-0.033 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:30.48 -13:53:31.0: 11.98 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:30.48 -13:53:31.0: 11.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3771-13.8919,2461324.8564,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3771-13.8919 20261011.3564 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 10.99 07:04:47.67 -14:09:04.2
227.04259 -3.50951 galactic CMa Second-epoch detections are separated by 0.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.1987-14.1512 | 07:04:47.70 -14:09:04.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.864+/-0.033 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:47.67 -14:09:04.2: 11.95 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:47.67 -14:09:04.2: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1987-14.1512,2461324.8564,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1987-14.1512 20261011.3564 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 10.96 07:09:28.31 -13:55:00.5
227.35393 -2.39363 galactic CMa Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3679-13.9168 | 07:09:28.30 -13:55:00.6 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.414+/-0.033 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:28.31 -13:55:00.5: 11.90 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:28.31 -13:55:00.5: 11.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3679-13.9168,2461324.8564,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3679-13.9168 20261011.3564 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 10.86 07:09:27.63 -13:58:53.0
227.41007 -2.42577 galactic CMa Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3652-13.9813 | 07:09:27.65 -13:58:52.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.712+/-0.035 (K)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:27.63 -13:58:53.0: 11.78 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:27.63 -13:58:53.0: 11.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3652-13.9813,2461324.8564,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3652-13.9813 20261011.3564 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 12.26 07:09:36.49 -13:42:46.5
227.18797 -2.27046 galactic CMa Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.4003-13.7146 | 07:09:36.49 -13:42:46.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.426+/-0.042 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:36.49 -13:42:46.5: 13.47 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:36.49 -13:42:46.5: 13.38 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4003-13.7146,2461324.8564,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4003-13.7146 20261011.3564 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 10 11.3564 2461324.8564 10.70 07:05:32.36 -14:01:13.0
227.00841 -3.28908 galactic CMa Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.3851-14.0203 | 07:05:32.44 -14:01:13.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M1.5II-III 2010MacCon.unpub..M UCAC2 26624105 J-Ks=1.369+/-0.036 (Very red! L if it's a dwarf)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:32.36 -14:01:13.0: 11.69 +/- 0.01 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:32.36 -14:01:13.0: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3851-14.0203,2461324.8564,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3851-14.0203 20261011.3564 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 10.62 07:06:41.75 -13:43:33.3
226.87467 -2.90489 galactic CMa Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3044532892560428416 | 07:06:41.75 -13:43:33.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.001+/-0.034 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:41.75 -13:43:33.3: 11.47 +/- 0.01 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:41.75 -13:43:33.3: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3044532892560428416,2461324.8564,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044532892560428416 20261011.3564 10.62CV 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 10 11.3564 2461324.8564 12.32 07:09:10.60 -14:02:21.1
227.42978 -2.51348 galactic CMa Second-epoch detections are separated by 0.7" and 7.3 pix
The object was found in VSX18" Gaia DR3 3044471109457627904
Type: ROT
# Max. Min./Amp. JD0 Period
16.950 G 17.040 G A
ATTENTION: measured mag 12.32 is 4.6 mag brighter than the VSX record maximum brightness 16.95 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:10.60 -14:02:21.1: 13.42 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:10.60 -14:02:21.1: 13.35 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3044471109457627904,2461324.8564,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3044471109457627904 20261011.3564 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 12.35 07:09:10.94 -14:02:48.1
227.43708 -2.51571 galactic CMa Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2954-14.0464 | 07:09:10.94 -14:02:48.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.256+/-0.034 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:10.94 -14:02:48.1: 13.40 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:10.94 -14:02:48.1: 13.42 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2954-14.0464,2461324.8564,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2954-14.0464 20261011.3564 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 10 11.3564 2461324.8564 12.25 07:09:20.42 -14:07:21.3
227.52217 -2.51655 galactic CMa Second-epoch detections are separated by 3.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.3367-14.1249 | 07:09:20.42 -14:07:21.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:20.42 -14:07:21.3: 13.38 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:20.42 -14:07:21.3: 13.38 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3367-14.1249,2461324.8564,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3367-14.1249 20261011.3564 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 10 11.3564 2461324.8564 12.17 07:08:51.54 -13:58:18.2
227.33436 -2.55093 galactic CMa Second-epoch detections are separated by 2.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2151-13.9717 | 07:08:51.54 -13:58:18.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.114+/-0.032 (M)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:51.54 -13:58:18.2: 13.36 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:51.54 -13:58:18.2: 13.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2151-13.9717,2461324.8564,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2151-13.9717 20261011.3564 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3564 2461324.8564 12.19 07:07:52.39 -13:41:14.9
226.97161 -2.63310 galactic CMa Second-epoch detections are separated by 3.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.9680-13.6874 | 07:07:52.39 -13:41:14.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.344+/-0.035 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:52.39 -13:41:14.9: 13.28 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:52.39 -13:41:14.9: 13.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.9680-13.6874,2461324.8564,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.9680-13.6874 20261011.3564 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 10 11.3564 2461324.8564 12.14 07:05:50.55 -14:07:17.9
227.13236 -3.26994 galactic CMa Second-epoch detections are separated by 1.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.4604-14.1215 | 07:05:50.55 -14:07:17.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.331+/-0.037 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:50.55 -14:07:17.9: 13.24 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:50.55 -14:07:17.9: 13.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4604-14.1215,2461324.8564,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4604-14.1215 20261011.3564 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 10 11.3564 2461324.8564 12.16 07:06:54.55 -13:24:15.9
226.61226 -2.71162 galactic CMa Second-epoch detections are separated by 1.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.7274-13.4044 | 07:06:54.55 -13:24:15.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.422+/-0.035 (G)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:54.55 -13:24:15.9: 13.21 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:54.55 -13:24:15.9: 13.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.7274-13.4044,2461324.8564,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.7274-13.4044 20261011.3564 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 10 11.3564 2461324.8564 12.24 07:09:11.21 -13:30:45.0
226.96275 -2.26919 galactic CMa Second-epoch detections are separated by 1.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2969-13.5125 | 07:09:11.21 -13:30:45.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.246+/-0.037 (F)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:11.21 -13:30:45.0: 13.22 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:11.21 -13:30:45.0: 13.18 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2969-13.5125,2461324.8564,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2969-13.5125 20261011.3564 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 10 11.3564 2461324.8564 12.18 07:04:37.38 -14:00:11.7
226.89169 -3.47913 galactic CMa Second-epoch detections are separated by 1.1" and 7.5 pix
The object was found in VSX 8" Gaia DR3 2948448255044794624
Type: ROT
# Max. Min./Amp. JD0 Period
14.970 G 15.000 G G
The object was not found in astcheck.
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:37.38 -14:00:11.7: 13.19 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:37.38 -14:00:11.7: 13.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.23 +/- 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 2948448255044794624,2461324.8564,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2948448255044794624 20261011.3564 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461139.59921253 09.04.2026 02:22:41.963 /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
First image: 2461139.59921253 09.04.2026 02:22:41.963 /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
Last image: 2461324.85671753 11.10.2026 08:33:30.395 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 18980
Objects passed selection criteria: 18828
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 10867
Average stars matched: 10366 (95.3897 %)
Memory usage VmPeak: 244936 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 11 03:39:05 CDT 2026
Host name: tau
############################################################
ERROR: large change in astrometric-star counts between the two new images (q1: 128 -> 386, 66.839% > 20%; fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits vs fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
ERROR: large change in astrometric-star counts between the two new images (q2: 442 -> 278, 37.104% > 20%; fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits vs fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461139.59921253 09.04.2026 02:22:41.963 /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
First image: 2461139.59921253 09.04.2026 02:22:41.963 /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
Last image: 2461324.85671753 11.10.2026 08:33:30.395 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 295
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.48
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: 22 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): 135294
Objects passed selection criteria: 134794
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 81904
Average stars matched: 77620.5 (94.7701 %)
Memory usage VmPeak: 558400 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 11 03:40:08 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
SExtractor catalog cache: saved Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.cat to cache
SExtractor catalog cache: saved Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.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/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461324.85603358
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_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits exists and is non-empty
wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits exists and is non-empty
wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits exists and is non-empty
wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits (1st reference image)
verification OK: wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:31.944 -09:59:40.78 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_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits (1st new image)
verification OK: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
Image size: 938.7'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 06:51:11.474 -09:59:05.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:31.944 -09:59:40.78
Second-epoch image center 06:51:11.474 -09:59:05.22
Angular distance between the image centers 0.0846 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits (2nd new image)
verification OK: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Image size: 938.7'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 06:51:13.641 -09:58:33.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:31.944 -09:59:40.78
Second-epoch image center 06:51:13.641 -09:58:33.84
Angular distance between the image centers 0.0774 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 06:51:11.474 -09:59:05.22
Second-epoch second image center 06:51:13.641 -09:58:33.84
Angular distance between the image centers 0.01245 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/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits &> /tmp/tmp.PScVxxhD8r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits &> /tmp/tmp.e9r0gK2Jfo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits &> /tmp/tmp.yoCeBdGXFi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits &> /tmp/tmp.LAGUbHOmhx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.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_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits and wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.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_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits and wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat
Found non-empty wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits and wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat
The reference image (wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits) and catalog (wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat) found
'wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat' -> 'wcsmag.cat'
Read 23708 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.8919 to 111.0361 deg, Dec -15.2871 to -4.5750 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 94.8919 to 111.0361 deg, Dec -15.2871 to -4.5750 deg
Loaded 21843 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): 14945 out of 16014 total matches.
Matched with Tycho-2 16014 out of 23708 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.662200
a=0.000000 b=1.000000 c=22.662200
From vast_summary.log: estimated ref. image limiting mag.: -7.75
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.91
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.91
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23708 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.8919 to 111.0361 deg, Dec -15.2871 to -4.5750 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 94.8919 to 111.0361 deg, Dec -15.2871 to -4.5750 deg
Loaded 21843 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): 14945 out of 16014 total matches.
Matched with Tycho-2 16014 out of 23708 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
Forced-photometry filter: calibrated wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits -> calib.txt_param_ref_wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits (aperture=6.4)
Read 23764 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.8842 to 111.0361 deg, Dec -15.2871 to -4.5672 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 94.8842 to 111.0361 deg, Dec -15.2871 to -4.5672 deg
Loaded 21874 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): 14942 out of 16019 total matches.
Matched with Tycho-2 16019 out of 23764 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
Forced-photometry filter: calibrated wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits -> calib.txt_param_ref_wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits (aperture=6.4)
____ 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:
2.5 pix Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
2.5 pix Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
2.4 pix fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
2.5 pix fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Limiting magnitude estimates:
14.9 mag. Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
14.9 mag. Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
11.8 mag. fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
11.4 mag. fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
All-image limiting magnitude estimate: 11.4 (SNR ) 9.6 (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.PScVxxhD8r (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits' -> 'wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.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/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
WCS-calibrated image found: wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
Checking if the catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat corresponding to the image wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat corresponding to the image wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
WCS catalog name: wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2215, bad_region=3520, passed=23708
Got 23708 stars (including 18215 good ones) from the SExtractor catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat
util/solve_plate_with_UCAC5 got 23708 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 4920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 20988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 20988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 20988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4920 stars left (next iteration limit 5412)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits N_match=4920 sigma_overall_arcsec=0.508 sigma_q1_arcsec=0.492 sigma_q2_arcsec=0.520 sigma_q3_arcsec=0.499 sigma_q4_arcsec=0.518 n_q1=1864 n_q2=824 n_q3=1516 n_q4=716 worst_quadrant_to_overall_ratio=1.024
The image catalog is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits -region wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.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.e9r0gK2Jfo (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits' -> 'wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.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/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
WCS_IMAGE_NAME=wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
WCS-calibrated image found: wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
Checking if the catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat corresponding to the image wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits alredy exist and is non-empty...
Catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat corresponding to the image wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
WCS catalog name: wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2234, bad_region=3533, passed=23764
Got 23764 stars (including 18241 good ones) from the SExtractor catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat
util/solve_plate_with_UCAC5 got 23764 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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 4918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 21034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 21034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 21034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 4916 stars left (next iteration limit 5408)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits N_match=4916 sigma_overall_arcsec=0.518 sigma_q1_arcsec=0.510 sigma_q2_arcsec=0.547 sigma_q3_arcsec=0.505 sigma_q4_arcsec=0.518 n_q1=1869 n_q2=820 n_q3=1506 n_q4=721 worst_quadrant_to_overall_ratio=1.056
The image catalog is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits -region wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.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.yoCeBdGXFi (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_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.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_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
WCS_IMAGE_NAME=wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
WCS-calibrated image found: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
Checking if the catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat corresponding to the image wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat corresponding to the image wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
WCS catalog name: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=178, bad_region=1633, passed=3314
Got 3314 stars (including 1603 good ones) from the SExtractor catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat
util/solve_plate_with_UCAC5 got 3314 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 1568 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1550 matched stars entering correct_measured_positions(), 1537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1550 matched stars entering correct_measured_positions(), 1907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 1569 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1551 matched stars entering correct_measured_positions(), 1906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 1551 matched stars entering correct_measured_positions(), 1906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 1551 stars left (next iteration limit 1705)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1551 robust_rms=9.016 arcsec worst_region_rms=14.251 arcsec outer_annulus_rms=13.883 arcsec
SIP_REFIT: SIP order 3 trial: matched=1551 robust_rms=0.686 arcsec worst_region_rms=1.055 arcsec outer_annulus_rms=1.055 arcsec
SIP_REFIT: SIP order 5 trial: matched=1551 robust_rms=0.503 arcsec worst_region_rms=0.782 arcsec outer_annulus_rms=0.782 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1551 robust_rms_before=1.222 arcsec robust_rms_before_corrected=0.571 arcsec robust_rms_after=0.503 arcsec worst_region_rms_before=0.925 worst_region_rms_after=0.782 outer_annulus_rms_before=2.323 outer_annulus_rms_after=0.782
verification OK: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
verification OK: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
Image size: 938.7'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 06:51:11.419 -09:59:05.35 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3314 stars ###
'wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/correct_sextractor_wcs_catalog_usingxy2sky2531353.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.222 -> 0.503 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (cycle 1, search radius 3.0 arcsec, 1551 pairs from the previous matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 1484 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 1484 pairs (1551 from the previous matching)
SIP_REFIT: SIP order 2 trial: matched=1484 robust_rms=8.770 arcsec worst_region_rms=13.661 arcsec outer_annulus_rms=13.446 arcsec
SIP_REFIT: SIP order 3 trial: matched=1484 robust_rms=0.675 arcsec worst_region_rms=1.015 arcsec outer_annulus_rms=1.015 arcsec
SIP_REFIT: SIP order 5 trial: matched=1484 robust_rms=0.492 arcsec worst_region_rms=0.741 arcsec outer_annulus_rms=0.741 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1484 robust_rms_before=0.494 arcsec robust_rms_before_corrected=0.494 arcsec robust_rms_after=0.492 arcsec worst_region_rms_before=0.741 worst_region_rms_after=0.741 outer_annulus_rms_before=0.741 outer_annulus_rms_after=0.741
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-region 0.741 vs 0.741 arcsec) - keeping the current solution
SIP_REFIT: the refit on the re-matched pairs was not applied - keeping the current solution
Accuracy estimation diagnostic: 1484 matched stars entering correct_measured_positions(), 1905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 1484 matched stars entering correct_measured_positions(), 1899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
WCS_QUALITY_DIAG: file=fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits N_match=1484 sigma_overall_arcsec=0.501 sigma_q1_arcsec=0.686 sigma_q2_arcsec=0.432 sigma_q3_arcsec=0.648 sigma_q4_arcsec=0.474 n_q1=128 n_q2=442 n_q3=406 n_q4=508 worst_quadrant_to_overall_ratio=1.370
The image catalog is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits -region wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.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.LAGUbHOmhx (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_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.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_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
WCS_IMAGE_NAME=wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
WCS-calibrated image found: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Checking if the catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
WCS catalog name: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=156, bad_region=1508, passed=3146
Got 3146 stars (including 1568 good ones) from the SExtractor catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat
util/solve_plate_with_UCAC5 got 3146 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 1537 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1517 matched stars entering correct_measured_positions(), 1502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1517 matched stars entering correct_measured_positions(), 1913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 1537 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1517 matched stars entering correct_measured_positions(), 1912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 1517 matched stars entering correct_measured_positions(), 1912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 1517 stars left (next iteration limit 1668)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1517 robust_rms=9.404 arcsec worst_region_rms=11.154 arcsec outer_annulus_rms=8.189 arcsec
SIP_REFIT: SIP order 3 trial: matched=1517 robust_rms=0.765 arcsec worst_region_rms=0.990 arcsec outer_annulus_rms=0.778 arcsec
SIP_REFIT: SIP order 5 trial: matched=1517 robust_rms=0.584 arcsec worst_region_rms=0.700 arcsec outer_annulus_rms=0.696 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1517 robust_rms_before=1.290 arcsec robust_rms_before_corrected=0.597 arcsec robust_rms_after=0.584 arcsec worst_region_rms_before=0.759 worst_region_rms_after=0.700 outer_annulus_rms_before=2.030 outer_annulus_rms_after=0.696
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.759 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits worst_region_rms_kept=0.759 arcsec robust_rms_kept=0.597 arcsec matched=1517
WCS_QUALITY_DIAG: file=fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits N_match=1517 sigma_overall_arcsec=0.569 sigma_q1_arcsec=0.655 sigma_q2_arcsec=0.505 sigma_q3_arcsec=0.744 sigma_q4_arcsec=0.509 n_q1=386 n_q2=278 n_q3=413 n_q4=440 worst_quadrant_to_overall_ratio=1.307
The image catalog is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits -region wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.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_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits to local_wcs_cache/
'wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits' -> 'local_wcs_cache/wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits'
Saving the final (post-refit) wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits to local_wcs_cache/
'wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits' -> 'local_wcs_cache/wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits'
Saving the final (post-refit) wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits to local_wcs_cache/
'wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits' -> 'local_wcs_cache/wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits'
Saving the final (post-refit) wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits to local_wcs_cache/
'wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits' -> 'local_wcs_cache/wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits sigma_overall=0.508 worst_q_ratio=1.024
ref2=Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits sigma_overall=0.518 worst_q_ratio=1.056
new1=fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits sigma_overall=0.501 worst_q_ratio=1.370
new2=fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits sigma_overall=0.569 worst_q_ratio=1.307
reference average sigma_overall=0.513 worst_q_ratio=1.04
warn-on-ratio threshold: 2.0x reference
###################################
ERROR: large change in astrometric-star counts between the two new images (q1: 128 -> 386, 66.839% > 20%; fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits vs fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
ERROR: large change in astrometric-star counts between the two new images (q2: 442 -> 278, 37.104% > 20%; fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits vs fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023_astrometric_residuals.png (4920 matched stars from wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024_astrometric_residuals.png (4916 matched stars from wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291_astrometric_residuals.png (1484 matched stars from wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292_astrometric_residuals.png (1517 matched stars from wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits'
Saving fully-calibrated image wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits'
Preparing the HTML report for the field Mon-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Mon-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
SExtractor catalog cache: saved Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.cat to cache
SExtractor catalog cache: saved Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
Creating symlink local_wcs_cache/wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Checking 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_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits exists and is non-empty
wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits exists and is non-empty
wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits exists and is non-empty
wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits (1st reference image)
verification OK: wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:31.944 -09:59:40.78 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_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits (1st new image)
verification OK: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
Image size: 938.7'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 06:51:11.419 -09:59:05.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:31.944 -09:59:40.78
Second-epoch image center 06:51:11.419 -09:59:05.35
Angular distance between the image centers 0.0848 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits (2nd new image)
verification OK: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Image size: 938.7'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 06:51:13.641 -09:58:33.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:31.944 -09:59:40.78
Second-epoch image center 06:51:13.641 -09:58:33.84
Angular distance between the image centers 0.0774 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 06:51:11.419 -09:59:05.35
Second-epoch second image center 06:51:13.641 -09:58:33.84
Angular distance between the image centers 0.01264 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/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits &> /tmp/tmp.o0gwQZO1ui
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits &> /tmp/tmp.XiWKfJuIW2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits &> /tmp/tmp.IRiW8t18GR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits &> /tmp/tmp.930XPmSHdF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.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_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits and wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.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_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits and wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat
Found non-empty wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits and wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat
The reference image (wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits) and catalog (wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat) found
'wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat' -> 'wcsmag.cat'
Read 163412 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.8860 to 111.0563 deg, Dec -15.2906 to -4.5674 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 94.8860 to 111.0563 deg, Dec -15.2906 to -4.5674 deg
Loaded 21923 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): 14198 out of 18773 total matches.
Matched with Tycho-2 18773 out of 163412 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.494450
a=0.000000 b=1.000000 c=22.494450
From vast_summary.log: estimated ref. image limiting mag.: -7.48
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 163412 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.8860 to 111.0563 deg, Dec -15.2906 to -4.5674 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 94.8860 to 111.0563 deg, Dec -15.2906 to -4.5674 deg
Loaded 21923 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): 14198 out of 18773 total matches.
Matched with Tycho-2 18773 out of 163412 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
Forced-photometry filter: calibrated wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits -> calib.txt_param_ref_wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits (aperture=4.9)
Read 164110 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.8842 to 111.0510 deg, Dec -15.2898 to -4.5672 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 94.8842 to 111.0510 deg, Dec -15.2898 to -4.5672 deg
Loaded 21912 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): 14201 out of 18778 total matches.
Matched with Tycho-2 18778 out of 164110 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
Forced-photometry filter: calibrated wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits -> calib.txt_param_ref_wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 130 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
2.3 pix Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
2.2 pix fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
2.3 pix fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Limiting magnitude estimates:
15.0 mag. Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
15.0 mag. Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
12.6 mag. fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
12.5 mag. fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 12.0 (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.o0gwQZO1ui (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits' -> 'wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.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/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
WCS-calibrated image found: wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
Checking if the catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat corresponding to the image wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat corresponding to the image wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits
WCS catalog name: wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=21454, bad_region=16234, passed=163374
Got 163374 stars (including 127676 good ones) from the SExtractor catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat
util/solve_plate_with_UCAC5 got 163374 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4929 matched stars entering correct_measured_positions(), 4929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4929 matched stars entering correct_measured_positions(), 151624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4929 matched stars entering correct_measured_positions(), 151624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4929 matched stars entering correct_measured_positions(), 151623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4929 stars left (next iteration limit 5421)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.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_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits N_match=4929 sigma_overall_arcsec=0.498 sigma_q1_arcsec=0.496 sigma_q2_arcsec=0.523 sigma_q3_arcsec=0.476 sigma_q4_arcsec=0.510 n_q1=1782 n_q2=860 n_q3=1471 n_q4=816 worst_quadrant_to_overall_ratio=1.049
The image catalog is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits -region wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.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.XiWKfJuIW2 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits' -> 'wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.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/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
WCS_IMAGE_NAME=wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
WCS-calibrated image found: wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
Checking if the catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat corresponding to the image wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits alredy exist and is non-empty...
Catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat corresponding to the image wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits
WCS catalog name: wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=49, blended=21473, bad_region=16292, passed=164061
Got 164061 stars (including 128281 good ones) from the SExtractor catalog wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat
util/solve_plate_with_UCAC5 got 164061 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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 4923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 152209 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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 152209 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 152209 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4922 stars left (next iteration limit 5415)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.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_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits N_match=4922 sigma_overall_arcsec=0.519 sigma_q1_arcsec=0.505 sigma_q2_arcsec=0.534 sigma_q3_arcsec=0.511 sigma_q4_arcsec=0.535 n_q1=1775 n_q2=868 n_q3=1488 n_q4=791 worst_quadrant_to_overall_ratio=1.031
The image catalog is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits -region wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.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.IRiW8t18GR (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_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.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_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
WCS_IMAGE_NAME=wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
WCS-calibrated image found: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
Checking if the catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat corresponding to the image wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat corresponding to the image wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
WCS catalog name: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1561, bad_region=15995, passed=34533
Got 34533 stars (including 17825 good ones) from the SExtractor catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat
util/solve_plate_with_UCAC5 got 34533 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 4872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 21707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 21707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 21707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4875 stars left (next iteration limit 5363)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.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=4875 robust_rms=8.514 arcsec worst_region_rms=17.507 arcsec outer_annulus_rms=17.507 arcsec
SIP_REFIT: SIP order 3 trial: matched=4875 robust_rms=0.728 arcsec worst_region_rms=1.450 arcsec outer_annulus_rms=1.450 arcsec
SIP_REFIT: SIP order 5 trial: matched=4875 robust_rms=0.574 arcsec worst_region_rms=1.016 arcsec outer_annulus_rms=1.016 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4875 robust_rms_before=0.578 arcsec robust_rms_before_corrected=0.583 arcsec robust_rms_after=0.574 arcsec worst_region_rms_before=1.035 worst_region_rms_after=1.016 outer_annulus_rms_before=1.035 outer_annulus_rms_after=1.016
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 1.035 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits worst_region_rms_kept=1.035 arcsec robust_rms_kept=0.578 arcsec matched=4875
WCS_QUALITY_DIAG: file=fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits N_match=4875 sigma_overall_arcsec=0.586 sigma_q1_arcsec=0.829 sigma_q2_arcsec=0.462 sigma_q3_arcsec=0.802 sigma_q4_arcsec=0.549 n_q1=469 n_q2=1542 n_q3=1190 n_q4=1674 worst_quadrant_to_overall_ratio=1.415
The image catalog is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits -region wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.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.930XPmSHdF (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_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.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_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
WCS_IMAGE_NAME=wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
WCS-calibrated image found: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Checking if the catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
WCS catalog name: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1329, bad_region=14620, passed=31291
Got 31291 stars (including 16089 good ones) from the SExtractor catalog wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat
util/solve_plate_with_UCAC5 got 31291 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 20028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 4911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 20027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 20027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 4862 stars left (next iteration limit 5348)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.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=4862 robust_rms=9.133 arcsec worst_region_rms=11.809 arcsec outer_annulus_rms=8.990 arcsec
SIP_REFIT: SIP order 3 trial: matched=4862 robust_rms=0.832 arcsec worst_region_rms=1.139 arcsec outer_annulus_rms=0.984 arcsec
SIP_REFIT: SIP order 5 trial: matched=4862 robust_rms=0.655 arcsec worst_region_rms=0.881 arcsec outer_annulus_rms=0.804 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4862 robust_rms_before=1.320 arcsec robust_rms_before_corrected=0.645 arcsec robust_rms_after=0.655 arcsec worst_region_rms_before=0.891 worst_region_rms_after=0.881 outer_annulus_rms_before=2.033 outer_annulus_rms_after=0.804
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.891 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits worst_region_rms_kept=0.891 arcsec robust_rms_kept=0.645 arcsec matched=4862
WCS_QUALITY_DIAG: file=fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits N_match=4862 sigma_overall_arcsec=0.629 sigma_q1_arcsec=0.739 sigma_q2_arcsec=0.510 sigma_q3_arcsec=0.856 sigma_q4_arcsec=0.540 n_q1=1109 n_q2=981 n_q3=1242 n_q4=1530 worst_quadrant_to_overall_ratio=1.361
The image catalog is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits -region wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.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_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.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_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-32-31_20.00sec_-0.00C_LIGHT_0291.fits
Saving fully-calibrated image wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.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_2026-10-11_CI_Mon-05-Q2b1x1_033455_TTUQ2b1x1_2346203_PThiCQIs/wcs_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292.fits
Preparing the HTML report for the field Mon-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 06:39:49.92 -05:52:12.8: 10.68 +/- 0.00 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:58.00 -14:01:10.6: 13.22 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:04.89 -14:04:33.8: 13.31 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 06:39:49.92 -05:52:12.8: 10.71 +/- 0.00 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:43.87 -13:54:15.5: 13.40 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:10.99 -13:53:31.6: 13.47 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:51.49 -13:40:57.7: 13.48 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:42.94 -13:25:52.4: 13.28 +/- 0.06 detection
Forced photometry reference-image weighted average: 10.70 +/- 0.00
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:42.40 -13:56:55.1: 11.77 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 06:39:49.92 -05:52:12.8: ref_mag=10.70 +/- 0.00 new_mean_mag=10.8115 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:58.00 -14:01:10.6: 13.32 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:04.89 -14:04:33.8: 13.28 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.04
Forced photometry filter KEPT candidate at 07:05:58.00 -14:01:10.6: ref_mag=13.26 +/- 0.04 new_mean_mag=12.0753 delta=1.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.29 +/- 0.04
Forced photometry filter KEPT candidate at 07:05:04.89 -14:04:33.8: ref_mag=13.29 +/- 0.04 new_mean_mag=12.0832 delta=1.21 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:45.75 -13:52:19.0: 11.99 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:42.94 -13:25:52.4: 13.23 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:10.99 -13:53:31.6: 13.40 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:43.87 -13:54:15.5: 13.23 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:42.40 -13:56:55.1: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.05
Forced photometry reference-image weighted average: 13.25 +/- 0.04
Forced photometry filter KEPT candidate at 07:09:10.99 -13:53:31.6: ref_mag=13.43 +/- 0.05 new_mean_mag=12.2208 delta=1.21 (need > 0.90)
Forced photometry filter KEPT candidate at 07:09:42.94 -13:25:52.4: ref_mag=13.25 +/- 0.04 new_mean_mag=12.1986 delta=1.05 (need > 0.90)
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Forced photometry reference-image weighted average: 13.30 +/- 0.04
Forced photometry filter KEPT candidate at 07:05:42.40 -13:56:55.1: ref_mag=11.76 +/- 0.01 new_mean_mag=10.8394 delta=0.92 (need > 0.90)
Forced photometry filter KEPT candidate at 07:05:43.87 -13:54:15.5: ref_mag=13.30 +/- 0.04 new_mean_mag=12.0913 delta=1.21 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:51.49 -13:40:57.7: 13.58 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.05
Forced photometry filter KEPT candidate at 07:05:51.49 -13:40:57.7: ref_mag=13.53 +/- 0.05 new_mean_mag=12.2200 delta=1.31 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:29.73 -14:01:32.5: 12.00 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:45.75 -13:52:19.0: 11.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter REJECTED candidate at 07:04:45.75 -13:52:19.0: ref_mag=11.98 +/- 0.01 new_mean_mag=11.0801 delta=0.90 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:29.73 -14:01:32.5: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter KEPT candidate at 07:05:29.73 -14:01:32.5: ref_mag=12.02 +/- 0.01 new_mean_mag=11.0390 delta=0.98 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:28.87 -14:03:21.3: 12.02 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:28.87 -14:03:21.3: 12.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry filter KEPT candidate at 07:04:28.87 -14:03:21.3: ref_mag=12.01 +/- 0.01 new_mean_mag=11.0921 delta=0.92 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:32.38 -14:01:26.9: 12.09 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:32.38 -14:01:26.9: 12.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter KEPT candidate at 07:09:32.38 -14:01:26.9: ref_mag=12.09 +/- 0.01 new_mean_mag=11.1443 delta=0.95 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:00.79 -14:03:10.6: 12.14 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:00.79 -14:03:10.6: 12.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter KEPT candidate at 07:06:00.79 -14:03:10.6: ref_mag=12.12 +/- 0.01 new_mean_mag=11.1056 delta=1.02 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:35.89 -13:42:00.8: 12.15 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:35.89 -13:42:00.8: 12.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 07:05:35.89 -13:42:00.8: ref_mag=12.18 +/- 0.01 new_mean_mag=11.2193 delta=0.96 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:39.63 -14:03:02.4: 12.26 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:39.63 -14:03:02.4: 12.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Forced photometry filter KEPT candidate at 07:09:39.63 -14:03:02.4: ref_mag=12.28 +/- 0.02 new_mean_mag=11.2950 delta=0.99 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:15.62 -14:01:49.0: 12.47 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:57.25 -14:09:08.1: 12.49 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:06.86 -13:52:57.1: 12.51 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:06.93 -14:07:11.7: 12.57 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:30.73 -13:26:20.8: 12.63 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:15.62 -14:01:49.0: 12.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Forced photometry filter KEPT candidate at 07:08:15.62 -14:01:49.0: ref_mag=12.42 +/- 0.02 new_mean_mag=11.4648 delta=0.95 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:57.25 -14:09:08.1: 12.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.02
Forced photometry filter KEPT candidate at 07:08:57.25 -14:09:08.1: ref_mag=12.52 +/- 0.02 new_mean_mag=11.4711 delta=1.05 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:06.93 -14:07:11.7: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Forced photometry filter KEPT candidate at 07:04:06.93 -14:07:11.7: ref_mag=12.57 +/- 0.02 new_mean_mag=11.6346 delta=0.93 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:06.86 -13:52:57.1: 12.50 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:30.73 -13:26:20.8: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Forced photometry filter KEPT candidate at 07:06:06.86 -13:52:57.1: ref_mag=12.50 +/- 0.02 new_mean_mag=11.5169 delta=0.99 (need > 0.90)
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Forced photometry filter KEPT candidate at 07:06:30.73 -13:26:20.8: ref_mag=12.64 +/- 0.02 new_mean_mag=11.5743 delta=1.07 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:15.75 -13:41:05.7: 12.66 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:59.71 -13:22:12.9: 12.70 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:15.75 -13:41:05.7: 12.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.03
Forced photometry filter KEPT candidate at 07:07:15.75 -13:41:05.7: ref_mag=12.69 +/- 0.03 new_mean_mag=11.6593 delta=1.03 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:59.71 -13:22:12.9: 12.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry filter KEPT candidate at 07:07:59.71 -13:22:12.9: ref_mag=12.68 +/- 0.02 new_mean_mag=11.7327 delta=0.95 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:05.02 -14:03:20.5: 12.78 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:05.02 -14:03:20.5: 12.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:05.02 -14:03:20.5: ref_mag=12.75 +/- 0.03 new_mean_mag=11.8117 delta=0.94 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:45.43 -13:38:19.2: 12.80 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:45.43 -13:38:19.2: 12.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:45.43 -13:38:19.2: ref_mag=12.77 +/- 0.03 new_mean_mag=11.8361 delta=0.94 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:04.23 -13:49:41.3: 12.83 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:04.23 -13:49:41.3: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:04.23 -13:49:41.3: ref_mag=12.86 +/- 0.03 new_mean_mag=11.9099 delta=0.95 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:16.88 -14:00:54.5: 12.78 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:11.26 -14:08:16.7: 12.94 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:16.88 -14:00:54.5: 12.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.03
Forced photometry filter REJECTED candidate at 07:06:16.88 -14:00:54.5: ref_mag=12.81 +/- 0.03 new_mean_mag=11.9540 delta=0.86 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:58.60 -13:42:04.5: 13.10 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:11.26 -14:08:16.7: 13.00 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:19.63 -14:04:46.4: 12.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:11.26 -14:08:16.7: ref_mag=12.96 +/- 0.03 new_mean_mag=11.8681 delta=1.09 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:58.60 -13:42:04.5: 13.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.04
Forced photometry filter KEPT candidate at 07:05:58.60 -13:42:04.5: ref_mag=13.13 +/- 0.04 new_mean_mag=11.9481 delta=1.18 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:19.63 -14:04:46.4: 13.04 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:43.37 -13:38:04.2: 13.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:19.63 -14:04:46.4: ref_mag=13.01 +/- 0.03 new_mean_mag=11.9330 delta=1.08 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:48.83 -13:36:32.5: 13.16 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:43.37 -13:38:04.2: 13.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.04
Forced photometry filter KEPT candidate at 07:08:43.37 -13:38:04.2: ref_mag=13.12 +/- 0.04 new_mean_mag=11.9671 delta=1.15 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:48.83 -13:36:32.5: 13.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.04
Forced photometry filter KEPT candidate at 07:06:48.83 -13:36:32.5: ref_mag=13.08 +/- 0.04 new_mean_mag=11.9468 delta=1.14 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:55.10 -12:57:33.2: 13.17 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:29.40 -14:02:13.5: 13.14 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:55.10 -12:57:33.2: 13.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
Forced photometry filter KEPT candidate at 07:07:55.10 -12:57:33.2: ref_mag=13.16 +/- 0.04 new_mean_mag=12.1256 delta=1.03 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:29.40 -14:02:13.5: 13.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.04
Forced photometry filter KEPT candidate at 07:09:29.40 -14:02:13.5: ref_mag=13.11 +/- 0.04 new_mean_mag=12.0218 delta=1.09 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:26.92 -13:38:23.1: 13.19 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:26.92 -13:38:23.1: 13.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.04
Forced photometry filter KEPT candidate at 07:09:26.92 -13:38:23.1: ref_mag=13.09 +/- 0.04 new_mean_mag=12.1133 delta=0.98 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:13.88 -13:56:14.0: 13.11 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:13.88 -13:56:14.0: 13.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.04
Forced photometry filter KEPT candidate at 07:09:13.88 -13:56:14.0: ref_mag=13.09 +/- 0.04 new_mean_mag=12.0366 delta=1.06 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:01.06 -14:09:59.8: 13.12 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:01.06 -14:09:59.8: 13.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.04
Forced photometry filter KEPT candidate at 07:05:01.06 -14:09:59.8: ref_mag=13.10 +/- 0.04 new_mean_mag=12.0081 delta=1.10 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:04.59 -13:42:22.7: 13.10 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:45.96 -13:58:36.5: 13.08 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:04.59 -13:42:22.7: 13.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter KEPT candidate at 07:06:04.59 -13:42:22.7: ref_mag=13.12 +/- 0.03 new_mean_mag=12.0291 delta=1.09 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:45.96 -13:58:36.5: 13.18 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.04
Forced photometry filter KEPT candidate at 07:05:45.96 -13:58:36.5: ref_mag=13.13 +/- 0.04 new_mean_mag=11.8771 delta=1.25 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:24.98 -14:02:52.4: 13.05 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:53.83 -14:04:32.8: 13.02 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:24.98 -14:02:52.4: 13.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.04
Forced photometry filter KEPT candidate at 07:05:24.98 -14:02:52.4: ref_mag=13.08 +/- 0.04 new_mean_mag=11.9524 delta=1.13 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:53.83 -14:04:32.8: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Forced photometry filter KEPT candidate at 07:07:53.83 -14:04:32.8: ref_mag=13.02 +/- 0.03 new_mean_mag=12.0316 delta=0.98 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:05.91 -13:53:47.2: 13.05 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:05.91 -13:53:47.2: 13.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:05.91 -13:53:47.2: ref_mag=13.03 +/- 0.03 new_mean_mag=11.9338 delta=1.10 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:28.85 -14:06:43.6: 12.98 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:22.60 -13:25:31.0: 12.97 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:28.85 -14:06:43.6: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.03
Forced photometry filter KEPT candidate at 07:08:28.85 -14:06:43.6: ref_mag=12.96 +/- 0.03 new_mean_mag=11.9109 delta=1.05 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:22.60 -13:25:31.0: 13.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Forced photometry filter KEPT candidate at 07:06:22.60 -13:25:31.0: ref_mag=13.02 +/- 0.03 new_mean_mag=11.8433 delta=1.17 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:05.83 -13:25:34.5: 12.98 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:05.83 -13:25:34.5: 12.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.03
Forced photometry filter KEPT candidate at 07:08:05.83 -13:25:34.5: ref_mag=12.97 +/- 0.03 new_mean_mag=11.9370 delta=1.04 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:10.29 -13:41:36.4: 12.96 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:10.29 -13:41:36.4: 12.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:10.29 -13:41:36.4: ref_mag=12.94 +/- 0.03 new_mean_mag=11.9364 delta=1.00 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:23.71 -14:07:36.1: 12.98 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:28.88 -14:00:34.6: 12.96 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:45.43 -13:04:15.4: 12.94 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:23.71 -14:07:36.1: 12.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.04
Forced photometry filter KEPT candidate at 07:09:23.71 -14:07:36.1: ref_mag=12.98 +/- 0.04 new_mean_mag=11.8899 delta=1.09 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:28.88 -14:00:34.6: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.03
Forced photometry filter KEPT candidate at 07:08:28.88 -14:00:34.6: ref_mag=12.96 +/- 0.03 new_mean_mag=11.9594 delta=1.00 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:45.43 -13:04:15.4: 12.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Forced photometry filter KEPT candidate at 07:06:45.43 -13:04:15.4: ref_mag=12.91 +/- 0.03 new_mean_mag=11.9658 delta=0.94 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:49.70 -13:27:28.7: 12.92 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:49.70 -13:27:28.7: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Forced photometry filter KEPT candidate at 07:06:49.70 -13:27:28.7: ref_mag=12.91 +/- 0.03 new_mean_mag=11.7694 delta=1.14 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:44.04 -13:47:21.9: 12.89 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:44.04 -13:47:21.9: 12.85 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:25.12 -13:58:59.6: 12.89 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.03
Forced photometry filter KEPT candidate at 07:05:44.04 -13:47:21.9: ref_mag=12.87 +/- 0.03 new_mean_mag=11.7703 delta=1.10 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:25.12 -13:58:59.6: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:25.12 -13:58:59.6: ref_mag=12.92 +/- 0.03 new_mean_mag=11.9506 delta=0.97 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:12.23 -13:44:14.7: 12.88 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:12.23 -13:44:14.7: 12.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Forced photometry filter KEPT candidate at 07:06:12.23 -13:44:14.7: ref_mag=12.85 +/- 0.03 new_mean_mag=11.7394 delta=1.11 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:18.69 -13:59:28.4: 12.82 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:18.69 -13:59:28.4: 12.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:18.69 -13:59:28.4: ref_mag=12.86 +/- 0.03 new_mean_mag=11.9045 delta=0.96 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:42.73 -13:36:41.8: 12.85 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:45.89 -13:28:55.8: 12.87 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:42.73 -13:36:41.8: 12.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:42.73 -13:36:41.8: ref_mag=12.87 +/- 0.03 new_mean_mag=11.8408 delta=1.03 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:45.89 -13:28:55.8: 12.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.03
Forced photometry filter KEPT candidate at 07:07:45.89 -13:28:55.8: ref_mag=12.89 +/- 0.03 new_mean_mag=11.9020 delta=0.99 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:58.17 -13:50:32.2: 12.82 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:58.17 -13:50:32.2: 12.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.03
Forced photometry filter KEPT candidate at 07:05:58.17 -13:50:32.2: ref_mag=12.82 +/- 0.03 new_mean_mag=11.7321 delta=1.08 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:27.43 -14:08:48.0: 12.77 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:27.43 -14:08:48.0: 12.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.03
Forced photometry filter KEPT candidate at 07:08:27.43 -14:08:48.0: ref_mag=12.75 +/- 0.03 new_mean_mag=11.8204 delta=0.93 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:30.77 -13:56:57.3: 12.76 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:02.84 -13:24:57.4: 12.76 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:30.77 -13:56:57.3: 12.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.03
Forced photometry filter KEPT candidate at 07:04:30.77 -13:56:57.3: ref_mag=12.76 +/- 0.03 new_mean_mag=11.7418 delta=1.01 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:02.84 -13:24:57.4: 12.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.03
Forced photometry filter KEPT candidate at 07:06:02.84 -13:24:57.4: ref_mag=12.77 +/- 0.03 new_mean_mag=11.7812 delta=0.99 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:32.28 -13:13:35.8: 12.77 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:32.28 -13:13:35.8: 12.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.03
Forced photometry filter KEPT candidate at 07:07:32.28 -13:13:35.8: ref_mag=12.72 +/- 0.03 new_mean_mag=11.7880 delta=0.93 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:25.25 -13:58:31.3: 12.74 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:25.25 -13:58:31.3: 12.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:25.25 -13:58:31.3: ref_mag=12.73 +/- 0.03 new_mean_mag=11.7251 delta=1.01 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:03.29 -13:48:18.0: 12.74 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:03.29 -13:48:18.0: 12.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry filter KEPT candidate at 07:06:03.29 -13:48:18.0: ref_mag=12.72 +/- 0.02 new_mean_mag=11.6414 delta=1.08 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:27.09 -13:29:22.5: 12.74 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:27.09 -13:29:22.5: 12.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.03
Forced photometry filter KEPT candidate at 07:09:27.09 -13:29:22.5: ref_mag=12.76 +/- 0.03 new_mean_mag=11.8241 delta=0.94 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:53.33 -14:04:30.4: 12.68 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:53.33 -14:04:30.4: 12.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter KEPT candidate at 07:08:53.33 -14:04:30.4: ref_mag=12.66 +/- 0.02 new_mean_mag=11.6808 delta=0.98 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:45.65 -13:03:00.9: 12.74 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:45.65 -13:03:00.9: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Forced photometry filter KEPT candidate at 07:06:45.65 -13:03:00.9: ref_mag=12.77 +/- 0.02 new_mean_mag=11.8174 delta=0.95 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:00.75 -13:20:33.2: 12.72 +/- 0.04 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:00.75 -13:20:33.2: 12.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.03
Forced photometry filter KEPT candidate at 07:08:00.75 -13:20:33.2: ref_mag=12.73 +/- 0.03 new_mean_mag=11.7831 delta=0.95 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:49.57 -13:55:21.4: 12.67 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:49.57 -13:55:21.4: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Forced photometry filter KEPT candidate at 07:08:49.57 -13:55:21.4: ref_mag=12.67 +/- 0.02 new_mean_mag=11.7552 delta=0.91 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:42.39 -13:32:26.3: 12.66 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:42.39 -13:32:26.3: 12.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Forced photometry filter KEPT candidate at 07:09:42.39 -13:32:26.3: ref_mag=12.64 +/- 0.02 new_mean_mag=11.6782 delta=0.97 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:50.67 -13:30:13.3: 12.65 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:50.67 -13:30:13.3: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry filter KEPT candidate at 07:06:50.67 -13:30:13.3: ref_mag=12.65 +/- 0.02 new_mean_mag=11.5810 delta=1.07 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:35.18 -13:47:41.1: 12.64 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:34.04 -14:03:41.5: 12.65 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:35.18 -13:47:41.1: 12.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry filter KEPT candidate at 07:05:35.18 -13:47:41.1: ref_mag=12.62 +/- 0.02 new_mean_mag=11.5006 delta=1.12 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:34.04 -14:03:41.5: 12.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter KEPT candidate at 07:08:34.04 -14:03:41.5: ref_mag=12.66 +/- 0.02 new_mean_mag=11.7183 delta=0.95 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:14.63 -13:36:34.3: 12.64 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:14.63 -13:36:34.3: 12.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry filter KEPT candidate at 07:06:14.63 -13:36:34.3: ref_mag=12.62 +/- 0.02 new_mean_mag=11.5977 delta=1.02 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:06.37 -13:52:36.9: 12.57 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:06.37 -13:52:36.9: 12.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Forced photometry filter KEPT candidate at 07:06:06.37 -13:52:36.9: ref_mag=12.56 +/- 0.02 new_mean_mag=11.6063 delta=0.96 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:57.92 -13:31:14.6: 12.59 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:57.92 -13:31:14.6: 12.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Forced photometry filter KEPT candidate at 07:06:57.92 -13:31:14.6: ref_mag=12.60 +/- 0.02 new_mean_mag=11.5642 delta=1.03 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:54.20 -14:02:58.9: 12.56 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:54.20 -14:02:58.9: 12.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Forced photometry filter KEPT candidate at 07:08:54.20 -14:02:58.9: ref_mag=12.58 +/- 0.02 new_mean_mag=11.5243 delta=1.05 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:50.37 -14:06:20.4: 12.56 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:50.37 -14:06:20.4: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Forced photometry filter KEPT candidate at 07:08:50.37 -14:06:20.4: ref_mag=12.57 +/- 0.02 new_mean_mag=11.5028 delta=1.06 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:35.38 -14:05:07.6: 12.50 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:35.38 -14:05:07.6: 12.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Forced photometry filter KEPT candidate at 07:04:35.38 -14:05:07.6: ref_mag=12.47 +/- 0.02 new_mean_mag=11.4685 delta=1.00 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:50.50 -14:04:19.2: 12.53 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:50.50 -14:04:19.2: 12.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Forced photometry filter KEPT candidate at 07:04:50.50 -14:04:19.2: ref_mag=12.53 +/- 0.02 new_mean_mag=11.4713 delta=1.06 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:45.17 -13:48:33.7: 12.50 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:49.44 -13:54:04.2: 12.43 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:45.17 -13:48:33.7: 12.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Forced photometry filter KEPT candidate at 07:06:45.17 -13:48:33.7: ref_mag=12.51 +/- 0.02 new_mean_mag=11.4700 delta=1.04 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:49.44 -13:54:04.2: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.02
Forced photometry filter KEPT candidate at 07:09:49.44 -13:54:04.2: ref_mag=12.44 +/- 0.02 new_mean_mag=11.3696 delta=1.07 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:13.56 -13:43:57.1: 12.42 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:13.56 -13:43:57.1: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.02
Forced photometry filter KEPT candidate at 07:05:13.56 -13:43:57.1: ref_mag=12.43 +/- 0.02 new_mean_mag=11.4289 delta=1.00 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:47.45 -14:00:56.7: 12.45 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:47.45 -14:00:56.7: 12.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.02
Forced photometry filter KEPT candidate at 07:09:47.45 -14:00:56.7: ref_mag=12.41 +/- 0.02 new_mean_mag=11.3256 delta=1.08 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:55.37 -13:46:41.3: 12.43 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:55.37 -13:46:41.3: 12.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.02
Forced photometry filter KEPT candidate at 07:05:55.37 -13:46:41.3: ref_mag=12.41 +/- 0.02 new_mean_mag=11.3018 delta=1.11 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:13.84 -13:16:37.8: 12.39 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:13.84 -13:16:37.8: 12.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Forced photometry filter KEPT candidate at 07:06:13.84 -13:16:37.8: ref_mag=12.35 +/- 0.02 new_mean_mag=11.4180 delta=0.93 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:51.43 -14:04:29.1: 12.38 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:51.43 -14:04:29.1: 12.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.02
Forced photometry filter KEPT candidate at 07:08:51.43 -14:04:29.1: ref_mag=12.40 +/- 0.02 new_mean_mag=11.3909 delta=1.01 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:36.98 -13:26:37.9: 12.38 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:36.98 -13:26:37.9: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Forced photometry filter KEPT candidate at 07:06:36.98 -13:26:37.9: ref_mag=12.36 +/- 0.02 new_mean_mag=11.3067 delta=1.05 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:53.49 -13:35:56.4: 12.36 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:53.49 -13:35:56.4: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.02
Forced photometry filter KEPT candidate at 07:05:53.49 -13:35:56.4: ref_mag=12.39 +/- 0.02 new_mean_mag=11.3988 delta=0.99 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:53.68 -13:59:44.8: 12.36 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:45.64 -14:02:58.8: 12.34 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:53.68 -13:59:44.8: 12.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Forced photometry filter KEPT candidate at 07:04:53.68 -13:59:44.8: ref_mag=12.36 +/- 0.02 new_mean_mag=11.3203 delta=1.04 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:45.64 -14:02:58.8: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Forced photometry filter KEPT candidate at 07:04:45.64 -14:02:58.8: ref_mag=12.33 +/- 0.02 new_mean_mag=11.2996 delta=1.03 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:22.65 -13:58:34.7: 12.33 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:22.65 -13:58:34.7: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Forced photometry filter KEPT candidate at 07:05:22.65 -13:58:34.7: ref_mag=12.33 +/- 0.02 new_mean_mag=11.3057 delta=1.02 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:21.67 -14:08:18.5: 12.26 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:40.01 -14:00:48.2: 12.23 +/- 0.03 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:01.71 -14:05:04.7: 12.18 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:21.67 -14:08:18.5: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Forced photometry filter KEPT candidate at 07:08:21.67 -14:08:18.5: ref_mag=12.25 +/- 0.02 new_mean_mag=11.3081 delta=0.94 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:40.01 -14:00:48.2: 12.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Forced photometry filter KEPT candidate at 07:09:40.01 -14:00:48.2: ref_mag=12.25 +/- 0.02 new_mean_mag=11.2831 delta=0.96 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:01.71 -14:05:04.7: 12.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 07:09:01.71 -14:05:04.7: ref_mag=12.18 +/- 0.01 new_mean_mag=11.2433 delta=0.93 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:44.01 -13:46:09.9: 12.17 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:44.01 -13:46:09.9: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.02
Forced photometry filter KEPT candidate at 07:09:44.01 -13:46:09.9: ref_mag=12.17 +/- 0.02 new_mean_mag=11.1711 delta=0.99 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:48.57 -14:04:34.5: 12.15 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:48.57 -14:04:34.5: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.02
Forced photometry filter KEPT candidate at 07:08:48.57 -14:04:34.5: ref_mag=12.17 +/- 0.02 new_mean_mag=11.2060 delta=0.96 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:34.86 -13:30:56.8: 12.08 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:34.86 -13:30:56.8: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry filter REJECTED candidate at 07:07:34.86 -13:30:56.8: ref_mag=12.10 +/- 0.01 new_mean_mag=11.2255 delta=0.88 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:16.09 -14:05:31.0: 12.13 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:16.09 -14:05:31.0: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.02
Forced photometry filter KEPT candidate at 07:09:16.09 -14:05:31.0: ref_mag=12.14 +/- 0.02 new_mean_mag=11.1683 delta=0.97 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:49.56 -13:22:51.3: 12.12 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:49.56 -13:22:51.3: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter KEPT candidate at 07:06:49.56 -13:22:51.3: ref_mag=12.12 +/- 0.01 new_mean_mag=11.2119 delta=0.91 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:47.41 -13:38:15.2: 12.09 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:47.41 -13:38:15.2: 12.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter KEPT candidate at 07:06:47.41 -13:38:15.2: ref_mag=12.06 +/- 0.01 new_mean_mag=11.1061 delta=0.95 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:42.65 -13:36:28.3: 12.10 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:42.65 -13:36:28.3: 12.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter KEPT candidate at 07:05:42.65 -13:36:28.3: ref_mag=12.11 +/- 0.01 new_mean_mag=11.1152 delta=1.00 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:44.76 -13:54:06.4: 12.08 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:44.76 -13:54:06.4: 12.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter KEPT candidate at 07:09:44.76 -13:54:06.4: ref_mag=12.06 +/- 0.01 new_mean_mag=11.0603 delta=1.00 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:21.81 -14:06:20.0: 12.09 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:21.81 -14:06:20.0: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry filter KEPT candidate at 07:04:21.81 -14:06:20.0: ref_mag=12.04 +/- 0.01 new_mean_mag=11.0888 delta=0.96 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:15.06 -14:00:32.8: 12.02 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:05.03 -13:31:34.4: 11.99 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:15.06 -14:00:32.8: 12.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter KEPT candidate at 07:09:15.06 -14:00:32.8: ref_mag=12.02 +/- 0.01 new_mean_mag=11.0844 delta=0.93 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:05.03 -13:31:34.4: 11.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter KEPT candidate at 07:07:05.03 -13:31:34.4: ref_mag=11.98 +/- 0.01 new_mean_mag=11.0557 delta=0.92 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:30.48 -13:53:31.0: 11.98 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:30.48 -13:53:31.0: 11.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter KEPT candidate at 07:09:30.48 -13:53:31.0: ref_mag=11.98 +/- 0.01 new_mean_mag=11.0253 delta=0.96 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:47.67 -14:09:04.2: 11.95 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:47.67 -14:09:04.2: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter KEPT candidate at 07:04:47.67 -14:09:04.2: ref_mag=11.98 +/- 0.01 new_mean_mag=10.9326 delta=1.05 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:28.31 -13:55:00.5: 11.90 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:28.31 -13:55:00.5: 11.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter KEPT candidate at 07:09:28.31 -13:55:00.5: ref_mag=11.90 +/- 0.01 new_mean_mag=10.9681 delta=0.93 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:27.63 -13:58:53.0: 11.78 +/- 0.02 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:27.63 -13:58:53.0: 11.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Forced photometry filter KEPT candidate at 07:09:27.63 -13:58:53.0: ref_mag=11.79 +/- 0.01 new_mean_mag=10.8671 delta=0.93 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:36.49 -13:42:46.5: 13.47 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:36.49 -13:42:46.5: 13.38 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.05
Forced photometry filter KEPT candidate at 07:09:36.49 -13:42:46.5: ref_mag=13.42 +/- 0.05 new_mean_mag=12.2431 delta=1.18 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:32.36 -14:01:13.0: 11.69 +/- 0.01 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:32.36 -14:01:13.0: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Forced photometry filter KEPT candidate at 07:05:32.36 -14:01:13.0: ref_mag=11.67 +/- 0.01 new_mean_mag=10.6503 delta=1.02 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:41.75 -13:43:33.3: 11.47 +/- 0.01 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:41.75 -13:43:33.3: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Forced photometry filter KEPT candidate at 07:06:41.75 -13:43:33.3: ref_mag=11.46 +/- 0.01 new_mean_mag=10.5127 delta=0.95 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:10.60 -14:02:21.1: 13.42 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:10.60 -14:02:21.1: 13.35 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
Forced photometry filter KEPT candidate at 07:09:10.60 -14:02:21.1: ref_mag=13.38 +/- 0.05 new_mean_mag=12.3143 delta=1.06 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:10.94 -14:02:48.1: 13.40 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:20.42 -14:07:21.3: 13.38 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:10.94 -14:02:48.1: 13.42 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:08:51.54 -13:58:18.2: 13.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.05
Forced photometry filter KEPT candidate at 07:09:10.94 -14:02:48.1: ref_mag=13.41 +/- 0.05 new_mean_mag=12.3408 delta=1.07 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:20.42 -14:07:21.3: 13.38 +/- 0.07 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:08:51.54 -13:58:18.2: 13.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
Forced photometry reference-image weighted average: 13.27 +/- 0.04
Forced photometry filter KEPT candidate at 07:09:20.42 -14:07:21.3: ref_mag=13.38 +/- 0.05 new_mean_mag=12.2375 delta=1.14 (need > 0.90)
Forced photometry filter KEPT candidate at 07:08:51.54 -13:58:18.2: ref_mag=13.27 +/- 0.04 new_mean_mag=12.1765 delta=1.10 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:07:52.39 -13:41:14.9: 13.28 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:07:52.39 -13:41:14.9: 13.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.04
Forced photometry filter KEPT candidate at 07:07:52.39 -13:41:14.9: ref_mag=13.28 +/- 0.04 new_mean_mag=12.1121 delta=1.17 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:05:50.55 -14:07:17.9: 13.24 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:05:50.55 -14:07:17.9: 13.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.04
Forced photometry filter KEPT candidate at 07:05:50.55 -14:07:17.9: ref_mag=13.23 +/- 0.04 new_mean_mag=12.0539 delta=1.18 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:06:54.55 -13:24:15.9: 13.21 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:06:54.55 -13:24:15.9: 13.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.04
Forced photometry filter KEPT candidate at 07:06:54.55 -13:24:15.9: ref_mag=13.22 +/- 0.04 new_mean_mag=12.1200 delta=1.10 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:09:11.21 -13:30:45.0: 13.22 +/- 0.05 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:09:11.21 -13:30:45.0: 13.18 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.04
Forced photometry filter KEPT candidate at 07:09:11.21 -13:30:45.0: ref_mag=13.20 +/- 0.04 new_mean_mag=12.2311 delta=0.97 (need > 0.90)
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-22-41_20.00sec_-4.90C_LIGHT_0023.fits at 07:04:37.38 -14:00:11.7: 13.19 +/- 0.06 detection
Forced photometry on wcs_Mon-05-Q2b1x1_2026-04-08_21-23-15_20.00sec_-4.90C_LIGHT_0024.fits at 07:04:37.38 -14:00:11.7: 13.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.04
Forced photometry filter KEPT candidate at 07:04:37.38 -14:00:11.7: ref_mag=13.23 +/- 0.04 new_mean_mag=12.1557 delta=1.07 (need > 0.90)
Adding exclusion_list_local.txt__out116239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163255.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 119s
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: 60s
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Considering the candidate 186512_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 186512_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
**** FOUND 07:07:56.41 -06:01:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186513_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 186513_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
**** FOUND 07:05:46.05 -12:48:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186517_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 186517_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
**** FOUND 07:07:13.95 -08:02:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186518_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 186518_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
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Considering the candidate 188231_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 188231_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
**** FOUND 07:07:00.20 -12:15:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188497_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 188497_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
**** FOUND 06:58:31.21 -07:10:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188519_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 188519_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
**** FOUND 07:05:43.64 -10:39:34.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 73896_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 73896_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
**** FOUND 06:41:56.68 -09:10:05.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 163224_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 163224_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162556_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162556_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 121030_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 121030_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 146666_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 146666_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 118213_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 118213_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 148030_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 148030_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 146158_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 146158_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 118007_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 118007_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
**** FOUND 07:07:01.05 -13:41:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146229_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 146229_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
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Considering the candidate 163172_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 163172_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162826_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162826_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162665_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162665_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162858_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162858_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 116379_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 116379_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162605_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162605_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162762_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162762_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 161169_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161169_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162186_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162186_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 144042_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 144042_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 121201_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 121201_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 116389_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 116389_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 116697_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 116697_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162721_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162721_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 118111_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 118111_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 141723_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 141723_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 163308_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 163308_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
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Considering the candidate 161049_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161049_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162063_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162063_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 116370_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 116370_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 118324_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 118324_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 118874_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 118874_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 128452_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 128452_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162595_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162595_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 118104_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 118104_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 149905_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 149905_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 161223_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161223_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117465_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 117465_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 149901_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 149901_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162894_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162894_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162128_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162128_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 149379_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 149379_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162048_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162048_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 121422_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 121422_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 121238_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 121238_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 117884_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 117884_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 161141_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161141_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162998_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162998_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 126745_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 126745_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 121164_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 121164_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 134784_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 134784_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 163041_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 163041_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 117949_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 117949_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 163155_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 163155_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 118356_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 118356_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 116656_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 116656_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 140979_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 140979_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 161757_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161757_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 147113_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 147113_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 122464_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 122464_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 124240_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 124240_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162996_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162996_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 137690_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 137690_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 120259_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 120259_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162105_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162105_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 127211_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 127211_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 122514_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 122514_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 148229_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 148229_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 119564_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 119564_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 120351_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 120351_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 116272_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 116272_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
**** FOUND 07:05:03.13 -13:54:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133304_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 133304_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162589_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162589_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 118784_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 118784_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 144049_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 144049_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 120030_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 120030_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162321_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162321_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 161723_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161723_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 161619_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161619_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 162748_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162748_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 135749_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 135749_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
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Considering the candidate 116240_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 116240_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117125_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 117125_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162834_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162834_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130622_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 130622_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123655_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 123655_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162091_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162091_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121317_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 121317_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119054_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 119054_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162400_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162400_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163087_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 163087_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150076_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 150076_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161290_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161290_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162841_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162841_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162213_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162213_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138575_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 138575_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161997_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161997_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119768_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 119768_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161783_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161783_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122238_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 122238_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118495_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 118495_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118941_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 118941_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116239_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 116239_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162205_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162205_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163255_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 163255_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119607_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 119607_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147990_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 147990_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161502_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161502_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150714_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 150714_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163055_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 163055_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127684_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 127684_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163173_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 163173_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117218_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 117218_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162578_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162578_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161238_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161238_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161243_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 161243_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163234_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 163234_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117634_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 117634_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162074_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 162074_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122219_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 122219_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120117_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 120117_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163032_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
Preparing report for the candidate 163032_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71161_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292
The candidate 71161_fd_Mon-05-Q2b1x1_2026-10-11_03-33-30_20.00sec_-0.00C_LIGHT_0292 did not pass the final checks
**** FOUND 06:47:37.29 -08:59:56.3 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 11s
make_report_in_HTML.sh TOTAL: 190s
Prepared the HTML report for the field Mon-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:09:44.76 -13:54:06.4
07:09:49.44 -13:54:04.2
07:05:58.60 -13:42:04.5
07:05:35.89 -13:42:00.8
07:07:15.75 -13:41:05.7
07:07:45.89 -13:28:55.8
07:07:59.71 -13:22:12.9
07:05:13.56 -13:43:57.1
07:06:41.75 -13:43:33.3
07:06:04.59 -13:42:22.7
07:07:52.39 -13:41:14.9
07:09:10.29 -13:41:36.4
07:06:12.23 -13:44:14.7
07:09:26.92 -13:38:23.1
07:09:45.43 -13:38:19.2
07:05:51.49 -13:40:57.7
07:08:43.37 -13:38:04.2
07:09:42.73 -13:36:41.8
07:06:47.41 -13:38:15.2
07:06:14.63 -13:36:34.3
07:06:48.83 -13:36:32.5
07:05:42.65 -13:36:28.3
07:05:53.49 -13:35:56.4
07:09:42.39 -13:32:26.3
07:07:05.03 -13:31:34.4
07:06:57.92 -13:31:14.6
07:09:11.21 -13:30:45.0
07:09:27.09 -13:29:22.5
07:06:50.67 -13:30:13.3
07:09:42.94 -13:25:52.4
07:06:49.70 -13:27:28.7
07:06:30.73 -13:26:20.8
07:08:05.83 -13:25:34.5
07:06:36.98 -13:26:37.9
07:06:22.60 -13:25:31.0
07:06:54.55 -13:24:15.9
07:06:49.56 -13:22:51.3
07:06:02.84 -13:24:57.4
07:08:00.75 -13:20:33.2
07:06:13.84 -13:16:37.8
07:07:32.28 -13:13:35.8
07:06:45.43 -13:04:15.4
07:06:45.65 -13:03:00.9
07:09:36.49 -13:42:46.5
07:07:55.10 -12:57:33.2
07:05:55.37 -13:46:41.3
07:05:35.18 -13:47:41.1
07:05:44.04 -13:47:21.9
07:06:45.17 -13:48:33.7
07:06:03.29 -13:48:18.0
07:09:44.01 -13:46:09.9
07:05:58.17 -13:50:32.2
07:09:04.23 -13:49:41.3
07:06:06.86 -13:52:57.1
07:06:06.37 -13:52:36.9
07:09:10.99 -13:53:31.6
07:05:43.87 -13:54:15.5
07:04:30.77 -13:56:57.3
07:09:30.48 -13:53:31.0
07:05:42.40 -13:56:55.1
07:08:49.57 -13:55:21.4
07:09:05.91 -13:53:47.2
07:05:45.96 -13:58:36.5
07:09:13.88 -13:56:14.0
07:05:22.65 -13:58:34.7
07:09:28.31 -13:55:00.5
07:09:11.26 -14:08:16.7
07:09:23.71 -14:07:36.1
07:08:57.25 -14:09:08.1
07:05:01.06 -14:09:59.8
07:09:10.94 -14:02:48.1
07:09:20.42 -14:07:21.3
07:08:21.67 -14:08:18.5
07:04:47.67 -14:09:04.2
07:04:35.38 -14:05:07.6
07:08:50.37 -14:06:20.4
07:08:27.43 -14:08:48.0
07:09:16.09 -14:05:31.0
07:08:48.57 -14:04:34.5
07:08:28.85 -14:06:43.6
07:09:19.63 -14:04:46.4
07:05:50.55 -14:07:17.9
07:08:51.43 -14:04:29.1
07:08:53.33 -14:04:30.4
07:07:53.83 -14:04:32.8
07:04:06.93 -14:07:11.7
07:04:21.81 -14:06:20.0
07:09:01.71 -14:05:04.7
07:08:54.20 -14:02:58.9
07:04:53.68 -13:59:44.8
07:05:04.89 -14:04:33.8
07:09:10.60 -14:02:21.1
07:08:34.04 -14:03:41.5
07:09:29.40 -14:02:13.5
07:09:39.63 -14:03:02.4
07:09:32.38 -14:01:26.9
07:09:05.02 -14:03:20.5
07:04:50.50 -14:04:19.2
07:08:15.62 -14:01:49.0
07:04:28.87 -14:03:21.3
07:09:47.45 -14:00:56.7
07:09:40.01 -14:00:48.2
07:06:00.79 -14:03:10.6
07:05:24.98 -14:02:52.4
07:09:25.25 -13:58:31.3
07:08:28.88 -14:00:34.6
07:04:37.38 -14:00:11.7
07:09:25.12 -13:58:59.6
07:09:27.63 -13:58:53.0
07:04:45.64 -14:02:58.8
07:09:18.69 -13:59:28.4
07:05:29.73 -14:01:32.5
07:05:32.36 -14:01:13.0
07:05:58.00 -14:01:10.6
07:08:51.54 -13:58:18.2
07:09:15.06 -14:00:32.8
########### Completed Mon-05-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
07:05:58.00 -14:01:10.6
07:05:04.89 -14:04:33.8
07:09:42.94 -13:25:52.4
07:05:43.87 -13:54:15.5
07:05:51.49 -13:40:57.7
07:05:42.40 -13:56:55.1
07:09:10.99 -13:53:31.6
07:05:29.73 -14:01:32.5
07:04:28.87 -14:03:21.3
07:09:32.38 -14:01:26.9
07:06:00.79 -14:03:10.6
07:05:35.89 -13:42:00.8
07:09:39.63 -14:03:02.4
07:08:15.62 -14:01:49.0
07:08:57.25 -14:09:08.1
07:04:06.93 -14:07:11.7
07:06:06.86 -13:52:57.1
07:06:30.73 -13:26:20.8
07:07:15.75 -13:41:05.7
07:07:59.71 -13:22:12.9
07:09:05.02 -14:03:20.5
07:09:45.43 -13:38:19.2
07:09:04.23 -13:49:41.3
07:09:11.26 -14:08:16.7
07:09:19.63 -14:04:46.4
07:05:58.60 -13:42:04.5
07:08:43.37 -13:38:04.2
07:06:48.83 -13:36:32.5
07:07:55.10 -12:57:33.2
07:09:29.40 -14:02:13.5
07:09:26.92 -13:38:23.1
07:09:13.88 -13:56:14.0
07:05:01.06 -14:09:59.8
07:06:04.59 -13:42:22.7
07:05:45.96 -13:58:36.5
07:05:24.98 -14:02:52.4
07:07:53.83 -14:04:32.8
07:09:05.91 -13:53:47.2
07:08:28.85 -14:06:43.6
07:06:22.60 -13:25:31.0
07:08:05.83 -13:25:34.5
07:09:10.29 -13:41:36.4
07:09:23.71 -14:07:36.1
07:08:28.88 -14:00:34.6
07:06:45.43 -13:04:15.4
07:06:49.70 -13:27:28.7
07:05:44.04 -13:47:21.9
07:09:25.12 -13:58:59.6
07:06:12.23 -13:44:14.7
07:09:18.69 -13:59:28.4
07:09:42.73 -13:36:41.8
07:07:45.89 -13:28:55.8
07:05:58.17 -13:50:32.2
07:08:27.43 -14:08:48.0
07:04:30.77 -13:56:57.3
07:06:02.84 -13:24:57.4
07:07:32.28 -13:13:35.8
07:09:25.25 -13:58:31.3
07:06:03.29 -13:48:18.0
07:09:27.09 -13:29:22.5
07:08:53.33 -14:04:30.4
07:06:45.65 -13:03:00.9
07:08:00.75 -13:20:33.2
07:08:49.57 -13:55:21.4
07:09:42.39 -13:32:26.3
07:06:50.67 -13:30:13.3
07:05:35.18 -13:47:41.1
07:08:34.04 -14:03:41.5
07:06:14.63 -13:36:34.3
07:06:06.37 -13:52:36.9
07:06:57.92 -13:31:14.6
07:08:54.20 -14:02:58.9
07:08:50.37 -14:06:20.4
07:04:35.38 -14:05:07.6
07:04:50.50 -14:04:19.2
07:06:45.17 -13:48:33.7
07:09:49.44 -13:54:04.2
07:05:13.56 -13:43:57.1
07:09:47.45 -14:00:56.7
07:05:55.37 -13:46:41.3
07:06:13.84 -13:16:37.8
07:08:51.43 -14:04:29.1
07:06:36.98 -13:26:37.9
07:05:53.49 -13:35:56.4
07:04:53.68 -13:59:44.8
07:04:45.64 -14:02:58.8
07:05:22.65 -13:58:34.7
07:08:21.67 -14:08:18.5
07:09:40.01 -14:00:48.2
07:09:01.71 -14:05:04.7
07:09:44.01 -13:46:09.9
07:08:48.57 -14:04:34.5
07:09:16.09 -14:05:31.0
07:06:49.56 -13:22:51.3
07:06:47.41 -13:38:15.2
07:05:42.65 -13:36:28.3
07:09:44.76 -13:54:06.4
07:04:21.81 -14:06:20.0
07:09:15.06 -14:00:32.8
07:07:05.03 -13:31:34.4
07:09:30.48 -13:53:31.0
07:04:47.67 -14:09:04.2
07:09:28.31 -13:55:00.5
07:09:27.63 -13:58:53.0
07:09:36.49 -13:42:46.5
07:05:32.36 -14:01:13.0
07:06:41.75 -13:43:33.3
07:09:10.60 -14:02:21.1
07:09:10.94 -14:02:48.1
07:09:20.42 -14:07:21.3
07:08:51.54 -13:58:18.2
07:07:52.39 -13:41:14.9
07:05:50.55 -14:07:17.9
07:06:54.55 -13:24:15.9
07:09:11.21 -13:30:45.0
07:04:37.38 -14:00:11.7
###################################################################################
07:05:58.00 -14:01:10.6 -- not an asteroid (will add it to exclusion list)
07:05:04.89 -14:04:33.8 -- not an asteroid (will add it to exclusion list)
07:09:42.94 -13:25:52.4 -- not an asteroid (will add it to exclusion list)
07:05:43.87 -13:54:15.5 -- not an asteroid (will add it to exclusion list)
07:05:51.49 -13:40:57.7 -- not an asteroid (will add it to exclusion list)
07:05:42.40 -13:56:55.1 -- not an asteroid (will add it to exclusion list)
07:09:10.99 -13:53:31.6 -- not an asteroid (will add it to exclusion list)
07:05:29.73 -14:01:32.5 -- not an asteroid (will add it to exclusion list)
07:04:28.87 -14:03:21.3 -- not an asteroid (will add it to exclusion list)
07:09:32.38 -14:01:26.9 -- not an asteroid (will add it to exclusion list)
07:06:00.79 -14:03:10.6 -- not an asteroid (will add it to exclusion list)
07:05:35.89 -13:42:00.8 -- not an asteroid (will add it to exclusion list)
07:09:39.63 -14:03:02.4 -- not an asteroid (will add it to exclusion list)
07:08:15.62 -14:01:49.0 -- not an asteroid (will add it to exclusion list)
07:08:57.25 -14:09:08.1 -- not an asteroid (will add it to exclusion list)
07:04:06.93 -14:07:11.7 -- not an asteroid (will add it to exclusion list)
07:06:06.86 -13:52:57.1 -- not an asteroid (will add it to exclusion list)
07:06:30.73 -13:26:20.8 -- not an asteroid (will add it to exclusion list)
07:07:15.75 -13:41:05.7 -- not an asteroid (will add it to exclusion list)
07:07:59.71 -13:22:12.9 -- not an asteroid (will add it to exclusion list)
07:09:05.02 -14:03:20.5 -- not an asteroid (will add it to exclusion list)
07:09:45.43 -13:38:19.2 -- not an asteroid (will add it to exclusion list)
07:09:04.23 -13:49:41.3 -- not an asteroid (will add it to exclusion list)
07:09:11.26 -14:08:16.7 -- not an asteroid (will add it to exclusion list)
07:09:19.63 -14:04:46.4 -- not an asteroid (will add it to exclusion list)
07:05:58.60 -13:42:04.5 -- not an asteroid (will add it to exclusion list)
07:08:43.37 -13:38:04.2 -- not an asteroid (will add it to exclusion list)
07:06:48.83 -13:36:32.5 -- not an asteroid (will add it to exclusion list)
07:07:55.10 -12:57:33.2 -- not an asteroid (will add it to exclusion list)
07:09:29.40 -14:02:13.5 -- not an asteroid (will add it to exclusion list)
07:09:26.92 -13:38:23.1 -- not an asteroid (will add it to exclusion list)
07:09:13.88 -13:56:14.0 -- not an asteroid (will add it to exclusion list)
07:05:01.06 -14:09:59.8 -- not an asteroid (will add it to exclusion list)
07:06:04.59 -13:42:22.7 -- not an asteroid (will add it to exclusion list)
07:05:45.96 -13:58:36.5 -- not an asteroid (will add it to exclusion list)
07:05:24.98 -14:02:52.4 -- not an asteroid (will add it to exclusion list)
07:07:53.83 -14:04:32.8 -- not an asteroid (will add it to exclusion list)
07:09:05.91 -13:53:47.2 -- not an asteroid (will add it to exclusion list)
07:08:28.85 -14:06:43.6 -- not an asteroid (will add it to exclusion list)
07:06:22.60 -13:25:31.0 -- not an asteroid (will add it to exclusion list)
07:08:05.83 -13:25:34.5 -- not an asteroid (will add it to exclusion list)
07:09:10.29 -13:41:36.4 -- not an asteroid (will add it to exclusion list)
07:09:23.71 -14:07:36.1 -- not an asteroid (will add it to exclusion list)
07:08:28.88 -14:00:34.6 -- not an asteroid (will add it to exclusion list)
07:06:45.43 -13:04:15.4 -- not an asteroid (will add it to exclusion list)
07:06:49.70 -13:27:28.7 -- not an asteroid (will add it to exclusion list)
07:05:44.04 -13:47:21.9 -- not an asteroid (will add it to exclusion list)
07:09:25.12 -13:58:59.6 -- not an asteroid (will add it to exclusion list)
07:06:12.23 -13:44:14.7 -- not an asteroid (will add it to exclusion list)
07:09:18.69 -13:59:28.4 -- not an asteroid (will add it to exclusion list)
07:09:42.73 -13:36:41.8 -- not an asteroid (will add it to exclusion list)
07:07:45.89 -13:28:55.8 -- not an asteroid (will add it to exclusion list)
07:05:58.17 -13:50:32.2 -- not an asteroid (will add it to exclusion list)
07:08:27.43 -14:08:48.0 -- not an asteroid (will add it to exclusion list)
07:04:30.77 -13:56:57.3 -- not an asteroid (will add it to exclusion list)
07:06:02.84 -13:24:57.4 -- not an asteroid (will add it to exclusion list)
07:07:32.28 -13:13:35.8 -- not an asteroid (will add it to exclusion list)
07:09:25.25 -13:58:31.3 -- not an asteroid (will add it to exclusion list)
07:06:03.29 -13:48:18.0 -- not an asteroid (will add it to exclusion list)
07:09:27.09 -13:29:22.5 -- not an asteroid (will add it to exclusion list)
07:08:53.33 -14:04:30.4 -- not an asteroid (will add it to exclusion list)
07:06:45.65 -13:03:00.9 -- not an asteroid (will add it to exclusion list)
07:08:00.75 -13:20:33.2 -- not an asteroid (will add it to exclusion list)
07:08:49.57 -13:55:21.4 -- not an asteroid (will add it to exclusion list)
07:09:42.39 -13:32:26.3 -- not an asteroid (will add it to exclusion list)
07:06:50.67 -13:30:13.3 -- not an asteroid (will add it to exclusion list)
07:05:35.18 -13:47:41.1 -- not an asteroid (will add it to exclusion list)
07:08:34.04 -14:03:41.5 -- not an asteroid (will add it to exclusion list)
07:06:14.63 -13:36:34.3 -- not an asteroid (will add it to exclusion list)
07:06:06.37 -13:52:36.9 -- not an asteroid (will add it to exclusion list)
07:06:57.92 -13:31:14.6 -- not an asteroid (will add it to exclusion list)
07:08:54.20 -14:02:58.9 -- not an asteroid (will add it to exclusion list)
07:08:50.37 -14:06:20.4 -- not an asteroid (will add it to exclusion list)
07:04:35.38 -14:05:07.6 -- not an asteroid (will add it to exclusion list)
07:04:50.50 -14:04:19.2 -- not an asteroid (will add it to exclusion list)
07:06:45.17 -13:48:33.7 -- not an asteroid (will add it to exclusion list)
07:09:49.44 -13:54:04.2 -- not an asteroid (will add it to exclusion list)
07:05:13.56 -13:43:57.1 -- not an asteroid (will add it to exclusion list)
07:09:47.45 -14:00:56.7 -- not an asteroid (will add it to exclusion list)
07:05:55.37 -13:46:41.3 -- not an asteroid (will add it to exclusion list)
07:06:13.84 -13:16:37.8 -- not an asteroid (will add it to exclusion list)
07:08:51.43 -14:04:29.1 -- not an asteroid (will add it to exclusion list)
07:06:36.98 -13:26:37.9 -- not an asteroid (will add it to exclusion list)
07:05:53.49 -13:35:56.4 -- not an asteroid (will add it to exclusion list)
07:04:53.68 -13:59:44.8 -- not an asteroid (will add it to exclusion list)
07:04:45.64 -14:02:58.8 -- not an asteroid (will add it to exclusion list)
07:05:22.65 -13:58:34.7 -- not an asteroid (will add it to exclusion list)
07:08:21.67 -14:08:18.5 -- not an asteroid (will add it to exclusion list)
07:09:40.01 -14:00:48.2 -- not an asteroid (will add it to exclusion list)
07:09:01.71 -14:05:04.7 -- not an asteroid (will add it to exclusion list)
07:09:44.01 -13:46:09.9 -- not an asteroid (will add it to exclusion list)
07:08:48.57 -14:04:34.5 -- not an asteroid (will add it to exclusion list)
07:09:16.09 -14:05:31.0 -- not an asteroid (will add it to exclusion list)
07:06:49.56 -13:22:51.3 -- not an asteroid (will add it to exclusion list)
07:06:47.41 -13:38:15.2 -- not an asteroid (will add it to exclusion list)
07:05:42.65 -13:36:28.3 -- not an asteroid (will add it to exclusion list)
07:09:44.76 -13:54:06.4 -- not an asteroid (will add it to exclusion list)
07:04:21.81 -14:06:20.0 -- not an asteroid (will add it to exclusion list)
07:09:15.06 -14:00:32.8 -- not an asteroid (will add it to exclusion list)
07:07:05.03 -13:31:34.4 -- not an asteroid (will add it to exclusion list)
07:09:30.48 -13:53:31.0 -- not an asteroid (will add it to exclusion list)
07:04:47.67 -14:09:04.2 -- not an asteroid (will add it to exclusion list)
07:09:28.31 -13:55:00.5 -- not an asteroid (will add it to exclusion list)
07:09:27.63 -13:58:53.0 -- not an asteroid (will add it to exclusion list)
07:09:36.49 -13:42:46.5 -- not an asteroid (will add it to exclusion list)
07:05:32.36 -14:01:13.0 -- not an asteroid (will add it to exclusion list)
07:06:41.75 -13:43:33.3 -- not an asteroid (will add it to exclusion list)
07:09:10.60 -14:02:21.1 -- not an asteroid (will add it to exclusion list)
07:09:10.94 -14:02:48.1 -- not an asteroid (will add it to exclusion list)
07:09:20.42 -14:07:21.3 -- not an asteroid (will add it to exclusion list)
07:08:51.54 -13:58:18.2 -- not an asteroid (will add it to exclusion list)
07:07:52.39 -13:41:14.9 -- not an asteroid (will add it to exclusion list)
07:05:50.55 -14:07:17.9 -- not an asteroid (will add it to exclusion list)
07:06:54.55 -13:24:15.9 -- not an asteroid (will add it to exclusion list)
07:09:11.21 -13:30:45.0 -- not an asteroid (will add it to exclusion list)
07:04:37.38 -14:00:11.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
07:04:06.93 -14:07:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:21.81 -14:06:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:28.87 -14:03:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:30.77 -13:56:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:35.38 -14:05:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:37.38 -14:00:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:45.64 -14:02:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:47.67 -14:09:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:50.50 -14:04:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:53.68 -13:59:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:01.06 -14:09:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:04.89 -14:04:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:13.56 -13:43:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:22.65 -13:58:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:24.98 -14:02:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:29.73 -14:01:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:32.36 -14:01:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:35.18 -13:47:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:35.89 -13:42:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:42.40 -13:56:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:42.65 -13:36:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:43.87 -13:54:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:44.04 -13:47:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:45.96 -13:58:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:50.55 -14:07:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:51.49 -13:40:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:53.49 -13:35:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:55.37 -13:46:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:58.00 -14:01:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:58.17 -13:50:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:58.60 -13:42:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:00.79 -14:03:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:02.84 -13:24:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:03.29 -13:48:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:04.59 -13:42:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:06.37 -13:52:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:06.86 -13:52:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:12.23 -13:44:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:13.84 -13:16:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:14.63 -13:36:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:22.60 -13:25:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:30.73 -13:26:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:36.98 -13:26:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:41.75 -13:43:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:45.17 -13:48:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:45.43 -13:04:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:45.65 -13:03:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:47.41 -13:38:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:48.83 -13:36:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:49.56 -13:22:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:49.70 -13:27:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:50.67 -13:30:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:54.55 -13:24:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:57.92 -13:31:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:05.03 -13:31:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:15.75 -13:41:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:32.28 -13:13:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:45.89 -13:28:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:52.39 -13:41:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:53.83 -14:04:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:55.10 -12:57:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:59.71 -13:22:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:00.75 -13:20:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:05.83 -13:25:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:15.62 -14:01:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:21.67 -14:08:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:27.43 -14:08:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:28.85 -14:06:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:28.88 -14:00:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:34.04 -14:03:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.37 -13:38:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:48.57 -14:04:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:49.57 -13:55:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:50.37 -14:06:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:51.43 -14:04:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:51.54 -13:58:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:53.33 -14:04:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:54.20 -14:02:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:57.25 -14:09:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:01.71 -14:05:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:04.23 -13:49:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:05.02 -14:03:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:05.91 -13:53:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:10.29 -13:41:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:10.60 -14:02:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:10.94 -14:02:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:10.99 -13:53:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:11.21 -13:30:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:11.26 -14:08:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:13.88 -13:56:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:15.06 -14:00:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:16.09 -14:05:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:18.69 -13:59:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:19.63 -14:04:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:20.42 -14:07:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:23.71 -14:07:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:25.12 -13:58:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:25.25 -13:58:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:26.92 -13:38:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:27.09 -13:29:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:27.63 -13:58:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:28.31 -13:55:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:29.40 -14:02:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:30.48 -13:53:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:32.38 -14:01:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:36.49 -13:42:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:39.63 -14:03:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:40.01 -14:00:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:42.39 -13:32:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:42.73 -13:36:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:42.94 -13:25:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:44.01 -13:46:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:44.76 -13:54:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:45.43 -13:38:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:47.45 -14:00:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:49.44 -13:54:04.2 -- 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)
07:04:06.93 -14:07:11.7 -- not a known variable star
07:04:21.81 -14:06:20.0 -- a known variable star
07:04:28.87 -14:03:21.3 -- not a known variable star
07:04:30.77 -13:56:57.3 -- not a known variable star
07:04:35.38 -14:05:07.6 -- not a known variable star
07:04:37.38 -14:00:11.7 -- a known variable star
07:04:45.64 -14:02:58.8 -- not a known variable star
07:04:47.67 -14:09:04.2 -- not a known variable star
07:04:50.50 -14:04:19.2 -- not a known variable star
07:04:53.68 -13:59:44.8 -- a known variable star
07:05:01.06 -14:09:59.8 -- not a known variable star
07:05:04.89 -14:04:33.8 -- not a known variable star
07:05:13.56 -13:43:57.1 -- not a known variable star
07:05:22.65 -13:58:34.7 -- not a known variable star
07:05:24.98 -14:02:52.4 -- not a known variable star
07:05:29.73 -14:01:32.5 -- not a known variable star
07:05:32.36 -14:01:13.0 -- not a known variable star
07:05:35.18 -13:47:41.1 -- not a known variable star
07:05:35.89 -13:42:00.8 -- not a known variable star
07:05:42.40 -13:56:55.1 -- not a known variable star
07:05:42.65 -13:36:28.3 -- not a known variable star
07:05:43.87 -13:54:15.5 -- a known variable star
07:05:44.04 -13:47:21.9 -- a known variable star
07:05:45.96 -13:58:36.5 -- a known variable star
07:05:50.55 -14:07:17.9 -- not a known variable star
07:05:51.49 -13:40:57.7 -- not a known variable star
07:05:53.49 -13:35:56.4 -- a known variable star
07:05:55.37 -13:46:41.3 -- not a known variable star
07:05:58.00 -14:01:10.6 -- not a known variable star
07:05:58.17 -13:50:32.2 -- not a known variable star
07:05:58.60 -13:42:04.5 -- not a known variable star
07:06:00.79 -14:03:10.6 -- not a known variable star
07:06:02.84 -13:24:57.4 -- not a known variable star
07:06:03.29 -13:48:18.0 -- not a known variable star
07:06:04.59 -13:42:22.7 -- a known variable star
07:06:06.37 -13:52:36.9 -- not a known variable star
07:06:06.86 -13:52:57.1 -- not a known variable star
07:06:12.23 -13:44:14.7 -- not a known variable star
07:06:13.84 -13:16:37.8 -- not a known variable star
07:06:14.63 -13:36:34.3 -- not a known variable star
07:06:22.60 -13:25:31.0 -- not a known variable star
07:06:30.73 -13:26:20.8 -- not a known variable star
07:06:36.98 -13:26:37.9 -- a known variable star
07:06:41.75 -13:43:33.3 -- not a known variable star
07:06:45.17 -13:48:33.7 -- not a known variable star
07:06:45.43 -13:04:15.4 -- not a known variable star
07:06:45.65 -13:03:00.9 -- not a known variable star
07:06:47.41 -13:38:15.2 -- not a known variable star
07:06:48.83 -13:36:32.5 -- not a known variable star
07:06:49.56 -13:22:51.3 -- not a known variable star
07:06:49.70 -13:27:28.7 -- not a known variable star
07:06:50.67 -13:30:13.3 -- a known variable star
07:06:54.55 -13:24:15.9 -- not a known variable star
07:06:57.92 -13:31:14.6 -- not a known variable star
07:07:05.03 -13:31:34.4 -- not a known variable star
07:07:15.75 -13:41:05.7 -- not a known variable star
07:07:32.28 -13:13:35.8 -- not a known variable star
07:07:45.89 -13:28:55.8 -- not a known variable star
07:07:52.39 -13:41:14.9 -- not a known variable star
07:07:53.83 -14:04:32.8 -- not a known variable star
07:07:55.10 -12:57:33.2 -- a known variable star
07:07:59.71 -13:22:12.9 -- not a known variable star
07:08:00.75 -13:20:33.2 -- not a known variable star
07:08:05.83 -13:25:34.5 -- not a known variable star
07:08:15.62 -14:01:49.0 -- not a known variable star
07:08:21.67 -14:08:18.5 -- not a known variable star
07:08:27.43 -14:08:48.0 -- a known variable star
07:08:28.85 -14:06:43.6 -- not a known variable star
07:08:28.88 -14:00:34.6 -- a known variable star
07:08:34.04 -14:03:41.5 -- a known variable star
07:08:43.37 -13:38:04.2 -- a known variable star
07:08:48.57 -14:04:34.5 -- not a known variable star
07:08:49.57 -13:55:21.4 -- not a known variable star
07:08:50.37 -14:06:20.4 -- not a known variable star
07:08:51.43 -14:04:29.1 -- not a known variable star
07:08:51.54 -13:58:18.2 -- not a known variable star
07:08:53.33 -14:04:30.4 -- not a known variable star
07:08:54.20 -14:02:58.9 -- not a known variable star
07:08:57.25 -14:09:08.1 -- a known variable star
07:09:01.71 -14:05:04.7 -- not a known variable star
07:09:04.23 -13:49:41.3 -- not a known variable star
07:09:05.02 -14:03:20.5 -- not a known variable star
07:09:05.91 -13:53:47.2 -- not a known variable star
07:09:10.29 -13:41:36.4 -- not a known variable star
07:09:10.60 -14:02:21.1 -- a known variable star
07:09:10.94 -14:02:48.1 -- not a known variable star
07:09:10.99 -13:53:31.6 -- not a known variable star
07:09:11.21 -13:30:45.0 -- not a known variable star
07:09:11.26 -14:08:16.7 -- not a known variable star
07:09:13.88 -13:56:14.0 -- not a known variable star
07:09:15.06 -14:00:32.8 -- not a known variable star
07:09:16.09 -14:05:31.0 -- not a known variable star
07:09:18.69 -13:59:28.4 -- not a known variable star
07:09:19.63 -14:04:46.4 -- not a known variable star
07:09:20.42 -14:07:21.3 -- not a known variable star
07:09:23.71 -14:07:36.1 -- not a known variable star
07:09:25.12 -13:58:59.6 -- not a known variable star
07:09:25.25 -13:58:31.3 -- not a known variable star
07:09:26.92 -13:38:23.1 -- not a known variable star
07:09:27.09 -13:29:22.5 -- not a known variable star
07:09:27.63 -13:58:53.0 -- not a known variable star
07:09:28.31 -13:55:00.5 -- not a known variable star
07:09:29.40 -14:02:13.5 -- not a known variable star
07:09:30.48 -13:53:31.0 -- not a known variable star
07:09:32.38 -14:01:26.9 -- a known variable star
07:09:36.49 -13:42:46.5 -- not a known variable star
07:09:39.63 -14:03:02.4 -- not a known variable star
07:09:40.01 -14:00:48.2 -- not a known variable star
07:09:42.39 -13:32:26.3 -- not a known variable star
07:09:42.73 -13:36:41.8 -- a known variable star
07:09:42.94 -13:25:52.4 -- not a known variable star
07:09:44.01 -13:46:09.9 -- not a known variable star
07:09:44.76 -13:54:06.4 -- not a known variable star
07:09:45.43 -13:38:19.2 -- not a known variable star
07:09:47.45 -14:00:56.7 -- not a known variable star
07:09:49.44 -13:54:04.2 -- not a known variable star
Found 97 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
116 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 116 (excluding asteroids and hot pixels, 97 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)2461324.85603358 -observatory V36
14:37:14.94 -18:19:09.1 Mercury (0.0mag)
14:07:23.71 -20:56:21.5 Venus (-4.5mag)
08:39:50.50 +19:37:07.0 Mars (1.0mag)
09:34:20.37 +15:05:27.5 Jupiter (-1.9mag)
00:42:27.28 +01:36:58.7 Saturn (0.4mag)
04:12:05.07 +20:57:58.4 Uranus (5.6mag)
00:10:20.92 -00:25:35.6 Neptune (7.7mag)
20:24:10.86 -23:43:30.4 Pluto (14.5mag)
13:31:04.80 -14:21:10.7 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Oct 11 03:39 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461324.85603358:
09:34:15.33 +15:05:55.9 Io (6.1mag)
09:34:29.81 +15:04:35.8 Europa (6.2mag)
09:34:34.78 +15:04:08.8 Ganymede (5.6mag)
09:33:56.15 +15:07:39.2 Callisto (6.9mag)
09:34:04.79 +15:25:58.3 Himalia (15.6mag)
09:34:17.65 +15:05:42.1 Thebe (16.4mag)
09:32:55.00 +15:27:06.3 Elara (17.5mag)
09:36:46.75 +14:28:17.3 Pasiphae (17.8mag)
09:32:56.73 +15:32:31.5 Carme (18.8mag)
00:42:14.19 +01:37:11.2 Titan (8.2mag)
00:42:30.69 +01:36:52.8 Rhea (9.6mag)
00:41:56.52 +01:34:11.8 Iapetus (11.0mag)
00:42:11.54 +01:36:50.4 Hyperion (14.1mag)
00:40:46.74 +01:24:39.5 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Oct 11 03:39 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461324.85603358:
02:48:38.97 +21:21:48.2 JWST
17:07:50.77 +39:53:04.9 Chandra
12:41:59.26 -62:05:17.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Oct 11 03:39 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461324.85603358 -observatory V36
03:46:08.99 +20:11:55.3 17.1mag P/1996 R2 (Lagerkvist)
18:24:41.21 -33:29:51.8 14.7mag P/2010 H2 (Vales)
07:39:48.12 -72:24:00.1 17.2mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:52.13 +34:38:58.7 17.7mag C/2017 K2 (PANSTARRS)
07:30:10.41 +25:27:31.0 16.9mag C/2022 N2 (PANSTARRS)
09:01:55.70 +35:39:52.7 16.2mag C/2024 E1 (Wierzchos)
18:26:45.39 +41:31:37.8 17.4mag C/2024 J3 (ATLAS)
05:46:11.82 -13:35:22.6 16.6mag C/2024 T5 (ATLAS)
12:17:02.00 +15:59:49.9 16.2mag C/2025 V2 (Rankin)
13:50:57.08 -02:43:03.8 16.5mag C/2025 Y1 (ATLAS)
18:42:28.80 +65:13:56.0 15.8mag C/2026 A2 (Bok)
02:36:09.85 +43:17:36.7 17.8mag C/2026 B2 (Sun-Gao)
12:45:37.67 +14:15:27.5 17.7mag A/2026 E1
16:29:17.96 -20:39:20.0 12.9mag P/2026 R2 (Leonard)
00:27:06.06 +19:00:08.8 17.6mag 2P/Encke
22:58:14.34 -31:42:16.3 14.5mag 10P/Tempel
02:10:44.76 +38:44:40.2 16.8mag 11P/Tempel-Swift-LINEAR
12:11:12.74 -08:09:36.7 16.3mag 29P/Schwassmann-Wachmann
00:22:26.63 -08:52:12.6 15.6mag 65P/Gunn
07:35:44.69 +16:00:53.1 13.9mag 78P/Gehrels
03:00:05.88 +14:20:34.4 17.6mag 88P/Howell
07:38:50.19 +40:14:21.4 17.1mag 112P/Urata-Niijima
09:02:34.45 +14:09:31.8 17.8mag 114P/Wiseman-Skiff
11:40:57.19 +13:16:06.5 14.8mag 123P/West-Hartley
14:06:37.65 -32:12:23.5 17.8mag 124P/Mrkos
06:50:48.86 +19:18:36.5 15.6mag 128P/Shoemaker-Holt
21:39:47.06 +03:24:38.8 9.5mag 161P/Hartley-IRAS
10:18:24.59 +01:39:35.4 14.3mag 169P/NEAT
03:29:21.11 +04:36:10.2 14.8mag 220P/McNaught
06:03:26.00 +45:12:43.9 15.4mag 260P/McNaught
07:27:34.76 +25:37:07.6 17.9mag 266P/Christensen
09:56:12.47 +31:37:43.8 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 1.6K Oct 11 03:39 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:39:14.97 +51:06:11.70 ASASSN-26fk 2026-10-5.53 -3.9
02:49:03.98 -49:55:57.00 SN 2026adfy 2026-10-4.88 16.61
22:03:46.31 -11:07:57.70 AT2026adgn 2026-10-4.28 -2.56
15:03:12.98 +49:51:05.40 ASASSN-26fj 2026-10-2.06 15.91
08:07:27.96 -65:51:03.90 ASASSN-26fi 2026-10-1.36 15.82
21:02:34.66 +23:57:26.20 ASASSN-26fh 2026-10-1.27 15.94
20:00:16.62 +03:26:29.90 AT2026adfv 2026-10-1.3 16.42
00:08:42.74 -32:33:16.50 SN2026abhc 2026-09-29.15 15.57
21:02:30.26 -19:27:41.80 SN2026acxa 2026-09-29.13 14.65
04:39:17.45 -28:06:12.40 ASASSN-26fg 2026-09-23.25 15.73
05:25:07.80 +04:38:32.40 SN2026aajs 2026-09-21.32 17.04
19:56:12.67 +08:25:27.70 AT2026acgs 2026-09-18.14 15.84
00:02:34.07 +52:55:19.10 ASASSN-26ff 2026-09-16.43 15.37
23:44:33.18 +17:46:12.20 SN2026yjv 2026-09-15.38 18.32
16:21:12.24 +57:37:51.30 SN 2026aafh 2026-09-14.11 15.02
23:36:00.27 -19:28:18.00 SN 2026aaks 2026-09-14.44 16.89
16:35:24.86 -05:32:38.20 SN2026aasi 2026-09-12.99 16.58
16:46:08.71 +37:25:21.80 SN2026aafk 2026-09-13.25 17.4
23:48:37.86 +50:25:24.60 SN2026aafs 2026-09-13.47 17
21:20:27.02 +02:10:42.50 SN2026aagh -------
08:02:26.85 -24:37:44.10 ASASSN-26fe 2026-09-13.34 13.67
02:29:34.91 +23:06:56.30 SN2026aars 2026-09-12.27 16.93
02:47:25.52 -32:58:34.50 SN 2026znh 2026-09-9.92 16.26
04:59:14.53 -83:27:58.80 ASASSN-26fd 2026-09-9.11 17.27
17:52:06.79 -23:43:20.70 ASASSN-26fc 2026-09-8.79 12.14
03:52:53.26 -14:19:28.70 SN 2026zfw 2026-09-8 17.78
01:53:26.46 +10:07:25.10 SN2026aacj 2026-09-7.17 16.27
20:04:34.47 +62:38:38.10 SN2026zji 2026-09-7.14 15.87
22:37:05.59 +34:24:35.70 SN2026aaiv 2026-09-7.22 13.48
22:24:21.29 -10:25:31.60 ASASSN-26fb 2026-09-5.3 13.93
00:44:54.28 +41:33:10.50 AT2026aabo 2026-09-3.29 15.02
00:52:12.40 -58:22:08.60 SN 2026zhl 2026-08-31.92 16.51
19:53:57.87 +61:00:19.70 ASASSN-26fa 2026-08-31.18 14.63
00:21:50.96 -09:29:16.30 AT2026zwp 2026-08-31.41 15.59
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.79 -22:25:29.10 V8055 2026-08-30 10.76
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
-rw-r--r-- 1 apache apache 5.7K Oct 11 03:39 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
00:42:12.76 +41:16:28.4 PNV J00421276+4116284 2026-09-10.9176 18.67Cmag
17:52:06.80 -23:43:20.7 TCP J17520680-2343207 2026-09-08.7896 12.6mag
00:42:40.94 +41:15:37.1 PNV J00424094+4115371 2026-09-17.8925 18.3mag
08:49:20.13 -09:19:15.8 TCP J08492013-0919158 2026-09-18.4698 13.3mag
00:42:13.93 +41:16:35.6 PNV J00421393+4116356 2026-09-22.6597 19.66Cmag
18:14:01.58 +15:13:55.5 TCP J18140158+1513555 2026-09-24.4645 14.1mag
00:42:36.61 +41:13:50.5 TCP J00423661+4113505 2026-09-29.7462 17.4mag
22:03:46.29 -11:07:57.8 TCP J22034629-1107578 2026-09-29.7438 14.51Cmag
22:05:02.06 +20:49:01.2 TCP J22050206+2049012 2026-10-03.5715 17.13Cmag
00:38:15.01 +41:14:47.2 TCP J00381501+4114472 2026-10-08.5978 17.72Cmag
-rw-r--r-- 1 apache apache 191K Oct 11 03:39 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
18:28:46.287 +43:53:39.30 AT 2026acxz 2026-09-22.18 19.7418
18:50:25.837 +51:48:48.31 AT 2026acxy 2026-09-26.14 19.507
17:29:04.550 +70:58:39.69 AT 2026acxx 2026-09-18.17 19.9857
18:36:38.362 +53:14:52.16 AT 2026acxw 2026-09-22.17 19.6863
03:16:13.837 +33:07:04.16 AT 2026acxv 2026-09-24.50 20.55
05:52:14.054 +15:53:08.19 AT 2026acxu 2026-09-22.43 20.8781
08:02:21.458 +24:05:52.06 AT 2026acxt 2026-09-24.51 19.9945
08:26:53.421 +00:01:31.92 AT 2026acxs 2026-09-24.52 18.9046
08:04:09.422 +26:03:07.21 AT 2026acxr 2026-09-16.52 20.3455
09:49:29.452 +22:28:47.85 AT 2026acxq 2026-09-24.52 18.9887
10:39:38.343 +25:39:08.54 AT 2026acxp 2026-09-24.53 18.7327
10:46:46.678 +35:46:40.03 AT 2026acxo 2026-09-24.53 18.7833
07:54:42.514 -01:42:07.85 AT 2026acxn 2026-09-24.52 20.2449
08:05:13.593 +06:17:43.23 AT 2026acxm 2026-09-24.52 19.4626
08:21:28.246 +03:46:33.77 AT 2026acxl 2026-09-24.52 19.7999
04:46:32.556 +00:05:47.64 AT 2026acxk 2026-09-22.48 20.2187
03:43:52.593 +21:51:56.00 AT 2026acxj 2026-07-06.48 19.0551
07:17:54.475 +23:18:27.43 AT 2026acxi 2026-09-25.47 19.7261
05:06:29.004 +73:49:45.19 AT 2026acxh 2026-09-16.43 20.0492
02:06:05.697 -18:58:51.46 AT 2026acxg 2026-09-24.55 20.61
-rw-r--r-- 1 apache apache 89K Oct 11 03:39 tns_transients_list.txt
