This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib
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 07 16.3551 2461237.8551 12.92 12:33:33.89 +73:18:36.3
124.70706 43.75651 galactic Dra Second-epoch detections are separated by 0.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:33:33.89 +73:18:36.3 (user input) | T | P | (position from user input) J-Ks=0.479+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:33.89 +73:18:36.3: 14.17 +/- 0.07 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:33.89 +73:18:36.3: 14.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 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
target,2461237.8551,12.92,0.05,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
target 20260716.3551 12.92CV 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 07 16.3551 2461237.8551 12.86 12:27:06.38 +73:40:43.7
125.27849 43.33841 galactic Dra Second-epoch detections are separated by 2.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:27:06.38 +73:40:43.7 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:27:06.38 +73:40:43.7: 13.85 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:27:06.38 +73:40:43.7: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.86,0.05,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
target 20260716.3551 12.86CV 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 07 16.3551 2461237.8551 11.45 12:46:18.77 +72:18:08.6
123.48100 44.82040 galactic Dra Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689552138956532864 | 12:46:18.77 +72:18:08.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.517+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:18.77 +72:18:08.6: 12.46 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:18.77 +72:18:08.6: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 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 1689552138956532864,2461237.8551,11.45,0.05,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 1689552138956532864 20260716.3551 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 11.47 12:19:05.94 +66:59:08.9
127.82207 49.83427 galactic Dra Second-epoch detections are separated by 0.4" and 6.4 pix
The object was found in VSX 3" Gaia DR3 1681561270698572032
Type: ROT
# Max. Min./Amp. JD0 Period
12.030 G 12.110 G K
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:19:05.94 +66:59:08.9: 12.49 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:19:05.94 +66:59:08.9: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.50 +/- 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 1681561270698572032,2461237.8551,11.47,0.05,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 1681561270698572032 20260716.3551 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 11.59 12:41:43.81 +72:29:30.6
123.95739 44.61708 galactic Dra Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689746378853849728 | 12:41:43.90 +72:29:30.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.617+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:41:43.81 +72:29:30.6: 12.50 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:41:43.81 +72:29:30.6: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 1689746378853849728,2461237.8551,11.59,0.05,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
Gaia DR3 1689746378853849728 20260716.3551 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 07 16.3551 2461237.8551 11.58 12:47:27.01 +72:18:12.4
123.35914 44.82150 galactic Dra Second-epoch detections are separated by 0.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689643162199543424 | 12:47:27.09 +72:18:12.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.340+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:47:27.01 +72:18:12.4: 12.51 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:47:27.01 +72:18:12.4: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 1689643162199543424,2461237.8551,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689643162199543424 20260716.3551 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.19 12:16:06.82 +73:29:26.2
126.37431 43.40075 galactic Dra Second-epoch detections are separated by 1.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:16:06.82 +73:29:26.2 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.035 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:16:06.82 +73:29:26.2: 13.17 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:16:06.82 +73:29:26.2: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.19,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.42 12:49:26.91 +70:35:39.0
123.17213 46.53316 galactic Dra Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:49:26.91 +70:35:39.0 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:49:26.91 +70:35:39.0: 13.44 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:49:26.91 +70:35:39.0: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 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
target,2461237.8551,12.42,0.05,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 20260716.3551 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.60 12:35:39.48 +73:23:00.0
124.49123 43.69711 galactic Dra Second-epoch detections are separated by 2.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:39.48 +73:23:00.0 (user input) | T | P | (position from user input) J-Ks=0.271+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:39.48 +73:23:00.0: 13.65 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:39.48 +73:23:00.0: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461237.8551,12.60,0.05,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 20260716.3551 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 11.92 12:33:44.00 +73:02:32.2
124.72580 44.02425 galactic Dra Second-epoch detections are separated by 0.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:33:44.00 +73:02:32.2 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:44.00 +73:02:32.2: 12.87 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:44.00 +73:02:32.2: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,11.92,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.54 12:19:19.80 +66:59:07.5
127.78784 49.83902 galactic Dra Second-epoch detections are separated by 3.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:19:19.80 +66:59:07.5 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:19:19.80 +66:59:07.5: 13.69 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:19:19.80 +66:59:07.5: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461237.8551,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 11.96 12:46:21.75 +72:11:05.0
123.48030 44.93812 galactic Dra Second-epoch detections are separated by 0.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:46:21.75 +72:11:05.0 (user input) | T | P | (position from user input) J-Ks=0.260+/-0.030 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:21.75 +72:11:05.0: 12.89 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:21.75 +72:11:05.0: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,11.96,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.28 12:16:55.88 +73:15:12.8
126.35595 43.64455 galactic Dra Second-epoch detections are separated by 0.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:16:55.88 +73:15:12.8 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:16:55.88 +73:15:12.8: 13.24 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:16:55.88 +73:15:12.8: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.56 12:17:52.76 +73:29:22.7
126.20480 43.42471 galactic Dra Second-epoch detections are separated by 0.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:17:52.76 +73:29:22.7 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:17:52.76 +73:29:22.7: 13.48 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:17:52.76 +73:29:22.7: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 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
target,2461237.8551,12.56,0.05,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
target 20260716.3551 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.34 12:27:36.87 +73:50:18.6
125.20200 43.18459 galactic Dra Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:27:36.87 +73:50:18.6 (user input) | T | P | (position from user input) J-Ks=0.494+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:27:36.87 +73:50:18.6: 13.26 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:27:36.87 +73:50:18.6: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.45 12:34:01.41 +73:27:55.3
124.64161 43.60503 galactic Dra Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:01.41 +73:27:55.3 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.031 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:01.41 +73:27:55.3: 13.49 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:01.41 +73:27:55.3: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 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,2461237.8551,12.45,0.05,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 20260716.3551 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.59 11:18:56.84 +67:42:46.6
135.56521 47.08212 galactic UMa Second-epoch detections are separated by 2.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:18:56.84 +67:42:46.6 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:56.84 +67:42:46.6: 13.53 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:18:56.84 +67:42:46.6: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 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!
TCP 2026 07 16.3551* 11 18 56.84 +67 42 46.6 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.59,0.05,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
target 20260716.3551 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.68 12:33:36.51 +73:09:38.4
124.72260 43.90554 galactic Dra Second-epoch detections are separated by 1.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:33:36.51 +73:09:38.4 (user input) | T | P | (position from user input) J-Ks=0.503+/-0.027 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:36.51 +73:09:38.4: 13.90 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:36.51 +73:09:38.4: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461237.8551,12.68,0.05,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
target 20260716.3551 12.68CV 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 07 16.3551 2461237.8551 11.64 12:42:16.37 +72:34:53.7
123.89383 44.52955 galactic Dra Second-epoch detections are separated by 0.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689840765055334016 | 12:42:16.47 +72:34:53.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.644+/-0.027 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:16.37 +72:34:53.7: 12.61 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:42:16.37 +72:34:53.7: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689840765055334016,2461237.8551,11.64,0.05,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
Gaia DR3 1689840765055334016 20260716.3551 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 07 16.3551 2461237.8551 12.80 12:48:46.53 +71:40:17.1
123.23030 45.45529 galactic Dra Second-epoch detections are separated by 1.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:48:46.53 +71:40:17.1 (user input) | T | P | (position from user input) J-Ks=0.475+/-0.037 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:48:46.53 +71:40:17.1: 13.90 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:48:46.53 +71:40:17.1: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461237.8551,12.80,0.05,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
target 20260716.3551 12.80CV 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 07 16.3551 2461237.8551 12.81 12:12:36.11 +73:30:32.6
126.70558 43.33349 galactic Dra Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:12:36.11 +73:30:32.6 (user input) | T | P | (position from user input) J-Ks=0.342+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:12:36.11 +73:30:32.6: 13.76 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:12:36.11 +73:30:32.6: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461237.8551,12.81,0.05,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
target 20260716.3551 12.81CV 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 07 16.3551 2461237.8551 12.63 12:13:08.91 +73:46:38.1
126.57865 43.07883 galactic Dra Second-epoch detections are separated by 1.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:13:08.91 +73:46:38.1 (user input) | T | P | (position from user input) J-Ks=0.641+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:08.91 +73:46:38.1: 13.55 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:08.91 +73:46:38.1: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 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,2461237.8551,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 11.96 12:43:22.18 +72:26:24.5
123.78755 44.67471 galactic Dra Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:43:22.18 +72:26:24.5 (user input) | T | P | (position from user input) J-Ks=0.485+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:43:22.18 +72:26:24.5: 13.02 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:43:22.18 +72:26:24.5: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,11.96,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.13 11:19:12.07 +68:16:09.6
135.12010 46.61579 galactic UMa Second-epoch detections are separated by 1.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:19:12.07 +68:16:09.6 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:19:12.07 +68:16:09.6: 13.04 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:19:12.07 +68:16:09.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3551* 11 19 12.07 +68 16 09.6 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.79 12:33:21.13 +73:47:19.0
124.66425 43.27875 galactic Dra Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:33:21.13 +73:47:19.0 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:21.13 +73:47:19.0: 13.76 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:21.13 +73:47:19.0: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 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,2461237.8551,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.57 12:41:14.90 +72:17:54.1
124.02337 44.80829 galactic Dra Second-epoch detections are separated by 0.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:41:14.90 +72:17:54.1 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:41:14.90 +72:17:54.1: 13.77 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:41:14.90 +72:17:54.1: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 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
target,2461237.8551,12.57,0.05,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
target 20260716.3551 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.10 12:42:11.36 +72:31:43.3
123.90632 44.58205 galactic Dra Second-epoch detections are separated by 0.7" and 6.1 pix
The object was found in VSX 0" Gaia DR3 1689746722450759296
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.940 G 12.970 G F
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:11.36 +72:31:43.3: 13.11 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:42:11.36 +72:31:43.3: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689746722450759296,2461237.8551,12.10,0.05,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
Gaia DR3 1689746722450759296 20260716.3551 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.66 12:26:32.48 +72:25:57.6
125.56462 44.56810 galactic Dra Second-epoch detections are separated by 1.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:26:32.48 +72:25:57.6 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:26:32.48 +72:25:57.6: 13.58 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:26:32.48 +72:25:57.6: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.66,0.05,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
target 20260716.3551 12.66CV 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 07 16.3551 2461237.8551 12.63 12:34:01.16 +73:14:03.4
124.67191 43.83508 galactic Dra Second-epoch detections are separated by 2.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:01.16 +73:14:03.4 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:01.16 +73:14:03.4: 13.82 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:01.16 +73:14:03.4: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 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
target,2461237.8551,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.74 12:19:37.07 +66:59:37.8
127.74253 49.83615 galactic Dra Second-epoch detections are separated by 1.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:19:37.07 +66:59:37.8 (user input) | T | P | (position from user input) J-Ks=0.519+/-0.033 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:19:37.07 +66:59:37.8: 13.93 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:19:37.07 +66:59:37.8: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461237.8551,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.77 12:31:07.67 +73:44:08.9
124.88420 43.31537 galactic Dra Second-epoch detections are separated by 3.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:31:07.67 +73:44:08.9 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.035 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:31:07.67 +73:44:08.9: 13.98 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:31:07.67 +73:44:08.9: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461237.8551,12.77,0.05,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
target 20260716.3551 12.77CV 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 07 16.3551 2461237.8551 12.71 12:35:39.02 +72:53:08.0
124.55080 44.19304 galactic Dra Second-epoch detections are separated by 2.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:39.02 +72:53:08.0 (user input) | T | P | (position from user input) J-Ks=0.277+/-0.031 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:39.02 +72:53:08.0: 13.62 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:39.02 +72:53:08.0: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461237.8551,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 11.71 12:44:17.97 +72:28:44.4
123.68688 44.63879 galactic Dra Second-epoch detections are separated by 0.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:44:17.97 +72:28:44.4 (user input) | T | P | (position from user input) J-Ks=0.511+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:44:17.97 +72:28:44.4: 12.75 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:44:17.97 +72:28:44.4: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 11.77 12:34:54.20 +73:05:44.5
124.60103 43.97893 galactic Dra Second-epoch detections are separated by 0.4" and 6.1 pix
The object was found in VSX 1" Gaia DR3 1689925805407391232
Type: ROT
# Max. Min./Amp. JD0 Period
12.620 G 12.650 G G
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:54.20 +73:05:44.5: 12.81 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:54.20 +73:05:44.5: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 1689925805407391232,2461237.8551,11.77,0.05,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 1689925805407391232 20260716.3551 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 07 16.3551 2461237.8551 12.55 12:51:58.10 +71:26:32.8
122.87151 45.68574 galactic Dra Second-epoch detections are separated by 2.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:51:58.10 +71:26:32.8 (user input) | T | P | (position from user input) J-Ks=0.494+/-0.039 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:51:58.10 +71:26:32.8: 13.66 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:51:58.10 +71:26:32.8: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.55,0.05,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 20260716.3551 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.66 11:16:20.83 +68:23:25.9
135.35800 46.37646 galactic UMa Second-epoch detections are separated by 2.5" and 5.5 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 | 11:16:20.83 +68:23:25.9 (user input) | T | P | (position from user input) J-Ks=0.491+/-0.033 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:20.83 +68:23:25.9: 13.64 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:16:20.83 +68:23:25.9: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 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!
TCP 2026 07 16.3551* 11 16 20.83 +68 23 25.9 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.66,0.05,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
target 20260716.3551 12.66CV 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 07 16.3551 2461237.8551 12.90 12:13:53.60 +73:46:37.5
126.50892 43.08943 galactic Dra Second-epoch detections are separated by 0.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:13:53.60 +73:46:37.5 (user input) | T | P | (position from user input) J-Ks=0.354+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:53.60 +73:46:37.5: 14.00 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:53.60 +73:46:37.5: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461237.8551,12.90,0.05,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
target 20260716.3551 12.90CV 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 07 16.3551 2461237.8551 12.79 12:29:31.29 +73:18:12.5
125.10765 43.73207 galactic Dra Second-epoch detections are separated by 1.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:29:31.29 +73:18:12.5 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:29:31.29 +73:18:12.5: 14.29 +/- 0.07 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:29:31.29 +73:18:12.5: 14.24 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 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
target,2461237.8551,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.58 12:23:16.64 +74:08:08.4
125.55121 42.84907 galactic Dra Second-epoch detections are separated by 1.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:23:16.64 +74:08:08.4 (user input) | T | P | (position from user input) J-Ks=0.589+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:23:16.64 +74:08:08.4: 13.62 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:23:16.64 +74:08:08.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 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,2461237.8551,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.57 12:46:30.27 +72:08:14.3
123.46677 44.98582 galactic Dra Second-epoch detections are separated by 0.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:46:30.27 +72:08:14.3 (user input) | T | P | (position from user input) J-Ks=0.525+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:30.27 +72:08:14.3: 13.61 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:30.27 +72:08:14.3: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.57,0.05,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
target 20260716.3551 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.71 12:20:46.73 +73:34:16.1
125.90693 43.37957 galactic Dra Second-epoch detections are separated by 1.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:20:46.73 +73:34:16.1 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:20:46.73 +73:34:16.1: 13.62 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:20:46.73 +73:34:16.1: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 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,2461237.8551,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.55 12:18:11.97 +67:18:27.9
127.85686 49.50145 galactic Dra Second-epoch detections are separated by 2.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:18:11.97 +67:18:27.9 (user input) | T | P | (position from user input) J-Ks=0.545+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:18:11.97 +67:18:27.9: 13.61 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:18:11.97 +67:18:27.9: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.55,0.05,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 20260716.3551 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.96 12:29:42.57 +73:46:19.6
125.01405 43.26819 galactic Dra Second-epoch detections are separated by 2.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:29:42.57 +73:46:19.6 (user input) | T | P | (position from user input) J-Ks=0.715+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:29:42.57 +73:46:19.6: 14.25 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:29:42.57 +73:46:19.6: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 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
target,2461237.8551,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.62 12:34:53.81 +73:27:17.3
124.55744 43.62120 galactic Dra Second-epoch detections are separated by 0.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:53.81 +73:27:17.3 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:53.81 +73:27:17.3: 13.84 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:53.81 +73:27:17.3: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461237.8551,12.62,0.05,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
target 20260716.3551 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.82 12:46:33.76 +72:02:26.0
123.46413 45.08266 galactic Dra Second-epoch detections are separated by 0.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:46:33.76 +72:02:26.0 (user input) | T | P | (position from user input) J-Ks=0.494+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:33.76 +72:02:26.0: 13.83 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:33.76 +72:02:26.0: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 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
target,2461237.8551,12.82,0.05,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
target 20260716.3551 12.82CV 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 07 16.3551 2461237.8551 12.70 12:15:36.06 +67:06:22.6
128.30065 49.64674 galactic Dra Second-epoch detections are separated by 2.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:15:36.06 +67:06:22.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:15:36.06 +67:06:22.6: 13.82 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:15:36.06 +67:06:22.6: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 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
target,2461237.8551,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 13.15 12:35:42.19 +73:05:12.4
124.52159 43.99287 galactic Dra Second-epoch detections are separated by 1.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:42.19 +73:05:12.4 (user input) | T | P | (position from user input) J-Ks=0.314+/-0.039 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:42.19 +73:05:12.4: 14.43 +/- 0.08 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:42.19 +73:05:12.4: 14.65 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.75 12:34:31.80 +73:48:33.1
124.54927 43.26592 galactic Dra Second-epoch detections are separated by 2.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:31.80 +73:48:33.1 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:31.80 +73:48:33.1: 13.59 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:31.80 +73:48:33.1: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461237.8551,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.65 12:35:08.19 +72:20:07.5
124.67164 44.73773 galactic Dra Second-epoch detections are separated by 2.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:08.19 +72:20:07.5 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:08.19 +72:20:07.5: 13.73 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:08.19 +72:20:07.5: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461237.8551,12.65,0.05,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
target 20260716.3551 12.65CV 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 07 16.3551 2461237.8551 12.81 12:44:46.35 +72:39:08.9
123.62804 44.46677 galactic Dra Second-epoch detections are separated by 1.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:44:46.35 +72:39:08.9 (user input) | T | P | (position from user input) J-Ks=0.401+/-0.027 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:44:46.35 +72:39:08.9: 13.80 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:44:46.35 +72:39:08.9: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461237.8551,12.81,0.05,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
target 20260716.3551 12.81CV 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 07 16.3551 2461237.8551 12.39 12:45:12.32 +72:31:52.1
123.58864 44.58916 galactic Dra Second-epoch detections are separated by 1.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:45:12.32 +72:31:52.1 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:45:12.32 +72:31:52.1: 13.56 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:45:12.32 +72:31:52.1: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 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,2461237.8551,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.86 12:47:27.35 +70:51:39.9
123.40401 46.26352 galactic Dra Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:47:27.35 +70:51:39.9 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.037 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:47:27.35 +70:51:39.9: 13.93 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:47:27.35 +70:51:39.9: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461237.8551,12.86,0.05,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
target 20260716.3551 12.86CV 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 07 16.3551 2461237.8551 12.32 12:13:16.90 +73:28:57.8
126.64799 43.36914 galactic Dra Second-epoch detections are separated by 1.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:13:16.90 +73:28:57.8 (user input) | T | P | (position from user input) J-Ks=0.871+/-0.030 (M)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:16.90 +73:28:57.8: 13.41 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:16.90 +73:28:57.8: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.32,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.43 12:34:31.30 +73:02:42.5
124.64584 44.02677 galactic Dra Second-epoch detections are separated by 1.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:31.30 +73:02:42.5 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.027 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:31.30 +73:02:42.5: 13.41 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:31.30 +73:02:42.5: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.48 11:17:48.09 +68:56:05.5
134.78978 45.97772 galactic UMa Second-epoch detections are separated by 1.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:17:48.09 +68:56:05.5 (user input) | T | P | (position from user input) J-Ks=0.589+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:48.09 +68:56:05.5: 13.41 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:17:48.09 +68:56:05.5: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3551* 11 17 48.09 +68 56 05.5 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.48,0.05,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 20260716.3551 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.16 12:27:31.36 +66:35:33.8
126.65103 50.36248 galactic Dra Second-epoch detections are separated by 2.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:27:31.36 +66:35:33.8 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:27:31.36 +66:35:33.8: 13.12 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:27:31.36 +66:35:33.8: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.16,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.21 12:35:23.75 +73:36:45.5
124.48985 43.46705 galactic Dra Second-epoch detections are separated by 1.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:23.75 +73:36:45.5 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.027 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:23.75 +73:36:45.5: 13.11 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:23.75 +73:36:45.5: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.21,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.62 12:47:24.17 +72:23:50.4
123.36129 44.72755 galactic Dra Second-epoch detections are separated by 0.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:47:24.17 +72:23:50.4 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.033 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:47:24.17 +72:23:50.4: 13.77 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:47:24.17 +72:23:50.4: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 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
target,2461237.8551,12.62,0.05,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
target 20260716.3551 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.72 12:37:37.46 +72:09:48.0
124.42517 44.92485 galactic Dra Second-epoch detections are separated by 1.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:37:37.46 +72:09:48.0 (user input) | T | P | (position from user input) J-Ks=0.469+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:37:37.46 +72:09:48.0: 13.76 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:37:37.46 +72:09:48.0: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 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
target,2461237.8551,12.72,0.05,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
target 20260716.3551 12.72CV 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 07 16.3551 2461237.8551 12.58 12:41:44.17 +72:16:41.2
123.97270 44.83053 galactic Dra Second-epoch detections are separated by 1.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:41:44.17 +72:16:41.2 (user input) | T | P | (position from user input) J-Ks=0.482+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:41:44.17 +72:16:41.2: 13.76 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:41:44.17 +72:16:41.2: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 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
target,2461237.8551,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.77 11:14:11.70 +68:44:55.5
135.32902 45.96834 galactic UMa Second-epoch detections are separated by 2.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:14:11.70 +68:44:55.5 (user input) | T | P | (position from user input) J-Ks=0.381+/-0.033 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:14:11.70 +68:44:55.5: 13.77 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:14:11.70 +68:44:55.5: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 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!
TCP 2026 07 16.3551* 11 14 11.70 +68 44 55.5 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.77,0.05,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
target 20260716.3551 12.77CV 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 07 16.3551 2461237.8551 12.14 11:36:43.94 +66:56:50.4
133.85456 48.56605 galactic Dra Second-epoch detections are separated by 1.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:36:43.94 +66:56:50.4 (user input) | T | P | (position from user input) J-Ks=0.436+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:36:43.94 +66:56:50.4: 13.07 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:36:43.94 +66:56:50.4: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.14,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.65 12:18:16.53 +73:09:08.8
126.24917 43.76157 galactic Dra Second-epoch detections are separated by 1.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:18:16.53 +73:09:08.8 (user input) | T | P | (position from user input) J-Ks=0.342+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:18:16.53 +73:09:08.8: 13.74 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:18:16.53 +73:09:08.8: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 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
target,2461237.8551,12.65,0.05,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
target 20260716.3551 12.65CV 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 07 16.3551 2461237.8551 12.10 12:13:18.15 +73:27:38.0
126.65218 43.39115 galactic Dra Second-epoch detections are separated by 1.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:13:18.15 +73:27:38.0 (user input) | T | P | (position from user input) J-Ks=0.305+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:18.15 +73:27:38.0: 13.06 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:18.15 +73:27:38.0: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.10,0.05,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
target 20260716.3551 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.44 12:41:13.20 +72:36:46.7
124.00175 44.49405 galactic Dra Second-epoch detections are separated by 1.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:41:13.20 +72:36:46.7 (user input) | T | P | (position from user input) J-Ks=0.411+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:41:13.20 +72:36:46.7: 13.58 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:41:13.20 +72:36:46.7: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.64 12:22:43.80 +74:08:25.3
125.60068 42.83881 galactic Dra Second-epoch detections are separated by 2.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:22:43.80 +74:08:25.3 (user input) | T | P | (position from user input) J-Ks=0.691+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:22:43.80 +74:08:25.3: 13.54 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:22:43.80 +74:08:25.3: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.64,0.05,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
target 20260716.3551 12.64CV 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 07 16.3551 2461237.8551 12.00 11:16:27.10 +68:34:43.3
135.20480 46.22059 galactic UMa Second-epoch detections are separated by 0.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:16:27.10 +68:34:43.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:27.10 +68:34:43.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:16:27.10 +68:34:43.3: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 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!
TCP 2026 07 16.3551* 11 16 27.10 +68 34 43.3 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.00,0.05,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 20260716.3551 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 11.97 12:43:19.37 +72:16:40.0
123.80266 44.83675 galactic Dra Second-epoch detections are separated by 0.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:43:19.37 +72:16:40.0 (user input) | T | P | (position from user input) J-Ks=0.373+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:43:19.37 +72:16:40.0: 13.01 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:43:19.37 +72:16:40.0: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,11.97,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.80 12:13:24.55 +73:43:06.7
126.57044 43.14003 galactic Dra Second-epoch detections are separated by 2.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:13:24.55 +73:43:06.7 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.032 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:24.55 +73:43:06.7: 13.92 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:24.55 +73:43:06.7: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 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,2461237.8551,12.80,0.05,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
target 20260716.3551 12.80CV 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 07 16.3551 2461237.8551 12.79 12:34:18.61 +73:40:29.7
124.58709 43.39825 galactic Dra Second-epoch detections are separated by 1.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:18.61 +73:40:29.7 (user input) | T | P | (position from user input) J-Ks=0.399+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:18.61 +73:40:29.7: 13.94 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:18.61 +73:40:29.7: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 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
target,2461237.8551,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.37 12:15:44.91 +73:30:29.8
126.40476 43.37850 galactic Dra Second-epoch detections are separated by 1.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:15:44.91 +73:30:29.8 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.037 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:15:44.91 +73:30:29.8: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:15:44.91 +73:30:29.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.37,0.05,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
target 20260716.3551 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.23 12:45:10.51 +72:24:24.9
123.59778 44.71324 galactic Dra Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:45:10.51 +72:24:24.9 (user input) | T | P | (position from user input) J-Ks=0.435+/-0.026 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:45:10.51 +72:24:24.9: 13.37 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:45:10.51 +72:24:24.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.23,0.05,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 20260716.3551 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.33 12:25:22.18 +74:06:25.1
125.36355 42.89798 galactic Dra Second-epoch detections are separated by 1.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:25:22.18 +74:06:25.1 (user input) | T | P | (position from user input) J-Ks=0.591+/-0.027 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:25:22.18 +74:06:25.1: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:25:22.18 +74:06:25.1: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.60 11:24:38.33 +67:31:06.8
135.01680 47.52152 galactic UMa Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:24:38.33 +67:31:06.8 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:24:38.33 +67:31:06.8: 13.56 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:24:38.33 +67:31:06.8: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 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!
TCP 2026 07 16.3551* 11 24 38.33 +67 31 06.8 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.60,0.05,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 20260716.3551 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.57 11:17:30.19 +68:06:10.0
135.44172 46.67804 galactic UMa Second-epoch detections are separated by 1.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:17:30.19 +68:06:10.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:30.19 +68:06:10.0: 13.57 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:17:30.19 +68:06:10.0: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 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!
TCP 2026 07 16.3551* 11 17 30.19 +68 06 10.0 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.57,0.05,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
target 20260716.3551 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.62 12:31:20.66 +73:03:17.8
124.96486 43.99390 galactic Dra Second-epoch detections are separated by 1.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:31:20.66 +73:03:17.8 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:31:20.66 +73:03:17.8: 13.56 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:31:20.66 +73:03:17.8: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 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,2461237.8551,12.62,0.05,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
target 20260716.3551 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.43 12:13:55.09 +73:35:56.1
126.55519 43.26439 galactic Dra Second-epoch detections are separated by 0.5" and 6.0 pix
The object was found in VSX 1" Gaia DR3 1690859771815327616
Type: ROT
# Max. Min./Amp. JD0 Period
13.040 G 13.070 G K
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:55.09 +73:35:56.1: 13.35 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:55.09 +73:35:56.1: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1690859771815327616,2461237.8551,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1690859771815327616 20260716.3551 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.57 11:38:53.39 +68:47:24.9
132.43271 46.97713 galactic Dra Second-epoch detections are separated by 1.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:38:53.39 +68:47:24.9 (user input) | T | P | (position from user input) J-Ks=0.379+/-0.034 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:38:53.39 +68:47:24.9: 13.54 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:38:53.39 +68:47:24.9: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 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
target,2461237.8551,12.57,0.05,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
target 20260716.3551 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.97 12:46:35.90 +70:57:52.2
123.50159 46.15840 galactic Dra Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:46:35.90 +70:57:52.2 (user input) | T | P | (position from user input) J-Ks=0.322+/-0.038 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:35.90 +70:57:52.2: 14.11 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:35.90 +70:57:52.2: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 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
target,2461237.8551,12.97,0.05,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
target 20260716.3551 12.97CV 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 07 16.3551 2461237.8551 12.36 12:27:08.47 +73:54:09.9
125.23543 43.11666 galactic Dra Second-epoch detections are separated by 0.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:27:08.47 +73:54:09.9 (user input) | T | P | (position from user input) J-Ks=0.544+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:27:08.47 +73:54:09.9: 13.36 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:27:08.47 +73:54:09.9: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 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
target,2461237.8551,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.37 11:41:38.30 +65:51:58.4
133.87141 49.75329 galactic Dra Second-epoch detections are separated by 1.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:41:38.30 +65:51:58.4 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:41:38.30 +65:51:58.4: 13.35 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:41:38.30 +65:51:58.4: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.37,0.05,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
target 20260716.3551 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.62 12:06:29.03 +74:13:10.6
127.05745 42.54664 galactic Dra Second-epoch detections are separated by 0.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:06:29.03 +74:13:10.6 (user input) | T | P | (position from user input) J-Ks=0.243+/-0.035 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:06:29.03 +74:13:10.6: 13.52 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:06:29.03 +74:13:10.6: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 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
target,2461237.8551,12.62,0.05,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
target 20260716.3551 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.76 12:48:12.83 +72:07:10.9
123.28193 45.00637 galactic Dra Second-epoch detections are separated by 1.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:48:12.83 +72:07:10.9 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:48:12.83 +72:07:10.9: 13.89 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:48:12.83 +72:07:10.9: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461237.8551,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.39 11:25:07.12 +68:30:23.3
134.25920 46.67769 galactic UMa Second-epoch detections are separated by 2.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:25:07.12 +68:30:23.3 (user input) | T | P | (position from user input) J-Ks=0.654+/-0.032 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:25:07.12 +68:30:23.3: 13.31 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:25:07.12 +68:30:23.3: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 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!
TCP 2026 07 16.3551* 11 25 07.12 +68 30 23.3 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.10 12:44:29.56 +72:26:09.8
123.66875 44.68226 galactic Dra Second-epoch detections are separated by 0.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:44:29.56 +72:26:09.8 (user input) | T | P | (position from user input) J-Ks=0.648+/-0.024 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:44:29.56 +72:26:09.8: 13.31 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:44:29.56 +72:26:09.8: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.10,0.05,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
target 20260716.3551 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.76 12:09:04.15 +67:40:37.2
129.03438 48.94618 galactic Dra Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:09:04.15 +67:40:37.2 (user input) | T | P | (position from user input) J-Ks=0.595+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:09:04.15 +67:40:37.2: 13.74 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:09:04.15 +67:40:37.2: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 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,2461237.8551,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.71 12:24:20.30 +73:48:45.9
125.51679 43.17923 galactic Dra Second-epoch detections are separated by 0.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:24:20.30 +73:48:45.9 (user input) | T | P | (position from user input) J-Ks=0.441+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:24:20.30 +73:48:45.9: 13.72 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:24:20.30 +73:48:45.9: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 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
target,2461237.8551,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.78 12:36:36.44 +72:03:34.6
124.54674 45.02211 galactic Dra Second-epoch detections are separated by 2.4" and 6.5 pix
The object was found in VSX 1" Gaia DR3 1689764795673206528
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.590 G 13.620 G F
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:36.44 +72:03:34.6: 13.73 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:36:36.44 +72:03:34.6: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689764795673206528,2461237.8551,12.78,0.05,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 1689764795673206528 20260716.3551 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.84 12:30:10.75 +73:50:40.8
124.95801 43.19985 galactic Dra Second-epoch detections are separated by 1.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:30:10.75 +73:50:40.8 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:30:10.75 +73:50:40.8: 13.90 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:30:10.75 +73:50:40.8: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461237.8551,12.84,0.05,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 20260716.3551 12.84CV 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 07 16.3551 2461237.8551 12.55 12:29:53.29 +73:53:18.5
124.97871 43.15403 galactic Dra Second-epoch detections are separated by 0.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:29:53.29 +73:53:18.5 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:29:53.29 +73:53:18.5: 13.49 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:29:53.29 +73:53:18.5: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.55,0.05,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 20260716.3551 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.32 12:23:57.52 +66:48:25.8
127.14306 50.09580 galactic Dra Second-epoch detections are separated by 1.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:23:57.52 +66:48:25.8 (user input) | T | P | (position from user input) J-Ks=0.282+/-0.032 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:23:57.52 +66:48:25.8: 13.30 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:23:57.52 +66:48:25.8: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.32,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.43 11:35:08.28 +66:53:29.5
134.10381 48.54833 galactic Dra Second-epoch detections are separated by 2.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:35:08.28 +66:53:29.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:35:08.28 +66:53:29.5: 13.30 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:35:08.28 +66:53:29.5: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.28 12:14:18.44 +73:33:43.3
126.52820 43.30599 galactic Dra Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:14:18.44 +73:33:43.3 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:14:18.44 +73:33:43.3: 13.28 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:14:18.44 +73:33:43.3: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.99 12:36:28.95 +72:36:52.9
124.49643 44.46810 galactic Dra Second-epoch detections are separated by 3.1" 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 | target | 12:36:28.95 +72:36:52.9 (user input) | T | P | (position from user input) J-Ks=0.486+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:28.95 +72:36:52.9: 14.08 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:36:28.95 +72:36:52.9: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 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
target,2461237.8551,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.99CV 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 07 16.3551 2461237.8551 12.45 12:14:15.87 +73:28:53.5
126.55416 43.38431 galactic Dra Second-epoch detections are separated by 1.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:14:15.87 +73:28:53.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:14:15.87 +73:28:53.5: 13.52 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:14:15.87 +73:28:53.5: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.45,0.05,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 20260716.3551 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.26 12:19:49.21 +67:01:52.8
127.70141 49.80310 galactic Dra Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:19:49.21 +67:01:52.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:19:49.21 +67:01:52.8: 13.26 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:19:49.21 +67:01:52.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 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 07 16.3551 2461237.8551 12.21 12:14:00.83 +67:09:28.6
128.51541 49.56262 galactic Dra Second-epoch detections are separated by 1.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:14:00.83 +67:09:28.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:14:00.83 +67:09:28.6: 13.27 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:14:00.83 +67:09:28.6: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.21,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.26 12:28:29.70 +66:28:10.3
126.52819 50.49822 galactic Dra Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:29.70 +66:28:10.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:28:29.70 +66:28:10.3: 13.25 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:28:29.70 +66:28:10.3: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 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 07 16.3551 2461237.8551 12.31 12:28:50.72 +73:52:20.0
125.07987 43.16168 galactic Dra Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:28:50.72 +73:52:20.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:28:50.72 +73:52:20.0: 13.24 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:28:50.72 +73:52:20.0: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.35 12:36:32.73 +72:11:36.1
124.53802 44.88842 galactic Dra Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:36:32.73 +72:11:36.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:32.73 +72:11:36.1: 13.22 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:36:32.73 +72:11:36.1: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 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
target,2461237.8551,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 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 07 16.3551 2461237.8551 12.30 11:19:42.04 +68:26:58.3
134.92986 46.48361 galactic UMa Second-epoch detections are separated by 1.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:19:42.04 +68:26:58.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:19:42.04 +68:26:58.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:19:42.04 +68:26:58.3: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3551* 11 19 42.04 +68 26 58.3 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.30,0.05,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 20260716.3551 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.36 11:26:20.46 +67:56:17.4
134.50974 47.23138 galactic UMa Second-epoch detections are separated by 1.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:26:20.46 +67:56:17.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:20.46 +67:56:17.4: 13.23 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:26:20.46 +67:56:17.4: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3551* 11 26 20.46 +67 56 17.4 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.66 12:34:57.46 +72:58:46.6
124.60993 44.09491 galactic Dra Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:34:57.46 +72:58:46.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:57.46 +72:58:46.6: 13.68 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:57.46 +72:58:46.6: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 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
target,2461237.8551,12.66,0.05,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
target 20260716.3551 12.66CV 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 07 16.3551 2461237.8551 12.15 12:44:51.41 +72:33:23.2
123.62407 44.56296 galactic Dra Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:44:51.41 +72:33:23.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:44:51.41 +72:33:23.2: 13.20 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:44:51.41 +72:33:23.2: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.74 12:35:31.36 +73:12:26.5
124.52541 43.87161 galactic Dra Second-epoch detections are separated by 1.4" and 5.8 pix
The object was found in VSX 4" Gaia DR3 1689920754525857536
Type: ROT
# Max. Min./Amp. JD0 Period
13.500 G 13.520 G M
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:31.36 +73:12:26.5: 14.06 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:31.36 +73:12:26.5: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 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 1689920754525857536,2461237.8551,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689920754525857536 20260716.3551 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.37 12:46:29.17 +72:13:40.8
123.46528 44.89512 galactic Dra Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:46:29.17 +72:13:40.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:29.17 +72:13:40.8: 13.46 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:29.17 +72:13:40.8: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.37,0.05,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
target 20260716.3551 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.47 11:25:52.19 +68:27:05.9
134.20883 46.75868 galactic UMa Second-epoch detections are separated by 1.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:25:52.19 +68:27:05.9 (user input) | T | P | (position from user input) J-Ks=0.532+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:25:52.19 +68:27:05.9: 13.48 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:25:52.19 +68:27:05.9: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 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!
TCP 2026 07 16.3551* 11 25 52.19 +68 27 05.9 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8551,12.47,0.05,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 20260716.3551 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.54 12:33:29.33 +72:54:00.9
124.76965 44.16390 galactic Dra Second-epoch detections are separated by 0.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:33:29.33 +72:54:00.9 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:29.33 +72:54:00.9: 13.45 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:29.33 +72:54:00.9: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 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
target,2461237.8551,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.43 12:17:16.47 +67:04:49.4
128.06294 49.70612 galactic Dra Second-epoch detections are separated by 1.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:17:16.47 +67:04:49.4 (user input) | T | P | (position from user input) J-Ks=0.596+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:17:16.47 +67:04:49.4: 13.45 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:17:16.47 +67:04:49.4: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 11.86 12:42:25.55 +72:31:09.5
123.88208 44.59232 galactic Dra Second-epoch detections are separated by 0.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:42:25.55 +72:31:09.5 (user input) | T | P | (position from user input) J-Ks=0.390+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:25.55 +72:31:09.5: 12.89 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:42:25.55 +72:31:09.5: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,11.86,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.85 12:41:05.79 +72:22:30.0
124.03351 44.73113 galactic Dra Second-epoch detections are separated by 1.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:41:05.79 +72:22:30.0 (user input) | T | P | (position from user input) J-Ks=0.382+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:41:05.79 +72:22:30.0: 14.06 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:41:05.79 +72:22:30.0: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 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
target,2461237.8551,12.85,0.05,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
target 20260716.3551 12.85CV 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 07 16.3551 2461237.8551 12.71 12:18:46.30 +67:14:30.9
127.79331 49.57686 galactic Dra Second-epoch detections are separated by 0.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:18:46.30 +67:14:30.9 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.033 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:18:46.30 +67:14:30.9: 13.68 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:18:46.30 +67:14:30.9: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461237.8551,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.73 11:36:31.39 +68:52:57.6
132.66187 46.80496 galactic Dra Second-epoch detections are separated by 0.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:36:31.39 +68:52:57.6 (user input) | T | P | (position from user input) J-Ks=0.766+/-0.032 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:36:31.39 +68:52:57.6: 13.70 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:36:31.39 +68:52:57.6: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 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
target,2461237.8551,12.73,0.05,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
target 20260716.3551 12.73CV 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 07 16.3551 2461237.8551 12.58 12:33:52.74 +73:43:29.5
124.62218 43.34572 galactic Dra Second-epoch detections are separated by 2.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:33:52.74 +73:43:29.5 (user input) | T | P | (position from user input) J-Ks=0.381+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:52.74 +73:43:29.5: 13.67 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:52.74 +73:43:29.5: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.30 12:36:58.03 +72:09:33.1
124.49649 44.92507 galactic Dra Second-epoch detections are separated by 0.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:36:58.03 +72:09:33.1 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:58.03 +72:09:33.1: 13.18 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:36:58.03 +72:09:33.1: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.30,0.05,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 20260716.3551 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 13.01 12:40:30.91 +72:25:31.6
124.09111 44.67821 galactic Dra Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:40:30.91 +72:25:31.6 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.036 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:40:30.91 +72:25:31.6: 14.37 +/- 0.08 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:40:30.91 +72:25:31.6: 14.38 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,13.01,0.05,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 20260716.3551 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.51 12:42:16.11 +72:21:54.1
123.90951 44.74581 galactic Dra Second-epoch detections are separated by 0.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:42:16.11 +72:21:54.1 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.031 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:16.11 +72:21:54.1: 13.67 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:42:16.11 +72:21:54.1: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461237.8551,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.63 12:24:22.55 +74:07:00.6
125.45358 42.87866 galactic Dra Second-epoch detections are separated by 1.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:24:22.55 +74:07:00.6 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:24:22.55 +74:07:00.6: 13.66 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:24:22.55 +74:07:00.6: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461237.8551,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.63 12:24:12.62 +74:10:38.4
125.45700 42.81717 galactic Dra Second-epoch detections are separated by 0.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:24:12.62 +74:10:38.4 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:24:12.62 +74:10:38.4: 13.67 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:24:12.62 +74:10:38.4: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461237.8551,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.29 12:32:07.92 +73:42:35.2
124.79179 43.34869 galactic Dra Second-epoch detections are separated by 0.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:07.92 +73:42:35.2 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:32:07.92 +73:42:35.2: 13.16 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:32:07.92 +73:42:35.2: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.29,0.05,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
target 20260716.3551 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 07 16.3551 2461237.8551 12.54 12:40:37.33 +72:07:08.2
124.10536 44.98466 galactic Dra Second-epoch detections are separated by 1.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:40:37.33 +72:07:08.2 (user input) | T | P | (position from user input) J-Ks=0.486+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:40:37.33 +72:07:08.2: 13.48 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:40:37.33 +72:07:08.2: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.45 12:25:40.11 +74:05:57.6
125.33731 42.90835 galactic Dra Second-epoch detections are separated by 0.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:25:40.11 +74:05:57.6 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:25:40.11 +74:05:57.6: 13.43 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:25:40.11 +74:05:57.6: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 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
target,2461237.8551,12.45,0.05,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 20260716.3551 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.72 12:46:38.71 +72:25:37.5
123.44080 44.69643 galactic Dra Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:46:38.71 +72:25:37.5 (user input) | T | P | (position from user input) J-Ks=0.661+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:38.71 +72:25:37.5: 13.86 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:38.71 +72:25:37.5: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 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
target,2461237.8551,12.72,0.05,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
target 20260716.3551 12.72CV 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 07 16.3551 2461237.8551 12.84 12:29:19.35 +73:22:37.8
125.11520 43.65721 galactic Dra Second-epoch detections are separated by 1.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:29:19.35 +73:22:37.8 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:29:19.35 +73:22:37.8: 13.85 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:29:19.35 +73:22:37.8: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461237.8551,12.84,0.05,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 20260716.3551 12.84CV 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 07 16.3551 2461237.8551 12.48 12:45:22.96 +72:19:08.7
123.57983 44.80155 galactic Dra Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:45:22.96 +72:19:08.7 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:45:22.96 +72:19:08.7: 13.64 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:45:22.96 +72:19:08.7: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.48,0.05,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 20260716.3551 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.76 12:36:16.45 +72:18:06.2
124.55452 44.77872 galactic Dra Second-epoch detections are separated by 1.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:36:16.45 +72:18:06.2 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:16.45 +72:18:06.2: 13.63 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:36:16.45 +72:18:06.2: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8551,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3551 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3551 2461237.8551 12.86 12:35:28.75 +73:05:16.0
124.54403 43.99049 galactic Dra Second-epoch detections are separated by 2.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:28.75 +73:05:16.0 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.033 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:28.75 +73:05:16.0: 14.01 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:28.75 +73:05:16.0: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461237.8551,12.86,0.05,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
target 20260716.3551 12.86CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
First image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Last image: 2461237.85542528 16.07.2026 08:31:38.744 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5819
Objects passed selection criteria: 5780
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 3633.75
Average stars matched: 3433.5 (94.4892 %)
Memory usage VmPeak: 115404 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 04:20:58 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
First image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Last image: 2461237.85542528 16.07.2026 08:31:38.744 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 158
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.22
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: 12 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 33594
Objects passed selection criteria: 33492
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 21651.8
Average stars matched: 20191.8 (93.2569 %)
Memory usage VmPeak: 140272 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 04:22:42 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.cat to cache
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.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/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461237.85483734
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_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits exists and is non-empty
Saving wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits to local_wcs_cache/
'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits exists and is non-empty
Saving wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits to local_wcs_cache/
'wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits' -> 'local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits'
wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits exists and is non-empty
Saving wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits to local_wcs_cache/
'wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits' -> 'local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits'
wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits exists and is non-empty
Saving wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits to local_wcs_cache/
'wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits' -> 'local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (1st reference image)
verification OK: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:37.960 +69:59:44.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits (1st new image)
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
Image size: 937.5'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 11:59:59.565 +69:59:39.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:37.960 +69:59:44.31
Second-epoch image center 11:59:59.565 +69:59:39.36
Angular distance between the image centers 0.0308 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits (2nd new image)
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
Image size: 937.5'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 11:59:55.504 +69:59:09.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:37.960 +69:59:44.31
Second-epoch image center 11:59:55.504 +69:59:09.45
Angular distance between the image centers 0.0268 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 11:59:59.565 +69:59:39.36
Second-epoch second image center 11:59:55.504 +69:59:09.45
Angular distance between the image centers 0.01013 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/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits &> /tmp/tmp.eC0TcASEPR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits &> /tmp/tmp.QRi5zJcAYL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits &> /tmp/tmp.fu8bEOqBfA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits &> /tmp/tmp.WU3CIyrsv9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Found non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
The reference image (wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits) and catalog (wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat) found
'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat' -> 'wcsmag.cat'
Read 7645 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.6428 to 206.7164 deg, Dec +62.8285 to +75.5474 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 151.6428 to 206.7164 deg, Dec 62.8285 to 75.5474 deg
Loaded 8253 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): 4551 out of 4756 total matches.
Matched with Tycho-2 4756 out of 7645 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.845900
a=0.000000 b=1.000000 c=22.845900
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7645 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.6428 to 206.7164 deg, Dec +62.8285 to +75.5474 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 151.6428 to 206.7164 deg, Dec 62.8285 to 75.5474 deg
Loaded 8253 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): 4551 out of 4756 total matches.
Matched with Tycho-2 4756 out of 7645 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits:
Forced-photometry filter: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -> calib.txt_param_ref_wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (aperture=6.1)
Read 7626 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.6431 to 206.7164 deg, Dec +62.8284 to +75.5474 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 151.6431 to 206.7164 deg, Dec 62.8284 to 75.5474 deg
Loaded 8253 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): 4547 out of 4752 total matches.
Matched with Tycho-2 4752 out of 7626 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits:
Forced-photometry filter: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits -> calib.txt_param_ref_wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.1 pix Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
2.8 pix fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
2.8 pix fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
2.1 pix wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.1 pix wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Limiting magnitude estimates:
15.3 mag. Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
15.3 mag. Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
13.0 mag. fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
13.0 mag. fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 10.6 (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
############ /tmp/tmp.eC0TcASEPR (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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=549, bad_region=1822, passed=7645
Got 7645 stars (including 5397 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
util/solve_plate_with_UCAC5 got 7645 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits N_match=966 sigma_overall_arcsec=0.395 sigma_q1_arcsec=0.503 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.371 n_q1=312 n_q2=173 n_q3=294 n_q4=187 worst_quadrant_to_overall_ratio=1.275
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -region wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QRi5zJcAYL (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits' -> 'wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.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=542, bad_region=1843, passed=7626
Got 7626 stars (including 5360 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat
util/solve_plate_with_UCAC5 got 7626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits N_match=965 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.453 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.298 n_q1=306 n_q2=173 n_q3=296 n_q4=190 worst_quadrant_to_overall_ratio=1.251
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits -region wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fu8bEOqBfA (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_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.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_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.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=121, bad_region=626, passed=2077
Got 2077 stars (including 1382 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat
util/solve_plate_with_UCAC5 got 2077 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 1490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 1491 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 1491 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits N_match=958 sigma_overall_arcsec=0.446 sigma_q1_arcsec=0.412 sigma_q2_arcsec=0.556 sigma_q3_arcsec=0.448 sigma_q4_arcsec=0.463 n_q1=374 n_q2=175 n_q3=222 n_q4=187 worst_quadrant_to_overall_ratio=1.249
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits -region wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WU3CIyrsv9 (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_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.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_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.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=115, bad_region=671, passed=2219
Got 2219 stars (including 1480 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat
util/solve_plate_with_UCAC5 got 2219 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 1636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 1637 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 1637 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits N_match=964 sigma_overall_arcsec=0.505 sigma_q1_arcsec=0.413 sigma_q2_arcsec=0.597 sigma_q3_arcsec=0.571 sigma_q4_arcsec=0.560 n_q1=367 n_q2=173 n_q3=225 n_q4=199 worst_quadrant_to_overall_ratio=1.182
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits -region wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits sigma_overall=0.395 worst_q_ratio=1.275
ref2=Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits sigma_overall=0.362 worst_q_ratio=1.251
new1=fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits sigma_overall=0.446 worst_q_ratio=1.249
new2=fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits sigma_overall=0.505 worst_q_ratio=1.182
reference average sigma_overall=0.3785 worst_q_ratio=1.263
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294_astrometric_residuals.png (966 matched stars from wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295_astrometric_residuals.png (965 matched stars from wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236_astrometric_residuals.png (958 matched stars from wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237_astrometric_residuals.png (964 matched stars from wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits'
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits'
Preparing the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.cat to cache
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Creating symlink local_wcs_cache/wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits exists and is non-empty
wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits exists and is non-empty
wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits exists and is non-empty
wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (1st reference image)
verification OK: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:37.960 +69:59:44.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits (1st new image)
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
Image size: 937.5'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 11:59:59.565 +69:59:39.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:37.960 +69:59:44.31
Second-epoch image center 11:59:59.565 +69:59:39.36
Angular distance between the image centers 0.0308 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits (2nd new image)
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
Image size: 937.5'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 11:59:55.504 +69:59:09.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:37.960 +69:59:44.31
Second-epoch image center 11:59:55.504 +69:59:09.45
Angular distance between the image centers 0.0268 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 11:59:59.565 +69:59:39.36
Second-epoch second image center 11:59:55.504 +69:59:09.45
Angular distance between the image centers 0.01013 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/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits &> /tmp/tmp.exnuHwig0X
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits &> /tmp/tmp.JqL5EgBgiT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits &> /tmp/tmp.mkkAQseU6T
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits &> /tmp/tmp.gmjlM6FfIB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Found non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
The reference image (wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits) and catalog (wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat) found
'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat' -> 'wcsmag.cat'
Read 42210 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3664 to 206.9040 deg, Dec +62.7303 to +75.5592 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 151.3664 to 206.9040 deg, Dec 62.7303 to 75.5592 deg
Loaded 8396 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): 4348 out of 4842 total matches.
Matched with Tycho-2 4842 out of 42210 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.724750
a=0.000000 b=1.000000 c=22.724750
From vast_summary.log: estimated ref. image limiting mag.: -7.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 42210 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3664 to 206.9040 deg, Dec +62.7303 to +75.5592 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 151.3664 to 206.9040 deg, Dec 62.7303 to 75.5592 deg
Loaded 8396 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): 4348 out of 4842 total matches.
Matched with Tycho-2 4842 out of 42210 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits:
Forced-photometry filter: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -> calib.txt_param_ref_wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (aperture=4.7)
Read 42071 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3666 to 206.9042 deg, Dec +62.7305 to +75.5474 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 151.3666 to 206.9042 deg, Dec 62.7305 to 75.5474 deg
Loaded 8393 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): 4349 out of 4835 total matches.
Matched with Tycho-2 4835 out of 42071 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits:
Forced-photometry filter: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits -> calib.txt_param_ref_wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits (aperture=4.7)
____ 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:
2.0 pix Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.0 pix Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
2.5 pix fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
2.5 pix fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
2.0 pix wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.0 pix wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Limiting magnitude estimates:
15.5 mag. Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
15.5 mag. Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
13.1 mag. fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
13.2 mag. fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.8 (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.exnuHwig0X (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.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=11, blended=2006, bad_region=8242, passed=42199
Got 42199 stars (including 32315 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
util/solve_plate_with_UCAC5 got 42199 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 34770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 34770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 34772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits N_match=971 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.456 sigma_q2_arcsec=0.358 sigma_q3_arcsec=0.329 sigma_q4_arcsec=0.364 n_q1=306 n_q2=173 n_q3=308 n_q4=184 worst_quadrant_to_overall_ratio=1.196
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -region wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JqL5EgBgiT (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits' -> 'wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.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=12, blended=1960, bad_region=8155, passed=42059
Got 42059 stars (including 32270 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat
util/solve_plate_with_UCAC5 got 42059 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 34605 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 34605 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 34605 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits N_match=968 sigma_overall_arcsec=0.364 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.346 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.317 n_q1=304 n_q2=168 n_q3=305 n_q4=191 worst_quadrant_to_overall_ratio=1.198
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits -region wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.mkkAQseU6T (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_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.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_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.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=675, bad_region=2625, passed=12129
Got 12129 stars (including 9318 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat
util/solve_plate_with_UCAC5 got 12129 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 9697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 9698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 9698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits N_match=951 sigma_overall_arcsec=0.431 sigma_q1_arcsec=0.403 sigma_q2_arcsec=0.550 sigma_q3_arcsec=0.456 sigma_q4_arcsec=0.437 n_q1=379 n_q2=164 n_q3=226 n_q4=182 worst_quadrant_to_overall_ratio=1.277
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits -region wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.gmjlM6FfIB (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_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.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_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=676, bad_region=2844, passed=12568
Got 12568 stars (including 9513 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat
util/solve_plate_with_UCAC5 got 12568 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 10159 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
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 10161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 10161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits N_match=957 sigma_overall_arcsec=0.498 sigma_q1_arcsec=0.417 sigma_q2_arcsec=0.574 sigma_q3_arcsec=0.576 sigma_q4_arcsec=0.531 n_q1=368 n_q2=162 n_q3=232 n_q4=195 worst_quadrant_to_overall_ratio=1.158
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits -region wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.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_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-30-47_20.00sec_4.90C_LIGHT_0236.fits
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.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_2026-07-16_CI_Dra-03-Q2b1x1_033217_TTUQ2b1x1_2119428_tB6L5Rib/wcs_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237.fits
Preparing the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:27:06.38 +73:40:43.7: 13.85 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:47:27.01 +72:18:12.4: 12.51 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:18.77 +72:18:08.6: 12.46 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:41:43.81 +72:29:30.6: 12.50 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:33.89 +73:18:36.3: 14.17 +/- 0.07 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:49:26.91 +70:35:39.0: 13.44 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:16:06.82 +73:29:26.2: 13.17 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:39.48 +73:23:00.0: 13.65 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:19:05.94 +66:59:08.9: 12.49 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:44.00 +73:02:32.2: 12.87 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:27:06.38 +73:40:43.7: 13.89 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:47:27.01 +72:18:12.4: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Forced photometry filter KEPT candidate at 12:47:27.01 +72:18:12.4: ref_mag=12.51 +/- 0.01 new_mean_mag=11.5810 delta=0.93 (need > 0.90)
Forced photometry filter KEPT candidate at 12:27:06.38 +73:40:43.7: ref_mag=13.87 +/- 0.04 new_mean_mag=12.8020 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:41:43.81 +72:29:30.6: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter KEPT candidate at 12:41:43.81 +72:29:30.6: ref_mag=12.51 +/- 0.01 new_mean_mag=11.5653 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:33.89 +73:18:36.3: 14.33 +/- 0.07 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:49:26.91 +70:35:39.0: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.05
Forced photometry filter KEPT candidate at 12:33:33.89 +73:18:36.3: ref_mag=14.24 +/- 0.05 new_mean_mag=12.9140 delta=1.33 (need > 0.90)
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter KEPT candidate at 12:49:26.91 +70:35:39.0: ref_mag=13.44 +/- 0.02 new_mean_mag=12.4244 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:18.77 +72:18:08.6: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter KEPT candidate at 12:46:18.77 +72:18:08.6: ref_mag=12.47 +/- 0.01 new_mean_mag=11.4479 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:39.48 +73:23:00.0: 13.70 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:16:06.82 +73:29:26.2: 13.14 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:19:05.94 +66:59:08.9: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 12:35:39.48 +73:23:00.0: ref_mag=13.67 +/- 0.03 new_mean_mag=12.5832 delta=1.09 (need > 0.90)
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter KEPT candidate at 12:19:05.94 +66:59:08.9: ref_mag=12.50 +/- 0.01 new_mean_mag=11.4696 delta=1.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 12:16:06.82 +73:29:26.2: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1859 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:44.00 +73:02:32.2: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 12:33:44.00 +73:02:32.2: ref_mag=12.88 +/- 0.01 new_mean_mag=11.9194 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:19:19.80 +66:59:07.5: 13.69 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:19:19.80 +66:59:07.5: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 12:19:19.80 +66:59:07.5: ref_mag=13.66 +/- 0.03 new_mean_mag=12.5394 delta=1.12 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:21.75 +72:11:05.0: 12.89 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:16:55.88 +73:15:12.8: 13.24 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:21.75 +72:11:05.0: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter KEPT candidate at 12:46:21.75 +72:11:05.0: ref_mag=12.91 +/- 0.01 new_mean_mag=11.9344 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:16:55.88 +73:15:12.8: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 12:16:55.88 +73:15:12.8: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2741 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:17:52.76 +73:29:22.7: 13.48 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:27:36.87 +73:50:18.6: 13.26 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:17:52.76 +73:29:22.7: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Forced photometry filter KEPT candidate at 12:17:52.76 +73:29:22.7: ref_mag=13.51 +/- 0.02 new_mean_mag=12.5423 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:27:36.87 +73:50:18.6: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 12:27:36.87 +73:50:18.6: ref_mag=13.31 +/- 0.02 new_mean_mag=12.2749 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:01.41 +73:27:55.3: 13.49 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:01.41 +73:27:55.3: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:01.41 +73:27:55.3: ref_mag=13.51 +/- 0.03 new_mean_mag=12.3816 delta=1.13 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:56.84 +67:42:46.6: 13.53 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:36.51 +73:09:38.4: 13.90 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:18:56.84 +67:42:46.6: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Forced photometry filter KEPT candidate at 11:18:56.84 +67:42:46.6: ref_mag=13.52 +/- 0.02 new_mean_mag=12.5873 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:16.37 +72:34:53.7: 12.61 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:36.51 +73:09:38.4: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter KEPT candidate at 12:33:36.51 +73:09:38.4: ref_mag=13.93 +/- 0.04 new_mean_mag=12.6792 delta=1.25 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:42:16.37 +72:34:53.7: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 12:42:16.37 +72:34:53.7: ref_mag=12.60 +/- 0.01 new_mean_mag=11.6031 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:48:46.53 +71:40:17.1: 13.90 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:48:46.53 +71:40:17.1: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter KEPT candidate at 12:48:46.53 +71:40:17.1: ref_mag=13.93 +/- 0.04 new_mean_mag=12.8034 delta=1.12 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:12:36.11 +73:30:32.6: 13.76 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:12:36.11 +73:30:32.6: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 12:12:36.11 +73:30:32.6: ref_mag=13.79 +/- 0.03 new_mean_mag=12.7823 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:08.91 +73:46:38.1: 13.55 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:43:22.18 +72:26:24.5: 13.02 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:08.91 +73:46:38.1: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:43:22.18 +72:26:24.5: 13.01 +/- 0.02 detection
Forced photometry filter KEPT candidate at 12:13:08.91 +73:46:38.1: ref_mag=13.55 +/- 0.03 new_mean_mag=12.6267 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 12:43:22.18 +72:26:24.5: ref_mag=13.01 +/- 0.02 new_mean_mag=11.9420 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:19:12.07 +68:16:09.6: 13.04 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:19:12.07 +68:16:09.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 11:19:12.07 +68:16:09.6: ref_mag=13.08 +/- 0.02 new_mean_mag=12.1085 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:21.13 +73:47:19.0: 13.76 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:21.13 +73:47:19.0: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Forced photometry filter KEPT candidate at 12:33:21.13 +73:47:19.0: ref_mag=13.80 +/- 0.03 new_mean_mag=12.7778 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:41:14.90 +72:17:54.1: 13.77 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:11.36 +72:31:43.3: 13.11 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:41:14.90 +72:17:54.1: 13.77 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:26:32.48 +72:25:57.6: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter KEPT candidate at 12:41:14.90 +72:17:54.1: ref_mag=13.77 +/- 0.03 new_mean_mag=12.5725 delta=1.20 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:42:11.36 +72:31:43.3: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 12:42:11.36 +72:31:43.3: ref_mag=13.11 +/- 0.02 new_mean_mag=12.0260 delta=1.08 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:26:32.48 +72:25:57.6: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 12:26:32.48 +72:25:57.6: ref_mag=13.62 +/- 0.03 new_mean_mag=12.6353 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:19:37.07 +66:59:37.8: 13.93 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:01.16 +73:14:03.4: 13.82 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:31:07.67 +73:44:08.9: 13.98 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:01.16 +73:14:03.4: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:01.16 +73:14:03.4: ref_mag=13.89 +/- 0.03 new_mean_mag=12.5716 delta=1.32 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:19:37.07 +66:59:37.8: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 12:19:37.07 +66:59:37.8: ref_mag=13.94 +/- 0.04 new_mean_mag=12.7406 delta=1.20 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:31:07.67 +73:44:08.9: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.04
Forced photometry filter KEPT candidate at 12:31:07.67 +73:44:08.9: ref_mag=14.07 +/- 0.04 new_mean_mag=12.7567 delta=1.32 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:39.02 +72:53:08.0: 13.62 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:39.02 +72:53:08.0: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 12:35:39.02 +72:53:08.0: ref_mag=13.65 +/- 0.03 new_mean_mag=12.6391 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:44:17.97 +72:28:44.4: 12.75 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:44:17.97 +72:28:44.4: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 12:44:17.97 +72:28:44.4: ref_mag=12.78 +/- 0.01 new_mean_mag=11.6933 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:54.20 +73:05:44.5: 12.81 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:54.20 +73:05:44.5: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 12:34:54.20 +73:05:44.5: ref_mag=12.82 +/- 0.01 new_mean_mag=11.7707 delta=1.05 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:51:58.10 +71:26:32.8: 13.66 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:20.83 +68:23:25.9: 13.64 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:51:58.10 +71:26:32.8: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry filter KEPT candidate at 12:51:58.10 +71:26:32.8: ref_mag=13.63 +/- 0.03 new_mean_mag=12.5107 delta=1.11 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:16:20.83 +68:23:25.9: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 11:16:20.83 +68:23:25.9: ref_mag=13.66 +/- 0.03 new_mean_mag=12.6683 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:53.60 +73:46:37.5: 14.00 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:53.60 +73:46:37.5: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.04
Forced photometry filter KEPT candidate at 12:13:53.60 +73:46:37.5: ref_mag=14.04 +/- 0.04 new_mean_mag=12.9062 delta=1.13 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:29:31.29 +73:18:12.5: 14.29 +/- 0.07 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:29:31.29 +73:18:12.5: 14.24 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.05
Forced photometry filter KEPT candidate at 12:29:31.29 +73:18:12.5: ref_mag=14.27 +/- 0.05 new_mean_mag=12.7735 delta=1.49 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:23:16.64 +74:08:08.4: 13.62 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:23:16.64 +74:08:08.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter KEPT candidate at 12:23:16.64 +74:08:08.4: ref_mag=13.60 +/- 0.03 new_mean_mag=12.5611 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:30.27 +72:08:14.3: 13.61 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:30.27 +72:08:14.3: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 12:46:30.27 +72:08:14.3: ref_mag=13.62 +/- 0.03 new_mean_mag=12.5454 delta=1.08 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:20:46.73 +73:34:16.1: 13.62 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:18:11.97 +67:18:27.9: 13.61 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:20:46.73 +73:34:16.1: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Forced photometry filter KEPT candidate at 12:20:46.73 +73:34:16.1: ref_mag=13.58 +/- 0.03 new_mean_mag=12.6514 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:29:42.57 +73:46:19.6: 14.25 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:18:11.97 +67:18:27.9: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter KEPT candidate at 12:18:11.97 +67:18:27.9: ref_mag=13.59 +/- 0.03 new_mean_mag=12.5418 delta=1.05 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:29:42.57 +73:46:19.6: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.05
Forced photometry filter KEPT candidate at 12:29:42.57 +73:46:19.6: ref_mag=14.23 +/- 0.05 new_mean_mag=12.9557 delta=1.28 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:53.81 +73:27:17.3: 13.84 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:33.76 +72:02:26.0: 13.83 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:53.81 +73:27:17.3: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:53.81 +73:27:17.3: ref_mag=13.78 +/- 0.03 new_mean_mag=12.5516 delta=1.23 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:33.76 +72:02:26.0: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter KEPT candidate at 12:46:33.76 +72:02:26.0: ref_mag=13.85 +/- 0.03 new_mean_mag=12.8123 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:15:36.06 +67:06:22.6: 13.82 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:15:36.06 +67:06:22.6: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter KEPT candidate at 12:15:36.06 +67:06:22.6: ref_mag=13.77 +/- 0.03 new_mean_mag=12.6842 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:42.19 +73:05:12.4: 14.43 +/- 0.08 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:42.19 +73:05:12.4: 14.65 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.06
Forced photometry filter KEPT candidate at 12:35:42.19 +73:05:12.4: ref_mag=14.51 +/- 0.06 new_mean_mag=13.1530 delta=1.36 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:31.80 +73:48:33.1: 13.59 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:31.80 +73:48:33.1: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:31.80 +73:48:33.1: ref_mag=13.65 +/- 0.03 new_mean_mag=12.7465 delta=0.90 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:08.19 +72:20:07.5: 13.73 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:08.19 +72:20:07.5: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Forced photometry filter KEPT candidate at 12:35:08.19 +72:20:07.5: ref_mag=13.74 +/- 0.03 new_mean_mag=12.5953 delta=1.14 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:44:46.35 +72:39:08.9: 13.80 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:44:46.35 +72:39:08.9: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 12:44:46.35 +72:39:08.9: ref_mag=13.79 +/- 0.03 new_mean_mag=12.7885 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:45:12.32 +72:31:52.1: 13.56 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:45:12.32 +72:31:52.1: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Forced photometry filter KEPT candidate at 12:45:12.32 +72:31:52.1: ref_mag=13.58 +/- 0.03 new_mean_mag=12.3861 delta=1.19 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:47:27.35 +70:51:39.9: 13.93 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:47:27.35 +70:51:39.9: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Forced photometry filter KEPT candidate at 12:47:27.35 +70:51:39.9: ref_mag=13.92 +/- 0.04 new_mean_mag=12.8391 delta=1.08 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:16.90 +73:28:57.8: 13.41 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:16.90 +73:28:57.8: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter KEPT candidate at 12:13:16.90 +73:28:57.8: ref_mag=13.46 +/- 0.02 new_mean_mag=12.3152 delta=1.14 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:31.30 +73:02:42.5: 13.41 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:31.30 +73:02:42.5: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 12:34:31.30 +73:02:42.5: ref_mag=13.42 +/- 0.02 new_mean_mag=12.4312 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:48.09 +68:56:05.5: 13.41 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:27:31.36 +66:35:33.8: 13.12 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:17:48.09 +68:56:05.5: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 11:17:48.09 +68:56:05.5: ref_mag=13.37 +/- 0.02 new_mean_mag=12.4337 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:23.75 +73:36:45.5: 13.11 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:27:31.36 +66:35:33.8: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 12:27:31.36 +66:35:33.8: ref_mag=13.11 +/- 0.02 new_mean_mag=12.1595 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:23.75 +73:36:45.5: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 12:35:23.75 +73:36:45.5: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1987 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:47:24.17 +72:23:50.4: 13.77 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:37:37.46 +72:09:48.0: 13.76 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:41:44.17 +72:16:41.2: 13.76 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:47:24.17 +72:23:50.4: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter KEPT candidate at 12:47:24.17 +72:23:50.4: ref_mag=13.77 +/- 0.03 new_mean_mag=12.6137 delta=1.16 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:41:44.17 +72:16:41.2: 13.71 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:37:37.46 +72:09:48.0: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter KEPT candidate at 12:41:44.17 +72:16:41.2: ref_mag=13.73 +/- 0.03 new_mean_mag=12.5777 delta=1.15 (need > 0.90)
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter KEPT candidate at 12:37:37.46 +72:09:48.0: ref_mag=13.77 +/- 0.03 new_mean_mag=12.6744 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:14:11.70 +68:44:55.5: 13.77 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:14:11.70 +68:44:55.5: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter KEPT candidate at 11:14:11.70 +68:44:55.5: ref_mag=13.77 +/- 0.03 new_mean_mag=12.7584 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:36:43.94 +66:56:50.4: 13.07 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:36:43.94 +66:56:50.4: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 11:36:43.94 +66:56:50.4: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1353 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:18:16.53 +73:09:08.8: 13.74 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:18:16.53 +73:09:08.8: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 12:18:16.53 +73:09:08.8: ref_mag=13.75 +/- 0.03 new_mean_mag=12.6338 delta=1.11 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:18.15 +73:27:38.0: 13.06 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:18.15 +73:27:38.0: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 12:13:18.15 +73:27:38.0: ref_mag=13.07 +/- 0.02 new_mean_mag=12.0463 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:41:13.20 +72:36:46.7: 13.58 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:22:43.80 +74:08:25.3: 13.54 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:41:13.20 +72:36:46.7: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter KEPT candidate at 12:41:13.20 +72:36:46.7: ref_mag=13.59 +/- 0.03 new_mean_mag=12.4152 delta=1.18 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:22:43.80 +74:08:25.3: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter KEPT candidate at 12:22:43.80 +74:08:25.3: ref_mag=13.56 +/- 0.03 new_mean_mag=12.6287 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:27.10 +68:34:43.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:16:27.10 +68:34:43.3: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 11:16:27.10 +68:34:43.3: ref_mag=13.03 +/- 0.01 new_mean_mag=11.9984 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:43:19.37 +72:16:40.0: 13.01 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:24.55 +73:43:06.7: 13.92 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:43:19.37 +72:16:40.0: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 12:43:19.37 +72:16:40.0: ref_mag=13.02 +/- 0.02 new_mean_mag=11.9187 delta=1.10 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:24.55 +73:43:06.7: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Forced photometry filter KEPT candidate at 12:13:24.55 +73:43:06.7: ref_mag=13.95 +/- 0.04 new_mean_mag=12.7908 delta=1.16 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:18.61 +73:40:29.7: 13.94 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:15:44.91 +73:30:29.8: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:18.61 +73:40:29.7: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.04
Forced photometry filter KEPT candidate at 12:34:18.61 +73:40:29.7: ref_mag=13.98 +/- 0.04 new_mean_mag=12.7895 delta=1.19 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:15:44.91 +73:30:29.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry filter KEPT candidate at 12:15:44.91 +73:30:29.8: ref_mag=13.35 +/- 0.02 new_mean_mag=12.3548 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:45:10.51 +72:24:24.9: 13.37 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:45:10.51 +72:24:24.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 12:45:10.51 +72:24:24.9: ref_mag=13.37 +/- 0.02 new_mean_mag=12.2223 delta=1.14 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:25:22.18 +74:06:25.1: 13.38 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:25:22.18 +74:06:25.1: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 12:25:22.18 +74:06:25.1: ref_mag=13.38 +/- 0.02 new_mean_mag=12.3211 delta=1.05 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:24:38.33 +67:31:06.8: 13.56 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:24:38.33 +67:31:06.8: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 11:24:38.33 +67:31:06.8: ref_mag=13.57 +/- 0.03 new_mean_mag=12.6030 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:30.19 +68:06:10.0: 13.57 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:17:30.19 +68:06:10.0: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Forced photometry filter KEPT candidate at 11:17:30.19 +68:06:10.0: ref_mag=13.55 +/- 0.02 new_mean_mag=12.5689 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:31:20.66 +73:03:17.8: 13.56 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:31:20.66 +73:03:17.8: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter KEPT candidate at 12:31:20.66 +73:03:17.8: ref_mag=13.55 +/- 0.03 new_mean_mag=12.6146 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:13:55.09 +73:35:56.1: 13.35 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:13:55.09 +73:35:56.1: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 12:13:55.09 +73:35:56.1: ref_mag=13.34 +/- 0.02 new_mean_mag=12.3820 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:38:53.39 +68:47:24.9: 13.54 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:38:53.39 +68:47:24.9: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Forced photometry filter KEPT candidate at 11:38:53.39 +68:47:24.9: ref_mag=13.57 +/- 0.02 new_mean_mag=12.5462 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:35.90 +70:57:52.2: 14.11 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:27:08.47 +73:54:09.9: 13.36 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:35.90 +70:57:52.2: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.05
Forced photometry filter KEPT candidate at 12:46:35.90 +70:57:52.2: ref_mag=14.15 +/- 0.05 new_mean_mag=12.9488 delta=1.20 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:27:08.47 +73:54:09.9: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 12:27:08.47 +73:54:09.9: ref_mag=13.40 +/- 0.02 new_mean_mag=12.3435 delta=1.05 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:41:38.30 +65:51:58.4: 13.35 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:41:38.30 +65:51:58.4: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 11:41:38.30 +65:51:58.4: ref_mag=13.36 +/- 0.02 new_mean_mag=12.3503 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:06:29.03 +74:13:10.6: 13.52 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:06:29.03 +74:13:10.6: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Forced photometry filter KEPT candidate at 12:06:29.03 +74:13:10.6: ref_mag=13.51 +/- 0.02 new_mean_mag=12.5962 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:48:12.83 +72:07:10.9: 13.89 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:25:07.12 +68:30:23.3: 13.31 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:48:12.83 +72:07:10.9: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Forced photometry filter KEPT candidate at 12:48:12.83 +72:07:10.9: ref_mag=13.92 +/- 0.04 new_mean_mag=12.7045 delta=1.21 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:25:07.12 +68:30:23.3: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 11:25:07.12 +68:30:23.3: ref_mag=13.31 +/- 0.02 new_mean_mag=12.3624 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:44:29.56 +72:26:09.8: 13.31 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:44:29.56 +72:26:09.8: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 12:44:29.56 +72:26:09.8: ref_mag=13.30 +/- 0.02 new_mean_mag=12.0868 delta=1.21 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:09:04.15 +67:40:37.2: 13.74 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:09:04.15 +67:40:37.2: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry filter KEPT candidate at 12:09:04.15 +67:40:37.2: ref_mag=13.76 +/- 0.03 new_mean_mag=12.7452 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:24:20.30 +73:48:45.9: 13.72 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:24:20.30 +73:48:45.9: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 12:24:20.30 +73:48:45.9: ref_mag=13.75 +/- 0.03 new_mean_mag=12.7078 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:36.44 +72:03:34.6: 13.73 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:30:10.75 +73:50:40.8: 13.90 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:30:10.75 +73:50:40.8: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 12:30:10.75 +73:50:40.8: ref_mag=13.94 +/- 0.04 new_mean_mag=12.8293 delta=1.12 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:36:36.44 +72:03:34.6: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 12:36:36.44 +72:03:34.6: ref_mag=13.71 +/- 0.03 new_mean_mag=12.7772 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:29:53.29 +73:53:18.5: 13.49 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:23:57.52 +66:48:25.8: 13.30 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:29:53.29 +73:53:18.5: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter KEPT candidate at 12:29:53.29 +73:53:18.5: ref_mag=13.50 +/- 0.03 new_mean_mag=12.5458 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:23:57.52 +66:48:25.8: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 12:23:57.52 +66:48:25.8: ref_mag=13.30 +/- 0.02 new_mean_mag=12.3065 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:35:08.28 +66:53:29.5: 13.30 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:14:18.44 +73:33:43.3: 13.28 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:35:08.28 +66:53:29.5: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 11:35:08.28 +66:53:29.5: ref_mag=13.31 +/- 0.02 new_mean_mag=12.3590 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:14:18.44 +73:33:43.3: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 12:14:18.44 +73:33:43.3: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2655 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:28.95 +72:36:52.9: 14.08 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:36:28.95 +72:36:52.9: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.04
Forced photometry filter KEPT candidate at 12:36:28.95 +72:36:52.9: ref_mag=14.11 +/- 0.04 new_mean_mag=12.9420 delta=1.16 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:14:15.87 +73:28:53.5: 13.52 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:14:15.87 +73:28:53.5: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry filter KEPT candidate at 12:14:15.87 +73:28:53.5: ref_mag=13.49 +/- 0.02 new_mean_mag=12.4479 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:19:49.21 +67:01:52.8: 13.26 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:14:00.83 +67:09:28.6: 13.27 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:19:49.21 +67:01:52.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 12:19:49.21 +67:01:52.8: ref_mag=13.31 +/- 0.02 new_mean_mag=12.2351 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:28:50.72 +73:52:20.0: 13.24 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:32.73 +72:11:36.1: 13.22 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:28:29.70 +66:28:10.3: 13.25 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:14:00.83 +67:09:28.6: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 12:14:00.83 +67:09:28.6: ref_mag=13.23 +/- 0.02 new_mean_mag=12.1898 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:57.46 +72:58:46.6: 13.68 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:20.46 +67:56:17.4: 13.23 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:19:42.04 +68:26:58.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:28:50.72 +73:52:20.0: 13.22 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:36:32.73 +72:11:36.1: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:28:29.70 +66:28:10.3: 13.15 +/- 0.03 detection
Forced photometry filter KEPT candidate at 12:28:50.72 +73:52:20.0: ref_mag=13.23 +/- 0.02 new_mean_mag=12.3069 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 12:36:32.73 +72:11:36.1: ref_mag=13.25 +/- 0.02 new_mean_mag=12.2771 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 12:28:29.70 +66:28:10.3: ref_mag=13.20 +/- 0.02 new_mean_mag=12.2490 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:44:51.41 +72:33:23.2: 13.20 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:31.36 +73:12:26.5: 14.06 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:34:57.46 +72:58:46.6: 13.85 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:26:20.46 +67:56:17.4: 13.25 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:19:42.04 +68:26:58.3: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 12:34:57.46 +72:58:46.6: ref_mag=13.75 +/- 0.03 new_mean_mag=12.6146 delta=1.13 (need > 0.90)
Forced photometry filter KEPT candidate at 11:19:42.04 +68:26:58.3: ref_mag=13.26 +/- 0.02 new_mean_mag=12.3092 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 11:26:20.46 +67:56:17.4: ref_mag=13.24 +/- 0.02 new_mean_mag=12.2875 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:31.36 +73:12:26.5: 14.04 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:44:51.41 +72:33:23.2: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.04
Forced photometry filter KEPT candidate at 12:35:31.36 +73:12:26.5: ref_mag=14.05 +/- 0.04 new_mean_mag=12.7238 delta=1.33 (need > 0.90)
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 12:44:51.41 +72:33:23.2: ref_mag=13.20 +/- 0.02 new_mean_mag=12.1231 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:29.17 +72:13:40.8: 13.46 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:29.17 +72:13:40.8: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter KEPT candidate at 12:46:29.17 +72:13:40.8: ref_mag=13.50 +/- 0.03 new_mean_mag=12.3602 delta=1.14 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:25:52.19 +68:27:05.9: 13.48 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:25:52.19 +68:27:05.9: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 11:25:52.19 +68:27:05.9: ref_mag=13.45 +/- 0.02 new_mean_mag=12.4597 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:29.33 +72:54:00.9: 13.45 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:17:16.47 +67:04:49.4: 13.45 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:29.33 +72:54:00.9: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter KEPT candidate at 12:33:29.33 +72:54:00.9: ref_mag=13.44 +/- 0.02 new_mean_mag=12.5371 delta=0.90 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:17:16.47 +67:04:49.4: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter KEPT candidate at 12:17:16.47 +67:04:49.4: ref_mag=13.46 +/- 0.02 new_mean_mag=12.3860 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:25.55 +72:31:09.5: 12.89 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:42:25.55 +72:31:09.5: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 12:42:25.55 +72:31:09.5: ref_mag=12.88 +/- 0.01 new_mean_mag=11.7900 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:24:39.12 +73:59:11.4: 12.87 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:41:05.79 +72:22:30.0: 14.06 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:18:46.30 +67:14:30.9: 13.68 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:24:39.12 +73:59:11.4: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter REJECTED candidate at 12:24:39.12 +73:59:11.4: ref_mag=12.89 +/- 0.01 new_mean_mag=11.9898 delta=0.90 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:41:05.79 +72:22:30.0: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Forced photometry filter KEPT candidate at 12:41:05.79 +72:22:30.0: ref_mag=14.10 +/- 0.05 new_mean_mag=12.8489 delta=1.25 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:18:46.30 +67:14:30.9: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 12:18:46.30 +67:14:30.9: ref_mag=13.67 +/- 0.03 new_mean_mag=12.6993 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:36:31.39 +68:52:57.6: 13.70 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 11:36:31.39 +68:52:57.6: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter KEPT candidate at 11:36:31.39 +68:52:57.6: ref_mag=13.73 +/- 0.03 new_mean_mag=12.7197 delta=1.01 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:33:52.74 +73:43:29.5: 13.67 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:33:52.74 +73:43:29.5: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 12:33:52.74 +73:43:29.5: ref_mag=13.68 +/- 0.03 new_mean_mag=12.5519 delta=1.13 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:58.03 +72:09:33.1: 13.18 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:40:30.91 +72:25:31.6: 14.37 +/- 0.08 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:36:58.03 +72:09:33.1: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 12:36:58.03 +72:09:33.1: ref_mag=13.20 +/- 0.02 new_mean_mag=12.2619 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:40:30.91 +72:25:31.6: 14.38 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.06
Forced photometry filter KEPT candidate at 12:40:30.91 +72:25:31.6: ref_mag=14.37 +/- 0.06 new_mean_mag=13.0064 delta=1.37 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:16.11 +72:21:54.1: 13.67 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:42:16.11 +72:21:54.1: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Forced photometry filter KEPT candidate at 12:42:16.11 +72:21:54.1: ref_mag=13.64 +/- 0.03 new_mean_mag=12.5187 delta=1.12 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:24:22.55 +74:07:00.6: 13.66 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:24:22.55 +74:07:00.6: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 12:24:22.55 +74:07:00.6: ref_mag=13.67 +/- 0.03 new_mean_mag=12.6365 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:24:12.62 +74:10:38.4: 13.67 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:24:12.62 +74:10:38.4: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 12:24:12.62 +74:10:38.4: ref_mag=13.67 +/- 0.03 new_mean_mag=12.5967 delta=1.08 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:32:07.92 +73:42:35.2: 13.16 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:32:07.92 +73:42:35.2: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 12:32:07.92 +73:42:35.2: ref_mag=13.20 +/- 0.02 new_mean_mag=12.2436 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:40:37.33 +72:07:08.2: 13.48 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:40:37.33 +72:07:08.2: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry filter KEPT candidate at 12:40:37.33 +72:07:08.2: ref_mag=13.47 +/- 0.02 new_mean_mag=12.5095 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:25:40.11 +74:05:57.6: 13.43 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:25:40.11 +74:05:57.6: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 12:25:40.11 +74:05:57.6: ref_mag=13.43 +/- 0.02 new_mean_mag=12.4566 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:38.71 +72:25:37.5: 13.86 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:46:38.71 +72:25:37.5: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.03
Forced photometry filter KEPT candidate at 12:46:38.71 +72:25:37.5: ref_mag=13.87 +/- 0.03 new_mean_mag=12.6746 delta=1.19 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:45:22.96 +72:19:08.7: 13.64 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:29:19.35 +73:22:37.8: 13.85 +/- 0.05 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:45:22.96 +72:19:08.7: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 12:45:22.96 +72:19:08.7: ref_mag=13.62 +/- 0.03 new_mean_mag=12.4731 delta=1.15 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:29:19.35 +73:22:37.8: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.03
Forced photometry filter KEPT candidate at 12:29:19.35 +73:22:37.8: ref_mag=13.84 +/- 0.03 new_mean_mag=12.7870 delta=1.06 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:16.45 +72:18:06.2: 13.63 +/- 0.04 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:36:16.45 +72:18:06.2: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry filter KEPT candidate at 12:36:16.45 +72:18:06.2: ref_mag=13.63 +/- 0.03 new_mean_mag=12.7009 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:35:28.75 +73:05:16.0: 14.01 +/- 0.06 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-11-10_20.00sec_-14.90C_LIGHT_0295.fits at 12:35:28.75 +73:05:16.0: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter KEPT candidate at 12:35:28.75 +73:05:16.0: ref_mag=13.93 +/- 0.04 new_mean_mag=12.8410 delta=1.09 (need > 0.90)
Adding exclusion_list_local.txt__out05231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41080.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 481s
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: 66s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52310_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
The candidate 52310_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237 did not pass the final checks
**** FOUND 11:17:13.28 +66:09:13.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29284_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29284_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35239_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 35239_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29932_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29932_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07335_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 07335_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39482_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39482_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29931_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29931_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29218_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29218_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21183_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 21183_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28047_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 28047_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37635_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 37635_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07381_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 07381_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40592_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 40592_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36531_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 36531_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35716_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 35716_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34639_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 34639_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36050_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 36050_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14558_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 14558_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37188_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 37188_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39172_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39172_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30255_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 30255_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35588_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 35588_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34583_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 34583_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39739_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39739_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16641_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 16641_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34866_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 34866_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29952_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29952_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29771_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29771_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29869_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29869_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36863_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 36863_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07397_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 07397_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29091_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29091_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23927_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
The candidate 23927_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237 did not pass the final checks
**** FOUND 11:19:05.24 +70:06:09.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38101_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 38101_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29848_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29848_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29360_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29360_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30999_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 30999_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17553_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 17553_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34567_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 34567_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36646_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 36646_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33493_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 33493_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40738_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 40738_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35319_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 35319_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08588_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 08588_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34852_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 34852_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36024_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 36024_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41080_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 41080_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07967_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 07967_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29369_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29369_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34847_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 34847_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29915_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29915_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38922_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 38922_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29777_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29777_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22342_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 22342_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35590_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 35590_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37599_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 37599_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19416_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 19416_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05724_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 05724_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35584_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 35584_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39797_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39797_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40729_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 40729_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40244_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 40244_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19164_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 19164_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09857_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 09857_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37010_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 37010_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35780_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 35780_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39101_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39101_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33404_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 33404_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18259_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 18259_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40206_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 40206_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29054_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29054_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35368_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 35368_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35615_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 35615_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39602_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39602_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33680_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 33680_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13159_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 13159_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16211_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 16211_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37501_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 37501_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29158_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29158_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16567_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 16567_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22764_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 22764_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34460_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 34460_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05598_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 05598_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32691_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 32691_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40805_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 40805_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16901_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 16901_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29881_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29881_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10304_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 10304_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34732_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 34732_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40964_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 40964_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34673_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 34673_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34348_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 34348_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06576_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 06576_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09823_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 09823_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35464_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 35464_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39135_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39135_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29204_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29204_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07508_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 07508_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08197_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 08197_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05231_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 05231_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34485_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 34485_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40602_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 40602_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17334_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 17334_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14532_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 14532_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37843_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 37843_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39318_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39318_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37030_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 37030_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29954_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29954_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16561_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 16561_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29601_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29601_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07773_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 07773_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39443_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39443_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33911_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
The candidate 33911_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39941_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39941_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08348_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 08348_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17163_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 17163_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29102_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29102_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40679_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 40679_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39724_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39724_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39785_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39785_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33417_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 33417_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28848_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 28848_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35156_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 35156_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40796_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 40796_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33648_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 33648_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39755_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 39755_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28040_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 28040_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40153_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 40153_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29940_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29940_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29383_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
Preparing report for the candidate 29383_fd_Dra-03-Q2b1x1_2026-07-16_03-31-38_20.00sec_5.00C_LIGHT_0237
make_report_in_HTML.sh Phase 2 (HTML assembly): 10s
make_report_in_HTML.sh TOTAL: 557s
Prepared the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
12:28:29.70 +66:28:10.3
11:41:38.30 +65:51:58.4
12:27:31.36 +66:35:33.8
12:23:57.52 +66:48:25.8
12:19:05.94 +66:59:08.9
12:19:19.80 +66:59:07.5
12:19:37.07 +66:59:37.8
12:19:49.21 +67:01:52.8
12:17:16.47 +67:04:49.4
12:15:36.06 +67:06:22.6
12:14:00.83 +67:09:28.6
12:18:46.30 +67:14:30.9
12:18:11.97 +67:18:27.9
11:35:08.28 +66:53:29.5
11:36:43.94 +66:56:50.4
12:09:04.15 +67:40:37.2
11:24:38.33 +67:31:06.8
11:26:20.46 +67:56:17.4
11:18:56.84 +67:42:46.6
11:17:30.19 +68:06:10.0
11:25:52.19 +68:27:05.9
11:38:53.39 +68:47:24.9
11:19:12.07 +68:16:09.6
11:25:07.12 +68:30:23.3
11:36:31.39 +68:52:57.6
11:19:42.04 +68:26:58.3
11:16:20.83 +68:23:25.9
11:16:27.10 +68:34:43.3
11:14:11.70 +68:44:55.5
11:17:48.09 +68:56:05.5
12:49:26.91 +70:35:39.0
12:47:27.35 +70:51:39.9
12:46:35.90 +70:57:52.2
12:29:19.35 +73:22:37.8
12:35:39.48 +73:23:00.0
12:24:12.62 +74:10:38.4
12:13:24.55 +73:43:06.7
12:31:07.67 +73:44:08.9
12:33:52.74 +73:43:29.5
12:13:55.09 +73:35:56.1
12:14:15.87 +73:28:53.5
12:16:06.82 +73:29:26.2
12:33:33.89 +73:18:36.3
12:34:54.20 +73:05:44.5
12:35:42.19 +73:05:12.4
12:35:28.75 +73:05:16.0
12:33:29.33 +72:54:00.9
12:42:11.36 +72:31:43.3
12:45:12.32 +72:31:52.1
12:44:17.97 +72:28:44.4
12:26:32.48 +72:25:57.6
12:44:29.56 +72:26:09.8
12:35:08.19 +72:20:07.5
12:47:27.01 +72:18:12.4
12:46:18.77 +72:18:08.6
12:36:16.45 +72:18:06.2
12:41:14.90 +72:17:54.1
12:46:29.17 +72:13:40.8
12:48:46.53 +71:40:17.1
12:51:58.10 +71:26:32.8
12:06:29.03 +74:13:10.6
12:22:43.80 +74:08:25.3
12:24:22.55 +74:07:00.6
12:23:16.64 +74:08:08.4
12:25:40.11 +74:05:57.6
12:25:22.18 +74:06:25.1
12:29:53.29 +73:53:18.5
12:27:08.47 +73:54:09.9
12:28:50.72 +73:52:20.0
12:13:53.60 +73:46:37.5
12:13:08.91 +73:46:38.1
12:27:36.87 +73:50:18.6
12:30:10.75 +73:50:40.8
12:24:20.30 +73:48:45.9
12:34:31.80 +73:48:33.1
12:29:42.57 +73:46:19.6
12:33:21.13 +73:47:19.0
12:32:07.92 +73:42:35.2
12:27:06.38 +73:40:43.7
12:20:46.73 +73:34:16.1
12:34:18.61 +73:40:29.7
12:14:18.44 +73:33:43.3
12:35:23.75 +73:36:45.5
12:12:36.11 +73:30:32.6
12:13:16.90 +73:28:57.8
12:15:44.91 +73:30:29.8
12:17:52.76 +73:29:22.7
12:13:18.15 +73:27:38.0
12:34:53.81 +73:27:17.3
12:34:01.41 +73:27:55.3
12:16:55.88 +73:15:12.8
12:29:31.29 +73:18:12.5
12:34:01.16 +73:14:03.4
12:18:16.53 +73:09:08.8
12:35:31.36 +73:12:26.5
12:33:36.51 +73:09:38.4
12:31:20.66 +73:03:17.8
12:34:31.30 +73:02:42.5
12:33:44.00 +73:02:32.2
12:34:57.46 +72:58:46.6
12:35:39.02 +72:53:08.0
12:44:46.35 +72:39:08.9
12:41:13.20 +72:36:46.7
12:36:28.95 +72:36:52.9
12:42:16.37 +72:34:53.7
12:44:51.41 +72:33:23.2
12:42:25.55 +72:31:09.5
12:41:43.81 +72:29:30.6
12:45:10.51 +72:24:24.9
12:40:30.91 +72:25:31.6
12:43:22.18 +72:26:24.5
12:46:38.71 +72:25:37.5
12:42:16.11 +72:21:54.1
12:47:24.17 +72:23:50.4
12:41:05.79 +72:22:30.0
12:45:22.96 +72:19:08.7
12:43:19.37 +72:16:40.0
12:41:44.17 +72:16:41.2
12:46:21.75 +72:11:05.0
12:36:32.73 +72:11:36.1
12:36:58.03 +72:09:33.1
12:37:37.46 +72:09:48.0
12:46:30.27 +72:08:14.3
12:40:37.33 +72:07:08.2
12:48:12.83 +72:07:10.9
12:36:36.44 +72:03:34.6
12:46:33.76 +72:02:26.0
########### Completed Dra-03-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 ####
12:33:33.89 +73:18:36.3
12:27:06.38 +73:40:43.7
12:46:18.77 +72:18:08.6
12:19:05.94 +66:59:08.9
12:41:43.81 +72:29:30.6
12:47:27.01 +72:18:12.4
12:16:06.82 +73:29:26.2
12:49:26.91 +70:35:39.0
12:35:39.48 +73:23:00.0
12:33:44.00 +73:02:32.2
12:19:19.80 +66:59:07.5
12:46:21.75 +72:11:05.0
12:16:55.88 +73:15:12.8
12:17:52.76 +73:29:22.7
12:27:36.87 +73:50:18.6
12:34:01.41 +73:27:55.3
11:18:56.84 +67:42:46.6
12:33:36.51 +73:09:38.4
12:42:16.37 +72:34:53.7
12:48:46.53 +71:40:17.1
12:12:36.11 +73:30:32.6
12:13:08.91 +73:46:38.1
12:43:22.18 +72:26:24.5
11:19:12.07 +68:16:09.6
12:33:21.13 +73:47:19.0
12:41:14.90 +72:17:54.1
12:42:11.36 +72:31:43.3
12:26:32.48 +72:25:57.6
12:34:01.16 +73:14:03.4
12:19:37.07 +66:59:37.8
12:31:07.67 +73:44:08.9
12:35:39.02 +72:53:08.0
12:44:17.97 +72:28:44.4
12:34:54.20 +73:05:44.5
12:51:58.10 +71:26:32.8
11:16:20.83 +68:23:25.9
12:13:53.60 +73:46:37.5
12:29:31.29 +73:18:12.5
12:23:16.64 +74:08:08.4
12:46:30.27 +72:08:14.3
12:20:46.73 +73:34:16.1
12:18:11.97 +67:18:27.9
12:29:42.57 +73:46:19.6
12:34:53.81 +73:27:17.3
12:46:33.76 +72:02:26.0
12:15:36.06 +67:06:22.6
12:35:42.19 +73:05:12.4
12:34:31.80 +73:48:33.1
12:35:08.19 +72:20:07.5
12:44:46.35 +72:39:08.9
12:45:12.32 +72:31:52.1
12:47:27.35 +70:51:39.9
12:13:16.90 +73:28:57.8
12:34:31.30 +73:02:42.5
11:17:48.09 +68:56:05.5
12:27:31.36 +66:35:33.8
12:35:23.75 +73:36:45.5
12:47:24.17 +72:23:50.4
12:37:37.46 +72:09:48.0
12:41:44.17 +72:16:41.2
11:14:11.70 +68:44:55.5
11:36:43.94 +66:56:50.4
12:18:16.53 +73:09:08.8
12:13:18.15 +73:27:38.0
12:41:13.20 +72:36:46.7
12:22:43.80 +74:08:25.3
11:16:27.10 +68:34:43.3
12:43:19.37 +72:16:40.0
12:13:24.55 +73:43:06.7
12:34:18.61 +73:40:29.7
12:15:44.91 +73:30:29.8
12:45:10.51 +72:24:24.9
12:25:22.18 +74:06:25.1
11:24:38.33 +67:31:06.8
11:17:30.19 +68:06:10.0
12:31:20.66 +73:03:17.8
12:13:55.09 +73:35:56.1
11:38:53.39 +68:47:24.9
12:46:35.90 +70:57:52.2
12:27:08.47 +73:54:09.9
11:41:38.30 +65:51:58.4
12:06:29.03 +74:13:10.6
12:48:12.83 +72:07:10.9
11:25:07.12 +68:30:23.3
12:44:29.56 +72:26:09.8
12:09:04.15 +67:40:37.2
12:24:20.30 +73:48:45.9
12:36:36.44 +72:03:34.6
12:30:10.75 +73:50:40.8
12:29:53.29 +73:53:18.5
12:23:57.52 +66:48:25.8
11:35:08.28 +66:53:29.5
12:14:18.44 +73:33:43.3
12:36:28.95 +72:36:52.9
12:14:15.87 +73:28:53.5
12:19:49.21 +67:01:52.8
12:14:00.83 +67:09:28.6
12:28:29.70 +66:28:10.3
12:28:50.72 +73:52:20.0
12:36:32.73 +72:11:36.1
11:19:42.04 +68:26:58.3
11:26:20.46 +67:56:17.4
12:34:57.46 +72:58:46.6
12:44:51.41 +72:33:23.2
12:35:31.36 +73:12:26.5
12:46:29.17 +72:13:40.8
11:25:52.19 +68:27:05.9
12:33:29.33 +72:54:00.9
12:17:16.47 +67:04:49.4
12:42:25.55 +72:31:09.5
12:41:05.79 +72:22:30.0
12:18:46.30 +67:14:30.9
11:36:31.39 +68:52:57.6
12:33:52.74 +73:43:29.5
12:36:58.03 +72:09:33.1
12:40:30.91 +72:25:31.6
12:42:16.11 +72:21:54.1
12:24:22.55 +74:07:00.6
12:24:12.62 +74:10:38.4
12:32:07.92 +73:42:35.2
12:40:37.33 +72:07:08.2
12:25:40.11 +74:05:57.6
12:46:38.71 +72:25:37.5
12:29:19.35 +73:22:37.8
12:45:22.96 +72:19:08.7
12:36:16.45 +72:18:06.2
12:35:28.75 +73:05:16.0
###################################################################################
12:33:33.89 +73:18:36.3 -- not an asteroid (will add it to exclusion list)
12:27:06.38 +73:40:43.7 -- not an asteroid (will add it to exclusion list)
12:46:18.77 +72:18:08.6 -- not an asteroid (will add it to exclusion list)
12:19:05.94 +66:59:08.9 -- not an asteroid (will add it to exclusion list)
12:41:43.81 +72:29:30.6 -- not an asteroid (will add it to exclusion list)
12:47:27.01 +72:18:12.4 -- not an asteroid (will add it to exclusion list)
12:16:06.82 +73:29:26.2 -- not an asteroid (will add it to exclusion list)
12:49:26.91 +70:35:39.0 -- not an asteroid (will add it to exclusion list)
12:35:39.48 +73:23:00.0 -- not an asteroid (will add it to exclusion list)
12:33:44.00 +73:02:32.2 -- not an asteroid (will add it to exclusion list)
12:19:19.80 +66:59:07.5 -- not an asteroid (will add it to exclusion list)
12:46:21.75 +72:11:05.0 -- not an asteroid (will add it to exclusion list)
12:16:55.88 +73:15:12.8 -- not an asteroid (will add it to exclusion list)
12:17:52.76 +73:29:22.7 -- not an asteroid (will add it to exclusion list)
12:27:36.87 +73:50:18.6 -- not an asteroid (will add it to exclusion list)
12:34:01.41 +73:27:55.3 -- not an asteroid (will add it to exclusion list)
11:18:56.84 +67:42:46.6 -- not an asteroid (will add it to exclusion list)
12:33:36.51 +73:09:38.4 -- not an asteroid (will add it to exclusion list)
12:42:16.37 +72:34:53.7 -- not an asteroid (will add it to exclusion list)
12:48:46.53 +71:40:17.1 -- not an asteroid (will add it to exclusion list)
12:12:36.11 +73:30:32.6 -- not an asteroid (will add it to exclusion list)
12:13:08.91 +73:46:38.1 -- not an asteroid (will add it to exclusion list)
12:43:22.18 +72:26:24.5 -- not an asteroid (will add it to exclusion list)
11:19:12.07 +68:16:09.6 -- not an asteroid (will add it to exclusion list)
12:33:21.13 +73:47:19.0 -- not an asteroid (will add it to exclusion list)
12:41:14.90 +72:17:54.1 -- not an asteroid (will add it to exclusion list)
12:42:11.36 +72:31:43.3 -- not an asteroid (will add it to exclusion list)
12:26:32.48 +72:25:57.6 -- not an asteroid (will add it to exclusion list)
12:34:01.16 +73:14:03.4 -- not an asteroid (will add it to exclusion list)
12:19:37.07 +66:59:37.8 -- not an asteroid (will add it to exclusion list)
12:31:07.67 +73:44:08.9 -- not an asteroid (will add it to exclusion list)
12:35:39.02 +72:53:08.0 -- not an asteroid (will add it to exclusion list)
12:44:17.97 +72:28:44.4 -- not an asteroid (will add it to exclusion list)
12:34:54.20 +73:05:44.5 -- not an asteroid (will add it to exclusion list)
12:51:58.10 +71:26:32.8 -- not an asteroid (will add it to exclusion list)
11:16:20.83 +68:23:25.9 -- not an asteroid (will add it to exclusion list)
12:13:53.60 +73:46:37.5 -- not an asteroid (will add it to exclusion list)
12:29:31.29 +73:18:12.5 -- not an asteroid (will add it to exclusion list)
12:23:16.64 +74:08:08.4 -- not an asteroid (will add it to exclusion list)
12:46:30.27 +72:08:14.3 -- not an asteroid (will add it to exclusion list)
12:20:46.73 +73:34:16.1 -- not an asteroid (will add it to exclusion list)
12:18:11.97 +67:18:27.9 -- not an asteroid (will add it to exclusion list)
12:29:42.57 +73:46:19.6 -- not an asteroid (will add it to exclusion list)
12:34:53.81 +73:27:17.3 -- not an asteroid (will add it to exclusion list)
12:46:33.76 +72:02:26.0 -- not an asteroid (will add it to exclusion list)
12:15:36.06 +67:06:22.6 -- not an asteroid (will add it to exclusion list)
12:35:42.19 +73:05:12.4 -- not an asteroid (will add it to exclusion list)
12:34:31.80 +73:48:33.1 -- not an asteroid (will add it to exclusion list)
12:35:08.19 +72:20:07.5 -- not an asteroid (will add it to exclusion list)
12:44:46.35 +72:39:08.9 -- not an asteroid (will add it to exclusion list)
12:45:12.32 +72:31:52.1 -- not an asteroid (will add it to exclusion list)
12:47:27.35 +70:51:39.9 -- not an asteroid (will add it to exclusion list)
12:13:16.90 +73:28:57.8 -- not an asteroid (will add it to exclusion list)
12:34:31.30 +73:02:42.5 -- not an asteroid (will add it to exclusion list)
11:17:48.09 +68:56:05.5 -- not an asteroid (will add it to exclusion list)
12:27:31.36 +66:35:33.8 -- not an asteroid (will add it to exclusion list)
12:35:23.75 +73:36:45.5 -- not an asteroid (will add it to exclusion list)
12:47:24.17 +72:23:50.4 -- not an asteroid (will add it to exclusion list)
12:37:37.46 +72:09:48.0 -- not an asteroid (will add it to exclusion list)
12:41:44.17 +72:16:41.2 -- not an asteroid (will add it to exclusion list)
11:14:11.70 +68:44:55.5 -- not an asteroid (will add it to exclusion list)
11:36:43.94 +66:56:50.4 -- not an asteroid (will add it to exclusion list)
12:18:16.53 +73:09:08.8 -- not an asteroid (will add it to exclusion list)
12:13:18.15 +73:27:38.0 -- not an asteroid (will add it to exclusion list)
12:41:13.20 +72:36:46.7 -- not an asteroid (will add it to exclusion list)
12:22:43.80 +74:08:25.3 -- not an asteroid (will add it to exclusion list)
11:16:27.10 +68:34:43.3 -- not an asteroid (will add it to exclusion list)
12:43:19.37 +72:16:40.0 -- not an asteroid (will add it to exclusion list)
12:13:24.55 +73:43:06.7 -- not an asteroid (will add it to exclusion list)
12:34:18.61 +73:40:29.7 -- not an asteroid (will add it to exclusion list)
12:15:44.91 +73:30:29.8 -- not an asteroid (will add it to exclusion list)
12:45:10.51 +72:24:24.9 -- not an asteroid (will add it to exclusion list)
12:25:22.18 +74:06:25.1 -- not an asteroid (will add it to exclusion list)
11:24:38.33 +67:31:06.8 -- not an asteroid (will add it to exclusion list)
11:17:30.19 +68:06:10.0 -- not an asteroid (will add it to exclusion list)
12:31:20.66 +73:03:17.8 -- not an asteroid (will add it to exclusion list)
12:13:55.09 +73:35:56.1 -- not an asteroid (will add it to exclusion list)
11:38:53.39 +68:47:24.9 -- not an asteroid (will add it to exclusion list)
12:46:35.90 +70:57:52.2 -- not an asteroid (will add it to exclusion list)
12:27:08.47 +73:54:09.9 -- not an asteroid (will add it to exclusion list)
11:41:38.30 +65:51:58.4 -- not an asteroid (will add it to exclusion list)
12:06:29.03 +74:13:10.6 -- not an asteroid (will add it to exclusion list)
12:48:12.83 +72:07:10.9 -- not an asteroid (will add it to exclusion list)
11:25:07.12 +68:30:23.3 -- not an asteroid (will add it to exclusion list)
12:44:29.56 +72:26:09.8 -- not an asteroid (will add it to exclusion list)
12:09:04.15 +67:40:37.2 -- not an asteroid (will add it to exclusion list)
12:24:20.30 +73:48:45.9 -- not an asteroid (will add it to exclusion list)
12:36:36.44 +72:03:34.6 -- not an asteroid (will add it to exclusion list)
12:30:10.75 +73:50:40.8 -- not an asteroid (will add it to exclusion list)
12:29:53.29 +73:53:18.5 -- not an asteroid (will add it to exclusion list)
12:23:57.52 +66:48:25.8 -- not an asteroid (will add it to exclusion list)
11:35:08.28 +66:53:29.5 -- not an asteroid (will add it to exclusion list)
12:14:18.44 +73:33:43.3 -- not an asteroid (will add it to exclusion list)
12:36:28.95 +72:36:52.9 -- not an asteroid (will add it to exclusion list)
12:14:15.87 +73:28:53.5 -- not an asteroid (will add it to exclusion list)
12:19:49.21 +67:01:52.8 -- not an asteroid (will add it to exclusion list)
12:14:00.83 +67:09:28.6 -- not an asteroid (will add it to exclusion list)
12:28:29.70 +66:28:10.3 -- not an asteroid (will add it to exclusion list)
12:28:50.72 +73:52:20.0 -- not an asteroid (will add it to exclusion list)
12:36:32.73 +72:11:36.1 -- not an asteroid (will add it to exclusion list)
11:19:42.04 +68:26:58.3 -- not an asteroid (will add it to exclusion list)
11:26:20.46 +67:56:17.4 -- not an asteroid (will add it to exclusion list)
12:34:57.46 +72:58:46.6 -- not an asteroid (will add it to exclusion list)
12:44:51.41 +72:33:23.2 -- not an asteroid (will add it to exclusion list)
12:35:31.36 +73:12:26.5 -- not an asteroid (will add it to exclusion list)
12:46:29.17 +72:13:40.8 -- not an asteroid (will add it to exclusion list)
11:25:52.19 +68:27:05.9 -- not an asteroid (will add it to exclusion list)
12:33:29.33 +72:54:00.9 -- not an asteroid (will add it to exclusion list)
12:17:16.47 +67:04:49.4 -- not an asteroid (will add it to exclusion list)
12:42:25.55 +72:31:09.5 -- not an asteroid (will add it to exclusion list)
12:41:05.79 +72:22:30.0 -- not an asteroid (will add it to exclusion list)
12:18:46.30 +67:14:30.9 -- not an asteroid (will add it to exclusion list)
11:36:31.39 +68:52:57.6 -- not an asteroid (will add it to exclusion list)
12:33:52.74 +73:43:29.5 -- not an asteroid (will add it to exclusion list)
12:36:58.03 +72:09:33.1 -- not an asteroid (will add it to exclusion list)
12:40:30.91 +72:25:31.6 -- not an asteroid (will add it to exclusion list)
12:42:16.11 +72:21:54.1 -- not an asteroid (will add it to exclusion list)
12:24:22.55 +74:07:00.6 -- not an asteroid (will add it to exclusion list)
12:24:12.62 +74:10:38.4 -- not an asteroid (will add it to exclusion list)
12:32:07.92 +73:42:35.2 -- not an asteroid (will add it to exclusion list)
12:40:37.33 +72:07:08.2 -- not an asteroid (will add it to exclusion list)
12:25:40.11 +74:05:57.6 -- not an asteroid (will add it to exclusion list)
12:46:38.71 +72:25:37.5 -- not an asteroid (will add it to exclusion list)
12:29:19.35 +73:22:37.8 -- not an asteroid (will add it to exclusion list)
12:45:22.96 +72:19:08.7 -- not an asteroid (will add it to exclusion list)
12:36:16.45 +72:18:06.2 -- not an asteroid (will add it to exclusion list)
12:35:28.75 +73:05:16.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
11:14:11.70 +68:44:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:16:20.83 +68:23:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:16:27.10 +68:34:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:30.19 +68:06:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:48.09 +68:56:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:56.84 +67:42:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:19:12.07 +68:16:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:19:42.04 +68:26:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:24:38.33 +67:31:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:25:07.12 +68:30:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:25:52.19 +68:27:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:26:20.46 +67:56:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:08.28 +66:53:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:31.39 +68:52:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:43.94 +66:56:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:53.39 +68:47:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:41:38.30 +65:51:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:06:29.03 +74:13:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:09:04.15 +67:40:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:12:36.11 +73:30:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:13:08.91 +73:46:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:13:16.90 +73:28:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:13:18.15 +73:27:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:13:24.55 +73:43:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:13:53.60 +73:46:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:13:55.09 +73:35:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:14:00.83 +67:09:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:14:15.87 +73:28:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:14:18.44 +73:33:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:15:36.06 +67:06:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:15:44.91 +73:30:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:16:06.82 +73:29:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:16:55.88 +73:15:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:17:16.47 +67:04:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:17:52.76 +73:29:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:18:11.97 +67:18:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:18:16.53 +73:09:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:18:46.30 +67:14:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:19:05.94 +66:59:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:19:19.80 +66:59:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:19:37.07 +66:59:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:19:49.21 +67:01:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:20:46.73 +73:34:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:22:43.80 +74:08:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:23:16.64 +74:08:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:23:57.52 +66:48:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:24:12.62 +74:10:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:24:20.30 +73:48:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:24:22.55 +74:07:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:25:22.18 +74:06:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:25:40.11 +74:05:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:26:32.48 +72:25:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:27:06.38 +73:40:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:27:08.47 +73:54:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:27:31.36 +66:35:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:27:36.87 +73:50:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:29.70 +66:28:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:28:50.72 +73:52:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:29:19.35 +73:22:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:29:31.29 +73:18:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:29:42.57 +73:46:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:29:53.29 +73:53:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:30:10.75 +73:50:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:31:07.67 +73:44:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:31:20.66 +73:03:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:32:07.92 +73:42:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:21.13 +73:47:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:29.33 +72:54:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:33.89 +73:18:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:36.51 +73:09:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:44.00 +73:02:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:33:52.74 +73:43:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:01.16 +73:14:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:01.41 +73:27:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:18.61 +73:40:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:31.30 +73:02:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:31.80 +73:48:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:53.81 +73:27:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:54.20 +73:05:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:57.46 +72:58:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:08.19 +72:20:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:23.75 +73:36:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:28.75 +73:05:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:31.36 +73:12:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:39.02 +72:53:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:39.48 +73:23:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:35:42.19 +73:05:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:16.45 +72:18:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:28.95 +72:36:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:32.73 +72:11:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:36.44 +72:03:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:58.03 +72:09:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:37:37.46 +72:09:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:30.91 +72:25:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:37.33 +72:07:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:05.79 +72:22:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:13.20 +72:36:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:14.90 +72:17:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:43.81 +72:29:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:44.17 +72:16:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:11.36 +72:31:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:16.11 +72:21:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:16.37 +72:34:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:25.55 +72:31:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:43:19.37 +72:16:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:43:22.18 +72:26:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:17.97 +72:28:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:29.56 +72:26:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:46.35 +72:39:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:51.41 +72:33:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:10.51 +72:24:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:12.32 +72:31:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:22.96 +72:19:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:18.77 +72:18:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:21.75 +72:11:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:29.17 +72:13:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:30.27 +72:08:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:33.76 +72:02:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:35.90 +70:57:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:38.71 +72:25:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:24.17 +72:23:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:27.01 +72:18:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:27.35 +70:51:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:12.83 +72:07:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:46.53 +71:40:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:26.91 +70:35:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:58.10 +71:26:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
11:14:11.70 +68:44:55.5 -- not a known variable star
11:16:20.83 +68:23:25.9 -- not a known variable star
11:16:27.10 +68:34:43.3 -- not a known variable star
11:17:30.19 +68:06:10.0 -- not a known variable star
11:17:48.09 +68:56:05.5 -- not a known variable star
11:18:56.84 +67:42:46.6 -- not a known variable star
11:19:12.07 +68:16:09.6 -- not a known variable star
11:19:42.04 +68:26:58.3 -- not a known variable star
11:24:38.33 +67:31:06.8 -- not a known variable star
11:25:07.12 +68:30:23.3 -- not a known variable star
11:25:52.19 +68:27:05.9 -- not a known variable star
11:26:20.46 +67:56:17.4 -- not a known variable star
11:35:08.28 +66:53:29.5 -- not a known variable star
11:36:31.39 +68:52:57.6 -- not a known variable star
11:36:43.94 +66:56:50.4 -- not a known variable star
11:38:53.39 +68:47:24.9 -- not a known variable star
11:41:38.30 +65:51:58.4 -- not a known variable star
12:06:29.03 +74:13:10.6 -- not a known variable star
12:09:04.15 +67:40:37.2 -- not a known variable star
12:12:36.11 +73:30:32.6 -- not a known variable star
12:13:08.91 +73:46:38.1 -- not a known variable star
12:13:16.90 +73:28:57.8 -- not a known variable star
12:13:18.15 +73:27:38.0 -- not a known variable star
12:13:24.55 +73:43:06.7 -- not a known variable star
12:13:53.60 +73:46:37.5 -- not a known variable star
12:13:55.09 +73:35:56.1 -- a known variable star
12:14:00.83 +67:09:28.6 -- not a known variable star
12:14:15.87 +73:28:53.5 -- not a known variable star
12:14:18.44 +73:33:43.3 -- not a known variable star
12:15:36.06 +67:06:22.6 -- not a known variable star
12:15:44.91 +73:30:29.8 -- not a known variable star
12:16:06.82 +73:29:26.2 -- not a known variable star
12:16:55.88 +73:15:12.8 -- not a known variable star
12:17:16.47 +67:04:49.4 -- not a known variable star
12:17:52.76 +73:29:22.7 -- not a known variable star
12:18:11.97 +67:18:27.9 -- not a known variable star
12:18:16.53 +73:09:08.8 -- not a known variable star
12:18:46.30 +67:14:30.9 -- not a known variable star
12:19:05.94 +66:59:08.9 -- a known variable star
12:19:19.80 +66:59:07.5 -- not a known variable star
12:19:37.07 +66:59:37.8 -- not a known variable star
12:19:49.21 +67:01:52.8 -- not a known variable star
12:20:46.73 +73:34:16.1 -- not a known variable star
12:22:43.80 +74:08:25.3 -- not a known variable star
12:23:16.64 +74:08:08.4 -- not a known variable star
12:23:57.52 +66:48:25.8 -- not a known variable star
12:24:12.62 +74:10:38.4 -- not a known variable star
12:24:20.30 +73:48:45.9 -- not a known variable star
12:24:22.55 +74:07:00.6 -- not a known variable star
12:25:22.18 +74:06:25.1 -- not a known variable star
12:25:40.11 +74:05:57.6 -- not a known variable star
12:26:32.48 +72:25:57.6 -- not a known variable star
12:27:06.38 +73:40:43.7 -- not a known variable star
12:27:08.47 +73:54:09.9 -- not a known variable star
12:27:31.36 +66:35:33.8 -- not a known variable star
12:27:36.87 +73:50:18.6 -- not a known variable star
12:28:29.70 +66:28:10.3 -- not a known variable star
12:28:50.72 +73:52:20.0 -- not a known variable star
12:29:19.35 +73:22:37.8 -- not a known variable star
12:29:31.29 +73:18:12.5 -- not a known variable star
12:29:42.57 +73:46:19.6 -- not a known variable star
12:29:53.29 +73:53:18.5 -- not a known variable star
12:30:10.75 +73:50:40.8 -- not a known variable star
12:31:07.67 +73:44:08.9 -- not a known variable star
12:31:20.66 +73:03:17.8 -- not a known variable star
12:32:07.92 +73:42:35.2 -- not a known variable star
12:33:21.13 +73:47:19.0 -- not a known variable star
12:33:29.33 +72:54:00.9 -- not a known variable star
12:33:33.89 +73:18:36.3 -- not a known variable star
12:33:36.51 +73:09:38.4 -- not a known variable star
12:33:44.00 +73:02:32.2 -- not a known variable star
12:33:52.74 +73:43:29.5 -- not a known variable star
12:34:01.16 +73:14:03.4 -- not a known variable star
12:34:01.41 +73:27:55.3 -- not a known variable star
12:34:18.61 +73:40:29.7 -- not a known variable star
12:34:31.30 +73:02:42.5 -- not a known variable star
12:34:31.80 +73:48:33.1 -- not a known variable star
12:34:53.81 +73:27:17.3 -- not a known variable star
12:34:54.20 +73:05:44.5 -- a known variable star
12:34:57.46 +72:58:46.6 -- not a known variable star
12:35:08.19 +72:20:07.5 -- not a known variable star
12:35:23.75 +73:36:45.5 -- not a known variable star
12:35:28.75 +73:05:16.0 -- not a known variable star
12:35:31.36 +73:12:26.5 -- a known variable star
12:35:39.02 +72:53:08.0 -- not a known variable star
12:35:39.48 +73:23:00.0 -- not a known variable star
12:35:42.19 +73:05:12.4 -- not a known variable star
12:36:16.45 +72:18:06.2 -- not a known variable star
12:36:28.95 +72:36:52.9 -- not a known variable star
12:36:32.73 +72:11:36.1 -- not a known variable star
12:36:36.44 +72:03:34.6 -- a known variable star
12:36:58.03 +72:09:33.1 -- not a known variable star
12:37:37.46 +72:09:48.0 -- not a known variable star
12:40:30.91 +72:25:31.6 -- not a known variable star
12:40:37.33 +72:07:08.2 -- not a known variable star
12:41:05.79 +72:22:30.0 -- not a known variable star
12:41:13.20 +72:36:46.7 -- not a known variable star
12:41:14.90 +72:17:54.1 -- not a known variable star
12:41:43.81 +72:29:30.6 -- not a known variable star
12:41:44.17 +72:16:41.2 -- not a known variable star
12:42:11.36 +72:31:43.3 -- a known variable star
12:42:16.11 +72:21:54.1 -- not a known variable star
12:42:16.37 +72:34:53.7 -- not a known variable star
12:42:25.55 +72:31:09.5 -- not a known variable star
12:43:19.37 +72:16:40.0 -- not a known variable star
12:43:22.18 +72:26:24.5 -- not a known variable star
12:44:17.97 +72:28:44.4 -- not a known variable star
12:44:29.56 +72:26:09.8 -- not a known variable star
12:44:46.35 +72:39:08.9 -- not a known variable star
12:44:51.41 +72:33:23.2 -- not a known variable star
12:45:10.51 +72:24:24.9 -- not a known variable star
12:45:12.32 +72:31:52.1 -- not a known variable star
12:45:22.96 +72:19:08.7 -- not a known variable star
12:46:18.77 +72:18:08.6 -- not a known variable star
12:46:21.75 +72:11:05.0 -- not a known variable star
12:46:29.17 +72:13:40.8 -- not a known variable star
12:46:30.27 +72:08:14.3 -- not a known variable star
12:46:33.76 +72:02:26.0 -- not a known variable star
12:46:35.90 +70:57:52.2 -- not a known variable star
12:46:38.71 +72:25:37.5 -- not a known variable star
12:47:24.17 +72:23:50.4 -- not a known variable star
12:47:27.01 +72:18:12.4 -- not a known variable star
12:47:27.35 +70:51:39.9 -- not a known variable star
12:48:12.83 +72:07:10.9 -- not a known variable star
12:48:46.53 +71:40:17.1 -- not a known variable star
12:49:26.91 +70:35:39.0 -- not a known variable star
12:51:58.10 +71:26:32.8 -- not a known variable star
Found 121 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
127 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 127 (excluding asteroids and hot pixels, 121 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)2461237.85483734 -observatory V36
07:16:34.90 +17:18:11.2 Mercury (4.8mag)
10:36:23.09 +09:58:53.9 Venus (-4.1mag)
04:41:58.39 +22:06:40.9 Mars (1.3mag)
08:22:08.54 +19:53:56.5 Jupiter (-1.8mag)
00:56:23.91 +03:22:06.6 Saturn (0.7mag)
04:08:20.72 +20:48:02.6 Uranus (5.8mag)
00:16:57.74 +00:19:56.3 Neptune (7.7mag)
20:30:21.29 -23:20:39.1 Pluto (14.4mag)
09:31:48.20 +14:47:05.0 Moon (-8.8mag)
-rw-r--r-- 1 apache apache 361 Jul 16 04:20 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461237.85483734:
08:22:08.12 +19:53:57.5 Io (6.0mag)
08:22:00.05 +19:54:29.8 Europa (6.3mag)
08:22:14.56 +19:53:37.9 Ganymede (5.6mag)
08:21:45.42 +19:55:22.1 Callisto (6.8mag)
08:20:24.07 +19:40:45.0 Himalia (15.7mag)
08:22:06.69 +19:54:04.7 Thebe (16.6mag)
08:19:44.84 +19:43:53.4 Elara (17.7mag)
08:25:51.32 +19:44:54.7 Pasiphae (17.9mag)
08:26:45.54 +19:59:55.3 Carme (19.0mag)
00:56:35.83 +03:21:52.3 Titan (8.5mag)
00:56:26.22 +03:21:51.7 Rhea (9.8mag)
00:55:49.12 +03:20:12.7 Iapetus (11.2mag)
00:56:10.53 +03:22:18.0 Hyperion (14.5mag)
00:56:16.60 +03:18:28.0 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 16 04:21 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461237.85483734:
17:54:55.92 -31:34:25.1 JWST
17:42:01.88 +35:10:06.7 Chandra
04:18:06.83 +54:42:35.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 16 04:20 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461237.85483734 -observatory V36
02:44:41.98 +15:07:36.1 17.8mag P/1996 R2 (Lagerkvist)
18:13:28.85 -34:30:29.7 13.8mag P/2010 H2 (Vales)
06:31:40.23 -68:14:43.8 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:02:52.04 +32:33:02.7 17.6mag C/2017 K2 (PANSTARRS)
02:19:17.93 +18:36:25.9 15.7mag P/2021 N1 (ZTF)
22:55:47.12 +32:15:01.0 17.3mag C/2022 E2 (ATLAS)
06:19:11.97 +26:52:05.8 16.7mag C/2022 N2 (PANSTARRS)
10:00:46.98 +29:30:39.2 16.9mag C/2022 QE78 (ATLAS)
09:13:38.03 +05:06:17.1 17.9mag C/2022 R6 (PANSTARRS)
18:03:38.32 +21:02:35.6 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:07.33 -11:32:01.5 17.8mag P/2023 B1 (PANSTARRS)
21:41:46.19 +67:32:12.6 17.8mag C/2023 H5 (Lemmon)
16:19:32.64 -10:42:03.9 14.0mag C/2023 R1 (PANSTARRS)
08:11:11.32 +66:02:20.8 17.9mag C/2024 A1 (ATLAS)
07:40:36.06 +30:18:10.0 14.8mag C/2024 E1 (Wierzchos)
15:13:35.38 +15:28:00.6 17.6mag C/2024 G6 (ATLAS)
19:33:32.12 +40:29:56.9 13.7mag C/2024 J3 (ATLAS)
21:41:06.04 +46:52:26.1 17.8mag C/2024 R4 (PANSTARRS)
04:55:15.66 -13:32:27.3 15.7mag C/2024 T5 (ATLAS)
06:39:29.10 +28:04:02.5 18.0mag C/2025 J1 (Borisov)
07:18:25.66 -13:26:40.8 16.8mag C/2025 R3 (PANSTARRS)
10:03:10.45 +22:10:09.0 17.6mag C/2025 V2 (Rankin)
12:46:45.89 +03:40:05.2 17.1mag C/2025 Y1 (ATLAS)
16:35:43.97 +79:09:29.9 17.2mag C/2026 A2 (Bok)
02:52:21.00 +45:29:27.8 16.8mag C/2026 B2 (Sun-Gao)
11:29:26.99 +05:33:52.8 17.0mag A/2026 E1
21:28:17.73 -17:20:13.6 7.1mag 10P/Tempel
11:16:20.71 -02:09:14.0 16.2mag 29P/Schwassmann-Wachmann
04:08:45.73 +30:11:51.4 17.9mag 47P/Ashbrook-Jackson
10:20:35.99 +12:05:25.2 17.1mag 63P/Wild
00:50:45.19 -05:02:51.5 15.5mag 65P/Gunn
04:41:53.52 +20:27:24.8 13.7mag 78P/Gehrels
02:31:48.21 +11:24:29.8 16.3mag 88P/Howell
06:53:14.95 +30:08:07.6 15.8mag 93P/Lovas
04:40:35.80 +31:18:30.2 16.7mag 114P/Wiseman-Skiff
08:23:21.79 +30:00:20.8 15.2mag 123P/West-Hartley
10:59:23.13 -01:14:52.7 16.9mag 124P/Mrkos
05:01:20.50 +20:58:10.1 16.2mag 128P/Shoemaker-Holt
05:47:31.65 +19:38:47.6 17.8mag 131P/Mueller
00:02:58.67 +03:08:56.0 17.9mag 139P/Vaisala-Oterma
07:35:09.25 +15:41:41.5 16.3mag 141P-D/Machholz
03:19:10.64 -20:37:37.6 15.2mag 161P/Hartley-IRAS
05:54:43.45 +35:09:28.6 15.4mag 162P/SidingSpring
18:46:34.66 +19:03:58.6 14.2mag 169P/NEAT
01:55:11.04 +08:13:52.3 17.6mag 220P/McNaught
16:35:30.08 -08:38:49.4 17.2mag 235P/LINEAR
08:57:52.47 +32:43:51.9 18.0mag 240P/NEAT
20:39:08.60 -50:48:10.3 17.8mag 259P/Garradd
02:16:11.46 +14:54:03.7 15.6mag 260P/McNaught
05:55:30.10 +37:16:33.1 17.4mag 295P/LINEAR
15:06:29.48 +05:30:28.9 17.6mag 391P/Kowalski
08:40:00.93 +19:25:42.1 17.9mag 450P/LONEOS
08:01:09.60 +38:42:51.3 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 16 04:21 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
-rw-r--r-- 1 apache apache 5.6K Jul 16 04:20 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
-rw-r--r-- 1 apache apache 189K Jul 16 04:20 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
18:58:49.786 -21:29:54.27 AT 2026ssv 2026-07-06.26 21.93
21:15:32.626 -21:37:53.76 AT 2026ssu 2026-06-27.33 21.39
22:49:45.273 -15:16:33.71 AT 2026sst 2026-06-27.41 21.88
22:21:22.865 -18:28:38.60 AT 2026sss 2026-06-26.37 22.73
21:48:11.294 -15:58:33.77 AT 2026ssr 2026-06-26.41 21.95
21:56:29.244 -10:33:36.38 AT 2026ssq 2026-06-26.39 22.31
22:04:36.634 -18:37:38.63 AT 2026ssp 2026-06-26.37 22.56
21:52:03.725 -20:04:23.97 AT 2026sso 2026-06-26.39 22.15
22:28:31.768 -14:13:03.02 AT 2026ssn 2026-06-26.40 23.19
22:10:38.868 -20:00:07.81 AT 2026ssm 2026-06-26.37 21.5
00:37:08.843 -05:37:20.31 AT 2026ssl 2026-06-23.58 20.49
16:50:39.367 +12:02:04.48 AT 2026ssk 2026-06-23.30 21.04
21:28:51.588 -30:52:46.37 AT 2026ssj 2026-06-23.54 20.48
13:14:31.067 +38:32:01.92 AT 2026ssi 2026-06-11.32 19.048
00:23:13.025 -04:43:14.99 AT 2026ssh 2026-06-23.58 20.7
21:26:53.186 +04:17:24.51 AT 2026ssg 2026-06-23.48 20.92
22:34:24.397 -29:59:37.51 AT 2026ssf 2026-06-25.56 20.68
22:26:15.310 -27:42:10.55 AT 2026sse 2026-06-25.56 21.41
22:13:00.422 -28:48:04.48 AT 2026ssd 2026-06-25.55 21.47
22:13:31.243 -26:34:31.26 AT 2026ssc 2026-06-25.55 21.32
-rw-r--r-- 1 apache apache 89K Jul 16 04:20 tns_transients_list.txt
