This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 9.76 10:21:47.29 +74:22:09.5
135.09498 39.01955 galactic Dra Second-epoch detections are separated by 0.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1126488665255548032 | 10:21:47.37 +74:22:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.637+/-0.038 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:21:47.29 +74:22:09.5: 10.67 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:21:47.29 +74:22:09.5: 10.68 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.67 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1126488665255548032,2461258.8011,9.76,0.05,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 1126488665255548032 20260806.3011 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.15 10:21:54.04 +74:33:31.6
134.91866 38.88857 galactic Dra Second-epoch detections are separated by 0.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1126546767573135616 | 10:21:53.87 +74:33:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.779+/-0.035 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:21:54.04 +74:33:31.6: 11.09 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:21:54.04 +74:33:31.6: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1126546767573135616,2461258.8011,10.15,0.05,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 1126546767573135616 20260806.3011 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.46 10:35:05.58 +73:46:59.7
134.73320 40.06737 galactic Dra Second-epoch detections are separated by 0.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078376132368260992 | 10:35:05.50 +73:46:59.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.374+/-0.035 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:35:05.58 +73:46:59.7: 11.49 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:35:05.58 +73:46:59.7: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078376132368260992,2461258.8011,10.46,0.05,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 1078376132368260992 20260806.3011 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.71 10:37:08.89 +74:02:50.9
134.36829 39.95798 galactic Dra Second-epoch detections are separated by 1.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078395129008142976 | 10:37:08.79 +74:02:51.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.017+/-0.035 (A)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:37:08.89 +74:02:50.9: 11.72 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:37:08.89 +74:02:50.9: 11.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078395129008142976,2461258.8011,10.71,0.05,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 1078395129008142976 20260806.3011 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.90 10:24:07.46 +74:52:54.6
134.49664 38.75545 galactic Dra Second-epoch detections are separated by 1.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1126587445207580160 | 10:24:07.48 +74:52:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.595+/-0.026 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:24:07.46 +74:52:54.6: 11.77 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:24:07.46 +74:52:54.6: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1126587445207580160,2461258.8011,10.90,0.05,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 1126587445207580160 20260806.3011 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.88 11:02:39.58 +73:16:14.5
133.07162 41.64776 galactic Dra Second-epoch detections are separated by 0.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078710693140652032 | 11:02:39.65 +73:16:14.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.600+/-0.030 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:02:39.58 +73:16:14.5: 11.76 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:02:39.58 +73:16:14.5: 11.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078710693140652032,2461258.8011,10.88,0.05,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
Gaia DR3 1078710693140652032 20260806.3011 10.88CV 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 08 06.3011 2461258.8011 10.86 10:26:41.33 +74:18:27.1
134.84003 39.29179 galactic Dra Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1126478872730139008 | 10:26:41.34 +74:18:27.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.661+/-0.033 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:26:41.33 +74:18:27.1: 12.01 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:26:41.33 +74:18:27.1: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1126478872730139008,2461258.8011,10.86,0.05,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
Gaia DR3 1126478872730139008 20260806.3011 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.02 10:52:24.12 +73:24:09.5
133.78041 41.12312 galactic Dra Second-epoch detections are separated by 1.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1077461269974336384 | 10:52:24.18 +73:24:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.370+/-0.030 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:52:24.12 +73:24:09.5: 12.02 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:52:24.12 +73:24:09.5: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1077461269974336384,2461258.8011,11.02,0.05,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 1077461269974336384 20260806.3011 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.09 10:31:45.82 +74:42:03.6
134.17479 39.22567 galactic Dra Second-epoch detections are separated by 1.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1126514881735843968 | 10:31:45.90 +74:42:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.656+/-0.026 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:31:45.82 +74:42:03.6: 12.03 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:31:45.82 +74:42:03.6: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1126514881735843968,2461258.8011,11.09,0.05,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 1126514881735843968 20260806.3011 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.05 10:40:45.77 +74:17:07.3
133.92286 39.93047 galactic Dra Second-epoch detections are separated by 1.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078498178158840832 | 10:40:45.64 +74:17:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.755+/-0.027 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:40:45.77 +74:17:07.3: 12.03 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:40:45.77 +74:17:07.3: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078498178158840832,2461258.8011,11.05,0.05,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 1078498178158840832 20260806.3011 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.85 10:32:06.90 +74:06:06.9
134.66321 39.69178 galactic Dra Second-epoch detections are separated by 0.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078440415142612992 | 10:32:07.08 +74:06:05.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:32:06.90 +74:06:06.9: 12.09 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:32:06.90 +74:06:06.9: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078440415142612992,2461258.8011,10.85,0.05,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
Gaia DR3 1078440415142612992 20260806.3011 10.85CV 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 08 06.3011 2461258.8011 11.24 10:26:35.09 +74:51:53.7
134.36030 38.87697 galactic Dra Second-epoch detections are separated by 1.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1126576209573134464 | 10:26:35.00 +74:51:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.664+/-0.035 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:26:35.09 +74:51:53.7: 12.12 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:26:35.09 +74:51:53.7: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1126576209573134464,2461258.8011,11.24,0.05,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 1126576209573134464 20260806.3011 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.34 11:10:48.83 +72:52:18.9
132.67677 42.29977 galactic Dra Second-epoch detections are separated by 0.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1075649373595591936 | 11:10:48.77 +72:52:18.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.427+/-0.029 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:10:48.83 +72:52:18.9: 12.24 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:10:48.83 +72:52:18.9: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1075649373595591936,2461258.8011,11.34,0.05,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
Gaia DR3 1075649373595591936 20260806.3011 11.34CV 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 08 06.3011 2461258.8011 11.28 10:30:24.83 +74:22:38.1
134.53874 39.40904 galactic Dra Second-epoch detections are separated by 0.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078462375311559552 | 10:30:24.88 +74:22:38.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.311+/-0.037 (F)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:30:24.83 +74:22:38.1: 12.35 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:30:24.83 +74:22:38.1: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078462375311559552,2461258.8011,11.28,0.05,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
Gaia DR3 1078462375311559552 20260806.3011 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.52 10:49:14.86 +74:05:02.4
133.48447 40.44286 galactic Dra Second-epoch detections are separated by 2.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078298719877643264 | 10:49:14.78 +74:05:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.529+/-0.029 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:49:14.86 +74:05:02.4: 12.48 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:49:14.86 +74:05:02.4: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078298719877643264,2461258.8011,11.52,0.05,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 1078298719877643264 20260806.3011 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.50 10:36:59.47 +74:26:19.5
134.05248 39.65081 galactic Dra Second-epoch detections are separated by 2.1" and 5.4 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 | 10:36:59.47 +74:26:19.5 (user input) | T | P | (position from user input) J-Ks=0.287+/-0.035 (F)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:36:59.47 +74:26:19.5: 12.49 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:36:59.47 +74:26:19.5: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8011,11.50,0.05,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 20260806.3011 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.22 10:29:16.91 +74:07:10.3
134.83583 39.54954 galactic Dra Second-epoch detections are separated by 1.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078454266413342720 | 10:29:17.07 +74:07:09.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.379+/-0.034 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:29:16.91 +74:07:10.3: 12.52 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:29:16.91 +74:07:10.3: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078454266413342720,2461258.8011,11.22,0.05,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 1078454266413342720 20260806.3011 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.33 10:35:12.34 +73:53:32.6
134.63262 39.98964 galactic Dra Second-epoch detections are separated by 0.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078380736573204736 | 10:35:12.07 +73:53:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.386+/-0.035 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:35:12.34 +73:53:32.6: 12.52 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:35:12.34 +73:53:32.6: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078380736573204736,2461258.8011,11.33,0.05,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 1078380736573204736 20260806.3011 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.46 10:36:15.94 +74:14:39.2
134.26360 39.76854 galactic Dra Second-epoch detections are separated by 3.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:36:15.94 +74:14:39.2 (user input) | T | P | (position from user input) J-Ks=0.423+/-0.033 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:36:15.94 +74:14:39.2: 12.75 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:36:15.94 +74:14:39.2: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461258.8011,11.46,0.05,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 20260806.3011 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.74 10:32:53.60 +74:16:18.7
134.46604 39.59881 galactic Dra Second-epoch detections are separated by 2.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:32:53.60 +74:16:18.7 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.033 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:32:53.60 +74:16:18.7: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:32:53.60 +74:16:18.7: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461258.8011,11.74,0.05,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 20260806.3011 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 12.31 13:09:20.48 +81:49:28.4
122.15303 35.27660 galactic Cam Second-epoch detections are separated by 1.5" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:09:20.48 +81:49:28.4 (user input) | T | P | (position from user input) J-Ks=0.622+/-0.033 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 13:09:20.48 +81:49:28.4: 13.21 +/- 0.03 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 13:09:20.48 +81:49:28.4: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461258.8011,12.31,0.05,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 20260806.3011 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 12.28 12:56:01.03 +82:15:23.0
122.74392 34.87019 galactic Cam Second-epoch detections are separated by 1.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:56:01.03 +82:15:23.0 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.028 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 12:56:01.03 +82:15:23.0: 13.19 +/- 0.03 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 12:56:01.03 +82:15:23.0: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8011,12.28,0.05,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 20260806.3011 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 08 06.3011 2461258.8011 11.64 10:43:05.53 +74:06:37.4
133.90305 40.16612 galactic Dra Second-epoch detections are separated by 1.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:43:05.53 +74:06:37.4 (user input) | T | P | (position from user input) J-Ks=0.740+/-0.029 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:43:05.53 +74:06:37.4: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:43:05.53 +74:06:37.4: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 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,2461258.8011,11.64,0.05,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 20260806.3011 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.60 10:57:48.10 +73:28:19.8
133.30883 41.28751 galactic Dra Second-epoch detections are separated by 1.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:57:48.10 +73:28:19.8 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.030 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:57:48.10 +73:28:19.8: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:57:48.10 +73:28:19.8: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8011,11.60,0.05,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 20260806.3011 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.52 10:33:52.68 +73:58:40.7
134.65051 39.86485 galactic Dra Second-epoch detections are separated by 2.1" and 6.2 pix
The object was found in VSX 2" Gaia DR3 1078396640835934080
Type: ROT
# Max. Min./Amp. JD0 Period
12.640 G 12.680 G K
The object was not found in astcheck.
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:33:52.68 +73:58:40.7: 12.92 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:33:52.68 +73:58:40.7: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078396640835934080,2461258.8011,11.52,0.05,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 1078396640835934080 20260806.3011 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.62 10:59:51.74 +73:23:15.2
133.20965 41.43984 galactic Dra Second-epoch detections are separated by 0.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:59:51.74 +73:23:15.2 (user input) | T | P | (position from user input) J-Ks=0.499+/-0.028 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:59:51.74 +73:23:15.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:59:51.74 +73:23:15.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8011,11.62,0.05,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 20260806.3011 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.50 10:33:02.61 +74:25:46.5
134.32203 39.48635 galactic Dra Second-epoch detections are separated by 1.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078467765495050240 | 10:33:02.45 +74:25:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.743+/-0.028 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:33:02.61 +74:25:46.5: 12.77 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:33:02.61 +74:25:46.5: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078467765495050240,2461258.8011,11.50,0.05,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 1078467765495050240 20260806.3011 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.48 10:53:34.81 +73:33:33.7
133.56887 41.04470 galactic Dra Second-epoch detections are separated by 3.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:53:34.81 +73:33:33.7 (user input) | T | P | (position from user input) J-Ks=0.381+/-0.027 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:53:34.81 +73:33:33.7: 12.75 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:53:34.81 +73:33:33.7: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461258.8011,11.48,0.05,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 20260806.3011 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.49 10:32:38.15 +74:20:22.6
134.42536 39.53628 galactic Dra Second-epoch detections are separated by 2.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:32:38.15 +74:20:22.6 (user input) | T | P | (position from user input) J-Ks=0.488+/-0.028 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:32:38.15 +74:20:22.6: 12.72 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:32:38.15 +74:20:22.6: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.8011,11.49,0.05,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 20260806.3011 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.54 10:55:10.49 +73:51:21.9
133.22147 40.86659 galactic Dra Second-epoch detections are separated by 4.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J163.7939+73.8563 | 10:55:10.54 +73:51:23.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.790+/-0.028 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:55:10.49 +73:51:21.9: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:55:10.49 +73:51:21.9: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J163.7939+73.8563,2461258.8011,11.54,0.05,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
ATO J163.7939+73.8563 20260806.3011 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.51 10:30:20.58 +74:38:34.8
134.31522 39.20721 galactic Dra Second-epoch detections are separated by 1.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1126524639901544192 | 10:30:20.56 +74:38:35.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.346+/-0.033 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:30:20.58 +74:38:34.8: 12.50 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:30:20.58 +74:38:34.8: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1126524639901544192,2461258.8011,11.51,0.05,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
Gaia DR3 1126524639901544192 20260806.3011 11.51CV 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 08 06.3011 2461258.8011 11.37 10:53:15.85 +73:39:52.3
133.51199 40.94614 galactic Dra Second-epoch detections are separated by 1.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1077479510699700736 | 10:53:15.87 +73:39:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.331+/-0.027 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:53:15.85 +73:39:52.3: 12.37 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:53:15.85 +73:39:52.3: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1077479510699700736,2461258.8011,11.37,0.05,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 1077479510699700736 20260806.3011 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.27 10:47:36.00 +74:06:19.5
133.58652 40.35823 galactic Dra Second-epoch detections are separated by 1.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078302430729392640 | 10:47:35.99 +74:06:20.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.372+/-0.029 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:47:36.00 +74:06:19.5: 12.34 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:47:36.00 +74:06:19.5: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078302430729392640,2461258.8011,11.27,0.05,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 1078302430729392640 20260806.3011 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.41 11:01:45.03 +73:30:27.5
132.97173 41.41372 galactic Dra Second-epoch detections are separated by 1.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078907570145462272 | 11:01:44.98 +73:30:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.541+/-0.026 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:01:45.03 +73:30:27.5: 12.33 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:01:45.03 +73:30:27.5: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078907570145462272,2461258.8011,11.41,0.05,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 1078907570145462272 20260806.3011 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.16 10:24:56.60 +74:13:04.5
135.03080 39.27652 galactic Dra Second-epoch detections are separated by 2.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1126476879865271936 | 10:24:56.45 +74:13:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.348+/-0.032 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:24:56.60 +74:13:04.5: 12.34 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:24:56.60 +74:13:04.5: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1126476879865271936,2461258.8011,11.16,0.05,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 1126476879865271936 20260806.3011 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.35 10:48:42.18 +74:10:42.9
133.44985 40.34469 galactic Dra Second-epoch detections are separated by 0.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078303839478665088 | 10:48:42.17 +74:10:41.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.730+/-0.027 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:48:42.18 +74:10:42.9: 12.30 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:48:42.18 +74:10:42.9: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078303839478665088,2461258.8011,11.35,0.05,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 1078303839478665088 20260806.3011 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.26 10:46:57.44 +74:09:09.4
133.59527 40.29409 galactic Dra Second-epoch detections are separated by 4.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078313838162533760 | 10:46:57.34 +74:09:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.344+/-0.029 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:46:57.44 +74:09:09.4: 12.27 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:46:57.44 +74:09:09.4: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078313838162533760,2461258.8011,11.26,0.05,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 1078313838162533760 20260806.3011 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.23 11:08:12.35 +73:06:51.9
132.72812 41.99363 galactic Dra Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078667915266755584 | 11:08:12.48 +73:06:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.386+/-0.027 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:08:12.35 +73:06:51.9: 12.21 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:08:12.35 +73:06:51.9: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078667915266755584,2461258.8011,11.23,0.05,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 1078667915266755584 20260806.3011 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.27 10:49:20.71 +73:51:29.9
133.65404 40.62827 galactic Dra Second-epoch detections are separated by 2.5" and 5.5 pix
The object was found in VSX 2" ASASSN-V J104920.69+735131.6
Type: ROT
# Max. Min./Amp. JD0 Period
12.810 g Y 0.080 g 2458477.99300 1.043600000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:49:20.71 +73:51:29.9: 12.19 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:49:20.71 +73:51:29.9: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J104920.69+735131.6,2461258.8011,11.27,0.05,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
ASASSN-V J104920.69+735131.6 20260806.3011 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.16 10:16:27.01 +74:44:27.3
135.08325 38.50545 galactic Dra Second-epoch detections are separated by 1.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1126749077712723712 | 10:16:27.08 +74:44:26.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.386+/-0.027 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:16:27.01 +74:44:27.3: 12.14 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:16:27.01 +74:44:27.3: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1126749077712723712,2461258.8011,11.16,0.05,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 1126749077712723712 20260806.3011 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.00 10:28:12.73 +74:02:20.5
134.97647 39.55969 galactic Dra Second-epoch detections are separated by 1.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078430416458748672 | 10:28:12.51 +74:02:21.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.423+/-0.034 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:28:12.73 +74:02:20.5: 12.14 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:28:12.73 +74:02:20.5: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078430416458748672,2461258.8011,11.00,0.05,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 1078430416458748672 20260806.3011 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.12 10:31:52.06 +74:38:51.8
134.21335 39.27033 galactic Dra Second-epoch detections are separated by 0.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1126512304755463168 | 10:31:52.13 +74:38:52.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.348+/-0.027 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:31:52.06 +74:38:51.8: 12.08 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:31:52.06 +74:38:51.8: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1126512304755463168,2461258.8011,11.12,0.05,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 1126512304755463168 20260806.3011 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 11.03 10:51:03.72 +73:54:47.0
133.48479 40.65465 galactic Dra Second-epoch detections are separated by 0.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078251642740023168 | 10:51:03.71 +73:54:47.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.371+/-0.028 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:51:03.72 +73:54:47.0: 12.02 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:51:03.72 +73:54:47.0: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078251642740023168,2461258.8011,11.03,0.05,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 1078251642740023168 20260806.3011 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.80 10:36:29.57 +74:11:01.1
134.29898 39.82485 galactic Dra Second-epoch detections are separated by 1.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078399870652036864 | 10:36:29.43 +74:11:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.771+/-0.036 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:36:29.57 +74:11:01.1: 11.95 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:36:29.57 +74:11:01.1: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078399870652036864,2461258.8011,10.80,0.05,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 1078399870652036864 20260806.3011 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.80 10:40:45.62 +74:09:58.9
134.02039 40.02307 galactic Dra Second-epoch detections are separated by 0.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078478966769176960 | 10:40:45.86 +74:09:57.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:40:45.62 +74:09:58.9: 11.89 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:40:45.62 +74:09:58.9: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078478966769176960,2461258.8011,10.80,0.05,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 1078478966769176960 20260806.3011 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.88 11:06:16.65 +73:13:24.2
132.81084 41.82759 galactic Dra Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1078718527160034560 | 11:06:16.63 +73:13:25.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.465+/-0.031 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:06:16.65 +73:13:24.2: 11.88 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:06:16.65 +73:13:24.2: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1078718527160034560,2461258.8011,10.88,0.05,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
Large-amplitude variable Gaia DR2 1078718527160034560 20260806.3011 10.88CV 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 08 06.3011 2461258.8011 10.82 10:57:41.89 +73:41:29.4
133.15277 41.10211 galactic Dra Second-epoch detections are separated by 1.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078967635264124416 | 10:57:41.87 +73:41:29.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.680+/-0.028 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:57:41.89 +73:41:29.4: 11.82 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:57:41.89 +73:41:29.4: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078967635264124416,2461258.8011,10.82,0.05,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 1078967635264124416 20260806.3011 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.84 11:04:16.94 +73:07:37.5
133.04368 41.83198 galactic Dra Second-epoch detections are separated by 0.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078694367968901120 | 11:04:16.79 +73:07:37.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.686+/-0.027 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:04:16.94 +73:07:37.5: 11.77 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:04:16.94 +73:07:37.5: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078694367968901120,2461258.8011,10.84,0.05,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 1078694367968901120 20260806.3011 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.53 10:30:41.12 +74:00:45.1
134.83574 39.69351 galactic Dra Second-epoch detections are separated by 0.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078438151696036224 | 10:30:41.17 +74:00:45.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.424+/-0.033 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:30:41.12 +74:00:45.1: 11.71 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:30:41.12 +74:00:45.1: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078438151696036224,2461258.8011,10.53,0.05,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 1078438151696036224 20260806.3011 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.68 10:24:07.23 +74:33:43.7
134.77825 38.98812 galactic Dra Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1126544602909610368 | 10:24:07.07 +74:33:43.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.674+/-0.028 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:24:07.23 +74:33:43.7: 11.58 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:24:07.23 +74:33:43.7: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1126544602909610368,2461258.8011,10.68,0.05,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
Gaia DR3 1126544602909610368 20260806.3011 10.68CV 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 08 06.3011 2461258.8011 10.68 10:59:46.38 +73:34:10.8
133.08203 41.28482 galactic Dra Second-epoch detections are separated by 1.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078921352696530304 | 10:59:46.49 +73:34:10.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.321+/-0.028 (F)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:59:46.38 +73:34:10.8: 11.53 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:59:46.38 +73:34:10.8: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078921352696530304,2461258.8011,10.68,0.05,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
Gaia DR3 1078921352696530304 20260806.3011 10.68CV 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 08 06.3011 2461258.8011 10.29 10:34:40.87 +74:18:28.7
134.31643 39.65049 galactic Dra Second-epoch detections are separated by 0.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078452033030295552 | 10:34:40.97 +74:18:28.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.401+/-0.033 (G)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:34:40.87 +74:18:28.7: 11.25 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:34:40.87 +74:18:28.7: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.26 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078452033030295552,2461258.8011,10.29,0.05,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 1078452033030295552 20260806.3011 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 10.09 10:59:20.06 +73:27:08.9
133.20323 41.36494 galactic Dra Second-epoch detections are separated by 0.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078902179962918912 | 10:59:20.29 +73:27:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:59:20.06 +73:27:08.9: 11.04 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:59:20.06 +73:27:08.9: 11.01 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078902179962918912,2461258.8011,10.09,0.05,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 1078902179962918912 20260806.3011 10.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 9.85 10:33:58.76 +74:14:46.8
134.41544 39.66632 galactic Dra Second-epoch detections are separated by 0.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078450173309006848 | 10:33:58.74 +74:14:46.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1949UppAn...3c....S [S49] 22 J-Ks=0.320+/-0.031 (F)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:33:58.76 +74:14:46.8: 10.75 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:33:58.76 +74:14:46.8: 10.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078450173309006848,2461258.8011,9.85,0.05,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
Gaia DR3 1078450173309006848 20260806.3011 9.85CV 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 08 06.3011 2461258.8011 9.56 10:43:58.86 +73:36:31.4
134.24681 40.59846 galactic Dra Second-epoch detections are separated by 0.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078217768334087808 | 10:43:58.93 +73:36:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K2III 1949UppAn...3c....S BD+74 441 J-Ks=0.955+/-0.028 (M)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:43:58.86 +73:36:31.4: 10.45 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:43:58.86 +73:36:31.4: 10.38 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.42 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078217768334087808,2461258.8011,9.56,0.05,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 1078217768334087808 20260806.3011 9.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3011 2461258.8011 9.46 10:26:11.04 +74:07:36.4
135.03161 39.40087 galactic Dra Second-epoch detections are separated by 0.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1078433925448239360 | 10:26:11.11 +74:07:36.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.710+/-0.034 (K)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:26:11.04 +74:07:36.4: 10.39 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:26:11.04 +74:07:36.4: 10.37 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.38 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1078433925448239360,2461258.8011,9.46,0.05,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 1078433925448239360 20260806.3011 9.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79122913 11.02.2026 06:59:12.197 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
First image: 2461082.79122913 11.02.2026 06:59:12.197 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
Last image: 2461258.80150912 06.08.2026 07:14:00.388 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7541
Objects passed selection criteria: 7526
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 5064.75
Average stars matched: 4558 (89.9946 %)
Memory usage VmPeak: 234768 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 02:16:55 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79122913 11.02.2026 06:59:12.197 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
First image: 2461082.79122913 11.02.2026 06:59:12.197 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
Last image: 2461258.80150912 06.08.2026 07:14:00.388 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 76
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 10 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 41429
Objects passed selection criteria: 41318
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: 29445.5
Average stars matched: 27358 (92.9106 %)
Memory usage VmPeak: 268624 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 02:17:39 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
SExtractor catalog cache: saved Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.cat to cache
SExtractor catalog cache: saved Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.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/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.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: 2461258.80075970
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits exists and is non-empty
Saving wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits to local_wcs_cache/
'wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits' -> 'local_wcs_cache/wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits'
wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits exists and is non-empty
Saving wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits to local_wcs_cache/
'wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits' -> 'local_wcs_cache/wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits'
wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits exists and is non-empty
Saving wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits to local_wcs_cache/
'wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits' -> 'local_wcs_cache/wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits'
wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits exists and is non-empty
Saving wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits to local_wcs_cache/
'wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits' -> 'local_wcs_cache/wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits (1st reference image)
verification OK: wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
Image size: 941.9'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:58.925 +77:29:59.77 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_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits (1st new image)
verification OK: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
Image size: 941.4'x627.0' 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: 12:00:55.445 +77:30:25.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:58.925 +77:29:59.77
Second-epoch image center 12:00:55.445 +77:30:25.62
Angular distance between the image centers 0.0515 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits (2nd new image)
verification OK: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
Image size: 941.4'x627.0' 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: 12:00:53.026 +77:30:55.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:58.925 +77:29:59.77
Second-epoch image center 12:00:53.026 +77:30:55.47
Angular distance between the image centers 0.0512 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:00:55.445 +77:30:25.62
Second-epoch second image center 12:00:53.026 +77:30:55.47
Angular distance between the image centers 0.00857 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits &> /tmp/tmp.NSMEDvNNoU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits &> /tmp/tmp.1KreiA0dwD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits &> /tmp/tmp.6dNrAKlCIp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits &> /tmp/tmp.4g2UtOv0Ou
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.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_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits and wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits and wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat
Found non-empty wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits and wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat
The reference image (wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits) and catalog (wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat) found
'wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat' -> 'wcsmag.cat'
Read 8935 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 137.2520 to 228.8003 deg, Dec +69.4278 to +83.2203 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 137.2520 to 228.8003 deg, Dec 69.4278 to 83.2203 deg
Loaded 11837 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): 5410 out of 5718 total matches.
Matched with Tycho-2 5718 out of 8935 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.862250
a=0.000000 b=1.000000 c=22.862250
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8935 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 137.2520 to 228.8003 deg, Dec +69.4278 to +83.2203 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 137.2520 to 228.8003 deg, Dec 69.4278 to 83.2203 deg
Loaded 11837 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): 5410 out of 5718 total matches.
Matched with Tycho-2 5718 out of 8935 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
Forced-photometry filter: calibrated wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits -> calib.txt_param_ref_wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits (aperture=6.2)
Read 9444 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 132.7167 to 226.3162 deg, Dec +70.5552 to +82.7628 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 132.7167 to 226.3162 deg, Dec 70.5552 to 82.7628 deg
Loaded 10553 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): 3703 out of 3846 total matches.
Matched with Tycho-2 3846 out of 9444 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
Forced-photometry filter: calibrated wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits -> calib.txt_param_ref_wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
2.3 pix Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
2.1 pix fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
2.1 pix fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
Limiting magnitude estimates:
15.3 mag. Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
15.2 mag. Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
12.1 mag. fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
12.0 mag. fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
All-image limiting magnitude estimate: 12.0 (SNR ) 9.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.NSMEDvNNoU (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits' -> 'wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
WCS_IMAGE_NAME=wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
WCS-calibrated image found: wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
Checking if the catalog wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat corresponding to the image wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits alredy exist and is non-empty...
Catalog wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat corresponding to the image wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
WCS catalog name: wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=680, bad_region=0, passed=8935
Got 8935 stars (including 8237 good ones) from the SExtractor catalog wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat
util/solve_plate_with_UCAC5 got 8935 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 797 to 868 (Dec 69.4 to 83.2)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 8935 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 797 to 868 (Dec 69.4 to 83.2)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 8935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 8935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4901 stars left (next iteration limit 5391)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits N_match=4901 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.462 sigma_q2_arcsec=0.359 sigma_q3_arcsec=0.342 sigma_q4_arcsec=0.305 n_q1=1059 n_q2=1199 n_q3=1313 n_q4=1330 worst_quadrant_to_overall_ratio=1.299
The image catalog is written to wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits -region wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1KreiA0dwD (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits' -> 'wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
WCS_IMAGE_NAME=wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
WCS-calibrated image found: wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
Checking if the catalog wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat corresponding to the image wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits alredy exist and is non-empty...
Catalog wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat corresponding to the image wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
WCS catalog name: wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=593, bad_region=0, passed=9444
Got 9444 stars (including 8840 good ones) from the SExtractor catalog wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat
util/solve_plate_with_UCAC5 got 9444 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.6 to 82.8)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 4895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 9444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.6 to 82.8)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 9444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 9444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4896 stars left (next iteration limit 5384)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits N_match=4896 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.369 sigma_q3_arcsec=0.318 sigma_q4_arcsec=0.311 n_q1=1140 n_q2=1167 n_q3=1319 n_q4=1270 worst_quadrant_to_overall_ratio=1.150
The image catalog is written to wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits -region wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6dNrAKlCIp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
WCS_IMAGE_NAME=wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
WCS-calibrated image found: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
Checking if the catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat corresponding to the image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat corresponding to the image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
WCS catalog name: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=52, bad_region=0, passed=1003
Got 1003 stars (including 950 good ones) from the SExtractor catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat
util/solve_plate_with_UCAC5 got 1003 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.4 to 82.7)
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.4 to 82.7)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 912 stars left (next iteration limit 1001)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=912 robust_rms=9.483 arcsec worst_quadrant_rms=23.903 arcsec
SIP_REFIT: SIP order 3 trial: matched=912 robust_rms=0.497 arcsec worst_quadrant_rms=0.585 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=912 robust_rms_before=0.831 arcsec robust_rms_before_corrected=0.409 arcsec robust_rms_after=0.497 arcsec worst_quadrant_rms_before=0.465 worst_quadrant_rms_after=0.585
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.465 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits N_match=912 sigma_overall_arcsec=0.429 sigma_q1_arcsec=0.412 sigma_q2_arcsec=0.483 sigma_q3_arcsec=0.424 sigma_q4_arcsec=0.420 n_q1=323 n_q2=173 n_q3=249 n_q4=167 worst_quadrant_to_overall_ratio=1.127
The image catalog is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits -region wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4g2UtOv0Ou (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
WCS_IMAGE_NAME=wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
WCS-calibrated image found: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
Checking if the catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat corresponding to the image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat corresponding to the image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
WCS catalog name: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=52, bad_region=0, passed=1017
Got 1017 stars (including 964 good ones) from the SExtractor catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat
util/solve_plate_with_UCAC5 got 1017 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 866 (Dec 70.4 to 82.8)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 1001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 866 (Dec 70.4 to 82.8)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 1000 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 1000 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 923 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=923 robust_rms=9.114 arcsec worst_quadrant_rms=17.689 arcsec
SIP_REFIT: SIP order 3 trial: matched=923 robust_rms=0.487 arcsec worst_quadrant_rms=0.533 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=923 robust_rms_before=0.829 arcsec robust_rms_before_corrected=0.418 arcsec robust_rms_after=0.487 arcsec worst_quadrant_rms_before=0.423 worst_quadrant_rms_after=0.533
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.423 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits N_match=923 sigma_overall_arcsec=0.418 sigma_q1_arcsec=0.392 sigma_q2_arcsec=0.420 sigma_q3_arcsec=0.419 sigma_q4_arcsec=0.464 n_q1=307 n_q2=189 n_q3=254 n_q4=173 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits -region wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits sigma_overall=0.355 worst_q_ratio=1.299
ref2=Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits sigma_overall=0.320 worst_q_ratio=1.150
new1=fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits sigma_overall=0.429 worst_q_ratio=1.127
new2=fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits sigma_overall=0.418 worst_q_ratio=1.108
reference average sigma_overall=0.3375 worst_q_ratio=1.2245
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284_astrometric_residuals.png (4901 matched stars from wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280_astrometric_residuals.png (4896 matched stars from wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260_astrometric_residuals.png (912 matched stars from wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261_astrometric_residuals.png (923 matched stars from wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits'
Saving fully-calibrated image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits'
Preparing the HTML report for the field Cam-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cam-05-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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
SExtractor catalog cache: saved Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.cat to cache
SExtractor catalog cache: saved Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
Creating symlink local_wcs_cache/wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.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_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits exists and is non-empty
wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits exists and is non-empty
wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits exists and is non-empty
wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits (1st reference image)
verification OK: wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
Image size: 941.9'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:58.925 +77:29:59.77 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_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits (1st new image)
verification OK: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
Image size: 941.4'x627.0' 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: 12:00:55.445 +77:30:25.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:58.925 +77:29:59.77
Second-epoch image center 12:00:55.445 +77:30:25.62
Angular distance between the image centers 0.0515 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits (2nd new image)
verification OK: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
Image size: 941.4'x627.0' 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: 12:00:53.026 +77:30:55.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:58.925 +77:29:59.77
Second-epoch image center 12:00:53.026 +77:30:55.47
Angular distance between the image centers 0.0512 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:00:55.445 +77:30:25.62
Second-epoch second image center 12:00:53.026 +77:30:55.47
Angular distance between the image centers 0.00857 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits &> /tmp/tmp.sI18F8xLH8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits &> /tmp/tmp.QmmJ9XwY9j
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits &> /tmp/tmp.GZLsW3Xei3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits &> /tmp/tmp.TqUoLfMT1t
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.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_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits and wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits and wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat
Found non-empty wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits and wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat
The reference image (wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits) and catalog (wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat) found
'wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat' -> 'wcsmag.cat'
Read 51561 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 136.5617 to 229.0190 deg, Dec +69.4278 to +83.2318 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 136.5617 to 229.0190 deg, Dec 69.4278 to 83.2318 deg
Loaded 12006 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): 5102 out of 5807 total matches.
Matched with Tycho-2 5807 out of 51561 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.749000
a=0.000000 b=1.000000 c=22.749000
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 51561 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 136.5617 to 229.0190 deg, Dec +69.4278 to +83.2318 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 136.5617 to 229.0190 deg, Dec 69.4278 to 83.2318 deg
Loaded 12006 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): 5102 out of 5807 total matches.
Matched with Tycho-2 5807 out of 51561 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
Forced-photometry filter: calibrated wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits -> calib.txt_param_ref_wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits (aperture=4.8)
Read 48477 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 132.3942 to 226.7803 deg, Dec +70.4537 to +82.7794 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 132.3942 to 226.7803 deg, Dec 70.4537 to 82.7794 deg
Loaded 10790 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): 3498 out of 3909 total matches.
Matched with Tycho-2 3909 out of 48477 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
Forced-photometry filter: calibrated wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits -> calib.txt_param_ref_wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits (aperture=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 73 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
2.2 pix Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
1.9 pix fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
2.0 pix fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
Limiting magnitude estimates:
15.4 mag. Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
15.4 mag. Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
12.5 mag. fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
12.5 mag. fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.sI18F8xLH8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits' -> 'wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
WCS_IMAGE_NAME=wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
WCS-calibrated image found: wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
Checking if the catalog wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat corresponding to the image wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits alredy exist and is non-empty...
Catalog wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat corresponding to the image wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits
WCS catalog name: wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=2563, bad_region=1, passed=51537
Got 51537 stars (including 48894 good ones) from the SExtractor catalog wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat
util/solve_plate_with_UCAC5 got 51537 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 797 to 868 (Dec 69.4 to 83.2)
Done reading UCAC5 zone files...
Matched 4900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 4896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 51537 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 797 to 868 (Dec 69.4 to 83.2)
Done reading UCAC5 zone files...
Matched 4900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 51537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 51537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4896 stars left (next iteration limit 5385)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits N_match=4896 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.344 sigma_q3_arcsec=0.324 sigma_q4_arcsec=0.296 n_q1=1055 n_q2=1197 n_q3=1288 n_q4=1356 worst_quadrant_to_overall_ratio=1.284
The image catalog is written to wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits -region wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QmmJ9XwY9j (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits' -> 'wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
WCS_IMAGE_NAME=wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
WCS-calibrated image found: wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
Checking if the catalog wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat corresponding to the image wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits alredy exist and is non-empty...
Catalog wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat corresponding to the image wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits
WCS catalog name: wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=2481, bad_region=0, passed=48460
Got 48460 stars (including 45910 good ones) from the SExtractor catalog wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat
util/solve_plate_with_UCAC5 got 48460 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.5 to 82.8)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 4888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 48460 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.5 to 82.8)
Done reading UCAC5 zone files...
Matched 4891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 48460 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 48460 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4890 stars left (next iteration limit 5376)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits N_match=4890 sigma_overall_arcsec=0.317 sigma_q1_arcsec=0.294 sigma_q2_arcsec=0.354 sigma_q3_arcsec=0.315 sigma_q4_arcsec=0.320 n_q1=1139 n_q2=1198 n_q3=1281 n_q4=1272 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits -region wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GZLsW3Xei3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
WCS_IMAGE_NAME=wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
WCS-calibrated image found: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
Checking if the catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat corresponding to the image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat corresponding to the image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
WCS catalog name: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=208, bad_region=2, passed=9299
Got 9299 stars (including 9069 good ones) from the SExtractor catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat
util/solve_plate_with_UCAC5 got 9299 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.4 to 82.8)
Done reading UCAC5 zone files...
Matched 4860 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4851 matched stars entering correct_measured_positions(), 4851 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4851 matched stars entering correct_measured_positions(), 9299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.4 to 82.8)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 9299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 9299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4853 stars left (next iteration limit 5336)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits N_match=4853 sigma_overall_arcsec=0.542 sigma_q1_arcsec=0.488 sigma_q2_arcsec=0.559 sigma_q3_arcsec=0.569 sigma_q4_arcsec=0.588 n_q1=1791 n_q2=1135 n_q3=1131 n_q4=796 worst_quadrant_to_overall_ratio=1.084
The image catalog is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits -region wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TqUoLfMT1t (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
WCS_IMAGE_NAME=wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
WCS-calibrated image found: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
Checking if the catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat corresponding to the image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat corresponding to the image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
WCS catalog name: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=179, bad_region=4, passed=9339
Got 9339 stars (including 9132 good ones) from the SExtractor catalog wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat
util/solve_plate_with_UCAC5 got 9339 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 866 (Dec 70.4 to 82.8)
Done reading UCAC5 zone files...
Matched 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 4859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 9338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 866 (Dec 70.4 to 82.8)
Done reading UCAC5 zone files...
Matched 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 9338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 9338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4860 stars left (next iteration limit 5346)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits N_match=4860 sigma_overall_arcsec=0.541 sigma_q1_arcsec=0.508 sigma_q2_arcsec=0.553 sigma_q3_arcsec=0.568 sigma_q4_arcsec=0.558 n_q1=1681 n_q2=1138 n_q3=1191 n_q4=850 worst_quadrant_to_overall_ratio=1.050
The image catalog is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits -region wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-12-55_20.00sec_-0.00C_LIGHTs_0260.fits
Saving fully-calibrated image wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Cam-05-Q1b1x1_021435_TTUQ1b1x1_2466978_UJUJmjlP/wcs_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261.fits
Preparing the HTML report for the field Cam-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:27:02.29 +79:37:52.9: 10.53 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 13:41:48.81 +80:13:24.1: 12.37 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:21:47.29 +74:22:09.5: 10.67 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:21:54.04 +74:33:31.6: 11.09 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:35:05.58 +73:46:59.7: 11.49 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:52:24.12 +73:24:09.5: 12.02 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:02:39.58 +73:16:14.5: 11.76 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:37:08.89 +74:02:50.9: 11.72 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:24:07.46 +74:52:54.6: 11.77 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:26:41.33 +74:18:27.1: 12.01 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:27:02.29 +79:37:52.9: 10.45 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 13:41:48.81 +80:13:24.1: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.49 +/- 0.00
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter REJECTED candidate at 11:27:02.29 +79:37:52.9: ref_mag=10.49 +/- 0.00 new_mean_mag=10.9178 delta=-0.43 (need > 0.90)
Forced photometry filter REJECTED candidate at 13:41:48.81 +80:13:24.1: ref_mag=12.35 +/- 0.01 new_mean_mag=11.7520 delta=0.60 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:21:47.29 +74:22:09.5: 10.68 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.67 +/- 0.00
Forced photometry filter KEPT candidate at 10:21:47.29 +74:22:09.5: ref_mag=10.67 +/- 0.00 new_mean_mag=9.7601 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:21:54.04 +74:33:31.6: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.00
Forced photometry filter KEPT candidate at 10:21:54.04 +74:33:31.6: ref_mag=11.09 +/- 0.00 new_mean_mag=10.0769 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:35:05.58 +73:46:59.7: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.00
Forced photometry filter KEPT candidate at 10:35:05.58 +73:46:59.7: ref_mag=11.51 +/- 0.00 new_mean_mag=10.4077 delta=1.10 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:02:39.58 +73:16:14.5: 11.74 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:37:08.89 +74:02:50.9: 11.74 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:26:41.33 +74:18:27.1: 12.00 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:24:07.46 +74:52:54.6: 11.81 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:52:24.12 +73:24:09.5: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter KEPT candidate at 11:02:39.58 +73:16:14.5: ref_mag=11.75 +/- 0.01 new_mean_mag=10.8395 delta=0.91 (need > 0.90)
Forced photometry filter KEPT candidate at 10:37:08.89 +74:02:50.9: ref_mag=11.73 +/- 0.01 new_mean_mag=10.7073 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 10:26:41.33 +74:18:27.1: ref_mag=12.00 +/- 0.01 new_mean_mag=10.8342 delta=1.17 (need > 0.90)
Forced photometry filter KEPT candidate at 10:24:07.46 +74:52:54.6: ref_mag=11.79 +/- 0.01 new_mean_mag=10.8664 delta=0.92 (need > 0.90)
Forced photometry filter KEPT candidate at 10:52:24.12 +73:24:09.5: ref_mag=12.02 +/- 0.01 new_mean_mag=10.9843 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:40:45.77 +74:17:07.3: 12.03 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:31:45.82 +74:42:03.6: 12.03 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:40:45.77 +74:17:07.3: 11.98 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:31:45.82 +74:42:03.6: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Forced photometry filter KEPT candidate at 10:40:45.77 +74:17:07.3: ref_mag=12.01 +/- 0.01 new_mean_mag=11.0425 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 10:31:45.82 +74:42:03.6: ref_mag=12.03 +/- 0.01 new_mean_mag=11.0271 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:32:06.90 +74:06:06.9: 12.09 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:26:35.09 +74:51:53.7: 12.12 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:10:48.83 +72:52:18.9: 12.24 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:30:24.83 +74:22:38.1: 12.35 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:32:06.90 +74:06:06.9: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter KEPT candidate at 10:32:06.90 +74:06:06.9: ref_mag=12.09 +/- 0.01 new_mean_mag=10.8062 delta=1.29 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:26:35.09 +74:51:53.7: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 10:26:35.09 +74:51:53.7: ref_mag=12.13 +/- 0.01 new_mean_mag=11.2184 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:10:48.83 +72:52:18.9: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry filter KEPT candidate at 11:10:48.83 +72:52:18.9: ref_mag=12.22 +/- 0.01 new_mean_mag=11.3134 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:30:24.83 +74:22:38.1: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 10:30:24.83 +74:22:38.1: ref_mag=12.36 +/- 0.01 new_mean_mag=11.2574 delta=1.10 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:49:14.86 +74:05:02.4: 12.48 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:36:59.47 +74:26:19.5: 12.49 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:49:14.86 +74:05:02.4: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter KEPT candidate at 10:49:14.86 +74:05:02.4: ref_mag=12.49 +/- 0.01 new_mean_mag=11.5230 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:36:59.47 +74:26:19.5: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter KEPT candidate at 10:36:59.47 +74:26:19.5: ref_mag=12.50 +/- 0.01 new_mean_mag=11.4622 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:29:16.91 +74:07:10.3: 12.52 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:35:12.34 +73:53:32.6: 12.52 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:36:15.94 +74:14:39.2: 12.75 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:29:16.91 +74:07:10.3: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter KEPT candidate at 10:29:16.91 +74:07:10.3: ref_mag=12.51 +/- 0.01 new_mean_mag=11.2219 delta=1.29 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:35:12.34 +73:53:32.6: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 10:35:12.34 +73:53:32.6: ref_mag=12.54 +/- 0.01 new_mean_mag=11.2807 delta=1.26 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:36:15.94 +74:14:39.2: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 10:36:15.94 +74:14:39.2: ref_mag=12.77 +/- 0.01 new_mean_mag=11.4697 delta=1.30 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:32:53.60 +74:16:18.7: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:32:53.60 +74:16:18.7: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 10:32:53.60 +74:16:18.7: ref_mag=13.08 +/- 0.02 new_mean_mag=11.7426 delta=1.34 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 13:09:20.48 +81:49:28.4: 13.21 +/- 0.03 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 13:09:20.48 +81:49:28.4: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 13:09:20.48 +81:49:28.4: ref_mag=13.27 +/- 0.02 new_mean_mag=12.3038 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 12:56:01.03 +82:15:23.0: 13.19 +/- 0.03 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:43:05.53 +74:06:37.4: 12.95 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:57:48.10 +73:28:19.8: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 12:56:01.03 +82:15:23.0: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 12:56:01.03 +82:15:23.0: ref_mag=13.25 +/- 0.02 new_mean_mag=12.2398 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:43:05.53 +74:06:37.4: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 10:43:05.53 +74:06:37.4: ref_mag=12.94 +/- 0.02 new_mean_mag=11.6088 delta=1.33 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:57:48.10 +73:28:19.8: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 10:57:48.10 +73:28:19.8: ref_mag=12.90 +/- 0.01 new_mean_mag=11.6016 delta=1.30 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:33:52.68 +73:58:40.7: 12.92 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:59:51.74 +73:23:15.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:33:52.68 +73:58:40.7: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 10:33:52.68 +73:58:40.7: ref_mag=12.84 +/- 0.01 new_mean_mag=11.5075 delta=1.34 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:59:51.74 +73:23:15.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 10:59:51.74 +73:23:15.2: ref_mag=12.76 +/- 0.01 new_mean_mag=11.6243 delta=1.14 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:33:02.61 +74:25:46.5: 12.77 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:53:34.81 +73:33:33.7: 12.75 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:32:38.15 +74:20:22.6: 12.72 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:33:02.61 +74:25:46.5: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 10:33:02.61 +74:25:46.5: ref_mag=12.76 +/- 0.01 new_mean_mag=11.5128 delta=1.24 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:55:10.49 +73:51:21.9: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:53:34.81 +73:33:33.7: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 10:53:34.81 +73:33:33.7: ref_mag=12.77 +/- 0.01 new_mean_mag=11.4725 delta=1.30 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:32:38.15 +74:20:22.6: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 10:32:38.15 +74:20:22.6: ref_mag=12.71 +/- 0.01 new_mean_mag=11.4891 delta=1.22 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:55:10.49 +73:51:21.9: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 10:55:10.49 +73:51:21.9: ref_mag=12.72 +/- 0.01 new_mean_mag=11.5464 delta=1.18 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:30:20.58 +74:38:34.8: 12.50 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:30:20.58 +74:38:34.8: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 10:30:20.58 +74:38:34.8: ref_mag=12.52 +/- 0.01 new_mean_mag=11.4719 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:53:15.85 +73:39:52.3: 12.37 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:47:36.00 +74:06:19.5: 12.34 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:53:15.85 +73:39:52.3: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 10:53:15.85 +73:39:52.3: ref_mag=12.36 +/- 0.01 new_mean_mag=11.3520 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:47:36.00 +74:06:19.5: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 10:47:36.00 +74:06:19.5: ref_mag=12.33 +/- 0.01 new_mean_mag=11.2674 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:01:45.03 +73:30:27.5: 12.33 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:24:56.60 +74:13:04.5: 12.34 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:01:45.03 +73:30:27.5: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 11:01:45.03 +73:30:27.5: ref_mag=12.31 +/- 0.01 new_mean_mag=11.3670 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:24:56.60 +74:13:04.5: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 10:24:56.60 +74:13:04.5: ref_mag=12.36 +/- 0.01 new_mean_mag=11.1516 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:48:42.18 +74:10:42.9: 12.30 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:46:57.44 +74:09:09.4: 12.27 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:48:42.18 +74:10:42.9: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter KEPT candidate at 10:48:42.18 +74:10:42.9: ref_mag=12.30 +/- 0.01 new_mean_mag=11.3247 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:46:57.44 +74:09:09.4: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:57.44 +74:09:09.4: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2374 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:08:12.35 +73:06:51.9: 12.21 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:49:20.71 +73:51:29.9: 12.19 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:08:12.35 +73:06:51.9: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 11:08:12.35 +73:06:51.9: ref_mag=12.18 +/- 0.01 new_mean_mag=11.2331 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:16:27.01 +74:44:27.3: 12.14 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:49:20.71 +73:51:29.9: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter KEPT candidate at 10:49:20.71 +73:51:29.9: ref_mag=12.20 +/- 0.01 new_mean_mag=11.2712 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:16:27.01 +74:44:27.3: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry filter KEPT candidate at 10:16:27.01 +74:44:27.3: ref_mag=12.15 +/- 0.01 new_mean_mag=11.1364 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:28:12.73 +74:02:20.5: 12.14 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:28:12.73 +74:02:20.5: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter KEPT candidate at 10:28:12.73 +74:02:20.5: ref_mag=12.14 +/- 0.01 new_mean_mag=10.9903 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:31:52.06 +74:38:51.8: 12.08 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:31:52.06 +74:38:51.8: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry filter KEPT candidate at 10:31:52.06 +74:38:51.8: ref_mag=12.10 +/- 0.01 new_mean_mag=11.0502 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:51:03.72 +73:54:47.0: 12.02 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:36:29.57 +74:11:01.1: 11.95 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:40:45.62 +74:09:58.9: 11.89 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:51:03.72 +73:54:47.0: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter KEPT candidate at 10:51:03.72 +73:54:47.0: ref_mag=12.02 +/- 0.01 new_mean_mag=10.9952 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:36:29.57 +74:11:01.1: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Forced photometry filter KEPT candidate at 10:36:29.57 +74:11:01.1: ref_mag=11.94 +/- 0.01 new_mean_mag=10.7844 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:40:45.62 +74:09:58.9: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Forced photometry filter KEPT candidate at 10:40:45.62 +74:09:58.9: ref_mag=11.89 +/- 0.01 new_mean_mag=10.7914 delta=1.10 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:57:41.89 +73:41:29.4: 11.82 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:06:16.65 +73:13:24.2: 11.88 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 11:04:16.94 +73:07:37.5: 11.77 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:57:41.89 +73:41:29.4: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry filter KEPT candidate at 10:57:41.89 +73:41:29.4: ref_mag=11.81 +/- 0.01 new_mean_mag=10.7709 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:06:16.65 +73:13:24.2: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.01
Forced photometry filter KEPT candidate at 11:06:16.65 +73:13:24.2: ref_mag=11.86 +/- 0.01 new_mean_mag=10.8822 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 11:04:16.94 +73:07:37.5: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter KEPT candidate at 11:04:16.94 +73:07:37.5: ref_mag=11.77 +/- 0.01 new_mean_mag=10.8025 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:30:41.12 +74:00:45.1: 11.71 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:30:41.12 +74:00:45.1: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Forced photometry filter KEPT candidate at 10:30:41.12 +74:00:45.1: ref_mag=11.72 +/- 0.01 new_mean_mag=10.5353 delta=1.19 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:24:07.23 +74:33:43.7: 11.58 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:24:07.23 +74:33:43.7: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.00
Forced photometry filter KEPT candidate at 10:24:07.23 +74:33:43.7: ref_mag=11.58 +/- 0.00 new_mean_mag=10.6303 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:59:46.38 +73:34:10.8: 11.53 +/- 0.01 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:59:46.38 +73:34:10.8: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.00
Forced photometry filter KEPT candidate at 10:59:46.38 +73:34:10.8: ref_mag=11.52 +/- 0.00 new_mean_mag=10.6071 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:34:40.87 +74:18:28.7: 11.25 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:34:40.87 +74:18:28.7: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.26 +/- 0.00
Forced photometry filter KEPT candidate at 10:34:40.87 +74:18:28.7: ref_mag=11.26 +/- 0.00 new_mean_mag=10.2902 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:59:20.06 +73:27:08.9: 11.04 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:33:58.76 +74:14:46.8: 10.75 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:43:58.86 +73:36:31.4: 10.45 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:33:58.76 +74:14:46.8: 10.77 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:59:20.06 +73:27:08.9: 11.01 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.00
Forced photometry filter KEPT candidate at 10:33:58.76 +74:14:46.8: ref_mag=10.76 +/- 0.00 new_mean_mag=9.8319 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Forced photometry filter KEPT candidate at 10:59:20.06 +73:27:08.9: ref_mag=11.02 +/- 0.00 new_mean_mag=10.0812 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:43:58.86 +73:36:31.4: 10.38 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.42 +/- 0.00
Forced photometry filter KEPT candidate at 10:43:58.86 +73:36:31.4: ref_mag=10.42 +/- 0.00 new_mean_mag=9.5147 delta=0.90 (need > 0.90)
Forced photometry on wcs_Cam-05-Q1b1x1_2026-02-11_00-59-12_20.00sec_-15.00C_LIGHT_0284.fits at 10:26:11.04 +74:07:36.4: 10.39 +/- 0.00 detection
Forced photometry on wcs_Cam-05-Q1b1x1_2026-03-21_01-39-13_20.00sec_-14.90C_LIGHT_0280.fits at 10:26:11.04 +74:07:36.4: 10.37 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.38 +/- 0.00
Forced photometry filter KEPT candidate at 10:26:11.04 +74:07:36.4: ref_mag=10.38 +/- 0.00 new_mean_mag=9.4568 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out09007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41283.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 77s
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: 27s
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Considering the candidate 69543_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69543_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
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Considering the candidate 69544_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69544_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
**** FOUND 10:42:28.99 +81:14:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69567_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69567_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 69633_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69633_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 69671_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69671_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
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Considering the candidate 69674_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69674_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
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Considering the candidate 69686_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69686_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
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Considering the candidate 69722_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69722_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 69744_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69744_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
**** FOUND 14:33:05.41 +79:38:43.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 69745_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69745_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
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Considering the candidate 69756_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69756_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
Rejecting candidate due to large distance (27.0") between the two second-epoch detections
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Considering the candidate 69759_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69759_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
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Considering the candidate 69765_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69765_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
Rejecting candidate due to large distance (27.8") between the two second-epoch detections
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Considering the candidate 69769_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69769_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 69784_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 69784_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
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Considering the candidate 23686_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 23686_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 24408_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 24408_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 18651_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 18651_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 19226_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 19226_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 25262_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 25262_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 11770_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 11770_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 22475_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 22475_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 14058_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 14058_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 23003_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 23003_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 19547_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 19547_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 20529_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 20529_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 24716_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 24716_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 09007_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 09007_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 21915_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 21915_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 17264_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 17264_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 20940_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 20940_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 21187_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 21187_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 19079_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 19079_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 20300_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 20300_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 21104_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 21104_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 41283_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 41283_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 39158_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 39158_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 18486_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 18486_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 13399_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 13399_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 19743_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 19743_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 12720_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 12720_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 21674_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 21674_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 14484_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 14484_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 21401_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 21401_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 15391_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 15391_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 23122_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 23122_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 14931_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 14931_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 17630_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 17630_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 12883_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 12883_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 22505_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 22505_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 17709_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 17709_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 17929_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 17929_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 10371_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 10371_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 16365_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 16365_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
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Considering the candidate 26363_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 26363_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21041_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 21041_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22713_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 22713_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16269_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 16269_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19959_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 19959_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19101_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 19101_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11022_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 11022_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14259_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 14259_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10989_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 10989_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20432_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 20432_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24011_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 24011_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13407_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 13407_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20723_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 20723_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12968_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 12968_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20600_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 20600_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16205_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 16205_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21697_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
Preparing report for the candidate 21697_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17237_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 17237_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
**** FOUND 10:41:02.45 +73:46:15.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25864_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261
The candidate 25864_fd_Cam-05-Q1b1x1_2026-08-06_02-14-00_20.00sec_-0.00C_LIGHTs_0261 did not pass the final checks
**** FOUND 10:35:05.39 +75:42:47.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 108s
Prepared the HTML report for the field Cam-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:10:48.83 +72:52:18.9
11:08:12.35 +73:06:51.9
11:04:16.94 +73:07:37.5
11:06:16.65 +73:13:24.2
11:02:39.58 +73:16:14.5
10:59:51.74 +73:23:15.2
11:01:45.03 +73:30:27.5
10:59:20.06 +73:27:08.9
10:57:48.10 +73:28:19.8
10:59:46.38 +73:34:10.8
10:52:24.12 +73:24:09.5
10:57:41.89 +73:41:29.4
10:53:34.81 +73:33:33.7
10:53:15.85 +73:39:52.3
10:55:10.49 +73:51:21.9
10:43:58.86 +73:36:31.4
10:51:03.72 +73:54:47.0
10:49:20.71 +73:51:29.9
10:49:14.86 +74:05:02.4
10:47:36.00 +74:06:19.5
10:48:42.18 +74:10:42.9
10:46:57.44 +74:09:09.4
10:43:05.53 +74:06:37.4
10:35:05.58 +73:46:59.7
10:35:12.34 +73:53:32.6
10:40:45.62 +74:09:58.9
10:37:08.89 +74:02:50.9
10:40:45.77 +74:17:07.3
10:33:52.68 +73:58:40.7
10:36:29.57 +74:11:01.1
10:36:15.94 +74:14:39.2
10:30:41.12 +74:00:45.1
10:32:06.90 +74:06:06.9
10:33:58.76 +74:14:46.8
10:34:40.87 +74:18:28.7
10:36:59.47 +74:26:19.5
10:28:12.73 +74:02:20.5
10:32:53.60 +74:16:18.7
10:29:16.91 +74:07:10.3
10:32:38.15 +74:20:22.6
10:33:02.61 +74:25:46.5
10:26:11.04 +74:07:36.4
10:30:24.83 +74:22:38.1
10:26:41.33 +74:18:27.1
10:24:56.60 +74:13:04.5
10:31:52.06 +74:38:51.8
10:31:45.82 +74:42:03.6
10:30:20.58 +74:38:34.8
10:21:47.29 +74:22:09.5
10:24:07.23 +74:33:43.7
10:21:54.04 +74:33:31.6
10:26:35.09 +74:51:53.7
10:24:07.46 +74:52:54.6
10:16:27.01 +74:44:27.3
12:56:01.03 +82:15:23.0
13:09:20.48 +81:49:28.4
########### Completed Cam-05-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 ####
10:21:47.29 +74:22:09.5
10:21:54.04 +74:33:31.6
10:35:05.58 +73:46:59.7
10:37:08.89 +74:02:50.9
10:24:07.46 +74:52:54.6
11:02:39.58 +73:16:14.5
10:26:41.33 +74:18:27.1
10:52:24.12 +73:24:09.5
10:31:45.82 +74:42:03.6
10:40:45.77 +74:17:07.3
10:32:06.90 +74:06:06.9
10:26:35.09 +74:51:53.7
11:10:48.83 +72:52:18.9
10:30:24.83 +74:22:38.1
10:49:14.86 +74:05:02.4
10:36:59.47 +74:26:19.5
10:29:16.91 +74:07:10.3
10:35:12.34 +73:53:32.6
10:36:15.94 +74:14:39.2
10:32:53.60 +74:16:18.7
13:09:20.48 +81:49:28.4
12:56:01.03 +82:15:23.0
10:43:05.53 +74:06:37.4
10:57:48.10 +73:28:19.8
10:33:52.68 +73:58:40.7
10:59:51.74 +73:23:15.2
10:33:02.61 +74:25:46.5
10:53:34.81 +73:33:33.7
10:32:38.15 +74:20:22.6
10:55:10.49 +73:51:21.9
10:30:20.58 +74:38:34.8
10:53:15.85 +73:39:52.3
10:47:36.00 +74:06:19.5
11:01:45.03 +73:30:27.5
10:24:56.60 +74:13:04.5
10:48:42.18 +74:10:42.9
10:46:57.44 +74:09:09.4
11:08:12.35 +73:06:51.9
10:49:20.71 +73:51:29.9
10:16:27.01 +74:44:27.3
10:28:12.73 +74:02:20.5
10:31:52.06 +74:38:51.8
10:51:03.72 +73:54:47.0
10:36:29.57 +74:11:01.1
10:40:45.62 +74:09:58.9
11:06:16.65 +73:13:24.2
10:57:41.89 +73:41:29.4
11:04:16.94 +73:07:37.5
10:30:41.12 +74:00:45.1
10:24:07.23 +74:33:43.7
10:59:46.38 +73:34:10.8
10:34:40.87 +74:18:28.7
10:59:20.06 +73:27:08.9
10:33:58.76 +74:14:46.8
10:43:58.86 +73:36:31.4
10:26:11.04 +74:07:36.4
###################################################################################
10:21:47.29 +74:22:09.5 -- not an asteroid (will add it to exclusion list)
10:21:54.04 +74:33:31.6 -- not an asteroid (will add it to exclusion list)
10:35:05.58 +73:46:59.7 -- not an asteroid (will add it to exclusion list)
10:37:08.89 +74:02:50.9 -- not an asteroid (will add it to exclusion list)
10:24:07.46 +74:52:54.6 -- not an asteroid (will add it to exclusion list)
11:02:39.58 +73:16:14.5 -- not an asteroid (will add it to exclusion list)
10:26:41.33 +74:18:27.1 -- not an asteroid (will add it to exclusion list)
10:52:24.12 +73:24:09.5 -- not an asteroid (will add it to exclusion list)
10:31:45.82 +74:42:03.6 -- not an asteroid (will add it to exclusion list)
10:40:45.77 +74:17:07.3 -- not an asteroid (will add it to exclusion list)
10:32:06.90 +74:06:06.9 -- not an asteroid (will add it to exclusion list)
10:26:35.09 +74:51:53.7 -- not an asteroid (will add it to exclusion list)
11:10:48.83 +72:52:18.9 -- not an asteroid (will add it to exclusion list)
10:30:24.83 +74:22:38.1 -- not an asteroid (will add it to exclusion list)
10:49:14.86 +74:05:02.4 -- not an asteroid (will add it to exclusion list)
10:36:59.47 +74:26:19.5 -- not an asteroid (will add it to exclusion list)
10:29:16.91 +74:07:10.3 -- not an asteroid (will add it to exclusion list)
10:35:12.34 +73:53:32.6 -- not an asteroid (will add it to exclusion list)
10:36:15.94 +74:14:39.2 -- not an asteroid (will add it to exclusion list)
10:32:53.60 +74:16:18.7 -- not an asteroid (will add it to exclusion list)
13:09:20.48 +81:49:28.4 -- not an asteroid (will add it to exclusion list)
12:56:01.03 +82:15:23.0 -- not an asteroid (will add it to exclusion list)
10:43:05.53 +74:06:37.4 -- not an asteroid (will add it to exclusion list)
10:57:48.10 +73:28:19.8 -- not an asteroid (will add it to exclusion list)
10:33:52.68 +73:58:40.7 -- not an asteroid (will add it to exclusion list)
10:59:51.74 +73:23:15.2 -- not an asteroid (will add it to exclusion list)
10:33:02.61 +74:25:46.5 -- not an asteroid (will add it to exclusion list)
10:53:34.81 +73:33:33.7 -- not an asteroid (will add it to exclusion list)
10:32:38.15 +74:20:22.6 -- not an asteroid (will add it to exclusion list)
10:55:10.49 +73:51:21.9 -- not an asteroid (will add it to exclusion list)
10:30:20.58 +74:38:34.8 -- not an asteroid (will add it to exclusion list)
10:53:15.85 +73:39:52.3 -- not an asteroid (will add it to exclusion list)
10:47:36.00 +74:06:19.5 -- not an asteroid (will add it to exclusion list)
11:01:45.03 +73:30:27.5 -- not an asteroid (will add it to exclusion list)
10:24:56.60 +74:13:04.5 -- not an asteroid (will add it to exclusion list)
10:48:42.18 +74:10:42.9 -- not an asteroid (will add it to exclusion list)
10:46:57.44 +74:09:09.4 -- not an asteroid (will add it to exclusion list)
11:08:12.35 +73:06:51.9 -- not an asteroid (will add it to exclusion list)
10:49:20.71 +73:51:29.9 -- not an asteroid (will add it to exclusion list)
10:16:27.01 +74:44:27.3 -- not an asteroid (will add it to exclusion list)
10:28:12.73 +74:02:20.5 -- not an asteroid (will add it to exclusion list)
10:31:52.06 +74:38:51.8 -- not an asteroid (will add it to exclusion list)
10:51:03.72 +73:54:47.0 -- not an asteroid (will add it to exclusion list)
10:36:29.57 +74:11:01.1 -- not an asteroid (will add it to exclusion list)
10:40:45.62 +74:09:58.9 -- not an asteroid (will add it to exclusion list)
11:06:16.65 +73:13:24.2 -- not an asteroid (will add it to exclusion list)
10:57:41.89 +73:41:29.4 -- not an asteroid (will add it to exclusion list)
11:04:16.94 +73:07:37.5 -- not an asteroid (will add it to exclusion list)
10:30:41.12 +74:00:45.1 -- not an asteroid (will add it to exclusion list)
10:24:07.23 +74:33:43.7 -- not an asteroid (will add it to exclusion list)
10:59:46.38 +73:34:10.8 -- not an asteroid (will add it to exclusion list)
10:34:40.87 +74:18:28.7 -- not an asteroid (will add it to exclusion list)
10:59:20.06 +73:27:08.9 -- not an asteroid (will add it to exclusion list)
10:33:58.76 +74:14:46.8 -- not an asteroid (will add it to exclusion list)
10:43:58.86 +73:36:31.4 -- not an asteroid (will add it to exclusion list)
10:26:11.04 +74:07:36.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
10:16:27.01 +74:44:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:21:47.29 +74:22:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:21:54.04 +74:33:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:24:07.23 +74:33:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:24:07.46 +74:52:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:24:56.60 +74:13:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:26:11.04 +74:07:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:26:35.09 +74:51:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:26:41.33 +74:18:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:28:12.73 +74:02:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:29:16.91 +74:07:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:30:20.58 +74:38:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:30:24.83 +74:22:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:30:41.12 +74:00:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:31:45.82 +74:42:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:31:52.06 +74:38:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:32:06.90 +74:06:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:32:38.15 +74:20:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:32:53.60 +74:16:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:33:02.61 +74:25:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:33:52.68 +73:58:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:33:58.76 +74:14:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:34:40.87 +74:18:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:35:05.58 +73:46:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:35:12.34 +73:53:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:15.94 +74:14:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:29.57 +74:11:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:59.47 +74:26:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:37:08.89 +74:02:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:40:45.62 +74:09:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:40:45.77 +74:17:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:43:05.53 +74:06:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:43:58.86 +73:36:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:57.44 +74:09:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:36.00 +74:06:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:42.18 +74:10:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:14.86 +74:05:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:20.71 +73:51:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:51:03.72 +73:54:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:52:24.12 +73:24:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:53:15.85 +73:39:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:53:34.81 +73:33:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:55:10.49 +73:51:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:57:41.89 +73:41:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:57:48.10 +73:28:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:59:20.06 +73:27:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:59:46.38 +73:34:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:59:51.74 +73:23:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:01:45.03 +73:30:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:02:39.58 +73:16:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:04:16.94 +73:07:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:06:16.65 +73:13:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:08:12.35 +73:06:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:10:48.83 +72:52:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:01.03 +82:15:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:09:20.48 +81:49:28.4 -- 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)
10:16:27.01 +74:44:27.3 -- not a known variable star
10:21:47.29 +74:22:09.5 -- not a known variable star
10:21:54.04 +74:33:31.6 -- not a known variable star
10:24:07.23 +74:33:43.7 -- not a known variable star
10:24:07.46 +74:52:54.6 -- not a known variable star
10:24:56.60 +74:13:04.5 -- not a known variable star
10:26:11.04 +74:07:36.4 -- not a known variable star
10:26:35.09 +74:51:53.7 -- not a known variable star
10:26:41.33 +74:18:27.1 -- not a known variable star
10:28:12.73 +74:02:20.5 -- not a known variable star
10:29:16.91 +74:07:10.3 -- not a known variable star
10:30:20.58 +74:38:34.8 -- not a known variable star
10:30:24.83 +74:22:38.1 -- not a known variable star
10:30:41.12 +74:00:45.1 -- not a known variable star
10:31:45.82 +74:42:03.6 -- not a known variable star
10:31:52.06 +74:38:51.8 -- not a known variable star
10:32:06.90 +74:06:06.9 -- not a known variable star
10:32:38.15 +74:20:22.6 -- not a known variable star
10:32:53.60 +74:16:18.7 -- not a known variable star
10:33:02.61 +74:25:46.5 -- not a known variable star
10:33:52.68 +73:58:40.7 -- a known variable star
10:33:58.76 +74:14:46.8 -- not a known variable star
10:34:40.87 +74:18:28.7 -- not a known variable star
10:35:05.58 +73:46:59.7 -- not a known variable star
10:35:12.34 +73:53:32.6 -- not a known variable star
10:36:15.94 +74:14:39.2 -- not a known variable star
10:36:29.57 +74:11:01.1 -- not a known variable star
10:36:59.47 +74:26:19.5 -- not a known variable star
10:37:08.89 +74:02:50.9 -- not a known variable star
10:40:45.62 +74:09:58.9 -- not a known variable star
10:40:45.77 +74:17:07.3 -- not a known variable star
10:43:05.53 +74:06:37.4 -- not a known variable star
10:43:58.86 +73:36:31.4 -- not a known variable star
10:46:57.44 +74:09:09.4 -- not a known variable star
10:47:36.00 +74:06:19.5 -- not a known variable star
10:48:42.18 +74:10:42.9 -- not a known variable star
10:49:14.86 +74:05:02.4 -- not a known variable star
10:49:20.71 +73:51:29.9 -- a known variable star
10:51:03.72 +73:54:47.0 -- not a known variable star
10:52:24.12 +73:24:09.5 -- not a known variable star
10:53:15.85 +73:39:52.3 -- not a known variable star
10:53:34.81 +73:33:33.7 -- not a known variable star
10:55:10.49 +73:51:21.9 -- not a known variable star
10:57:41.89 +73:41:29.4 -- not a known variable star
10:57:48.10 +73:28:19.8 -- not a known variable star
10:59:20.06 +73:27:08.9 -- not a known variable star
10:59:46.38 +73:34:10.8 -- not a known variable star
10:59:51.74 +73:23:15.2 -- not a known variable star
11:01:45.03 +73:30:27.5 -- not a known variable star
11:02:39.58 +73:16:14.5 -- not a known variable star
11:04:16.94 +73:07:37.5 -- not a known variable star
11:06:16.65 +73:13:24.2 -- not a known variable star
11:08:12.35 +73:06:51.9 -- not a known variable star
11:10:48.83 +72:52:18.9 -- not a known variable star
12:56:01.03 +82:15:23.0 -- not a known variable star
13:09:20.48 +81:49:28.4 -- not a known variable star
Found 54 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
56 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 56 (excluding asteroids and hot pixels, 54 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)2461258.80075970 -observatory V36
07:46:05.55 +20:23:18.8 Mercury (-0.3mag)
11:55:58.66 -00:06:23.3 Venus (-4.3mag)
05:43:40.73 +23:32:49.6 Mars (1.3mag)
08:41:12.57 +18:47:42.0 Jupiter (-1.8mag)
00:56:32.68 +03:16:43.9 Saturn (0.6mag)
04:11:30.32 +20:56:22.1 Uranus (5.8mag)
00:16:12.53 +00:13:56.8 Neptune (7.7mag)
20:28:19.52 -23:29:26.2 Pluto (14.4mag)
02:51:51.05 +21:05:58.8 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Aug 6 02:16 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461258.80075970:
08:41:18.43 +18:47:16.8 Io (6.0mag)
08:41:08.10 +18:48:01.7 Europa (6.3mag)
08:41:10.18 +18:47:56.2 Ganymede (5.6mag)
08:40:59.54 +18:48:40.9 Callisto (6.7mag)
08:38:48.36 +18:45:54.8 Himalia (15.7mag)
08:41:11.03 +18:47:49.1 Thebe (16.6mag)
08:38:19.06 +18:44:49.1 Elara (17.7mag)
08:45:18.52 +18:28:04.3 Pasiphae (17.9mag)
08:44:31.06 +18:57:33.4 Carme (19.0mag)
00:56:30.05 +03:17:10.9 Titan (8.4mag)
00:56:26.77 +03:16:46.4 Rhea (9.7mag)
00:56:36.54 +03:15:06.9 Iapetus (11.1mag)
00:56:19.10 +03:16:57.5 Hyperion (14.4mag)
00:55:57.61 +03:10:09.9 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 6 02:17 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461258.80075970:
18:55:29.49 -24:00:22.2 JWST
17:18:27.43 +39:42:35.8 Chandra
10:05:32.52 -56:26:10.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 6 02:16 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461258.80075970 -observatory V36
03:11:28.91 +17:12:52.2 17.7mag P/1996 R2 (Lagerkvist)
18:02:22.89 -34:38:22.2 14.0mag P/2010 H2 (Vales)
06:51:59.55 -68:49:49.7 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:09:18.37 +32:57:11.3 17.7mag C/2017 K2 (PANSTARRS)
03:37:58.06 +36:46:19.4 16.7mag P/2021 N1 (ZTF)
22:40:12.82 +31:33:40.4 17.3mag C/2022 E2 (ATLAS)
06:41:33.74 +26:34:26.8 16.8mag C/2022 N2 (PANSTARRS)
10:19:47.39 +28:33:22.0 17.0mag C/2022 QE78 (ATLAS)
09:27:34.29 +05:17:44.4 17.9mag C/2022 R6 (PANSTARRS)
15:12:09.87 -12:12:39.3 17.9mag P/2023 B1 (PANSTARRS)
21:13:18.55 +66:13:25.8 17.9mag C/2023 H5 (Lemmon)
15:49:49.22 -12:45:23.0 14.3mag C/2023 R1 (PANSTARRS)
08:05:55.65 +31:15:33.5 15.2mag C/2024 E1 (Wierzchos)
15:07:16.89 +15:36:57.9 17.7mag C/2024 G6 (ATLAS)
19:05:34.23 +42:58:01.0 13.7mag C/2024 J3 (ATLAS)
21:13:33.15 +49:05:02.5 17.6mag C/2024 R4 (PANSTARRS)
05:13:35.25 -12:59:34.4 15.5mag C/2024 T5 (ATLAS)
06:54:58.11 +24:29:39.6 17.9mag C/2025 J1 (Borisov)
07:29:59.11 -15:52:38.8 17.7mag C/2025 R3 (PANSTARRS)
10:30:14.02 +21:01:34.6 17.3mag C/2025 V2 (Rankin)
12:56:59.16 +02:28:37.2 17.0mag C/2025 Y1 (ATLAS)
16:03:39.84 +78:00:40.4 16.8mag C/2026 A2 (Bok)
03:06:45.01 +46:08:49.9 17.1mag C/2026 B2 (Sun-Gao)
11:45:12.66 +08:20:27.9 17.3mag A/2026 E1
21:56:11.72 -26:29:24.3 6.9mag 10P/Tempel
11:27:48.79 -03:16:52.1 16.2mag 29P/Schwassmann-Wachmann
04:36:51.30 +32:16:09.8 18.0mag 47P/Ashbrook-Jackson
11:03:46.03 +05:16:16.8 17.2mag 63P/Wild
00:54:17.81 -05:22:52.1 15.4mag 65P/Gunn
05:31:10.75 +20:43:43.3 13.7mag 78P/Gehrels
20:39:43.13 -23:18:04.6 17.8mag 84P/Giclas
02:58:48.34 +13:32:45.2 16.7mag 88P/Howell
07:50:57.84 +27:55:06.1 16.1mag 93P/Lovas
04:00:56.83 +16:07:35.4 17.6mag 112P/Urata-Niijima
05:50:07.52 +30:30:27.3 16.3mag 114P/Wiseman-Skiff
09:13:55.91 +26:58:23.7 15.0mag 123P/West-Hartley
11:39:53.26 -09:31:40.9 17.1mag 124P/Mrkos
05:33:42.77 +21:11:10.4 16.1mag 128P/Shoemaker-Holt
06:25:13.10 +18:59:33.6 17.9mag 131P/Mueller
00:03:41.20 +03:25:20.2 17.6mag 139P/Vaisala-Oterma
03:21:33.02 -19:44:44.2 14.0mag 161P/Hartley-IRAS
07:09:30.53 +37:41:41.1 15.8mag 162P/SidingSpring
15:48:35.83 +39:33:17.7 12.3mag 169P/NEAT
02:39:27.11 +09:28:38.6 17.6mag 220P/McNaught
16:40:37.44 -09:56:59.6 17.7mag 235P/LINEAR
20:23:40.29 -52:50:57.1 17.8mag 259P/Garradd
03:16:30.59 +24:21:10.7 15.4mag 260P/McNaught
06:59:34.26 +37:45:13.2 17.3mag 295P/LINEAR
15:09:52.33 +03:21:01.8 17.7mag 391P/Kowalski
08:59:07.92 +18:28:13.0 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 6 02:16 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
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
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
-rw-r--r-- 1 apache apache 5.7K Aug 6 02:16 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
-rw-r--r-- 1 apache apache 189K Aug 6 02:16 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:39:31.292 -08:28:35.35 AT 2026vla 2026-02-21.40 20.65
17:07:24.157 +32:28:59.94 AT 2026vkz 2026-06-16.33 21.89
18:55:34.805 +34:42:05.78 AT 2026vky 2026-06-22.39 21.01
15:27:13.875 -10:50:21.14 AT 2026vkx 2026-06-14.35 20.55
13:36:43.476 +25:28:01.16 AT 2026vkw 2026-06-25.38 20.6
04:43:04.292 -16:08:54.64 AT 2026vkv 2026-01-12.30 21.72
04:48:25.928 -18:19:58.05 AT 2026vku 2026-01-26.25 21.35
12:55:24.686 +13:58:33.13 AT 2026vkt 2026-06-05.34 21.42
11:39:28.884 +47:23:59.43 AT 2026vks 2026-01-14.61 21.82
10:26:55.799 -14:09:20.42 AT 2026vkr 2026-01-13.55 21.98
12:26:22.284 +20:06:25.68 AT 2026vkq 2026-02-13.60 20.86
12:08:12.778 +41:30:56.83 AT 2026vkp 2026-06-15.27 20.88
05:11:50.298 -12:02:24.75 AT 2026vko 2026-02-15.23 20.49
00:35:37.087 -45:29:22.45 AT 2026vkn 2026-06-26.42 23.13
04:11:06.535 -49:23:35.67 AT 2026vkm 2026-07-09.42 22.31
23:40:19.411 -26:01:53.34 AT 2026vkl 2026-07-20.59 21.47
22:23:27.160 +00:54:32.97 AT 2026vkk 2026-07-14.55 21.17
21:14:05.875 -09:55:36.50 AT 2026vkj 2026-07-20.46 21.9
17:17:56.970 +19:09:32.22 AT 2026vki 2026-07-19.39 21.8
17:18:18.165 +24:21:20.44 AT 2026vkh 2026-07-19.40 21.78
-rw-r--r-- 1 apache apache 87K Aug 6 02:16 tns_transients_list.txt
