This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov
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 17.2045 2461238.7045 11.66 12:52:33.71 +20:13:00.7
305.12206 83.08383 galactic Com Second-epoch detections are separated by 0.9" and 10.5 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 | 12:52:33.71 +20:13:00.7 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.339+/-0.031 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:33.71 +20:13:00.7: 12.66 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:33.71 +20:13:00.7: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 52 33.71 +20 13 00.7 11.7 U Com 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,2461238.7045,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.95 12:51:45.76 +19:49:09.9
303.53226 82.69079 galactic Com Second-epoch detections are separated by 0.8" and 10.2 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 | 12:51:45.76 +19:49:09.9 (user input) | T | P | (position from user input) J-Ks=0.304+/-0.026 (F)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:45.76 +19:49:09.9: 12.99 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:45.76 +19:49:09.9: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 17.2045* 12 51 45.76 +19 49 09.9 11.9 U Com 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,2461238.7045,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.43 12:51:06.78 +21:10:29.3
302.20166 84.04609 galactic Com Second-epoch detections are separated by 0.4" and 10.4 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 | 12:51:06.78 +21:10:29.3 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.429+/-0.030 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:06.78 +21:10:29.3: 13.56 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:06.78 +21:10:29.3: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 17.2045* 12 51 06.78 +21 10 29.3 12.4 U Com 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,2461238.7045,12.43,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.44 12:53:14.45 +20:50:17.6
306.77141 83.69653 galactic Com Second-epoch detections are separated by 2.3" and 10.6 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 | 12:53:14.45 +20:50:17.6 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.586+/-0.031 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:14.45 +20:50:17.6: 13.38 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:14.45 +20:50:17.6: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 53 14.45 +20 50 17.6 12.4 U Com 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,2461238.7045,12.44,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.32 12:54:37.85 +19:13:02.9
308.39339 82.05534 galactic Com Second-epoch detections are separated by 0.2" and 10.1 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 | 12:54:37.85 +19:13:02.9 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.335+/-0.030 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:54:37.85 +19:13:02.9: 13.38 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:54:37.85 +19:13:02.9: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 54 37.85 +19 13 02.9 12.3 U Com 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,2461238.7045,12.32,0.05,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 20260717.2045 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 17.2045 2461238.7045 11.29 12:51:08.57 +20:51:56.1
302.30002 83.73697 galactic Com Second-epoch detections are separated by 0.8" and 10.4 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 3954726171563804672 | 12:51:08.58 +20:51:56.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.467+/-0.026 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:08.57 +20:51:56.1: 12.22 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:08.57 +20:51:56.1: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 51 08.57 +20 51 56.1 11.3 U Com 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
Gaia DR3 3954726171563804672,2461238.7045,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3954726171563804672 20260717.2045 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.28 12:50:58.44 +20:14:14.8
302.02498 83.10838 galactic Com Second-epoch detections are separated by 0.2" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J192.7440+20.2318 | 12:50:58.44 +20:14:14.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.633+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:58.44 +20:14:14.8: 12.24 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:58.44 +20:14:14.8: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 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 17.2045* 12 50 58.44 +20 14 14.8 11.3 U Com 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
ATO J192.7440+20.2318,2461238.7045,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J192.7440+20.2318 20260717.2045 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.14 12:50:18.76 +21:24:05.9
300.30874 84.26766 galactic Com Second-epoch detections are separated by 0.3" and 10.4 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 | 12:50:18.76 +21:24:05.9 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.581+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:18.76 +21:24:05.9: 13.20 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:18.76 +21:24:05.9: 13.30 +/- 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!
TCP 2026 07 17.2045* 12 50 18.76 +21 24 05.9 12.1 U Com 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,2461238.7045,12.14,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.19 12:48:52.96 +21:47:58.3
296.56981 84.63968 galactic Com Second-epoch detections are separated by 1.2" and 10.1 pix
The object was found in VSX 1" Gaia DR3 3955044518835321600
Type: ROT
# Max. Min./Amp. JD0 Period
12.920 G 12.940 G K
The object was not found in astcheck.
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:48:52.96 +21:47:58.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:48:52.96 +21:47:58.3: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 48 52.96 +21 47 58.3 12.2 U Com 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
Gaia DR3 3955044518835321600,2461238.7045,12.19,0.05,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
Gaia DR3 3955044518835321600 20260717.2045 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 17.2045 2461238.7045 12.15 12:38:54.13 +24:53:08.4
250.76273 86.39996 galactic Com Second-epoch detections are separated by 0.2" and 9.9 pix
The object was found in VSX 1" ASAS J123854+2453.2
Type: RRAB
# Max. Min./Amp. JD0 Period
12.880 V 13.250 V 2453471.33120 0.628353000000
The object was not found in astcheck.
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:38:54.13 +24:53:08.4: 13.20 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:38:54.13 +24:53:08.4: 13.13 +/- 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!
TCP 2026 07 17.2045* 12 38 54.13 +24 53 08.4 12.2 U Com 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
ASAS J123854+2453.2,2461238.7045,12.15,0.05,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
ASAS J123854+2453.2 20260717.2045 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 17.2045 2461238.7045 12.27 12:49:39.84 +20:28:04.9
299.35389 83.32745 galactic Com Second-epoch detections are separated by 1.0" and 10.3 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 | 12:49:39.84 +20:28:04.9 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.604+/-0.031 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:39.84 +20:28:04.9: 13.19 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:39.84 +20:28:04.9: 13.28 +/- 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!
TCP 2026 07 17.2045* 12 49 39.84 +20 28 04.9 12.3 U Com 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,2461238.7045,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.17 12:49:11.89 +21:58:00.2
297.17795 84.81343 galactic Com Second-epoch detections are separated by 1.7" and 10.0 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 | 12:49:11.89 +21:58:00.2 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.509+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:11.89 +21:58:00.2: 13.19 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:11.89 +21:58:00.2: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 49 11.89 +21 58 00.2 12.2 U Com 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,2461238.7045,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.96 12:51:14.80 +20:05:21.2
302.56549 82.96083 galactic Com Second-epoch detections are separated by 0.6" and 10.3 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 | 12:51:14.80 +20:05:21.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.572+/-0.028 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:14.80 +20:05:21.2: 13.16 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:14.80 +20:05:21.2: 13.16 +/- 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!
TCP 2026 07 17.2045* 12 51 14.80 +20 05 21.2 12.0 U Com 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,2461238.7045,11.96,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.54 13:06:34.11 +24:52:08.1
0.16715 85.91830 galactic Com Second-epoch detections are separated by 1.6" and 10.6 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 | 13:06:34.11 +24:52:08.1 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.268+/-0.033 (F)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 13:06:34.11 +24:52:08.1: 13.43 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 13:06:34.11 +24:52:08.1: 13.56 +/- 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!
TCP 2026 07 17.2045* 13 06 34.11 +24 52 08.1 12.5 U Com 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,2461238.7045,12.54,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.44 12:48:23.71 +22:22:11.9
294.50945 85.19188 galactic Com Second-epoch detections are separated by 0.4" and 10.1 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 | 12:48:23.71 +22:22:11.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:48:23.71 +22:22:11.9: 13.48 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:48:23.71 +22:22:11.9: 13.46 +/- 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!
TCP 2026 07 17.2045* 12 48 23.71 +22 22 11.9 12.4 U Com 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,2461238.7045,12.44,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.55 12:51:36.23 +20:09:59.6
303.25314 83.03820 galactic Com Second-epoch detections are separated by 2.9" and 10.8 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 | 12:51:36.23 +20:09:59.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.404+/-0.035 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:36.23 +20:09:59.6: 13.94 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:36.23 +20:09:59.6: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.99 +/- 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!
TCP 2026 07 17.2045* 12 51 36.23 +20 09 59.6 12.6 U Com 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,2461238.7045,12.55,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.65 12:50:15.53 +20:58:02.1
300.36877 83.83313 galactic Com Second-epoch detections are separated by 1.7" and 10.1 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 | 12:50:15.53 +20:58:02.1 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:15.53 +20:58:02.1: 13.99 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:15.53 +20:58:02.1: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 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!
TCP 2026 07 17.2045* 12 50 15.53 +20 58 02.1 12.7 U Com 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,2461238.7045,12.65,0.05,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 20260717.2045 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 17.2045 2461238.7045 11.63 12:49:44.58 +20:32:20.4
299.47790 83.39938 galactic Com Second-epoch detections are separated by 0.3" and 10.3 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 3942329143600877440 | 12:49:44.58 +20:32:20.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.442+/-0.030 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:44.58 +20:32:20.4: 12.61 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:44.58 +20:32:20.4: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 49 44.58 +20 32 20.4 11.6 U Com 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
Gaia DR3 3942329143600877440,2461238.7045,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3942329143600877440 20260717.2045 11.63CV 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 17.2045 2461238.7045 12.06 12:48:56.74 +21:03:48.1
297.44441 83.90854 galactic Com Second-epoch detections are separated by 1.1" and 10.2 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 | 12:48:56.74 +21:03:48.1 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.496+/-0.032 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:48:56.74 +21:03:48.1: 13.18 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:48:56.74 +21:03:48.1: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 48 56.74 +21 03 48.1 12.1 U Com 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,2461238.7045,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.89 12:51:41.68 +20:06:45.2
303.42536 82.98406 galactic Com Second-epoch detections are separated by 1.1" and 10.5 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 | 12:51:41.68 +20:06:45.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.286+/-0.034 (F)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:41.68 +20:06:45.2: 12.95 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:41.68 +20:06:45.2: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 17.2045* 12 51 41.68 +20 06 45.2 11.9 U Com 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,2461238.7045,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.32 12:51:13.10 +20:05:07.2
302.51142 82.95690 galactic Com Second-epoch detections are separated by 0.9" and 10.2 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 | 12:51:13.10 +20:05:07.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.408+/-0.030 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:13.10 +20:05:07.2: 13.42 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:13.10 +20:05:07.2: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 51 13.10 +20 05 07.2 12.3 U Com 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,2461238.7045,12.32,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.04 12:50:51.57 +20:16:35.4
301.79506 83.14697 galactic Com Second-epoch detections are separated by 0.5" and 10.3 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 | 12:50:51.57 +20:16:35.4 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.630+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:51.57 +20:16:35.4: 13.15 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:51.57 +20:16:35.4: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 50 51.57 +20 16 35.4 12.0 U Com 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,2461238.7045,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.14 12:49:46.52 +21:56:29.6
298.67452 84.79956 galactic Com Second-epoch detections are separated by 2.4" and 9.7 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 | 12:49:46.52 +21:56:29.6 (user input) | T | P | (position from user input) SpType: F4 (LAMOST DR5) J-Ks=0.385+/-0.029 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:46.52 +21:56:29.6: 13.15 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:46.52 +21:56:29.6: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 49 46.52 +21 56 29.6 12.1 U Com 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,2461238.7045,12.14,0.05,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 20260717.2045 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 17.2045 2461238.7045 11.85 12:51:26.79 +20:30:16.5
302.94933 83.37633 galactic Com Second-epoch detections are separated by 0.6" and 10.4 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 | 12:51:26.79 +20:30:16.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.510+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:26.79 +20:30:16.5: 12.94 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:26.79 +20:30:16.5: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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 17.2045* 12 51 26.79 +20 30 16.5 11.8 U Com 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,2461238.7045,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.37 12:50:18.68 +20:27:41.4
300.66006 83.32828 galactic Com Second-epoch detections are separated by 1.1" and 10.4 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 | 12:50:18.68 +20:27:41.4 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.033 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:18.68 +20:27:41.4: 13.69 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:18.68 +20:27:41.4: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 17.2045* 12 50 18.68 +20 27 41.4 12.4 U Com 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,2461238.7045,12.37,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.21 12:43:55.04 +23:38:19.7
276.56674 86.11927 galactic Com Second-epoch detections are separated by 0.8" and 10.1 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 | 12:43:55.04 +23:38:19.7 (user input) | T | P | (position from user input) J-Ks=0.355+/-0.034 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:43:55.04 +23:38:19.7: 13.13 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:43:55.04 +23:38:19.7: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 43 55.04 +23 38 19.7 12.2 U Com 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,2461238.7045,12.21,0.05,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 20260717.2045 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 17.2045 2461238.7045 11.96 12:49:36.75 +20:55:44.9
298.99038 83.78691 galactic Com Second-epoch detections are separated by 1.8" and 10.7 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 | 12:49:36.75 +20:55:44.9 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.583+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:36.75 +20:55:44.9: 13.12 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:36.75 +20:55:44.9: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 49 36.75 +20 55 44.9 12.0 U Com 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,2461238.7045,11.96,0.05,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 20260717.2045 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 17.2045 2461238.7045 11.74 12:49:39.43 +20:53:52.5
299.10490 83.75643 galactic Com Second-epoch detections are separated by 0.9" and 10.3 pix
The object was found in VSX15" Gaia DR3 3954365810923372288
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.760 G M
The object was not found in astcheck.
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:39.43 +20:53:52.5: 12.89 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:39.43 +20:53:52.5: 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!
TCP 2026 07 17.2045* 12 49 39.43 +20 53 52.5 11.7 U Com 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
Gaia DR3 3954365810923372288,2461238.7045,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3954365810923372288 20260717.2045 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.48 12:49:33.90 +21:30:36.4
298.49051 84.36570 galactic Com Second-epoch detections are separated by 1.2" and 10.2 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 | 12:49:33.90 +21:30:36.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.535+/-0.028 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:33.90 +21:30:36.4: 13.62 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:33.90 +21:30:36.4: 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!
TCP 2026 07 17.2045* 12 49 33.90 +21 30 36.4 12.5 U Com 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,2461238.7045,12.48,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.37 12:52:26.94 +20:45:40.2
305.06230 83.62873 galactic Com Second-epoch detections are separated by 0.5" and 10.4 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 | 12:52:26.94 +20:45:40.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.405+/-0.032 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:26.94 +20:45:40.2: 13.40 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:26.94 +20:45:40.2: 13.34 +/- 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 17.2045* 12 52 26.94 +20 45 40.2 12.4 U Com 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,2461238.7045,12.37,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.02 12:50:26.09 +20:21:57.8
300.93607 83.23392 galactic Com Second-epoch detections are separated by 0.7" and 10.3 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 | 12:50:26.09 +20:21:57.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.328+/-0.033 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:26.09 +20:21:57.8: 13.12 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:26.09 +20:21:57.8: 13.07 +/- 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!
TCP 2026 07 17.2045* 12 50 26.09 +20 21 57.8 12.0 U Com 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,2461238.7045,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.91 12:49:46.18 +21:01:04.4
299.27904 83.87780 galactic Com Second-epoch detections are separated by 1.0" and 10.2 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 | 12:49:46.18 +21:01:04.4 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:46.18 +21:01:04.4: 13.11 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:46.18 +21:01:04.4: 13.08 +/- 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!
TCP 2026 07 17.2045* 12 49 46.18 +21 01 04.4 11.9 U Com 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,2461238.7045,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.54 12:51:26.48 +20:25:58.2
302.93877 83.30458 galactic Com Second-epoch detections are separated by 2.4" and 10.7 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 | 12:51:26.48 +20:25:58.2 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.257+/-0.033 (F)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:26.48 +20:25:58.2: 13.83 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:26.48 +20:25:58.2: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 17.2045* 12 51 26.48 +20 25 58.2 12.5 U Com 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,2461238.7045,12.54,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.43 12:49:45.46 +20:45:33.2
299.39523 83.61943 galactic Com Second-epoch detections are separated by 1.1" and 10.3 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 | 12:49:45.46 +20:45:33.2 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.484+/-0.035 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:45.46 +20:45:33.2: 13.83 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:45.46 +20:45:33.2: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 17.2045* 12 49 45.46 +20 45 33.2 12.4 U Com 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,2461238.7045,12.43,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.27 12:50:53.96 +20:04:53.4
301.90119 82.95217 galactic Com Second-epoch detections are separated by 1.0" and 10.5 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 | 12:50:53.96 +20:04:53.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.405+/-0.033 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:53.96 +20:04:53.4: 13.41 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:53.96 +20:04:53.4: 13.45 +/- 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!
TCP 2026 07 17.2045* 12 50 53.96 +20 04 53.4 12.3 U Com 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,2461238.7045,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.04 12:39:02.50 +24:52:48.3
251.15234 86.42087 galactic Com Second-epoch detections are separated by 3.0" and 9.5 pix
The object was found in VSX 1" Gaia DR3 3959669030382271488
Type: ROT
# Max. Min./Amp. JD0 Period
12.640 G 12.660 G G
The object was not found in astcheck.
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:39:02.50 +24:52:48.3: 12.86 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:39:02.50 +24:52:48.3: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 17.2045* 12 39 02.50 +24 52 48.3 12.0 U Com 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
Gaia DR3 3959669030382271488,2461238.7045,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3959669030382271488 20260717.2045 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.41 12:52:42.13 +20:16:36.8
305.41572 83.14254 galactic Com Second-epoch detections are separated by 0.9" and 10.5 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 | 12:52:42.13 +20:16:36.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.421+/-0.033 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:42.13 +20:16:36.8: 13.61 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:42.13 +20:16:36.8: 13.58 +/- 0.03 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!
TCP 2026 07 17.2045* 12 52 42.13 +20 16 36.8 12.4 U Com 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,2461238.7045,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.50 12:53:01.00 +19:44:50.1
305.82128 82.61014 galactic Com Second-epoch detections are separated by 0.6" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3942041969203671424 | 12:53:01.04 +19:44:50.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.301+/-0.030 (F)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:01.00 +19:44:50.1: 12.53 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:01.00 +19:44:50.1: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 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 17.2045* 12 53 01.00 +19 44 50.1 11.5 U Com 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
Gaia DR3 3942041969203671424,2461238.7045,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 3942041969203671424 20260717.2045 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.09 12:53:10.69 +19:21:09.8
305.96334 82.21423 galactic Com Second-epoch detections are separated by 1.0" and 10.0 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 | 12:53:10.69 +19:21:09.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:10.69 +19:21:09.8: 13.12 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:10.69 +19:21:09.8: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 53 10.69 +19 21 09.8 12.1 U Com 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,2461238.7045,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260717.2045 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 17.2045 2461238.7045 12.10 12:52:00.15 +20:31:44.3
304.08193 83.39946 galactic Com Second-epoch detections are separated by 2.1" and 10.7 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 | 12:52:00.15 +20:31:44.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.357+/-0.028 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:00.15 +20:31:44.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:00.15 +20:31:44.3: 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!
TCP 2026 07 17.2045* 12 52 00.15 +20 31 44.3 12.1 U Com 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,2461238.7045,12.10,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.49 12:51:54.21 +20:15:58.7
303.84573 83.13723 galactic Com Second-epoch detections are separated by 1.8" and 10.4 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 | 12:51:54.21 +20:15:58.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.443+/-0.035 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:54.21 +20:15:58.7: 13.82 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:54.21 +20:15:58.7: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 17.2045* 12 51 54.21 +20 15 58.7 12.5 U Com 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,2461238.7045,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.54 12:50:05.81 +21:27:46.0
299.77422 84.32630 galactic Com Second-epoch detections are separated by 0.6" and 10.4 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 | 12:50:05.81 +21:27:46.0 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.587+/-0.033 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:05.81 +21:27:46.0: 13.79 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:05.81 +21:27:46.0: 13.81 +/- 0.04 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!
TCP 2026 07 17.2045* 12 50 05.81 +21 27 46.0 12.5 U Com 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,2461238.7045,12.54,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.56 13:07:44.04 +24:38:42.1
359.71711 85.57330 galactic Com Second-epoch detections are separated by 4.1" and 11.0 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 | 13:07:44.04 +24:38:42.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.398+/-0.038 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 13:07:44.04 +24:38:42.1: 13.59 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 13:07:44.04 +24:38:42.1: 13.56 +/- 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!
TCP 2026 07 17.2045* 13 07 44.04 +24 38 42.1 12.6 U Com 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,2461238.7045,12.56,0.05,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 20260717.2045 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 17.2045 2461238.7045 11.71 12:50:10.27 +20:36:53.1
300.32059 83.48007 galactic Com Second-epoch detections are separated by 0.7" and 10.4 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 | 12:50:10.27 +20:36:53.1 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.563+/-0.029 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:10.27 +20:36:53.1: 12.86 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:10.27 +20:36:53.1: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 17.2045* 12 50 10.27 +20 36 53.1 11.7 U Com 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,2461238.7045,11.71,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.54 12:52:36.32 +21:07:15.0
305.53157 83.98669 galactic Com Second-epoch detections are separated by 2.1" and 10.3 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 | 12:52:36.32 +21:07:15.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:36.32 +21:07:15.0: 13.63 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:36.32 +21:07:15.0: 13.68 +/- 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 17.2045* 12 52 36.32 +21 07 15.0 12.5 U Com 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,2461238.7045,12.54,0.05,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 20260717.2045 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 17.2045 2461238.7045 11.89 12:52:48.81 +20:42:44.2
305.80824 83.57634 galactic Com Second-epoch detections are separated by 0.8" and 10.2 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 | 12:52:48.81 +20:42:44.2 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.621+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:48.81 +20:42:44.2: 12.83 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:48.81 +20:42:44.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 17.2045* 12 52 48.81 +20 42 44.2 11.9 U Com 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,2461238.7045,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 10.80 12:48:57.80 +21:11:53.7
297.36538 84.04323 galactic Com Second-epoch detections are separated by 0.8" and 10.4 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 3954798434389021568 | 12:48:57.75 +21:11:54.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.408+/-0.032 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:48:57.80 +21:11:53.7: 11.73 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:48:57.80 +21:11:53.7: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 48 57.80 +21 11 53.7 10.8 U Com 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
Gaia DR3 3954798434389021568,2461238.7045,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3954798434389021568 20260717.2045 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.80 12:49:06.69 +20:47:18.9
298.01891 83.63813 galactic Com Second-epoch detections are separated by 0.2" and 10.3 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 | 12:49:06.69 +20:47:18.9 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.362+/-0.032 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:06.69 +20:47:18.9: 12.82 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:06.69 +20:47:18.9: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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 17.2045* 12 49 06.69 +20 47 18.9 11.8 U Com 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,2461238.7045,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.02 12:50:14.19 +20:16:06.9
300.57412 83.13483 galactic Com Second-epoch detections are separated by 1.1" and 10.4 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 3942309459766630016 | 12:50:13.69 +20:16:42.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.579+/-0.031 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:14.19 +20:16:06.9: 13.02 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:14.19 +20:16:06.9: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 50 14.19 +20 16 06.9 12.0 U Com 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
Gaia DR3 3942309459766630016,2461238.7045,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3942309459766630016 20260717.2045 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.39 12:51:30.09 +20:07:19.7
303.05427 82.99387 galactic Com Second-epoch detections are separated by 1.6" and 10.6 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 | 12:51:30.09 +20:07:19.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.361+/-0.029 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:30.09 +20:07:19.7: 13.60 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:30.09 +20:07:19.7: 13.64 +/- 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!
TCP 2026 07 17.2045* 12 51 30.09 +20 07 19.7 12.4 U Com 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,2461238.7045,12.39,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.40 12:52:58.90 +20:33:36.0
306.08802 83.42229 galactic Com Second-epoch detections are separated by 0.0" and 10.4 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 | 12:52:58.90 +20:33:36.0 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.553+/-0.035 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:58.90 +20:33:36.0: 13.58 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:58.90 +20:33:36.0: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 52 58.90 +20 33 36.0 12.4 U Com 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,2461238.7045,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.02 12:50:18.75 +20:23:04.4
300.68704 83.25140 galactic Com Second-epoch detections are separated by 0.5" and 10.4 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 | 12:50:18.75 +20:23:04.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.304+/-0.033 (F)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:18.75 +20:23:04.4: 13.07 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:18.75 +20:23:04.4: 13.10 +/- 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 17.2045* 12 50 18.75 +20 23 04.4 12.0 U Com 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,2461238.7045,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.52 12:49:14.27 +20:43:44.3
298.32572 83.58104 galactic Com Second-epoch detections are separated by 0.9" and 10.4 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 | 12:49:14.27 +20:43:44.3 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.651+/-0.036 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:14.27 +20:43:44.3: 13.91 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:14.27 +20:43:44.3: 13.88 +/- 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!
TCP 2026 07 17.2045* 12 49 14.27 +20 43 44.3 12.5 U Com 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,2461238.7045,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260717.2045 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 17.2045 2461238.7045 11.73 12:52:07.73 +20:00:42.7
304.24178 82.88185 galactic Com Second-epoch detections are separated by 0.5" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J193.0322+20.0118 | 12:52:07.73 +20:00:42.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.386+/-0.030 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:07.73 +20:00:42.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:07.73 +20:00:42.7: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 52 07.73 +20 00 42.7 11.7 U Com 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
ATO J193.0322+20.0118,2461238.7045,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J193.0322+20.0118 20260717.2045 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.90 12:50:16.66 +20:45:21.9
300.48940 83.62233 galactic Com Second-epoch detections are separated by 0.8" and 10.5 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 | 12:50:16.66 +20:45:21.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.374+/-0.029 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:16.66 +20:45:21.9: 13.06 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:16.66 +20:45:21.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 50 16.66 +20 45 21.9 11.9 U Com 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,2461238.7045,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.78 12:45:16.05 +23:06:47.0
283.41914 85.74897 galactic Com Second-epoch detections are separated by 2.2" and 10.3 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 | 12:45:16.05 +23:06:47.0 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.033 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:45:16.05 +23:06:47.0: 14.36 +/- 0.07 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:45:16.05 +23:06:47.0: 14.21 +/- 0.06 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!
TCP 2026 07 17.2045* 12 45 16.05 +23 06 47.0 12.8 U Com 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,2461238.7045,12.78,0.05,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
target 20260717.2045 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 17.2045 2461238.7045 12.49 12:50:08.39 +20:21:20.6
300.35350 83.22097 galactic Com Second-epoch detections are separated by 2.5" and 10.7 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 | 12:50:08.39 +20:21:20.6 (user input) | T | P | (position from user input) SpType: M2 (LAMOST DR5) J-Ks=0.345+/-0.034 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:08.39 +20:21:20.6: 13.77 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:08.39 +20:21:20.6: 13.74 +/- 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!
TCP 2026 07 17.2045* 12 50 08.39 +20 21 20.6 12.5 U Com 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,2461238.7045,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.64 12:50:51.80 +21:28:40.0
301.57451 84.34801 galactic Com Second-epoch detections are separated by 0.6" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J192.7147+21.4765 | 12:50:51.80 +21:28:40.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.473+/-0.042 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:51.80 +21:28:40.0: 13.75 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:51.80 +21:28:40.0: 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!
TCP 2026 07 17.2045* 12 50 51.80 +21 28 40.0 12.6 U Com 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
ATO J192.7147+21.4765,2461238.7045,12.64,0.05,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
ATO J192.7147+21.4765 20260717.2045 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 17.2045 2461238.7045 12.65 12:49:44.32 +22:08:10.5
298.41858 84.99310 galactic Com Second-epoch detections are separated by 1.6" and 10.3 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 | 12:49:44.32 +22:08:10.5 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.384+/-0.029 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:44.32 +22:08:10.5: 13.75 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:44.32 +22:08:10.5: 13.73 +/- 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!
TCP 2026 07 17.2045* 12 49 44.32 +22 08 10.5 12.7 U Com 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,2461238.7045,12.65,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.18 12:51:24.98 +20:38:05.0
302.88725 83.50647 galactic Com Second-epoch detections are separated by 1.8" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J192.8542+20.6347 | 12:51:24.98 +20:38:05.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.396+/-0.032 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:24.98 +20:38:05.0: 13.35 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:24.98 +20:38:05.0: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 51 24.98 +20 38 05.0 12.2 U Com 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
ATO J192.8542+20.6347,2461238.7045,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J192.8542+20.6347 20260717.2045 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.18 12:49:13.72 +20:39:33.5
298.35391 83.51141 galactic Com Second-epoch detections are separated by 0.8" and 10.2 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 | 12:49:13.72 +20:39:33.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.312+/-0.034 (F)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:13.72 +20:39:33.5: 13.33 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:13.72 +20:39:33.5: 13.29 +/- 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 17.2045* 12 49 13.72 +20 39 33.5 12.2 U Com 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,2461238.7045,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.49 12:50:15.70 +20:59:25.3
300.36574 83.85625 galactic Com Second-epoch detections are separated by 0.2" and 10.3 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 | 12:50:15.70 +20:59:25.3 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.466+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:15.70 +20:59:25.3: 13.74 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:15.70 +20:59:25.3: 13.59 +/- 0.03 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!
TCP 2026 07 17.2045* 12 50 15.70 +20 59 25.3 12.5 U Com 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,2461238.7045,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.60 12:47:09.13 +23:00:58.2
289.42239 85.77503 galactic Com Second-epoch detections are separated by 1.3" and 10.0 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 | 12:47:09.13 +23:00:58.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.338+/-0.031 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:09.13 +23:00:58.2: 13.71 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:09.13 +23:00:58.2: 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!
TCP 2026 07 17.2045* 12 47 09.13 +23 00 58.2 12.6 U Com 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,2461238.7045,12.60,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.10 12:51:05.67 +19:49:15.6
302.29691 82.69233 galactic Com Second-epoch detections are separated by 0.9" and 10.4 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 | 12:51:05.67 +19:49:15.6 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.036 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:05.67 +19:49:15.6: 13.05 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:05.67 +19:49:15.6: 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!
TCP 2026 07 17.2045* 12 51 05.67 +19 49 15.6 12.1 U Com 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,2461238.7045,12.10,0.05,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 20260717.2045 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 17.2045 2461238.7045 11.84 12:47:48.60 +22:16:38.1
293.09906 85.07958 galactic Com Second-epoch detections are separated by 0.4" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J191.9629+22.2833 | 12:47:48.60 +22:16:38.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A6IV (LAMOST DR5) J-Ks=0.096+/-0.032 (A)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:48.60 +22:16:38.1: 12.78 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:48.60 +22:16:38.1: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 17.2045* 12 47 48.60 +22 16 38.1 11.8 U Com 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
ATO J191.9629+22.2833,2461238.7045,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J191.9629+22.2833 20260717.2045 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.36 12:47:55.77 +22:08:26.8
293.66373 84.94927 galactic Com Second-epoch detections are separated by 1.2" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3955112276239366016 | 12:47:55.77 +22:08:26.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: K7 (LAMOST DR5) J-Ks=0.832+/-0.038 (M)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:55.77 +22:08:26.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:55.77 +22:08:26.8: 13.46 +/- 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!
TCP 2026 07 17.2045* 12 47 55.77 +22 08 26.8 12.4 U Com 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
Large-amplitude variable Gaia DR2 3955112276239366016,2461238.7045,12.36,0.05,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
Large-amplitude variable Gaia DR2 3955112276239366016 20260717.2045 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 17.2045 2461238.7045 12.74 12:48:39.38 +21:04:26.5
296.80138 83.91264 galactic Com Second-epoch detections are separated by 4.4" and 11.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:48:39.38 +21:04:26.5 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:48:39.38 +21:04:26.5: 14.04 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:48:39.38 +21:04:26.5: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 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!
TCP 2026 07 17.2045* 12 48 39.38 +21 04 26.5 12.7 U Com 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,2461238.7045,12.74,0.05,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 20260717.2045 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 17.2045 2461238.7045 10.99 12:50:47.02 +20:39:55.3
301.57252 83.53538 galactic Com Second-epoch detections are separated by 0.7" and 10.3 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 3942337188075120000 | 12:50:47.09 +20:39:55.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:47.02 +20:39:55.3: 11.92 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:47.02 +20:39:55.3: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 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 17.2045* 12 50 47.02 +20 39 55.3 11.0 U Com 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
Gaia DR3 3942337188075120000,2461238.7045,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3942337188075120000 20260717.2045 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.08 12:50:59.65 +20:23:34.6
302.04536 83.26393 galactic Com Second-epoch detections are separated by 0.3" and 10.4 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 | 12:50:59.65 +20:23:34.6 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.742+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:59.65 +20:23:34.6: 13.33 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:59.65 +20:23:34.6: 13.35 +/- 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!
TCP 2026 07 17.2045* 12 50 59.65 +20 23 34.6 12.1 U Com 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,2461238.7045,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.49 12:47:29.62 +22:06:17.0
292.60502 84.89720 galactic Com Second-epoch detections are separated by 0.7" and 10.1 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 | 12:47:29.62 +22:06:17.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.346+/-0.037 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:29.62 +22:06:17.0: 13.72 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:29.62 +22:06:17.0: 13.82 +/- 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!
TCP 2026 07 17.2045* 12 47 29.62 +22 06 17.0 12.5 U Com 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,2461238.7045,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.11 12:47:32.49 +22:18:54.9
292.30778 85.10642 galactic Com Second-epoch detections are separated by 0.4" and 10.0 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 | 12:47:32.49 +22:18:54.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.389+/-0.030 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:32.49 +22:18:54.9: 13.05 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:32.49 +22:18:54.9: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 47 32.49 +22 18 54.9 12.1 U Com 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,2461238.7045,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.09 12:46:51.86 +22:48:12.6
289.20851 85.55286 galactic Com Second-epoch detections are separated by 0.9" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J191.7080+22.7977 | 12:46:51.86 +22:48:12.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.485+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:46:51.86 +22:48:12.6: 13.01 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:46:51.86 +22:48:12.6: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 17.2045* 12 46 51.86 +22 48 12.6 12.1 U Com 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
ATO J191.7080+22.7977,2461238.7045,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J191.7080+22.7977 20260717.2045 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 17.2045 2461238.7045 12.02 12:53:24.57 +19:30:11.8
306.42948 82.36163 galactic Com Second-epoch detections are separated by 0.2" and 10.2 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 | 12:53:24.57 +19:30:11.8 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.311+/-0.028 (F)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:24.57 +19:30:11.8: 13.02 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:24.57 +19:30:11.8: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 53 24.57 +19 30 11.8 12.0 U Com 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,2461238.7045,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.92 12:51:24.09 +20:07:43.3
302.86176 83.00044 galactic Com Second-epoch detections are separated by 0.7" and 10.2 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 | 12:51:24.09 +20:07:43.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.452+/-0.031 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:24.09 +20:07:43.3: 12.99 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:24.09 +20:07:43.3: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 17.2045* 12 51 24.09 +20 07 43.3 11.9 U Com 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,2461238.7045,11.92,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.01 12:54:01.46 +19:31:33.3
307.52932 82.37457 galactic Com Second-epoch detections are separated by 0.9" and 10.2 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 | 12:54:01.46 +19:31:33.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.480+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:54:01.46 +19:31:33.3: 13.03 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:54:01.46 +19:31:33.3: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 54 01.46 +19 31 33.3 12.0 U Com 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,2461238.7045,12.01,0.05,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 20260717.2045 12.01CV 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 17.2045 2461238.7045 11.73 12:49:47.66 +20:58:24.2
299.35771 83.83373 galactic Com Second-epoch detections are separated by 0.2" and 10.3 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 | 12:49:47.66 +20:58:24.2 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.520+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:47.66 +20:58:24.2: 12.74 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:47.66 +20:58:24.2: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 49 47.66 +20 58 24.2 11.7 U Com 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,2461238.7045,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.85 12:44:37.29 +23:21:45.5
280.30288 85.93132 galactic Com Second-epoch detections are separated by 1.0" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:44:37.29 +23:21:45.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.366+/-0.032 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:44:37.29 +23:21:45.5: 12.70 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:44:37.29 +23:21:45.5: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 17.2045* 12 44 37.29 +23 21 45.5 11.8 U Com 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,2461238.7045,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.65 12:50:23.91 +20:54:06.5
300.69473 83.76904 galactic Com Second-epoch detections are separated by 0.4" and 10.3 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 | 12:50:23.91 +20:54:06.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.438+/-0.027 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:23.91 +20:54:06.5: 12.71 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:23.91 +20:54:06.5: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 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 17.2045* 12 50 23.91 +20 54 06.5 11.7 U Com 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,2461238.7045,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.79 12:49:03.95 +20:31:37.8
298.11130 83.37670 galactic Com Second-epoch detections are separated by 0.5" and 10.4 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 3954337940879977856 | 12:49:03.93 +20:31:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.620+/-0.033 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:03.95 +20:31:37.8: 12.70 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:03.95 +20:31:37.8: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 49 03.95 +20 31 37.8 11.8 U Com 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
Gaia DR3 3954337940879977856,2461238.7045,11.79,0.05,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
Gaia DR3 3954337940879977856 20260717.2045 11.79CV 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 17.2045 2461238.7045 12.02 12:49:31.57 +22:09:55.7
297.82818 85.01826 galactic Com Second-epoch detections are separated by 2.3" and 9.8 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 | 12:49:31.57 +22:09:55.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.317+/-0.029 (F)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:31.57 +22:09:55.7: 12.97 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:31.57 +22:09:55.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 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 17.2045* 12 49 31.57 +22 09 55.7 12.0 U Com 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,2461238.7045,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.73 12:49:38.19 +21:05:54.3
298.93813 83.95619 galactic Com Second-epoch detections are separated by 1.2" and 10.1 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 | 12:49:38.19 +21:05:54.3 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.550+/-0.032 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:38.19 +21:05:54.3: 14.05 +/- 0.06 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:38.19 +21:05:54.3: 14.10 +/- 0.05 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!
TCP 2026 07 17.2045* 12 49 38.19 +21 05 54.3 12.7 U Com 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,2461238.7045,12.73,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.24 12:51:43.99 +20:06:43.4
303.49932 82.98348 galactic Com Second-epoch detections are separated by 1.0" and 10.3 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 | 12:51:43.99 +20:06:43.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.441+/-0.034 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:43.99 +20:06:43.4: 13.46 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:43.99 +20:06:43.4: 13.44 +/- 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 17.2045* 12 51 43.99 +20 06 43.4 12.2 U Com 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,2461238.7045,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.31 12:51:15.12 +21:06:49.7
302.51810 83.98540 galactic Com Second-epoch detections are separated by 1.5" and 10.2 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 | 12:51:15.12 +21:06:49.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.390+/-0.028 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:15.12 +21:06:49.7: 13.30 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:15.12 +21:06:49.7: 13.24 +/- 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 17.2045* 12 51 15.12 +21 06 49.7 12.3 U Com 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,2461238.7045,12.31,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.10 12:51:31.58 +20:33:23.3
303.11274 83.42819 galactic Com Second-epoch detections are separated by 1.3" and 10.6 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 | 12:51:31.58 +20:33:23.3 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.528+/-0.028 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:31.58 +20:33:23.3: 13.27 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:31.58 +20:33:23.3: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 17.2045* 12 51 31.58 +20 33 23.3 12.1 U Com 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,2461238.7045,12.10,0.05,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 20260717.2045 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 17.2045 2461238.7045 11.40 12:49:57.04 +21:13:30.8
299.56549 84.08725 galactic Com Second-epoch detections are separated by 0.1" and 10.4 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 3954755656514782720 | 12:49:57.04 +21:13:31.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G9 (LAMOST DR5) J-Ks=0.578+/-0.026 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:57.04 +21:13:30.8: 12.35 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:57.04 +21:13:30.8: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 49 57.04 +21 13 30.8 11.4 U Com 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
Gaia DR3 3954755656514782720,2461238.7045,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3954755656514782720 20260717.2045 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.60 12:49:19.81 +21:08:23.0
298.23092 83.99222 galactic Com Second-epoch detections are separated by 0.2" and 10.3 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 | 12:49:19.81 +21:08:23.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.305+/-0.031 (F)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:19.81 +21:08:23.0: 12.65 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:19.81 +21:08:23.0: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 49 19.81 +21 08 23.0 11.6 U Com 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,2461238.7045,11.60,0.05,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 20260717.2045 11.60CV 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 17.2045 2461238.7045 12.02 12:47:39.27 +22:36:50.3
291.96678 85.40495 galactic Com Second-epoch detections are separated by 0.8" and 10.2 pix
The object was found in VSX 1" Gaia DR3 3955145055429752960
Type: ROT
# Max. Min./Amp. JD0 Period
12.810 G 12.850 G G
The object was not found in astcheck.
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:39.27 +22:36:50.3: 12.98 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:39.27 +22:36:50.3: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 17.2045* 12 47 39.27 +22 36 50.3 12.0 U Com 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
Gaia DR3 3955145055429752960,2461238.7045,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3955145055429752960 20260717.2045 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.07 12:49:15.92 +20:50:31.4
298.30536 83.69428 galactic Com Second-epoch detections are separated by 0.5" and 10.4 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 | 12:49:15.92 +20:50:31.4 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.599+/-0.032 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:15.92 +20:50:31.4: 13.28 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:15.92 +20:50:31.4: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 49 15.92 +20 50 31.4 12.1 U Com 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,2461238.7045,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 11.36 12:53:08.58 +19:34:51.1
305.98697 82.44249 galactic Com Second-epoch detections are separated by 0.9" and 10.1 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 | 12:53:08.58 +19:34:51.1 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.038 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:08.58 +19:34:51.1: 12.33 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:08.58 +19:34:51.1: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 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 17.2045* 12 53 08.58 +19 34 51.1 11.4 U Com 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,2461238.7045,11.36,0.05,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 20260717.2045 11.36CV 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 17.2045 2461238.7045 12.15 12:49:26.63 +21:15:23.7
298.39916 84.11077 galactic Com Second-epoch detections are separated by 1.1" and 10.2 pix
The object was found in VSX 0" Gaia DR3 3954797987712425728
Type: RS
# Max. Min./Amp. JD0 Period
13.030 G 13.140 G K
The object was not found in astcheck.
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:26.63 +21:15:23.7: 13.27 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:26.63 +21:15:23.7: 13.23 +/- 0.02 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!
TCP 2026 07 17.2045* 12 49 26.63 +21 15 23.7 12.2 U Com 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
Gaia DR3 3954797987712425728,2461238.7045,12.15,0.05,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
Gaia DR3 3954797987712425728 20260717.2045 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 17.2045 2461238.7045 11.96 12:51:31.11 +20:26:42.9
303.09411 83.31697 galactic Com Second-epoch detections are separated by 1.0" and 10.5 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 | 12:51:31.11 +20:26:42.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.705+/-0.028 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:31.11 +20:26:42.9: 13.23 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:31.11 +20:26:42.9: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 17.2045* 12 51 31.11 +20 26 42.9 12.0 U Com 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,2461238.7045,11.96,0.05,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 20260717.2045 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 17.2045 2461238.7045 12.38 12:53:00.63 +20:26:13.4
306.09069 83.29916 galactic Com Second-epoch detections are separated by 1.6" and 10.4 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 | 12:53:00.63 +20:26:13.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.228+/-0.046 (F)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:00.63 +20:26:13.4: 13.68 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:00.63 +20:26:13.4: 13.59 +/- 0.03 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!
TCP 2026 07 17.2045* 12 53 00.63 +20 26 13.4 12.4 U Com 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,2461238.7045,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260717.2045 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 17.2045 2461238.7045 12.55 12:47:15.43 +22:27:05.5
291.23995 85.22807 galactic Com Second-epoch detections are separated by 1.8" and 10.4 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 | 12:47:15.43 +22:27:05.5 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.451+/-0.035 (G)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:15.43 +22:27:05.5: 13.68 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:15.43 +22:27:05.5: 13.67 +/- 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!
TCP 2026 07 17.2045* 12 47 15.43 +22 27 05.5 12.6 U Com 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,2461238.7045,12.55,0.05,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 20260717.2045 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 17.2045 2461238.7045 11.62 12:50:30.35 +20:28:23.5
301.04885 83.34153 galactic Com Second-epoch detections are separated by 0.6" and 10.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3942330109969035264 | 12:50:30.36 +20:28:23.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.473+/-0.030 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:30.35 +20:28:23.5: 12.66 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:30.35 +20:28:23.5: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 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 17.2045* 12 50 30.35 +20 28 23.5 11.6 U Com 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
Gaia DR3 3942330109969035264,2461238.7045,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3942330109969035264 20260717.2045 11.62CV 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 17.2045 2461238.7045 12.23 12:51:17.73 +21:08:56.7
302.61313 84.02074 galactic Com Second-epoch detections are separated by 0.7" and 10.2 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 | 12:51:17.73 +21:08:56.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.673+/-0.025 (K)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:17.73 +21:08:56.7: 13.23 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:17.73 +21:08:56.7: 13.26 +/- 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!
TCP 2026 07 17.2045* 12 51 17.73 +21 08 56.7 12.2 U Com 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,2461238.7045,12.23,0.05,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 20260717.2045 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461173.75458943 13.05.2026 06:06:26.527 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
First image: 2461173.75458943 13.05.2026 06:06:26.527 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
Last image: 2461238.70482231 17.07.2026 04:54:46.648 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 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): 3768
Objects passed selection criteria: 3749
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 2317.5
Average stars matched: 2269.5 (97.9288 %)
Memory usage VmPeak: 113772 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Jul 16 05:04:38 CDT 2026
VaST build number 1.0rc89-156-g3b0d8dc3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 17 01:00:36 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: 2461173.75458943 13.05.2026 06:06:26.527 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
First image: 2461173.75458943 13.05.2026 06:06:26.527 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
Last image: 2461238.70482231 17.07.2026 04:54:46.648 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 102
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: 10 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): 19374
Objects passed selection criteria: 19323
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 12847
Average stars matched: 12308.2 (95.8064 %)
Memory usage VmPeak: 128592 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Jul 16 05:04:38 CDT 2026
VaST build number 1.0rc89-156-g3b0d8dc3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 17 01:02:04 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/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
SExtractor catalog cache: saved Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.cat to cache
SExtractor catalog cache: saved Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.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/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.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: 2461238.70422976
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
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits exists and is non-empty
Saving wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits to local_wcs_cache/
'wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits' -> 'local_wcs_cache/wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits'
wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits exists and is non-empty
Saving wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits to local_wcs_cache/
'wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits' -> 'local_wcs_cache/wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits'
wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits exists and is non-empty
Saving wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits to local_wcs_cache/
'wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits' -> 'local_wcs_cache/wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits'
wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits exists and is non-empty
Saving wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits to local_wcs_cache/
'wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits' -> 'local_wcs_cache/wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits (1st reference image)
verification OK: wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:55:21.550 +21:59:57.00 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits (1st new image)
verification OK: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:55:22.049 +22:00:22.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:55:21.550 +21:59:57.00
Second-epoch image center 12:55:22.049 +22:00:22.57
Angular distance between the image centers 0.0074 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits (2nd new image)
verification OK: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:55:18.684 +21:59:45.15 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:55:21.550 +21:59:57.00
Second-epoch image center 12:55:18.684 +21:59:45.15
Angular distance between the image centers 0.0116 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 12:55:22.049 +22:00:22.57
Second-epoch second image center 12:55:18.684 +21:59:45.15
Angular distance between the image centers 0.01664 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/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits &> /tmp/tmp.lgsJVr36dg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits &> /tmp/tmp.CPVwhNRWtn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits &> /tmp/tmp.efbL6ZpuVP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits &> /tmp/tmp.7PuCI8kf5P
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
Calibrating the magnitude scale
Found non-empty wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.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_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits and wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.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_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits and wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat
Found non-empty wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits and wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat
The reference image (wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits) and catalog (wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat) found
'wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat' -> 'wcsmag.cat'
Read 5207 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.0887 to 202.5730 deg, Dec +16.5938 to +27.2565 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 185.0887 to 202.5730 deg, Dec 16.5938 to 27.2565 deg
Loaded 3757 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): 2863 out of 2945 total matches.
Matched with Tycho-2 2945 out of 5207 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.753400
a=0.000000 b=1.000000 c=22.753400
From vast_summary.log: estimated ref. image limiting mag.: -7.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5207 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.0887 to 202.5730 deg, Dec +16.5938 to +27.2565 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 185.0887 to 202.5730 deg, Dec 16.5938 to 27.2565 deg
Loaded 3757 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): 2863 out of 2945 total matches.
Matched with Tycho-2 2945 out of 5207 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits:
Forced-photometry filter: calibrated wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits -> calib.txt_param_ref_wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits (aperture=6.4)
Read 5177 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.0879 to 202.5737 deg, Dec +16.5936 to +27.2555 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 185.0879 to 202.5737 deg, Dec 16.5936 to 27.2555 deg
Loaded 3754 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): 2870 out of 2953 total matches.
Matched with Tycho-2 2953 out of 5177 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits:
Forced-photometry filter: calibrated wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits -> calib.txt_param_ref_wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
2.3 pix Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
2.6 pix fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
2.7 pix fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
2.3 pix wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
2.3 pix wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
Limiting magnitude estimates:
15.3 mag. Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
15.3 mag. Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
12.6 mag. fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
12.5 mag. fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 10.0 (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.lgsJVr36dg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits' -> 'wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
WCS_IMAGE_NAME=wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
WCS-calibrated image found: wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
Checking if the catalog wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat corresponding to the image wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits alredy exist and is non-empty...
Catalog wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat corresponding to the image wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
WCS catalog name: wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.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=313, bad_region=1135, passed=5207
Got 5207 stars (including 3846 good ones) from the SExtractor catalog wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat
util/solve_plate_with_UCAC5 got 5207 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 532 to 588 (Dec 16.6 to 27.3)
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(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 4176 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 532 to 588 (Dec 16.6 to 27.3)
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(), 4177 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 4177 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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=Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits N_match=965 sigma_overall_arcsec=0.394 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.443 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.424 n_q1=307 n_q2=186 n_q3=287 n_q4=185 worst_quadrant_to_overall_ratio=1.124
The image catalog is written to wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits -region wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.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.CPVwhNRWtn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits' -> 'wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
WCS_IMAGE_NAME=wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
WCS-calibrated image found: wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
Checking if the catalog wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat corresponding to the image wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits alredy exist and is non-empty...
Catalog wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat corresponding to the image wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
WCS catalog name: wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.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=312, bad_region=1224, passed=5177
Got 5177 stars (including 3711 good ones) from the SExtractor catalog wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat
util/solve_plate_with_UCAC5 got 5177 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 532 to 588 (Dec 16.6 to 27.3)
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(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 4070 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 532 to 588 (Dec 16.6 to 27.3)
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(), 4070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 4070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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=Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits N_match=965 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.364 sigma_q2_arcsec=0.372 sigma_q3_arcsec=0.379 sigma_q4_arcsec=0.372 n_q1=309 n_q2=190 n_q3=283 n_q4=183 worst_quadrant_to_overall_ratio=0.994
The image catalog is written to wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits -region wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.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.efbL6ZpuVP (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_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.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_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
WCS-calibrated image found: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
Checking if the catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
WCS catalog name: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.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=65, bad_region=211, passed=820
Got 820 stars (including 560 good ones) from the SExtractor catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 820 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 527 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 527 matched stars entering correct_measured_positions(), 492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 527 matched stars entering correct_measured_positions(), 577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 526 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 526 matched stars entering correct_measured_positions(), 574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 526 matched stars entering correct_measured_positions(), 574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 526 stars left (next iteration limit 579)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits N_match=526 sigma_overall_arcsec=0.628 sigma_q1_arcsec=0.616 sigma_q2_arcsec=0.535 sigma_q3_arcsec=0.665 sigma_q4_arcsec=0.597 n_q1=148 n_q2=101 n_q3=183 n_q4=94 worst_quadrant_to_overall_ratio=1.060
The image catalog is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits -region wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.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.7PuCI8kf5P (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_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.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_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
Checking if the catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
WCS catalog name: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.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=35, bad_region=88, passed=789
Got 789 stars (including 673 good ones) from the SExtractor catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 789 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 534 to 588 (Dec 16.8 to 27.2)
Done reading UCAC5 zone files...
Matched 640 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 640 matched stars entering correct_measured_positions(), 603 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 640 matched stars entering correct_measured_positions(), 658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 534 to 588 (Dec 16.8 to 27.2)
Done reading UCAC5 zone files...
Matched 640 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 640 matched stars entering correct_measured_positions(), 655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 640 matched stars entering correct_measured_positions(), 655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 640 stars left (next iteration limit 704)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits N_match=640 sigma_overall_arcsec=0.563 sigma_q1_arcsec=0.523 sigma_q2_arcsec=0.516 sigma_q3_arcsec=0.664 sigma_q4_arcsec=0.702 n_q1=359 n_q2=94 n_q3=140 n_q4=47 worst_quadrant_to_overall_ratio=1.247
The image catalog is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits -region wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.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=Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits sigma_overall=0.394 worst_q_ratio=1.124
ref2=Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits sigma_overall=0.382 worst_q_ratio=0.994
new1=fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits sigma_overall=0.628 worst_q_ratio=1.060
new2=fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits sigma_overall=0.563 worst_q_ratio=1.247
reference average sigma_overall=0.388 worst_q_ratio=1.059
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195_astrometric_residuals.png (965 matched stars from wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549_astrometric_residuals.png (965 matched stars from wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138_astrometric_residuals.png (526 matched stars from wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139_astrometric_residuals.png (640 matched stars from wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits'
Saving fully-calibrated image wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits'
Preparing the HTML report for the field Com-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Com-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/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
SExtractor catalog cache: saved Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.cat to cache
SExtractor catalog cache: saved Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
Creating symlink local_wcs_cache/wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
Creating symlink local_wcs_cache/wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
Creating symlink local_wcs_cache/wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.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_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits exists and is non-empty
wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits exists and is non-empty
wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits exists and is non-empty
wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits (1st reference image)
verification OK: wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:55:21.550 +21:59:57.00 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits (1st new image)
verification OK: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:55:22.049 +22:00:22.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:55:21.550 +21:59:57.00
Second-epoch image center 12:55:22.049 +22:00:22.57
Angular distance between the image centers 0.0074 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits (2nd new image)
verification OK: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:55:18.684 +21:59:45.15 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:55:21.550 +21:59:57.00
Second-epoch image center 12:55:18.684 +21:59:45.15
Angular distance between the image centers 0.0116 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 12:55:22.049 +22:00:22.57
Second-epoch second image center 12:55:18.684 +21:59:45.15
Angular distance between the image centers 0.01664 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/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits &> /tmp/tmp.yusoPdj6hF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits &> /tmp/tmp.82NZelsW4t
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits &> /tmp/tmp.t1gpWGnLJu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits &> /tmp/tmp.hqYNnoWr5B
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
Calibrating the magnitude scale
Found non-empty wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.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_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits and wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.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_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits and wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat
Found non-empty wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits and wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat
The reference image (wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits) and catalog (wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat) found
'wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat' -> 'wcsmag.cat'
Read 24766 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.0887 to 202.5729 deg, Dec +16.5783 to +27.2612 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 185.0887 to 202.5729 deg, Dec 16.5783 to 27.2612 deg
Loaded 3760 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): 2768 out of 2976 total matches.
Matched with Tycho-2 2976 out of 24766 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.639900
a=0.000000 b=1.000000 c=22.639900
From vast_summary.log: estimated ref. image limiting mag.: -7.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 24766 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.0887 to 202.5729 deg, Dec +16.5783 to +27.2612 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 185.0887 to 202.5729 deg, Dec 16.5783 to 27.2612 deg
Loaded 3760 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): 2768 out of 2976 total matches.
Matched with Tycho-2 2976 out of 24766 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits:
Forced-photometry filter: calibrated wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits -> calib.txt_param_ref_wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits (aperture=5.1)
Read 25696 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.0879 to 202.5737 deg, Dec +16.5766 to +27.2592 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 185.0879 to 202.5737 deg, Dec 16.5766 to 27.2592 deg
Loaded 3761 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): 2795 out of 2990 total matches.
Matched with Tycho-2 2990 out of 25696 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits:
Forced-photometry filter: calibrated wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits -> calib.txt_param_ref_wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 99 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
2.2 pix Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
2.3 pix fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
2.2 pix fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
2.2 pix wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
2.2 pix wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
Limiting magnitude estimates:
15.4 mag. Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
15.4 mag. Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
12.9 mag. fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
13.0 mag. fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.yusoPdj6hF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits' -> 'wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
WCS_IMAGE_NAME=wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
WCS-calibrated image found: wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
Checking if the catalog wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat corresponding to the image wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits alredy exist and is non-empty...
Catalog wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat corresponding to the image wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits
WCS catalog name: wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.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=7, blended=1293, bad_region=3913, passed=24759
Got 24759 stars (including 20119 good ones) from the SExtractor catalog wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat
util/solve_plate_with_UCAC5 got 24759 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 21258 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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 21257 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 21257 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits N_match=963 sigma_overall_arcsec=0.383 sigma_q1_arcsec=0.347 sigma_q2_arcsec=0.431 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.457 n_q1=312 n_q2=186 n_q3=285 n_q4=180 worst_quadrant_to_overall_ratio=1.196
The image catalog is written to wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits -region wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.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.82NZelsW4t (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits' -> 'wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
WCS_IMAGE_NAME=wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
WCS-calibrated image found: wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
Checking if the catalog wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat corresponding to the image wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits alredy exist and is non-empty...
Catalog wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat corresponding to the image wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits
WCS catalog name: wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.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=5, blended=1035, bad_region=4413, passed=25691
Got 25691 stars (including 20487 good ones) from the SExtractor catalog wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat
util/solve_plate_with_UCAC5 got 25691 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 532 to 588 (Dec 16.6 to 27.3)
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(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 21794 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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 21794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 21794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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=Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits N_match=964 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.373 sigma_q3_arcsec=0.361 sigma_q4_arcsec=0.359 n_q1=309 n_q2=193 n_q3=278 n_q4=184 worst_quadrant_to_overall_ratio=0.991
The image catalog is written to wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits -region wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.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.t1gpWGnLJu (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_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.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_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
WCS-calibrated image found: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
Checking if the catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
WCS catalog name: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.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=155, bad_region=1134, passed=5580
Got 5580 stars (including 4318 good ones) from the SExtractor catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 5580 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits N_match=944 sigma_overall_arcsec=0.527 sigma_q1_arcsec=0.511 sigma_q2_arcsec=0.487 sigma_q3_arcsec=0.563 sigma_q4_arcsec=0.544 n_q1=262 n_q2=199 n_q3=307 n_q4=176 worst_quadrant_to_overall_ratio=1.070
The image catalog is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits -region wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.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.hqYNnoWr5B (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_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.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_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
Checking if the catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
WCS catalog name: wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=101, bad_region=489, passed=5701
Got 5701 stars (including 5118 good ones) from the SExtractor catalog wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 5701 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5071 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5071 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits N_match=945 sigma_overall_arcsec=0.523 sigma_q1_arcsec=0.475 sigma_q2_arcsec=0.466 sigma_q3_arcsec=0.699 sigma_q4_arcsec=0.617 n_q1=498 n_q2=153 n_q3=204 n_q4=90 worst_quadrant_to_overall_ratio=1.335
The image catalog is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits -region wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.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_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.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_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/wcs_fd_Com-03-Q2b1x1_2026-07-16_23-53-55_20.00sec_4.90C_LIGHT_0138.fits
Saving fully-calibrated image wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.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_2026-07-17_CI_Com-03-Q2b1x1_001228_TTUQ2b1x1_2666605_dfEjv4Ov/wcs_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139.fits
Preparing the HTML report for the field Com-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:38:54.13 +24:53:08.4: 13.20 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:18.76 +21:24:05.9: 13.20 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:48:52.96 +21:47:58.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:58.44 +20:14:14.8: 12.24 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:14.45 +20:50:17.6: 13.38 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:33.71 +20:13:00.7: 12.66 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:45.76 +19:49:09.9: 12.99 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:54:37.85 +19:13:02.9: 13.38 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:06.78 +21:10:29.3: 13.56 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:08.57 +20:51:56.1: 12.22 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:33.71 +20:13:00.7: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 12:52:33.71 +20:13:00.7: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6532 delta=0.99 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:38:54.13 +24:53:08.4: 13.13 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:54:37.85 +19:13:02.9: 13.40 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:48:52.96 +21:47:58.3: 13.15 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:58.44 +20:14:14.8: 12.24 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:18.76 +21:24:05.9: 13.30 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:06.78 +21:10:29.3: 13.52 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:14.45 +20:50:17.6: 13.40 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:45.76 +19:49:09.9: 12.96 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:08.57 +20:51:56.1: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 12:38:54.13 +24:53:08.4: ref_mag=13.16 +/- 0.02 new_mean_mag=12.0474 delta=1.12 (need > 0.90)
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Forced photometry filter KEPT candidate at 12:54:37.85 +19:13:02.9: ref_mag=13.39 +/- 0.02 new_mean_mag=12.3197 delta=1.07 (need > 0.90)
Forced photometry filter KEPT candidate at 12:48:52.96 +21:47:58.3: ref_mag=13.17 +/- 0.02 new_mean_mag=12.1137 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 12:50:58.44 +20:14:14.8: ref_mag=12.24 +/- 0.01 new_mean_mag=11.2853 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry filter KEPT candidate at 12:51:06.78 +21:10:29.3: ref_mag=13.54 +/- 0.02 new_mean_mag=12.4270 delta=1.12 (need > 0.90)
Forced photometry filter KEPT candidate at 12:50:18.76 +21:24:05.9: ref_mag=13.25 +/- 0.02 new_mean_mag=12.1246 delta=1.12 (need > 0.90)
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 12:53:14.45 +20:50:17.6: ref_mag=13.39 +/- 0.02 new_mean_mag=12.4112 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 12:51:08.57 +20:51:56.1: ref_mag=12.22 +/- 0.01 new_mean_mag=11.2907 delta=0.93 (need > 0.90)
Forced photometry filter KEPT candidate at 12:51:45.76 +19:49:09.9: ref_mag=12.97 +/- 0.01 new_mean_mag=11.9488 delta=1.02 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:39.84 +20:28:04.9: 13.19 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:11.89 +21:58:00.2: 13.19 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:39.84 +20:28:04.9: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 12:49:39.84 +20:28:04.9: ref_mag=13.23 +/- 0.02 new_mean_mag=12.2657 delta=0.97 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:11.89 +21:58:00.2: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 12:49:11.89 +21:58:00.2: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1214 delta=1.07 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:14.80 +20:05:21.2: 13.16 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:14.80 +20:05:21.2: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 12:51:14.80 +20:05:21.2: ref_mag=13.16 +/- 0.02 new_mean_mag=11.9684 delta=1.19 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:48:23.71 +22:22:11.9: 13.48 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 13:06:34.11 +24:52:08.1: 13.43 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:36.23 +20:09:59.6: 13.94 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:44.58 +20:32:20.4: 12.61 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:15.53 +20:58:02.1: 13.99 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:48:56.74 +21:03:48.1: 13.18 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:48:23.71 +22:22:11.9: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 13:06:34.11 +24:52:08.1: 13.56 +/- 0.03 detection
Forced photometry filter KEPT candidate at 12:48:23.71 +22:22:11.9: ref_mag=13.47 +/- 0.02 new_mean_mag=12.3884 delta=1.08 (need > 0.90)
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:36.23 +20:09:59.6: 14.03 +/- 0.05 detection
Forced photometry filter KEPT candidate at 13:06:34.11 +24:52:08.1: ref_mag=13.49 +/- 0.02 new_mean_mag=12.5372 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 13.99 +/- 0.04
Forced photometry filter KEPT candidate at 12:51:36.23 +20:09:59.6: ref_mag=13.99 +/- 0.04 new_mean_mag=12.5539 delta=1.43 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:44.58 +20:32:20.4: 12.57 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:15.53 +20:58:02.1: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry reference-image weighted average: 13.97 +/- 0.04
Forced photometry filter KEPT candidate at 12:49:44.58 +20:32:20.4: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6071 delta=0.98 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:48:56.74 +21:03:48.1: 13.21 +/- 0.02 detection
Forced photometry filter KEPT candidate at 12:50:15.53 +20:58:02.1: ref_mag=13.97 +/- 0.04 new_mean_mag=12.6318 delta=1.34 (need > 0.90)
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 12:48:56.74 +21:03:48.1: ref_mag=13.19 +/- 0.02 new_mean_mag=11.9657 delta=1.22 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:41.68 +20:06:45.2: 12.95 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:41.68 +20:06:45.2: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 12:51:41.68 +20:06:45.2: ref_mag=12.97 +/- 0.01 new_mean_mag=11.8885 delta=1.08 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:13.10 +20:05:07.2: 13.42 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:13.10 +20:05:07.2: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Forced photometry filter KEPT candidate at 12:51:13.10 +20:05:07.2: ref_mag=13.41 +/- 0.02 new_mean_mag=12.3099 delta=1.10 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:51.57 +20:16:35.4: 13.15 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:51.57 +20:16:35.4: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 12:50:51.57 +20:16:35.4: ref_mag=13.12 +/- 0.02 new_mean_mag=12.0506 delta=1.07 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:46.52 +21:56:29.6: 13.15 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:46.52 +21:56:29.6: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 12:49:46.52 +21:56:29.6: ref_mag=13.12 +/- 0.02 new_mean_mag=12.0766 delta=1.04 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:18.68 +20:27:41.4: 13.69 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:26.79 +20:30:16.5: 12.94 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:43:55.04 +23:38:19.7: 13.13 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:36.75 +20:55:44.9: 13.12 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:18.68 +20:27:41.4: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry filter KEPT candidate at 12:50:18.68 +20:27:41.4: ref_mag=13.70 +/- 0.03 new_mean_mag=12.3784 delta=1.33 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:26.79 +20:30:16.5: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 12:51:26.79 +20:30:16.5: ref_mag=12.93 +/- 0.01 new_mean_mag=11.8448 delta=1.08 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:39.43 +20:53:52.5: 12.89 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:43:55.04 +23:38:19.7: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 12:43:55.04 +23:38:19.7: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1229 delta=1.01 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:33.90 +21:30:36.4: 13.62 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:36.75 +20:55:44.9: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 12:49:36.75 +20:55:44.9: ref_mag=13.10 +/- 0.02 new_mean_mag=11.8963 delta=1.20 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:39.43 +20:53:52.5: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter KEPT candidate at 12:49:39.43 +20:53:52.5: ref_mag=12.91 +/- 0.01 new_mean_mag=11.6910 delta=1.22 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:33.90 +21:30:36.4: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry filter KEPT candidate at 12:49:33.90 +21:30:36.4: ref_mag=13.63 +/- 0.03 new_mean_mag=12.4308 delta=1.20 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:26.94 +20:45:40.2: 13.40 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:26.94 +20:45:40.2: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 12:52:26.94 +20:45:40.2: ref_mag=13.37 +/- 0.02 new_mean_mag=12.3304 delta=1.04 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:36:07.99 +25:33:23.6: 12.86 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:36:07.99 +25:33:23.6: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter REJECTED candidate at 12:36:07.99 +25:33:23.6: ref_mag=12.78 +/- 0.01 new_mean_mag=11.9017 delta=0.88 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:26.09 +20:21:57.8: 13.12 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:26.09 +20:21:57.8: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 12:50:26.09 +20:21:57.8: ref_mag=13.09 +/- 0.02 new_mean_mag=12.0167 delta=1.08 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:46.18 +21:01:04.4: 13.11 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:46.18 +21:01:04.4: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 12:49:46.18 +21:01:04.4: ref_mag=13.09 +/- 0.02 new_mean_mag=11.8682 delta=1.23 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:26.48 +20:25:58.2: 13.83 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:26.48 +20:25:58.2: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter KEPT candidate at 12:51:26.48 +20:25:58.2: ref_mag=13.81 +/- 0.03 new_mean_mag=12.5445 delta=1.27 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:45.46 +20:45:33.2: 13.83 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:45.46 +20:45:33.2: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Forced photometry filter KEPT candidate at 12:49:45.46 +20:45:33.2: ref_mag=13.83 +/- 0.03 new_mean_mag=12.3716 delta=1.46 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:53.96 +20:04:53.4: 13.41 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:53.96 +20:04:53.4: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 12:50:53.96 +20:04:53.4: ref_mag=13.43 +/- 0.02 new_mean_mag=12.2546 delta=1.17 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:39:02.50 +24:52:48.3: 12.86 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:42.13 +20:16:36.8: 13.61 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:01.00 +19:44:50.1: 12.53 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:39:02.50 +24:52:48.3: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 12:39:02.50 +24:52:48.3: ref_mag=12.85 +/- 0.01 new_mean_mag=11.9283 delta=0.92 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:42.13 +20:16:36.8: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter KEPT candidate at 12:52:42.13 +20:16:36.8: ref_mag=13.59 +/- 0.03 new_mean_mag=12.4160 delta=1.18 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:10.69 +19:21:09.8: 13.12 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:01.00 +19:44:50.1: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry filter KEPT candidate at 12:53:01.00 +19:44:50.1: ref_mag=12.53 +/- 0.01 new_mean_mag=11.4989 delta=1.04 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:10.69 +19:21:09.8: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 12:53:10.69 +19:21:09.8: ref_mag=13.12 +/- 0.02 new_mean_mag=12.1015 delta=1.02 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:00.15 +20:31:44.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:00.15 +20:31:44.3: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 12:52:00.15 +20:31:44.3: ref_mag=13.09 +/- 0.02 new_mean_mag=12.0537 delta=1.04 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:54.21 +20:15:58.7: 13.82 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:54.21 +20:15:58.7: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter KEPT candidate at 12:51:54.21 +20:15:58.7: ref_mag=13.81 +/- 0.03 new_mean_mag=12.4927 delta=1.32 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:05.81 +21:27:46.0: 13.79 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:05.81 +21:27:46.0: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Forced photometry filter KEPT candidate at 12:50:05.81 +21:27:46.0: ref_mag=13.80 +/- 0.03 new_mean_mag=12.4930 delta=1.31 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 13:07:44.04 +24:38:42.1: 13.59 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:10.27 +20:36:53.1: 12.86 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 13:07:44.04 +24:38:42.1: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Forced photometry filter KEPT candidate at 13:07:44.04 +24:38:42.1: ref_mag=13.58 +/- 0.03 new_mean_mag=12.5577 delta=1.02 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:10.27 +20:36:53.1: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 12:50:10.27 +20:36:53.1: ref_mag=12.86 +/- 0.01 new_mean_mag=11.6844 delta=1.17 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:36.32 +21:07:15.0: 13.63 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:36.32 +21:07:15.0: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 12:52:36.32 +21:07:15.0: ref_mag=13.66 +/- 0.03 new_mean_mag=12.5416 delta=1.12 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:48.81 +20:42:44.2: 12.83 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:48.81 +20:42:44.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 12:52:48.81 +20:42:44.2: ref_mag=12.85 +/- 0.01 new_mean_mag=11.8974 delta=0.95 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:48:57.80 +21:11:53.7: 11.73 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:06.69 +20:47:18.9: 12.82 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:14.19 +20:16:06.9: 13.02 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:06.69 +20:47:18.9: 12.85 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:48:57.80 +21:11:53.7: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry reference-image weighted average: 11.71 +/- 0.00
Forced photometry filter KEPT candidate at 12:49:06.69 +20:47:18.9: ref_mag=12.83 +/- 0.01 new_mean_mag=11.7439 delta=1.09 (need > 0.90)
Forced photometry filter KEPT candidate at 12:48:57.80 +21:11:53.7: ref_mag=11.71 +/- 0.00 new_mean_mag=10.7098 delta=1.00 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:14.19 +20:16:06.9: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 12:50:14.19 +20:16:06.9: ref_mag=13.00 +/- 0.02 new_mean_mag=11.9919 delta=1.01 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:25.79 +20:23:49.3: 11.88 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:25.79 +20:23:49.3: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Forced photometry filter REJECTED candidate at 12:51:25.79 +20:23:49.3: ref_mag=11.89 +/- 0.01 new_mean_mag=11.0985 delta=0.79 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:18.75 +20:23:04.4: 13.07 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:58.90 +20:33:36.0: 13.58 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:30.09 +20:07:19.7: 13.60 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:18.75 +20:23:04.4: 13.10 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:58.90 +20:33:36.0: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 12:50:18.75 +20:23:04.4: ref_mag=13.08 +/- 0.02 new_mean_mag=12.0170 delta=1.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.60 +/- 0.02
Forced photometry filter KEPT candidate at 12:52:58.90 +20:33:36.0: ref_mag=13.60 +/- 0.02 new_mean_mag=12.3796 delta=1.22 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:30.09 +20:07:19.7: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 12:51:30.09 +20:07:19.7: ref_mag=13.62 +/- 0.03 new_mean_mag=12.3666 delta=1.25 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:14.27 +20:43:44.3: 13.91 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:14.27 +20:43:44.3: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Forced photometry filter KEPT candidate at 12:49:14.27 +20:43:44.3: ref_mag=13.89 +/- 0.03 new_mean_mag=12.4997 delta=1.39 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:52:07.73 +20:00:42.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:52:07.73 +20:00:42.7: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 12:52:07.73 +20:00:42.7: ref_mag=12.81 +/- 0.01 new_mean_mag=11.7375 delta=1.07 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:16.66 +20:45:21.9: 13.06 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:16.66 +20:45:21.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Forced photometry filter KEPT candidate at 12:50:16.66 +20:45:21.9: ref_mag=13.01 +/- 0.01 new_mean_mag=11.8939 delta=1.12 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:45:16.05 +23:06:47.0: 14.36 +/- 0.07 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:45:16.05 +23:06:47.0: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.05
Forced photometry filter KEPT candidate at 12:45:16.05 +23:06:47.0: ref_mag=14.27 +/- 0.05 new_mean_mag=12.7154 delta=1.56 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:08.39 +20:21:20.6: 13.77 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:08.39 +20:21:20.6: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 12:50:08.39 +20:21:20.6: ref_mag=13.75 +/- 0.03 new_mean_mag=12.5017 delta=1.25 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:51.80 +21:28:40.0: 13.75 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:44.32 +22:08:10.5: 13.75 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:51.80 +21:28:40.0: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:44.32 +22:08:10.5: 13.73 +/- 0.04 detection
Forced photometry filter KEPT candidate at 12:50:51.80 +21:28:40.0: ref_mag=13.73 +/- 0.03 new_mean_mag=12.6378 delta=1.09 (need > 0.90)
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Forced photometry filter KEPT candidate at 12:49:44.32 +22:08:10.5: ref_mag=13.74 +/- 0.03 new_mean_mag=12.6502 delta=1.09 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:24.98 +20:38:05.0: 13.35 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:13.72 +20:39:33.5: 13.33 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:24.98 +20:38:05.0: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 12:51:24.98 +20:38:05.0: ref_mag=13.33 +/- 0.02 new_mean_mag=12.1691 delta=1.17 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:13.72 +20:39:33.5: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter KEPT candidate at 12:49:13.72 +20:39:33.5: ref_mag=13.31 +/- 0.02 new_mean_mag=12.1280 delta=1.18 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:15.70 +20:59:25.3: 13.74 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:09.13 +23:00:58.2: 13.71 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:15.70 +20:59:25.3: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:09.13 +23:00:58.2: 13.78 +/- 0.04 detection
Forced photometry filter KEPT candidate at 12:50:15.70 +20:59:25.3: ref_mag=13.65 +/- 0.03 new_mean_mag=12.4435 delta=1.21 (need > 0.90)
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 12:47:09.13 +23:00:58.2: ref_mag=13.75 +/- 0.03 new_mean_mag=12.5891 delta=1.16 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:05.67 +19:49:15.6: 13.05 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:05.67 +19:49:15.6: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 12:51:05.67 +19:49:15.6: ref_mag=13.07 +/- 0.02 new_mean_mag=12.0630 delta=1.00 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:48.60 +22:16:38.1: 12.78 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:48.60 +22:16:38.1: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 12:47:48.60 +22:16:38.1: ref_mag=12.77 +/- 0.01 new_mean_mag=11.7246 delta=1.04 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:55.77 +22:08:26.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:55.77 +22:08:26.8: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry filter KEPT candidate at 12:47:55.77 +22:08:26.8: ref_mag=13.49 +/- 0.02 new_mean_mag=12.3035 delta=1.18 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:48:39.38 +21:04:26.5: 14.04 +/- 0.05 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:48:39.38 +21:04:26.5: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.04
Forced photometry filter KEPT candidate at 12:48:39.38 +21:04:26.5: ref_mag=14.00 +/- 0.04 new_mean_mag=12.6976 delta=1.31 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:47.02 +20:39:55.3: 11.92 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:47.02 +20:39:55.3: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Forced photometry filter KEPT candidate at 12:50:47.02 +20:39:55.3: ref_mag=11.94 +/- 0.01 new_mean_mag=10.9915 delta=0.95 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:59.65 +20:23:34.6: 13.33 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:29.62 +22:06:17.0: 13.72 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:59.65 +20:23:34.6: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 12:50:59.65 +20:23:34.6: ref_mag=13.34 +/- 0.02 new_mean_mag=12.0827 delta=1.26 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:29.62 +22:06:17.0: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry filter KEPT candidate at 12:47:29.62 +22:06:17.0: ref_mag=13.76 +/- 0.03 new_mean_mag=12.3948 delta=1.37 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:32.49 +22:18:54.9: 13.05 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:32.49 +22:18:54.9: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 12:47:32.49 +22:18:54.9: ref_mag=13.05 +/- 0.02 new_mean_mag=12.0184 delta=1.03 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:46:51.86 +22:48:12.6: 13.01 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:24.57 +19:30:11.8: 13.02 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:24.09 +20:07:43.3: 12.99 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:46:51.86 +22:48:12.6: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 12:46:51.86 +22:48:12.6: ref_mag=12.97 +/- 0.01 new_mean_mag=12.0011 delta=0.97 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:24.57 +19:30:11.8: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 12:53:24.57 +19:30:11.8: ref_mag=13.00 +/- 0.02 new_mean_mag=12.0187 delta=0.98 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:24.09 +20:07:43.3: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry filter KEPT candidate at 12:51:24.09 +20:07:43.3: ref_mag=13.00 +/- 0.01 new_mean_mag=11.8974 delta=1.10 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:54:01.46 +19:31:33.3: 13.03 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:54:01.46 +19:31:33.3: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 12:54:01.46 +19:31:33.3: ref_mag=13.02 +/- 0.02 new_mean_mag=12.0199 delta=1.00 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:47.66 +20:58:24.2: 12.74 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:47.66 +20:58:24.2: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 12:49:47.66 +20:58:24.2: ref_mag=12.73 +/- 0.01 new_mean_mag=11.6613 delta=1.07 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:44:37.29 +23:21:45.5: 12.70 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:44:37.29 +23:21:45.5: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 12:44:37.29 +23:21:45.5: ref_mag=12.68 +/- 0.01 new_mean_mag=11.7237 delta=0.96 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:23.91 +20:54:06.5: 12.71 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:03.95 +20:31:37.8: 12.70 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:23.91 +20:54:06.5: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 12:50:23.91 +20:54:06.5: ref_mag=12.70 +/- 0.01 new_mean_mag=11.6369 delta=1.06 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:03.95 +20:31:37.8: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 12:49:03.95 +20:31:37.8: ref_mag=12.67 +/- 0.01 new_mean_mag=11.7449 delta=0.93 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:31.57 +22:09:55.7: 12.97 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:38.19 +21:05:54.3: 14.05 +/- 0.06 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:31.57 +22:09:55.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:38.19 +21:05:54.3: 14.10 +/- 0.05 detection
Forced photometry filter KEPT candidate at 12:49:31.57 +22:09:55.7: ref_mag=12.94 +/- 0.01 new_mean_mag=12.0245 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 14.07 +/- 0.04
Forced photometry filter KEPT candidate at 12:49:38.19 +21:05:54.3: ref_mag=14.07 +/- 0.04 new_mean_mag=12.6647 delta=1.41 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:43.99 +20:06:43.4: 13.46 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:15.12 +21:06:49.7: 13.30 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:43.99 +20:06:43.4: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 12:51:43.99 +20:06:43.4: ref_mag=13.45 +/- 0.02 new_mean_mag=12.2373 delta=1.21 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:15.12 +21:06:49.7: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 12:51:15.12 +21:06:49.7: ref_mag=13.26 +/- 0.02 new_mean_mag=12.3174 delta=0.95 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:31.58 +20:33:23.3: 13.27 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:31.58 +20:33:23.3: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 12:51:31.58 +20:33:23.3: ref_mag=13.32 +/- 0.02 new_mean_mag=12.0971 delta=1.23 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:57.04 +21:13:30.8: 12.35 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:57.04 +21:13:30.8: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 12:49:57.04 +21:13:30.8: ref_mag=12.36 +/- 0.01 new_mean_mag=11.3522 delta=1.01 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:19.81 +21:08:23.0: 12.65 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:19.81 +21:08:23.0: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 12:49:19.81 +21:08:23.0: ref_mag=12.65 +/- 0.01 new_mean_mag=11.5268 delta=1.12 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:39.27 +22:36:50.3: 12.98 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:39.27 +22:36:50.3: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 12:47:39.27 +22:36:50.3: ref_mag=12.97 +/- 0.01 new_mean_mag=12.0041 delta=0.96 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:15.92 +20:50:31.4: 13.28 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:15.92 +20:50:31.4: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 12:49:15.92 +20:50:31.4: ref_mag=13.27 +/- 0.02 new_mean_mag=12.0014 delta=1.27 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:08.58 +19:34:51.1: 12.33 +/- 0.01 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:49:26.63 +21:15:23.7: 13.27 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:08.58 +19:34:51.1: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 12:53:08.58 +19:34:51.1: ref_mag=12.32 +/- 0.01 new_mean_mag=11.3631 delta=0.96 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:31.11 +20:26:42.9: 13.23 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:49:26.63 +21:15:23.7: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 12:49:26.63 +21:15:23.7: ref_mag=13.25 +/- 0.02 new_mean_mag=12.0697 delta=1.18 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:31.11 +20:26:42.9: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 12:51:31.11 +20:26:42.9: ref_mag=13.21 +/- 0.02 new_mean_mag=11.9326 delta=1.28 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:53:00.63 +20:26:13.4: 13.68 +/- 0.04 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:53:00.63 +20:26:13.4: 13.59 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:47:15.43 +22:27:05.5: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 12:53:00.63 +20:26:13.4: ref_mag=13.62 +/- 0.03 new_mean_mag=12.3876 delta=1.24 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:47:15.43 +22:27:05.5: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 12:47:15.43 +22:27:05.5: ref_mag=13.68 +/- 0.03 new_mean_mag=12.4562 delta=1.22 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:50:30.35 +20:28:23.5: 12.66 +/- 0.02 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-13_01-06-26_20.00sec_-0.00C_LIGHT_0195.fits at 12:51:17.73 +21:08:56.7: 13.23 +/- 0.03 detection
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:50:30.35 +20:28:23.5: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 12:50:30.35 +20:28:23.5: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6093 delta=1.02 (need > 0.90)
Forced photometry on wcs_Com-03-Q2b1x1_2026-05-18_00-32-04_20.00sec_5.00C_LIGHT_1549.fits at 12:51:17.73 +21:08:56.7: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 12:51:17.73 +21:08:56.7: ref_mag=13.25 +/- 0.02 new_mean_mag=12.2083 delta=1.04 (need > 0.90)
Adding exclusion_list_local.txt__out05298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24737.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 144s
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: 57s
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Considering the candidate 23926_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23926_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 23030_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23030_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 14449_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14449_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 17653_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17653_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 21656_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 21656_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 17690_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17690_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 24029_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24029_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 13910_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 13910_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 12927_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 12927_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 05298_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 05298_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 24514_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24514_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 12533_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 12533_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 23673_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23673_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 05437_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 05437_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 11547_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 11547_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 23715_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23715_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 14913_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14913_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 24601_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24601_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 14673_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14673_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 23695_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23695_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 23669_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23669_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 24114_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24114_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 12614_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 12614_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
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Considering the candidate 24609_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24609_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24516_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24516_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08390_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 08390_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17925_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17925_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17797_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17797_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13650_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 13650_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17463_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17463_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03653_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
The candidate 03653_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24338_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24338_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14769_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14769_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24515_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24515_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17489_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17489_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23686_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23686_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05312_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 05312_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23343_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23343_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22870_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 22870_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21531_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 21531_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24570_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24570_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16932_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 16932_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13763_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 13763_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05938_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 05938_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17083_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17083_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14593_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14593_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17371_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17371_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14340_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14340_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17550_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17550_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23957_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23957_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24379_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
The candidate 24379_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23654_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23654_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17018_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17018_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24345_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24345_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17429_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17429_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23474_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23474_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17410_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17410_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09756_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 09756_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24294_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24294_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13726_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 13726_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12165_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 12165_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17148_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17148_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17257_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17257_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14862_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14862_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09996_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 09996_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23114_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23114_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11759_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 11759_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12141_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 12141_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14664_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14664_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11189_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
The candidate 11189_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139 did not pass the final checks
**** FOUND 12:47:02.38 +22:30:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17235_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17235_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24416_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24416_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12213_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 12213_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11652_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 11652_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10513_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 10513_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22320_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 22320_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23761_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23761_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22293_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 22293_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14876_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14876_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09076_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 09076_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17867_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17867_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24606_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24606_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12068_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 12068_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14631_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14631_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23661_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 23661_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14598_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14598_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24737_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24737_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14322_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14322_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14505_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14505_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10956_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 10956_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17715_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 17715_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14130_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
The candidate 14130_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139 did not pass the final checks
**** FOUND 12:49:10.57 +21:17:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22492_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 22492_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14265_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14265_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24439_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24439_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24428_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24428_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11342_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 11342_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24567_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 24567_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14513_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
Preparing report for the candidate 14513_fd_Com-03-Q2b1x1_2026-07-16_23-54-46_20.00sec_5.00C_LIGHT_0139
make_report_in_HTML.sh Phase 2 (HTML assembly): 13s
make_report_in_HTML.sh TOTAL: 214s
Prepared the HTML report for the field Com-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
12:38:54.13 +24:53:08.4
12:39:02.50 +24:52:48.3
13:06:34.11 +24:52:08.1
13:07:44.04 +24:38:42.1
12:43:55.04 +23:38:19.7
12:44:37.29 +23:21:45.5
12:45:16.05 +23:06:47.0
12:47:09.13 +23:00:58.2
12:46:51.86 +22:48:12.6
12:47:39.27 +22:36:50.3
12:47:15.43 +22:27:05.5
12:48:23.71 +22:22:11.9
12:47:32.49 +22:18:54.9
12:47:48.60 +22:16:38.1
12:49:31.57 +22:09:55.7
12:47:55.77 +22:08:26.8
12:49:44.32 +22:08:10.5
12:47:29.62 +22:06:17.0
12:49:11.89 +21:58:00.2
12:49:46.52 +21:56:29.6
12:48:52.96 +21:47:58.3
12:49:33.90 +21:30:36.4
12:50:51.80 +21:28:40.0
12:50:05.81 +21:27:46.0
12:50:18.76 +21:24:05.9
12:49:26.63 +21:15:23.7
12:49:57.04 +21:13:30.8
12:48:57.80 +21:11:53.7
12:51:06.78 +21:10:29.3
12:49:19.81 +21:08:23.0
12:51:17.73 +21:08:56.7
12:52:36.32 +21:07:15.0
12:51:15.12 +21:06:49.7
12:49:38.19 +21:05:54.3
12:48:39.38 +21:04:26.5
12:48:56.74 +21:03:48.1
12:49:46.18 +21:01:04.4
12:50:15.70 +20:59:25.3
12:49:47.66 +20:58:24.2
12:50:15.53 +20:58:02.1
12:51:54.21 +20:15:58.7
12:52:58.90 +20:33:36.0
12:50:10.27 +20:36:53.1
12:51:24.98 +20:38:05.0
12:50:47.02 +20:39:55.3
12:49:13.72 +20:39:33.5
12:52:48.81 +20:42:44.2
12:50:16.66 +20:45:21.9
12:49:14.27 +20:43:44.3
12:52:26.94 +20:45:40.2
12:49:45.46 +20:45:33.2
12:49:06.69 +20:47:18.9
12:53:14.45 +20:50:17.6
12:51:08.57 +20:51:56.1
12:49:15.92 +20:50:31.4
12:49:39.43 +20:53:52.5
12:50:23.91 +20:54:06.5
12:49:36.75 +20:55:44.9
12:53:10.69 +19:21:09.8
12:54:37.85 +19:13:02.9
12:54:01.46 +19:31:33.3
12:53:24.57 +19:30:11.8
12:53:08.58 +19:34:51.1
12:53:01.00 +19:44:50.1
12:51:45.76 +19:49:09.9
12:51:05.67 +19:49:15.6
12:52:42.13 +20:16:36.8
12:52:07.73 +20:00:42.7
12:51:30.09 +20:07:19.7
12:51:43.99 +20:06:43.4
12:51:13.10 +20:05:07.2
12:51:14.80 +20:05:21.2
12:50:53.96 +20:04:53.4
12:51:41.68 +20:06:45.2
12:51:36.23 +20:09:59.6
12:51:24.09 +20:07:43.3
12:52:33.71 +20:13:00.7
12:50:14.19 +20:16:06.9
12:50:58.44 +20:14:14.8
12:50:51.57 +20:16:35.4
12:50:08.39 +20:21:20.6
12:50:26.09 +20:21:57.8
12:50:18.75 +20:23:04.4
12:50:59.65 +20:23:34.6
12:53:00.63 +20:26:13.4
12:51:31.11 +20:26:42.9
12:49:39.84 +20:28:04.9
12:51:26.48 +20:25:58.2
12:50:18.68 +20:27:41.4
12:50:30.35 +20:28:23.5
12:52:00.15 +20:31:44.3
12:49:44.58 +20:32:20.4
12:49:03.95 +20:31:37.8
12:51:26.79 +20:30:16.5
12:51:31.58 +20:33:23.3
########### Completed Com-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 ####
12:52:33.71 +20:13:00.7
12:51:45.76 +19:49:09.9
12:51:06.78 +21:10:29.3
12:53:14.45 +20:50:17.6
12:54:37.85 +19:13:02.9
12:51:08.57 +20:51:56.1
12:50:58.44 +20:14:14.8
12:50:18.76 +21:24:05.9
12:48:52.96 +21:47:58.3
12:38:54.13 +24:53:08.4
12:49:39.84 +20:28:04.9
12:49:11.89 +21:58:00.2
12:51:14.80 +20:05:21.2
13:06:34.11 +24:52:08.1
12:48:23.71 +22:22:11.9
12:51:36.23 +20:09:59.6
12:50:15.53 +20:58:02.1
12:49:44.58 +20:32:20.4
12:48:56.74 +21:03:48.1
12:51:41.68 +20:06:45.2
12:51:13.10 +20:05:07.2
12:50:51.57 +20:16:35.4
12:49:46.52 +21:56:29.6
12:51:26.79 +20:30:16.5
12:50:18.68 +20:27:41.4
12:43:55.04 +23:38:19.7
12:49:36.75 +20:55:44.9
12:49:39.43 +20:53:52.5
12:49:33.90 +21:30:36.4
12:52:26.94 +20:45:40.2
12:50:26.09 +20:21:57.8
12:49:46.18 +21:01:04.4
12:51:26.48 +20:25:58.2
12:49:45.46 +20:45:33.2
12:50:53.96 +20:04:53.4
12:39:02.50 +24:52:48.3
12:52:42.13 +20:16:36.8
12:53:01.00 +19:44:50.1
12:53:10.69 +19:21:09.8
12:52:00.15 +20:31:44.3
12:51:54.21 +20:15:58.7
12:50:05.81 +21:27:46.0
13:07:44.04 +24:38:42.1
12:50:10.27 +20:36:53.1
12:52:36.32 +21:07:15.0
12:52:48.81 +20:42:44.2
12:48:57.80 +21:11:53.7
12:49:06.69 +20:47:18.9
12:50:14.19 +20:16:06.9
12:51:30.09 +20:07:19.7
12:52:58.90 +20:33:36.0
12:50:18.75 +20:23:04.4
12:49:14.27 +20:43:44.3
12:52:07.73 +20:00:42.7
12:50:16.66 +20:45:21.9
12:45:16.05 +23:06:47.0
12:50:08.39 +20:21:20.6
12:50:51.80 +21:28:40.0
12:49:44.32 +22:08:10.5
12:51:24.98 +20:38:05.0
12:49:13.72 +20:39:33.5
12:50:15.70 +20:59:25.3
12:47:09.13 +23:00:58.2
12:51:05.67 +19:49:15.6
12:47:48.60 +22:16:38.1
12:47:55.77 +22:08:26.8
12:48:39.38 +21:04:26.5
12:50:47.02 +20:39:55.3
12:50:59.65 +20:23:34.6
12:47:29.62 +22:06:17.0
12:47:32.49 +22:18:54.9
12:46:51.86 +22:48:12.6
12:53:24.57 +19:30:11.8
12:51:24.09 +20:07:43.3
12:54:01.46 +19:31:33.3
12:49:47.66 +20:58:24.2
12:44:37.29 +23:21:45.5
12:50:23.91 +20:54:06.5
12:49:03.95 +20:31:37.8
12:49:31.57 +22:09:55.7
12:49:38.19 +21:05:54.3
12:51:43.99 +20:06:43.4
12:51:15.12 +21:06:49.7
12:51:31.58 +20:33:23.3
12:49:57.04 +21:13:30.8
12:49:19.81 +21:08:23.0
12:47:39.27 +22:36:50.3
12:49:15.92 +20:50:31.4
12:53:08.58 +19:34:51.1
12:49:26.63 +21:15:23.7
12:51:31.11 +20:26:42.9
12:53:00.63 +20:26:13.4
12:47:15.43 +22:27:05.5
12:50:30.35 +20:28:23.5
12:51:17.73 +21:08:56.7
###################################################################################
12:52:33.71 +20:13:00.7 -- not an asteroid (will add it to exclusion list)
12:51:45.76 +19:49:09.9 -- not an asteroid (will add it to exclusion list)
12:51:06.78 +21:10:29.3 -- not an asteroid (will add it to exclusion list)
12:53:14.45 +20:50:17.6 -- not an asteroid (will add it to exclusion list)
12:54:37.85 +19:13:02.9 -- not an asteroid (will add it to exclusion list)
12:51:08.57 +20:51:56.1 -- not an asteroid (will add it to exclusion list)
12:50:58.44 +20:14:14.8 -- not an asteroid (will add it to exclusion list)
12:50:18.76 +21:24:05.9 -- not an asteroid (will add it to exclusion list)
12:48:52.96 +21:47:58.3 -- not an asteroid (will add it to exclusion list)
12:38:54.13 +24:53:08.4 -- not an asteroid (will add it to exclusion list)
12:49:39.84 +20:28:04.9 -- not an asteroid (will add it to exclusion list)
12:49:11.89 +21:58:00.2 -- not an asteroid (will add it to exclusion list)
12:51:14.80 +20:05:21.2 -- not an asteroid (will add it to exclusion list)
13:06:34.11 +24:52:08.1 -- not an asteroid (will add it to exclusion list)
12:48:23.71 +22:22:11.9 -- not an asteroid (will add it to exclusion list)
12:51:36.23 +20:09:59.6 -- not an asteroid (will add it to exclusion list)
12:50:15.53 +20:58:02.1 -- not an asteroid (will add it to exclusion list)
12:49:44.58 +20:32:20.4 -- not an asteroid (will add it to exclusion list)
12:48:56.74 +21:03:48.1 -- not an asteroid (will add it to exclusion list)
12:51:41.68 +20:06:45.2 -- not an asteroid (will add it to exclusion list)
12:51:13.10 +20:05:07.2 -- not an asteroid (will add it to exclusion list)
12:50:51.57 +20:16:35.4 -- not an asteroid (will add it to exclusion list)
12:49:46.52 +21:56:29.6 -- not an asteroid (will add it to exclusion list)
12:51:26.79 +20:30:16.5 -- not an asteroid (will add it to exclusion list)
12:50:18.68 +20:27:41.4 -- not an asteroid (will add it to exclusion list)
12:43:55.04 +23:38:19.7 -- not an asteroid (will add it to exclusion list)
12:49:36.75 +20:55:44.9 -- not an asteroid (will add it to exclusion list)
12:49:39.43 +20:53:52.5 -- not an asteroid (will add it to exclusion list)
12:49:33.90 +21:30:36.4 -- not an asteroid (will add it to exclusion list)
12:52:26.94 +20:45:40.2 -- not an asteroid (will add it to exclusion list)
12:50:26.09 +20:21:57.8 -- not an asteroid (will add it to exclusion list)
12:49:46.18 +21:01:04.4 -- not an asteroid (will add it to exclusion list)
12:51:26.48 +20:25:58.2 -- not an asteroid (will add it to exclusion list)
12:49:45.46 +20:45:33.2 -- not an asteroid (will add it to exclusion list)
12:50:53.96 +20:04:53.4 -- not an asteroid (will add it to exclusion list)
12:39:02.50 +24:52:48.3 -- not an asteroid (will add it to exclusion list)
12:52:42.13 +20:16:36.8 -- not an asteroid (will add it to exclusion list)
12:53:01.00 +19:44:50.1 -- not an asteroid (will add it to exclusion list)
12:53:10.69 +19:21:09.8 -- not an asteroid (will add it to exclusion list)
12:52:00.15 +20:31:44.3 -- not an asteroid (will add it to exclusion list)
12:51:54.21 +20:15:58.7 -- not an asteroid (will add it to exclusion list)
12:50:05.81 +21:27:46.0 -- not an asteroid (will add it to exclusion list)
13:07:44.04 +24:38:42.1 -- not an asteroid (will add it to exclusion list)
12:50:10.27 +20:36:53.1 -- not an asteroid (will add it to exclusion list)
12:52:36.32 +21:07:15.0 -- not an asteroid (will add it to exclusion list)
12:52:48.81 +20:42:44.2 -- not an asteroid (will add it to exclusion list)
12:48:57.80 +21:11:53.7 -- not an asteroid (will add it to exclusion list)
12:49:06.69 +20:47:18.9 -- not an asteroid (will add it to exclusion list)
12:50:14.19 +20:16:06.9 -- not an asteroid (will add it to exclusion list)
12:51:30.09 +20:07:19.7 -- not an asteroid (will add it to exclusion list)
12:52:58.90 +20:33:36.0 -- not an asteroid (will add it to exclusion list)
12:50:18.75 +20:23:04.4 -- not an asteroid (will add it to exclusion list)
12:49:14.27 +20:43:44.3 -- not an asteroid (will add it to exclusion list)
12:52:07.73 +20:00:42.7 -- not an asteroid (will add it to exclusion list)
12:50:16.66 +20:45:21.9 -- not an asteroid (will add it to exclusion list)
12:45:16.05 +23:06:47.0 -- not an asteroid (will add it to exclusion list)
12:50:08.39 +20:21:20.6 -- not an asteroid (will add it to exclusion list)
12:50:51.80 +21:28:40.0 -- not an asteroid (will add it to exclusion list)
12:49:44.32 +22:08:10.5 -- not an asteroid (will add it to exclusion list)
12:51:24.98 +20:38:05.0 -- not an asteroid (will add it to exclusion list)
12:49:13.72 +20:39:33.5 -- not an asteroid (will add it to exclusion list)
12:50:15.70 +20:59:25.3 -- not an asteroid (will add it to exclusion list)
12:47:09.13 +23:00:58.2 -- not an asteroid (will add it to exclusion list)
12:51:05.67 +19:49:15.6 -- not an asteroid (will add it to exclusion list)
12:47:48.60 +22:16:38.1 -- not an asteroid (will add it to exclusion list)
12:47:55.77 +22:08:26.8 -- not an asteroid (will add it to exclusion list)
12:48:39.38 +21:04:26.5 -- not an asteroid (will add it to exclusion list)
12:50:47.02 +20:39:55.3 -- not an asteroid (will add it to exclusion list)
12:50:59.65 +20:23:34.6 -- not an asteroid (will add it to exclusion list)
12:47:29.62 +22:06:17.0 -- not an asteroid (will add it to exclusion list)
12:47:32.49 +22:18:54.9 -- not an asteroid (will add it to exclusion list)
12:46:51.86 +22:48:12.6 -- not an asteroid (will add it to exclusion list)
12:53:24.57 +19:30:11.8 -- not an asteroid (will add it to exclusion list)
12:51:24.09 +20:07:43.3 -- not an asteroid (will add it to exclusion list)
12:54:01.46 +19:31:33.3 -- not an asteroid (will add it to exclusion list)
12:49:47.66 +20:58:24.2 -- not an asteroid (will add it to exclusion list)
12:44:37.29 +23:21:45.5 -- not an asteroid (will add it to exclusion list)
12:50:23.91 +20:54:06.5 -- not an asteroid (will add it to exclusion list)
12:49:03.95 +20:31:37.8 -- not an asteroid (will add it to exclusion list)
12:49:31.57 +22:09:55.7 -- not an asteroid (will add it to exclusion list)
12:49:38.19 +21:05:54.3 -- not an asteroid (will add it to exclusion list)
12:51:43.99 +20:06:43.4 -- not an asteroid (will add it to exclusion list)
12:51:15.12 +21:06:49.7 -- not an asteroid (will add it to exclusion list)
12:51:31.58 +20:33:23.3 -- not an asteroid (will add it to exclusion list)
12:49:57.04 +21:13:30.8 -- not an asteroid (will add it to exclusion list)
12:49:19.81 +21:08:23.0 -- not an asteroid (will add it to exclusion list)
12:47:39.27 +22:36:50.3 -- not an asteroid (will add it to exclusion list)
12:49:15.92 +20:50:31.4 -- not an asteroid (will add it to exclusion list)
12:53:08.58 +19:34:51.1 -- not an asteroid (will add it to exclusion list)
12:49:26.63 +21:15:23.7 -- not an asteroid (will add it to exclusion list)
12:51:31.11 +20:26:42.9 -- not an asteroid (will add it to exclusion list)
12:53:00.63 +20:26:13.4 -- not an asteroid (will add it to exclusion list)
12:47:15.43 +22:27:05.5 -- not an asteroid (will add it to exclusion list)
12:50:30.35 +20:28:23.5 -- not an asteroid (will add it to exclusion list)
12:51:17.73 +21:08:56.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
12:38:54.13 +24:53:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:39:02.50 +24:52:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:43:55.04 +23:38:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:37.29 +23:21:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:16.05 +23:06:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:51.86 +22:48:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:09.13 +23:00:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:15.43 +22:27:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:29.62 +22:06:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:32.49 +22:18:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:39.27 +22:36:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:48.60 +22:16:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:55.77 +22:08:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:23.71 +22:22:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:39.38 +21:04:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:52.96 +21:47:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:56.74 +21:03:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:57.80 +21:11:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:03.95 +20:31:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:06.69 +20:47:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:11.89 +21:58:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:13.72 +20:39:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:14.27 +20:43:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:15.92 +20:50:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:19.81 +21:08:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:26.63 +21:15:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:31.57 +22:09:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:33.90 +21:30:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:36.75 +20:55:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:38.19 +21:05:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:39.43 +20:53:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:39.84 +20:28:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:44.32 +22:08:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:44.58 +20:32:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:45.46 +20:45:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:46.18 +21:01:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:46.52 +21:56:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:47.66 +20:58:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:57.04 +21:13:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:05.81 +21:27:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:08.39 +20:21:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:10.27 +20:36:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:14.19 +20:16:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:15.53 +20:58:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:15.70 +20:59:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:16.66 +20:45:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:18.68 +20:27:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:18.75 +20:23:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:18.76 +21:24:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:23.91 +20:54:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:26.09 +20:21:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:30.35 +20:28:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:47.02 +20:39:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:51.57 +20:16:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:51.80 +21:28:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:53.96 +20:04:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:58.44 +20:14:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:59.65 +20:23:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:05.67 +19:49:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:06.78 +21:10:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:08.57 +20:51:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:13.10 +20:05:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:14.80 +20:05:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:15.12 +21:06:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:17.73 +21:08:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:24.09 +20:07:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:24.98 +20:38:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:26.48 +20:25:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:26.79 +20:30:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:30.09 +20:07:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:31.11 +20:26:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:31.58 +20:33:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:36.23 +20:09:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:41.68 +20:06:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:43.99 +20:06:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:45.76 +19:49:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:54.21 +20:15:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:00.15 +20:31:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:07.73 +20:00:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:26.94 +20:45:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:33.71 +20:13:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:36.32 +21:07:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:42.13 +20:16:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:48.81 +20:42:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:58.90 +20:33:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:00.63 +20:26:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:01.00 +19:44:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:08.58 +19:34:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:10.69 +19:21:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:14.45 +20:50:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:24.57 +19:30:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:54:01.46 +19:31:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:54:37.85 +19:13:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:34.11 +24:52:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:44.04 +24:38:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
12:38:54.13 +24:53:08.4 -- a known variable star
12:39:02.50 +24:52:48.3 -- a known variable star
12:43:55.04 +23:38:19.7 -- not a known variable star
12:44:37.29 +23:21:45.5 -- not a known variable star
12:45:16.05 +23:06:47.0 -- not a known variable star
12:46:51.86 +22:48:12.6 -- not a known variable star
12:47:09.13 +23:00:58.2 -- not a known variable star
12:47:15.43 +22:27:05.5 -- not a known variable star
12:47:29.62 +22:06:17.0 -- not a known variable star
12:47:32.49 +22:18:54.9 -- not a known variable star
12:47:39.27 +22:36:50.3 -- a known variable star
12:47:48.60 +22:16:38.1 -- not a known variable star
12:47:55.77 +22:08:26.8 -- not a known variable star
12:48:23.71 +22:22:11.9 -- not a known variable star
12:48:39.38 +21:04:26.5 -- not a known variable star
12:48:52.96 +21:47:58.3 -- a known variable star
12:48:56.74 +21:03:48.1 -- not a known variable star
12:48:57.80 +21:11:53.7 -- not a known variable star
12:49:03.95 +20:31:37.8 -- not a known variable star
12:49:06.69 +20:47:18.9 -- not a known variable star
12:49:11.89 +21:58:00.2 -- not a known variable star
12:49:13.72 +20:39:33.5 -- not a known variable star
12:49:14.27 +20:43:44.3 -- not a known variable star
12:49:15.92 +20:50:31.4 -- not a known variable star
12:49:19.81 +21:08:23.0 -- not a known variable star
12:49:26.63 +21:15:23.7 -- a known variable star
12:49:31.57 +22:09:55.7 -- not a known variable star
12:49:33.90 +21:30:36.4 -- not a known variable star
12:49:36.75 +20:55:44.9 -- not a known variable star
12:49:38.19 +21:05:54.3 -- not a known variable star
12:49:39.43 +20:53:52.5 -- a known variable star
12:49:39.84 +20:28:04.9 -- not a known variable star
12:49:44.32 +22:08:10.5 -- not a known variable star
12:49:44.58 +20:32:20.4 -- not a known variable star
12:49:45.46 +20:45:33.2 -- not a known variable star
12:49:46.18 +21:01:04.4 -- not a known variable star
12:49:46.52 +21:56:29.6 -- not a known variable star
12:49:47.66 +20:58:24.2 -- not a known variable star
12:49:57.04 +21:13:30.8 -- not a known variable star
12:50:05.81 +21:27:46.0 -- not a known variable star
12:50:08.39 +20:21:20.6 -- not a known variable star
12:50:10.27 +20:36:53.1 -- not a known variable star
12:50:14.19 +20:16:06.9 -- not a known variable star
12:50:15.53 +20:58:02.1 -- not a known variable star
12:50:15.70 +20:59:25.3 -- not a known variable star
12:50:16.66 +20:45:21.9 -- not a known variable star
12:50:18.68 +20:27:41.4 -- not a known variable star
12:50:18.75 +20:23:04.4 -- not a known variable star
12:50:18.76 +21:24:05.9 -- not a known variable star
12:50:23.91 +20:54:06.5 -- not a known variable star
12:50:26.09 +20:21:57.8 -- not a known variable star
12:50:30.35 +20:28:23.5 -- not a known variable star
12:50:47.02 +20:39:55.3 -- not a known variable star
12:50:51.57 +20:16:35.4 -- not a known variable star
12:50:51.80 +21:28:40.0 -- not a known variable star
12:50:53.96 +20:04:53.4 -- not a known variable star
12:50:58.44 +20:14:14.8 -- not a known variable star
12:50:59.65 +20:23:34.6 -- not a known variable star
12:51:05.67 +19:49:15.6 -- not a known variable star
12:51:06.78 +21:10:29.3 -- not a known variable star
12:51:08.57 +20:51:56.1 -- not a known variable star
12:51:13.10 +20:05:07.2 -- not a known variable star
12:51:14.80 +20:05:21.2 -- not a known variable star
12:51:15.12 +21:06:49.7 -- not a known variable star
12:51:17.73 +21:08:56.7 -- not a known variable star
12:51:24.09 +20:07:43.3 -- not a known variable star
12:51:24.98 +20:38:05.0 -- not a known variable star
12:51:26.48 +20:25:58.2 -- not a known variable star
12:51:26.79 +20:30:16.5 -- not a known variable star
12:51:30.09 +20:07:19.7 -- not a known variable star
12:51:31.11 +20:26:42.9 -- not a known variable star
12:51:31.58 +20:33:23.3 -- not a known variable star
12:51:36.23 +20:09:59.6 -- not a known variable star
12:51:41.68 +20:06:45.2 -- not a known variable star
12:51:43.99 +20:06:43.4 -- not a known variable star
12:51:45.76 +19:49:09.9 -- not a known variable star
12:51:54.21 +20:15:58.7 -- not a known variable star
12:52:00.15 +20:31:44.3 -- not a known variable star
12:52:07.73 +20:00:42.7 -- not a known variable star
12:52:26.94 +20:45:40.2 -- not a known variable star
12:52:33.71 +20:13:00.7 -- not a known variable star
12:52:36.32 +21:07:15.0 -- not a known variable star
12:52:42.13 +20:16:36.8 -- not a known variable star
12:52:48.81 +20:42:44.2 -- not a known variable star
12:52:58.90 +20:33:36.0 -- not a known variable star
12:53:00.63 +20:26:13.4 -- not a known variable star
12:53:01.00 +19:44:50.1 -- not a known variable star
12:53:08.58 +19:34:51.1 -- not a known variable star
12:53:10.69 +19:21:09.8 -- not a known variable star
12:53:14.45 +20:50:17.6 -- not a known variable star
12:53:24.57 +19:30:11.8 -- not a known variable star
12:54:01.46 +19:31:33.3 -- not a known variable star
12:54:37.85 +19:13:02.9 -- not a known variable star
13:06:34.11 +24:52:08.1 -- not a known variable star
13:07:44.04 +24:38:42.1 -- not a known variable star
Found 89 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
95 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 95 (excluding asteroids and hot pixels, 89 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)2461238.70422976 -observatory V36
07:14:41.20 +17:23:21.7 Mercury (4.4mag)
10:39:48.42 +09:35:20.9 Venus (-4.2mag)
04:44:29.22 +22:11:56.0 Mars (1.3mag)
08:22:54.97 +19:51:24.3 Jupiter (-1.8mag)
00:56:27.48 +03:22:13.5 Saturn (0.7mag)
04:08:29.72 +20:48:26.7 Uranus (5.8mag)
00:16:56.85 +00:19:47.8 Neptune (7.7mag)
20:30:16.45 -23:21:01.3 Pluto (14.4mag)
10:14:06.99 +09:49:04.0 Moon (-9.0mag)
-rw-r--r-- 1 apache apache 361 Jul 17 01:00 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461238.70422976:
08:22:57.45 +19:51:16.7 Io (6.0mag)
08:22:53.21 +19:51:32.7 Europa (6.3mag)
08:23:10.15 +19:50:28.2 Ganymede (5.6mag)
08:22:28.77 +19:53:03.3 Callisto (6.8mag)
08:21:08.37 +19:38:36.7 Himalia (15.7mag)
08:22:57.36 +19:51:15.5 Thebe (16.6mag)
08:20:29.23 +19:41:34.2 Elara (17.7mag)
08:26:39.10 +19:41:55.5 Pasiphae (17.9mag)
08:27:28.95 +19:57:31.1 Carme (19.0mag)
00:56:39.48 +03:22:08.6 Titan (8.5mag)
00:56:32.51 +03:22:08.4 Rhea (9.8mag)
00:55:52.73 +03:20:12.3 Iapetus (11.2mag)
00:56:13.57 +03:22:16.0 Hyperion (14.5mag)
00:56:19.05 +03:18:27.5 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 17 01:00 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461238.70422976:
17:57:11.10 -31:22:53.7 JWST
19:42:22.24 +00:08:16.1 Chandra
08:59:13.10 -50:40:22.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 17 01:00 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461238.70422976 -observatory V36
02:45:52.09 +15:13:18.5 17.8mag P/1996 R2 (Lagerkvist)
18:12:53.34 -34:31:28.4 13.8mag P/2010 H2 (Vales)
06:32:30.80 -68:15:45.8 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:03:09.11 +32:33:57.1 17.6mag C/2017 K2 (PANSTARRS)
02:23:17.21 +19:48:53.0 15.7mag P/2021 N1 (ZTF)
22:55:13.60 +32:14:23.2 17.3mag C/2022 E2 (ATLAS)
06:20:08.86 +26:51:32.3 16.7mag C/2022 N2 (PANSTARRS)
10:01:32.14 +29:28:20.9 16.9mag C/2022 QE78 (ATLAS)
09:14:11.37 +05:07:03.5 17.9mag C/2022 R6 (PANSTARRS)
18:03:08.99 +21:00:12.8 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:05.06 -11:33:22.6 17.8mag P/2023 B1 (PANSTARRS)
21:40:40.26 +67:30:53.8 17.8mag C/2023 H5 (Lemmon)
16:18:02.51 -10:47:17.2 14.0mag C/2023 R1 (PANSTARRS)
08:12:42.28 +66:05:15.9 17.9mag C/2024 A1 (ATLAS)
07:41:40.93 +30:20:37.2 14.8mag C/2024 E1 (Wierzchos)
15:13:14.20 +15:28:56.7 17.6mag C/2024 G6 (ATLAS)
19:32:24.77 +40:38:29.7 13.7mag C/2024 J3 (ATLAS)
21:40:07.67 +46:59:22.9 17.8mag C/2024 R4 (PANSTARRS)
04:56:02.62 -13:30:30.7 15.7mag C/2024 T5 (ATLAS)
06:40:09.79 +27:55:30.0 18.0mag C/2025 J1 (Borisov)
07:18:58.54 -13:31:42.0 16.8mag C/2025 R3 (PANSTARRS)
10:04:12.01 +22:07:44.7 17.6mag C/2025 V2 (Rankin)
12:47:05.90 +03:37:37.6 17.1mag C/2025 Y1 (ATLAS)
16:33:37.83 +79:08:53.0 17.2mag C/2026 A2 (Bok)
02:53:08.46 +45:31:26.7 16.8mag C/2026 B2 (Sun-Gao)
11:30:01.82 +05:41:58.2 17.0mag A/2026 E1
21:29:34.74 -17:40:44.8 7.1mag 10P/Tempel
11:16:46.21 -02:11:38.0 16.2mag 29P/Schwassmann-Wachmann
04:09:57.56 +30:17:11.8 17.9mag 47P/Ashbrook-Jackson
10:22:21.87 +11:49:00.9 17.1mag 63P/Wild
00:51:02.69 -05:02:46.7 15.5mag 65P/Gunn
04:43:55.86 +20:29:19.6 13.7mag 78P/Gehrels
02:33:05.06 +11:30:51.2 16.3mag 88P/Howell
06:55:42.85 +30:04:09.6 15.8mag 93P/Lovas
04:43:23.25 +31:19:12.6 16.7mag 114P/Wiseman-Skiff
08:25:25.92 +29:54:02.5 15.2mag 123P/West-Hartley
11:00:59.28 -01:35:25.6 16.9mag 124P/Mrkos
05:02:41.43 +20:59:17.0 16.2mag 128P/Shoemaker-Holt
05:49:06.33 +19:37:56.9 17.8mag 131P/Mueller
07:38:05.27 +15:30:06.3 16.4mag 141P-D/Machholz
03:19:27.32 -20:33:49.8 15.1mag 161P/Hartley-IRAS
05:57:47.35 +35:18:39.2 15.4mag 162P/SidingSpring
18:43:29.00 +19:41:46.1 14.1mag 169P/NEAT
01:57:08.41 +08:18:39.0 17.6mag 220P/McNaught
16:35:30.69 -08:41:21.7 17.2mag 235P/LINEAR
08:59:38.15 +32:38:51.5 18.0mag 240P/NEAT
20:38:38.06 -50:57:25.1 17.8mag 259P/Garradd
02:18:35.69 +15:17:46.5 15.6mag 260P/McNaught
05:58:05.73 +37:19:35.0 17.4mag 295P/LINEAR
15:06:30.90 +05:25:38.2 17.6mag 391P/Kowalski
08:40:47.06 +19:23:31.8 17.9mag 450P/LONEOS
08:02:28.64 +38:38:33.1 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 17 01:00 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:33:53.06 -07:15:00.80 ASASSN-26eg 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -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
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
19:33:53.06 -07:15:00.80 2026-07-14.15 15.5
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
-rw-r--r-- 1 apache apache 5.6K Jul 17 01:00 asassn_transients_list.txt
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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 17 01:00 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:27:50.004 -06:44:08.56 AT 2026svd 2026-06-26.40 23.3852
04:22:38.209 -47:20:55.00 AT 2026svc 2026-06-26.43 22.5609
21:50:00.261 -07:57:05.98 AT 2026svb 2026-06-26.41 23.0326
00:44:37.185 -43:22:31.83 AT 2026sva 2026-06-26.42 21.6706
21:35:19.036 -19:34:24.34 AT 2026suz 2026-06-26.41 23.3439
22:40:47.013 -09:25:04.67 AT 2026suy 2026-06-26.40 23.289
22:05:53.553 -08:24:29.60 AT 2026sux 2026-06-26.41 22.2593
22:33:25.333 -02:10:00.75 AT 2026suw 2026-06-26.40 22.6919
22:01:05.082 -07:26:52.26 AT 2026suv 2026-06-26.41 22.9876
22:30:12.816 -04:52:34.67 AT 2026suu 2026-06-26.40 21.9579
21:54:55.644 -07:45:32.24 AT 2026sut 2026-06-26.41 21.0171
18:17:40.907 -50:01:40.94 AT 2026sus 2026-07-07.95 19.363
20:17:07.701 -31:44:39.62 SN 2026sur 2026-07-08.18 19.091
03:21:24.733 -45:31:36.65 AT 2026suq 2026-07-08.14 18.759
21:15:50.298 -66:09:30.96 AT 2026sup 2026-07-07.05 18.911
22:32:27.822 -20:22:41.23 AT 2026suo 2026-07-06.46 19.8035
04:03:27.102 -57:43:47.16 AT 2026sun 2026-07-08.15 18.325
23:58:57.947 -03:02:20.39 AT 2026sum 2026-07-08.38 19.6555
00:36:59.677 +43:01:07.64 AT 2026sul 2026-07-05.38 20.0025
14:33:14.800 +42:54:37.00 AT 2026suk 2026-06-30.71 21.4
-rw-r--r-- 1 apache apache 89K Jul 17 01:00 tns_transients_list.txt
