This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980
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 06 08.1743 2461199.6743 10.94 11:30:40.49 -11:13:19.3
273.20883 46.93562 galactic Crt Second-epoch detections are separated by 0.4" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.15 Eunomia -1 -1 1 11.1 0 -0
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:30:40.49 -11:13:19.3: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:30:40.49 -11:13:19.3: 15.70 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6743,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260608.1743 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.68 11:05:57.38 -06:58:04.4
262.28163 47.40627 galactic Crt Second-epoch detections are separated by 1.9" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:05:57.38 -06:58:04.4 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.033 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:57.38 -06:58:04.4: 13.55 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:57.38 -06:58:04.4: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.93 11:16:43.67 -09:08:51.7
267.33091 47.07204 galactic Crt Second-epoch detections are separated by 0.2" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:16:43.67 -09:08:51.7 (user input) | T | P | (position from user input) J-Ks=0.681+/-0.033 (K)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:16:43.67 -09:08:51.7: 14.02 +/- 0.07 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:16:43.67 -09:08:51.7: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.93CV 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 06 08.1743 2461199.6743 12.70 11:32:18.56 -12:16:28.5
274.40770 46.16864 galactic Crt Second-epoch detections are separated by 1.0" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:32:18.56 -12:16:28.5 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.034 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:32:18.56 -12:16:28.5: 13.68 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:32:18.56 -12:16:28.5: 13.63 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461199.6743,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.78 11:05:57.48 -06:28:44.3
261.85698 47.80258 galactic Leo Second-epoch detections are separated by 1.8" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J166.4870-06.4816 | 11:05:57.48 -06:28:44.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.399+/-0.035 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:57.48 -06:28:44.3: 13.66 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:57.48 -06:28:44.3: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 05 57.48 -06 28 44.3 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J166.4870-06.4816,2461199.6743,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J166.4870-06.4816 20260608.1743 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.93 11:12:52.79 -07:50:50.3
265.11402 47.65659 galactic Crt Second-epoch detections are separated by 1.1" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:12:52.79 -07:50:50.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.465+/-0.034 (K)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:12:52.79 -07:50:50.3: 13.95 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:12:52.79 -07:50:50.3: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.93CV 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 06 08.1743 2461199.6743 12.54 11:17:21.46 -08:39:39.7
267.14882 47.56782 galactic Crt Second-epoch detections are separated by 0.7" and 9.3 pix
The object was found in VSX 2" Gaia DR3 3783186144130264576
Type: ROT
# Max. Min./Amp. JD0 Period
13.150 G 13.180 G K
The object was not found in astcheck.
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:17:21.46 -08:39:39.7: 13.51 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:17:21.46 -08:39:39.7: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 3783186144130264576,2461199.6743,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3783186144130264576 20260608.1743 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.64 11:08:28.69 -06:28:21.2
262.61062 48.17343 galactic Leo Second-epoch detections are separated by 0.7" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:08:28.69 -06:28:21.2 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.035 (K)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:08:28.69 -06:28:21.2: 13.48 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:08:28.69 -06:28:21.2: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 08 28.69 -06 28 21.2 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.44 11:06:10.04 -06:41:28.3
262.10482 47.66132 galactic Crt Second-epoch detections are separated by 0.5" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:06:10.04 -06:41:28.3 (user input) | T | P | (position from user input) J-Ks=0.831+/-0.044 (M)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:06:10.04 -06:41:28.3: 13.46 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:06:10.04 -06:41:28.3: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.51 11:05:34.33 -06:39:18.1
261.89578 47.60384 galactic Leo Second-epoch detections are separated by 1.1" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:05:34.33 -06:39:18.1 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.033 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:34.33 -06:39:18.1: 13.48 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:34.33 -06:39:18.1: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 05 34.33 -06 39 18.1 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.38 11:09:03.82 -07:13:21.5
263.43154 47.64338 galactic Crt Second-epoch detections are separated by 0.8" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:09:03.82 -07:13:21.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:09:03.82 -07:13:21.5: 13.32 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:09:03.82 -07:13:21.5: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.58 11:07:02.53 -07:02:53.9
262.67489 47.49762 galactic Crt Second-epoch detections are separated by 1.0" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J166.7606-07.0484 | 11:07:02.53 -07:02:53.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.312+/-0.062 (F)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:07:02.53 -07:02:53.9: 13.45 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:07:02.53 -07:02:53.9: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J166.7606-07.0484,2461199.6743,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J166.7606-07.0484 20260608.1743 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.47 11:19:15.70 -09:28:24.8
268.36426 47.11742 galactic Crt Second-epoch detections are separated by 0.8" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:19:15.70 -09:28:24.8 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.033 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:19:15.70 -09:28:24.8: 13.30 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:19:15.70 -09:28:24.8: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 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,2461199.6743,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.91 11:09:34.50 -07:21:31.8
263.70123 47.60355 galactic Crt Second-epoch detections are separated by 0.7" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:09:34.50 -07:21:31.8 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.035 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:09:34.50 -07:21:31.8: 14.13 +/- 0.07 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:09:34.50 -07:21:31.8: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.91CV 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 06 08.1743 2461199.6743 12.88 11:11:03.29 -07:37:46.3
264.37677 47.58668 galactic Crt Second-epoch detections are separated by 1.4" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:11:03.29 -07:37:46.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.375+/-0.038 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:11:03.29 -07:37:46.3: 13.81 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:11:03.29 -07:37:46.3: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.43 11:08:40.02 -07:33:56.7
263.60124 47.30539 galactic Crt Second-epoch detections are separated by 0.4" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:08:40.02 -07:33:56.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.360+/-0.035 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:08:40.02 -07:33:56.7: 13.42 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:08:40.02 -07:33:56.7: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.75 11:05:41.10 -06:42:56.8
261.98233 47.57116 galactic Crt Second-epoch detections are separated by 0.4" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:05:41.10 -06:42:56.8 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.034 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:41.10 -06:42:56.8: 13.69 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:41.10 -06:42:56.8: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.62 11:04:35.81 -06:39:09.7
261.60411 47.46284 galactic Leo Second-epoch detections are separated by 1.0" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:04:35.81 -06:39:09.7 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.034 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:04:35.81 -06:39:09.7: 13.69 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:04:35.81 -06:39:09.7: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 04 35.81 -06 39 09.7 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.51 11:06:59.85 -07:11:23.0
262.78258 47.37590 galactic Crt Second-epoch detections are separated by 0.8" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:06:59.85 -07:11:23.0 (user input) | T | P | (position from user input) SpType: F4 (LAMOST DR5) J-Ks=0.283+/-0.044 (F)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:06:59.85 -07:11:23.0: 13.40 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:06:59.85 -07:11:23.0: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.28 11:07:05.87 -06:56:38.7
262.60203 47.59054 galactic Crt Second-epoch detections are separated by 1.5" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:07:05.87 -06:56:38.7 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.275+/-0.038 (F)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:07:05.87 -06:56:38.7: 13.26 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:07:05.87 -06:56:38.7: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.69 11:03:45.34 -06:10:48.4
260.93799 47.71815 galactic Leo Second-epoch detections are separated by 0.8" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:03:45.34 -06:10:48.4 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.038 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:03:45.34 -06:10:48.4: 13.80 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:03:45.34 -06:10:48.4: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 03 45.34 -06 10 48.4 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.94 11:07:31.27 -07:12:27.9
262.95465 47.43617 galactic Crt Second-epoch detections are separated by 2.2" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:07:31.27 -07:12:27.9 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.036 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:07:31.27 -07:12:27.9: 14.06 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:07:31.27 -07:12:27.9: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461199.6743,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.85 11:06:50.95 -06:39:42.1
262.28333 47.78426 galactic Leo Second-epoch detections are separated by 2.1" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:06:50.95 -06:39:42.1 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.032 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:06:50.95 -06:39:42.1: 13.93 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:06:50.95 -06:39:42.1: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 06 50.95 -06 39 42.1 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.70 11:30:39.74 -12:08:10.1
273.79811 46.11632 galactic Crt Second-epoch detections are separated by 0.8" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:30:39.74 -12:08:10.1 (user input) | T | P | (position from user input) J-Ks=0.363+/-0.035 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:30:39.74 -12:08:10.1: 13.69 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:30:39.74 -12:08:10.1: 13.65 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461199.6743,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.34 11:05:45.87 -06:17:18.6
261.63167 47.92805 galactic Leo Second-epoch detections are separated by 0.6" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:05:45.87 -06:17:18.6 (user input) | T | P | (position from user input) J-Ks=0.508+/-0.030 (K)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:45.87 -06:17:18.6: 13.25 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:45.87 -06:17:18.6: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 05 45.87 -06 17 18.6 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.72 11:03:54.32 -06:28:49.3
261.24823 47.49955 galactic Leo Second-epoch detections are separated by 1.3" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:03:54.32 -06:28:49.3 (user input) | T | P | (position from user input) J-Ks=0.557+/-0.035 (K)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:03:54.32 -06:28:49.3: 13.68 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:03:54.32 -06:28:49.3: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 03 54.32 -06 28 49.3 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.79 11:08:56.63 -07:04:02.3
263.26339 47.75385 galactic Crt Second-epoch detections are separated by 0.6" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:08:56.63 -07:04:02.3 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.037 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:08:56.63 -07:04:02.3: 13.65 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:08:56.63 -07:04:02.3: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.65 11:28:55.32 -12:01:31.6
273.17828 46.02498 galactic Crt Second-epoch detections are separated by 1.3" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:28:55.32 -12:01:31.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:28:55.32 -12:01:31.6: 13.64 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:28:55.32 -12:01:31.6: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461199.6743,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.64 11:06:55.07 -06:42:28.1
262.34396 47.75675 galactic Crt Second-epoch detections are separated by 0.1" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:06:55.07 -06:42:28.1 (user input) | T | P | (position from user input) J-Ks=0.340+/-0.035 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:06:55.07 -06:42:28.1: 13.65 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:06:55.07 -06:42:28.1: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.86 11:05:20.07 -06:43:50.8
261.89111 47.50787 galactic Crt Second-epoch detections are separated by 2.0" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:05:20.07 -06:43:50.8 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.033 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:20.07 -06:43:50.8: 13.90 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:20.07 -06:43:50.8: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 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,2461199.6743,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.78 11:09:07.36 -07:19:42.3
263.53880 47.56481 galactic Crt Second-epoch detections are separated by 1.8" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:09:07.36 -07:19:42.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.305+/-0.037 (F)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:09:07.36 -07:19:42.3: 13.91 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:09:07.36 -07:19:42.3: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461199.6743,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.77 11:21:06.26 -09:17:08.8
268.80035 47.51039 galactic Crt Second-epoch detections are separated by 1.8" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:21:06.26 -09:17:08.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.481+/-0.039 (K)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:21:06.26 -09:17:08.8: 13.74 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:21:06.26 -09:17:08.8: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.68 11:05:17.96 -06:21:41.9
261.55723 47.80072 galactic Leo Second-epoch detections are separated by 0.3" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:05:17.96 -06:21:41.9 (user input) | T | P | (position from user input) J-Ks=0.396+/-0.035 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:17.96 -06:21:41.9: 13.63 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:17.96 -06:21:41.9: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 05 17.96 -06 21 41.9 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.60 11:08:29.48 -07:17:50.9
263.32225 47.50087 galactic Crt Second-epoch detections are separated by 1.0" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:08:29.48 -07:17:50.9 (user input) | T | P | (position from user input) J-Ks=0.293+/-0.034 (F)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:08:29.48 -07:17:50.9: 13.62 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:08:29.48 -07:17:50.9: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.70 11:30:57.65 -11:54:20.3
273.74494 46.35529 galactic Crt Second-epoch detections are separated by 2.6" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:30:57.65 -11:54:20.3 (user input) | T | P | (position from user input) J-Ks=0.411+/-0.046 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:30:57.65 -11:54:20.3: 13.72 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:30:57.65 -11:54:20.3: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461199.6743,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.69 11:07:25.83 -07:14:45.3
262.96000 47.39202 galactic Crt Second-epoch detections are separated by 2.1" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:07:25.83 -07:14:45.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.397+/-0.043 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:07:25.83 -07:14:45.3: 13.74 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:07:25.83 -07:14:45.3: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.70 11:09:54.14 -07:23:27.7
263.82748 47.62303 galactic Crt Second-epoch detections are separated by 0.6" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:09:54.14 -07:23:27.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.597+/-0.037 (K)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:09:54.14 -07:23:27.7: 13.74 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:09:54.14 -07:23:27.7: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.78 11:16:11.08 -09:14:19.7
267.23388 46.92408 galactic Crt Second-epoch detections are separated by 2.5" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:16:11.08 -09:14:19.7 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.551+/-0.031 (K)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:16:11.08 -09:14:19.7: 13.71 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:16:11.08 -09:14:19.7: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.74 11:07:35.34 -06:34:17.0
262.42745 47.96471 galactic Leo Second-epoch detections are separated by 1.3" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:07:35.34 -06:34:17.0 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.035 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:07:35.34 -06:34:17.0: 13.71 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:07:35.34 -06:34:17.0: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 07 35.34 -06 34 17.0 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.69 11:10:50.71 -07:39:41.0
264.33942 47.53119 galactic Crt Second-epoch detections are separated by 0.8" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:10:50.71 -07:39:41.0 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.370+/-0.035 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:10:50.71 -07:39:41.0: 13.59 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:10:50.71 -07:39:41.0: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.64 11:19:29.88 -09:25:55.1
268.40661 47.18297 galactic Crt Second-epoch detections are separated by 1.2" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:19:29.88 -09:25:55.1 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.032 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:19:29.88 -09:25:55.1: 13.59 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:19:29.88 -09:25:55.1: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.49 11:33:45.85 -12:15:18.9
274.85924 46.33953 galactic Crt Second-epoch detections are separated by 1.6" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:33:45.85 -12:15:18.9 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.034 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:33:45.85 -12:15:18.9: 13.36 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:33:45.85 -12:15:18.9: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.85 11:05:23.93 -06:28:05.2
261.68054 47.72946 galactic Leo Second-epoch detections are separated by 1.5" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:05:23.93 -06:28:05.2 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.037 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:23.93 -06:28:05.2: 14.03 +/- 0.07 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:23.93 -06:28:05.2: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 05 23.93 -06 28 05.2 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.45 11:06:15.34 -06:28:19.3
261.93998 47.85168 galactic Leo Second-epoch detections are separated by 0.7" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:06:15.34 -06:28:19.3 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.030 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:06:15.34 -06:28:19.3: 13.37 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:06:15.34 -06:28:19.3: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 06 15.34 -06 28 19.3 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1743 2461199.6743 12.63 11:04:24.86 -06:17:57.3
261.23890 47.72036 galactic Leo Second-epoch detections are separated by 1.2" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:04:24.86 -06:17:57.3 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.035 (G)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:04:24.86 -06:17:57.3: 13.55 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:04:24.86 -06:17:57.3: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1743* 11 04 24.86 -06 17 57.3 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6743,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1743 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.71399943 16.04.2026 05:07:59.551 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
First image: 2461146.71399943 16.04.2026 05:07:59.551 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Last image: 2461199.67457476 08.06.2026 04:11:13.259 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.76
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: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5909
Objects passed selection criteria: 5873
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: 3535
Average stars matched: 3444.25 (97.4328 %)
Memory usage VmPeak: 112088 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 00:59:05 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: 2461146.71399943 16.04.2026 05:07:59.551 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
First image: 2461146.71399943 16.04.2026 05:07:59.551 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Last image: 2461199.67457476 08.06.2026 04:11:13.259 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 47
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 36222
Objects passed selection criteria: 36098
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: 22938.2
Average stars matched: 22151.2 (96.569 %)
Memory usage VmPeak: 139272 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 01:01:19 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
SExtractor catalog cache: saved Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat to cache
SExtractor catalog cache: saved Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.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/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.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: 2461199.67404529
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'
Plate-solving the images
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits exists and is non-empty
Saving wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits to local_wcs_cache/
'wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits' -> 'local_wcs_cache/wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits'
wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits exists and is non-empty
Saving wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits to local_wcs_cache/
'wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits' -> 'local_wcs_cache/wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits'
wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits exists and is non-empty
Saving wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits to local_wcs_cache/
'wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits' -> 'local_wcs_cache/wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits'
wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits exists and is non-empty
Saving wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits to local_wcs_cache/
'wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits' -> 'local_wcs_cache/wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits (1st reference image)
verification OK: wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:39.514 -10:01:01.99 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits (1st new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:39.569 -09:59:06.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:39.514 -10:01:01.99
Second-epoch image center 11:08:39.569 -09:59:06.53
Angular distance between the image centers 0.0321 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits (2nd new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:36.930 -09:59:47.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:39.514 -10:01:01.99
Second-epoch image center 11:08:36.930 -09:59:47.08
Angular distance between the image centers 0.0234 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:39.569 -09:59:06.53
Second-epoch second image center 11:08:36.930 -09:59:47.08
Angular distance between the image centers 0.01562 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits &> /tmp/tmp.2d3TEd1NGn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits &> /tmp/tmp.aHwE1R7sXB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits &> /tmp/tmp.B7CBts7txn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits &> /tmp/tmp.1HoTvNBjgB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
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_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
Found non-empty wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
The reference image (wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits) and catalog (wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat) found
'wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat' -> 'wcsmag.cat'
Read 6296 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7581 to 175.3333 deg, Dec -15.6773 to -4.2200 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 158.7581 to 175.3333 deg, Dec -15.6773 to -4.2200 deg
Loaded 5071 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): 3683 out of 3829 total matches.
Matched with Tycho-2 3829 out of 6296 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.798000
a=0.000000 b=1.000000 c=22.798000
From vast_summary.log: estimated ref. image limiting mag.: -7.76
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6296 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7581 to 175.3333 deg, Dec -15.6773 to -4.2200 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 158.7581 to 175.3333 deg, Dec -15.6773 to -4.2200 deg
Loaded 5071 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): 3683 out of 3829 total matches.
Matched with Tycho-2 3829 out of 6296 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits:
Forced-photometry filter: calibrated wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits -> calib.txt_param_ref_wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits (aperture=6.2)
Read 6303 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7581 to 175.3333 deg, Dec -15.6774 to -4.2201 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 158.7581 to 175.3333 deg, Dec -15.6774 to -4.2201 deg
Loaded 5071 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): 3677 out of 3827 total matches.
Matched with Tycho-2 3827 out of 6303 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits:
Forced-photometry filter: calibrated wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits -> calib.txt_param_ref_wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits (aperture=6.2)
____ 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: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
2.2 pix Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
2.2 pix fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
2.2 pix fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
2.1 pix wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
2.2 pix wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Limiting magnitude estimates:
15.0 mag. Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
15.0 mag. Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
12.7 mag. fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
12.7 mag. fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 10.4 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2d3TEd1NGn (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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits' -> 'wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS-calibrated image found: wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Checking if the catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS catalog name: wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=454, passed=6296
Got 6296 stars (including 5835 good ones) from the SExtractor catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
util/solve_plate_with_UCAC5 got 6296 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits N_match=964 sigma_overall_arcsec=0.345 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.328 n_q1=225 n_q2=210 n_q3=245 n_q4=284 worst_quadrant_to_overall_ratio=1.184
The image catalog is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits -region wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.aHwE1R7sXB (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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits' -> 'wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS-calibrated image found: wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Checking if the catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS catalog name: wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=463, passed=6303
Got 6303 stars (including 5835 good ones) from the SExtractor catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat
util/solve_plate_with_UCAC5 got 6303 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6227 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 6227 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits N_match=964 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.348 sigma_q2_arcsec=0.434 sigma_q3_arcsec=0.302 sigma_q4_arcsec=0.328 n_q1=230 n_q2=202 n_q3=245 n_q4=287 worst_quadrant_to_overall_ratio=1.277
The image catalog is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits -region wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.B7CBts7txn (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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=44, passed=856
Got 856 stars (including 810 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat
util/solve_plate_with_UCAC5 got 856 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 429 (Dec -15.6 to -4.4)
Done reading UCAC5 zone files...
Matched 780 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 780 matched stars entering correct_measured_positions(), 762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 780 matched stars entering correct_measured_positions(), 830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 429 (Dec -15.6 to -4.4)
Done reading UCAC5 zone files...
Matched 780 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 780 matched stars entering correct_measured_positions(), 829 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 780 matched stars entering correct_measured_positions(), 829 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 780 stars left (next iteration limit 858)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits N_match=780 sigma_overall_arcsec=0.311 sigma_q1_arcsec=0.310 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.487 n_q1=302 n_q2=132 n_q3=296 n_q4=50 worst_quadrant_to_overall_ratio=1.566
The image catalog is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits -region wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1HoTvNBjgB (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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=47, passed=795
Got 795 stars (including 747 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat
util/solve_plate_with_UCAC5 got 795 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 428 (Dec -15.5 to -4.7)
Done reading UCAC5 zone files...
Matched 719 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 719 matched stars entering correct_measured_positions(), 698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 719 matched stars entering correct_measured_positions(), 765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 428 (Dec -15.5 to -4.7)
Done reading UCAC5 zone files...
Matched 719 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 719 matched stars entering correct_measured_positions(), 764 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 719 matched stars entering correct_measured_positions(), 764 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 719 stars left (next iteration limit 790)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits N_match=719 sigma_overall_arcsec=0.326 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.357 sigma_q3_arcsec=0.325 sigma_q4_arcsec=0.501 n_q1=339 n_q2=73 n_q3=241 n_q4=66 worst_quadrant_to_overall_ratio=1.536
The image catalog is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits -region wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits sigma_overall=0.345 worst_q_ratio=1.184
ref2=Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits sigma_overall=0.340 worst_q_ratio=1.277
new1=fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits sigma_overall=0.311 worst_q_ratio=1.566
new2=fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits sigma_overall=0.326 worst_q_ratio=1.536
reference average sigma_overall=0.3425 worst_q_ratio=1.2305
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077_astrometric_residuals.png (see messages above)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits'
Saving fully-calibrated image wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits'
Preparing the HTML report for the field Crt-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Crt-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
SExtractor catalog cache: saved Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat to cache
SExtractor catalog cache: saved Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Creating symlink local_wcs_cache/wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits exists and is non-empty
wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits exists and is non-empty
wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits exists and is non-empty
wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits (1st reference image)
verification OK: wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:39.514 -10:01:01.99 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits (1st new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:39.569 -09:59:06.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:39.514 -10:01:01.99
Second-epoch image center 11:08:39.569 -09:59:06.53
Angular distance between the image centers 0.0321 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits (2nd new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:36.930 -09:59:47.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:39.514 -10:01:01.99
Second-epoch image center 11:08:36.930 -09:59:47.08
Angular distance between the image centers 0.0234 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:39.569 -09:59:06.53
Second-epoch second image center 11:08:36.930 -09:59:47.08
Angular distance between the image centers 0.01562 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits &> /tmp/tmp.oAbCnUoqZV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits &> /tmp/tmp.yf8EqJY0Tt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits &> /tmp/tmp.xoc2FRovIC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits &> /tmp/tmp.94tmrmzyIQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.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_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
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_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
Found non-empty wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits and wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
The reference image (wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits) and catalog (wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat) found
'wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat' -> 'wcsmag.cat'
Read 39431 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7287 to 175.3638 deg, Dec -15.6780 to -4.2043 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 158.7287 to 175.3638 deg, Dec -15.6780 to -4.2043 deg
Loaded 5089 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): 3634 out of 3983 total matches.
Matched with Tycho-2 3983 out of 39431 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.670250
a=0.000000 b=1.000000 c=22.670250
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 39431 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7287 to 175.3638 deg, Dec -15.6780 to -4.2043 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 158.7287 to 175.3638 deg, Dec -15.6780 to -4.2043 deg
Loaded 5089 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): 3634 out of 3983 total matches.
Matched with Tycho-2 3983 out of 39431 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits:
Forced-photometry filter: calibrated wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits -> calib.txt_param_ref_wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits (aperture=4.7)
Read 39513 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.7263 to 175.3473 deg, Dec -15.6782 to -4.2043 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 158.7263 to 175.3473 deg, Dec -15.6782 to -4.2043 deg
Loaded 5089 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): 3641 out of 3987 total matches.
Matched with Tycho-2 3987 out of 39513 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits:
Forced-photometry filter: calibrated wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits -> calib.txt_param_ref_wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 47 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
2.0 pix Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
2.1 pix fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
2.1 pix fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
2.0 pix wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
2.0 pix wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Limiting magnitude estimates:
15.2 mag. Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
15.2 mag. Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
13.2 mag. fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
13.2 mag. fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.9 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.oAbCnUoqZV (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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits' -> 'wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS-calibrated image found: wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
Checking if the catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits
WCS catalog name: wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=1628, passed=39410
Got 39410 stars (including 37728 good ones) from the SExtractor catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat
util/solve_plate_with_UCAC5 got 39410 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 38968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 38966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 38967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits N_match=963 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.406 sigma_q3_arcsec=0.341 sigma_q4_arcsec=0.331 n_q1=220 n_q2=217 n_q3=246 n_q4=280 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits -region wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yf8EqJY0Tt (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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits' -> 'wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS-calibrated image found: wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
Checking if the catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits
WCS catalog name: wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1588, passed=39493
Got 39493 stars (including 37848 good ones) from the SExtractor catalog wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat
util/solve_plate_with_UCAC5 got 39493 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 38958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 38961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 38961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits N_match=964 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.355 sigma_q2_arcsec=0.447 sigma_q3_arcsec=0.323 sigma_q4_arcsec=0.320 n_q1=222 n_q2=209 n_q3=247 n_q4=286 worst_quadrant_to_overall_ratio=1.267
The image catalog is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits -region wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xoc2FRovIC (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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=107, passed=7116
Got 7116 stars (including 6995 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat
util/solve_plate_with_UCAC5 got 7116 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 6964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 6961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 6961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits N_match=967 sigma_overall_arcsec=0.299 sigma_q1_arcsec=0.291 sigma_q2_arcsec=0.295 sigma_q3_arcsec=0.297 sigma_q4_arcsec=0.415 n_q1=384 n_q2=180 n_q3=349 n_q4=54 worst_quadrant_to_overall_ratio=1.390
The image catalog is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits -region wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.94tmrmzyIQ (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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=125, passed=6510
Got 6510 stars (including 6376 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat
util/solve_plate_with_UCAC5 got 6510 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 6251 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 6251 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 6251 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits N_match=967 sigma_overall_arcsec=0.312 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.281 sigma_q3_arcsec=0.331 sigma_q4_arcsec=0.501 n_q1=475 n_q2=108 n_q3=306 n_q4=78 worst_quadrant_to_overall_ratio=1.605
The image catalog is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits -region wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits.cat.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_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-10-27_20.00sec_-0.00C_LIGHTs_0076.fits
Saving fully-calibrated image wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.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_2026-06-07_CI_Crt-01-Q1b1x1_235248_TTUQ1b1x1_2089185_EfqP5980/wcs_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077.fits
Preparing the HTML report for the field Crt-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:30:40.49 -11:13:19.3: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:20:25.18 -10:16:54.6: 12.81 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:29:26.47 -12:03:29.4: 13.43 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:17:21.46 -08:39:39.7: 13.51 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:16:43.67 -09:08:51.7: 14.02 +/- 0.07 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:57.38 -06:58:04.4: 13.55 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:12:52.79 -07:50:50.3: 13.95 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:08:28.69 -06:28:21.2: 13.48 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:57.48 -06:28:44.3: 13.66 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:32:18.56 -12:16:28.5: 13.68 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:30:40.49 -11:13:19.3: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:20:25.18 -10:16:54.6: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter REJECTED candidate at 11:20:25.18 -10:16:54.6: ref_mag=12.81 +/- 0.02 new_mean_mag=12.3313 delta=0.47 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:17:21.46 -08:39:39.7: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter KEPT candidate at 11:17:21.46 -08:39:39.7: ref_mag=13.48 +/- 0.03 new_mean_mag=12.4470 delta=1.04 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:08:28.69 -06:28:21.2: 13.49 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:12:52.79 -07:50:50.3: 14.03 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:29:26.47 -12:03:29.4: 13.40 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:57.48 -06:28:44.3: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry reference-image weighted average: 13.99 +/- 0.04
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:32:18.56 -12:16:28.5: 13.63 +/- 0.06 detection
Forced photometry filter KEPT candidate at 11:08:28.69 -06:28:21.2: ref_mag=13.49 +/- 0.03 new_mean_mag=12.5306 delta=0.96 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:16:43.67 -09:08:51.7: 13.98 +/- 0.06 detection
Forced photometry filter KEPT candidate at 11:12:52.79 -07:50:50.3: ref_mag=13.99 +/- 0.04 new_mean_mag=12.8868 delta=1.10 (need > 0.90)
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:57.38 -06:58:04.4: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter KEPT candidate at 11:05:57.48 -06:28:44.3: ref_mag=13.70 +/- 0.03 new_mean_mag=12.7245 delta=0.97 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:29:26.47 -12:03:29.4: ref_mag=13.41 +/- 0.03 new_mean_mag=12.5238 delta=0.89 (need > 0.90)
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Forced photometry filter KEPT candidate at 11:32:18.56 -12:16:28.5: ref_mag=13.65 +/- 0.04 new_mean_mag=12.6970 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 11:16:43.67 -09:08:51.7: ref_mag=14.00 +/- 0.05 new_mean_mag=12.9219 delta=1.08 (need > 0.90)
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter KEPT candidate at 11:05:57.38 -06:58:04.4: ref_mag=13.55 +/- 0.03 new_mean_mag=12.6222 delta=0.93 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:06:10.04 -06:41:28.3: 13.46 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:34.33 -06:39:18.1: 13.48 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:06:10.04 -06:41:28.3: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry filter KEPT candidate at 11:06:10.04 -06:41:28.3: ref_mag=13.47 +/- 0.03 new_mean_mag=12.4355 delta=1.03 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:34.33 -06:39:18.1: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 11:05:34.33 -06:39:18.1: ref_mag=13.45 +/- 0.03 new_mean_mag=12.5069 delta=0.94 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:09:03.82 -07:13:21.5: 13.32 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:09:03.82 -07:13:21.5: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 11:09:03.82 -07:13:21.5: ref_mag=13.30 +/- 0.02 new_mean_mag=12.3795 delta=0.92 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:07:02.53 -07:02:53.9: 13.45 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:07:02.53 -07:02:53.9: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter KEPT candidate at 11:07:02.53 -07:02:53.9: ref_mag=13.48 +/- 0.03 new_mean_mag=12.5512 delta=0.93 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:19:15.70 -09:28:24.8: 13.30 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:19:15.70 -09:28:24.8: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 11:19:15.70 -09:28:24.8: ref_mag=13.35 +/- 0.03 new_mean_mag=12.4469 delta=0.90 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:09:34.50 -07:21:31.8: 14.13 +/- 0.07 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:09:34.50 -07:21:31.8: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Forced photometry filter KEPT candidate at 11:09:34.50 -07:21:31.8: ref_mag=14.04 +/- 0.05 new_mean_mag=12.9162 delta=1.13 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:11:03.29 -07:37:46.3: 13.81 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:11:03.29 -07:37:46.3: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Forced photometry filter KEPT candidate at 11:11:03.29 -07:37:46.3: ref_mag=13.82 +/- 0.04 new_mean_mag=12.8601 delta=0.96 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:41.10 -06:42:56.8: 13.69 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:08:40.02 -07:33:56.7: 13.42 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:41.10 -06:42:56.8: 13.75 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:08:40.02 -07:33:56.7: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Forced photometry filter KEPT candidate at 11:08:40.02 -07:33:56.7: ref_mag=13.44 +/- 0.03 new_mean_mag=12.4016 delta=1.04 (need > 0.90)
Forced photometry filter KEPT candidate at 11:05:41.10 -06:42:56.8: ref_mag=13.72 +/- 0.03 new_mean_mag=12.7317 delta=0.99 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:04:35.81 -06:39:09.7: 13.69 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:04:35.81 -06:39:09.7: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 11:04:35.81 -06:39:09.7: ref_mag=13.68 +/- 0.03 new_mean_mag=12.6204 delta=1.06 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:06:59.85 -07:11:23.0: 13.40 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:07:05.87 -06:56:38.7: 13.26 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:06:59.85 -07:11:23.0: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 11:06:59.85 -07:11:23.0: ref_mag=13.37 +/- 0.02 new_mean_mag=12.4546 delta=0.92 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:07:05.87 -06:56:38.7: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 11:07:05.87 -06:56:38.7: ref_mag=13.30 +/- 0.02 new_mean_mag=12.2765 delta=1.02 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:03:45.34 -06:10:48.4: 13.80 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:03:45.34 -06:10:48.4: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry filter KEPT candidate at 11:03:45.34 -06:10:48.4: ref_mag=13.76 +/- 0.03 new_mean_mag=12.6585 delta=1.10 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:07:31.27 -07:12:27.9: 14.06 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:07:31.27 -07:12:27.9: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.04
Forced photometry filter KEPT candidate at 11:07:31.27 -07:12:27.9: ref_mag=14.03 +/- 0.04 new_mean_mag=12.8971 delta=1.13 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:06:50.95 -06:39:42.1: 13.93 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:06:50.95 -06:39:42.1: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.04
Forced photometry filter KEPT candidate at 11:06:50.95 -06:39:42.1: ref_mag=13.91 +/- 0.04 new_mean_mag=12.8431 delta=1.07 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:30:39.74 -12:08:10.1: 13.69 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:45.87 -06:17:18.6: 13.25 +/- 0.03 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:30:39.74 -12:08:10.1: 13.65 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:45.87 -06:17:18.6: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 11:30:39.74 -12:08:10.1: ref_mag=13.66 +/- 0.04 new_mean_mag=12.6972 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 11:05:45.87 -06:17:18.6: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2890 delta=0.93 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:03:54.32 -06:28:49.3: 13.68 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:03:54.32 -06:28:49.3: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 11:03:54.32 -06:28:49.3: ref_mag=13.68 +/- 0.03 new_mean_mag=12.7285 delta=0.95 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:08:56.63 -07:04:02.3: 13.65 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:28:55.32 -12:01:31.6: 13.64 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:08:56.63 -07:04:02.3: 13.73 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:28:55.32 -12:01:31.6: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Forced photometry filter KEPT candidate at 11:08:56.63 -07:04:02.3: ref_mag=13.69 +/- 0.03 new_mean_mag=12.7597 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter KEPT candidate at 11:28:55.32 -12:01:31.6: ref_mag=13.69 +/- 0.04 new_mean_mag=12.6486 delta=1.04 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:06:55.07 -06:42:28.1: 13.65 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:20.07 -06:43:50.8: 13.90 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:06:55.07 -06:42:28.1: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 11:06:55.07 -06:42:28.1: ref_mag=13.62 +/- 0.03 new_mean_mag=12.6361 delta=0.99 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:20.07 -06:43:50.8: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Forced photometry filter KEPT candidate at 11:05:20.07 -06:43:50.8: ref_mag=13.96 +/- 0.04 new_mean_mag=12.8556 delta=1.10 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:09:07.36 -07:19:42.3: 13.91 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:09:07.36 -07:19:42.3: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.04
Forced photometry filter KEPT candidate at 11:09:07.36 -07:19:42.3: ref_mag=13.89 +/- 0.04 new_mean_mag=12.7469 delta=1.14 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:21:06.26 -09:17:08.8: 13.74 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:21:06.26 -09:17:08.8: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Forced photometry filter KEPT candidate at 11:21:06.26 -09:17:08.8: ref_mag=13.69 +/- 0.03 new_mean_mag=12.7043 delta=0.99 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:17.96 -06:21:41.9: 13.63 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:17.96 -06:21:41.9: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 11:05:17.96 -06:21:41.9: ref_mag=13.65 +/- 0.03 new_mean_mag=12.6728 delta=0.98 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:08:29.48 -07:17:50.9: 13.62 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:30:57.65 -11:54:20.3: 13.72 +/- 0.06 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:08:29.48 -07:17:50.9: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 11:08:29.48 -07:17:50.9: ref_mag=13.65 +/- 0.03 new_mean_mag=12.5789 delta=1.07 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:30:57.65 -11:54:20.3: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter KEPT candidate at 11:30:57.65 -11:54:20.3: ref_mag=13.69 +/- 0.04 new_mean_mag=12.6835 delta=1.01 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:07:25.83 -07:14:45.3: 13.74 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:09:54.14 -07:23:27.7: 13.74 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:16:11.08 -09:14:19.7: 13.71 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:07:25.83 -07:14:45.3: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 11:07:25.83 -07:14:45.3: ref_mag=13.68 +/- 0.03 new_mean_mag=12.6685 delta=1.01 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:16:11.08 -09:14:19.7: 13.65 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:09:54.14 -07:23:27.7: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 11:16:11.08 -09:14:19.7: ref_mag=13.68 +/- 0.03 new_mean_mag=12.7131 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry filter KEPT candidate at 11:09:54.14 -07:23:27.7: ref_mag=13.70 +/- 0.03 new_mean_mag=12.6923 delta=1.01 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:07:35.34 -06:34:17.0: 13.71 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:10:50.71 -07:39:41.0: 13.59 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:10:50.71 -07:39:41.0: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:07:35.34 -06:34:17.0: 13.76 +/- 0.05 detection
Forced photometry filter KEPT candidate at 11:10:50.71 -07:39:41.0: ref_mag=13.64 +/- 0.03 new_mean_mag=12.6838 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter KEPT candidate at 11:07:35.34 -06:34:17.0: ref_mag=13.73 +/- 0.03 new_mean_mag=12.6974 delta=1.03 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:19:29.88 -09:25:55.1: 13.59 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:19:29.88 -09:25:55.1: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter KEPT candidate at 11:19:29.88 -09:25:55.1: ref_mag=13.56 +/- 0.03 new_mean_mag=12.6157 delta=0.94 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:33:45.85 -12:15:18.9: 13.36 +/- 0.05 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:33:45.85 -12:15:18.9: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter KEPT candidate at 11:33:45.85 -12:15:18.9: ref_mag=13.39 +/- 0.03 new_mean_mag=12.4768 delta=0.91 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:05:23.93 -06:28:05.2: 14.03 +/- 0.07 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:05:23.93 -06:28:05.2: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Forced photometry filter KEPT candidate at 11:05:23.93 -06:28:05.2: ref_mag=13.98 +/- 0.05 new_mean_mag=12.8531 delta=1.12 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:06:15.34 -06:28:19.3: 13.37 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:06:15.34 -06:28:19.3: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter KEPT candidate at 11:06:15.34 -06:28:19.3: ref_mag=13.39 +/- 0.03 new_mean_mag=12.4388 delta=0.95 (need > 0.90)
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-07-59_20.00sec_-4.90C_LIGHTs_0142.fits at 11:04:24.86 -06:17:57.3: 13.55 +/- 0.04 detection
Forced photometry on wcs_Crt-01-Q1b1x1_2026-04-16_00-08-54_20.00sec_-5.00C_LIGHTs_0143.fits at 11:04:24.86 -06:17:57.3: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 11:04:24.86 -06:17:57.3: ref_mag=13.57 +/- 0.03 new_mean_mag=12.6218 delta=0.95 (need > 0.90)
Adding exclusion_list_local.txt__out05199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52983.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 78s
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 52983_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 52983_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
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Considering the candidate 53022_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
The candidate 53022_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077 did not pass the final checks
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Considering the candidate 07833_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 07833_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
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Considering the candidate 15292_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 15292_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
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Considering the candidate 37908_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 37908_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
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Considering the candidate 06152_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 06152_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
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Considering the candidate 10653_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 10653_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
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Considering the candidate 13383_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 13383_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
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Considering the candidate 05964_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 05964_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
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Considering the candidate 38560_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
The candidate 38560_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077 did not pass the final checks
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Considering the candidate 06835_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 06835_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
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Considering the candidate 06759_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 06759_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
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Considering the candidate 08576_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 08576_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
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Considering the candidate 08034_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 08034_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16399_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 16399_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09075_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 09075_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09953_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 09953_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09849_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 09849_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06989_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 06989_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06799_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 06799_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08574_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 08574_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07666_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 07666_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05199_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 05199_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08622_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 08622_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06720_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 06720_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38397_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 38397_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05459_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 05459_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06274_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 06274_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08013_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 08013_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34862_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 34862_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06881_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 06881_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07038_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 07038_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08972_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 08972_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15562_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 15562_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05759_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 05759_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08895_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 08895_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39107_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 39107_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08764_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 08764_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09171_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 09171_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15685_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 15685_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06355_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 06355_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10045_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 10045_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16259_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 16259_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38090_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 38090_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06145_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 06145_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06108_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 06108_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05601_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
Preparing report for the candidate 05601_fd_Crt-01-Q1b1x1_2026-06-07_23-11-13_20.00sec_-0.00C_LIGHTs_0077
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 105s
Prepared the HTML report for the field Crt-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:03:45.34 -06:10:48.4
11:05:45.87 -06:17:18.6
11:04:24.86 -06:17:57.3
11:05:17.96 -06:21:41.9
11:08:28.69 -06:28:21.2
11:06:15.34 -06:28:19.3
11:05:23.93 -06:28:05.2
11:05:57.48 -06:28:44.3
11:03:54.32 -06:28:49.3
11:07:35.34 -06:34:17.0
11:06:50.95 -06:39:42.1
11:05:34.33 -06:39:18.1
11:04:35.81 -06:39:09.7
11:06:10.04 -06:41:28.3
11:06:55.07 -06:42:28.1
11:05:41.10 -06:42:56.8
11:05:20.07 -06:43:50.8
11:07:05.87 -06:56:38.7
11:05:57.38 -06:58:04.4
11:08:56.63 -07:04:02.3
11:07:02.53 -07:02:53.9
11:06:59.85 -07:11:23.0
11:09:03.82 -07:13:21.5
11:07:31.27 -07:12:27.9
11:07:25.83 -07:14:45.3
11:08:29.48 -07:17:50.9
11:09:07.36 -07:19:42.3
11:09:34.50 -07:21:31.8
11:09:54.14 -07:23:27.7
11:08:40.02 -07:33:56.7
11:11:03.29 -07:37:46.3
11:10:50.71 -07:39:41.0
11:12:52.79 -07:50:50.3
11:17:21.46 -08:39:39.7
11:16:43.67 -09:08:51.7
11:21:06.26 -09:17:08.8
11:16:11.08 -09:14:19.7
11:19:29.88 -09:25:55.1
11:19:15.70 -09:28:24.8
11:28:55.32 -12:01:31.6
11:32:18.56 -12:16:28.5
11:33:45.85 -12:15:18.9
11:30:39.74 -12:08:10.1
11:30:57.65 -11:54:20.3
11:30:40.49 -11:13:19.3
########### Completed Crt-01-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
11:30:40.49 -11:13:19.3
11:05:57.38 -06:58:04.4
11:16:43.67 -09:08:51.7
11:32:18.56 -12:16:28.5
11:05:57.48 -06:28:44.3
11:12:52.79 -07:50:50.3
11:17:21.46 -08:39:39.7
11:08:28.69 -06:28:21.2
11:06:10.04 -06:41:28.3
11:05:34.33 -06:39:18.1
11:09:03.82 -07:13:21.5
11:07:02.53 -07:02:53.9
11:19:15.70 -09:28:24.8
11:09:34.50 -07:21:31.8
11:11:03.29 -07:37:46.3
11:08:40.02 -07:33:56.7
11:05:41.10 -06:42:56.8
11:04:35.81 -06:39:09.7
11:06:59.85 -07:11:23.0
11:07:05.87 -06:56:38.7
11:03:45.34 -06:10:48.4
11:07:31.27 -07:12:27.9
11:06:50.95 -06:39:42.1
11:30:39.74 -12:08:10.1
11:05:45.87 -06:17:18.6
11:03:54.32 -06:28:49.3
11:08:56.63 -07:04:02.3
11:28:55.32 -12:01:31.6
11:06:55.07 -06:42:28.1
11:05:20.07 -06:43:50.8
11:09:07.36 -07:19:42.3
11:21:06.26 -09:17:08.8
11:05:17.96 -06:21:41.9
11:08:29.48 -07:17:50.9
11:30:57.65 -11:54:20.3
11:07:25.83 -07:14:45.3
11:09:54.14 -07:23:27.7
11:16:11.08 -09:14:19.7
11:07:35.34 -06:34:17.0
11:10:50.71 -07:39:41.0
11:19:29.88 -09:25:55.1
11:33:45.85 -12:15:18.9
11:05:23.93 -06:28:05.2
11:06:15.34 -06:28:19.3
11:04:24.86 -06:17:57.3
###################################################################################
11:30:40.49 -11:13:19.3 -- asteroid (will NOT add it to exclusion list)
11:05:57.38 -06:58:04.4 -- not an asteroid (will add it to exclusion list)
11:16:43.67 -09:08:51.7 -- not an asteroid (will add it to exclusion list)
11:32:18.56 -12:16:28.5 -- not an asteroid (will add it to exclusion list)
11:05:57.48 -06:28:44.3 -- not an asteroid (will add it to exclusion list)
11:12:52.79 -07:50:50.3 -- not an asteroid (will add it to exclusion list)
11:17:21.46 -08:39:39.7 -- not an asteroid (will add it to exclusion list)
11:08:28.69 -06:28:21.2 -- not an asteroid (will add it to exclusion list)
11:06:10.04 -06:41:28.3 -- not an asteroid (will add it to exclusion list)
11:05:34.33 -06:39:18.1 -- not an asteroid (will add it to exclusion list)
11:09:03.82 -07:13:21.5 -- not an asteroid (will add it to exclusion list)
11:07:02.53 -07:02:53.9 -- not an asteroid (will add it to exclusion list)
11:19:15.70 -09:28:24.8 -- not an asteroid (will add it to exclusion list)
11:09:34.50 -07:21:31.8 -- not an asteroid (will add it to exclusion list)
11:11:03.29 -07:37:46.3 -- not an asteroid (will add it to exclusion list)
11:08:40.02 -07:33:56.7 -- not an asteroid (will add it to exclusion list)
11:05:41.10 -06:42:56.8 -- not an asteroid (will add it to exclusion list)
11:04:35.81 -06:39:09.7 -- not an asteroid (will add it to exclusion list)
11:06:59.85 -07:11:23.0 -- not an asteroid (will add it to exclusion list)
11:07:05.87 -06:56:38.7 -- not an asteroid (will add it to exclusion list)
11:03:45.34 -06:10:48.4 -- not an asteroid (will add it to exclusion list)
11:07:31.27 -07:12:27.9 -- not an asteroid (will add it to exclusion list)
11:06:50.95 -06:39:42.1 -- not an asteroid (will add it to exclusion list)
11:30:39.74 -12:08:10.1 -- not an asteroid (will add it to exclusion list)
11:05:45.87 -06:17:18.6 -- not an asteroid (will add it to exclusion list)
11:03:54.32 -06:28:49.3 -- not an asteroid (will add it to exclusion list)
11:08:56.63 -07:04:02.3 -- not an asteroid (will add it to exclusion list)
11:28:55.32 -12:01:31.6 -- not an asteroid (will add it to exclusion list)
11:06:55.07 -06:42:28.1 -- not an asteroid (will add it to exclusion list)
11:05:20.07 -06:43:50.8 -- not an asteroid (will add it to exclusion list)
11:09:07.36 -07:19:42.3 -- not an asteroid (will add it to exclusion list)
11:21:06.26 -09:17:08.8 -- not an asteroid (will add it to exclusion list)
11:05:17.96 -06:21:41.9 -- not an asteroid (will add it to exclusion list)
11:08:29.48 -07:17:50.9 -- not an asteroid (will add it to exclusion list)
11:30:57.65 -11:54:20.3 -- not an asteroid (will add it to exclusion list)
11:07:25.83 -07:14:45.3 -- not an asteroid (will add it to exclusion list)
11:09:54.14 -07:23:27.7 -- not an asteroid (will add it to exclusion list)
11:16:11.08 -09:14:19.7 -- not an asteroid (will add it to exclusion list)
11:07:35.34 -06:34:17.0 -- not an asteroid (will add it to exclusion list)
11:10:50.71 -07:39:41.0 -- not an asteroid (will add it to exclusion list)
11:19:29.88 -09:25:55.1 -- not an asteroid (will add it to exclusion list)
11:33:45.85 -12:15:18.9 -- not an asteroid (will add it to exclusion list)
11:05:23.93 -06:28:05.2 -- not an asteroid (will add it to exclusion list)
11:06:15.34 -06:28:19.3 -- not an asteroid (will add it to exclusion list)
11:04:24.86 -06:17:57.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
11:03:45.34 -06:10:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:03:54.32 -06:28:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:04:24.86 -06:17:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:04:35.81 -06:39:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:05:17.96 -06:21:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:05:20.07 -06:43:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:05:23.93 -06:28:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:05:34.33 -06:39:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:05:41.10 -06:42:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:05:45.87 -06:17:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:05:57.38 -06:58:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:05:57.48 -06:28:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:06:10.04 -06:41:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:06:15.34 -06:28:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:06:50.95 -06:39:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:06:55.07 -06:42:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:06:59.85 -07:11:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:07:02.53 -07:02:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:07:05.87 -06:56:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:07:25.83 -07:14:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:07:31.27 -07:12:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:07:35.34 -06:34:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:08:28.69 -06:28:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:08:29.48 -07:17:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:08:40.02 -07:33:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:08:56.63 -07:04:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:09:03.82 -07:13:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:09:07.36 -07:19:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:09:34.50 -07:21:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:09:54.14 -07:23:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:10:50.71 -07:39:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:11:03.29 -07:37:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:12:52.79 -07:50:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:16:11.08 -09:14:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:16:43.67 -09:08:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:21.46 -08:39:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:19:15.70 -09:28:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:19:29.88 -09:25:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:21:06.26 -09:17:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:28:55.32 -12:01:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:30:39.74 -12:08:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:30:57.65 -11:54:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:32:18.56 -12:16:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:33:45.85 -12:15:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
11:03:45.34 -06:10:48.4 -- not a known variable star
11:03:54.32 -06:28:49.3 -- not a known variable star
11:04:24.86 -06:17:57.3 -- not a known variable star
11:04:35.81 -06:39:09.7 -- not a known variable star
11:05:17.96 -06:21:41.9 -- not a known variable star
11:05:20.07 -06:43:50.8 -- not a known variable star
11:05:23.93 -06:28:05.2 -- not a known variable star
11:05:34.33 -06:39:18.1 -- not a known variable star
11:05:41.10 -06:42:56.8 -- not a known variable star
11:05:45.87 -06:17:18.6 -- not a known variable star
11:05:57.38 -06:58:04.4 -- not a known variable star
11:05:57.48 -06:28:44.3 -- not a known variable star
11:06:10.04 -06:41:28.3 -- not a known variable star
11:06:15.34 -06:28:19.3 -- not a known variable star
11:06:50.95 -06:39:42.1 -- not a known variable star
11:06:55.07 -06:42:28.1 -- not a known variable star
11:06:59.85 -07:11:23.0 -- not a known variable star
11:07:02.53 -07:02:53.9 -- not a known variable star
11:07:05.87 -06:56:38.7 -- not a known variable star
11:07:25.83 -07:14:45.3 -- not a known variable star
11:07:31.27 -07:12:27.9 -- not a known variable star
11:07:35.34 -06:34:17.0 -- not a known variable star
11:08:28.69 -06:28:21.2 -- not a known variable star
11:08:29.48 -07:17:50.9 -- not a known variable star
11:08:40.02 -07:33:56.7 -- not a known variable star
11:08:56.63 -07:04:02.3 -- not a known variable star
11:09:03.82 -07:13:21.5 -- not a known variable star
11:09:07.36 -07:19:42.3 -- not a known variable star
11:09:34.50 -07:21:31.8 -- not a known variable star
11:09:54.14 -07:23:27.7 -- not a known variable star
11:10:50.71 -07:39:41.0 -- not a known variable star
11:11:03.29 -07:37:46.3 -- not a known variable star
11:12:52.79 -07:50:50.3 -- not a known variable star
11:16:11.08 -09:14:19.7 -- not a known variable star
11:16:43.67 -09:08:51.7 -- not a known variable star
11:17:21.46 -08:39:39.7 -- a known variable star
11:19:15.70 -09:28:24.8 -- not a known variable star
11:19:29.88 -09:25:55.1 -- not a known variable star
11:21:06.26 -09:17:08.8 -- not a known variable star
11:28:55.32 -12:01:31.6 -- not a known variable star
11:30:39.74 -12:08:10.1 -- not a known variable star
11:30:57.65 -11:54:20.3 -- not a known variable star
11:32:18.56 -12:16:28.5 -- not a known variable star
11:33:45.85 -12:15:18.9 -- not a known variable star
Found 43 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
44 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 44 (excluding asteroids and hot pixels, 43 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)2461199.67404529 -observatory V36
06:43:37.70 +25:00:16.7 Mercury (0.1mag)
07:42:45.80 +23:22:58.8 Venus (-4.0mag)
02:49:33.43 +15:42:36.1 Mars (1.3mag)
07:48:25.35 +21:31:29.4 Jupiter (-1.9mag)
00:49:22.14 +02:48:39.2 Saturn (0.9mag)
04:00:12.15 +20:25:27.1 Uranus (5.8mag)
00:16:08.47 +00:16:48.0 Neptune (7.8mag)
20:33:21.46 -23:04:32.4 Pluto (14.5mag)
23:02:21.62 -05:45:32.9 Moon (-10.4mag)
-rw-r--r-- 1 apache apache 362 Jun 8 00:59 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461199.67404529:
07:48:26.00 +21:31:29.7 Io (6.0mag)
07:48:25.36 +21:31:31.6 Europa (6.2mag)
07:48:09.45 +21:32:16.7 Ganymede (5.6mag)
07:48:44.10 +21:30:28.9 Callisto (6.7mag)
07:48:42.77 +21:07:47.0 Himalia (15.6mag)
07:48:29.96 +21:31:15.2 Thebe (16.5mag)
07:48:42.24 +21:23:14.0 Elara (17.5mag)
07:50:35.99 +21:43:11.8 Pasiphae (17.7mag)
07:55:00.49 +21:33:11.8 Carme (18.9mag)
00:49:12.68 +02:48:38.1 Titan (8.7mag)
00:49:19.12 +02:48:52.4 Rhea (9.9mag)
00:49:54.43 +02:50:48.5 Iapetus (11.3mag)
00:49:18.06 +02:48:16.2 Hyperion (14.7mag)
00:50:04.43 +02:50:35.9 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 8 00:59 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461199.67404529:
17:26:43.51 -35:14:53.9 JWST
14:31:17.34 +57:28:23.7 Chandra
18:36:27.74 -23:30:21.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 8 00:59 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461199.67404529 -observatory V36
18:43:31.51 -32:39:09.1 13.6mag P/2010 H2 (Vales)
05:53:27.04 -68:03:51.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:49:03.10 +31:58:04.0 17.5mag C/2017 K2 (PANSTARRS)
17:14:44.44 +15:21:03.3 17.8mag C/2021 G2 (ATLAS)
21:12:05.67 -49:29:54.8 16.9mag P/2021 N1 (ZTF)
23:12:38.30 +31:35:28.6 17.2mag C/2022 E2 (ATLAS)
05:34:01.02 +26:58:31.4 16.5mag C/2022 N2 (PANSTARRS)
09:29:42.78 +31:05:00.2 16.6mag C/2022 QE78 (ATLAS)
08:50:32.10 +03:55:51.5 17.7mag C/2022 R6 (PANSTARRS)
18:28:14.15 +21:36:07.1 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:19:22.84 -11:00:31.0 17.6mag P/2023 B1 (PANSTARRS)
22:14:26.35 +66:31:38.5 17.7mag C/2023 H5 (Lemmon)
17:46:26.30 -06:41:14.1 13.7mag C/2023 R1 (PANSTARRS)
13:18:06.43 +82:59:53.0 17.9mag C/2023 X2 (Lemmon)
07:10:23.15 +64:18:30.3 17.7mag C/2024 A1 (ATLAS)
06:47:14.39 +27:49:57.0 13.6mag C/2024 E1 (Wierzchos)
15:37:18.31 +13:31:28.7 17.4mag C/2024 G6 (ATLAS)
20:13:03.59 +31:07:45.4 14.0mag C/2024 J3 (ATLAS)
04:18:00.32 -15:57:10.2 16.0mag C/2024 T5 (ATLAS)
06:05:53.52 +34:29:42.4 17.9mag C/2025 J1 (Borisov)
11:34:54.92 +52:45:01.2 17.4mag C/2025 L1 (ATLAS)
06:44:55.05 -10:52:07.9 14.1mag C/2025 R3 (PANSTARRS)
09:24:08.69 +23:20:25.1 17.9mag C/2025 V2 (Rankin)
12:39:42.11 +04:41:28.1 17.2mag C/2025 Y1 (ATLAS)
18:12:55.20 +75:07:40.6 17.9mag C/2026 A2 (Bok)
02:00:37.76 +43:24:49.8 16.1mag C/2026 B2 (Sun-Gao)
11:11:18.49 -03:44:26.0 16.5mag A/2026 E1
20:23:36.80 -08:34:05.0 8.7mag 10P/Tempel
11:02:00.02 -00:58:03.7 16.0mag 29P/Schwassmann-Wachmann
03:11:41.32 +25:38:34.7 17.7mag 47P/Ashbrook-Jackson
08:59:56.16 +23:46:30.2 16.9mag 63P/Wild
00:26:54.56 -06:22:07.7 15.7mag 65P/Gunn
06:43:22.38 +33:25:40.8 16.9mag 76P/West-Kohoutek-Ikemura
03:09:07.86 +17:12:50.6 13.8mag 78P/Gehrels
01:20:42.84 +04:50:41.5 15.6mag 88P/Howell
04:54:34.43 +30:18:05.5 15.2mag 93P/Lovas
02:42:53.52 +27:37:22.0 17.6mag 114P/Wiseman-Skiff
06:50:29.89 +33:02:20.4 15.6mag 123P/West-Hartley
09:50:08.58 +14:38:46.8 16.5mag 124P/Mrkos
03:59:00.07 +19:14:56.8 16.4mag 128P/Shoemaker-Holt
04:33:31.33 +19:05:00.9 17.7mag 131P/Mueller
05:58:13.35 +18:40:04.0 14.6mag 141P/Machholz
06:00:51.53 +17:40:27.3 14.6mag 141P-A/Machholz
04:53:59.17 +16:10:15.2 11.6mag 141P-D/Machholz
02:57:39.80 -24:42:08.8 16.8mag 161P/Hartley-IRAS
03:41:28.73 +23:48:04.9 14.9mag 162P/SidingSpring
19:36:38.24 +01:43:23.6 16.9mag 169P/NEAT
00:18:16.82 +02:27:40.8 17.9mag 220P/McNaught
16:52:11.96 -08:28:36.5 16.4mag 235P/LINEAR
07:34:36.61 +35:29:34.1 17.5mag 240P/NEAT
00:32:17.77 -02:28:40.2 16.4mag 260P/McNaught
04:04:10.08 +32:28:38.2 17.6mag 295P/LINEAR
23:52:07.24 -09:44:12.1 17.6mag 320P/McNaught
15:15:14.86 +08:06:01.9 17.4mag 391P/Kowalski
08:07:07.22 +20:44:52.6 17.9mag 450P/LONEOS
06:59:56.33 +41:41:52.8 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 8 00:59 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
-rw-r--r-- 1 apache apache 5.6K Jun 8 00:59 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
-rw-r--r-- 1 apache apache 189K Jun 8 00:59 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:39:35.110 +15:17:58.28 AT 2026nsc 2026-05-09.80 20.76
16:42:48.680 +20:27:18.30 AT 2026nsb 2026-05-09.80 20.54
13:34:03.440 +31:37:31.73 AT 2026nsa 2026-05-07.80 21.26
13:50:28.150 +02:34:54.72 AT 2026nrz 2026-05-22.72 21.54
13:43:59.750 +03:47:21.63 AT 2026nry 2026-05-22.69 22.05
13:17:26.150 -01:26:00.12 AT 2026nrx 2026-05-21.64 21.7
00:35:20.216 -08:28:38.64 AT 2026nrw 2026-05-19.42 18.74
23:50:43.016 -01:09:12.25 AT 2026nrv 2026-05-23.48 19.5028
22:36:47.715 +37:31:34.81 AT 2026nru 2026-05-22.43 19.4626
23:58:04.247 +20:56:44.66 AT 2026nrt 2026-05-23.48 20.1237
16:08:58.229 +36:53:23.76 AT 2026nrs 2026-05-21.36 20.3819
19:44:04.734 +84:44:44.91 SN 2026nrr 2026-05-25.47 17.808
21:42:24.388 -20:21:08.51 SN 2026nrq 2026-05-25.56 18.623
22:03:20.669 -84:55:27.45 AT 2026nrp 2026-05-22.30 19.244
23:07:53.376 -39:04:26.84 AT 2026nro 2026-05-22.38 19.567
00:40:07.848 -39:10:21.32 AT 2026nrn 2026-05-12.41 18.737
23:05:28.381 -21:25:50.28 AT 2026nrm 2026-05-25.58 18.887
19:27:28.750 -48:42:52.35 AT 2026nrl 2026-05-22.24 19.107
12:33:38.422 +12:02:05.88 AT 2026nrk 2026-05-25.29 21.322
12:32:27.199 +02:39:54.51 AT 2026nrj 2026-05-25.29 21.0728
-rw-r--r-- 1 apache apache 30K Jun 8 00:59 tns_transients_list.txt
