This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ
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 08 22.3767 2461274.8767 11.17 00:02:37.97 -30:02:40.0
14.83353 -78.90291 galactic Scl Second-epoch detections are separated by 2.1" and 4.4 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 2320842718639458048 | 00:02:37.90 -30:02:38.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.269+/-0.035 (F)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:37.97 -30:02:40.0: 12.29 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:37.97 -30:02:40.0: 12.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.20 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2320842718639458048,2461274.8767,11.17,0.05,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
Gaia DR3 2320842718639458048 20260822.3767 11.17CV 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 08 22.3767 2461274.8767 11.22 00:08:50.29 -29:29:46.2
16.26661 -80.33382 galactic Scl Second-epoch detections are separated by 1.3" and 4.2 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 2320755414839175296 | 00:08:50.25 -29:29:46.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.264+/-0.031 (F)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:08:50.29 -29:29:46.2: 12.37 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:08:50.29 -29:29:46.2: 12.40 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320755414839175296,2461274.8767,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320755414839175296 20260822.3767 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.43 00:07:28.73 -30:13:33.4
12.52996 -79.87823 galactic Scl Second-epoch detections are separated by 1.7" and 4.2 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 2320693150697738496 | 00:07:28.68 -30:13:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.437+/-0.030 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:07:28.73 -30:13:33.4: 12.53 +/- 0.07 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:07:28.73 -30:13:33.4: 12.47 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.50 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2320693150697738496,2461274.8767,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320693150697738496 20260822.3767 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.40 00:04:00.72 -29:26:45.2
17.64261 -79.31062 galactic Scl Second-epoch detections are separated by 1.1" and 4.4 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 2320978512620414080 | 00:04:00.86 -29:26:46.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.473+/-0.032 (K)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:04:00.72 -29:26:45.2: 12.66 +/- 0.08 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:04:00.72 -29:26:45.2: 12.69 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320978512620414080,2461274.8767,11.40,0.05,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 2320978512620414080 20260822.3767 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 08 22.3767 2461274.8767 11.06 00:05:38.60 -29:27:36.3
17.22955 -79.65795 galactic Scl Second-epoch detections are separated by 1.3" and 4.4 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 2320934944472221440 | 00:05:38.60 -29:27:36.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.603+/-0.030 (K)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:38.60 -29:27:36.3: 12.00 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:38.60 -29:27:36.3: 12.03 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320934944472221440,2461274.8767,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320934944472221440 20260822.3767 11.06CV 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 08 22.3767 2461274.8767 11.18 00:01:11.07 -29:12:33.3
19.35756 -78.73682 galactic Scl Second-epoch detections are separated by 2.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2332927764473081216 | 00:01:11.03 -29:12:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.540+/-0.032 (K)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:01:11.07 -29:12:33.3: 12.12 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:01:11.07 -29:12:33.3: 12.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2332927764473081216,2461274.8767,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2332927764473081216 20260822.3767 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.18 00:08:19.95 -30:02:58.8
13.23880 -80.10175 galactic Scl Second-epoch detections are separated by 1.1" and 4.4 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 2320655359281006720 | 00:08:19.92 -30:02:58.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.361+/-0.032 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:08:19.95 -30:02:58.8: 12.23 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:08:19.95 -30:02:58.8: 12.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.21 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2320655359281006720,2461274.8767,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320655359281006720 20260822.3767 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.11 00:17:21.57 -29:28:57.7
13.51368 -82.14066 galactic Scl Second-epoch detections are separated by 0.7" and 4.4 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 2320368421105940224 | 00:17:21.59 -29:28:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.431+/-0.032 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:17:21.57 -29:28:57.7: 12.22 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:17:21.57 -29:28:57.7: 12.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320368421105940224,2461274.8767,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320368421105940224 20260822.3767 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.25 00:09:40.29 -29:14:52.4
17.52561 -80.55954 galactic Scl Second-epoch detections are separated by 0.2" and 4.3 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 2321140621866035200 | 00:09:40.23 -29:14:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.529+/-0.033 (K)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:40.29 -29:14:52.4: 12.22 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:40.29 -29:14:52.4: 12.26 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2321140621866035200,2461274.8767,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2321140621866035200 20260822.3767 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.10 00:05:14.31 -29:25:13.3
17.53223 -79.57812 galactic Scl Second-epoch detections are separated by 2.2" and 4.0 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 | Gaia DR3 2320934837097286144 | 00:05:14.34 -29:25:13.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.334+/-0.033 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:14.31 -29:25:13.3: 12.18 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:14.31 -29:25:13.3: 12.04 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320934837097286144,2461274.8767,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320934837097286144 20260822.3767 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.19 23:59:56.64 -29:23:20.5
18.64523 -78.44422 galactic Scl Second-epoch detections are separated by 1.5" and 4.5 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 | DocumentRef: VOTx1798270 | 23:59:56.64 -29:23:20.5 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:59:56.64 -29:23:20.5: 12.17 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:59:56.64 -29:23:20.5: 12.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx1798270,2461274.8767,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx1798270 20260822.3767 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.24 00:02:44.07 -29:27:08.1
17.85286 -79.03526 galactic Scl Second-epoch detections are separated by 1.1" and 4.2 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 2320899996323604736 | 00:02:44.00 -29:27:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.350+/-0.031 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:44.07 -29:27:08.1: 12.14 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:44.07 -29:27:08.1: 12.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320899996323604736,2461274.8767,11.24,0.05,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
Gaia DR3 2320899996323604736 20260822.3767 11.24CV 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 08 22.3767 2461274.8767 11.09 00:09:40.75 -30:02:58.9
12.79871 -80.38346 galactic Scl Second-epoch detections are separated by 1.5" and 4.4 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 2320663846136437376 | 00:09:40.77 -30:02:58.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.667+/-0.033 (K)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:40.75 -30:02:58.9: 12.10 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:40.75 -30:02:58.9: 12.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2320663846136437376,2461274.8767,11.09,0.05,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
Gaia DR3 2320663846136437376 20260822.3767 11.09CV 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 08 22.3767 2461274.8767 11.15 00:10:17.40 -29:40:22.5
14.81448 -80.60413 galactic Scl Second-epoch detections are separated by 0.8" and 4.4 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 | 00:10:17.40 -29:40:22.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:10:17.40 -29:40:22.5: 12.08 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:10:17.40 -29:40:22.5: 12.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8767,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3767 11.15CV 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 08 22.3767 2461274.8767 11.05 00:06:17.82 -29:18:40.3
17.91460 -79.82395 galactic Scl Second-epoch detections are separated by 1.2" and 4.2 pix
The object was found in VSX 0" Gaia DR3 2320959820922837760
Type: ROT
# Max. Min./Amp. JD0 Period
11.850 G 11.900 G 2.137660000000 G
The object was not found in astcheck.
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:06:17.82 -29:18:40.3: 12.08 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:06:17.82 -29:18:40.3: 12.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320959820922837760,2461274.8767,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320959820922837760 20260822.3767 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.04 00:05:35.02 -30:02:09.9
14.12243 -79.52758 galactic Scl Second-epoch detections are separated by 1.7" and 4.5 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 2320620209268098944 | 00:05:35.06 -30:02:10.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.459+/-0.030 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:35.02 -30:02:09.9: 12.07 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:35.02 -30:02:09.9: 12.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.09 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2320620209268098944,2461274.8767,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320620209268098944 20260822.3767 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.12 00:05:36.71 -29:46:28.6
15.52307 -79.59068 galactic Scl Second-epoch detections are separated by 1.2" and 4.2 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 | 00:05:36.71 -29:46:28.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:36.71 -29:46:28.6: 12.05 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:36.71 -29:46:28.6: 12.09 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8767,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3767 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.13 00:11:25.20 -29:36:01.8
14.90300 -80.85973 galactic Scl Second-epoch detections are separated by 0.7" and 4.5 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 2321069600286857856 | 00:11:25.20 -29:36:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.371+/-0.032 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:11:25.20 -29:36:01.8: 12.04 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:11:25.20 -29:36:01.8: 12.10 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2321069600286857856,2461274.8767,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2321069600286857856 20260822.3767 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.04 00:02:11.66 -29:41:39.5
16.71222 -78.87825 galactic Scl Second-epoch detections are separated by 1.2" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2320886222363524992 | 00:02:11.71 -29:41:39.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.386+/-0.033 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:11.66 -29:41:39.5: 12.03 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:11.66 -29:41:39.5: 11.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320886222363524992,2461274.8767,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320886222363524992 20260822.3767 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 10.93 00:03:44.23 -29:19:39.1
18.32326 -79.27067 galactic Scl Second-epoch detections are separated by 1.4" and 4.5 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 2320993218588433024 | 00:03:44.23 -29:19:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.313+/-0.033 (F)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:03:44.23 -29:19:39.1: 12.02 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:03:44.23 -29:19:39.1: 12.03 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320993218588433024,2461274.8767,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320993218588433024 20260822.3767 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 10.97 00:17:02.95 -29:36:21.2
12.78463 -82.04232 galactic Scl Second-epoch detections are separated by 1.2" and 4.4 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 2320365912845011584 | 00:17:02.96 -29:36:20.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.497+/-0.035 (K)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:17:02.95 -29:36:21.2: 11.99 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:17:02.95 -29:36:21.2: 11.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320365912845011584,2461274.8767,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320365912845011584 20260822.3767 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 10.98 00:09:14.94 -29:40:06.4
15.14851 -80.38479 galactic Scl Second-epoch detections are separated by 0.6" and 4.4 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 2320738372408948736 | 00:09:15.00 -29:40:05.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.414+/-0.030 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:14.94 -29:40:06.4: 11.98 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:14.94 -29:40:06.4: 12.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320738372408948736,2461274.8767,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320738372408948736 20260822.3767 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 10.97 00:07:32.28 -29:18:49.3
17.63428 -80.09004 galactic Scl Second-epoch detections are separated by 1.4" and 4.3 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 | DocumentRef: VOTx2053383 | 00:07:32.31 -29:18:49.1 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:07:32.28 -29:18:49.3: 11.97 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:07:32.28 -29:18:49.3: 11.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2053383,2461274.8767,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2053383 20260822.3767 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 10.93 00:09:03.74 -29:43:14.7
14.89793 -80.33362 galactic Scl Second-epoch detections are separated by 2.0" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.54085 2000 GY163 541 8 541 17.1 0 -0
ATTENTION: measured mag 10.93 is 6.2 mag brighter than the predicted asteroid brightness 17.1 - the transient may be an unrelated new object!
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:03.74 -29:43:14.7: 11.97 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:03.74 -29:43:14.7: 11.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461274.8767,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260822.3767 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.03 23:58:10.32 -29:30:32.7
18.33254 -78.04527 galactic Scl Second-epoch detections are separated by 1.3" and 4.5 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 2332939859101016192 | 23:58:10.38 -29:30:33.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.804+/-0.031 (K)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:58:10.32 -29:30:32.7: 11.95 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:58:10.32 -29:30:32.7: 11.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2332939859101016192,2461274.8767,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2332939859101016192 20260822.3767 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 10.98 00:10:30.75 -29:48:12.2
13.96732 -80.62029 galactic Scl Second-epoch detections are separated by 1.3" and 4.5 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 | 00:10:30.75 -29:48:12.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:10:30.75 -29:48:12.2: 11.96 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:10:30.75 -29:48:12.2: 11.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8767,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3767 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 10.93 00:04:33.59 -29:03:02.3
19.66845 -79.48850 galactic Scl Second-epoch detections are separated by 1.4" and 4.3 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 2321029463816744320 | 00:04:33.65 -29:03:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.363+/-0.033 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:04:33.59 -29:03:02.3: 11.89 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:04:33.59 -29:03:02.3: 11.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2321029463816744320,2461274.8767,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2321029463816744320 20260822.3767 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 10.91 00:00:49.76 -29:21:25.7
18.66537 -78.63968 galactic Scl Second-epoch detections are separated by 1.5" and 4.4 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 2332919208898184576 | 00:00:49.70 -29:21:27.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.279+/-0.035 (F)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:00:49.76 -29:21:25.7: 11.87 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:00:49.76 -29:21:25.7: 11.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2332919208898184576,2461274.8767,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2332919208898184576 20260822.3767 10.91CV 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 08 22.3767 2461274.8767 10.86 00:06:16.39 -30:05:56.9
13.58879 -79.65772 galactic Scl Second-epoch detections are separated by 0.2" and 4.3 pix
The object was found in VSX 0" Gaia DR3 2320709647667590784
Type: ROT
# Max. Min./Amp. JD0 Period
11.560 G 11.600 G G
The object was not found in astcheck.
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:06:16.39 -30:05:56.9: 11.80 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:06:16.39 -30:05:56.9: 11.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.80 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2320709647667590784,2461274.8767,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320709647667590784 20260822.3767 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 10.79 00:05:59.13 -29:39:05.4
16.10238 -79.69504 galactic Scl Second-epoch detections are separated by 0.4" and 4.4 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 2320916768170630912 | 00:05:59.07 -29:39:04.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.323+/-0.031 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:59.13 -29:39:05.4: 11.76 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:59.13 -29:39:05.4: 11.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320916768170630912,2461274.8767,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320916768170630912 20260822.3767 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 10.84 00:11:51.59 -30:04:32.9
11.86121 -80.83057 galactic Scl Second-epoch detections are separated by 0.8" and 4.3 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 2320287538281747456 | 00:11:51.56 -30:04:32.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.660+/-0.033 (K)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:11:51.59 -30:04:32.9: 11.76 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:11:51.59 -30:04:32.9: 11.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.78 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2320287538281747456,2461274.8767,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320287538281747456 20260822.3767 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 10.71 00:08:32.42 -30:03:06.2
13.16123 -80.14476 galactic Scl Second-epoch detections are separated by 1.1" and 4.5 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 | DocumentRef: VOTx2156444 | 00:08:32.46 -30:03:06.7 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=0.436+/-0.033 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:08:32.42 -30:03:06.2: 11.68 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:08:32.42 -30:03:06.2: 11.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2156444,2461274.8767,10.71,0.05,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
DocumentRef: VOTx2156444 20260822.3767 10.71CV 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 08 22.3767 2461274.8767 10.54 00:09:55.70 -30:00:59.0
12.90752 -80.44420 galactic Scl Second-epoch detections are separated by 0.4" and 4.2 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 2320670202688035328 | 00:09:55.71 -30:00:58.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.367+/-0.041 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:55.70 -30:00:59.0: 11.45 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:55.70 -30:00:59.0: 11.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.47 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2320670202688035328,2461274.8767,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320670202688035328 20260822.3767 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.41 00:08:40.23 -29:29:35.3
16.32771 -80.29868 galactic Scl Second-epoch detections are separated by 3.1" and 4.2 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 2320755822860246400 | 00:08:40.31 -29:29:35.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.578+/-0.030 (K)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:08:40.23 -29:29:35.3: 12.61 +/- 0.07 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:08:40.23 -29:29:35.3: 12.70 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320755822860246400,2461274.8767,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320755822860246400 20260822.3767 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.45 00:06:38.17 -28:57:06.0
19.87474 -79.95170 galactic Scl Second-epoch detections are separated by 1.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2321020190983174656 | 00:06:38.25 -28:57:06.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.395+/-0.032 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:06:38.17 -28:57:06.0: 12.61 +/- 0.07 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:06:38.17 -28:57:06.0: 12.56 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2321020190983174656,2461274.8767,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2321020190983174656 20260822.3767 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.41 00:05:56.17 -29:45:38.1
15.51830 -79.66244 galactic Scl Second-epoch detections are separated by 3.8" and 4.8 pix
The object was found in VSX 3" Gaia DR3 2320906254090694144
Type: ROT
# Max. Min./Amp. JD0 Period
12.230 G 12.260 G
The object was not found in astcheck.
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:56.17 -29:45:38.1: 12.51 +/- 0.07 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:56.17 -29:45:38.1: 12.63 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320906254090694144,2461274.8767,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320906254090694144 20260822.3767 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.35 00:02:52.40 -29:14:48.2
18.89935 -79.09655 galactic Scl Second-epoch detections are separated by 1.0" and 4.3 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 2333005795438947968 | 00:02:52.41 -29:14:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.032 (G)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:52.40 -29:14:48.2: 12.51 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:52.40 -29:14:48.2: 12.59 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2333005795438947968,2461274.8767,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2333005795438947968 20260822.3767 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.35 00:02:56.39 -30:04:45.0
14.58268 -78.96035 galactic Scl Second-epoch detections are separated by 2.7" and 4.8 pix
The object was found in VSX 0" Gaia DR3 2320795031617857152
Type: RS
# Max. Min./Amp. JD0 Period
12.100 G 12.170 G K
The object was not found in astcheck.
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:56.39 -30:04:45.0: 12.45 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:56.39 -30:04:45.0: 12.40 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.43 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2320795031617857152,2461274.8767,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320795031617857152 20260822.3767 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.39 00:05:14.56 -29:54:24.2
14.90531 -79.48448 galactic Scl Second-epoch detections are separated by 0.3" and 4.4 pix
The object was found in VSX 2" Gaia DR3 2320812486365053696
Type: ROT
# Max. Min./Amp. JD0 Period
12.120 G 12.160 G K
The object was not found in astcheck.
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:14.56 -29:54:24.2: 12.45 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:14.56 -29:54:24.2: 12.53 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320812486365053696,2461274.8767,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320812486365053696 20260822.3767 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.39 00:05:27.53 -29:28:44.1
17.16638 -79.61507 galactic Scl Second-epoch detections are separated by 2.4" and 4.3 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 2320933668866182912 | 00:05:27.52 -29:28:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.316+/-0.034 (F)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:27.53 -29:28:44.1: 12.44 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:27.53 -29:28:44.1: 12.69 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2320933668866182912,2461274.8767,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320933668866182912 20260822.3767 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.35 23:57:08.55 -29:13:03.5
19.85653 -77.86063 galactic Scl Second-epoch detections are separated by 3.3" and 4.5 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 2333147353265924352 | 23:57:08.59 -29:13:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.303+/-0.033 (F)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:57:08.55 -29:13:03.5: 12.47 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:57:08.55 -29:13:03.5: 12.41 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2333147353265924352,2461274.8767,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2333147353265924352 20260822.3767 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.30 23:59:26.63 -30:00:38.9
15.70104 -78.23356 galactic Scl Second-epoch detections are separated by 0.9" and 4.5 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 2326860277057857536 | 23:59:26.66 -30:00:40.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.195+/-0.040 (F)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:59:26.63 -30:00:38.9: 12.37 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:59:26.63 -30:00:38.9: 12.40 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.38 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2326860277057857536,2461274.8767,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2326860277057857536 20260822.3767 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.20 00:05:54.82 -30:06:24.7
13.65061 -79.58039 galactic Scl Second-epoch detections are separated by 2.1" and 4.1 pix
The object was found in VSX 2" Gaia DR3 2320615983021130752
Type: ROT
# Max. Min./Amp. JD0 Period
11.960 G 12.000 G G
The object was not found in astcheck.
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:54.82 -30:06:24.7: 12.32 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:54.82 -30:06:24.7: 12.26 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2320615983021130752,2461274.8767,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2320615983021130752 20260822.3767 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.32 00:10:29.60 -30:02:39.5
12.54933 -80.55483 galactic Scl Second-epoch detections are separated by 0.5" and 4.2 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 | DocumentRef: VOTx2926449 | 00:10:29.60 -30:02:39.5 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:10:29.60 -30:02:39.5: 12.32 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:10:29.60 -30:02:39.5: 12.35 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.34 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2926449,2461274.8767,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2926449 20260822.3767 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.20 00:02:20.76 -29:29:33.8
17.71555 -78.94526 galactic Scl Second-epoch detections are separated by 0.5" and 4.3 pix
The object was found in VSX 1" DW Scl
Type: RS
# Max. Min./Amp. JD0 Period
12.270 V 12.800 V 2451875.10000 3.143300000000 G6/K0III+K3III
The object was not found in astcheck.
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:20.76 -29:29:33.8: 12.32 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:20.76 -29:29:33.8: 12.41 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DW Scl,2461274.8767,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DW Scl 20260822.3767 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3767 2461274.8767 11.29 00:09:07.81 -29:38:54.0
15.29973 -80.36401 galactic Scl Second-epoch detections are separated by 1.6" and 4.2 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 | 00:09:07.81 -29:38:54.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:07.81 -29:38:54.0: 12.33 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:07.81 -29:38:54.0: 12.37 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8767,11.29,0.05,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
target 20260822.3767 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 08 22.3767 2461274.8767 11.32 00:02:12.87 -29:23:25.7
18.26541 -78.93316 galactic Scl Second-epoch detections are separated by 0.9" and 4.4 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 2332909519452014208 | 00:02:12.88 -29:23:25.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.589+/-0.034 (K)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:12.87 -29:23:25.7: 12.27 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:12.87 -29:23:25.7: 12.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2332909519452014208,2461274.8767,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2332909519452014208 20260822.3767 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461228.89270660 07.07.2026 09:25:19.850 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
First image: 2461228.89270660 07.07.2026 09:25:19.850 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Last image: 2461274.87698227 22.08.2026 09:02:41.268 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.60
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: 2 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 1429
Objects passed selection criteria: 1420
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: 853.5
Average stars matched: 817.5 (95.7821 %)
Memory usage VmPeak: 228580 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:08:32 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: 2461228.89270660 07.07.2026 09:25:19.850 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
First image: 2461228.89270660 07.07.2026 09:25:19.850 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Last image: 2461274.87698227 22.08.2026 09:02:41.268 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 54
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.27
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 9315
Objects passed selection criteria: 9282
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 5939.75
Average stars matched: 5630.25 (94.7893 %)
Memory usage VmPeak: 235972 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:09:10 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
SExtractor catalog cache: saved Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.cat to cache
SExtractor catalog cache: saved Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.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/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.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: 2461274.87640796
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits exists and is non-empty
wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits exists and is non-empty
wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits exists and is non-empty
wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits (1st reference image)
verification OK: wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Image size: 937.8'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 23:59:59.880 -25:59:51.98 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/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_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits (1st new image)
verification OK: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.818 -26:01:54.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:59.880 -25:59:51.98
Second-epoch image center 23:59:59.818 -26:01:54.01
Angular distance between the image centers 0.0339 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits (2nd new image)
verification OK: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.350 -26:02:19.55 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:59.880 -25:59:51.98
Second-epoch image center 23:59:59.350 -26:02:19.55
Angular distance between the image centers 0.0410 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 23:59:59.818 -26:01:54.01
Second-epoch second image center 23:59:59.350 -26:02:19.55
Angular distance between the image centers 0.00731 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/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits &> /tmp/tmp.KzPjtvavLO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits &> /tmp/tmp.T7nKKNrHKC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits &> /tmp/tmp.BcrNmZhp65
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits &> /tmp/tmp.y4zmfIINWS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Calibrating the magnitude scale
Found non-empty wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits and wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits and wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat
Found non-empty wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits and wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat
The reference image (wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits) and catalog (wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat) found
'wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 1832 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.0308 to 9.1144 deg, Dec -31.2631 to -20.5811 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 351.0308 to 9.1144 deg, Dec -31.2631 to -20.5811 deg
Loaded 4401 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): 1460 out of 1482 total matches.
Matched with Tycho-2 1482 out of 1832 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.281850
a=0.000000 b=1.000000 c=22.281850
From vast_summary.log: estimated ref. image limiting mag.: -8.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.68
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 1832 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.0308 to 9.1144 deg, Dec -31.2631 to -20.5811 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 351.0308 to 9.1144 deg, Dec -31.2631 to -20.5811 deg
Loaded 4401 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): 1460 out of 1482 total matches.
Matched with Tycho-2 1482 out of 1832 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Forced-photometry filter: calibrated wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits -> calib.txt_param_ref_wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits (aperture=6.4)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 1834 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.0288 to 9.1191 deg, Dec -31.2300 to -20.5810 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 351.0288 to 9.1191 deg, Dec -31.2300 to -20.5810 deg
Loaded 4388 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): 1496 out of 1514 total matches.
Matched with Tycho-2 1514 out of 1834 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
Forced-photometry filter: calibrated wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits -> calib.txt_param_ref_wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
2.3 pix Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
2.7 pix fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
2.3 pix fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Limiting magnitude estimates:
13.7 mag. Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
13.7 mag. Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
11.5 mag. fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
11.7 mag. fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
All-image limiting magnitude estimate: 11.5 (SNR ) 9.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.KzPjtvavLO (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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits' -> 'wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
WCS_IMAGE_NAME=wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
WCS-calibrated image found: wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Checking if the catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat corresponding to the image wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits alredy exist and is non-empty...
Catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat corresponding to the image wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
WCS catalog name: wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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=186, bad_region=377, passed=1832
Got 1832 stars (including 1317 good ones) from the SExtractor catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat
util/solve_plate_with_UCAC5 got 1832 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
RA wraps around 0/360 boundary: field RA 351.0308 through 0 to 9.1144, gap 9.1144 to 351.0308
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 1271 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1269 matched stars entering correct_measured_positions(), 1269 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1269 matched stars entering correct_measured_positions(), 1524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.0294 through 0 to 9.1143, gap 9.1143 to 351.0294
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 1271 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1269 matched stars entering correct_measured_positions(), 1524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 1269 matched stars entering correct_measured_positions(), 1524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 1269 stars left (next iteration limit 1395)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits N_match=1269 sigma_overall_arcsec=0.421 sigma_q1_arcsec=0.376 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.452 sigma_q4_arcsec=0.425 n_q1=428 n_q2=224 n_q3=406 n_q4=211 worst_quadrant_to_overall_ratio=1.074
The image catalog is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits -region wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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.T7nKKNrHKC (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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits' -> 'wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
WCS_IMAGE_NAME=wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
WCS-calibrated image found: wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
Checking if the catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat corresponding to the image wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits alredy exist and is non-empty...
Catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat corresponding to the image wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
WCS catalog name: wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.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=187, bad_region=373, passed=1834
Got 1834 stars (including 1319 good ones) from the SExtractor catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat
util/solve_plate_with_UCAC5 got 1834 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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
RA wraps around 0/360 boundary: field RA 351.0288 through 0 to 9.1191, gap 9.1191 to 351.0288
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.2 to -20.6)
Done reading UCAC5 zone files...
Matched 1275 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1273 matched stars entering correct_measured_positions(), 1273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1273 matched stars entering correct_measured_positions(), 1529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.0291 through 0 to 9.1191, gap 9.1191 to 351.0291
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.2 to -20.6)
Done reading UCAC5 zone files...
Matched 1275 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1273 matched stars entering correct_measured_positions(), 1529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 1273 matched stars entering correct_measured_positions(), 1529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 1273 stars left (next iteration limit 1400)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits N_match=1273 sigma_overall_arcsec=0.387 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.447 sigma_q4_arcsec=0.389 n_q1=432 n_q2=226 n_q3=403 n_q4=212 worst_quadrant_to_overall_ratio=1.156
The image catalog is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits -region wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.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.BcrNmZhp65 (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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
WCS-calibrated image found: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
Checking if the catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
WCS catalog name: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.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=17, bad_region=40, passed=301
Got 301 stars (including 246 good ones) from the SExtractor catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 301 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
RA wraps around 0/360 boundary: field RA 351.1779 through 0 to 8.8163, gap 8.8163 to 351.1779
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.2 to -20.7)
Done reading UCAC5 zone files...
Matched 227 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 227 matched stars entering correct_measured_positions(), 135 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 227 matched stars entering correct_measured_positions(), 153 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.1781 through 0 to 8.8166, gap 8.8166 to 351.1781
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.2 to -20.7)
Done reading UCAC5 zone files...
Matched 228 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 228 matched stars entering correct_measured_positions(), 153 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 228 matched stars entering correct_measured_positions(), 153 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 228 stars left (next iteration limit 249)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=228 robust_rms=5.622 arcsec worst_quadrant_rms=6.737 arcsec
SIP_REFIT: SIP order 3 trial: matched=228 robust_rms=0.433 arcsec worst_quadrant_rms=0.475 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=228 robust_rms_before=1.073 arcsec robust_rms_before_corrected=0.500 arcsec robust_rms_after=0.433 arcsec worst_quadrant_rms_before=0.574 worst_quadrant_rms_after=0.475
verification OK: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
verification OK: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.867 -26:01:54.65 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 301 stars ###
'wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/correct_sextractor_wcs_catalog_usingxy2sky1193956.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 1.073 -> 0.433 arcsec)
WCS_QUALITY_DIAG: file=fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits N_match=228 sigma_overall_arcsec=0.465 sigma_q1_arcsec=0.514 sigma_q2_arcsec=0.363 sigma_q3_arcsec=0.472 sigma_q4_arcsec=0.464 n_q1=46 n_q2=41 n_q3=99 n_q4=42 worst_quadrant_to_overall_ratio=1.104
The image catalog is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits -region wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.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.y4zmfIINWS (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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
WCS_IMAGE_NAME=wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
WCS-calibrated image found: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Checking if the catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits alredy exist and is non-empty...
Catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
WCS catalog name: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.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=20, bad_region=46, passed=309
Got 309 stars (including 243 good ones) from the SExtractor catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat
util/solve_plate_with_UCAC5 got 309 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
RA wraps around 0/360 boundary: field RA 351.1776 through 0 to 8.8163, gap 8.8163 to 351.1776
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.7)
Done reading UCAC5 zone files...
Matched 223 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 223 matched stars entering correct_measured_positions(), 136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 223 matched stars entering correct_measured_positions(), 156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.1778 through 0 to 8.8165, gap 8.8165 to 351.1778
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.7)
Done reading UCAC5 zone files...
Matched 224 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 224 matched stars entering correct_measured_positions(), 155 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 224 matched stars entering correct_measured_positions(), 155 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 224 stars left (next iteration limit 245)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=224 robust_rms=6.003 arcsec worst_quadrant_rms=6.762 arcsec
SIP_REFIT: SIP order 3 trial: matched=224 robust_rms=0.386 arcsec worst_quadrant_rms=0.393 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=224 robust_rms_before=1.018 arcsec robust_rms_before_corrected=0.420 arcsec robust_rms_after=0.386 arcsec worst_quadrant_rms_before=0.442 worst_quadrant_rms_after=0.393
verification OK: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
verification OK: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.401 -26:02:20.09 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 309 stars ###
'wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/correct_sextractor_wcs_catalog_usingxy2sky1193981.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 1.018 -> 0.386 arcsec)
WCS_QUALITY_DIAG: file=fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits N_match=224 sigma_overall_arcsec=0.427 sigma_q1_arcsec=0.397 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.439 sigma_q4_arcsec=0.423 n_q1=44 n_q2=41 n_q3=92 n_q4=47 worst_quadrant_to_overall_ratio=1.029
The image catalog is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits -region wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits to local_wcs_cache/
'wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits' -> 'local_wcs_cache/wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits'
Saving the final (post-refit) wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits to local_wcs_cache/
'wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits' -> 'local_wcs_cache/wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits'
Saving the final (post-refit) wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits to local_wcs_cache/
'wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits' -> 'local_wcs_cache/wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits'
Saving the final (post-refit) wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits to local_wcs_cache/
'wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits' -> 'local_wcs_cache/wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits sigma_overall=0.421 worst_q_ratio=1.074
ref2=Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits sigma_overall=0.387 worst_q_ratio=1.156
new1=fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits sigma_overall=0.465 worst_q_ratio=1.104
new2=fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits sigma_overall=0.427 worst_q_ratio=1.029
reference average sigma_overall=0.404 worst_q_ratio=1.115
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418_astrometric_residuals.png (1269 matched stars from wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419_astrometric_residuals.png (1273 matched stars from wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132_astrometric_residuals.png (228 matched stars from wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133_astrometric_residuals.png (224 matched stars from wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits'
Saving fully-calibrated image wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits'
Preparing the HTML report for the field Scl-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Scl-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
SExtractor catalog cache: saved Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.cat to cache
SExtractor catalog cache: saved Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Creating symlink local_wcs_cache/wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
Creating symlink local_wcs_cache/wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
Creating symlink local_wcs_cache/wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits exists and is non-empty
wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits exists and is non-empty
wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits exists and is non-empty
wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits (1st reference image)
verification OK: wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Image size: 937.8'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 23:59:59.880 -25:59:51.98 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/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_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits (1st new image)
verification OK: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.867 -26:01:54.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:59.880 -25:59:51.98
Second-epoch image center 23:59:59.867 -26:01:54.65
Angular distance between the image centers 0.0341 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits (2nd new image)
verification OK: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.401 -26:02:20.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:59.880 -25:59:51.98
Second-epoch image center 23:59:59.401 -26:02:20.09
Angular distance between the image centers 0.0412 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 23:59:59.867 -26:01:54.65
Second-epoch second image center 23:59:59.401 -26:02:20.09
Angular distance between the image centers 0.00728 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/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits &> /tmp/tmp.NrMLiIqd75
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits &> /tmp/tmp.n6B0uc9Hl9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits &> /tmp/tmp.0Mvg6cQPyr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits &> /tmp/tmp.8YY2JCnlgn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Calibrating the magnitude scale
Found non-empty wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits and wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits and wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat
Found non-empty wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits and wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat
The reference image (wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits) and catalog (wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat) found
'wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 11986 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 350.9560 to 9.1144 deg, Dec -31.2631 to -20.5314 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 350.9560 to 9.1144 deg, Dec -31.2631 to -20.5314 deg
Loaded 4450 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): 3548 out of 3632 total matches.
Matched with Tycho-2 3632 out of 11986 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.108150
a=0.000000 b=1.000000 c=22.108150
From vast_summary.log: estimated ref. image limiting mag.: -8.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.84
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 11986 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 350.9560 to 9.1144 deg, Dec -31.2631 to -20.5314 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 350.9560 to 9.1144 deg, Dec -31.2631 to -20.5314 deg
Loaded 4450 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): 3548 out of 3632 total matches.
Matched with Tycho-2 3632 out of 11986 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Forced-photometry filter: calibrated wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits -> calib.txt_param_ref_wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits (aperture=4.8)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 12014 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 350.9532 to 9.1191 deg, Dec -31.2609 to -20.5233 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 350.9532 to 9.1191 deg, Dec -31.2609 to -20.5233 deg
Loaded 4454 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): 3592 out of 3675 total matches.
Matched with Tycho-2 3675 out of 12014 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
Forced-photometry filter: calibrated wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits -> calib.txt_param_ref_wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 49 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
2.1 pix Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
2.7 pix fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
2.2 pix fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Limiting magnitude estimates:
13.8 mag. Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
13.8 mag. Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
11.8 mag. fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
11.7 mag. fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
All-image limiting magnitude estimate: 11.7 (SNR ) 11.5 (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.NrMLiIqd75 (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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits' -> 'wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
WCS_IMAGE_NAME=wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
WCS-calibrated image found: wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Checking if the catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat corresponding to the image wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits alredy exist and is non-empty...
Catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat corresponding to the image wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
WCS catalog name: wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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=4, blended=392, bad_region=2207, passed=11982
Got 11982 stars (including 9514 good ones) from the SExtractor catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat
util/solve_plate_with_UCAC5 got 11982 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
RA wraps around 0/360 boundary: field RA 350.9560 through 0 to 9.1144, gap 9.1144 to 350.9560
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 4850 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4842 matched stars entering correct_measured_positions(), 4843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4842 matched stars entering correct_measured_positions(), 10305 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.9542 through 0 to 9.1143, gap 9.1143 to 350.9542
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 4852 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 10305 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 10305 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4845 stars left (next iteration limit 5326)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits N_match=4845 sigma_overall_arcsec=0.527 sigma_q1_arcsec=0.507 sigma_q2_arcsec=0.494 sigma_q3_arcsec=0.635 sigma_q4_arcsec=0.457 n_q1=1606 n_q2=902 n_q3=1487 n_q4=850 worst_quadrant_to_overall_ratio=1.205
The image catalog is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits -region wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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.n6B0uc9Hl9 (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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits' -> 'wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
WCS_IMAGE_NAME=wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
WCS-calibrated image found: wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
Checking if the catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat corresponding to the image wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits alredy exist and is non-empty...
Catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat corresponding to the image wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
WCS catalog name: wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=351, bad_region=2140, passed=12012
Got 12012 stars (including 9580 good ones) from the SExtractor catalog wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat
util/solve_plate_with_UCAC5 got 12012 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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
RA wraps around 0/360 boundary: field RA 350.9532 through 0 to 9.1191, gap 9.1191 to 350.9532
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4841 matched stars entering correct_measured_positions(), 4841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4841 matched stars entering correct_measured_positions(), 10400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.9538 through 0 to 9.1190, gap 9.1190 to 350.9538
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4841 matched stars entering correct_measured_positions(), 10400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4841 matched stars entering correct_measured_positions(), 10400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4841 stars left (next iteration limit 5325)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits N_match=4841 sigma_overall_arcsec=0.513 sigma_q1_arcsec=0.485 sigma_q2_arcsec=0.461 sigma_q3_arcsec=0.658 sigma_q4_arcsec=0.462 n_q1=1613 n_q2=908 n_q3=1478 n_q4=842 worst_quadrant_to_overall_ratio=1.282
The image catalog is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits -region wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.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.0Mvg6cQPyr (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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
WCS-calibrated image found: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
Checking if the catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
WCS catalog name: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.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=47, bad_region=269, passed=2261
Got 2261 stars (including 1950 good ones) from the SExtractor catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 2261 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
RA wraps around 0/360 boundary: field RA 351.1393 through 0 to 9.0145, gap 9.0145 to 351.1393
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.7)
Done reading UCAC5 zone files...
Matched 1892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1891 matched stars entering correct_measured_positions(), 1888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1891 matched stars entering correct_measured_positions(), 2054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.1393 through 0 to 9.0151, gap 9.0151 to 351.1393
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.7)
Done reading UCAC5 zone files...
Matched 1893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1892 matched stars entering correct_measured_positions(), 2054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Accuracy estimation diagnostic: 1892 matched stars entering correct_measured_positions(), 2054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.00"
Excluding outliers - 1892 stars left (next iteration limit 2080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=1892 robust_rms=4.921 arcsec worst_quadrant_rms=6.437 arcsec
SIP_REFIT: SIP order 3 trial: matched=1892 robust_rms=1.023 arcsec worst_quadrant_rms=1.036 arcsec
SIP_REFIT: SIP order 5 trial: matched=1892 robust_rms=0.989 arcsec worst_quadrant_rms=1.036 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=1892 robust_rms_before=1.054 arcsec robust_rms_before_corrected=1.021 arcsec robust_rms_after=1.023 arcsec worst_quadrant_rms_before=1.086 worst_quadrant_rms_after=1.036
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.086 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits N_match=1892 sigma_overall_arcsec=0.938 sigma_q1_arcsec=0.988 sigma_q2_arcsec=1.012 sigma_q3_arcsec=0.897 sigma_q4_arcsec=0.904 n_q1=314 n_q2=407 n_q3=818 n_q4=353 worst_quadrant_to_overall_ratio=1.079
The image catalog is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits -region wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.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.8YY2JCnlgn (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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
WCS_IMAGE_NAME=wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
WCS-calibrated image found: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Checking if the catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits alredy exist and is non-empty...
Catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
WCS catalog name: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.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=38, bad_region=315, passed=2611
Got 2611 stars (including 2259 good ones) from the SExtractor catalog wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat
util/solve_plate_with_UCAC5 got 2611 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
RA wraps around 0/360 boundary: field RA 351.1135 through 0 to 9.0143, gap 9.0143 to 351.1135
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.7)
Done reading UCAC5 zone files...
Matched 2186 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2183 matched stars entering correct_measured_positions(), 2182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2183 matched stars entering correct_measured_positions(), 2385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.1136 through 0 to 9.0147, gap 9.0147 to 351.1136
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.7)
Done reading UCAC5 zone files...
Matched 2186 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2183 matched stars entering correct_measured_positions(), 2385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Accuracy estimation diagnostic: 2183 matched stars entering correct_measured_positions(), 2385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 2183 stars left (next iteration limit 2401)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=2183 robust_rms=5.245 arcsec worst_quadrant_rms=6.500 arcsec
SIP_REFIT: SIP order 3 trial: matched=2183 robust_rms=0.912 arcsec worst_quadrant_rms=0.995 arcsec
SIP_REFIT: SIP order 5 trial: matched=2183 robust_rms=0.881 arcsec worst_quadrant_rms=0.972 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=2183 robust_rms_before=0.933 arcsec robust_rms_before_corrected=0.907 arcsec robust_rms_after=0.912 arcsec worst_quadrant_rms_before=1.000 worst_quadrant_rms_after=0.995
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.000 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits N_match=2183 sigma_overall_arcsec=0.838 sigma_q1_arcsec=0.932 sigma_q2_arcsec=0.865 sigma_q3_arcsec=0.815 sigma_q4_arcsec=0.806 n_q1=386 n_q2=443 n_q3=915 n_q4=439 worst_quadrant_to_overall_ratio=1.111
The image catalog is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits -region wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.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_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-01-51_20.00sec_-0.00C_LIGHT_0132.fits
Saving fully-calibrated image wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.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_2026-08-22_CI_Scl-01-Q2b1x1_040451_TTUQ2b1x1_1051339_TXCyqgWQ/wcs_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133.fits
Preparing the HTML report for the field Scl-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:08:19.95 -30:02:58.8: 12.23 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:37.97 -30:02:40.0: 12.29 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:01:11.07 -29:12:33.3: 12.12 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:38.60 -29:27:36.3: 12.00 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:04:00.72 -29:26:45.2: 12.66 +/- 0.08 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:07:28.73 -30:13:33.4: 12.53 +/- 0.07 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:17:21.57 -29:28:57.7: 12.22 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:08:50.29 -29:29:46.2: 12.37 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:40.29 -29:14:52.4: 12.22 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:14.31 -29:25:13.3: 12.18 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:08:50.29 -29:29:46.2: 12.40 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:08:19.95 -30:02:58.8: 12.20 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:37.97 -30:02:40.0: 12.14 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:01:11.07 -29:12:33.3: 12.13 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:17:21.57 -29:28:57.7: 12.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.04
Forced photometry reference-image weighted average: 12.21 +/- 0.04
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:38.60 -29:27:36.3: 12.03 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:04:00.72 -29:26:45.2: 12.69 +/- 0.08 detection
Forced photometry filter KEPT candidate at 00:08:50.29 -29:29:46.2: ref_mag=12.38 +/- 0.04 new_mean_mag=11.2098 delta=1.17 (need > 0.90)
Forced photometry filter KEPT candidate at 00:08:19.95 -30:02:58.8: ref_mag=12.21 +/- 0.04 new_mean_mag=11.1677 delta=1.05 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:07:28.73 -30:13:33.4: 12.47 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.03
Forced photometry reference-image weighted average: 12.12 +/- 0.03
Forced photometry reference-image weighted average: 12.17 +/- 0.04
Forced photometry filter KEPT candidate at 00:02:37.97 -30:02:40.0: ref_mag=12.20 +/- 0.03 new_mean_mag=11.1592 delta=1.04 (need > 0.90)
Forced photometry reference-image weighted average: 12.02 +/- 0.03
Forced photometry filter KEPT candidate at 00:01:11.07 -29:12:33.3: ref_mag=12.12 +/- 0.03 new_mean_mag=11.1679 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 00:17:21.57 -29:28:57.7: ref_mag=12.17 +/- 0.04 new_mean_mag=11.1054 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.67 +/- 0.05
Forced photometry reference-image weighted average: 12.50 +/- 0.05
Forced photometry filter KEPT candidate at 00:05:38.60 -29:27:36.3: ref_mag=12.02 +/- 0.03 new_mean_mag=11.0596 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 00:04:00.72 -29:26:45.2: ref_mag=12.67 +/- 0.05 new_mean_mag=11.3938 delta=1.28 (need > 0.90)
Forced photometry filter KEPT candidate at 00:07:28.73 -30:13:33.4: ref_mag=12.50 +/- 0.05 new_mean_mag=11.3948 delta=1.10 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:40.29 -29:14:52.4: 12.26 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.04
Forced photometry filter KEPT candidate at 00:09:40.29 -29:14:52.4: ref_mag=12.24 +/- 0.04 new_mean_mag=11.2519 delta=0.99 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:14.31 -29:25:13.3: 12.04 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.03
Forced photometry filter KEPT candidate at 00:05:14.31 -29:25:13.3: ref_mag=12.10 +/- 0.03 new_mean_mag=11.1025 delta=1.00 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:59:56.64 -29:23:20.5: 12.17 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:59:56.64 -29:23:20.5: 12.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.03
Forced photometry filter KEPT candidate at 23:59:56.64 -29:23:20.5: ref_mag=12.16 +/- 0.03 new_mean_mag=11.1854 delta=0.97 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:44.07 -29:27:08.1: 12.14 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:44.07 -29:27:08.1: 12.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.03
Forced photometry filter KEPT candidate at 00:02:44.07 -29:27:08.1: ref_mag=12.17 +/- 0.03 new_mean_mag=11.1743 delta=0.99 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:40.75 -30:02:58.9: 12.10 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:40.75 -30:02:58.9: 12.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.03
Forced photometry filter KEPT candidate at 00:09:40.75 -30:02:58.9: ref_mag=12.12 +/- 0.03 new_mean_mag=11.0847 delta=1.04 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:10:17.40 -29:40:22.5: 12.08 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:06:17.82 -29:18:40.3: 12.08 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:10:17.40 -29:40:22.5: 12.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.03
Forced photometry filter KEPT candidate at 00:10:17.40 -29:40:22.5: ref_mag=12.08 +/- 0.03 new_mean_mag=11.1515 delta=0.93 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:06:17.82 -29:18:40.3: 12.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.03
Forced photometry filter KEPT candidate at 00:06:17.82 -29:18:40.3: ref_mag=12.05 +/- 0.03 new_mean_mag=11.0531 delta=1.00 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:35.02 -30:02:09.9: 12.07 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:35.02 -30:02:09.9: 12.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.03
Forced photometry filter KEPT candidate at 00:05:35.02 -30:02:09.9: ref_mag=12.09 +/- 0.03 new_mean_mag=11.0378 delta=1.05 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:36.71 -29:46:28.6: 12.05 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:11:25.20 -29:36:01.8: 12.04 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:11.66 -29:41:39.5: 12.03 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:03:44.23 -29:19:39.1: 12.02 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:36.71 -29:46:28.6: 12.09 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.03
Forced photometry filter KEPT candidate at 00:05:36.71 -29:46:28.6: ref_mag=12.07 +/- 0.03 new_mean_mag=11.1105 delta=0.96 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:11:25.20 -29:36:01.8: 12.10 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.03
Forced photometry filter KEPT candidate at 00:11:25.20 -29:36:01.8: ref_mag=12.07 +/- 0.03 new_mean_mag=11.1271 delta=0.94 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:11.66 -29:41:39.5: 11.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.03
Forced photometry filter KEPT candidate at 00:02:11.66 -29:41:39.5: ref_mag=11.96 +/- 0.03 new_mean_mag=11.0063 delta=0.96 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:03:44.23 -29:19:39.1: 12.03 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.03
Forced photometry filter KEPT candidate at 00:03:44.23 -29:19:39.1: ref_mag=12.02 +/- 0.03 new_mean_mag=10.9412 delta=1.08 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:17:02.95 -29:36:21.2: 11.99 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:17:02.95 -29:36:21.2: 11.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.03
Forced photometry filter KEPT candidate at 00:17:02.95 -29:36:21.2: ref_mag=11.90 +/- 0.03 new_mean_mag=10.9628 delta=0.93 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:14.94 -29:40:06.4: 11.98 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:07:32.28 -29:18:49.3: 11.97 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:14.94 -29:40:06.4: 12.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.03
Forced photometry filter KEPT candidate at 00:09:14.94 -29:40:06.4: ref_mag=12.00 +/- 0.03 new_mean_mag=10.9783 delta=1.02 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:07:32.28 -29:18:49.3: 11.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.03
Forced photometry filter KEPT candidate at 00:07:32.28 -29:18:49.3: ref_mag=11.97 +/- 0.03 new_mean_mag=10.9759 delta=0.99 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:03.74 -29:43:14.7: 11.97 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:03.74 -29:43:14.7: 11.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.03
Forced photometry filter KEPT candidate at 00:09:03.74 -29:43:14.7: ref_mag=11.98 +/- 0.03 new_mean_mag=10.9265 delta=1.05 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:58:10.32 -29:30:32.7: 11.95 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:58:10.32 -29:30:32.7: 11.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.03
Forced photometry filter KEPT candidate at 23:58:10.32 -29:30:32.7: ref_mag=11.89 +/- 0.03 new_mean_mag=10.9869 delta=0.91 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:10:30.75 -29:48:12.2: 11.96 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:10:30.75 -29:48:12.2: 11.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.03
Forced photometry filter KEPT candidate at 00:10:30.75 -29:48:12.2: ref_mag=11.90 +/- 0.03 new_mean_mag=10.9740 delta=0.93 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:04:33.59 -29:03:02.3: 11.89 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:04:33.59 -29:03:02.3: 11.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.03
Forced photometry filter KEPT candidate at 00:04:33.59 -29:03:02.3: ref_mag=11.89 +/- 0.03 new_mean_mag=10.9249 delta=0.96 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:00:49.76 -29:21:25.7: 11.87 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:00:49.76 -29:21:25.7: 11.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.02
Forced photometry filter KEPT candidate at 00:00:49.76 -29:21:25.7: ref_mag=11.86 +/- 0.02 new_mean_mag=10.9164 delta=0.94 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:06:16.39 -30:05:56.9: 11.80 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:06:16.39 -30:05:56.9: 11.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.03
Forced photometry filter KEPT candidate at 00:06:16.39 -30:05:56.9: ref_mag=11.80 +/- 0.03 new_mean_mag=10.8187 delta=0.98 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:59.13 -29:39:05.4: 11.76 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:59.13 -29:39:05.4: 11.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.02
Forced photometry filter KEPT candidate at 00:05:59.13 -29:39:05.4: ref_mag=11.72 +/- 0.02 new_mean_mag=10.7868 delta=0.94 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:11:51.59 -30:04:32.9: 11.76 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:11:51.59 -30:04:32.9: 11.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.02
Forced photometry filter KEPT candidate at 00:11:51.59 -30:04:32.9: ref_mag=11.78 +/- 0.02 new_mean_mag=10.8329 delta=0.95 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:08:32.42 -30:03:06.2: 11.68 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:55.70 -30:00:59.0: 11.45 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:08:32.42 -30:03:06.2: 11.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.02
Forced photometry filter KEPT candidate at 00:08:32.42 -30:03:06.2: ref_mag=11.68 +/- 0.02 new_mean_mag=10.6761 delta=1.00 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:55.70 -30:00:59.0: 11.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.02
Forced photometry filter KEPT candidate at 00:09:55.70 -30:00:59.0: ref_mag=11.47 +/- 0.02 new_mean_mag=10.5155 delta=0.96 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:08:40.23 -29:29:35.3: 12.61 +/- 0.07 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:08:40.23 -29:29:35.3: 12.70 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.05
Forced photometry filter KEPT candidate at 00:08:40.23 -29:29:35.3: ref_mag=12.65 +/- 0.05 new_mean_mag=11.4105 delta=1.24 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:06:38.17 -28:57:06.0: 12.61 +/- 0.07 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:06:38.17 -28:57:06.0: 12.56 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.05
Forced photometry filter KEPT candidate at 00:06:38.17 -28:57:06.0: ref_mag=12.58 +/- 0.05 new_mean_mag=11.4509 delta=1.13 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:56.17 -29:45:38.1: 12.51 +/- 0.07 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:56.17 -29:45:38.1: 12.63 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.05
Forced photometry filter KEPT candidate at 00:05:56.17 -29:45:38.1: ref_mag=12.57 +/- 0.05 new_mean_mag=11.4133 delta=1.15 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:52.40 -29:14:48.2: 12.51 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:52.40 -29:14:48.2: 12.59 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.05
Forced photometry filter KEPT candidate at 00:02:52.40 -29:14:48.2: ref_mag=12.55 +/- 0.05 new_mean_mag=11.3492 delta=1.20 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:56.39 -30:04:45.0: 12.45 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:56.39 -30:04:45.0: 12.40 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.04
Forced photometry filter KEPT candidate at 00:02:56.39 -30:04:45.0: ref_mag=12.43 +/- 0.04 new_mean_mag=11.3032 delta=1.12 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:14.56 -29:54:24.2: 12.45 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:14.56 -29:54:24.2: 12.53 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.05
Forced photometry filter KEPT candidate at 00:05:14.56 -29:54:24.2: ref_mag=12.49 +/- 0.05 new_mean_mag=11.3864 delta=1.10 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:27.53 -29:28:44.1: 12.44 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:27.53 -29:28:44.1: 12.69 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.05
Forced photometry filter KEPT candidate at 00:05:27.53 -29:28:44.1: ref_mag=12.54 +/- 0.05 new_mean_mag=11.3569 delta=1.18 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:57:08.55 -29:13:03.5: 12.47 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:57:08.55 -29:13:03.5: 12.41 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.04
Forced photometry filter KEPT candidate at 23:57:08.55 -29:13:03.5: ref_mag=12.44 +/- 0.04 new_mean_mag=11.3414 delta=1.09 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:59:26.63 -30:00:38.9: 12.37 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:59:26.63 -30:00:38.9: 12.40 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.04
Forced photometry filter KEPT candidate at 23:59:26.63 -30:00:38.9: ref_mag=12.38 +/- 0.04 new_mean_mag=11.2659 delta=1.12 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:05:54.82 -30:06:24.7: 12.32 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:05:54.82 -30:06:24.7: 12.26 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.04
Forced photometry filter KEPT candidate at 00:05:54.82 -30:06:24.7: ref_mag=12.29 +/- 0.04 new_mean_mag=11.1651 delta=1.12 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:10:29.60 -30:02:39.5: 12.32 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:10:29.60 -30:02:39.5: 12.35 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.04
Forced photometry filter KEPT candidate at 00:10:29.60 -30:02:39.5: ref_mag=12.34 +/- 0.04 new_mean_mag=11.2761 delta=1.06 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:20.76 -29:29:33.8: 12.32 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:20.76 -29:29:33.8: 12.41 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.04
Forced photometry filter KEPT candidate at 00:02:20.76 -29:29:33.8: ref_mag=12.36 +/- 0.04 new_mean_mag=11.1965 delta=1.17 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:09:07.81 -29:38:54.0: 12.33 +/- 0.06 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:09:07.81 -29:38:54.0: 12.37 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.04
Forced photometry filter KEPT candidate at 00:09:07.81 -29:38:54.0: ref_mag=12.35 +/- 0.04 new_mean_mag=11.2698 delta=1.08 (need > 0.90)
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:02:12.87 -29:23:25.7: 12.27 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q2b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:02:12.87 -29:23:25.7: 12.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.04
Forced photometry filter KEPT candidate at 00:02:12.87 -29:23:25.7: ref_mag=12.24 +/- 0.04 new_mean_mag=11.2858 delta=0.95 (need > 0.90)
Adding exclusion_list_local.txt__out00997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02385.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 1094s
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: 25s
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Considering the candidate 21143_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
The candidate 21143_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133 did not pass the final checks
Rejecting candidate due to large distance (27.6") between the two second-epoch detections
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Considering the candidate 21153_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
The candidate 21153_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 01201_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01201_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 01793_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01793_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 00997_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 00997_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 01885_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01885_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 01858_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01858_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 02142_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 02142_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 01182_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01182_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 01733_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01733_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 02061_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 02061_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 01902_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01902_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 01953_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01953_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01883_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01883_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 01165_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01165_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01586_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01586_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02017_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 02017_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01200_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01200_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01495_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01495_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01651_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01651_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01598_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01598_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 02008_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 02008_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01597_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01597_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01593_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01593_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02007_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 02007_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01545_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01545_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01819_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01819_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01428_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01428_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
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Considering the candidate 02292_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 02292_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01979_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01979_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01132_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01132_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01624_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01624_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01115_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01115_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01163_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01163_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01195_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01195_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01803_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01803_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02385_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 02385_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01511_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01511_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02098_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 02098_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01166_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01166_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01340_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01340_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01838_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01838_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02143_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 02143_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01232_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01232_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01121_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01121_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01164_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01164_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01830_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01830_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01617_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01617_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01943_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
Preparing report for the candidate 01943_fd_Scl-01-Q2b1x1_2026-08-22_04-02-41_20.00sec_-0.00C_LIGHT_0133
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 1123s
Prepared the HTML report for the field Scl-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:07:28.73 -30:13:33.4
00:11:51.59 -30:04:32.9
00:05:54.82 -30:06:24.7
00:06:16.39 -30:05:56.9
00:08:32.42 -30:03:06.2
00:10:29.60 -30:02:39.5
00:09:40.75 -30:02:58.9
00:02:56.39 -30:04:45.0
00:08:19.95 -30:02:58.8
00:09:55.70 -30:00:59.0
00:05:35.02 -30:02:09.9
00:02:37.97 -30:02:40.0
23:59:26.63 -30:00:38.9
00:05:14.56 -29:54:24.2
00:10:30.75 -29:48:12.2
00:05:36.71 -29:46:28.6
00:05:56.17 -29:45:38.1
00:09:03.74 -29:43:14.7
00:10:17.40 -29:40:22.5
00:09:14.94 -29:40:06.4
00:17:02.95 -29:36:21.2
00:02:11.66 -29:41:39.5
00:09:07.81 -29:38:54.0
00:05:59.13 -29:39:05.4
00:11:25.20 -29:36:01.8
00:17:21.57 -29:28:57.7
00:08:50.29 -29:29:46.2
00:08:40.23 -29:29:35.3
23:58:10.32 -29:30:32.7
00:02:20.76 -29:29:33.8
00:05:27.53 -29:28:44.1
00:05:38.60 -29:27:36.3
00:02:44.07 -29:27:08.1
00:04:00.72 -29:26:45.2
00:05:14.31 -29:25:13.3
00:02:12.87 -29:23:25.7
23:59:56.64 -29:23:20.5
00:00:49.76 -29:21:25.7
00:07:32.28 -29:18:49.3
00:03:44.23 -29:19:39.1
00:06:17.82 -29:18:40.3
00:09:40.29 -29:14:52.4
00:02:52.40 -29:14:48.2
00:01:11.07 -29:12:33.3
23:57:08.55 -29:13:03.5
00:04:33.59 -29:03:02.3
00:06:38.17 -28:57:06.0
########### Completed Scl-01-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 ####
00:02:37.97 -30:02:40.0
00:08:50.29 -29:29:46.2
00:07:28.73 -30:13:33.4
00:04:00.72 -29:26:45.2
00:05:38.60 -29:27:36.3
00:01:11.07 -29:12:33.3
00:08:19.95 -30:02:58.8
00:17:21.57 -29:28:57.7
00:09:40.29 -29:14:52.4
00:05:14.31 -29:25:13.3
23:59:56.64 -29:23:20.5
00:02:44.07 -29:27:08.1
00:09:40.75 -30:02:58.9
00:10:17.40 -29:40:22.5
00:06:17.82 -29:18:40.3
00:05:35.02 -30:02:09.9
00:05:36.71 -29:46:28.6
00:11:25.20 -29:36:01.8
00:02:11.66 -29:41:39.5
00:03:44.23 -29:19:39.1
00:17:02.95 -29:36:21.2
00:09:14.94 -29:40:06.4
00:07:32.28 -29:18:49.3
00:09:03.74 -29:43:14.7
23:58:10.32 -29:30:32.7
00:10:30.75 -29:48:12.2
00:04:33.59 -29:03:02.3
00:00:49.76 -29:21:25.7
00:06:16.39 -30:05:56.9
00:05:59.13 -29:39:05.4
00:11:51.59 -30:04:32.9
00:08:32.42 -30:03:06.2
00:09:55.70 -30:00:59.0
00:08:40.23 -29:29:35.3
00:06:38.17 -28:57:06.0
00:05:56.17 -29:45:38.1
00:02:52.40 -29:14:48.2
00:02:56.39 -30:04:45.0
00:05:14.56 -29:54:24.2
00:05:27.53 -29:28:44.1
23:57:08.55 -29:13:03.5
23:59:26.63 -30:00:38.9
00:05:54.82 -30:06:24.7
00:10:29.60 -30:02:39.5
00:02:20.76 -29:29:33.8
00:09:07.81 -29:38:54.0
00:02:12.87 -29:23:25.7
###################################################################################
00:02:37.97 -30:02:40.0 -- not an asteroid (will add it to exclusion list)
00:08:50.29 -29:29:46.2 -- not an asteroid (will add it to exclusion list)
00:07:28.73 -30:13:33.4 -- not an asteroid (will add it to exclusion list)
00:04:00.72 -29:26:45.2 -- not an asteroid (will add it to exclusion list)
00:05:38.60 -29:27:36.3 -- not an asteroid (will add it to exclusion list)
00:01:11.07 -29:12:33.3 -- not an asteroid (will add it to exclusion list)
00:08:19.95 -30:02:58.8 -- not an asteroid (will add it to exclusion list)
00:17:21.57 -29:28:57.7 -- not an asteroid (will add it to exclusion list)
00:09:40.29 -29:14:52.4 -- not an asteroid (will add it to exclusion list)
00:05:14.31 -29:25:13.3 -- not an asteroid (will add it to exclusion list)
23:59:56.64 -29:23:20.5 -- not an asteroid (will add it to exclusion list)
00:02:44.07 -29:27:08.1 -- not an asteroid (will add it to exclusion list)
00:09:40.75 -30:02:58.9 -- not an asteroid (will add it to exclusion list)
00:10:17.40 -29:40:22.5 -- not an asteroid (will add it to exclusion list)
00:06:17.82 -29:18:40.3 -- not an asteroid (will add it to exclusion list)
00:05:35.02 -30:02:09.9 -- not an asteroid (will add it to exclusion list)
00:05:36.71 -29:46:28.6 -- not an asteroid (will add it to exclusion list)
00:11:25.20 -29:36:01.8 -- not an asteroid (will add it to exclusion list)
00:02:11.66 -29:41:39.5 -- not an asteroid (will add it to exclusion list)
00:03:44.23 -29:19:39.1 -- not an asteroid (will add it to exclusion list)
00:17:02.95 -29:36:21.2 -- not an asteroid (will add it to exclusion list)
00:09:14.94 -29:40:06.4 -- not an asteroid (will add it to exclusion list)
00:07:32.28 -29:18:49.3 -- not an asteroid (will add it to exclusion list)
00:09:03.74 -29:43:14.7 -- asteroid (will NOT add it to exclusion list)
23:58:10.32 -29:30:32.7 -- not an asteroid (will add it to exclusion list)
00:10:30.75 -29:48:12.2 -- not an asteroid (will add it to exclusion list)
00:04:33.59 -29:03:02.3 -- not an asteroid (will add it to exclusion list)
00:00:49.76 -29:21:25.7 -- not an asteroid (will add it to exclusion list)
00:06:16.39 -30:05:56.9 -- not an asteroid (will add it to exclusion list)
00:05:59.13 -29:39:05.4 -- not an asteroid (will add it to exclusion list)
00:11:51.59 -30:04:32.9 -- not an asteroid (will add it to exclusion list)
00:08:32.42 -30:03:06.2 -- not an asteroid (will add it to exclusion list)
00:09:55.70 -30:00:59.0 -- not an asteroid (will add it to exclusion list)
00:08:40.23 -29:29:35.3 -- not an asteroid (will add it to exclusion list)
00:06:38.17 -28:57:06.0 -- not an asteroid (will add it to exclusion list)
00:05:56.17 -29:45:38.1 -- not an asteroid (will add it to exclusion list)
00:02:52.40 -29:14:48.2 -- not an asteroid (will add it to exclusion list)
00:02:56.39 -30:04:45.0 -- not an asteroid (will add it to exclusion list)
00:05:14.56 -29:54:24.2 -- not an asteroid (will add it to exclusion list)
00:05:27.53 -29:28:44.1 -- not an asteroid (will add it to exclusion list)
23:57:08.55 -29:13:03.5 -- not an asteroid (will add it to exclusion list)
23:59:26.63 -30:00:38.9 -- not an asteroid (will add it to exclusion list)
00:05:54.82 -30:06:24.7 -- not an asteroid (will add it to exclusion list)
00:10:29.60 -30:02:39.5 -- not an asteroid (will add it to exclusion list)
00:02:20.76 -29:29:33.8 -- not an asteroid (will add it to exclusion list)
00:09:07.81 -29:38:54.0 -- not an asteroid (will add it to exclusion list)
00:02:12.87 -29:23:25.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:49.76 -29:21:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:11.07 -29:12:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:11.66 -29:41:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:12.87 -29:23:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:20.76 -29:29:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:37.97 -30:02:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:44.07 -29:27:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:52.40 -29:14:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:56.39 -30:04:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:44.23 -29:19:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:00.72 -29:26:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:33.59 -29:03:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:14.31 -29:25:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:14.56 -29:54:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:27.53 -29:28:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:35.02 -30:02:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:36.71 -29:46:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:38.60 -29:27:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:54.82 -30:06:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:56.17 -29:45:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:59.13 -29:39:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:16.39 -30:05:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:17.82 -29:18:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:38.17 -28:57:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:28.73 -30:13:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:32.28 -29:18:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:19.95 -30:02:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:32.42 -30:03:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:40.23 -29:29:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:50.29 -29:29:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:07.81 -29:38:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:14.94 -29:40:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:40.29 -29:14:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:40.75 -30:02:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:55.70 -30:00:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:17.40 -29:40:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:29.60 -30:02:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:30.75 -29:48:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:25.20 -29:36:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:51.59 -30:04:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:02.95 -29:36:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:21.57 -29:28:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:08.55 -29:13:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:10.32 -29:30:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:26.63 -30:00:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:56.64 -29:23:20.5 -- 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)
00:00:49.76 -29:21:25.7 -- not a known variable star
00:01:11.07 -29:12:33.3 -- not a known variable star
00:02:11.66 -29:41:39.5 -- not a known variable star
00:02:12.87 -29:23:25.7 -- not a known variable star
00:02:20.76 -29:29:33.8 -- a known variable star
00:02:37.97 -30:02:40.0 -- not a known variable star
00:02:44.07 -29:27:08.1 -- not a known variable star
00:02:52.40 -29:14:48.2 -- not a known variable star
00:02:56.39 -30:04:45.0 -- a known variable star
00:03:44.23 -29:19:39.1 -- not a known variable star
00:04:00.72 -29:26:45.2 -- not a known variable star
00:04:33.59 -29:03:02.3 -- not a known variable star
00:05:14.31 -29:25:13.3 -- not a known variable star
00:05:14.56 -29:54:24.2 -- a known variable star
00:05:27.53 -29:28:44.1 -- not a known variable star
00:05:35.02 -30:02:09.9 -- not a known variable star
00:05:36.71 -29:46:28.6 -- not a known variable star
00:05:38.60 -29:27:36.3 -- not a known variable star
00:05:54.82 -30:06:24.7 -- a known variable star
00:05:56.17 -29:45:38.1 -- a known variable star
00:05:59.13 -29:39:05.4 -- not a known variable star
00:06:16.39 -30:05:56.9 -- a known variable star
00:06:17.82 -29:18:40.3 -- a known variable star
00:06:38.17 -28:57:06.0 -- not a known variable star
00:07:28.73 -30:13:33.4 -- not a known variable star
00:07:32.28 -29:18:49.3 -- not a known variable star
00:08:19.95 -30:02:58.8 -- not a known variable star
00:08:32.42 -30:03:06.2 -- not a known variable star
00:08:40.23 -29:29:35.3 -- not a known variable star
00:08:50.29 -29:29:46.2 -- not a known variable star
00:09:07.81 -29:38:54.0 -- not a known variable star
00:09:14.94 -29:40:06.4 -- not a known variable star
00:09:40.29 -29:14:52.4 -- not a known variable star
00:09:40.75 -30:02:58.9 -- not a known variable star
00:09:55.70 -30:00:59.0 -- not a known variable star
00:10:17.40 -29:40:22.5 -- not a known variable star
00:10:29.60 -30:02:39.5 -- not a known variable star
00:10:30.75 -29:48:12.2 -- not a known variable star
00:11:25.20 -29:36:01.8 -- not a known variable star
00:11:51.59 -30:04:32.9 -- not a known variable star
00:17:02.95 -29:36:21.2 -- not a known variable star
00:17:21.57 -29:28:57.7 -- not a known variable star
23:57:08.55 -29:13:03.5 -- not a known variable star
23:58:10.32 -29:30:32.7 -- not a known variable star
23:59:26.63 -30:00:38.9 -- not a known variable star
23:59:56.64 -29:23:20.5 -- not a known variable star
Found 39 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
46 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 46 (excluding asteroids and hot pixels, 39 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)2461274.87640796 -observatory V36
09:45:22.69 +15:18:09.7 Mercury (-1.7mag)
12:50:16.45 -07:47:10.3 Venus (-4.5mag)
06:29:55.61 +23:38:58.1 Mars (1.3mag)
08:55:31.07 +17:52:59.8 Jupiter (-1.8mag)
00:54:49.04 +03:01:30.9 Saturn (0.5mag)
04:13:02.34 +21:00:19.5 Uranus (5.7mag)
00:15:07.91 +00:06:15.8 Neptune (7.7mag)
20:26:50.51 -23:35:12.4 Pluto (14.5mag)
17:28:10.08 -28:27:58.9 Moon (-11.0mag)
-rw-r--r-- 1 apache apache 363 Aug 22 04:08 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461274.87640796:
08:55:34.31 +17:52:44.8 Io (6.1mag)
08:55:38.74 +17:52:25.1 Europa (6.3mag)
08:55:47.28 +17:51:46.0 Ganymede (5.6mag)
08:55:11.82 +17:54:30.3 Callisto (6.9mag)
08:52:59.30 +18:01:01.0 Himalia (15.7mag)
08:55:29.67 +17:53:07.0 Thebe (16.6mag)
08:52:38.55 +17:56:53.0 Elara (17.7mag)
08:59:38.66 +17:26:14.6 Pasiphae (17.9mag)
08:57:44.10 +18:06:35.2 Carme (19.0mag)
00:54:45.33 +03:01:56.3 Titan (8.4mag)
00:54:53.64 +03:01:22.2 Rhea (9.7mag)
00:55:24.50 +03:03:12.0 Iapetus (11.1mag)
00:54:56.81 +03:01:47.8 Hyperion (14.4mag)
00:53:53.79 +02:52:56.1 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Aug 22 04:08 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461274.87640796:
20:11:57.17 -14:02:31.1 JWST
17:36:04.39 +34:45:26.6 Chandra
11:18:22.36 -60:13:28.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 22 04:08 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461274.87640796 -observatory V36
03:28:16.38 +18:26:33.4 17.5mag P/1996 R2 (Lagerkvist)
17:59:54.63 -34:28:34.0 14.2mag P/2010 H2 (Vales)
07:06:31.35 -69:29:28.4 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:13:08.86 +33:18:28.8 17.7mag C/2017 K2 (PANSTARRS)
04:21:09.60 +42:24:48.1 17.5mag P/2021 N1 (ZTF)
22:26:42.86 +30:22:33.7 17.4mag C/2022 E2 (ATLAS)
06:56:55.78 +26:16:59.3 16.8mag C/2022 N2 (PANSTARRS)
10:34:43.57 +27:51:04.4 17.0mag C/2022 QE78 (ATLAS)
09:38:18.98 +05:17:59.3 18.0mag C/2022 R6 (PANSTARRS)
15:15:40.24 -12:52:44.8 18.0mag P/2023 B1 (PANSTARRS)
20:53:24.69 +64:04:04.1 18.0mag C/2023 H5 (Lemmon)
15:36:28.19 -14:14:05.4 14.6mag C/2023 R1 (PANSTARRS)
08:23:16.79 +32:00:48.9 15.5mag C/2024 E1 (Wierzchos)
15:05:42.21 +15:30:15.5 17.8mag C/2024 G6 (ATLAS)
18:46:50.19 +43:29:22.9 13.7mag C/2024 J3 (ATLAS)
20:49:22.81 +49:41:19.1 17.5mag C/2024 R4 (PANSTARRS)
05:25:46.54 -12:53:57.7 15.3mag C/2024 T5 (ATLAS)
07:04:37.29 +21:36:13.8 17.9mag C/2025 J1 (Borisov)
10:53:17.86 +19:57:23.5 17.1mag C/2025 V2 (Rankin)
13:07:24.55 +01:21:10.2 16.9mag C/2025 Y1 (ATLAS)
16:10:31.07 +76:17:14.3 16.5mag C/2026 A2 (Bok)
03:09:55.53 +46:20:59.4 17.3mag C/2026 B2 (Sun-Gao)
11:58:52.25 +09:55:46.9 17.4mag A/2026 E1
22:12:25.26 -32:18:27.8 7.1mag 10P/Tempel
11:37:44.03 -04:19:18.9 16.3mag 29P/Schwassmann-Wachmann
11:36:27.02 +00:01:04.5 17.4mag 63P/Wild
00:51:37.17 -06:06:13.3 15.4mag 65P/Gunn
06:06:49.32 +20:14:31.7 13.7mag 78P/Gehrels
20:25:48.98 -25:00:04.4 17.5mag 84P/Giclas
03:12:00.41 +14:32:17.1 16.9mag 88P/Howell
08:30:32.97 +25:35:00.6 16.4mag 93P/Lovas
04:47:37.53 +22:25:13.4 17.2mag 112P/Urata-Niijima
06:42:37.42 +28:17:40.4 16.1mag 114P/Wiseman-Skiff
09:51:41.63 +24:05:26.4 14.9mag 123P/West-Hartley
12:12:33.50 -15:36:43.7 17.3mag 124P/Mrkos
05:56:46.65 +21:01:44.4 16.0mag 128P/Shoemaker-Holt
06:51:58.81 +18:05:59.0 17.9mag 131P/Mueller
23:59:37.11 +03:05:59.6 17.4mag 139P/Vaisala-Oterma
03:09:36.05 -18:37:32.9 12.8mag 161P/Hartley-IRAS
08:03:40.46 +38:07:18.3 16.1mag 162P/Siding Spring
11:03:59.89 +29:54:24.2 12.2mag 169P/NEAT
03:06:12.33 +09:23:38.1 17.6mag 220P/McNaught
20:16:20.41 -51:48:27.1 18.0mag 259P/Garradd
04:03:19.33 +30:50:10.1 15.3mag 260P/McNaught
07:47:21.44 +37:05:13.5 17.3mag 295P/LINEAR
15:16:11.76 +01:33:09.9 17.8mag 391P/Kowalski
09:13:43.91 +17:40:00.8 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.3K Aug 22 04:08 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
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
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
-rw-r--r-- 1 apache apache 5.7K Aug 22 04:08 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
-rw-r--r-- 1 apache apache 190K Aug 22 04:08 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
08:44:08.771 +29:07:45.05 AT 2026xfr 2026-01-14.38 20.4
23:28:59.311 -21:41:17.71 AT 2026xfq 2026-07-19.57 21.15
20:34:55.430 -31:12:10.98 AT 2026xfp 2026-07-14.44 20
13:01:30.092 +38:12:35.50 AT 2026xfo 2026-06-23.28 20.85
23:22:05.758 +18:57:29.94 AT 2026xfn 2026-07-25.52 21.28
10:13:35.246 -20:37:42.73 AT 2026xfm 2026-01-27.58 21
21:57:25.287 +03:48:20.98 AT 2026xfl 2026-07-16.55 21.68
14:26:07.382 +33:39:52.18 AT 2026xfk 2026-06-13.34 20.9
02:09:31.559 -03:10:04.80 AT 2026xfj 2026-01-17.24 21.98
20:17:01.562 -20:06:27.94 AT 2026xfi 2026-05-20.56 20.93
21:08:09.912 -21:12:24.85 AT 2026xfh 2026-06-19.58 20.9
20:08:20.135 -25:53:36.34 AT 2026xfg 2026-07-19.45 20.74
14:51:25.078 +41:07:07.07 AT 2026xff 2026-06-13.34 21.62
22:33:15.210 +12:04:33.49 AT 2026xfe 2026-06-21.53 20.23
13:52:05.795 +29:21:47.19 AT 2026xfd 2026-04-24.32 20.92
13:30:27.613 +10:38:39.93 AT 2026xfc 2026-04-20.32 21.07
13:40:18.442 +39:30:10.71 AT 2026xfb 2026-05-24.29 20.6
20:02:32.611 -29:31:03.47 AT 2026xfa 2026-06-16.52 19.85
21:35:00.881 +03:50:25.49 AT 2026xez 2026-07-16.55 21.5
08:33:56.550 +06:59:43.01 AT 2026xey 2026-01-24.36 22.17
-rw-r--r-- 1 apache apache 87K Aug 22 04:08 tns_transients_list.txt
